The chemical composition of the Sun

Abstract

The solar chemical composition is an important ingredient in our understanding of the formation, structure and evolution of both the Sun and our solar system. Furthermore, it is an essential reference standard against which the elemental contents of other astronomical objects are compared. In this review we evaluate the current understanding of the solar photospheric composition. In particular, we present a re-determination of the abundances of nearly all available elements, using a realistic new 3-dimensional (3D), time-dependent hydrodynamical model of the solar atmosphere. We have carefully considered the atomic input data and selection of spectral lines, and accounted for departures from LTE whenever possible. The end result is a comprehensive and homogeneous compilation of the solar elemental abundances. Particularly noteworthy findings are significantly lower abundances of carbon, nitrogen, oxygen and neon compared with the widely-used values of a decade ago. The new solar chemical composition is supported by a high degree of internal consistency between available abundance indicators, and by agreement with values obtained in the solar neighborhood and from the most pristine meteorites. There is, however, a stark conflict with standard models of the solar interior according to helioseismology, a discrepancy that has yet to find a satisfactory resolution.

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• Atmospheric Signatures of Giant Exoplanet Formation by Pebble Accretion
• The Chemical Homogeneity of Sun-like Stars in the Solar Neighborhood
• Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members. II. age dependencies and new insights
• The most metal-poor damped Lyman-alpha systems: Insights into chemical evolution in the very metal-poor regime
• Detection of Pristine Gas Two Billion Years after the Big Bang
• The role of cold gas and environment on the stellar mass - metallicity relation of nearby galaxies
• The Dust-to-Gas and Dust-to-Metals Ratio in Galaxies from z=0-6
• Star formation, supernovae, iron, and alpha: consistent cosmic and Galactic histories
• Pre-galactic metal enrichment - The chemical signatures of the first stars
• Improvements to stellar structure models, based on a grid of 3D convection simulations. II. Calibrating the mixing-length formulation
• Multi-wavelength Observations of the Enduring Type IIn Supernovae 2005ip and 2006jd
• Tracing the total molecular gas in galaxies: [CII] and the CO-dark gas
• Linking dwarf galaxies to halo building blocks with the most metal-poor star in Sculptor
• Chemical abundances of the Milky Way thick disk and stellar halo II.: sodium, iron-peak and neutron-capture elements
• Line lists for the A2PI-X2Sigma+ (red) and {B2Sigma+-X2Sigma} (violet) Systems of CN, 13C14N, and 12C15N, and Application to Astronomical Spectra
• The role of mass transfer and common envelope evolution in the formation of merging binary black holes
• Metal-rich, Metal-poor: Updated Stellar Population Models for Old Stellar Systems
• Cosmic evolution and metal aversion in super-luminous supernova host galaxies
• The Eddington factor as the key to understand the winds of the most massive stars. Evidence for a Gamma-dependence of Wolf-Rayet type mass loss
• HD 140283: A Star in the Solar Neighborhood that Formed Shortly After the Big Bang
• Water in star-forming regions (WISH): Physics and chemistry from clouds to disks as probed by Herschel spectroscopy
• Mass profiles of Galaxy Clusters from X-ray analysis
• How drifting and evaporating pebbles shape giant planets I: Heavy element content and atmospheric C/O
• Giant star seismology
• Uniform Atmospheric Retrieval Analysis of Ultracool Dwarfs I: Characterizing Benchmarks, Gl570D and HD3651B
• Feedback first: the surprisingly weak effects of magnetic fields, viscosity, conduction, and metal diffusion on galaxy formation
• The SDSS-III APOGEE Spectral Line List for H-band Spectroscopy
• The Mass and Momentum Outflow Rates of Photoionized Galactic Outflows
• The formation of IRIS diagnostics I. A quintessential model atom of Mg II and general formation properties of the Mg II h&k lines
• Linking dust emission to fundamental properties in galaxies: The low-metallicity picture
• Hubble Space Telescope spectra of the type Ia supernova SN2011fe: a tail of low-density, high-velocity material with Z<Zsolar
• Globular cluster formation in the context of galaxy formation and evolution
• Extragalactic Background Light from Hierarchical Galaxy Formation: Gamma-ray Attenuation up to the Epoch of Cosmic Reionization and the First Stars
• VINTERGATAN I: The origins of chemically, kinematically and structurally distinct discs in a simulated Milky Way-mass galaxy
• Bayesian analysis of cosmic-ray propagation: evidence against homogeneous diffusion
• Modelling chemical abundance distributions for dwarf galaxies in the Local Group: the impact of turbulent metal diffusion
• Astrochemistry of dust, ice and gas: introduction and overview
• Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS) IV. A spectral inventory of atoms and molecules in the high-resolution transmission spectrum of WASP-121 b
• Sub-Inertial Gravity Modes in the B8V Star KIC 7760680 Reveal Moderate Core Overshooting and Low Vertical Diffusive Mixing
• Gaia FGK benchmark stars: abundances of alpha and iron-peak elements
• Gas Metallicities in the Extended Disks of NGC 1512 and NGC 3621. Chemical Signatures of Metal Mixing or Enriched Gas Accretion?
• Asteroseismology for "à la carte" stellar age-dating and weighing: Age and mass of the CoRoT exoplanet host HD 52265
• {\em Gaia}-derived luminosities of {\em Kepler} A/F stars and the pulsator fraction across the δ Scuti instability strip
• Carbon-rich Giant Planets: Atmospheric Chemistry, Thermal Inversions, Spectra, and Formation conditions
• JADES: Probing interstellar medium conditions at $z\sim 5.5-9.5$ with ultra-deep JWST/NIRSpec spectroscopy
• Nucleosynthesis and the Inhomogeneous Chemical Evolution of the Carina Dwarf Galaxy
• Dynamic mineral clouds on HD 189733b I. 3D RHD with kinetic, non-equilibrium cloud formation
• Evolution and nucleosynthesis of asymptotic giant branch stellar models of low metallicity
• Mapping metallicity variations across nearby galaxy disks
• The influence of atomic diffusion on stellar ages and chemical tagging
• An optical transmission spectrum for the ultra-hot Jupiter WASP-121b measured with the Hubble Space Telescope
• The $R$-Process Alliance: First Release from the Southern Search for $r$-Process-Enhanced Stars in the Galactic Halo
• EDGE: the mass-metallicity relation as a critical test of galaxy formation physics
• Lithium depletion in solar-like stars: no planet connection
• Super-AGB Stars and their role as Electron Capture Supernova progenitors
• Grand Unified Neutrino Spectrum at Earth: Sources and Spectral Components
• Solar axion flux from the axion-electron coupling
• Late-time spectral line formation in Type IIb supernovae, with application to SN 1993J, SN 2008ax, and SN 2011dh
• Iron and s-elements abundance variations in NGC5286: comparison with anomalous globular clusters and Milky Way satellites
• Ultra-fast outflows in radio-loud active galactic nuclei
• The History of R-Process Enrichment in the Milky Way
• SN 2006oz: rise of a super-luminous supernova observed by the SDSS-II SN Survey
• A library of near-infrared integral field spectra of young M-L dwarfs
• The Population of Giant Clumps in Simulated High-z Galaxies: In-situ and Ex-situ, Migration and Survival
• Carbon, oxygen, and iron abundances in disk and halo stars. Implications of 3D non-LTE spectral line formation
• Detailed Chemical Abundances in the r-Process-Rich Ultra-Faint Dwarf Galaxy Reticulum 2
• Revealing the cold dust in low-metallicity environments: I - Photometry analysis of the Dwarf Galaxy Survey with Herschel
• An absolute sodium abundance for a cloud-free 'hot Saturn' exoplanet
• Improved Mass and Radius Constraints for Quiescent Neutron Stars in Omega Cen and NGC 6397
• EIGER II. first spectroscopic characterisation of the young stars and ionised gas associated with strong H$\beta$ and [OIII] line-emission in galaxies at z=5-7 with JWST
• Detection of Elements at All Three r-process Peaks in the Metal-Poor Star HD 160617
• The COS/UVES Absorption Survey of the Magellanic Stream. III: Ionization, Total Mass, and Inflow Rate onto the Milky Way
• Fundamental properties of core-collapse Supernova and GRB progenitors: predicting the look of massive stars before death
• The cosmic ray ionization rate in the Galactic disk, as determined from observations of molecular ions
• A new, precise measurement of the primordial abundance of Deuterium
• A Grid of 3D Stellar Atmosphere Models of Solar Metallicity: I. General Properties, Granulation and Atmospheric Expansion
• Habitability and Biosignatures of Hycean Worlds
• A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS
• Different to the core: the pre-supernova structures of massive single and binary-stripped stars
• The Baryon Cycle of Dwarf Galaxies: Dark, Bursty, Gas-Rich Polluters
• NLTE analysis of Co I/Co II lines in spectra of cool stars with new laboratory hyperfine splitting constants
• An Elemental Assay of Very, Extremely, and Ultra Metal-Poor Stars
• The Role of Stellar Feedback in the Dynamics of HII Regions
• A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics
• Silver and palladium help unveil the nature of a second r-process
• The APOGEE Data Release 16 Spectral Line List
• Can non-ideal magnetohydrodynamics solve the magnetic braking catastrophe?
• Thresholds for Particle Clumping by the Streaming Instability
• Molecular line emission in NGC1068 imaged with ALMA: II. The chemistry of the dense molecular gas
• Effects of Pre-ionisation in Radiative Shocks I: Self-Consistent Models
• Magnetic Nanoparticles in the Interstellar Medium: Emission Spectrum and Polarization
• Pseudo 2D chemical model of hot Jupiter atmospheres: application to HD 209458b and HD 189733b
• Signatures of internal rotation discovered in the Kepler data of five slowly pulsating B stars
• The evolution of massive stars and their spectra I. A non-rotating 60 Msun star from the zero-age main sequence to the pre-supernova stage
• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations I: Black Hole-Neutron Star Mergers
• Where are the most ancient stars in the Milky Way?
• H2O abundances in the atmospheres of three hot Jupiters
• Abundance Profiling of Extremely Metal-Poor Stars and Supernova Properties in the Early Universe
• Mapping the Stellar Halo with the H3 Spectroscopic Survey
• The Stagger-grid: A grid of 3D stellar atmosphere models - III. The relation to mixing-length convection theory
• On the consistent treatment of the quasi-hydrostatic layers in hot star atmospheres
• Observations of Exoplanet Atmospheres
• First grids of low-mass stellar models and isochrones with self-consistent treatment of rotation : From 0.2 to 1.5 M_\odot at 7 metallicities from PMS to TAMS
• Elemental abundance differences in the 16 Cygni binary system: a signature of gas giant planet formation?
• Ionizing spectra of stars that lose their envelope through interaction with a binary companion: role of metallicity
• The expansion of stripped-envelope stars: consequences for supernovae and gravitational-wave progenitors
• A Reservoir of Ionized Gas in the Galactic Halo to Sustain Star Formation in the Milky Way
• Weighing the Giants V: Galaxy Cluster Scaling Relations
• The redshift evolution of the binary black hole merger rate: a weighty matter
• Retrieval of planetary and stellar properties in transmission spectroscopy with Aura
• The VLT-FLAMES Tarantula Survey - XI. A census of the hot luminous stars and their feedback in 30 Doradus
• Nitrogen enhancements 440 Myr after the Big Bang: super-solar N/O, a tidal disruption event or a dense stellar cluster in GN-z11?
• Oxygen Depletion in the Interstellar Medium: Implications for Grain Models and the Distribution of Elemental Oxygen
• Age Determinations of the Hyades, Praesepe, and Pleiades via MESA Models with Rotation
• POSYDON: A General-Purpose Population Synthesis Code with Detailed Binary-Evolution Simulations
• CHAOS IV: Gas-Phase Abundance Trends From The First Four CHAOS Galaxies
• Low-metallicity massive single stars with rotation. Evolutionary models applicable to I Zwicky 18
• The Stagger-grid: A grid of 3D stellar atmosphere models - IV. Limb darkening coefficients
• The Age and Age Spread of the Praesepe and Hyades Clusters: a Consistent, ~800 Myr Picture from Rotating Stellar Models
• The origin and evolution of r- and s-process elements in the Milky Way stellar disk
• Towards the Minimum Inner Edge Distance of the Habitable Zone
• New Hubble Space Telescope Observations of Heavy Elements in Four Metal-Poor Stars
• The Three Dimensional Evolution to Core Collapse of a Massive Star
• Stellar ages and convective cores in field main-sequence stars: first asteroseismic application to two Kepler targets
• Global Seismology of the Sun
• Progenitor Diagnostics for Stripped Core-Collapse Supernovae: Measured Metallicities at Explosion Sites
• Massive Warm/Hot Galaxy Coronae as Probed by UV/X-ray Oxygen Absorption and Emission: I - Basic Model
• The chemistry of vibrationally excited H2 in the interstellar medium
• The HARPS-N Rocky Planet Search I. HD219134b: A transiting rocky planet in a multi-planet system at 6.5 pc from the Sun
• The R-Process Alliance: First Release from the Northern Search for r-Process Enhanced Metal-Poor Stars in the Galactic Halo
• Energetic eruptions leading to a peculiar hydrogen-rich explosion of a massive star
• Metal Abundances, Radial Velocities and other Physical Characteristics for the RR Lyrae Stars in the Kepler Field
• ALFALFA Discovery of the Nearby Gas-Rich Dwarf Galaxy Leo~P. III. An Extremely Metal Deficient Galaxy
• Deriving a multivariate CO-to-H${}_2$ conversion function using the [CII]/CO(1-0) ratio and its application to molecular gas scaling relations
• Molecular abundances in the inner layers of IRC +10216
• A New Stellar Atmosphere Grid and Comparisons with HST/STIS Calspec Flux Distributions
• Pre-supernova evolution, compact object masses and explosion properties of stripped binary stars
• Stellar Models with Enhanced Abundances of C, N, O, Ne, Na, Mg, Si, S, Ca, and Ti, in Turn, at Constant Helium and Iron Abundances
• Slipping magnetic reconnection during an X-class solar flare observed by SDO/AIA
• Impact of the Rotation and Compactness of Progenitors on the Mass of Black Holes
• The water abundance in Jupiter's equatorial zone
• Two years of non-thermal emission from the binary neutron star merger GW170817: rapid fading of the jet afterglow and first constraints on the kilonova fastest ejecta
• Abundances in the Local Region II: F, G and K Dwarfs and Subgiants
• Retrieval of atmospheric properties of cloudy L dwarfs
• A broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18b
• Observational constraints on the origin of the elements. I. 3D NLTE formation of Mn lines in late-type stars
• The VIMOS Ultra Deep Survey: Nature, ISM properties, and ionizing spectra of CIII]1909 emitters at z=2-4
• Effective destruction of CO by cosmic rays: implications for tracing H${}_2$ gas in the Universe
• New axion and hidden photon constraints from a solar data global fit
• Towards a unified view of inhomogeneous stellar winds in isolated supergiant stars and supergiant high mass X-ray binaries
• Deep into the structure of the first galaxies: SERRA views
• Stellar Archaeology -- Exploring the Universe with Metal-Poor Stars
• Self-luminous and irradiated exoplanetary atmospheres explored with HELIOS
• YBC, a stellar bolometric corrections database with variable extinction coefficients: an application to PARSEC isochrones
• Spitzer 3.6 micron and 4.5 micron full-orbit lightcurves of WASP-18
• X-ray bursting neutron star atmosphere models: spectra and color corrections
• Improved Ti II log(gf) Values and Abundance Determinations in the Photospheres of the Metal-Poor Star HD 84937
• The Lyman alpha Reference Sample: II. HST imaging results, integrated properties and trends
• Nebular spectroscopy: A guide on H II regions and planetary nebulae
• Strong XUV irradiation of the Earth-sized exoplanets orbiting the ultracool dwarf TRAPPIST-1
• Explosive Nucleosynthesis in Near-Chandrasekhar Mass White Dwarf Models for Type Ia Supernovae: Dependence on Model Parameters
• Iron and neutron-capture element abundance variations in the globular cluster M2 (NGC 7089)
• Solar abundance of manganese: a case for the existence of near Chandrasekhar-mass Type Ia supernova progenitors
• Planet-forming material in a protoplanetary disc: the interplay between chemical evolution and pebble drift
• External photoevaporation of protoplanetary discs in sparse stellar groups: the impact of dust growth
• Kepler observations of variability in B-type stars
• Simulating the interstellar medium and stellar feedback on a moving mesh: Implementation and isolated galaxies
• Thermochemistry and Photochemistry in Cooler Hydrogen Dominated Extrasolar Planets: The Case of GJ436b
• Peering into the formation history of beta Pictoris b with VLTI/GRAVITY long baseline interferometry
• UCLCHEM: A Gas-Grain Chemical Code
• Re-Evaluating WASP-12b: Strong Emission at 2.315 micron, Deeper Occultations, and an Isothermal Atmosphere
• Light, Alpha, and Fe-Peak Element Abundances in the Galactic Bulge
• Sulphur chemistry in the L1544 pre-stellar core
• The Initial mass function of the first stars inferred from extremely metal-poor stars
• BANYAN. IV. Fundamental parameters of low-mass star candidates in nearby young stellar kinematic groups - Isochronal Age determination using Magnetic evolutionary models
• Ionization balance of Ti in the photospheres of the Sun and four late-type stars
• An R-process enhanced star in the dwarf galaxy Tucana III
• The formation of IRIS diagnostics. III. Near-ultraviolet Spectra and Images
• Constraining the metallicities, ages, star formation histories, and ionizing continua of extragalactic massive star populations
• FIRE-3: Updated Stellar Evolution Models, Yields, & Microphysics and Fitting Functions for Applications in Galaxy Simulations
• The MOSDEF Survey: Direct Observational Constraints on the Ionizing Photon Production Efficiency, ${\xi }_{\mathrm{ion}}$, at z~2
• Current challenges in the physics of white dwarf stars
• The primordial deuterium abundance of the most metal-poor damped Lyman-alpha system
• The Type IIb Supernova 2013df and Its Cool Supergiant Progenitor
• Herschel observations of EXtra-Ordinary Sources: Analysis of the HIFI 1.2 THz Wide Spectral Survey Toward Orion KL I. Methods
• Carbon and oxygen abundances in stellar populations
• Deep Mixing in Evolved Stars: I. The Effect of Reaction Rate Revisions from C to Al
• Leo P: An Unquenched Very Low-Mass Galaxy
• The GAPS programme with HARPS-N at TNG XI. Pr~0211 in M~44: the first multi-planet system in an open cluster
• A Chemical Kinetics Network for Lightning and Life in Planetary Atmospheres
• Astrochemical evolution along star formation: Overview of the IRAM Large Program ASAI
• The MOSDEF Survey: Significant Evolution in the Rest-Frame Optical Emission Line Equivalent Widths of Star-Forming Galaxies at z=1.4-3.8
• Metal-enriched galactic outflows shape the mass-metallicity relationship
• JWST NIRCam+NIRSpec: Interstellar medium and stellar populations of young galaxies with rising star formation and evolving gas reservoirs
• The Peculiar Atmospheric Chemistry of KELT-9b
• A new asteroseismic diagnostic for internal rotation in $\gamma$ Doradus stars
• Zooming on the internal structure of $z\simeq 6$ galaxies
• Chemical abundances in M31 from HII regions
• Simulating cosmic metal enrichment by the first galaxies
• Dust attenuation in 2<z<3 star-forming galaxies from deep ALMA observations of the Hubble Ultra Deep Field
• Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS): II. Cold Molecular Gas Evolution out to Redshift 6
• Revisiting the Integrated Star Formation Law. Paper I: Non-Starbursting Galaxies
• A High-Velocity Narrow Absorption Line Outflow in the Quasar J212329.46-005052.9
• Discovery of the broad-lined Type Ic SN 2013cq associated with the very energetic GRB 130427A
• Characterizing the Chemistry of the Milky Way Stellar Halo: Detailed Chemical Analysis of a Metal-Poor Stellar Stream
• A Window On The Earliest Star Formation: Extreme Photoionization Conditions of a High-Ionization, Low-Metallicity Lensed Galaxy at z~2
• JWST/NIRCam Probes Young Star Clusters in the Reionization Era Sunrise Arc
• ALMA observations of atomic carbon in z~4 dusty star-forming galaxies
• High-Resolution Spectroscopy of Extremely Metal-Poor Stars in the Least Evolved Galaxies: Leo IV
• The eROSITA Final Equatorial-Depth Survey (eFEDS): Catalog of galaxy clusters and groups
• A comparison of evolutionary tracks for single Galactic massive stars
• The Gaia-ESO Public Spectroscopic Survey: Motivation, implementation, GIRAFFE data processing, analysis, and final data products
• High-Resolution Spectroscopic Study of Extremely Metal-Poor Star Candidates from the SkyMapper Survey
• Measuring the Physical Conditions in High-Redshift Star-Forming Galaxies: Insights from KBSS-MOSFIRE
• Gravitationally Lensed Galaxies at 2<z<3.5: Direct Abundance Measurements of Lya Emitters
• The Palomar Transient Factory Core-Collapse Supernova Host-Galaxy Sample. I. Host-Galaxy Distribution Functions and Environment-Dependence of CCSNe
• Rotating models of young solar-type stars : Exploring braking laws and angular momentum transport processes
• Keck Spectroscopy of Gravitationally Lensed z=4 Galaxies: Improved Constraints on the Escape Fraction of Ionizing Photons
• A Chandrasekhar Mass Progenitor for the Type Ia Supernova Remnant 3C 397 from The Enhanced Abundances of Nickel and Manganese
• GRB 120422A/SN 2012bz: Bridging the Gap between Low- And High-Luminosity GRBs
• Non-LTE oxygen line formation in 3D hydrodynamic model stellar atmospheres
• s-Process in Low Metallicity Stars. III. Individual analysis of CEMP-s and CEMP-s/r with AGB models
• The Most Metal-Poor Stars. III. The Metallicity Distribution Function and CEMP Fraction
• Probing X-ray Absorption and Optical Extinction in the Interstellar Medium Using Chandra Observations of Supernova Remnants
• The impact of chemistry on the structure of high-z galaxies
• A more realistic representation of overshoot at the base of the solar convective envelope as seen by helioseismology
• A New Star-Formation Rate Calibration from Polycyclic Aromatic Hydrocarbon Emission Features and Application to High Redshift Galaxies
• Measuring the extent of convective cores in low-mass stars using Kepler data: towards a calibration of core overshooting
• The Connection Between Reddening, Gas Covering Fraction, and the Escape of Ionizing Radiation at High Redshift
• Smoothly-Rising Star Formation Histories During the Reionization Epoch
• Deriving Stellar Effective Temperatures of Metal-Poor Stars with the Excitation Potential Method
• On Variations Of Pre-Supernova Model Properties
• New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars II. A grid of O-type stars in the Galaxy and the Magellanic Clouds
• A translucent interstellar cloud at z=2.69: CO, H2 and HD in the line-of-sight to SDSS J123714.60+064759.5
• DUNE as the Next-Generation Solar Neutrino Experiment
• Connecting Giant Planet Atmosphere and Interior Modeling: Constraints on Atmospheric Metal Enrichment
• Age as a Major Factor in the Onset of Multiple Populations in Stellar Clusters
• On the sensitivity of gravito-inertial modes to differential rotation in intermediate-mass main-sequence stars
• Solar system genealogy revealed by extinct short-lived radionuclides in meteorites
• What FIREs Up Star Formation: the Emergence of the Kennicutt-Schmidt Law from Feedback
• Stellar Yields of Rotating First Stars. II. Pair Instability Supernovae and Comparison with Observations
• Galaxy Cold Gas Contents in Modern Cosmological Hydrodynamic Simulations
• Magnesium in the atmosphere of the planet HD209458b: Observations of the thermosphere-exosphere transition region
• Galaxy Counterparts of metal-rich Damped Lyman-alpha Absorbers - I: The case of the z=2.35 DLA towards Q2222-0946
• Interstellar chemistry of nitrogen hydrides in dark clouds
• A tale of two DIGs: The relative role of HII regions and low-mass hot evolved stars in powering the diffuse ionised gas (DIG) in PHANGS-MUSE galaxies
• Abundant refractory sulfur in protoplanetary disks
• Constraining planet structure from stellar chemistry: the cases of CoRoT-7, Kepler-10, and Kepler-93
• Radioactive nuclei from cosmochronology to habitability
• Diagnostics for PopIII galaxies and Direct Collapse Black Holes in the early universe
• Cosmic-ray induced destruction of CO in star-forming galaxies
• Bayesian Ages for Early-Type Stars from Isochrones Including Rotation, and a Possible Old Age for the Hyades
• WIYN Open Cluster Study. LXXV. Testing the Metallicity Dependence of Stellar Lithium Depletion Using Hyades-Aged Clusters. 1. Hyades & Praesepe
• Atmospheres from very low-mass stars to extrasolar planets
• The Primeval Populations of the Ultra-Faint Dwarf Galaxies
• The ALMA-PILS survey: The sulphur connection between protostars and comets: IRAS 16293-2422 B and 67P/Churyumov-Gerasimenko
• Jupiter's composition suggests its core assembled exterior to the N2 snowline
• Interpreting ALMA Observations of the ISM During the Epoch of Reionisation
• The star formation history and metal content of the "Green Peas". New detailed GTC-OSIRIS spectrophotometry of three galaxies
• Confirmation of circumstellar phosphine
• The early detection and follow-up of the highly obscured Type II supernova 2016ija/DLT16am
• The Distribution of the Elements in the Galactic Disk II. Azimuthal and Radial Variation in Abundances from Cepheids
• Elemental Abundances and their Implications for the Chemical Enrichment of the Boötes~I Ultra-Faint Galaxy
• ARIADNE: Measuring accurate and precise stellar parameters through SED fitting
• Abundances of Galactic Anticenter Planetary Nebulae and the Oxygen Abundance Gradient in the Galactic Disk
• The first view of $\delta$ Scuti and $\gamma$ Doradus stars with the TESS mission
• Modeling Dust and Starlight in Galaxies Observed by Spitzer and Herschel: NGC 628 and NGC 6946
• Planetesimal rings as the cause of the Solar System's planetary architecture
• MUSTANG High Angular Resolution Sunyaev-Zel'dovich Effect Imaging of Sub-Structure in Four Galaxy Clusters
• The GALAH survey: An abundance, age, and kinematic inventory of the solar neighbourhood made with TGAS
• Simple recipes for compact remnant masses and natal kicks
• High-precision abundances of elements in solar-type stars. Evidence of two distinct sequences in abundance-age relations
• Damped Lyman-alpha absorbers as a probe of stellar feedback
• Nearly-uniform internal rotation of solar-like main-sequence stars revealed by space-based asteroseismology and spectroscopic measurements
• The Fundamental Plane of Damped Lyman Alpha Systems
• Synthetic Gaia surveys from the FIRE cosmological simulations of Milky Way-mass galaxies
• A Survey of Atomic Carbon [C I] in High-redshift Main-Sequence Galaxies
• A library of ATMO forward model transmission spectra for hot Jupiter exoplanets
• Mass-loss rates for transiting exoplanets
• Empirical Isochrones for Low Mass Stars in Nearby Young Associations
• Fingerprints of giant planets in the photospheres of Herbig stars
• Spectroscopic survey of Kepler stars. I. HERMES/Mercator observations of A- and F-type stars
• The Gaia-ESO Survey: radial distribution of abundances in the Galactic disc from open clusters and young field stars
• Wolf-Rayet stars in the Small Magellanic Cloud: I. Analysis of the single WN stars
• L-GALAXIES 2020: Spatially resolved cold gas phases, star formation and chemical enrichment in galactic discs
• Extremely metal-poor stars from the cosmic dawn in the bulge of the Milky Way
• Descendants of the first stars: the distinct chemical signature of second generation stars
• Super-Earth masses sculpted by pebble isolation around stars of different masses
• Simulating an Isolated Dwarf Galaxy with Multi-Channel Feedback and Chemical Yields from Individual Stars
• Asymmetric dark matter and the Sun
• Mass loss on the red giant branch: the value and metallicity dependence of Reimers' η in globular clusters
• Observational Constraints on the Physical Properties of Interstellar Dust in the Post-Planck Era
• Retired A Stars Revisited: An Updated Giant Planet Occurrence Rate as a Function of Stellar Metallicity and Mass
• Gravito-inertial and pressure modes detected in the B3 IV CoRoT target HD 43317
• Four-hundred Very Metal-Poor Stars Studied with LAMOST and Subaru. II. Elemental abundances
• Modeling the atomic-to-molecular transition in cosmological simulations of galaxy formation
• Why is it so Cold in Here?: Explaining the Cold Temperatures Retrieved from Transmission Spectra of Exoplanet Atmospheres
• Stellar Chemical Abundances: In Pursuit of the Highest Achievable Precision
• Grain Growth in the Circumstellar Disks of the Young Stars CY Tau and DoAr 25
• Cosmological implications of the anisotropy of ten galaxy cluster scaling relations
• The Properties of Low Redshift Intergalactic O VI Absorbers Determined from High S/N Observations of 14 QSOs with the Cosmic Origins Spectrograph
• "Counterpart" method for abundance determinations in HII regions
• The Survey of HI in Extremely Low-mass Dwarfs (SHIELD)
• A Spectroscopic Analysis of the California-Kepler Survey Sample: I. Stellar Parameters, Planetary Radii and a Slope in the Radius Gap
• The X-factor in Galaxies: I. Dependence on Environment and Scale
• A giant impact as the likely origin of different twins in the Kepler-107 exoplanet system
• Discovery of transient infrared emission from dust heated by stellar tidal disruption flares
• Early magnetic B-type stars: X-ray emission and wind properties
• Helium enrichment and Carbon-star Production in Metal-rich Populations
• The Atacama Cosmology Telescope: Physical Properties and Purity of a Galaxy Cluster Sample Selected via the Sunyaev-Zel'dovich Effect
• Evidence for a Massive, Extended Circumgalactic Medium Around the Andromeda Galaxy
• A Nearby Galaxy Perspective on Dust Evolution. Scaling relations and constraints on the dust build-up in galaxies with the DustPedia and DGS samples
• Testing massive star evolution, star-formation history and feedback at low metallicity : Spectroscopic analysis of OB stars in the SMC Wing
• Resolving Vega and the inclination controversy with CHARA/MIRC
• Where is the Water? Jupiter-like C/H ratio but strong H${}_2$O depletion found on $\tau$ Boötis b using SPIRou
• The impact of atmospheric circulation on the chemistry of the hot Jupiter HD 209458b
• The VANDELS survey: the stellar metallicities of star-forming galaxies at 2.5 < z < 5.0
• The inner wind of IRC+10216 revisited: New exotic chemistry and diagnostic for dust condensation in carbon stars
• Signatures of broken protoplanetary discs in scattered light and in sub-millimetre observations
• Galactic and Circumgalactic OVI and its Impact on the Cosmological Metal and Baryon Budgets at 2<z<3.5
• The $R$-Process Alliance: Fourth Data Release from the Search for $r$-Process-Enhanced Stars in the Galactic Halo
• Sulphur-bearing molecules in diffuse molecular clouds: new results from SOFIA/GREAT and the IRAM 30 m telescope
• The Pisa Stellar Evolution Data Base for low-mass stars
• Dust-to-metal ratios in damped Lyman-alpha absorbers: Fresh clues to the origins of dust and optical extinction towards gamma-ray bursts
• Carbon and oxygen abundances from recombination lines in low-metallicity star-forming galaxies. Implications for chemical evolution
• Towards stellar effective temperatures and diameters at one per cent accuracy for future surveys
• Stellar Diameters and Temperatures VI. High angular resolution measurements of the transiting exoplanet host stars HD 189733 and HD 209458 and implications for models of cool dwarfs
• Form factors for dark matter capture by the Sun in effective theories
• Old and young stellar populations in DustPedia galaxies and their role in dust heating
• RR-Lyrae-type pulsations from a 0.26-solar-mass star in a binary system
• SN 2009md: Another faint supernova from a low mass progenitor
• An HST/COS legacy survey of high-velocity ultraviolet absorption in the Milky Way's circumgalactic medium and the Local Group
• Stellar Absorption Line Analysis of Local Star-Forming Galaxies: The Relation Between Stellar Mass, Metallicity, Dust Attenuation and Star Formation Rate
• A Universal Density Structure for Circum-Galactic Gas
• Solar structure and evolution
• CHAOS II: Gas-Phase Abundances in NGC 5194
• Thiols in the ISM: first detection of HC(O)SH and confirmation of C${}_2$H${}_5$SH
• Pulsation frequency distribution in Delta Scuti stars
• The host galaxy and late-time evolution of the Super-Luminous Supernova PTF12dam
• Mass loss in main-sequence B stars
• Dust in the diffuse interstellar medium: Extinction, emission, linear and circular polarisation
• The role of binaries in the enrichment of the early Galactic halo. II. Carbon-Enhanced Metal-Poor Stars - CEMP-no stars
• A hot and fast ultra-stripped supernova that likely formed a compact neutron star binary
• The gas-to-extinction ratio and the gas distribution in the Galaxy
• Hydrogen Cyanide in Nitrogen-Rich Atmospheres of Rocky Exoplanets
• Sulfur chemistry in protoplanetary disks: CS and H2CS
• Modelling Element Abundances in Semi-analytic Models of Galaxy Formation
• Very regular high-frequency pulsation modes in young intermediate-mass stars
• A surge of light at the birth of a supernova
• The discoveries of WASP-91b, WASP-105b and WASP-107b: two warm Jupiters and a planet in the transition region between ice giants and gas giants
• Searching for Extremely Blue UV Continuum Slopes at $z=7-11$ in JWST/NIRCam Imaging: Implications for Stellar Metallicity and Ionizing Photon Escape in Early Galaxies
• FastChem 2: An improved computer program to determine the gas-phase chemical equilibrium composition for arbitrary element distributions
• 18 Sco: a solar twin rich in refractory and neutron-capture elements. Implications for chemical tagging
• The COSMOS2015 galaxy stellar mass function: 13 billion years of stellar mass assembly in 10 snapshots
• Molecular depletion times and the CO-to-H2 conversion factor in metal-poor galaxies
• Current status and desired accuracy of the isotopic production cross sections relevant to astrophysics of cosmic rays I. Li, Be, B, C, N
• Yellow and Red Supergiants in the Large Magellanic Cloud
• Heavy-element yields and abundances of Asymptotic Giant Branch models with a Small Magellanic Cloud metallicity
• Accurate abundance analysis of late-type stars: advances in atomic physics
• Consensus report on 25 years of searches for damped Ly$\alpha$ galaxies in emission: Confirming their metallicity-luminosity relation at $z\gtrsim 2$
• Triangulum II: Not Especially Dense After All
• The Column Density, Kinematics, and Thermal State of Metal-Bearing Gas within the Virial Radius of z~2 Star-Forming Galaxies in the Keck Baryonic Structure Survey
• The dust and gas content of the Crab Nebula
• An Earth-sized exoplanet with a Mercury-like composition
• The Spatially Resolved [CII] Cooling Line Deficit in Galaxies
• A Comparison between Semi-Analytic Model Predictions for the CANDELS Survey
• The molecular gas reservoir of 6 low-metallicity galaxies from the Herschel Dwarf Galaxy Survey: A ground-based follow-up survey of CO(1-0), CO(2-1), and CO(3-2)
• FIREbox: Simulating galaxies at high dynamic range in a cosmological volume
• ALMA and ROSINA detections of phosphorus-bearing molecules: the interstellar thread between star-forming regions and comets
• High-precision stellar abundances of the elements - methods and applications
• Disk evolution, element abundances and cloud properties of young gas giant planets
• The quest for the solar g modes
• Barium & related stars and their white-dwarf companions I. Giant stars
• Mg line formation in late-type stellar atmospheres: I. The model atom
• Kinematics of $z\ge 6$ galaxies from [CII] line emission
• Hunting for extremely metal-poor emission-line galaxies in the Sloan Digital Sky Survey: MMT and 3.5m APO observations
• Astrophysical Axion Bounds: The 2024 Edition
• The Herschel Dwarf Galaxy Survey: II. Physical conditions, origin of [CII] emission, and porosity of the multiphase low-metallicity ISM
• Dust variations in the diffuse interstellar medium: constraints on Milky Way dust from Planck-HFI observations
• The D/H ratio in the atmospheres of Uranus and Neptune from Herschel PACS observations
• Star formation history and X-ray binary populations: the case of the Small Magellanic Cloud
• Radiative hydrodynamics simulations of red supergiant stars. IV gray versus non-gray opacities
• Stochastic star formation in early galaxies: JWST implications
• The hot dayside and asymmetric transit of WASP-189b seen by CHEOPS
• Photoionization Models for the Semi-Forbidden C III] 1909 Emission in Star-Forming Galaxies
• The EMBLA Survey -- Metal-poor stars in the Galactic bulge
• Simulating the cloudy atmospheres of HD 209458 b and HD 189733 b with the 3D Met Office Unified Model
• Discovery of a compact gas-rich DLA galaxy at z = 2.2: evidences for a starburst-driven outflow
• Verifying the mass-metallicity relation in damped Lyman-alpha selected galaxies at 0.1<z<3.2
• The CARMENES search for exoplanets around M dwarfs. Stellar atmospheric parameters of target stars with SteParSyn
• A physical model for [CII] line emission from galaxies
• Determination of Three-dimensional Spin-orbit Angle with Joint Analysis of Asteroseismology, Transit Lightcurve, and the Rossiter-McLaughlin Effect: Cases of HAT-P-7 and Kepler-25
• Iron-Group Abundances in the Metal-Poor Main Sequence Turnoff Star HD~84937
• Radiative cooling rates, ion fractions, molecule abundances and line emissivities including self-shielding and both local and metagalactic radiation fields
• Production of 26Al, 44Ti, and 60Fe in Core-Collapse Supernovae: Sensitivity to the Rates of the Triple Alpha and 12C(a,g)16O Reactions
• Improved Ni I log(gf) Values and Abundance Determinations in the Photospheres of the Sun and Metal-poor Star HD 84937
• The evolution of CNO isotopes: the impact of massive stellar rotators
• Chemical Abundances in the Ultra-Faint Dwarf Galaxies Grus I and Triangulum II: Neutron-Capture Elements as a Defining Feature of the Faintest Dwarfs
• Spectroscopic Measurements of the Far-Ultraviolet Dust Attenuation Curve at z~3
• The Galactic dust-to-metals ratio and metallicity using gamma-ray bursts
• Chemical equilibrium in AGB atmospheres: Successes, failures, and prospects for small molecules, clusters, and condensates
• Theoretical ISM pressure and electron density diagnostics for local and high-redshift galaxies
• Possible Signatures of a Cold-Flow Disk from MUSE using a z=1 galaxy--quasar pair towards SDSSJ1422-0001
• Star Formation and Metallicity Gradients in Semi-analytic Models of Disk Galaxy Formation
• The CARMENES search for exoplanets around M dwarfs - Photospheric parameters of target stars from high-resolution spectroscopy
• NLTE analysis of Sr lines in spectra of late-type stars with new R-matrix atomic data
• Carbon-enhanced metal-poor stars in dwarf galaxies
• Abundances and possible diffusion of elements in M67 stars
• Simulations of radiative turbulent mixing layers
• A Stellar Feedback Origin for Neutral Hydrogen in High-Redshift Quasar-Mass Halos
• Atmospheric dynamics and the variable transit of KELT-9 b
• The spin temperature of high-redshift damped Lyman-$\alpha$ systems
• The origin of diverse $\alpha$-element abundances in galaxy discs
• A WC/WO star exploding within an expanding carbon-oxygen-neon nebula
• Binary Black Hole Formation with Detailed Modeling: Stable Mass Transfer Leads to Lower Merger Rates
• Updated determination of the solar neutrino fluxes from solar neutrino data
• The assembly of dusty galaxies at $z\ge 4$: statistical properties
• On the Carbon-to-Oxygen Ratio Measurement in Nearby Sunlike Stars: Implications for Planet Formation and the Determination of Stellar Abundances
• Wolf-Rayet stars in the Small Magellanic Cloud: II. Analysis of the binaries
• Neutron Star Mass-Radius Constraints of the Quiescent Low-mass X-ray Binaries X7 and X5 in the Globular Cluster 47 Tuc
• Galaxy counterparts of metal-rich damped Lyman-alpha absorbers - II. A solar-metallicity and dusty DLA at z_abs=2.58
• The Dust Extinction Curves of Gamma-Ray Burst Host Galaxies
• The dissimilar chemical composition of the planet-hosting stars of the XO-2 binary system
• Coupling hydrodynamics with comoving frame radiative transfer: I. A unified approach for OB and WR stars
• The Photoevaporative Wind from the Disk of TW Hya
• Dissecting the properties of optically-thick hydrogen at the peak of cosmic star formation history
• Keeping it Cool: Much Orbit Migration, yet Little Heating, in the Galactic Disk
• Magnetic field topology of the unique chemically peculiar star CU Virginis
• Inference of the Local Interstellar Spectra of Cosmic Ray Nuclei Z<=28 with the GalProp-HelMod Framework
• Phosphorus-bearing molecules in solar-type star forming regions: First PO detection
• The GALAH Survey: Non-LTE departure coefficients for large spectroscopic surveys
• EMPRESS. V. Metallicity Diagnostics of Galaxies over 12+log(O/H)=~6.9-8.9 Established by a Local Galaxy Census: Preparing for JWST Spectroscopy
• Accurate p-mode measurements of the G0V metal-rich CoRoT target HD 52265
• Accurate spectroscopic parameters of WASP planet host stars
• The Distribution of Alpha Elements in Ultra-Faint Dwarf Galaxies
• Solar Energetic Particles (Second Edition)
• The dependence of convective core overshooting on stellar mass: Additional binary systems and improved calibration
• Resolving the Far-IR Line Deficit: Photoelectric Heating and Far-IR Line Cooling in NGC 1097 and NGC 4559
• Seismic and dynamical solar models i-the impact of the solar rotation history on neutrinos and seismic indicators
• Heavy Element Nucleosynthesis in the Brightest Galactic Asymptotic Giant Branch stars
• EMPRESS. VIII. A New Determination of Primordial He Abundance with Extremely Metal-Poor Galaxies: A Suggestion of the Lepton Asymmetry and Implications for the Hubble Tension
• Physics from solar neutrinos in dark matter direct detection experiments
• The uniformity and time-invariance of the intra-cluster metal distribution in galaxy clusters from the IllustrisTNG simulations
• A Swift survey of accretion onto stellar-mass black holes
• The ALMA REBELS Survey. Epoch of Reionization giants: properties of dusty galaxies at $z\approx 7$
• The Physical Conditions, Metallicity and Metal Abundance Ratios In a Highly Magnified Galaxy at z = 3.6252
• γ Doradus stars as test of angular momentum transport models
• The Low Mass End of the Fundamental Relation for Gravitationally Lensed Star Forming Galaxies at 1<z<6
• A first look at the SMACS0723 JWST ERO: spectroscopic redshifts, stellar masses and star-formation histories
• Effects of radial flows on the chemical evolution of the Milky Way disk
• Kepler-68: Three Planets, One With a Density Between That of Earth and Ice Giants
• Discovery of the Young L Dwarf WISE J1741102.78-464225.5
• The chemical composition of the Sun from helioseismic and solar neutrino data
• First stars XVI. STIS/HST abundances of heavy-elements in the uranium-rich star CS 31082-001
• Cloud busting: enstatite and quartz clouds in the atmosphere of 2M2224-0158
• The physical properties of z>2 Lyman limit systems: new constraints for feedback and accretion models
• Outward Migration of Jupiter and Saturn in Evolved Gaseous Disks
• Element Abundances: A New Diagnostic for the Solar Wind
• Evidence for Cold Accretion: Primitive Gas Flowing onto a Galaxy at z~0.274
• SIGAME simulations of the [CII], [OI] and [OIII] line emission from star forming galaxies at z ~ 6
• Exploring mass loss, low-Z accretion, and convective overshoot in solar models to mitigate the solar abundance problem
• GRB hosts through cosmic time - VLT/X-Shooter emission-line spectroscopy of 96 GRB-selected galaxies at 0.1 < z < 3.6
• Young stars and ionized nebulae in M83: comparing chemical abundances at high metallicity
• Evolution of surface CNO abundances in massive stars
• Exploring the Origin of Lithium, Carbon, Strontium and Barium with four new Ultra Metal-Poor Stars
• High Precision Abundances of the Old Solar Twin HIP 102152: Insights on Li Depletion from the Oldest Sun
• A Local Universe Host for the Repeating Fast Radio Burst FRB 20181030A
• Oxygen abundances in G- and F-type stars from HARPS
• The physics of multiphase gas flows: fragmentation of a radiatively cooling gas cloud in a hot wind
• Magnetic Activity Cycles in the Exoplanet Host Star epsilon Eridani
• Asteroseismic modelling of the two F-type hybrid pulsators KIC10080943A and KIC10080943B
• Forward asteroseismic modeling of stars with a convective core from gravity-mode oscillations: parameter estimation and stellar model selection
• Variability in quasar broad absorption line outflows II. Multi-epoch monitoring of SiIV and CIV BAL variability
• The GTC exoplanet transit spectroscopy survey IX. Detection of Haze, Na, K, and Li in the super-Neptune WASP-127b
• Planet population synthesis driven by pebble accretion in cluster environments
• Superluminous supernova progenitors have a half-solar metallicity threshold
• On the O/H, Mg/H, Si/H and Fe/H Gas and Dust Abundance Ratios in Galactic and Extragalactic H II Regions
• The origin of metals in the circum-galactic medium of massive galaxies at z=3
• Extreme N-emitters at high-redshift: signatures of supermassive stars and globular cluster or black hole formation in action?
• Gemini Planet Imager Spectroscopy of the HR 8799 planets c and d
• Double Detonations with Thin, Modestly Enriched Helium Layers Can Make Normal Type Ia Supernovae
• Supernova 2012aw - a high-energy clone of archetypal type IIP SN 1999em
• Measurement of acoustic glitches in solar-type stars from oscillation frequencies observed by Kepler
• The shape of convective core overshooting from gravity-mode period spacings
• The JWST-PRIMAL Legacy Survey. A JWST/NIRSpec reference sample for the physical properties and Lyman-$\alpha$ absorption and emission of $\sim 500$ galaxies at $z=5.5-13.4$
• The Spectrum of the Diffuse Galactic Light I: The Milky Way in Scattered Light
• GRB 100219A with X-shooter - abundances in a galaxy at z = 4.7
• Macroclumping as solution of the discrepancy between Hα and P v mass loss diagnostics for O-type stars
• How realistic are solar model atmospheres?
• Scientific rationale for Uranus and Neptune in situ explorations
• Dark matter in the Sun: scattering off electrons vs nucleons
• Variability in Quasar Broad Absorption Line Outflows III. What Happens on the Shortest Time-scales?
• The dependence of convective core overshooting on stellar mass: semi-empirical determination using the diffusive approach with two different element mixtures
• Solar Neutrinos as a Signal and Background in Direct-Detection Experiments Searching for Sub-GeV Dark Matter With Electron Recoils
• A survey of high-$z$ galaxies: SERRA simulations
• Cepheid Abundances: Multiphase Results and Spatial Gradients
• On Lithium-Rich Red Giants. I. Engulfment of Sub-Stellar Companions
• Efficient Production of S${}_8$ in Interstellar Ices: The effects of cosmic ray-driven radiation chemistry and non-diffusive bulk reactions
• Extremely metal-poor gas at a redshift of 7
• Binary stars in the Galactic thick disc
• The Massive Progenitor of the Type II-Linear SN 2009kr
• Isochrones for Old (> 5 Gyr) Stars and Stellar Populations. I. Models for $-2.4\le$ [Fe/H] $\le +0.6$, $0.25\le Y\le 0.33$, and $-0.4\le$ [$\alpha$\Fe] $\le +0.4$
• Evolution of the solar activity over time and effects on planetary atmospheres. II. kappa^1 Ceti, an analog of the Sun when life arose on Earth
• Improving Helium Abundance Determinations with Leo P as a Case Study
• The production of proton-rich isotopes beyond iron: The $\gamma$ process in stars
• Galaxies in the EAGLE hydrodynamical simulation and in the Durham and Munich semi-analytical models
• The chemical composition of the Orion star-forming region. III. C, N, Ne, Mg and Fe abundances in B-type stars revisited
• Silicon and Oxygen Abundances in Planet-Host Stars
• Detailed Abundances of the Solar Twins 16 Cygni A and B: Constraining Planet Formation Models
• Mass loss rate and local thermodynamic state of KELT-9 b thermosphere from the hydrogen Balmer series
• Simulations of the solar near-surface layers with the CO5BOLD, MURaM, and Stagger codes
• Metallicity-dependent wind parameter predictions for OB stars
• Spatially resolved stellar, dust and gas properties of the post-interacting Whirlpool Galaxy system
• C/O Ratios of Stars with Transiting Hot Jupiter Exoplanets
• Complexity in the light curves and spectra of slow-evolving superluminous supernovae
• On the duration of the embedded phase of star formation
• An Atomic Spectral Survey of WASP-76b: Resolving Chemical Gradients and Asymmetries
• M67-1194, an unusually Sun-like solar twin in M67
• GRB 130606A as a Probe of the Intergalactic Medium and the Interstellar Medium in a Star-forming Galaxy in the First Gyr After the Big Bang
• Physical Properties of Molecular Clouds at 2 parsec Resolution in the Low-Metallicity Dwarf Galaxy NGC 6822 and the Milky Way
• Exploring the Origin and Fate of the Magellanic Stream with Ultraviolet and Optical Absorption
• Constraining planet structure and composition from stellar chemistry: trends in different stellar populations
• The ALMA Fornax Cluster Survey I: stirring and stripping of the molecular gas in cluster galaxies
• The detection of [Ne v] emission in five blue compact dwarf galaxies
• The ARCiS framework for Exoplanet Atmospheres: Modelling Philosophy and Retrieval
• TOI-1338: TESS' First Transiting Circumbinary Planet
• Three-Dimensional Radiation-Hydrodynamics Calculations of the Envelopes of Young Planets Embedded in Protoplanetary Disks
• Carbonaceous dust grains seen in the first billion years of cosmic time
• Detailed dust modelling in the L-Galaxies semi-analytic model of galaxy formation
• Effect of low mass dark matter particles on the Sun
• Age and helium content of the open cluster NGC 6791 from multiple eclipsing binary members. I. Measurements, methods, and first results
• Towards universal hybrid star formation rate estimators
• Detection of neutral atomic species in the ultra-hot jupiter WASP-121b
• Exclusion of Cosmic Rays in Protoplanetary Disks. II. Chemical Gradients and Observational Signatures
• An empirical calibration to estimate cool dwarf fundamental parameters from H-band spectra
• The dependence of the galaxy mass-metallicity relation on environment and the implied metallicity of the IGM
• Near-Infrared Spectroscopy of TW Hya: A Revised Spectral Type and Comparison with Magnetospheric Accretion Models
• The R-Process Alliance: A Comprehensive Abundance Analysis of HD 222925, a Metal-Poor Star with an Extreme R-Process Enhancement of [Eu/H] = -0.14
• Stellar Abundances for Galactic Archaeology Database IV - Compilation of Stars in Dwarf Galaxies
• The CARMENES search for exoplanets around M dwarfs -- Photospheric parameters of target stars from high-resolution spectroscopy. II. Simultaneous multiwavelength range modeling of activity insensitive lines
• Five key exoplanet questions answered via the analysis of 25 hot Jupiter atmospheres in eclipse
• Absorbing gas around the WASP-12 planetary system
• The Hyades open cluster is chemically inhomogeneous
• ALFALFA Discovery of the Most Metal-Poor Gas-Rich Galaxy Known: AGC 198691
• Constraints on the Formation of the Galactic Bulge from Na, Al, and Heavy Element Abundances in Plaut's Field
• The Diverse Origins of Neutron-Capture Elements in the Metal-Poor Star HD 94028: Possible Detection of Products of i-process Nucleosynthesis
• Molecular Gas Dominated 50 kpc Ram Pressure Stripped Tail of the Coma Galaxy D100
• Radiative cooling of swept up gas in AGN-driven galactic winds and its implications for molecular outflows
• 3D Temperature Mapping of Solar Photospheric Fine Structure Using Ca II H Filtergrams
• Solar oxygen abundance
• Carbon-Enhanced Metal-Poor Stars: Relics from the Dark Ages
• The Rest-Frame Optical Spectroscopic Properties of Ly$\alpha$-Emitters at $z\sim 2.5$: The Physical Origins of Strong Ly$\alpha$ Emission
• Vertically resolved magma ocean-protoatmosphere evolution: H${}_2$, H${}_2$O, CO${}_2$, CH${}_4$, CO, O${}_2$, and N${}_2$ as primary absorbers
• Modelling the spectra of the kilonova AT2017gfo -- I: The photospheric epochs
• UV/Optical emission from the expanding envelopes of type II supernovae
• High Precision Differential Abundance Measurements in Globular Clusters: Chemical Inhomogeneities in NGC 6752
• WASP-77 Ab: A transiting hot Jupiter planet in a wide binary system
• X-ray scaling relations for a representative sample of Planck selected clusters observed with XMM-Newton
• A uniform metallicity in the outskirts of massive, nearby galaxy clusters
• Iron: A Key Element for Understanding the Origin and Evolution of Interstellar Dust
• The solar silicon abundance based on 3D non-LTE calculations
• Molecular Hydrogen in the Damped Lyman-alpha System towards GRB 120815A at z=2.36
• The Lifetime of Protoplanetary Disks in a Low-Metallicity Environment
• The ALMA view of the high-redshift relation between supermassive black holes and their host galaxies
• Stellar labels for hot stars from low-resolution spectra - I. the HotPayne method and results for 330,000 stars from LAMOST DR6
• The Large-scale Distribution of Cool Gas around Luminous Red Galaxies
• The Hamburg/ESO R-process Enhanced Star survey (HERES). V. Detailed abundance analysis of the r-process enhanced star HE 2327-5642
• Measurement of the 8B Solar Neutrino Flux with the KamLAND Liquid Scintillator Detector
• Optically-Thin Spatially-Resolved Mg II Emission Maps the Escape of Ionizing Photons
• Spectroscopic Properties of Star-Forming Host Galaxies and Type Ia Supernova Hubble Residuals in a Nearly Unbiased Sample
• Reproducing the Kinematics of Damped Lyman-alpha Systems
• A warm Neptune's methane reveals core mass and vigorous atmospheric mixing
• The Galactic Supernova Remnant W49B Likely Originates from a Jet-Driven, Core-Collapse Explosion
• Modeling Dust and Starlight in Galaxies Observed by Spitzer and Herschel: The KINGFISH Sample
• Scaling Properties of Galaxy Groups
• DarkBit: A GAMBIT module for computing dark matter observables and likelihoods
• Discovery of interstellar mercapto radicals (SH) with the GREAT instrument on SOFIA
• Neutron-Capture Nucleosynthesis in the First Stars
• Carbon star formation as seen through the non-monotonic initial-final mass relation
• Principal Component Analysis on Chemical Abundances Spaces
• Rocky super-Earths or waterworlds: the interplay of planet migration, pebble accretion and disc evolution
• How drifting and evaporating pebbles shape giant planets II: Volatiles and refractories in atmospheres
• On using the CMD morphology of M67 to test solar abundances
• Nucleosynthesis in a Primordial Supernova: Carbon and Oxygen Abundances in SMSS J031300.36-670839.31
• New Avenues for Thermal Inversions in hot Jupiters
• 3D NLTE spectral line formation of lithium in late-type stars
• s-Processing in the Galactic Disk. I. Super-Solar Abundances of Y, Zr, La, Ce in Young Open Clusters
• Dust Destruction by the Reverse Shock in the Cassiopeia A Supernova Remnant
• Dense cloud cores revealed by CO in the low metallicity dwarf galaxy WLM
• The impact of stellar rotation on the black hole mass-gap from pair-instability supernovae
• PS1-10bzj: A Fast, Hydrogen-Poor Superluminous Supernova in a Metal Poor Host Galaxy
• Astrophysical turbulence modeling
• PEPSI deep spectra. I. The Sun-as-a-star
• Study of the inner dust envelope and stellar photosphere of the AGB star R Doradus using SPHERE/ZIMPOL
• Nuclear Outflow of the Milky Way: Studying the Kinematics and Spatial Extent of the Northern Fermi Bubble
• Chemical Diversity in Protoplanetary Disks and Its Impact on the Formation History of Giant Planets
• TEA: A Code for Calculating Thermochemical Equilibrium Abundances
• Star-formation history and X-ray binary populations: the case of the Large Magellanic Cloud
• Grain opacity and the bulk composition of extrasolar planets. I. Results from scaling the ISM opacity
• The R-process Alliance: First Magellan/MIKE Release from the Southern Search for R-Process-enhanced Stars
• Forward seismic modelling of the pulsating magnetic B-type star HD 43317
• Influence of sub- and super-solar metallicities on the compositions of solid planetary building blocks
• Formation of Organic Molecules and Water in Warm Disk Atmospheres
• The LOFAR Two-metre Sky Survey Deep Fields Data Release 1: V. Survey description, source classifications and host galaxy properties
• Terrestrial modification of the Ivuna meteorite and a reassessment of the chemical composition of the CI type specimen
• The Type Icn SN 2021csp: Implications for the Origins of the Fastest Supernovae and the Fates of Wolf-Rayet Stars
• Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. I. Spatially Resolved Mass Outflow Rates for the Seyfert 2 Galaxy Markarian 573
• Nitrogen hydrides and the H2 ortho-to-para ratio in dark clouds
• The millimeter IRAM-30m line survey toward IK Tau
• Two massive rocky planets transiting a K-dwarf 6.5 parsecs away
• Multiphase Gas In Galaxy Halos: The OVI Lyman-limit System toward J1009+0713
• The Southern Stellar Stream Spectroscopic Survey (S5): Chemical Abundances of Seven Stellar Streams
• Hydrogen delivery onto white dwarfs from remnant exo-Oort cloud comets
• Comprehensive Study of a z = 2.35 DLA Galaxy: Mass, Metallicity, Age, Morphology and SFR from HST and VLT
• Legacy of star formation in the pre-reionization universe
• The ESO UVES Advanced Data Products Quasar Sample - VI. Sub-Damped Lyman-$\alpha$ Metallicity Measurements and the Circum-Galactic Medium
• Carina OB Stars: X-ray Signatures of Wind Shocks and Magnetic Fields
• Tracing the evolution of NGC6397 through the chemical composition of its stellar populations
• A new equation of state for dense hydrogen-helium mixtures II: taking into account hydrogen-helium interactions
• The R-Process Alliance: 2MASS J09544277+5246414, the Most Actinide-Enhanced R-II Star Known
• An emission spectrum for WASP-121b measured across the 0.8-1.1 micron wavelength range using the Hubble Space Telescope
• Spectroscopic and physical parameters of Galactic O-type stars. III. Mass discrepancy and rotational mixing
• SD 1313-0019 -- Another second-generation star with [Fe/H] = -5.0, observed with the Magellan Telescope
• The oldest and most metal poor stars in the APOSTLE Local Group simulations
• Metal-Poor Stars Observed with the Magellan Telescope. III. New Extremely and Ultra Metal-Poor Stars from SDSS/SEGUE and Insights on the Formation of Ultra Metal-Poor Stars
• 3D Model Atmospheres for Extremely Low-Mass White Dwarfs
• Chemical Abundances of Main-Sequence, Turnoff, Subgiant and red giant Stars from APOGEE spectra II: Atomic Diffusion in M67 Stars
• New insights on Ba over-abundance in open clusters. Evidence for the intermediate neutron-capture process at play?
• Heavy metal rules. I. Exoplanet incidence and metallicity
• Kronos & Krios: Evidence for accretion of a massive, rocky planetary system in a comoving pair of solar-type stars
• Dual constraints with ALMA: new [O III] 88 $\mu$m and dust-continuum observations reveal the ISM conditions of luminous LBGs at $z\sim 7$
• SDSS IV MaNGA -- Metallicity and ionisation parameter in local star-forming galaxies from Bayesian fitting to photoionisation models
• 3D NLTE analysis of the most iron-deficient star, SMSS0313-6708
• SPECIES I: Spectroscopic Parameters and atmosphEric ChemIstriEs of Stars
• PoWR grids of non-LTE model atmospheres for OB-type stars of various metallicities
• The first stars: CEMP--no stars and signatures of spinstars
• Planetesimal Compositions in Exoplanet Systems
• Measuring mass-loss rates and constraining shock physics using X-ray line profiles of O stars from the Chandra archive
• The i-process yields of rapidly-accreting white dwarfs from multicycle He-shell flash stellar evolution models with mixing parameterizations from 3D hydrodynamics simulations
• Transit detection of the long-period volatile-rich super-Earth ${\nu }^2$ Lupi d with $CHEOPS$
• Using dust, gas and stellar mass selected samples to probe dust sources and sinks in low metallicity galaxies
• Synthetic catalog of black holes in the Milky Way
• Growth and structure of multiphase gas in the cloud-crushing problem with cooling
• Directional Dark Matter Detection Beyond the Neutrino Bound
• Spectroscopic characterization of HD 95086 b with the Gemini Planet Imager
• The metallicity signature of evolved stars with planets
• JADES: Carbon enrichment 350 Myr after the Big Bang in a gas-rich galaxy
• The solar photospheric abundance of carbon.Analysis of atomic carbon lines with the CO5BOLD solar model
• Stellar origin of the 182Hf cosmochronometer and the presolar history of solar system matter
• The extent of chemically enriched gas around star-forming dwarf galaxies
• The COS/UVES Absorption Survey of the Magellanic Stream: II. Evidence for a complex enrichment history of the Stream from the Fairall 9 sightline
• The chemical compositions of solar twins in the open cluster M67
• The dependence of convective core overshooting on stellar mass: reality check, and additional evidence
• Using late-time optical and near-infrared spectra to constrain Type Ia supernova explosion properties
• Non-LTE line formation of Fe in late-type stars IV: Modelling of the solar centre-to-limb variation in 3D
• Dust Attenuation, Star Formation, and Metallicity in z ~ 2-3 Galaxies from KBSS-MOSFIRE
• Relative abundance constraints from high-resolution optical transmission spectroscopy of WASP-121b, and a fast model-filtering technique for accelerating retrievals
• The NIRVANDELS Survey: a robust detection of $\alpha$-enhancement in star-forming galaxies at $z\simeq 3.4$
• Chemical Composition of Faint (I~21 mag) Microlensed Bulge Dwarf OGLE-2007-BLG-514S
• Remnants and ejecta of thermonuclear electron-capture supernovae: Constraining oxygen-neon deflagrations in high-density white dwarfs
• Impact of rotation and disc lifetime on pre-main sequence lithium depletion of solar-type stars
• Stellar parameters for TRAPPIST-1
• The MOSDEF-LRIS Survey: The Interplay Between Massive Stars and Ionized Gas in High-Redshift Star-Forming Galaxies
• Faint Population III supernovae as the origin of the most iron-poor stars
• Detecting isotopologues in exoplanet atmospheres using ground-based high-dispersion spectroscopy
• Particle-physics constraints from the globular cluster M5: Neutrino Dipole Moments
• Nitrogen line spectroscopy in O-stars -- III. The earliest O-stars
• The light curve of SN 1987A revisited: constraining production masses of radioactive nuclides
• CNO abundances in the globular clusters NGC 1851 and NGC 6752
• Sn 2008in - bridging the gap between normal and faint supernovae of type IIP
• WASP-South transiting exoplanets: WASP-130b, WASP-131b, WASP-132b, WASP-139b, WASP-140b, WASP-141b & WASP-142b
• Constraints on core-collapse supernova progenitors from explosion site integral field spectroscopy
• Planetary Populations in the Mass-Period Diagram: A Statistical Treatment of Exoplanet Formation and the Role of Planet Traps
• Three Ancient Halo Subgiants: Precise Parallaxes, Compositions, Ages, and Implications for Globular Clusters
• Temperature-based metallicity measurements at z=0.8: direct calibration of strong-line diagnostics at intermediate redshift
• The host galaxy of the super-luminous SN 2010gx and limits on explosive nickel-56 production
• The mass-metallicity relation at z~1.4 revealed with Subaru/FMOS
• Metal-Poor Lithium-Rich Giants in the Radial Velocity Experiment Survey
• Double detonations of sub-Chandrasekhar mass CO white dwarfs: Can different core and He shell masses explain variations of Type Ia supernovae?
• The Type II-Plateau Supernova 2017eaw in NGC 6946 and Its Red Supergiant Progenitor
• The ACS LCID project. X. The Star Formation History of IC 1613: Revisiting the Over-Cooling Problem
• WASP-35b, WASP-48b and WASP-51b: Two new planets and an independent discovery of HAT-P-30b
• Determining the initial helium abundance of the Sun
• Age dating of an early Milky Way merger via asteroseismology of the naked-eye star $\nu$ Indi
• Effective temperature determinations of late-type stars based on 3D non-LTE Balmer line formation
• NGC 1624-2: A slowly rotating, X-ray luminous Of?cp star with an extraordinarily strong magnetic field
• Comprehensive abundance analysis of red giants in the open clusters NGC 752, NGC 1817, NGC 2360 and NGC 2506
• The bright Type IIP SN 2009bw, showing signs of interaction
• Interior Models of Saturn: Including the Uncertainties in Shape and Rotation
• Fundamental properties of nearby single early B-type stars
• The Star-Planet Connection I: Using Stellar Composition to Observationally Constrain Planetary Mineralogy for the Ten Closest Stars
• High-Redshift Metals. II. Probing Reionization Galaxies with Low-Ionization Absorption Lines at Redshift Six
• Neutron star mergers and rare core-collapse supernovae as sources of r-process enrichment in simulated galaxies
• Metallicity at the explosion sites of interacting transients
• HST hot-Jupiter transmission spectral survey: Clear skies for cool Saturn WASP-39b
• The COS/UVES Absorption Survey of the Magellanic Stream: I. One-Tenth Solar Abundances along the Body of the Stream
• The warm, the excited, and the molecular gas: GRB 121024A shining through its star-forming galaxy
• Multisite spectroscopic seismic study of the beta Cep star V2052 Oph: inhibition of mixing by its magnetic field
• Observational evidence of a slow downfall of star formation efficiency in massive galaxies during the last 10 Gyr
• Metallicity of stars formed throughout the cosmic history based on the observational properties of star forming galaxies
• Element Abundances in Solar Energetic Particles and the Solar Corona
• TESS Hunt for Young and Maturing Exoplanets (THYME) VI: an 11 Myr giant planet transiting a very low-mass star in Lower Centaurus Crux
• The metallicity and dust content of a redshift 5 gamma-ray burst host galaxy
• First Insights into the ISM at $z>8$ with JWST: Possible Physical Implications of a High [O III]$\lambda 4363$/[O III]$\lambda 5007$
• Toward the analysis of JWST exoplanet spectra: Identifying troublesome model parameters
• A Carbon-enhanced Metal-poor Damped Lyman alpha System: Probing Gas from Population III Nucleosynthesis?
• Models of the circumstellar medium of evolving, massive runaway stars moving through the Galactic plane
• X-shooter observations of main sequence stars in the globular cluster NGC 2808: first chemical tagging of a He-normal and a He-rich dwarf
• Constraints on Super-Earths Interiors from Stellar Abundances
• PPPC 4 DM$\nu$: A Poor Particle Physicist Cookbook for Neutrinos from DM annihilations in the Sun
• Project AMIGA: The Circumgalactic Medium of Andromeda
• Direct detection of dark energy: the XENON1T excess and future prospects
• Post first dredge-up [C/N] ratio as age indicator. Theoretical calibration
• Dust-depletion sequences in damped Lyman-α absorbers: a unified picture from low-metallicity systems to the Galaxy
• Simultaneous IRIS and Hinode/EIS observations and modelling of the 27 October 2014 X 2.0 class flare
• QSO Absorption Systems Detected in Ne VIII: High-Metallicity Clouds with a Large Effective Cross Section
• Metallicity inhomogeneities in local star-forming galaxies as sign of recent metal-poor gas accretion
• Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in planets I. From the PMS to the RGB at solar metallicity
• Hot gas around SN 1998bw: Inferring the progenitor from its environment
• Synthetic Stellar Photometry - II. Testing the bolometric flux scale, and tables of bolometric corrections for the Hipparcos/Tycho, Pan-STARRS1, SkyMapper and JWST systems
• CHEOPS observations of the HD 108236 planetary system: A fifth planet, improved ephemerides, and planetary radii
• Phosphorus in the Young Supernova Remnant Cassiopeia A
• The lowest detected stellar Fe abundance: The halo star SMSS J160540.18-144323.1
• There is no magnetic braking catastrophe: Low-mass star cluster and protostellar disc formation with non-ideal magnetohydrodynamics
• IMF and [Na/Fe] abundance ratios from optical and NIR Spectral Features in Early-type Galaxies
• Testing metallicity indicators at z~1.4 with the gravitationally lensed galaxy CASSOWARY 20
• Temperature and Metallicity Gradients in the Hot Gas Outflows of M82
• Changing the ${\nu }_{\max }$ Scaling Relation: The Need For a Mean Molecular Weight Term
• Characterizing the Circumgalactic Medium of Nearby Galaxies with HST/COS and HST/STIS Absorption-Line Spectroscopy: II. Methods and Models
• A high precision chemical abundance analysis of the HAT-P-1 stellar binary: constraints on planet formation
• MUSE searches for galaxies near very metal-poor gas clouds at z~3: new constraints for cold accretion models
• The Broad-band Counterpart of the Short GRB 200522A at $z=0.5536$: A Luminous Kilonova or a Collimated Outflow with a Reverse Shock?
• Moderately Luminous type II Supernovae
• Evidence for Late-stage Eruptive Mass-loss in the Progenitor to SN2018gep, a Broad-lined Ic Supernova: Pre-explosion Emission and a Rapidly Rising Luminous Transient
• Far-infrared metallicity diagnostics: Application to local ultraluminous infrared galaxies
• Gaia17biu/SN 2017egm in NGC 3191: The closest hydrogen-poor superluminous supernova to date is in a "normal", massive, metal-rich spiral galaxy
• The Evolution of O I over 3.2 < z < 6.5: Reionization of the Circumgalactic Medium
• Impact of radial migration on stellar and gas radial metallicity distribution
• Oxygen lines in solar granulation. II. Centre-to-limb variation, NLTE line formation, blends and the solar oxygen abundance
• CLASSY IV: Exploring UV diagnostics of the interstellar medium in local high-$z$ analogs at the dawn of the JWST era
• The Mean Ultraviolet Spectrum of a Representative Sample of Faint z~3 Lyman Alpha Emitters
• VLT spectroscopy of low-metallicity emission-line galaxies: abundance patterns and abundance discrepancies
• Electron-capture supernovae as origin of 48Ca
• AmFm and lithium gap stars: Stellar evolution models with mass loss
• Optical phase curve of the ultra-hot Jupiter WASP-121b
• Physical conditions in the gas phases of the giant HII region LMC-N11 unveiled by Herschel - I. Diffuse [CII] and [OIII] emission in LMC-N11B
• Optical and Near-IR Observations of the Faint and Fast 2008ha-like Supernova 2010ae
• Inelastic O+H collisions and the OI 777nm solar centre-to-limb variation
• Spectroscopic analysis of metal-poor stars from LAMOST: early results
• The Dependence of Theoretical Synthetic Spectra on $\alpha$-enhancement in Young, Binary Stellar Populations
• Equilibrium Model Constraints on Baryon Cycling Across Cosmic Time
• The peculiar Type Ia supernova iPTF14atg: Chandrasekhar-mass explosion or violent merger?
• The Interaction of the Fermi Bubbles with the Milky Way's Hot Gas Halo
• Chemical signatures of planets: beyond solar-twins
• Binarity among CEMP-no stars: an indication of multiple formation pathways?
• The origin of ICM enrichment in the outskirts of present-day galaxy clusters from cosmological hydrodynamical simulations
• The GJ 504 system revisited. Combining interferometric, radial velocity, and high contrast imaging data
• Very Large Interstellar Grains as Evidenced by the Mid-Infrared Extinction
• Thermal Phases of the Neutral Atomic Interstellar Medium -- from Solar Metallicity to Primordial Gas
• Extremely metal-poor galaxies with HST/COS: laboratories for models of low-metallicity massive stars and high-redshift galaxies
• The Fates of the Circumgalactic Medium in the FIRE Simulations
• 3D-HST Grism Spectroscopy of a Gravitationally Lensed, Low-metallicity Starburst Galaxy at z=1.847
• The Distribution of Metals in Cosmological Hydrodynamical Simulations of Dwarf Disk Galaxies
• What are the Sources of Solar Energetic Particles? Element Abundances and Source Plasma Temperatures
• The origin of dust in galaxies revisited: the mechanism determining dust content
• Discovery of a Perseus-like cloud in the early Universe: HI-to-H2 transition, carbon monoxide and small dust grains at zabs=2.53 towards the quasar J0000+0048
• Exothermic Double-Disk Dark Matter
• Are There Any Stars Lacking Neutron-Capture Elements? Evidence from Strontium and Barium
• The physics of gas phase metallicity gradients in galaxies
• On the fate of the secondary white dwarf in double-degenerate double-detonation Type Ia supernovae
• Lya escape from z~0.03 star-forming galaxies: the dominant role of outflows
• Equatorial anti-rotating day side wind flow in WASP-43b elicited by deep wind jets?
• Planetary Ices and the Linear Mixing Approximation
• Implications of the large OVI columns around low-redshift $L_{\ast }$ galaxies
• Column Density Profiles of Multi-Phase Gaseous Halos
• The Hazy and Metal-Rich Atmosphere of GJ 1214 b Constrained by Near and Mid-Infrared Transmission Spectroscopy
• From dense hot Jupiter to low-density Neptune: The discovery of WASP-127b, WASP-136b and WASP-138b
• The Massive Progenitor of the Possible Type II-Linear Supernova 2009hd in Messier 66
• Global Hydromagnetic Simulations of Protoplanetary Disks with Stellar Irradiation and Simplified Thermochemistry
• High-resolution spectroscopy of extremely metal-poor stars in the least evolved galaxies: Bootes II
• The Ionized Gas in Nearby Galaxies as Traced by the [NII] 122 and 205 μm Transitions
• An extensive VLT/X-Shooter library of photospheric templates of pre-main sequence stars
• Discovery of the benchmark metal poor T8 dwarf BD+01 2920B
• Metallicity dependence of HMXB populations
• Analysis of Early Science observations with the CHaracterising ExOPlanets Satellite (CHEOPS) using pycheops
• ΔY/ ΔZ from the analysis of local K dwarfs
• The First Billion Years project: constraining the dust attenuation law of star-forming galaxies at z $\simeq$ 5
• Sodium and Oxygen Abundances in the Open Cluster NGC 6791 from APOGEE H-Band Spectroscopy
• A Comparison of Stellar Elemental Abundance Techniques and Measurements
• SN 2010lp---a Type Ia supernova from a violent merger of two carbon--oxygen White Dwarfs
• Three-dimensional modeling of the Ca II H&K lines in the solar atmosphere
• New insights into the dust formation of oxygen-rich AGB stars
• Nebular phase observations of the type-Ib supernova iPTF13bvn favour a binary progenitor
• MultiDark-Galaxies: data release and first results
• Chemical Analysis of the Ninth Magnitude Carbon-Enhanced Metal-Poor Star BD+44 493
• Carbon and oxygen abundance gradients in NGC300 and M33 from optical recombination lines
• The Cosmic Evolution of the Metallicity Distribution of Ionized Gas Traced by Lyman Limit Systems
• Distinguishing oceans of water from magma on mini-Neptune K2-18b
• The Efficiency of Stellar Reionization: Effects of Rotation, Metallicity, and Initial Mass Function
• Beyond the Kepler/K2 bright limit: variability in the seven brightest members of the Pleiades
• Iron and alpha-element Production in the First One Billion Years after the Big Bang
• Barium & related stars and their white-dwarf companions II. Main-sequence and subgiant stars
• The Evolution and Properties of Rotating Massive Star Populations
• An Extreme Metallicity, Large-Scale Outflow from a Star-Forming Galaxy at z ~ 0.4
• The COS Absorption Survey of Baryon Harbors (CASBaH): Warm-hot Circumgalactic Gas Reservoirs Traced by Ne VIII Absorption
• The Submm and mm Excess of the SMC: Magnetic Dipole Emission from Magnetic Nanoparticles?
• Impacts of radiative accelerations on solar-like oscillating main-sequence stars
• The Herschel Virgo Cluster Survey. IX. Dust-to-gas mass ratio and metallicity gradients in four Virgo spiral galaxies
• Nebular Excitation in z~2 Star-forming Galaxies from the SINS and LUCI Surveys: The Influence of Shocks and AGN
• The eccentric massive binary V380 Cyg: revised orbital elements and interpretation of the intrinsic variability of the primary component
• CO/H2, C/CO, OH/CO, and OH/O2 in Dense Interstellar Gas: From High Ionization to Low Metallicity
• Opportunities for Fundamental Physics Research with Radioactive Molecules
• Extremely Metal-Poor Representatives Explored by the Subaru Survey (EMPRESS). I. A Successful Machine Learning Selection of Metal-Poor Galaxies and the Discovery of a Galaxy with M*<10^6 M_sun and 0.016 Z_sun
• NGC 2579 and the carbon and oxygen abundance gradients beyond the solar circle
• Quasars probing intermediate redshift star-forming galaxies
• Endurance of SN 2005ip after a decade: X-rays, radio, and H-alpha like SN 1988Z require long-lived pre-supernova mass loss
• The Metallicity Evolution of Star-Forming Galaxies from Redshift 0 to 3: Combining Magnitude Limited Survey with Gravitational Lensing
• Wind bubbles within H II regions around slowly moving stars
• The Sloan Digital Sky Survey Reverberation Mapping Project: Rapid CIV Broad Absorption Line Variability
• Direct Imaging and Astrometric Detection of a Gas Giant Planet Orbiting an Accelerating Star
• Directly imaging damped Ly-alpha galaxies at z>2. III: The star formation rates of neutral gas reservoirs at z~2.7
• The most metal-poor damped Lyman alpha systems: An insight into dwarf galaxies at high redshift
• Optical IFU Observations of the Brightest Cluster Galaxy NGC 4696: The Case for a Minor Merger and Shock-excited Filaments
• The Very Massive Star Content of the Nuclear Star Clusters in NGC 5253
• The magnetic fields of intermediate-mass T Tauri stars : I. Magnetic detections and fundamental stellar parameters
• A Tale of Two Anomalies: Depletion, Dispersion, and the Connection Between the Stellar Lithium Spread and Inflated Radii on the Pre-Main Sequence
• Deep Atmosphere Composition, Structure, Origin, and Exploration, with Particular Focus on Critical in situ Science at the Icy Giants
• Metal-Poor Stars Observed with the Magellan Telescope I. Constraints on Progenitor Mass and Metallicity of AGB Stars Undergoing s-Process Nucleosynthesis
• Ground-Based Transit Spectroscopy of the Hot-Jupiter WASP-19b in the Near-Infrared
• Long-term evolution of a magnetic massive merger product
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• Breaking Degeneracies in Formation Histories by Measuring Refractory Content in Gas Giants
• Star Formation in Accretion Disks and SMBH Growth
• Primordial 4He abundance: a determination based on the largest sample of HII regions with a methodology tested on model HII regions
• Measurements of Absolute Abundances in Solar Flares
• Iron and silicate dust growth in the Galactic interstellar medium: clues from element depletions
• The Solar-Stellar Connection
• Characterizing Transition Temperature Gas in the Galactic Corona
• Modeling the Anomalous Microwave Emission with Spinning Nanoparticles: No PAHs Required
• H-alpha features with hot onsets. I. Ellerman bombs
• Spectroscopic Comparison of Metal-Rich RRab Stars of the Galactic Field with Their Metal-Poor Counterparts
• Massive Dead Galaxies at z~2 with HST Grism Spectroscopy I. Star Formation Histories and Metallicity Enrichment
• The surface nitrogen abundance of a massive star in relation to its oscillations, rotation, and magnetic field
• Effect of uncertainties in stellar model parameters on estimated masses and radii of single stars
• Detection of (15)NNH+ in L1544: non-LTE modelling of dyazenilium hyperfine line emission and accurate (14)N/(15)N values
• Asteroseismic estimate of helium abundance of a solar analog binary system
• Chemo-dynamics of outer halo dwarf stars, including \textit{Gaia}-Sausage and \textit{Gaia}-Sequoia candidates
• Red Supergiant Stars as Cosmic Abundance Probes: KMOS Observations in NGC 6822
• Evidence for an aspherical Population III supernova explosion inferred from the hyper metal-poor star HE1327-2326
• Interacting supernovae from photoionization-confined shells around red supergiant stars
• The maximum accretion rate of hot gas in dark matter halos
• The Absence of an Environmental Dependence in the Mass-Metallicity Relation at z=2
• Nine New Metal-Poor Stars on the Subgiant and Red Horizontal Branches with High Levels of r-process Enhancement
• Quasars Probing Quasars VIII. The Physical Properties of the Cool Circumgalactic Medium Surrounding z ~ 2-3 Massive Galaxies Hosting Quasars
• Evolution of accretor stars in massive binaries: broader implications from modeling ζ Ophiuchi
• NLTE model atmospheres for the hottest white dwarfs: Spectral analysis of the compact component in nova V4743 Sgr
• The Effects of Stellar Population and Gas Covering Fraction on the Emergent Lyman Alpha Emission of High-Redshift Galaxies
• Carbon-rich planet formation in a solar composition disk
• A High-Resolution Spectroscopic Search for the Remaining Donor for Tycho's Supernova
• KIC 3240411 - the hottest known SPB star with the asymptotic g-mode period spacing
• Supersolar Ni/Fe production in the Type IIP SN 2012ec
• Two chemically similar stellar overdensities on opposite sides of the plane of the Galaxy
• The Contour Method: a new approach to finding modes of non-adiabatic stellar pulsations
• Solar neutrinos, helioseismology and the solar internal dynamics
• Reionization in Technicolor
• Automatic Determination of Stellar Parameters via Asteroseismology of Stochastically Oscillating Stars: Comparison with Direct Measurements
• An extremely metal poor star complex in the reionization era: Approaching Population III stars with JWST
• Stripped gas as fuel for newly formed HII regions in the encounter between VCC1249 and M49: a unified picture from NGVS and GUViCS
• A Comprehensive Comparative Test of Seven Widely-Used Spectral Synthesis Models Against Multi-Band Photometry of Young Massive Star Clusters
• RAVE J203843.2-002333: The first highly r-process-enhanced star identified in the RAVE survey
• New catalogue of Chemically Peculiar stars, and Statistical Analysis
• The Non-Uniformity of Galaxy Cluster Metallicity Profiles
• Period spacings of $\gamma$ Doradus pulsators in the \textit{Kepler} field: Rossby and gravity modes in 82 stars
• Carbon-enhanced metal-poor stars: a window on AGB nucleosynthesis and binary evolution. II. Statistical analysis of a sample of 67 CEMP-$s$ stars
• Rapid contraction of giant planets orbiting the 20 million-years old star V1298 Tau
• Molecular Cross Sections for High Resolution Spectroscopy of Super Earths, Warm Neptunes and Hot Jupiters
• AKARI Observations of Brown Dwarfs I.: CO and CO_2 Bands in the Near-Infrared Spectra
• Evolutionary tracks for Betelgeuse
• 7Be Solar Neutrino Measurement with KamLAND
• Metal-poor star formation triggered by the feedback effects from Pop III stars
• An MCMC determination of the primordial helium abundance
• Estimating gas masses and dust-to-gas ratios from optical spectroscopy
• Improvements to Stellar Structure Models, Based on a Grid of 3D Convection Simulations. I. $T(\tau )$-Relations
• Starbursting [O III] emitters and quiescent [C II] emitters in the reionization era
• Chemically Homogeneous Evolution: A rapid population synthesis approach
• Mid-Infrared Spectroscopy of Uranus from the Spitzer Infrared Spectrometer: 1. Determination of the Mean Temperature Structure of the Upper Troposphere and Stratosphere
• Lithium abundance patterns of late-F stars: an in-depth analysis of the lithium desert
• Chemical Abundances of Main-Sequence, Turn-off, Subgiant and red giant Stars from APOGEE spectra I: Signatures of Diffusion in the Open Cluster M67
• Potential Impact of Fast Flavor Oscillations on Neutrino-driven Winds and Their Nucleosynthesis
• The Cosmic Ultraviolet Baryon Survey (CUBS) I. Overview and the diverse environments of Lyman limit systems at z<1
• LBT/LUCIFER Observations of the z~2 Lensed Galaxy J0900+2234
• Near-ultraviolet Spectroscopy of Star-forming Galaxies from eBOSS: Signatures of Ubiquitous Galactic-scale Outflows
• A Clear View of a Cloudy Brown Dwarf Companion from High-Resolution Spectroscopy
• The solar-like CoRoT target HD 170987: spectroscopic and seismic observations
• Planetary Nebulae: Sources of Enlightenment
• Carbon-enhanced metal-poor stars: a window on AGB nucleosynthesis and binary evolution. I. Detailed analysis of 15 binary stars with known orbital periods
• Binary population synthesis with probabilistic remnant mass and kick prescriptions
• The metals-to-dust ratio to very low metallicities using GRB and QSO absorbers; extremely rapid dust formation
• Atmospheric NLTE-models for the spectroscopic analysis of blue stars with winds. IV. Porosity in physical and velocity space
• The Gaia-ESO Survey: open clusters in Gaia-DR1 - a way forward to stellar age calibration
• The Curious Case of Elemental Abundance Differences in the Dual Hot Jupiter Hosts WASP-94AB
• Abundance gradients in spiral disks: is the gradient inversion at high redshift real?
• Nuclear astrophysics: the unfinished quest for the origin of the elements
• Unveiling the dust nucleation zone of IRC+10216 with ALMA
• Gas phase Elemental abundances in Molecular cloudS (GEMS) VII. Sulfur elemental abundance
• Testing the effects of opacity and the chemical mixture on the excitation of pulsations in B stars of the Magellanic Clouds
• Metal-Poor Stars and the Chemical Enrichment of the Universe
• The Impact of Metallicity on the Evolution of Rotation and Magnetic Activity of Sun-Like Stars
• Can plume-induced internal gravity waves regulate the core rotation of subgiant stars?
• Unveiling cloudy exoplanets: the influence of cloud model choices on retrieval solutions
• Nebular water depletion as the cause of Jupiter's low oxygen abundance
• The distribution of gas in the Local Group from constrained cosmological simulations: the case for Andromeda and the Milky Way galaxies
• Old puzzle, new insights: a lithium rich giant quietly burning helium in its core
• First submillimeter observation of CO in the stratosphere of Uranus
• The atmospheric chemistry of the warm Neptune GJ 3470b: influence of metallicity and temperature on the CH4/CO ratio
• Evolution of the Milky Way with radial motions of stars and gas II. The evolution of abundance profiles from H to Ni
• Neutron-capture element deficiency of the Hercules dwarf spheroidal galaxy
• The Gaia-ESO Survey: a new approach to chemically characterising young open clusters
• The ISM scaling relations in DustPedia late-type galaxies: A benchmark study for the Local Universe
• Predicting the Presence of Companions for Stripped-Envelope Supernovae: The Case of the Broad-Lined Type Ic SN 2002ap
• iPTF16asu: A Luminous, Rapidly-Evolving, and High-Velocity Supernova
• The Brightest Young Star Clusters in NGC 5253
• The Calibration of Star Formation Rate Indicators for WISE 22 Micron Selected Galaxies in the SDSS
• Short Lifetime of Protoplanetary Disks in Low-metallicity Environments
• Metal deficiency in cluster star-forming galaxies at z=2
• A Comparative Study of Long and Short GRBs. I. Overlapping Properties
• Coping with loss: Stability of mass transfer from post-main sequence donor stars
• The MOSDEF Survey: Detection of [OIII]$\lambda$4363 and the direct-method oxygen abundance of a star-forming galaxy at z=3.08
• The formation of IRIS diagnostics V. A quintessential model atom of C II and general formation properties of the C II lines at 133.5 nm
• Diffuser-Assisted Infrared Transit Photometry for Four Dynamically Interacting \textit{Kepler} Systems
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• Stellar Yields of Rotating First Stars. I. Yields of Weak Supernovae and Abundances of Carbon-enhanced Hyper Metal Poor Stars
• The Metallicity of the Intracluster Medium Over Cosmic Time: Further Evidence for Early Enrichment
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• Solar Transition-Region Lines Observed by the Interface Region Imaging Spectrograph: Diagnostics for the O IV and Si IV Lines
• Beryllium and Alpha-Element Abundances in a Large Sample of Metal-Poor Stars
• Aurora: A Generalised Retrieval Framework for Exoplanetary Transmission Spectra
• Chemical evolution library for galaxy formation simulation
• Oxygen enrichment in carbon-rich planetary nebulae
• Massive Warm/Hot Galaxy Coronae: II. Isentropic Model
• The chemical evolution of the Bootes I ultra-faint dwarf galaxy
• Gravity-mode period spacings and near-core rotation rates of 611 $\gamma$ Doradus stars with \textit{Kepler}
• High-resolution abundance analysis of red giants in the globular cluster NGC 6522
• Metal-Poor Stars Observed with the Magellan Telescope II. Discovery of Four Stars with [Fe/H] < -3.5
• The puzzling chemical composition of GJ 436b's atmosphere: influence of tidal heating on the chemistry
• Calibration of the Mixing-Length Theory for Convective White Dwarf Envelopes
• KIC 3858884: a hybrid δ Sct pulsator in a highly eccentric eclipsing binary
• New predictions for radiation-driven, steady-state mass-loss and wind-momentum from hot, massive stars. I. Method and first results
• Direct evidence for a supernova interacting with a large amount of hydrogen-free circumstellar material
• Local tadpole galaxies: dynamics and metallicity
• Sparkling nights and very hot days on WASP-18b: the formation of clouds and the emergence of an ionosphere
• LYRA I: Simulating the multi-phase ISM of a dwarf galaxy with variable energy supernovae from individual stars
• Modelling Neutron Star-Black Hole Binaries: Future Pulsar Surveys and Gravitational Wave Detectors
• Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys
• Identifying close binary central stars of PN with Kepler
• The Search for Multiple Populations in Magellanic Cloud Clusters III: No evidence for Multiple Populations in the SMC cluster NGC 419
• A novel way of constraining WIMPs annihilations in the Sun: MeV neutrinos
• The ARAUCARIA project: Grid-Based Quantitative Spectroscopic Study of Massive Blue Stars in NGC55
• Observation of interstellar lithium in the low-metallicity Small Magellanic Cloud
• CO-dark molecular gas at high redshift: very large H${}_2$ content and high pressure in a low metallicity damped Lyman-alpha system
• Tracing the Cosmic Metal Evolution in the Low-Redshift Intergalactic Medium
• Retrieval survey of metals in six ultra-hot Jupiters: Trends in chemistry, rain-out, ionisation and atmospheric dynamics
• The Sensitivity of Convection Zone Depth to Stellar Abundances: An Absolute Stellar Abundance Scale from Asteroseismology
• Cosmic ray induced ionisation of a molecular cloud shocked by the W28 supernova remnant
• A Tale of Planet Formation: From Dust to Planets
• Long Term Spectral Evolution of Tidal Disruption Candidates Selected by Strong Coronal Lines
• Atmospheric Retrieval of Exoplanets
• Constraints on the Chemical Enrichment History of the Perseus Cluster of Galaxies from High-Resolution X-ray Spectroscopy
• The Physical Conditions of a Lensed Star-forming Galaxy at z=1.7
• Observable signatures of wind--driven chemistry with a fully consistent three dimensional radiative hydrodynamics model of HD 209458b
• Water content and wind acceleration in the envelope around the oxygen-rich AGB star IK Tau as seen by Herschel/HIFI
• Two bi-stability jumps in theoretical wind models for massive stars and the implications for Luminous Blue Variable supernovae
• The 2015 Decay of the Black Hole X-ray Binary V404 Cygni: Robust Disk-Jet Coupling and a Sharp Transition into Quiescence
• Evidence for Sub-Chandrasekhar Type Ia Supernovae from Stellar Abundances in Dwarf Galaxies
• Modelling Kepler Red Giants in Eclipsing Binaries:Calibrating the Mixing Length Parameter with Asteroseismology
• The spectral evolution of the first Galaxies. III. Simulated James Webb Space Telescope spectra of reionization-epoch galaxies with Lyman continuum leakage
• Unveiling the Secrets of Metallicity and Massive Star Formation Using DLAs along Gamma-ray Bursts
• Seismic evidence for near solid-body rotation in two Kepler subgiants and implications for angular momentum transport
• Observational Constraints on First-Star Nucleosynthesis. II. Spectroscopy of an Ultra Metal-Poor CEMP-no Star
• Searching for signatures of planet formation in stars with circumstellar debris discs
• Patchy Forsterite Clouds in the Atmospheres of Two Highly Variable Exoplanet Analogs
• [CII] 158 micron Emission from the Host Galaxies of Damped Lyman Alpha Systems
• Chemical (in)homogeneity and atomic diffusion in the open cluster M67
• The Kappa Andromedae System: New Constraints on the Companion Mass, System Age & Further Multiplicity
• Chemical Evolution on the Scale of Clusters of Galaxies: A Conundrum?
• The Magellan Uniform Survey of Damped Lyman alpha Systems I: Cosmic Metallicity Evolution
• On the dust abundance gradients in late-type galaxies: II. Analytical models as evidence for massive interstellar dust growth in SINGS galaxies
• A possible indication of momentum-dependent asymmetric dark matter in the Sun
• Diurnal variations in the stratosphere of the ultrahot giant exoplanet WASP-121b
• Classically and Asteroseismically constrained 1D Stellar Evolution Models of $\alpha$ Centauri A and B using Empirical Mixing Length Calibrations
• The chemistry of phosphorus-bearing molecules under energetic phenomena
• Evidence for a Dichotomy in the Interior Structures of Jupiter and Saturn from Helium Phase Separation
• Si IV Resonance Line Emission During Solar Flares: Non-LTE, Non-equilibrium, Radiation Transfer Simulations
• The collapse of a molecular cloud core to stellar densities using radiation non-ideal magnetohydrodynamics
• Non-LTE effects on the lead and thorium abundance determinations for cool stars
• Cumulative physical uncertainty in modern stellar models I. The case of low-mass stars
• A comparative study of host galaxy properties between Fast Radio Bursts and stellar transients
• Detection of Ongoing Mass Loss from HD 63433c, a Young Mini Neptune
• The nature of the Li enrichment in the most Li-rich giant star
• Post-AGB stars in the SMC as tracers of stellar evolution: the extreme s-process enrichment of the 21 micrometer star J004441.04-732136.4
• Luminous Red Novae: population models and future prospects
• What are little worlds made of? Stellar abundances and the building blocks of planets
• Far-Ultraviolet to Near-Infrared Observations of SN 2023ixf: A high energy explosion engulfed in complex circumstellar material
• The low-redshift intergalactic medium as seen in archival legacy Hubble/STIS and FUSE data
• CHAOS VI: Direct Abundances in NGC 2403
• Sodium and Potassium Signatures of Volcanic Satellites Orbiting Close-in Gas Giant Exoplanets
• Constraining the Origins of Neptune's Carbon Monoxide Abundance with CARMA Millimeter-wave Observations
• The GALAH Survey: Chemodynamics of the Solar Neighbourhood
• Partly burnt runaway stellar remnants from peculiar thermonuclear supernovae
• HICOSMO - Cosmology with a complete sample of galaxy clusters: I. Data analysis, sample selection and luminosity-mass scaling-relation
• The complex case of V445 Lyr observed with Kepler: Two Blazhko modulations, a non-radial mode, possible triple mode RR Lyrae pulsation, and more
• A physical model for the evolving UV luminosity function of high redshift galaxies and their contribution to the cosmic reionization
• Deuterated formaldehyde in rho Ophiuchi A
• Spectral Properties of Cool Stars: Extended Abundance Analysis of Kepler Objects of Interest
• Transit confirmation and improved stellar and planet parameters for the super-Earth HD 97658 b and its host star
• The IACOB project: A grid-based automatic tool for the quantitative spectroscopic analysis of O-stars
• The GAPS Programme with HARPS-N at TNG. X. Differential abundances in the XO-2 planet hosting binary
• The Stagger-grid: A Grid of 3D Stellar Atmosphere Models - II. Horizontal and Temporal Averaging and Spectral Line Formation
• The Future of Solar Neutrinos
• The Distribution of Alpha Elements in Andromeda Dwarf Galaxies
• The carbon-to-oxygen ratio in stars with planets
• The 3D thermal, dynamical and chemical structure of the atmosphere of HD 189733b: implications of wind-driven chemistry for the emission phase curve
• Bright Metal-Poor Stars from the Hamburg/ESO Survey. II. A Chemodynamical Analysis
• Constraining the PopIII IMF with high-z GRBs
• Low-metallicity Absorbers Account for Half of the Dense Circumgalactic Gas at z < 1
• The nature of proximate damped Lyman alpha systems
• From actinides to zinc: Using the full abundance pattern of the brightest star in Reticulum II to distinguish between different r-process sites
• Light WIMPs in the Sun: Constraints from Helioseismology
• Search for Extremely Metal-poor Galaxies in the Sloan Digital Sky Survey (II): high electron temperature objects
• The Gaia-ESO Survey: a quiescent Milky Way with no significant dark/stellar accreted disc
• A luminous and young galaxy at z=12.33 revealed by a JWST/MIRI detection of Hα and [OIII]
• Nitrogen line spectroscopy of O-stars -- I. Nitrogen III emission line formation revisited
• The Extreme High-Velocity Outflow in Quasar PG0935+417
• Ages and heavy element abundances from very metal-poor stars in the Sagittarius dwarf galaxy
• Dissecting the Gaseous Halos of z~2 Damped Ly$\alpha$ Systems with Close Quasar Pairs
• Dynamically Tagged Groups of Very Metal-poor Halo Stars from the HK and Hamburg/ESO Surveys
• The final data release of ALLSMOG: a survey of CO in typical local low-M* star-forming galaxies
• Three-dimensional simulations of gravitationally confined detonations compared to observations of SN 1991T
• Progenitors of Type IIb Supernovae: I. Evolutionary Pathways and Rates
• The Li-age correlation: the Sun is unusually Li deficient for its age
• Broad Non-Gaussian Fe XXIV Line Profiles in the Impulsive Phase of the 2017 September 10 X8.3 class Flare Observed by Hinode/EIS
• The spatial distribution of carbon dust in the early solar nebula and the carbon content of planetesimals
• Non-LTE analysis of K I in late-type stars
• The Effect of Star Formation on the Redshift Evolution of Interstellar Metals, Atomic and Molecular Gas in Galaxies
• Is the faint young Sun problem for Earth solved?
• The $\nu$ process in the light of an improved understanding of supernova neutrino spectra
• Discovery of extremely lead-rich subdwarfs: does heavy metal signal the formation of subdwarf B stars?
• Deciphering the oscillation spectrum of $\gamma$ Doradus and SPB stars
• Abundances of lithium, oxygen, and sodium in the turn-off stars of Galactic globular cluster 47 Tuc
• ALFALFA Discovery of the Nearby Gas-rich Dwarf Galaxy Leo P. V. Neutral Gas Dynamics and Kinematics
• A Bake-Off Between CMFGEN and FASTWIND: Modeling the Physical Properties of SMC and LMC O-type Stars
• Photoionization models of the CALIFA HII regions. I. Hybrid models
• Tidal Dissipation in WASP-12
• Nature of the Absorbing Gas associated with a Galaxy Group at z~0.4
• Deep Mixing in Evolved Stars. II. Interpreting Li Abundances in RGB and AGB Stars
• Heavy Element Dispersion in the Metal-Poor Globular Cluster M92
• Carbon and Oxygen Abundances in Cool Metal-rich Exoplanet Hosts: A Case Study of the C/O Ratio of 55 Cancri
• Evidence for the magnetar nature of 1E 161348-5055 in RCW 103
• The Implications of 3D Thermal Structure on 1D Atmospheric Retrieval
• VLT/X-shooter spectroscopy of the GRB 120327A afterglow
• On the evolutionary and pulsation mass of Classical Cepheids: III. the case of the eclipsing binary Cepheid CEP0227 in the Large Magellanic Cloud
• The MOSDEF-LRIS Survey: The Connection Between Massive Stars and Ionized Gas in Individual Galaxies at $z\sim 2$
• Population synthesis to constrain Galactic and Stellar Physics- I- Determining age and mass of thin-disc red-giant stars
• Chemical enrichment and physical conditions in I Zw 18
• Short-lived radioisotopes in meteorites from Galactic-scale correlated star formation
• Alive and well: a short review about standard solar models
• Jupiter formed as a pebble pile around the N${}_2$ ice line
• Scientific rationale of Saturn's in situ exploration
• The mass-metallicity relations for gas and stars in star-forming galaxies: strong outflow vs variable IMF
• First evidence of inertial modes in $\gamma$ Doradus stars: The core rotation revealed
• DES13S2cmm: The First Superluminous Supernova from the Dark Energy Survey
• Red Supergiant Stars as Cosmic Abundance Probes. III. NLTE effects in J-band Magnesium lines
• Deep ALMA redshift search of a z~12 GLASS-JWST galaxy candidate
• The Metallicity Dependence of the Minimum Mass for Core-Collapse Supernovae
• The Impact of Enhanced Iron Opacity on Massive Star Pulsations: Updated Instability Strips
• Chemical Signatures of the First Supernovae in the Sculptor Dwarf Spheroidal Galaxy
• The chemical evolution of local star forming galaxies: Radial profiles of ISM metallicity, gas mass, and stellar mass and constraints on galactic accretion and winds
• Seeding the Second Star: enrichment from population III, dust evolution, and cloud collapse
• A Bayesian approach to the modelling of alpha Cen A
• Late-Time Photometry of Type Ia Supernova SN 2012cg Reveals the Radioactive Decay of ${}^{57}$Co
• A spectroscopic study of blue supergiant stars in the Sculptor galaxy NGC 55: chemical evolution and distance
• Constraining stellar evolution theory with asteroseismology of $\gamma$ Doradus stars using deep learning
• Abundances in the Local Region I: G and K Giants
• Learning about the intermediate neutron-capture process from lead abundances
• On the Metallicity and Origin of the Smith High-Velocity Cloud
• The Pyrat Bay Framework for Exoplanet Atmospheric Modeling: A Population Study of Hubble/WFC3 Transmission Spectra
• Carbon monoxide emission lines reveal an inverted atmosphere in the ultra hot Jupiter WASP-33 b consistent with an eastward hot spot
• Asymmetric Type-Ia supernova origin of W49B as revealed from spatially resolved X-ray spectroscopic study
• Binary Asteroseismic Modelling: isochrone-cloud methodology and application to Kepler gravity-mode pulsators
• Chemical complexity in the Horsehead photodissociation region
• Chemical Abundances of new member stars in the Tucana II dwarf galaxy
• Jupiter's Ammonia Distribution Derived from VLA Maps at 3--37 GHz
• Heavy Element Absorption Systems at $5.0<z<6.8$: Metal-Poor Neutral Gas and a Diminishing Signature of Highly Ionized Circumgalactic Matter
• ZFIRE: Galaxy Cluster Kinematics, H$\alpha$ Star Formation Rates, and Gas-Phase Metallicities of XMM-LSS J02182-05102 at z=1.6233
• The BAyesian STellar Algorithm (BASTA): a fitting tool for stellar studies, asteroseismology, exoplanets, and Galactic archaeology
• NLTE for APOGEE: Simultaneous Multi-Element NLTE Radiative Transfer
• Modelling the Spectra of Planets, Brown Dwarfs and Stars using VSTAR
• The Herschel exploitation of local galaxy Andromeda (HELGA) V: Strengthening the case for substantial interstellar grain growth
• HyDRA-H: Simultaneous Hybrid Retrieval of Exoplanetary Emission Spectra
• The contribution from stars stripped in binaries to cosmic reionization of hydrogen and helium
• Cloud property trends in hot and ultra-hot giant gas planets (WASP-43b, WASP-103b, WASP-121b, HAT-P-7b, and WASP-18b)
• Detailed Abundances of Planet-Hosting Wide Binaries. I. Did Planet Formation Imprint Chemical Signatures in the Atmospheres of HD 20782/81?
• SN2019dge: a Helium-rich Ultra-Stripped Envelope Supernova
• Revisiting the pre-main-sequence evolution of stars I. Importance of accretion efficiency and deuterium abundance
• Asteroseismic inference on the spin-orbit misalignment and stellar parameters of HAT-P-7
• Cosmic Neutron Star Merger Rate and Gravitational Waves constrained by the R Process Nucleosynthesis
• The Tidal Disruption of Sun-like Stars by Massive Black Holes
• Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program IV. Carbon and C/O ratios for Galactic stellar populations and planet hosts
• 500 Days of SN 2013dy: spectra and photometry from the ultraviolet to the infrared
• Self-consistent predictions for LIER-like emission lines from post-AGB stars
• Sulfur Ice Astrochemistry: A Review of Laboratory Studies
• Unicorns and Giraffes in the binary zoo: stripped giants with subgiant companions
• Discovery of Multi-Phase Cold Accretion in a Massive Galaxy at z=0.7
• Abundances of carbon-enhanced metal-poor stars as constraints on their formation
• How Deep Is the Ocean? Exploring the phase structure of water-rich sub-Neptunes
• Enhanced constraints on the interior composition and structure of terrestrial exoplanets
• Measuring the stellar wind parameters in IGR J17544-2619 and Vela X-1 constrains the accretion physics in Supergiant Fast X-ray Transient and classical Supergiant X-ray Binaries
• Type II supernovae as probes of environment metallicity: observations of host HII regions
• Spectral modelling of the "Super-Chandra" Type Ia SN 2009dc - testing a 2 M_sun white dwarf explosion model and alternatives
• The Mass-Metallicity Relation at z=8: Direct-Method Metallicity Constraints and Near-Future Prospects
• Spitzer reveals what's behind Orion's Bar
• The missing gas problem in GRB host galaxies: evidence for a highly ionised component
• X-Shooting ULLYSES: massive stars at low metallicity. I. Project Description
• Comprehensive abundance analysis of red giants in the open clusters NGC 2527, 2682, 2482, 2539, 2335, 2251 and 2266
• Winds of low-metallicity OB-type stars: HST-COS spectroscopy in IC1613
• A stripped helium star in the potential black hole binary LB-1
• The first multi-dimensional view of mass loss from externally FUV irradiated protoplanetary discs
• Outflows and extended [CII] halos in high redshift galaxies
• Hot subdwarf stars in close-up view - III. Metal abundances of subdwarf B stars
• Slowly, slowly in the wind: 3D hydrodynamical simulations of wind mass transfer and angular-momentum loss in AGB binary systems
• Photometric and Spectroscopic Studies of Massive Binaries in the Large Magellanic Cloud. I. Introduction and Orbits for Two Detached Systems: Evidence for a Mass Discrepancy?
• Herschel observations of interstellar chloronium
• Common-Envelope Episodes that lead to Double Neutron Star formation
• Pristine IX: CFHT ESPaDOnS Spectroscopic Analysis of 115 Bright Metal-Poor Candidate Stars
• Interstellar Gas-phase Element Depletions in the Small Magellanic Cloud: A Guide to Correcting for Dust in QSO Absorption Line Systems
• Spatially-resolving the terminator: Variation of Fe, temperature and winds in WASP-76 b across planetary limbs and orbital phase
• SDSS-IV MaNGA: Modelling the metallicity gradients of gas and stars - radially dependent metal outflow vs IMF
• Coupling hydrodynamics with comoving frame radiative transfer: II. Stellar wind stratification in the high-mass X-ray binary Vela X-1
• Non-LTE Radiative Transfer with Turbospectrum
• The Magellan Evolution of Galaxies Spectroscopic and Ultraviolet Reference Atlas (MEGaSaURA) I: The Sample and the Spectra
• On the structure and energetics of quasar broad absorption-line outflows
• Making the Planetary Material Diversity During the Early Assembling of the Solar System
• The Stagger-grid: A grid of 3D stellar atmosphere models V. Synthetic stellar spectra and broad-band photometry
• The Formation of a 70 Msun Black Hole at High Metallicity
• An optical transmission spectrum of the ultra-hot Jupiter WASP-33b. First indication of AlO in an exoplanet
• The Evolution of Chemical Abundance in Quasar Broad Line Region
• Carbon Monoxide Clouds at Low-Metallicity in the WLM Galaxy
• Investigating Nearby Star-Forming Galaxies in the Ultraviolet with HST/COS Spectroscopy. I: Spectral Analysis and Interstellar Abundance Determinations
• Galactic planetary nebulae as probes of radial metallicity gradients and other abundance patterns
• 2D chemical evolution model: the impact of galactic disc asymmetries on azimuthal chemical abundance variations
• Explosion and nucleosynthesis of low redshift pair instability supernovae
• The eROSITA Final Equatorial-Depth Survey (eFEDS): Galaxy Clusters and Groups in Disguise
• EPIC 219388192 b - an inhabitant of the brown dwarf desert in the Ruprecht 147 open cluster
• Dynamical characterization of galaxies up to $z\sim 7$
• The First Observations of Low-Redshift Damped Lyman-α Systems with the Cosmic Origins Spectrograph: Chemical Abundances and Affiliated Galaxies
• Nucleosynthesis imprints from different Type Ia Supernova explosion scenarios and implications for galactic chemical evolution
• An unusually low density ultra-short period super-Earth and three mini-Neptunes around the old star TOI-561
• Are cold flows detectable with metal absorption lines?
• Constraining cosmic scatter in the Galactic halo through a differential analysis of metal-poor stars
• Domains of pulsational instability of low-frequency modes in rotating upper main-sequence stars
• The [NII] 205 micron Emission in Local Luminous Infrared Galaxies
• Simulating gas giant exoplanet atmospheres with Exo-FMS: Comparing semi-grey, picket fence and correlated-k radiative-transfer schemes
• Analyzing Atmospheric Temperature Profiles and Spectra of M dwarf Rocky Planets
• Stellar and nebular diagnostics in the UV for star-forming galaxies
• Velocity dispersion in the interstellar medium of early galaxies
• Chemical Abundance Analysis of Tucana III, the Second $r$-process Enhanced Ultra-Faint Dwarf Galaxy
• Abundances, Ionization States, Temperatures, and FIP in Solar Energetic Particles
• Cool DZ white dwarfs in the SDSS
• Red Supergiants as Cosmic Abundance Probes: The Sculptor Galaxy NGC 300
• The impact of updated Zr neutron-capture cross sections and new asymptotic giant branch models on our understanding of the s process and the origin of stardust
• Detailed homogeneous abundance studies of 14 Galactic s-process enriched post-AGB stars: In search of lead (Pb)
• Anisotropic turbulent transport in stably stratified rotating stellar radiation zones
• The determination of protoplanetary disk masses
• The Chemical Composition of the Galactic Bulge and Implications for its Evolution
• The presupernova core mass-radius relation of massive stars: understanding its formation and evolution
• The Close Binary Properties of Massive Stars in the Milky Way and Low-Metallicity Magellanic Clouds
• Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. II. Spatially Resolved Mass Outflow Rates for the QSO2 Markarian 34
• The metal and dust yields of the first massive stars
• Zirconium, Barium, Lanthanum and Europium Abundances in Open Clusters
• L-GALAXIES 2020: The evolution of radial metallicity profiles and global metallicities in disc galaxies
• A revised planetary nebula luminosity function distance to NGC 628 using MUSE
• The treatment of mixing in core helium burning models -- II. Constraints from cluster star counts
• Supernova 2010as: the Lowest-Velocity Member of a Family of Flat-Velocity Type IIb Supernovae
• On the Accuracy of the Differential Emission Measure Diagnostics of Solar Plasmas. Application to AIA/SDO. Part II: Multithermal plasmas
• A precise asteroseismic age and metallicity for HD 139614: a pre-main-sequence star with a protoplanetary disc in Upper-Centaurus Lupus
• Modeling magnesium escape from HD209458b atmosphere
• The sulfur depletion problem: upper limits on the H2S2, HS2, and S2 gas-phase abundances toward the low-mass warm core IRAS16293-2422
• Investigating the diversity of supernovae type Iax: A MUSE and NOT spectroscopic study of their environments
• Asteroseismic modelling of solar-type stars: internal systematics from input physics and surface correction methods
• Differences in the gas and dust distribution in the transitional disk of a sun-like young star, PDS 70
• No strong dependence of Lyman continuum leakage on physical properties of star-forming galaxies at $3.1\lesssim \mathbf{z}\lesssim 3.5$
• High-resolution spectroscopic studies of ultra metal-poor stars found in LAMOST survey
• First 3D Radiation-Hydrodynamic Simulations of Wolf-Rayet Winds
• A stellar stream remnant of a globular cluster below the metallicity floor
• The effects of surface fossil magnetic fields on massive star evolution: II. Implementation of magnetic braking in MESA and implications for the evolution of surface rotation in OB stars
• Element abundance ratios in the quiet Sun transition region
• Modelling the observed properties of carbon-enhanced metal-poor stars using binary population synthesis
• Host Galaxies of Type Ic and Broad-lined Type Ic Supernovae from the Palomar Transient Factory: Implication for Jet Production
• Four Distinct Pathways to the Element Abundances in Solar Energetic Particles
• Early results from GLASS-JWST. IV: Spatially resolved metallicity in a low-mass $z\sim 3$ galaxy with NIRISS
• Constraining galaxy cluster temperatures and redshifts with eROSITA survey data
• Modelling Double Neutron Stars: Radio and Gravitational Waves
• Herschel Galactic plane survey of [NII] fine structure emission
• Accelerated post-AGB evolution, initial-final mass relations, and the star-formation history of the Galactic bulge
• A constraint on light primordial black holes from the interstellar medium temperature
• Quantifying Feedback from Narrow Line Region Outflows in Nearby Active Galaxies. III. Results for the Seyfert 2 Galaxies Markarian 3, Markarian 78, and NGC 1068
• Uncovering multiple Wolf-Rayet star-clusters and the ionized ISM in Mrk178: the closest metal-poor Wolf-Rayet HII galaxy
• 3-D gas-phase elemental abundances across the formation histories of Milky Way-mass galaxies in the FIRE simulations: initial conditions for chemical tagging
• Discovery and Early Multi-Wavelength Measurements of the Energetic Type Ic Supernova PTF12gzk: A Massive-Star Explosion in a Dwarf Host Galaxy
• 129I and 247Cm in Meteorites Constrain the Last Astrophysical Source of Solar r-process Elements
• Understanding WASP-12b
• The Detailed Chemical Properties of M31 Star Clusters I. Fe, Alpha and Light Elements
• Effect of binary evolution on the inferred initial and final core masses of hydrogen-rich, Type~II supernova progenitors
• Reinvestigating $\alpha$ Cen AB in light of asteroseismic forward and inverse methods
• The excitation of solar-like oscillations in a delta Scuti star by efficient envelope convection
• GRACES observations of young [alpha/Fe]-rich stars
• Pre-main-sequence isochrones -- I. The Pleiades benchmark
• Evidence for diffuse molecular gas and dust in the hearts of gamma-ray burst host galaxies
• The VANDELS survey: the relation between UV continuum slope and stellar metallicity in star-forming galaxies at z~3
• Atlas of solar hidden photon emission
• Close-in ice lines and the super-stellar C/O ratio in discs around very low-mass stars
• New Results on Standard Solar Models
• Discovery of a very hot phase of the Milky Way CGM with non-solar abundance ratios
• The Kepler-19 system: a thick-envelope super-Earth with two Neptune-mass companions characterized using Radial Velocities and Transit Timing Variations
• Secondary eclipse observations for seven hot-Jupiters from the Anglo-Australian Telescope
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray Properties and Scaling Relations of Galaxy Clusters and Groups
• A Model of the H$\alpha$ and Na Transmission Spectrum of HD 189733b
• Empirical Determination of Dark Matter Velocities using Metal-Poor Stars
• Heading Gaia to measure atmospheric dynamics in AGB stars
• Improved measurement of solar neutrinos from the Carbon-Nitrogen-Oxygen cycle by Borexino and its implications for the Standard Solar Model
• The physics inside the scaling relations for X-ray galaxy clusters: gas clumpiness, gas mass fraction and slope of the pressure profile
• The virtual observatory service TheoSSA: Establishing a database of synthetic stellar flux standards. I. NLTE spectral analysis of the DA-type white dwarf G 191-B2B
• Three-dimensional hydrodynamical simulations of red giant stars: semi-global models for the interpretation of interferometric observations
• Whimper of a Bang: Documenting the Final Days of the Nearby Type Ia Supernova 2011fe
• Mass and p-factor of the type II Cepheid OGLE-LMC-T2CEP-098 in a binary system
• A grid of NLTE corrections for magnesium and calcium in late-type giant and supergiant stars: application to Gaia
• External Photoevaporation of the Solar Nebula: Jupiter's Noble Gas Enrichments
• Using the Standard Solar Model to Constrain Composition and S-Factors
• Discovery Of Cold, Pristine Gas Possibly Accreting Onto An Overdensity Of Star-Forming Galaxies At Redshift z ~ 1.6
• The s process in AGB stars as constrained by a large sample of Barium stars
• The origin of the $\alpha$-enhancement of massive galaxies
• Solar neutrino physics with low-threshold dark matter detectors
• Observability of signatures of transport-induced chemistry in clear atmospheres of hot gas giant exoplanets
• Lithium-7 surface abundance in pre-MS stars. Testing theory against clusters and binary systems
• Testing pre-main sequence models: the power of a Bayesian approach
• Lithium in M67: From the main sequence to the red giant branch
• Photoionization of ions with synchrotron radiation: From ions in space to atoms in cages
• On the use of field RR Lyrae as Galactic probes: I. The Oosterhoff dichotomy based on fundamental variables
• Exploring the production and depletion of lithium in the Milky Way stellar disk
• An Introductory Review on Cosmic Reionization
• The Star Formation History in The Far Outer Disc of M33
• Ionization correction factors and dust depletion patterns in giant HII regions
• Introducing TIGRESS-NCR: I. Co-Regulation of the Multiphase Interstellar Medium and Star Formation Rates
• On helium-dominated stellar evolution: the mysterious role of the O(He)-type stars
• Density diagnostics derived from the OIV and SIV intercombination lines observed by IRIS
• The evolution of planetary nebulae. VIII. True expansion rates and visibility times
• Spectral modeling of type II supernovae. I. Dilution factors
• Regional variations in the dense gas heating and cooling in M51 from Herschel far-infrared spectroscopy
• 3D LTE spectral line formation with scattering in red giant stars
• Low-mass low-metallicity AGB stars as an efficient i-process site explaining CEMP-rs stars
• Parent Stars of Extrasolar Planets. XI. Trends with Condensation Temperature Revisited
• Chemical distribution of HII regions towards the Galactic anticentre
• Evidence for multiple populations in the intermediate age cluster Lindsay 1 in the SMC
• Classification of extremely metal-poor stars: absent region in A(C)-[Fe/H] plane and the role of dust cooling
• Witnessing galaxy assembly in an extended z~3 structure
• Simulating Neutron Star Mergers as r-process Sources in Ultra Faint Dwarf Galaxies
• Multiphase quasar-driven outflows in PG 1114+445. I. Entrained ultra-fast outflows
• The Metal-Rich Atmosphere of the Neptune HAT-P-26b
• Radiation-driven winds of hot luminous stars. XVI. Expanding atmospheres of massive and very massive stars and the evolution of dense stellar clusters
• Production of interstellar hydrogen peroxide (H2O2) on the surface of dust grains
• Detection of the Second r-process Peak Element Tellurium in Metal-Poor Stars
• On the Use of Field RR Lyrae as Galactic Probes. II. A new $\Delta$S calibration to estimate their metallicity
• NLTE determination of the calcium abundance and 3D corrections in extremely metal-poor stars
• The X-factor in Galaxies: II. The molecular hydrogen -- star formation relation
• ALFALFA Discovery of the Nearby Gas-Rich Dwarf Galaxy Leo P. IV. Distance Measurement from LBT Optical Imaging
• Chemistry of the Most Metal-poor Stars in the Bulge and the z > 10 Universe
• Non-equilibrium helium ionization in an MHD simulation of the solar atmosphere
• The ${}^7$Be II Resonance Lines in Two Classical Novae V5668 Sgr and V2944 Oph
• A milestone toward understanding PDR properties in the extreme environment of LMC-30Dor
• The impact of an evolving stellar initial mass function on early galaxies and reionisation
• Modeling the disequilibrium species for Jupiter and Saturn: Implications for Juno and Saturn entry probe
• Large enhancement in high-energy photoionization of Fe XVII and missing continuum plasma opacity
• The quest for blue supergiants: binary merger models for the evolution of the progenitor of SN 1987A
• Hot Extended Galaxy Halos Around Local L* Galaxies From Sunyaev-Zeldovich Measurements
• Constraints on the presence of platinum and gold in the spectra of the kilonova AT2017gfo
• The Gaia-ESO survey: 3D NLTE abundances in the open cluster NGC 2420 suggest atomic diffusion and turbulent mixing at the origin of chemical abundance variations
• Predicting FIR lines from simulated galaxies
• The GALAH Survey: Verifying abundance trends in the open cluster M67 using non-LTE spectroscopy
• The COS CGM Compendium. III: Metallicity and Physical Properties of the Cool Circumgalactic Medium at z<1
• Discovery of a T dwarf + white dwarf binary system
• Rapid Rotation in the Kepler Field: Not a Single Star Phenomenon
• SteParSyn: A Bayesian code to infer stellar atmospheric parameters using spectral synthesis
• Star Formation from DLA Gas in the Outskirts of Lyman Break Galaxies at z~3
• Volatile-to-sulfur Ratios Can Recover a Gas Giant's Accretion History
• Neutral Cr and V in the atmosphere of ultra hot jupiter WASP-121 b
• Uncertainties in grid-based estimates of stellar mass and radius. SCEPtER: Stellar CharactEristics Pisa Estimation gRid
• METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble program. III. Interstellar Depletions, Dust-to-Metal, and Dust-to-Gas Ratios Versus Metallicity
• Correlation Between the Total Gravitating Mass of Groups and Clusters and the Supermassive Black Hole Mass of Brightest Galaxies
• Revisiting the abundance gradient in the maser host galaxy NGC 4258
• Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies
• On the origin and composition of Galactic cosmic rays
• Simulating the interstellar medium of galaxies with radiative transfer, non-equilibrium thermochemistry, and dust
• IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
• The very young resolved stellar populations around stripped-envelope supernovae
• WASP-127b transmission spectrum]{Abundance measurements of H${}_2$O and carbon-bearing species in the atmosphere of WASP-127b confirm its super-solar metallicity
• The formation of IRIS diagnostics VI. The Diagnostic Potential of the C II Lines at 133.5 nm in the Solar Atmosphere
• Signatures of Dark Radiation in Neutrino and Dark Matter Detectors
• A photometric and spectroscopic survey of solar twin stars within 50 parsecs of the Sun: I. Atmospheric parameters and color similarity to the Sun
• A Chandra/LETGS Survey of Main Sequence Stars
• The solar, exoplanet and cosmological lithium problems
• The Outburst Decay of the Low Magnetic Field Magnetar SWIFT J1822.3-1606: Phase-resolved Analysis and Evidence for a Variable Cyclotron Feature
• The Composition of Interstellar Grains Toward Zeta Ophiuchi: Constraining the Elemental Budget Near the Diffuse-Dense Cloud Transition
• Long-rising Type II supernovae from PTF and CCCP
• The gas and stellar content of a metal-poor galaxy at $z=8.496$ as revealed by JWST and ALMA
• Full-sky photon simulation of clusters and active galactic nuclei in the soft X-rays for eROSITA
• The resolved stellar populations around 12 Type IIP supernovae
• Germanium, Arsenic, and Selenium Abundances in Metal-Poor Stars
• Periodic mass loss episodes due to an oscillation mode with variable amplitude in the hot supergiant HD50064
• Lithium Abundances in a Sample of Planet Hosting Dwarfs
• Chemical Abundance Signature of J0023+0307 -- A Second-Generation Main-Sequence Star with [Fe/H]<-6
• Physical properties and transmission spectrum of the WASP-80 planetary system from multi-colour photometry
• The MOSDEF Survey: Metallicity Dependence of the PAH Emission at High Redshift and Implications for 24 micron-inferred IR Luminosities and Star Formation Rates at z~2
• Observational signatures of a warped disk associated with cold-flow accretion
• Testing models for molecular gas formation in galaxies: hydrostatic pressure or gas and dust shielding?
• The discovery of WASP-151b, WASP-153b, WASP-156b: Insights on giant planet migration and the upper boundary of the Neptunian desert
• VLT/UVES observations of extremely strong intervening damped Lyman-alpha systems: Molecular hydrogen and excited carbon, oxygen and silicon at log N(HI)=22.4
• Stellar Forensics with the Supernova-GRB Connection
• Tables of phase functions, opacities, albedos, equilibrium temperatures, and radiative accelerations of dust grains in exoplanets
• How plausible are the proposed formation scenarios of CEMP-r/s stars?
• The Gaia-ESO Survey: the origin and evolution of s-process elements
• The composition of the protosolar disk and the formation conditions for comets
• The XUV environments of exoplanets from Jupiter-size to super-Earth
• The late-time light curve of the type Ia supernova SN 2011fe
• The Similarity of Abundance Ratio Trends and Nucleosynthetic Patterns in the Milky Way Disk and Bulge
• On the Accuracy of the Differential Emission Measure Diagnostics of Solar Plasmas. Application to AIA/SDO. Part I: Isothermal plasmas
• Observational Constraints on Red and Blue Helium Burning Sequences
• When the tale comes true: multiple populations and wide binaries in the Orion Nebula Cluster
• Three-dimensional structure of a sunspot light bridge
• Code dependencies of pre-supernova evolution and nucleosynthesis in massive stars: Evolution to the end of core helium burning
• Kinematics and excitation of the ram pressure stripped ionized gas filaments in the Coma cluster of galaxies
• 3D non-LTE line formation of neutral carbon in the Sun
• The 14N(p,gamma)15O reaction studied with a composite germanium detector
• Detection of the Missing Baryons toward the Sightline of H1821+643
• Manganese Indicates a Transition from Sub- to Near-Chandrasekhar Type Ia Supernovae in Dwarf Galaxies
• Photochemistry and Heating/Cooling of the Multiphase Interstellar Medium with UV Radiative Transfer for Magnetohydrodynamic Simulations
• Four-of-a-kind? Comprehensive atmospheric characterisation of the HR 8799 planets with VLTI/GRAVITY
• Chemical abundance scaling relations for multiple elements in z~2-3 star-forming galaxies
• ALMA and HST kiloparsec-scale imaging of a quasar-galaxy merger at $z\approx 6.2$
• Binary-Stripped Stars as Core-Collapse Supernovae Progenitors
• Hot stars observed by XMM-Newton II. A survey of Oe and Be stars
• A new method for an objective, ${\chi }^2$-based spectroscopic analysis of early-type stars
• Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era
• A high resolution spectroscopic atlas of M subdwarfs - Effective temperature and metallicity
• SN 2016coi/ASASSN-16fp: An example of residual helium in a type Ic supernova?
• Witnessing galaxy assembly at the edge of the reionization epoch
• Uncovering Blue Diffuse Dwarf Galaxies
• A white dwarf accreting planetary material determined from X-ray observations
• Carbon and oxygen isotopic ratios in Arcturus and Aldebaran: Constraining the parameters for non convective mixing on the RGB
• The Keck+Magellan Survey for Lyman Limit Absorption III: Sample Definition and Column Density Measurements
• Do Metal-Rich Stars Make Metal-Rich Planets? New Insights on Giant Planet Formation from Host Star Abundances
• Photoelectric cross-sections of gas and dust in protoplanetary disks
• Fitting formulae for evolution tracks of massive stars under extreme metal poor environments for population synthesis calculations and star cluster simulations
• VUV-absorption cross section of carbon dioxide from 150 to 800 K and applications to warm exoplanetary atmospheres
• Internal rotation of 13 low-mass low-luminosity red giants in the Kepler field
• Dust production and mass loss in the Galactic globular cluster 47 Tucanae
• Binary population synthesis models for core-collapse gamma-ray burst progenitors
• Solar neutrino detection in a large volume double-phase liquid argon experiment
• The First Maps of ${\kappa }_d$ -- the Dust Mass Absorption Coefficient -- in Nearby Galaxies, with DustPedia
• Calcium H & K Induced by Galaxy Halos
• Confronting 2D delayed-detonation models with light curves and spectra of Type Ia supernovae
• Detectability of cold streams into high-redshift galaxies by absorption lines
• Clouds of Fluffy Aggregates: How They Form in Exoplanetary Atmospheres and Influence Transmission Spectra
• An Empirical Determination of the Dust Mass Absorption Coefficient, ${\kappa }_d$, Using the Herschel Reference Survey
• The long-lived Type IIn SN 2015da: Infrared echoes and strong interaction within an extended massive shell
• An XMM-Newton spatially-resolved study of metal abundance evolution in distant galaxy clusters
• Analysis of chemical abundances in planetary nebulae with [WC] central stars. II. Chemical abundances and the abundance discrepancy factor
• Hubble Space Telescope Observations of Sub-Damped Lyman-alpha Absorbers at z < 0.5, and Implications for Galaxy Chemical Evolution
• Carbon and oxygen in metal-poor halo stars
• The Solar Twin Planet Search. V. Close-in, low-mass planet candidates and evidence of planet accretion in the solar twin HIP 68468
• The Low Detection Rate of Pair Instability Supernovae and the Effect of the Core Carbon Fraction
• Carbon monoxide in an extremely metal-poor galaxy
• Gas phase Elemental abundances in Molecular cloudS (GEMS). IV. Observational results and statistical trends
• Discovery of a variable lead-rich hot subdwarf: UVO 0825+15
• TOI-1452 b: SPIRou and TESS reveal a super-Earth in a temperate orbit transiting an M4 dwarf
• Revisiting Spitzer transit observations with Independent Component Analysis: new results for the GJ436 system
• No Redshift Evolution in the Broad Line Region Metallicity up to z=7.54: Deep NIR Spectroscopy of ULAS J1342+0928
• The CN/C15 N isotopic ratio towards dark clouds
• Convective H-He Interactions in Massive Population III Stellar Evolution Models
• First stars XIII. Two extremely metal-poor RR Lyrae stars?
• Mg II absorbers: metallicity evolution and cloud morphology
• Hubble Space Telescope Near-Ultraviolet Spectroscopy of the Bright CEMP-no Star BD+44 493
• Spatially Resolved Galactic Wind in Lensed Galaxy RCSGA 032727-132609
• The chemical composition of red giants in 47 Tucanae I: Fundamental parameters and chemical abundance patterns
• DeSIRe: Departure coefficient aided Stokes Inversion based on Response functions
• Does circumgalactic OVI trace low-pressure gas beyond the accretion shock? Clues from HI and low-ion absorption, line kinematics, and dust extinction
• Statistical errors and systematic biases in the calibration of the convective core overshooting with eclipsing binaries. A case study: TZ Fornacis
• The Gas-Galaxy Connection at z = 0.35: OVI and HI Absorption Towards J0943+0531
• LMC Blue Supergiant Stars and the Calibration of the Flux-weighted Gravity--Luminosity Relationship
• Ultra Luminous X-ray Sources: a deeper insight into their spectral evolution
• NGC 1980 is not a foreground population of Orion: Spectroscopic survey of young stars with low extinction in Orion A
• The Abundance of SiC2 in Carbon Star Envelopes: Evidence that SiC2 is a gas-phase precursor of SiC dust
• Helium in natal HII regions: the origin of the X-ray absorption in gamma-ray burst afterglows
• Sulfur Chemistry in the Atmospheres of Warm and Hot Jupiters
• Evolution of dust extinction curves in galaxy simulation
• A High Signal-to-Noise Ratio Composite Spectrum of Gamma-ray Burst Afterglows
• Measuring stellar granulation during planet transits
• A metal-poor damped Ly-alpha system at redshift 6.4
• Evidence for the Direct Detection of the Thermal Spectrum of the Non-Transiting Hot Gas Giant HD 88133 b
• Laboratory atomic transition data for precise optical quasar absorption spectroscopy
• Zinc abundances in Galactic bulge field red giants: implications for DLA systems
• Hertzsprung-Russell diagram and mass distribution of barium stars
• Impacts of stellar evolution and dynamics on the habitable zone: The role of rotation and magnetic activity
• A critical reassessment of the fundamental properties of GJ 504: Chemical composition and age
• A Self-consistent Framework for Multiline Modeling in Line Intensity Mapping Experiments
• The Age of the Universe with Globular Clusters: Reducing Systematic Uncertainties
• The Volatility Trend of Protosolar and Terrestrial Elemental Abundances
• Benchmarking atomic data for astrophysics: a first look at the soft X-ray lines
• The fates of massive stars: exploring uncertainties in stellar evolution with METISSE
• 3D non-LTE iron abundances in FG-type dwarfs
• Stellar Models of Multiple Populations in Globular Clusters. I. The Main Sequence of NGC 6752
• Magnetic field topologies of the bright, weak-field Ap stars theta Aurigae and epsilon Ursae Majoris
• O VI Absorbers Tracing Hot Gas Associated with a Pair of Galaxies at z = 0.167
• Asymmetric supernova remnants generated by Galactic, massive runaway stars
• i-Process Contribution of Rapidly Accreting White Dwarfs to the Solar Composition of First-Peak Neutron-Capture Elements
• Prospects for Measuring Abundances of >20 Elements with Low-resolution Stellar Spectra
• History of the solar-type protostar IRAS16293-2422 as told by the cyanopolyynes
• Non-Maxwellian analysis of the transition-region line profiles observed by the Interface Region Imaging Spectrograph
• A study of the circum-galactic medium at z ~ 0.6 using DLA-galaxies
• OCCASO III. Iron peak and $\alpha$ elements of 18 open clusters. Comparison with chemical evolution models and field stars
• Horizons: Nuclear Astrophysics in the 2020s and Beyond
• X-ray emission from massive stars in Cyg OB2
• Spatially resolved integral field spectroscopy of the ionized gas in IZw18
• Effects of Mg/Si on Exoplanetary Refractory Oxygen Budget
• Chemical abundances of hydrostatic and explosive alpha-elements in Sagittarius stream stars
• Red Supergiants as Cosmic Abundance Probes: massive star clusters in M83, and the mass-metallicity relation of nearby galaxies
• Interpretation of the BRITE oscillation data of the hybrid pulsator $\nu$ Eridani: a call for the modification of stellar opacities
• Chemical abundances of Seyfert 2 AGNs $-$II. N2 metallicity calibration based on SDSS
• Spectroscopic Survey of γ Doradus Stars I. Comprehensive atmospheric parameters and abundance analysis of γ Doradus stars
• Stellar Populations of Highly Magnified Lensed Galaxies: Young Starbursts at z~2
• The Cosmic Ultraviolet Baryon Survey (CUBS) -- III. Physical properties and elemental abundances of Lyman limit systems at $z<1$
• Solar abundance corrections derived through 3D magnetoconvection simulations
• Gemini GMOS spectroscopy of HeII nebulae in M33
• The Quiescent X-ray Spectrum of Accreting Black Holes
• The COS CGM Compendium. II: Metallicities of the Partial and Lyman Limit Systems at z<1
• Cold-Mode Accretion: Driving the Fundamental Mass-Metallicity Relation at z~2
• Testing the effect of galactic feedback on the IGM at z ~ 6 with metal-line absorbers
• The "FIP Effect" and the Origins of Solar Energetic Particles and of the Solar Wind
• Planetary nebulae abundances and stellar evolution II
• Massive pulsating stars observed by BRITE-Constellation. I. The triple system Beta Centauri (Agena)
• The age of 47Tuc from self-consistent isochrone fits to colour-magnitude diagrams and the eclipsing member V69
• The Penn State - Torun Centre for Astronomy Planet Search stars. II. Lithium abundance analysis of the Red Giant Clump sample
• Ultraviolet spectra of extreme nearby star-forming regions: evidence for an overabundance of very massive stars
• Combined Effects of Rotation and Age Spreads on Extended Main Sequence Turn Offs
• PySME -- Spectroscopy Made Easier
• The Type Ib SN 1999dn: One Year of Photometric and Spectroscopic Monitoring
• The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z=3.5
• Seismic measurement of the locations of the base of convection zone and helium ionization zone for stars in the {\it Kepler} seismic LEGACY sample
• The Curious Conundrum Regarding Sulfur Abundances In Planetary Nebulae
• High-resolution transmission spectroscopy study of ultra-hot Jupiters HAT-P-57b, KELT-17b, KELT-21b, KELT-7b, MASCARA-1b, and WASP-189b
• How accurate are stellar ages based on stellar models ? I. The impact of stellar models uncertainties
• Impact of internal gravity waves on the rotation profile inside pre-main sequence low-mass stars
• KIC 8164262: a Heartbeat Star Showing Tidally Induced Pulsations with Resonant Locking
• Detection of 21-cm, H2 and Deuterium absorption at z>3 along the line-of-sight to J1337+3152
• Herschel observations of Extra-Ordinary Sources: H2S as a Probe of Dense Gas and Possibly Hidden Luminosity Toward the Orion KL Hot Core
• Detection of Neutral Phosphorus in the Near Ultraviolet Spectra of Late-Type Stars
• Revisiting longitudinal plasmon-axion conversion in external magnetic fields
• Helium Stars: Towards an Understanding of Wolf-Rayet Evolution
• Dynamically cold disks in the early Universe: myth or reality?
• JINGLE -- IV. Dust, HI gas and metal scaling laws in the local Universe
• The supernova remnant population of the Small Magellanic Cloud
• TOI-257b (HD 19916b): A Warm sub-Saturn Orbiting an Evolved F-type Star
• Abundance of 26Al and 60Fe in evolving Giant Molecular Clouds
• VLT/X-shooter spectroscopy of the GRB 090926A afterglow
• Computational issues in chemo-dynamical modelling of the formation and evolution of galaxies
• The benchmark halo giant HD 122563: CNO abundances revisited with three-dimensional hydrodynamic model stellar atmospheres
• MUFASA: The assembly of the red sequence
• A helium-flash-induced mixing event can explain the lithium abundances of red clump stars
• Metallicity-dependent nucleosynthetic yields of Type Ia supernovae originating from double detonations of sub-M${}_{\text{Ch}}$ white dwarfs
• Pre-supernova evolution and final fate of stellar mergers and accretors of binary mass transfer
• A new candidate for probing Population III nucleosynthesis with carbon-enhanced damped Lyman-alpha systems
• The Low Redshift Circumgalactic Medium in Simba
• Discovery of post-mass-transfer helium-burning red giants using asteroseismology
• Monitoring a high--amplitude Delta Sct star for 152 days: discovery of 12 additional modes and modulation effects in the light curve of CoRoT 101155310
• Grids of stellar models with rotation VII: Models from 0.8 to 300 M${}_{\odot }$ at super-solar metallicity (Z = 0.020)
• Detailed Chemical Abundances in NGC 5824: Another Metal-Poor Globular Cluster with Internal Heavy Element Abundance Variations
• Exploring the M-dwarf Luminosity--Temperature--Radius Relationships using Gaia DR2
• Extreme Emission-Line Galaxies in SDSS. I. Empirical and model-based calibrations of chemical abundances
• Near-ultraviolet Transmission Spectroscopy of HD 209458b: Evidence of Ionized Iron Beyond the Planetary Roche Lobe
• Solar models with convective overshoot, the solar-wind mass loss, and a PMS disk accretion: helioseismic quantities, Li depletion and neutrino fluxes
• Solar reflection of light dark matter with heavy mediators
• Exploring the Overabundance of ULXs in Metal- and Dust-poor Local Lyman Break Analogs
• IRC-10414: a bow-shock-producing red supergiant star
• MUSE-ALMA Halos V: Physical properties and environment of z < 1.4 HI quasar absorbers
• A Multiphase Absorber Containing O VI and Broad H I Directly Tracing 10^6 K Plasma at Low-Redshift Toward HE 0153-4520
• The chemical composition of HIP34407/HIP34426 and other twin-star comoving pairs
• Hubble Space Telescope Near-Ultraviolet Spectroscopy of Bright CEMP-s Stars
• First stars in Damped Lyman Alpha systems
• Prospects for asteroseismology
• 3-D non-LTE radiative transfer effects in Fe I lines: II. Line formation in 3-D radiation hydrodynamic simulations
• The effects of different Type Ia SN yields on Milky Way chemical evolution
• The GALAH survey: A census of lithium-rich giant stars
• Constraints on the Distance Moduli, Helium and Metal Abundances, and Ages of Globular Clusters from their RR Lyrae and Non-Variable Horizontal-Branch Stars. I. M3, M15, and M92
• Exoplanet Characterization by Multi-Observatory Transit Photometry with TESS and CHEOPS
• Constraints on the Initial-Final Mass Relation from Wide Double White Dwarfs
• Discovery of strongly variable X-ray polarization in the neutron star low-mass X-ray binary transient XTE J1701$-$462
• Comparative Modelling of the Spectra of Cool Giants
• ALMA observations of cool dust in a low-metallicity starburst, SBS0335-052
• Solar constraints on asymmetric dark matter
• The properties of ten O-type stars in the low-metallicity galaxies IC 1613, WLM and NGC 3109
• The Radial and Rotational Velocities of PSO J318.5338$-$22.8603, a Newly Confirmed Planetary-Mass Member of the $\beta$ Pictoris Moving Group
• JADES: The star-formation and chemical enrichment history of a luminous galaxy at z~9.43 probed by ultra-deep JWST/NIRSpec spectroscopy
• Modelling the He I triplet absorption at 10830 Angstroms in the atmospheres of HD 189733 b and GJ 3470 b
• The RRC Stars: Chemical Abundances and Envelope Kinematics
• The first evidence for multiple pulsation axes: a new roAp star in the Kepler field, KIC 10195926
• Stellar Metallicity of the Extended Disk and Distance of the Spiral Galaxy NGC 3621
• Wind mass-loss rates of stripped stars inferred from Cygnus X-1
• Lithium depletion and angular momentum transport in solar-type stars
• The r-Process Pattern of a Bright, Highly r-Process-Enhanced, Metal-Poor Halo Star at [Fe/H] ~ -2
• When binaries keep track of recent nucleosynthesis: The Zr - Nb pair in extrinsic stars as an s-process diagnostic
• Stellar Mass--Gas-phase Metallicity Relation at $0.5\le z\le 0.7$: A Power Law with Increasing Scatter toward the Low-mass Regime
• KIC7668647: a 14 day beaming sdB+WD binary with a pulsating subdwarf
• Multiple temperature components of the hot circumgalactic medium of the Milky Way
• The Populations of Carina. II. Chemical Enrichment
• Chemical evolution of classical and ultra-faint dwarf spheroidal galaxies
• The polluted atmospheres of cool white dwarfs and the magnetic field connection
• Carbon depletion observed inside T Tauri inner rims: Formation of icy, kilometer size planetesimals by 1 Myr
• Variability of newly identified B-type stars observed by Kepler
• The Herschel M33 extended survey (HerM33es): PACS spectroscopy of the star forming region BCLMP 302
• How Do Supernovae Impact the Circumgalactic Medium? I. Large-Scale Fountains Around a Milky Way-Like Galaxy
• The Photometric Metallicity and Carbon Distributions of the Milky Way's Halo and Solar Neighborhood from S-PLUS Observations of SDSS Stripe 82
• Constraints on explosive silicon burning in core-collapse supernovae from measured Ni/Fe ratios
• Excess C/H in Protoplanetary Disk Gas from Icy Pebble Drift across the CO Snowline
• Bow shock nebulae of hot massive stars in a magnetized medium
• Chemical Abundance Analysis of Three $\alpha$-Poor, Metal-Poor Stars in the Ultra-Faint Dwarf Galaxy Horologium I
• Light-travel-time diagnostics in early Supernova spectra: substantial mass loss of the IIb progenitor of SN 2013cu through a superwind
• KIC 9246715: The Double Red Giant Eclipsing Binary With Odd Oscillations
• A bayesian-like approach to derive chemical abundances in Type-2 Active Galactic Nuclei based on photoionization models
• The influence of accretion rate and metallicity on thermonuclear bursts: predictions from KEPLER models
• A statistically significant lack of debris discs in medium separation binary systems
• The chemical composition of nearby young associations: s-process element abundances in AB Doradus, Carina-Near, and Ursa Major
• The IRAM-30m line survey of the Horsehead PDR: I. CF+ as a tracer of C+ and a measure of the Fluorine abundance
• On the far-infrared metallicity diagnostics: applications to high-redshift galaxies
• Final results of Borexino on CNO solar neutrinos
• Pure-hydrogen 3D model atmospheres of cool white dwarfs
• A physically motivated and empirically calibrated method to measure effective temperature, metallicity, and Ti abundance of M dwarfs
• Chemical abundances in bright giants of the globular cluster M62 (NGC 6266)
• From interstellar abundances to grain composition: the major dust constituents Mg, Si and Fe
• Cosmic Origins Spectrograph Detection of Ne VIII Tracing Warm - Hot Gas Towards PKS 0405-123
• The influence of bulk composition on long-term interior-atmosphere evolution of terrestrial exoplanets
• The K2 Galactic Archaeology Program Data Release 3: Age-abundance patterns in C1-C8 and C10-C18
• The UK Infrared Telescope M33 monitoring project. II. The star formation history in the central square kiloparsec
• How much hydrogen is in Type Ib and IIb supernova progenitors?
• Lithium Enrichment Signatures of Planetary Engulfment Events in Evolved Stars
• The metal-enriched host of an energetic gamma-ray burst at z ~ 1.6
• A new prescription for the mass-loss rates of WC and WO stars
• Diffuse gas properties and stellar metallicities in cosmological simulations of disc galaxy formation
• The measured compositions of Uranus and Neptune from their formation on the CO iceline
• An analytical model for galaxy metallicity: What do metallicity relations tell us about star formation and outflow?
• The Galactic Dust-Up: Modeling Dust Evolution in FIRE
• Detailed Abundance Analysis of the Brightest Star in Segue 2, the Least Massive Galaxy
• A quasar reddened by a sub-parsec sized, metal-rich and dusty cloud in a damped Lyman-alpha absorber at z=2.13
• Populating the brown dwarf and stellar boundary: Five stars with transiting companions near the hydrogen-burning mass limit
• The role of the Galactic bar in the chemical evolution of the Milky Way
• Mass-to-Light versus Color Relations for Dwarf Irregular Galaxies
• The origin of slow Alfvénic solar wind at solar minimum
• Magnetic Field of the Eclipsing M Dwarf Binary YY Gem
• The Chemical Imprint of Silicate Dust on the Most Metal-Poor Stars
• Infrared [Fe II] Emission Lines from Radiative Atomic Shocks
• Oxygen lines in solar granulation. I. Testing 3D models against new observations with high spatial and spectral resolution
• Revived Fossil Plasma Sources in Galaxy Clusters
• Abundance ratios in GALAH DR2 and their implications for nucleosynthesis
• A newly discovered DLA and associated Ly-alpha emission in the spectra of the gravitationally lensed quasar UM 673A,B
• Probing the CO and methanol snow lines in young protostars. Results from the CALYPSO IRAM-PdBI survey
• Alkaline Exospheres of Exoplanet Systems: Evaporative Transmission Spectra
• Scaling relations and baryonic cycling in local star-forming galaxies: II. Gas content and star-formation efficiency
• A Catalog of Stellar Unified Properties (CATSUP) for 951 FGK-Stars Within 30 pc
• Stray-light contamination and spatial deconvolution of slit-spectrograph observations
• The Fractional Ionization of the Warm Neutral Interstellar Medium
• Discovery of Broad Soft X-ray Absorption Lines from the Quasar Wind in PDS 456
• Ultra metal-poor stars: Spectroscopic determination of stellar atmospheric parameters using iron Non-LTE line abundances
• Detection of a giant flare displaying quasi-periodic pulsations from a pre-main sequence M star with NGTS
• Benchmark ages for the Gaia benchmark stars
• Toward a New Kind of Asteroseismic Grid Fitting
• Galactic Chemical Evolution of Radioactive Isotopes
• The mass-metallicity relation of Lyman-break analogues and its dependence on galaxy properties
• Neutral gas heating by X-rays in primitive galaxies: Infrared observations of IZw18 with Herschel
• The dust content of the most metal-poor star-forming galaxies
• Cold accretion flows and chemical bimodality of the Milky Way galaxy
• Spectroscopic observations of PHz G237.01+42.50: A galaxy protocluster at z=2.16 in the Cosmos field
• A detailed analysis of the Gl 486 planetary system
• Leo P: How Many Metals can a Very Low-Mass, Isolated Galaxy Retain?
• RefleX: X-ray absorption and reflection in active galactic nuclei for arbitrary geometries
• Calcium H & K and sodium D absorption induced by the interstellar and circumgalactic media of the Milky Way
• The Homogeneous Study of Transiting Systems (HoSTS) I. The Pilot Study of WASP-13
• The origin of the enhanced metallicity of satellite galaxies
• Chemo-dynamical evolution of tidal dwarf galaxies. II. The long-term evolution and influence of a tidal field
• Multiple channels for nitrogen pollution by metal enriched supermassive stars and implications for GN-z11
• Carbon and Oxygen Abundances in the Hot Jupiter Exoplanet Host Star XO-2N and its Binary Companion
• NGTS-11 b / TOI-1847 b: A transiting warm Saturn recovered from a TESS single-transit event
• The Interstellar Oxygen Crisis, or Where Have All the Oxygen Atoms Gone?
• The Subaru FMOS Galaxy Redshift Survey (FastSound). III. The mass-metallicity relation and the fundamental metallicity relation at $z\sim 1.4$
• Probing the Role of Carbon in the Interstellar Ultraviolet Extinction
• Linking gas and galaxies at high redshift: MUSE surveys the environments of six damped Lyman alpha galaxies at z~3
• Planet Traps and Planetary Cores: Origins of the Planet-Metallicity Correlation
• Chandra X-ray spectroscopy of the very early O supergiant HD 93129A: constraints on wind shocks and the mass-loss rate
• Following The Cosmic Evolution Of Pristine Gas I: Implications For Milky Way Halo Stars
• The effects of rotation on the lithium depletion of G- and K-dwarfs in Messier 35
• Simultaneous X-ray and optical spectroscopy of the Oef supergiant lambda Cep
• Quantifying uncertainties in the solar axion flux and their impact on determining axion model parameters
• On the origin of the mass-metallicity gradient relation in the local Universe
• Dark Matter Halo Models of Stellar Mass-Dependent Galaxy Clustering in PRIMUS+DEEP2 at 0.2<z<1.2
• The host of the SN-less GRB 060505 in high resolution
• New constraints on the formation and settling of dust in the atmospheres of young M and L dwarfs
• Recycled stellar ejecta as fuel for star formation and implications for the origin of the galaxy mass-metallicity relation
• WASP-52b. The effect of starspot correction on atmospheric retrievals
• Evidence from stable isotopes and Be-10 for solar system formation triggered by a low-mass supernova
• Characterization of star-forming dwarf galaxies at 0.1 $\lesssim z\lesssim$ 0.9 in VUDS: Probing the low-mass end of the mass-metallicity relation
• The MUSE view of the host galaxy of GRB 100316D
• Detection of Na, K and H${}_2$O in the hazy atmosphere of WASP-6b
• A massive helium star with a sufficiently strong magnetic field to form a magnetar
• A Steady-State Picture of Solar Wind Acceleration and Charge State Composition Derived from a Global Wave-Driven MHD Model
• Three-dimensional interferometric, spectrometric, and planetary views of Procyon
• The bias of DLAs at z ~ 2.3: contraining stellar feedback in shallow potential wells
• Galactic Winds with MUSE: A Direct Detection of FeII* Emission from a z = 1.29 Galaxy
• The Chemical Evolution of the Milky Way: the Three Infall Model
• Pre-main-sequence isochrones -- III. The Cluster Collaboration isochrone server
• Kepler Eclipsing Binaries with $\delta$ Scuti/$\gamma$ Doradus Pulsating Components 1: KIC 9851944
• Detection of a population of carbon-enhanced metal-poor stars in the Sculptor dwarf spheroidal galaxy
• Spectroscopic evolution of massive stars on the main sequence
• Bottom-up dust nucleation theory in oxygen-rich evolved stars I. Aluminium oxide clusters
• How runaway stars boost galactic outflows
• S-process enrichment in the planetary nebula NGC 3918. Results from deep echelle spectrophotometry
• Redshift Measurement and Spectral Classification for eBOSS Galaxies with the Redmonster Software
• The diameter of the CoRoT target HD 49933. Combining the 3D limb darkening, asteroseismology, and interferometry
• Planetary nebulae in M33: probes of AGB nucleosynthesis and ISM abundances
• ALMA spectral survey of Supernova 1987A --- molecular inventory, chemistry, dynamics and explosive nucleosynthesis
• The EBLM project III. A Saturn-size low-mass star at the hydrogen-burning limit
• The MOSDEF Survey: A Comprehensive Analysis of the Rest-optical Emission-line Properties of $z\sim 2.3$ Star-forming Galaxies
• The chemistry of the most metal-rich damped Lyman $\alpha$ systems at z$\sim 2$ II. Context with the Local Group
• The origin of the most iron-poor star
• SIRIUS project. I. Star formation models for star-by-star simulations of star clusters and galaxy formation
• HIFI detection of HF in the carbon star envelope IRC +10216
• Iron in X-COP: tracing enrichment in cluster outskirts with high accuracy abundance profiles
• Chemical abundances of damped Lyman alpha systems in the XQ-100 survey
• Constraints on the opacity profile of the sun from helioseismic observables and solar neutrino flux measurements
• Testing excitation models of rapidly oscillating Ap stars with interferometry
• Detection of anhydrous hydrochloric acid, HCl, in IRC+10216 with the Herschel SPIRE and PACS spectrometers
• Time-dependent excitation and ionization modelling of absorption-line variability due to GRB 080310
• Observations of SN 2017ein Reveal Shock Breakout Emission and A Massive Progenitor Star for a Type Ic Supernova
• Insights into Pre-Enrichment of Star Clusters and Self-Enrichment of Dwarf Galaxies from their Intrinsic Metallicity Dispersions
• The COS Absorption Survey of Baryon Harbors: Unveiling the Physical Conditions of Circumgalactic Gas through Multiphase Bayesian Ionization Modeling
• Constraining Globular Cluster Age Uncertainties Using the IR Color-Magnitude Diagram
• Accretion in giant planet circumplanetary disks
• K2-111: an old system with two planets in near-resonance
• The Spatially Resolved Dust-to-Metals Ratio in M101
• Chemical abundances in the multiple sub-giant branch of 47 Tucanae: insights on its faint sub-giant branch component
• Chemical Evolution Models for Spiral Disks: the Milky Way, M31 and M33
• The evolution of planetary nebulae VII. Modelling planetary nebulae of distant stellar systems
• Hubble-COS Observations of Galactic High-Velocity Clouds: Four AGN Sight Lines through Complex C
• Helium Variation Across Two Solar Cycles Reveals A Speed-Dependent Phase Lag
• Spatially resolved MaNGA observations of the host galaxy of superluminous supernova 2017egm
• GRUMPY: a simple framework for realistic forward-modelling of dwarf galaxies
• An Ultra Metal-poor Star Near the Hydrogen-burning Limit
• On the Application of Bayesian Leave-One-Out Cross-Validation to Exoplanet Atmospheric Analysis
• Fully scalable forward model grid of exoplanet transmission spectra
• Properties of Dust Grains Probed with Extinction Curves
• Probing the metallicity and ionization state of the circumgalactic medium at z~6 and beyond with OI absorption
• The COS CGM Compendium (CCC). I: Survey Design and Initial Results
• Effective temperatures of red giants in the APOKASC catalogue and the mixing length calibration in stellar models
• Atmospheric parameters and chemical properties of red giants in the CoRoT asteroseismology fields
• O, Na, Ba and Eu abundance patterns in open clusters
• Solar Flare Element Abundances from the Solar Assembly for X-rays (SAX) on MESSENGER
• Dark Matter Search Using XMM-Newton Observations of Willman 1
• Galaxy And Mass Assembly (GAMA): The inferred mass--metallicity relation from z=0 to 3.5 via forensic SED fitting
• Photoionization modeling of oxygen K absorption in the interstellar medium:the Chandra grating spectra of XTE J1817-330
• Abundance gradients in low surface brightness spirals: clues on the origin of common gradients in galactic discs
• Ionised gas structure of 100 kpc in an over-dense region of the galaxy group COSMOS-Gr30 at z ~ 0.7
• H-alpha and Free-Free Emission from the WIM
• Chemical evolution of ultra-faint dwarf galaxies in the self-consistently calculated IGIMF theory
• A universal correlation between warm and hot gas in the stripped tails of cluster galaxies
• Minicharged Particles from the Sun: A Cutting-Edge Bound
• Evidence for a Sub-Chandrasekhar Mass Type~Ia Supernova in the Ursa Minor Dwarf Galaxy
• The detection of variable radio emission from the fast rotating magnetic hot B-star HR7355 and evidence for its X-ray aurorae
• Star-forming dwarf galaxies in the Virgo cluster: the link between molecular gas, atomic gas, and dust
• Setting the stage for the search for life with the Habitable Worlds Observatory: Properties of 164 promising planet survey targets
• The Galaxy Progenitors of Stellar Streams around Milky Way-mass Galaxies in the FIRE Cosmological Simulations
• A Minimum Dilution Scenario for Supernovae and Consequences for Extremely Metal-Poor Stars
• Plausible constraints on the range of bulk terrestrial exoplanet compositions in the Solar neighbourhood
• Retrieval of SDSS J1416+1348AB
• Solar-like oscillations from the depths of the red-giant star KIC 4351319 observed with Kepler
• Asteroseismology of 36 Kepler subgiants -- II: Determining ages from detailed modelling
• A needle in a haystack? Catching Pop III stars in the Epoch of Reionization: I. Pop III star forming environments
• The composition of hot Jupiter atmospheres assembled within chemically evolved protoplanetary discs
• EMPRESS. II. Highly Fe-Enriched Metal-poor Galaxies with $\sim 1.0$ (Fe/O)${}_{\odot }$ and $0.02$ (O/H)${}_{\odot }$ : Possible Traces of Super Massive ($>300M_{\odot }$) Stars in Early Galaxies
• INFERNO: Galactic winds in dwarf galaxies with star-by-star simulations including runaway stars
• A chemical confirmation of the faint Bootes II dwarf Spheroidal Galaxy
• HST/COS Spectra of Three QSOs That Probe The Circumgalactic Medium of a Single Spiral Galaxy: Evidence for Gas Recycling and Outflow
• Manganese abundances in Galactic bulge red giants
• Phosphorus-rich stars with unusual abundances are challenging theoretical predictions
• A metallicity study of 1987A-like supernova host galaxies
• Red Giant evolution and specific problems
• Fundamental Properties of the Highly Ionized Plasmas in the Milky Way
• An abundance study of red-giant-branch stars in the Hercules dwarf spheroidal galaxy
• On the seismic age and heavy-element abundance of the Sun
• Towards precise ages for single stars in the field. Gyrochronology constraints at several Gyr using wide binaries. I. Ages for initial sample
• The Magellan PFS Planet Search Program: Radial Velocity and Stellar Abundance Analyses of the 360 AU, Metal-Poor Binary "Twins" HD 133131A & B
• First Light: exploring the Spectra of High-Redshift Galaxies in the Renaissance Simulations
• Nucleosynthesis in AGB stars traced by oxygen isotopic ratios. I - Determining the stellar initial mass by means of the ${}^{17}$O/${}^{18}$O ratio
• NICIL: A stand alone library to self-consistently calculate non-ideal magnetohydrodynamic coefficients in molecular cloud cores
• The StaggerGrid Project: a Grid of 3D Model Atmospheres for High-Precision Spectroscopy
• Do meteoritic silicon carbide grains originate from asymptotic giant branch stars of super-solar metallicity?
• Deep Chandra Observations of the Compact Starburst Galaxy Henize 2-10: X-rays from the Massive Black Hole
• The intermediate neutron capture process. III. The i-process in AGB stars of different masses and metallicities without overshoot
• Chemical enrichment in very low-metallicity environments: Bootes I
• The Leoncino Dwarf Galaxy: Exploring the Low-Metallicity End of the Luminosity-Metallicity and Mass-Metallcity Relations
• From cold to hot irradiated gaseous exoplanets: Toward an observation-based classification scheme
• A Super-Solar Metallicity for the Progenitor of Kepler's Supernova
• High [OIII]/[CII] surface brightness ratios trace early starburst galaxies
• Multiple stellar populations and their evolution in globular clusters: A nucleosynthesis perspective
• Light Elements in the Universe
• The hot circumgalactic medium of the Milky Way: evidence for super-virial, virial, and sub-virial temperature, non-solar chemical composition, and non-thermal line broadening
• The stellar mass versus stellar metallicity relation of star-forming galaxies at $1.6\le z\le 3.0$ and implications for the evolution of the $\alpha$-enhancement
• WASP-117b: a 10-day-period Saturn in an eccentric and misaligned orbit
• Solar neutrino physics oscillations: Sensitivity to the electronic density in the Sun's core
• High-resolution atmospheric retrievals of WASP-121b transmission spectroscopy with ESPRESSO: Consistent relative abundance constraints across multiple epochs and instruments
• Properties of Convective Oxygen and Silicon Burning Shells in Supernova Progenitors
• Host star metallicity of directly imaged wide-orbit planets: implications for planet formation
• Towards A Removal of Temperature Dependencies from Abundance Determinations
• The VANDELS survey: Dust attenuation in star-forming galaxies at $\mathbf{z}=3-4$
• Chemical Cartography. I. A Carbonicity Map of the Galactic Halo
• The metal content of the hot atmospheres of galaxy groups
• Pressure profiles and mass estimates using high-resolution Sunyaev-Zel'dovich effect observations of Zwicky 3146 with MUSTANG-2
• The challenge of simultaneously matching the observed diversity of chemical abundance patterns in cosmological hydrodynamical simulations
• Directly imaging damped Ly-alpha galaxies at z>2. II: Imaging and spectroscopic observations of 32 quasar fields
• The Luminous Infrared Host Galaxy of Short-Duration GRB 100206A
• G64-12 and G64-37 are Carbon-Enhanced Metal-Poor Stars
• Assessing the sources of reionisation: a spectroscopic case study of a 30$\times$ lensed galaxy at $z\sim 5$ with Lyα, CIV, MgII, and [NeIII]
• Post-AGB stars in the Magellanic Clouds and neutron-capture processes in AGB stars
• Chemodynamics of Green Pea galaxies -- I. Outflows and turbulence driving the escape of ionising photons and chemical enrichment
• The white dwarf's carbon fraction as a secondary parameter of Type Ia supernovae
• What Do the Hitomi Observations Tell Us About the Turbulent Velocities in the Perseus Cluster? Probing the Velocity Field with Mock Observations
• Determining the Age of the Kepler Open Cluster NGC 6819 With a New Triple System and Other Eclipsing Binary Stars
• Bottlenecks to interstellar sulfur chemistry: Sulfur-bearing hydrides in UV-illuminated gas and grains
• Asteroseismology of 3,642 Kepler Red Giants: Correcting the Scaling Relations based on Detailed Modeling
• Enrichment of Zinc in galactic chemodynamical evolution models
• The Impact of Nuclear Reaction Rate Uncertainties On The Evolution of Core-Collapse Supernova Progenitors
• A new era of fine structure constant measurements at high redshift
• Quenched Cold Accretion of a Large Scale Metal-Poor Filament due to Virial Shocking in the Halo of a Massive z=0.7 Galaxy
• METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble program. II. Variations of interstellar depletions and dust-to-gas ratio within the LMC
• 15NH3 in the atmosphere of a cool brown dwarf
• Revisiting the 16 Cygni planet host at unprecedented precision and exploring automated tools for precise abundances
• Cos observations of metal line and broad lyman alpha absorption in the multi-phase o vi and ne viii system toward he 02226-4110
• The Gaia-ESO Survey: A new approach to chemically characterising young open clusters II. Abundances of the neutron-capture elements Cu, Sr, Y, Zr, Ba, La, and Ce
• Reconciling escape fractions and observed line emission in Lyman-continuum-leaking galaxies
• The SDSS-III APOGEE Radial Velocity Survey of M dwarfs I: Description of Survey and Science Goals
• The physics of Core-Collapse Supernovae: explosion mechanism and explosive nucleosynthesis
• Supernova 1987A: 3D Mixing and light curves for explosion models based on binary-merger progenitors
• Markov chain Monte Carlo analyses of the flux ratios of B, Be and Li with the DRAGON2 code
• Detection of Water Vapor in the Thermal Spectrum of the Non-Transiting Hot Jupiter upsilon Andromedae b
• Survey of non-linear hydrodynamic models of type-II Cepheids
• Observational evidence for high neutronization in supernova remnants: implications for Type Ia supernova progenitors
• On the type Ia supernovae 2007on and 2011iv: Evidence for Chandrasekhar-mass explosions at the faint end of the luminosity-width relationship
• Infrared emission of $z\sim 6$ galaxies: AGN imprints
• Integrated Light Chemical Tagging Analyses of Seven M31 Outer Halo Globular Clusters from the Pan-Andromeda Archaeological Survey
• Gemini/GRACES Spectroscopy of Stars in Triangulum II
• CRIRES+ and ESPRESSO reveal an atmosphere enriched in volatiles relative to refractories on the ultra-hot Jupiter WASP-121b
• Binary Interaction Dominates Mass Ejection in Classical Novae
• A step toward CNO solar neutrinos detection in liquid scintillators
• The Chemical Evolution of Fluorine in the Bulge - High-resolution K-band spectra of giants in three fields
• Tidally Induced Pulsations in Kepler Eclipsing Binary KIC 3230227
• Astraeus V: The emergence and evolution of metallicity scaling relations during the Epoch of Reionization
• The Mass and Absorption Columns of Galactic Gaseous Halos
• Axion Astrophysics
• Efficiency of radial transport of ices in protoplanetary disks probed with infrared observations: the case of CO${}_2$
• The galaxy group NGC 507: newly detected AGN remnant plasma transported by sloshing
• Resonance strengths in the 14N(p, γ)15O and 15N(p, αγ)12C reactions
• X-ray evidence for the accretion disc-outflow connection in 3C 111
• Molecule formation in dust-poor irradiated jets I. Stationary disk winds
• Unraveling the Origin of Overionized Plasma in the Galactic Supernova Remnant W49B
• X-ray Emission From Hot Gas in Galaxy Groups and Clusters in Simba
• The impact of non-ideal magnetohydrodynamics on binary star formation
• Akari Observations of Brown Dwarfs. II CO2 as Probe of Carbon and Oxygen Abundances in Brown Dwarfs
• Asteroseismic constraints on the cosmic-time variation of the gravitational constant from an ancient main-sequence star
• Characterising the surface magnetic fields of T Tauri stars with high-resolution near-infrared spectroscopy
• Revisiting the explodability of single massive star progenitors of stripped-envelope supernovae
• Chandra X-ray spectroscopy of a clear dip in GX 13+1
• METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble program. I. Overview and Initial Results
• MPS-ATLAS: A fast all-in-one code for synthesising stellar spectra
• Evolutionary models of red supergiants: Evidence for a metallicity-dependent mixing length and implications for Type IIP supernova progenitors
• Host galaxies of SNe Ic-BL with and without long gamma-ray bursts
• Mineral cloud and hydrocarbon haze particles in the atmosphere of the hot Jupiter JWST target WASP-43b
• Faint progenitors of luminous $z\sim 6$ quasars: why don't we see them?
• The role of C/O in nitrile astrochemistry in PDRs and planet-forming disks
• Connecting the metallicity dependence and redshift evolution of high-mass X-ray binaries
• Solar Fe abundance and magnetic fields - Towards a consistent reference metallicity
• Exploring the origin of thick disks using the NewHorizon and Galactica simulations
• Radial abundance gradients in the outer Galactic disk as traced by main-sequence OB stars
• Li Evolution and the Open Cluster NGC 6819: A Correlation Between Li Depletion and Spindown in Dwarfs More Massive Than the F-Dwarf Li-Dip
• Axion helioscopes as solar magnetometers
• Accreting protoplanets: Spectral signatures and magnitude of gas and dust extinction at H alpha
• New N-bearing species towards OH231.8+4.2: HNCO, HNCS, HC${}_3$N and NO
• Short-lived radioactivity in the early Solar System: the Super-AGB star hypothesis
• Radiation Pressure Confinement -- III. The origin of the broad ionization distribution in AGN outflows
• New Insights on Jupiter's Deep Water Abundance from Disequilibrium Species
• The Hyperactive L Dwarf 2MASS J13153094-2649513: Continued Emission and a Brown Dwarf Companion
• Bimodal black-hole mass distribution and chirp masses of binary black-hole mergers
• The environment of the SN-less GRB 111005A at z = 0.0133
• High-resolution spectroscopy of extremely metal-poor stars from SDSS/SEGUE. III. Unevolved Stars with $[Fe/H]\lesssim -3.5$
• Spectroscopic evolution of very massive stars at Z = 1/2.5 Zsun
• Red Supergiants as cosmic abundance probes: the first direct metallicity determination of NGC 4038 in the Antennae
• Origin of the PN molecule in star-forming regions: the enlarged sample
• On the Chemical Abundance of HR 8799 and the Planet c
• A comprehensive chemical abundance study of the outer halo globular cluster M 75
• Chandra View of the Warm-Hot IGM toward 1ES 1553+113: Absorption Line Detections and Identifications (Paper I)
• Using 21cm Absorption in Small Impact Parameter Galaxy-QSO Pairs to Probe Low-Redshift Damped and Sub-Damped Lyman-alpha System
• The High-Ion Content and Kinematics of Low-Redshift Lyman Limit Systems
• Core-Collapse Supernovae in Binaries as the Origin of Galactic Hyper-Runaway Stars
• Fluorine in the Solar neighborhood: No evidence for the neutrino process
• Luminous solar neutrinos I: Dipole portals
• X-ray Ionization of Heavy Elements Applied to Protoplanetary Disks
• iPTF 16hgs: A double-peaked Ca-rich gap transient in a metal poor, star forming dwarf galaxy
• The Relationship Between Galaxy ISM and Circumgalactic Gas Metallicities
• WISH VI. Constraints on UV and X-ray irradiation from a survey of hydrides in low- to high-mass YSOs
• Anomalous Double-Mode RR Lyrae Stars in the Magellanic Clouds
• Far-infrared study of tracers of oxygen chemistry in diffuse clouds
• Updating the theoretical tidal evolution constants: Apsidal motion and the moment of inertia
• The $\nu$-process with fully time-dependent supernova neutrino emission spectra
• Studying the merging cluster Abell 3266 with eROSITA
• Monte Carlo Method for Calculating Oxygen Abundances and Their Uncertainties from Strong-Line Flux Measurements
• Radial and vertical dust transport inhibit refractory carbon depletion in protoplanetary disks
• On the first $\delta$ Sct--roAp hybrid pulsator and the stability of p and g modes in chemically peculiar A/F stars
• Effects of rotation and magnetic fields on the lithium abundance and asteroseismic properties of exoplanet-host stars
• Mass-Metallicity and Star Formation Rate in Galaxies: a complex relation tuned to stellar age
• The Origin of the Iron-Rich Knot in Tycho's Supernova Remnant
• SALT reveals the barium central star of the planetary nebula Hen 2-39
• Forecasts for the WFIRST High Latitude Survey using the BlueTides Simulation
• Confronting uncertainties in stellar physics II. exploring differences in main-sequence stellar evolution tracks
• Molecular gas and star formation in an absorption-selected galaxy: Hitting the bull's eye at z = 2.46
• Diffuse Atomic and Molecular Gas in the Interstellar Medium of M82 toward SN 2014J
• Towards understanding the relation between the gas and the attenuation in galaxies at kpc scales
• Characterizing Extreme Emission Line Galaxies II: A Self-Consistent Model of Their Ionizing Spectrum
• Comprehensive abundance analysis of red giants in the open clusters NGC 1342, 1662, 1912, 2354 and 2447
• The physical mechanism behind M dwarf metallicity indicators and the role of C and O abundances
• Using rotation, magnetic activity and lithium to estimate the ages of low mass stars
• Spectroscopic and seismic analysis of red giants in eclipsing binaries discovered by Kepler
• Analysis of apsidal motion in eclipsing binaries using TESS data II. A test of internal stellar structure}
• On the variation of carbon abundance in galaxies and its implications
• The ALMA REBELS Survey: The Cosmic HI Gas Mass Density in Galaxies at $z\approx 7$
• Probing Final Stages of Stellar Evolution with X-Ray Observations of SN 2013ej
• Simplified 3D GCM modelling of the irradiated brown dwarf WD0137-349B
• Interaction of Cosmic Rays with Cold Clouds in Galactic Halos
• Time Evolution of Galaxy Scaling Relations in Cosmological Simulations
• Evidence for the accretion origin of halo stars with an extreme r-process enhancement
• The First Fluorine Abundance Determinations in Extragalactic AGB Carbon Stars
• Modelling depletion by re-accretion of gas from a dusty disc in post-AGB stars
• Three discoveries of gamma Cas analogs from dedicated XMM-Newton observations of Be stars
• The effect of the environment-dependent IMF on the formation and metallicities of stars over the cosmic history
• Modelling the cross-spectral variability of the black hole binary MAXI J1659-152 with propagating accretion rate fluctuations
• The F-CHROMA grid of 1D RADYN flare models
• New Perspectives on the Exoplanet Radius Gap from a Mathematica Tool and Visualized Water Equation of State
• BD-22 3467, a DAO-type star exciting the nebula Abell 35
• Detailed abundance study of four s-process enriched post-AGB stars in the Large Magellanic Cloud
• The stellar metallicities of massive quiescent galaxies at 1.0 < z < 1.3 from KMOS+VANDELS
• The effect of starspots on the ages of low-mass stars determined from the lithium depletion boundary
• Coronal Sources of the Solar F${}_{10.7}$ Radio Flux
• The nature of V39: an LBV candidate or LBV impostor in the very low metallicity galaxy IC 1613?
• The effect of isotopic splitting on the bisector and inversions of the solar Ca II 854.2 nm line
• A Variable PV Broad Absorption Line and Quasar Outflow Energetics
• Revisiting the pre-main-sequence evolution of stars II. Consequences of planet formation on stellar surface composition
• It's written in the massive stars: The role of stellar physics in the formation of black holes
• Fluorine in the solar neighborhood - is it all produced in AGB-stars?
• Retrieving C and O Abundance of HR 8799 c by Combining High- and Low-Resolution Data
• The [CII]--SFR correlation in dwarf galaxies across cosmic time
• Dual Effects of Ram Pressure on Star Formation in Multi-phase Disk Galaxies with Strong Stellar Feedback
• Lithium abundance and rotation of seismic solar analogues - Solar and stellar connection from Kepler and Hermes observations
• Using the Tip of the Red Giant Branch as a Distance Indicator in the Near Infrared
• A new solar fluorine abundance and a fluorine determination in the two open clusters M 67 and NGC 6404
• Rapid-response mode VLT/UVES spectroscopy of super iron-rich gas exposed to GRB 080310. Evidence of ionization in action and episodic star formation in the host
• Evolutionary modelling of subdwarf B stars using MESA with the predictive mixing and convective premixing schemes
• Transmission spectroscopy for the warm sub-Neptune HD3167c: evidence for molecular absorption and a possible high metallicity atmosphere
• Fluorine in the Solar Neighborhood: Chemical Evolution Models
• Spectroscopic analysis of the two subgiant branches of the globular cluster NGC1851
• SPLUSJ210428.01-004934.2: An Ultra Metal-Poor Star Identified from Narrowband Photometry
• Models of solar surface dynamics: impact on eigenfrequencies and radius
• On the observability of bow shocks of Galactic runaway OB stars
• Early chemo-dynamical evolution of dwarf galaxies deduced from enrichment of r-process elements
• VLT/X-shooter spectroscopy of the afterglow of the Swift GRB 130606A: Chemical abundances and reionisation at $z\sim 6$
• Towards a radially-resolved semi-analytic model for the evolution of disc galaxies tuned with machine learning
• Ammonium hydrosulfide (NH4SH) as a potentially significant sulfur sink in interstellar ices
• Zero and extremely low metallicity rotating massive stars: evolution, explosion, and nucleosynthesis up to the heaviest nuclei
• The Gas Composition and Deep Cloud Structure of Jupiter's Great Red Spot
• Mean density inversions for red giants and red clump stars
• On the dependence of the type Ia SNe luminosities on the metallicity of their host galaxies
• Radial Profile of the 3.55 keV line out to $R_{200}$ in the Perseus Cluster
• The R-Process Alliance: Discovery of the first metal-poor star with a combined r- and s-process element signature
• Abundances of neutron-capture elements in thin- and thick-disc stars in the solar neighbourhood
• The MOSDEF Survey: The Metallicity Dependence of X-ray Binary Populations at $z\sim 2$
• Observing Isotopologue Bands in Terrestrial Exoplanet Atmospheres with the James Webb Space Telescope---Implications for Identifying Past Atmospheric and Ocean Loss
• Consistently Simulating a Wide Range of Atmospheric Scenarios for K2-18b with a Flexible Radiative Transfer Module
• JADES: Primaeval Lyman-$\alpha$ emitting galaxies reveal early sites of reionisation out to redshift $z\sim 9$
• The Nature of Ionized Gas in the Milky Way Galactic Fountain
• The Effects of Initial Abundances on Nitrogen in Protoplanetary Disks
• A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
• Abundances of disk and Bulge giants from high-resolution optical spectra III. Sc, V, Cr, Mn, Co, Ni
• Seven years of coordinated Chandra-NuSTAR observations of SN2014C unfold the extreme mass-loss history of its stellar progenitor
• The FIP and Inverse FIP Effects in Solar Flares
• Dynamically Tagged Groups of Metal-Poor Stars from the Best \& Brightest Survey
• The galaxy cluster outskirts probed by Chandra
• Discovery of Rubidium, Cadmium, and Germanium Emission Lines in the Near-Infrared Spectra of Planetary Nebulae
• Neutrino Fluxes from CMSSM LSP Annihilations in the Sun
• Super-solar metallicity at the position of the ultra-long GRB130925A
• Stellar Winds and Coronae of Low-mass Pop. II/III Stars
• Combining multiple structural inversions to constrain the Solar modelling problem
• ${\zeta }^2$ Ret, its debris disk, and its lonely stellar companion ${\zeta }^1$ Ret. Different $T_{\mathrm{c}}$ trends for different spectra
• The stellar and wind parameters of six prototypical HMXBs and their evolutionary status
• Using seismic inversions to obtain an internal mixing processes indicator for main-sequence solar-like stars
• Magnetism, X-rays, and Accretion Rates in WD 1145+017 and other Polluted White Dwarf Systems
• Spectral modeling of type II supernovae II. A machine learning approach to quantitative spectroscopic analysis
• High-resolution observations of gas and dust around Mira using ALMA and SPHERE/ZIMPOL
• Progenitor Model of SN 1987A Based on the Slow Merger Scenario
• The Age and Stellar Parameters of the Procyon Binary System
• TESS Giants Transiting Giants II: The hottest Jupiters orbiting evolved stars
• The ionisation parameter of star-forming galaxies evolves with the specific star formation rate
• Constraints on the distance moduli, helium and metal abundances, and ages of globular clusters from their RR Lyrae and non-variable horizontal-branch stars. II. Multiple stellar populations in 47Tuc, M3, and M13
• A study of low-metallicity DLAs at high redshift and C II* as a probe of their physical conditions
• Probing the Physical Conditions of Atomic Gas at High Redshift
• On the Impact of Helium Content on the RR Lyrae Distance Scale
• Origin of Cosmic Chemical Abundances
• A synthetic population of Wolf-Rayet stars in the LMC based on detailed single and binary star evolution models
• Lithium depletion boundary, stellar associations, and Gaia
• Measuring Star-formation Rate and Far-Infrared Color in High-redshift Galaxies Using the CO (7-6) and [NII] 205 micron Lines
• A prescription for the asteroseismic surface correction
• The Evolution and Physical Parameters of WN3/O3s: a New Type of Wolf-Rayet Star
• Tidal dissipation in rotating low-mass stars and implications for the orbital evolution of close-in massive planets. II. Effect of stellar metallicity
• Star formation in the outskirts of DDO 154: A top-light IMF in a nearly dormant disc
• Stellar population astrophysics (SPA) with the TNG. Revisiting the metallicity of Praesepe (M44)
• An inefficient dwarf: Chemical abundances and the evolution of the Ursa Minor dwarf spheroidal galaxy
• The Galactic habitable zone around M and FGK stars with chemical evolution models with dust
• Spectral and Timing Nature of the Symbiotic X-ray Binary 4U 1954+319: The Slowest Rotating Neutron Star in an X-ray Binary System
• GASP XXXIV: Unfolding the thermal side of ram pressure stripping in the jellyfish galaxy JO201
• V1369 Cen high resolution panchromatic late nebular spectra in the context of a unified picture for nova ejecta
• The Herschel Virgo Cluster Survey. XI. Environmental effects on molecular gas and dust in spiral disks
• The Magellanic Stream: break up and accretion onto the hot Galactic corona
• Neutrino physics with dark matter detectors
• The chemical composition of a regular halo globular cluster: NGC 5897
• The Pristine survey -- XII: Gemini-GRACES chemo-dynamical study of newly discovered extremely metal-poor stars in the Galaxy
• PTF11mnb: the first analog of supernova 2005bf
• Chemical Abundances for Evolved Stars in M5: Lithium through Thorium
• The fate of the Antennae galaxies
• The Distribution and Origin of C${}_2$H in NGC 253 from ALCHEMI
• High resolution spectroscopic follow-up of the most metal-poor candidates from SkyMapper DR1.1
• Two distinct halo populations in the solar neighborhood. IV. Lithium abundances
• The detailed chemical abundance patterns of accreted halo stars from the optical to infrared
• Carbon abundance and the N/C ratio in atmospheres of A-, F- and G-type supergiants and bright giants
• Relationship between low and high frequencies in Delta Scuti stars: Photometric Kepler and spectroscopic analyses of the rapid rotator KIC 8054146
• Environmental Effects on the Metal Enrichment of Low Mass Galaxies in Nearby Clusters
• Resolving a dusty, star-forming SHiZELS galaxy at z=2.2 with HST, ALMA and SINFONI on kiloparsec scales
• Developing a self-consistent AGB wind model: II. Non-classical, non-equilibrium polymer nucleation in a chemical mixture
• How drifting and evaporating pebbles shape giant planets III: The formation of WASP-77A b and $\tau$ Boötis b
• Further insight on the hypervelocity white dwarf, LP 40-365 (GD 492): a nearby emissary from a single-degenerate Type Ia supernova
• Metal-Rich PNe in the Outer Reaches of M31
• Chemical abundances in Galactic planetary nebulae with Spitzer spectra
• Exploring Io's atmospheric composition with APEX: first measurement of 34SO2 and tentative detection of KCl
• Tomography of cool giant and supergiant star atmospheres II. Signature of convection in the atmosphere of the red supergiant star $\mu$ Cep
• GRB171010A / SN2017htp: a GRB-SN at z=0.33
• On the Use of Field RR Lyrae as Galactic Probes. III. The $\alpha$-element abundances
• Molecular observations of comets C/2012 S1 (ISON) and C/2013 R1 (Lovejoy): HNC/HCN ratios and upper limits to PH3
• Outflows from active galactic nuclei: The BLR-NLR metallicity correlation
• Seismic probing of the first dredge-up event through the eccentric red-giant & red-giant spectroscopic binary KIC9163796
• Nucleosynthesis in helium-enriched asymptotic giant branch models: Implications for Heavy Element Enrichment in Omega Centauri
• Seismic signature of electron degeneracy in the core of red giants: hints for mass transfer between close red-giant companions
• Differential rotation in main-sequence solar-like stars: Qualitative inference from asteroseismic data
• Galaxy gas flows inferred from a detailed, spatially resolved metal budget
• Cosmic Origins Spectrograph and FUSE Observations of T ~ 10^5 K Gas In A Nearby Galaxy Filament
• Blue diffuse dwarf galaxies: a clearer picture
• Metal-poor stars observed with the automated planet finder telescope. I. Discovery of five carbon-enhanced metal-poor stars from LAMOST
• Origin of the CEMP-no Group Morphology in the Milky Way
• A chemical kinetics code for modelling exoplanetary atmospheres
• The Ages of Galactic Bulge Stars with Realistic Uncertainties
• Detection of burning ashes from thermonuclear X-ray bursts
• High resolution elemental abundance analysis of the Hyades Supercluster
• Oxygen, neon, and iron X-ray absorption in the local interstellar medium
• The abundance and thermal history of water ice in the disk surrounding HD142527 from the DIGIT Herschel Key Program
• High precision analysis of the solar twin HIP 100963
• The Sunburst Arc with JWST: I. Detection of Wolf-Rayet stars injecting nitrogen into a low-metallicity, $z=2.37$ proto-globular cluster leaking ionizing photons
• Three-dimensional surface convection simulations of metal-poor stars -- The effect of scattering on the photospheric temperature stratification
• High-resolution abundance analysis of red giants in the metal-poor bulge globular cluster HP~1
• Theoretical Estimates of Stellar e-Captures. I. The half-life of 7Be in Evolved Stars
• Aluminium oxide in the atmosphere of hot Jupiter WASP-43b
• Missing cosmic metals revealed by X-ray absorption towards distant sources
• SN 2016iet: The Pulsational or Pair Instability Explosion of a Low Metallicity Massive CO Core Embedded in a Dense Hydrogen-Poor Circumstellar Medium
• Direct measurement of the [CI] luminosity to molecular gas mass conversion factor in high-redshift star-forming galaxies
• Probing the axion-nucleon coupling with the next generation of axion helioscopes
• Exoplanet Spectroscopy with JWST NIRISS: Diagnostics and Case Studies
• A quantitative in-depth analysis of the prototype sdB+BD system SDSS J08205+0008 revisited in the Gaia era
• How Environment Affects Galaxy Metallicity through Stripping and Formation History: Lessons from the Illustris Simulation
• The chemical composition of globular clusters in the Local Group
• Escaping Helium and a Highly Muted Spectrum Suggest a Metal-Enriched Atmosphere on Sub-Neptune GJ3090b from JWST Transit Spectroscopy
• Detecting axisymmetric magnetic fields using gravity modes in intermediate-mass stars
• Revealing the Milky Way's Hidden Circumgalactic Medium with the Cosmic Origins Spectrograph Quasar Database for Galactic Absorption Lines
• Physical Properties of II Zw 40's Super Star Cluster and Nebula: New Insights and Puzzles from UV Spectroscopy
• HST/COS observations of a new population of associated QSO absorbers
• Line broadening and the solar opacity problem
• Study of CS, SiO, and SiS abundances in carbon star envelopes: Assessing their role as gas-phase precursors of dust
• Considerations for Atmospheric Retrieval of High-Precision Brown Dwarf Spectra
• TOI-1759 b: a transiting sub-Neptune around a low mass star characterized with SPIRou and TESS
• Resonant scattering in galaxy clusters for anisotropic gas motions on various spatial scales
• MOVES IV. Modelling the influence of stellar XUV-flux, cosmic rays, and stellar energetic particles on the atmospheric composition of the hot Jupiter HD 189733b
• Highly-ionized metals as probes of the circumburst gas in the natal regions of gamma-ray bursts
• Significant uncertainties from calibrating overshooting with eclipsing binary systems
• TESS Hunt for Young and Maturing Exoplanets (THYME) IX: a 27 Myr extended population of Lower-Centaurus Crux with a transiting two-planet system
• On the Nature of the HII Regions in the Extended Ultraviolet Disc of NGC 4625
• Dense Gas in M33 (HerM33es)
• Rapid Elimination of Small Dust Grains in Molecular Clouds
• Three-dimensional chemically homogeneous and bi-abundance photoionization models of the "super-metal-rich" planetary nebula NGC 6153
• The solar energetic balance revisited by young solar analogs, helioseismology and neutrinos
• H2, CO, and Dust Absorption through Cold Molecular Clouds
• The R-Process Alliance: The Peculiar Chemical Abundance Pattern of RAVE J183013.5-455510
• The ANU WiFeS SuperNovA Program (AWSNAP)
• COS-Weak: Probing the CGM using analogs of weak Mg II absorbers at z < 0.3
• The puzzle of the CNO isotope ratios in AGB carbon stars
• On the kinematic separation of field and cluster stars across the Bulge globular NGC 6528
• Stellar wind models of subluminous hot stars
• Graphite Revisited
• Analysis of two SMC HII Regions Considering Thermal Inhomogeneities: Implications for the Determinations of Extragalactic Chemical Abundances
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• Jupiter's Deep Cloud Structure Revealed Using Keck Observations of Spectrally Resolved Line Shapes
• The carbon-to-oxygen ratio: implications for the spectra of hydrogen-dominated exoplanet atmospheres
• Properties of the post in-spiral common envelope ejecta II: dust formation
• The Cosmic Hunt for Members in the Outskirts of Ultra Faint Dwarf Galaxies: Ursa Major I, Coma Berenices, and Boötes I
• The Origin of Solar Filament Plasma Inferred from in situ Observations of Elemental Abundances
• Dust in brown dwarfs and extra-solar planets. VII. Cloud formation in diffusive atmospheres
• Ionized gas kinematics and chemical abundances of low-mass star-forming galaxies at $z\sim 3$
• Identifying Young $Kepler$ Planet Host Stars from Keck-HIRES Spectra of Lithium
• Aluminium-26 from massive binary stars I: non-rotating models
• Detailed Abundances of 15 Stars in the Metal-Poor Globular Cluster NGC 4833
• Spitzer 70~$\mu$m Emission as a SFR Indicator for Sub--Galactic Regions
• Luminosity Dependence and Redshift Evolution of Strong Emission-line Diagnostics in Star-Forming Galaxies
• A new galactic chemical evolution model with dust: results for dwarf irregular galaxies and DLA systems
• Radial velocity information content of M dwarf spectra in the near-infrared
• Detection of Phosphorus, Sulphur, and Zinc in the Carbon-Enhanced Metal-Poor Star BD+44 493
• Coupling 1D stellar evolution with 3D-hydrodynamical simulations on-the-fly II: Stellar Evolution and Asteroseismic Applications
• A new census of dust and polycyclic aromatic hydrocarbons at z=0.7-2 with JWST MIRI
• Stellar laboratories III. New Ba V, Ba VI, and Ba VII oscillator strengths and the barium abundance in the hot white dwarfs G191-B2B and RE0503-289
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• Modeling the Infrared Interstellar Extinction
• AGN Feedback in Galaxy Group 3C 88: Cavities, Shock and Jet Reorientation
• Pre-supernova feedback sets the star cluster mass function to a power law and reduces the cluster formation efficiency
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• ALMA detection of CO rotational line emission in red supergiant stars of the massive young star cluster RSGC1 -- Determination of a new mass-loss rate prescription for red supergiants
• Constraint on Light Dipole Dark Matter from Helioseismology
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• Gaia Gaps and the Physics of Low-Mass Stars. I. The Fully Convective Boundary
• Effects of thermohaline instability and rotation-induced mixing on the evolution of light elements in the Galaxy : D, 3He and 4He
• Homogeneous Analysis of Globular Clusters from the APOGEE Survey with the BACCHUS Code $-$ III. $\omega$ Cen
• Stellar laboratories IV. New Ga IV, Ga V, and Ga VI oscillator strengths and the gallium abundance in the hot white dwarfs G191-B2B and RE0503-289
• Herbig Stars: A Quarter Century of Progress
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• Spectroscopic study of CEMP-(s & r/s) stars- Revisiting classification criteria and formation scenarios, highlighting i-process nucleosynthesis
• Diagnostics of Stellar Modelling from Spectroscopy and Photometry of Globular Clusters
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• MgII in the JWST Era: a Probe of Lyman Continuum Escape?
• The [O III] Nebula of the Merger Remnant NGC 7252: A Likely Faint Ionization Echo
• Thermal and energetic processing of astrophysical ice analogues rich in SO${}_2$
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• Pre-Supernova Neutrinos in Large Dark Matter Direct Detection Experiments
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• Discovery of secular variations in the atmospheric abundances of magnetic Ap stars
• Pulsational amplitude growth of the star KIC 3429637 (HD 178875) in the context of Am and rho Puppis stars
• Five transiting hot Jupiters discovered using WASP-South, Euler and TRAPPIST: WASP-119 b, WASP-124 b, WASP-126 b, WASP-129 b and WASP-133 b
• Carbon abundances of the reference late-type stars from 1D analysis of atomic C I and molecular CH lines
• Spectrum Syntheses of High Resolution Integrated Light Spectra of Galactic Globular Clusters
• Advanced Scintillator Detector Concept (ASDC): A Concept Paper on the Physics Potential of Water-Based Liquid Scintillator
• A proto-helium white dwarf stripped by a substellar companion via common-envelope ejection -- Uncovering the true nature of a candidate hypervelocity B-type star
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• First extragalactic detection of a phosphorus-bearing molecule with ALCHEMI: phosphorus nitride (PN)
• Dust in the Wind: Composition and Kinematics of Galaxy Outflows at the Peak Epoch of Star Formation
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• An Early-Time Optical and Ultraviolet Excess in the type-Ic SN 2020oi
• The ESO UVES Advanced Data Products Quasar Sample - III. Evidence of Bimodality in the [N/alpha] Distribution
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• The Abundances of Light Neutron-Capture Elements in Planetary Nebulae III. The Impact of New Atomic Data on Nebular Selenium and Krypton Abundance Determinations
• The Semi-forbidden CIII]$\lambda$1909Å~ Emission in the Rest-Ultraviolet Spectra of Green Pea Galaxies
• Lenticular galaxy IC 719: current building of the counterrotating large-scale stellar disk
• Chemical Feature of Eu abundance in the Draco dwarf spheroidal galaxy
• A New Test of Copper and Zinc Abundances in Late-Type Stars Using Ultraviolet Cu II and Zn II Lines
• Detecting the warm-hot intergalactic medium through X-ray absorption lines
• TOI-1130: A photodynamical analysis of a hot Jupiter in resonance with an inner low-mass planet
• Interstellar polarization and grain alignment: the role of iron and silicon
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• The Gas-Star Formation Cycle in Nearby Star-forming Galaxies II. Resolved Distributions of CO and H$\alpha$ Emission for 49 PHANGS Galaxies
• Late-time Flattening of Type Ia Supernova Light Curves: Constraints From SN 2014J in M82
• Non-LTE analysis of copper abundances for the two distinct halo populations in the solar neighborhood
• Explaining the differences in massive star models from various simulations
• Using the local gas-phase oxygen abundances to explore a metallicity-dependence in SNe Ia luminosities
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• A new type of X-ray pulsar
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• Elemental Abundances of M Dwarfs Based on High-Resolution Near-Infrared Spectra: Verification by Binary Systems
• The Chemical Compositions of Very Metal-Poor Stars HD 122563 and HD 140283; A View From the Infrared
• Recipes for bolometric corrections and Gaia luminosities of B-type stars: Application to an asteroseismic sample
• Chemical abundance study of two strongly s-process enriched post-AGB stars in the LMC: J051213.81-693537.1 and J051848.86-700246.9
• The effect of a strong pressure bump in the Sun's natal disk: Terrestrial planet formation via planetesimal accretion rather than pebble accretion
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• Discovery of an X-ray Quasar Wind Driving the Cold Gas Outflow in the Ultraluminous Infrared Galaxy IRAS F05189-2524
• GPU-based Monte Carlo dust radiative transfer scheme applied to AGN
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• Near-infrared spectroscopy of five Blue Compact Dwarf galaxies: II Zw 40, Mrk 71, Mrk 930, Mrk 996 and SBS 0335-052E
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• Collapsar R-Process Yields Can Reproduce [Eu/Fe] Abundance Scatter in Metal-Poor Stars
• Mind the gap: Distinguishing disc substructures and their impact on the inner disc composition
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• Hydrogen chloride in diffuse interstellar clouds along the line of sight to W31C (G10.6-0.4)
• Retrieval study of cool, directly imaged exoplanet 51 Eri b
• Coupling 1D stellar evolution with 3D-hydrodynamical simulations on-the-fly I: A New Standard Solar Model
• Discovery of Rapidly Moving Partial X-ray Absorbers within gamma Cassiopeiae
• Understanding the orbital periods of CEMP-s stars
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• Astrophysical S-factor of the ${}^{14}\text{N(p,}\gamma {\text{)}}^{15}\text{O}$ reaction at 0.4 -- 1.3\,MeV
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• Modeling broadband X-ray absorption of massive star winds
• Thermal emission from bow shocks I: 2D Hydrodynamic Models of the Bubble Nebula
• Stars and gas in the most metal-poor galaxies I: COS and MUSE observations of SBS 0335-052E
• Limb darkening laws for two exoplanet host stars derived from 3D stellar model atmospheres
• Solar neutrino flux at keV energies
• Ca line formation in late-type stellar atmospheres: I. The model atom
• Non-LTE Sodium Abundance in Galactic Thick- and Thin-Disk Red Giants
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• Metal-poor Stars Observed with the Automated Planet Finder Telescope. II. Chemodynamical Analysis of Six Low-Metallicity Stars in the Halo System of the Milky Way
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• X-rays observations of a super-Chandrasekhar object reveal an ONeMg and a CO white dwarf merger product embedded in a putative SN Iax remnant
• Analysis of cool DO-type white dwarfs from the Sloan Digital Sky Survey Data Release 10
• Metallicity Distribution Functions of 13 Ultra-Faint Dwarf Galaxy Candidates from Hubble Space Telescope Narrowband Imaging
• Global hot-star wind models for stars from Magellanic Clouds
• OH/IR stars and their superwinds as observed by the Herschel Space Observatory
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• Detailed chemical abundances of stars in the outskirts of the Tucana II ultra-faint dwarf galaxy
• The relation between atomic gas and star formation rate densities in faint irregular galaxies
• The VLT-FLAMES Tarantula Survey: XXVIII. Nitrogen abundances for apparently single dwarf and giant B-type stars with small projected rotational velocities
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• HST Emission Line Galaxies at z ~ 2: The Mystery of Neon
• The eROSITA view of the Abell 3391/95 field: a case study from the Magneticum cosmological simulation
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• Methane in Analogs of Young Directly Imaged Exoplanets
• ALMACAL III: A combined ALMA and MUSE Survey for Neutral, Molecular, and Ionised Gas in an HI-Absorption-Selected System
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• The Luminous and Double-Peaked Type Ic Supernova 2019stc: Evidence for Multiple Energy Sources
• Chemical Abundances in the Leading Arm of the Magellanic Stream
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• X-ray binary accretion states in Active Galactic Nuclei? Sensing the accretion disc of supermassive black holes with mid-infrared nebular lines
• Circumstellar environment of the M-type AGB star R Dor. APEX spectral scan at $159.0-368.5$ GHz
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• Insights into the chemical composition of the metal-poor Milky Way halo globular cluster NGC 6426
• 21-cm absorption from galaxies at z ~ 0.3
• Evidence for the preferential disruption of moderately massive stars by supermassive black holes
• Planet and star synergy at high spectral resolution. A rationale for the characterisation of exoplanet atmospheres. I. The Infrared
• The radial abundance gradient of chlorine in the Milky Way
• Exploring the link between star and planet formation with Ariel
• Explosive Nucleosynthesis in Near-Chandrasekhar-mass White Dwarf Models for Type Iax Supernovae: Dependence on Model Parameters
• TAPAS - Tracking Advanced Planetary Systems with HARPS-N. II. Super Li-rich giant HD 107028
• Highly Excited Core Resonances in Photoionization of Fe XVII : Implications for Plasma Opacities
• Chemical analysis of CH stars - I: atmospheric parameters and elemental abundances
• A MeerKAT-meets-LOFAR Study of MS 1455.0+2232: A 590 kiloparsec 'Mini'-Halo in a Sloshing Cool-Core Cluster
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• The G+M eclipsing binary V530 Orionis: A stringent test of magnetic stellar evolution models for low-mass stars
• Herschel Spectroscopic Observations of LITTLE THINGS Dwarf Galaxies
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• Nucleosynthesis Constraints on the Explosion Mechanism for Type Ia Supernovae
• About Metallicity Variations in the Local Galactic Interstellar Medium
• GAMBIT and its Application in the Search for Physics Beyond the Standard Model
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• Resolving Ionisation and Metallicity on Parsec Scales Across Mrk 71 with HST-WFC3
• Evolutionary models for ultracool dwarfs
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• Lithium abundance in atmospheres of F- and G-type supergiants and bright giants
• The Chemical Evolution of Galaxy Clusters: Dissecting the Iron Mass Budget of the Intracluster Medium
• Non-LTE analysis of neutral copper in the late-type metal-poor stars
• A temporal study of oxygen-rich pulsating variable AGB star, T Cep: Investigation on dust formation and dust properties
• Time Dependent Non-Equilibrium Ionization of Transition Region Lines Observed with IRIS
• Abell 48 - a rare WN-type central star of a planetary nebula
• In-depth study of 16CygB using inversion techniques
• Stellar laboratories. VI. New Mo IV - VII oscillator strengths and the molybdenum abundance in the hot white dwarfs G191-B2B and RE0503-289
• A High-Resolution Investigation of the Multi-Phase ISM in a Galaxy during the First Two Billion Years
• Insight into the Starburst Nature of Galaxy GN-z11 with JWST MIRI Spectroscopy
• The initial gas-phase sulfur abundance in the Orion Molecular Cloud from sulfur radio recombination lines
• HD66051: the first eclipsing binary hosting an early-type magnetic star
• Phosphorous chemistry in the shocked region L1157 B1
• X-ray Properties of NGC 253's Starburst-Driven Outflow
• Planetary Nebula Luminosity Function distances for 19 galaxies observed by PHANGS-MUSE
• New mass-loss rates of B supergiants from global wind models
• Mass and Metallicity Requirement in Stellar Models for Galactic Chemical Evolution Applications
• The resolved scaling relations in DustPedia: Zooming in on the local Universe
• Dissecting the interstellar medium of a z=6.3 galaxy: X-shooter spectroscopy and HST imaging of the afterglow and environment of the Swift GRB 210905A
• Helium abundance and speed difference between helium ions and protons in the solar wind from coronal holes, active regions, and quiet Sun
• Full orbital solution for the binary system in the northern Galactic disc microlensing event Gaia16aye
• VLT/X-shooter observations of blue compact galaxies Haro 11 and ESO 338-IG 004
• A GMOS-N IFU study of the central H II region in the blue compact dwarf galaxy NGC 4449: Kinematics, Nebular Metallicity and Star-Formation
• The Lightweaver Framework for NLTE Radiative Transfer in Python
• Sulphur-bearing molecules in AGB stars II: Abundances and distributions of CS and SiS
• HI content, metallicities and spin temperatures of damped and sub-damped Lyman alpha systems in the redshift desert (0.6 < z < 1.7)
• The Impact of Star-Formation-Rate Surface Density on the Electron Density and Ionization Parameter of High-Redshift Galaxies
• The Mean Metal-line Absorption Spectrum of DLAs in BOSS
• ALMA + VLT observations of a Damped Lyman-α absorbing galaxy: Massive, wide CO emission, gas-rich but with very low SFR
• Giant planet engulfment by evolved giant stars: light curves, asteroseismology, and survivability
• New solar twins and the metallicity and temperature scales of the Geneva Copenhagen Survey
• Spectroscopic Observations of Fe XVIII in Solar Active Regions
• Pure iron grains are rare in the universe
• Tidal Disruptions of Main Sequence Stars of Varying Mass and Age: Inferences from the Composition of the Fallback Material
• Probing the large and massive CGM of a galaxy at z ~ 0.2 using a pair of quasars
• Iron-peak elements Sc, V, Mn, Cu and Zn in Galactic bulge globular clusters
• Critical angular velocity and anisotropic mass loss of rotating stars with radiation-driven winds
• The MOSDEF Survey: The Mass-Metallicity relationship and the existence of the FMR at z~1.5
• Star-forming galaxies are predicted to lie on a fundamental plane of mass, star formation rate and α-enhancement
• Advances in Global and Local Helioseismology: an Introductory Review
• A 3D Photoionization Model of the Extreme Planetary Nebula NGC 6302
• Spectroscopic detection of multiple populations in the ~2 Gyr old cluster Hodge 6 in the LMC
• Chemical analysis of CH stars - III: Atmospheric parameters and elemental abundances
• Shallow extra mixing in solar twins inferred from Be abundances
• Neutronization During Carbon Simmering In Type Ia Supernova Progenitors
• The 3D non-LTE solar nitrogen abundance from atomic lines
• Chemical evolution of elliptical galaxies with a variable IMF -- A publicly available code
• Investigating surface correction relations for RGB stars
• Observing the metal-poor solar neighbourhood: a comparison of galactic chemical evolution predictions
• Ages of massive galaxies at $0.5<z<2.0$ from 3D-HST rest-frame optical spectroscopy
• The Relation Between Galaxy ISM and Circumgalactic OVI Gas Kinematics Derived from Observations and $\Lambda$CDM Simulations
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• Constraints on stellar rotation from the evolution of Sr and Ba in the Galactic halo
• Implications of inhomogeneous metal mixing for stellar archaeology
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• KIC 7582608: A new Kepler roAp star with frequency variability
• A Low Metallicity Molecular Cloud In The Lower Galactic Halo
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• Light $p$-shell nuclei with cluster structures ($4\le A\le 16$) in nuclear matter
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• Chemical Evolution with Radial Mixing Redux: Extending beyond the Solar Neighborhood
• Molecular Hydrogen Absorption from the Halo of a z ~ 0.4 Galaxy
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• Far-UV HST Spectroscopy of An Unusual Hydrogen Poor Superluminous Supernova: SN2017egm
• The $\gamma$-process nucleosynthesis in core-collapse supernovae. I. A novel analysis of $\gamma$-process yields in massive stars
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• BOWIE-ALIGN: How formation and migration histories of giant planets impact atmospheric compositions
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• Heavy metals in intermediate He-rich hot subdwarfs: The chemical composition of HZ44 and HD127493
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• 2MASS J18082002-5104378: The brightest (V=11.9) ultra metal-poor star
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• Spectropolarimetric analysis of an active region filament. I. Magnetic and dynamical properties from single component inversions
• Elemental Abundances in the Ejecta of Old Classical Novae from Late-Epoch Spitzer Spectra
• Sodium abundances of AGB and RGB stars in Galactic globular clusters II. Analysis and results of NGC 104, NGC 6121 and NGC 6809
• Gaia-ESO Survey: Role of magnetic activity and starspots on pre-main sequence lithium evolution
• High-resolution abundance analysis of HD 140283
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• The Impact of Black Hole Formation on Population Averaged Supernova Yields
• H- and Dissociation in Ultra-hot Jupiters: A Retrieval Case Study of WASP-18b
• LAMOST Time-Domain Survey: First Results of four $K$2 plates
• Neptune's Latitudinal Variations as Viewed with ALMA
• The planetary nebula Abell 48 and its [WN] nucleus
• The R-Process Alliance: J1521-3538, a very metal-poor, extremely r-process-enhanced star with [Eu/Fe]=+2.2, and the class of r-III stars
• Heavy elements in barium stars
• Fluorine abundances in dwarf stars of the solar neighbourhood
• Cosmic nucleosynthesis: a multi-messenger challenge
• Physical properties of the X-ray gas as a dynamical diagnosis for galaxy clusters
• Rotational evolution of solar-type protostars during the star-disk interaction phase
• Dust extinction bias in the column density distribution of gamma-ray bursts; high column density, low redshift GRBs are more heavily obscured
• The effect of feedback on the emission properties of the Warm-Hot Intergalactic Medium
• Dust clearing by radial drift in evolving protoplanetary discs
• The EBLM Project VI. The mass and radius of five low-mass stars in F+M binaries discovered by the WASP survey
• K2-98 b: A 32-M${}_{\oplus }$ Neptune-sized planet in a 10-day orbit transiting an F8 star
• Evidence for massive warm-hot circumgalactic medium around NGC 3221
• A combined multiwavelength VLA/ALMA/Chandra study unveils the complex magnetosphere of the B-type star HR5907
• Non-Equilibrium Chemistry and Destruction of CO by X-ray Flares
• Stars stripped in binaries -- the living gravitational wave sources
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• Constraints on the structure of 16 Cyg A and 16 Cyg B using inversion techniques
• Modelling dust processing and the evolution of grain sizes in the ISM using the method of moments
• Nucleosynthesis of an $11.8M_{\odot }$ Supernova with 3D Simulation of the Inner Ejecta: Overall Yields and Implications for Short-Lived Radionuclides in the Early Solar System
• Chemical evolution of the Universe at 0.7 < z < 1.6 derived from abundance diagnostics of the broad-line region of quasars
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• The Detection of [O III]$\lambda$4363 in a Lensed, Dwarf Galaxy at $z$ = 2.59: Testing Metallicity Indicators and Scaling Relations at High Redshift and Low Mass
• Detection of emission lines from z ~ 3 DLAs towards the QSO J2358+0149
• A Lyα blob and zabs {\approx} zem damped Lyα absorber in the dark matter halo of the binary quasar Q 0151+048
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• Stellar modelling of Spica, a high-mass spectroscopic binary with a beta Cep variable primary component
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• Formation of star clusters and enrichment by massive stars in simulations of low-metallicity galaxies with a fully sampled initial stellar mass function
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• The First Robust Constraints on the Relationship Between Dust-to-Gas Ratio and Metallicity in Luminous Star-forming Galaxies at High Redshift
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• The R-Process Alliance: Chemical Abundances for a Trio of R-Process-Enhanced Stars -- One Strong, One Moderate, One Mild
• Quantitative Spectroscopic J-band Study of Red Supergiants in Perseus OB-1
• The Carina Project. V. The impact of NLTE effects on the iron content
• Evolution of the Stellar Mass-Metallicity Relation. II. Constraints on Galactic Outflows from the Mg Abundances of Quiescent Galaxies
• Thorium in solar twins: implications for habitability in rocky planets
• Imaging detection of the inner dust belt and the four exoplanets in the HR8799 system with JWST's MIRI coronagraph
• Resolving the Dust-to-Metals Ratio and CO-to-H${}_2$ Conversion Factor in the Nearby Universe
• Ultraviolet Spectroscopy of Circumnuclear Star Clusters in M83
• OCCASO V. Chemical-abundance trends with Galactocentric distance and age
• Late-time observations of the relativistic tidal disruption flare candidate Swift J1112.2-8238
• Isochrone-cloud fitting of the extended Main-Sequence Turn-Off of young clusters
• The chemical abundance pattern of the extremely metal-poor thin disk star 2MASS J1808-5104 and its origins
• The essential elements of dust evolution: A viable solution to the interstellar oxygen depletion problem?
• The Old, Super-Metal-Rich Open Cluster, NGC 6791 - Elemental Abundances in Turn-off Stars from Keck/HIRES Spectra
• The Puzzling Li-rich Red Giant Associated with NGC 6819
• First Light And Reionisation Epoch Simulations (FLARES) VII: The Star Formation and Metal Enrichment Histories of Galaxies in the early Universe
• The Three Hundred Project: the stellar and gas profiles
• A critical assessment of the metal content of the ICM
• RELICS: Spectroscopy of gravitationally-lensed $z\simeq 2$ reionization-era analogs and implications for CIII] detections at $z>6$
• An extreme paucity of second population AGB stars in the normal globular cluster M4
• The Galactic R Coronae Borealis stars : the C2 Swan bands, the carbon problem, and the 12C/13C ratio
• Inferring the composition of super-Jupiter mass companions of pulsars with radio line spectroscopy
• On the abiotic origin of dimethyl sulfide: discovery of DMS in the Interstellar Medium
• X-ray, UV and optical analysis of supergiants: $\epsilon$ Ori
• A Metal-Strong and Dust-Rich Damped \lya Absorption System toward the Quasar SDSS J115705.52+615521.7
• CMF models of hot star winds II. Reduction of O star wind mass-loss rates in global models
• Metal Mixing in Minihalos: The Descendants of Pair-Instability Supernovae
• Sodium abundances of AGB and RGB stars in galactic globular clusters I. Analysis and results of NGC 2808
• A Hydrogen-Poor Superluminous Supernova with Enhanced Iron-Group Absorption: A New Link Between SLSNe and Broad-Lined Type Ic SNe
• Impact of AGN feedback on galaxies and their multiphase ISM across cosmic time
• EMPRESS. VII. Ionizing Spectrum Shapes of Extremely Metal-Poor Galaxies: Uncovering the Origins of Strong HeII and the Impact on Cosmic Reionization
• FTS atlas of the Sun's spectrally resolved center-to-limb variation
• Small-scale Dynamo in Cool Stars: I. Changes in stratification and near-surface convection for main-sequence spectral types
• Low-Temperature Gas Opacities with AESOPUS 2.0
• Planet Engulfment Signatures in Twin Stars
• X-ray spectroscopy of the ADC source X1822-371 with Chandra and XMM-Newton
• A Channel to Form Fast-spinning Black Hole--Neutron Star Binary Mergers as Multi-messenger Sources
• Formation of carbon-enhanced metal-poor stars as a consequence of inhomogeneous metal mixing
• Mapping "out-of-the-box" the properties of the baryons in massive halos
• New solar metallicity measurements
• The Chemical Evolution of Phosphorus
• Lithium depletion and angular momentum transport in F-type and G-type stars in Galactic open clusters
• Chemical modeling of the L1498 and L1517B prestellar cores: CO and HCO+ depletion
• Direct determination of the solar neutrino fluxes from solar neutrino data
• The Chemical Compositions and Evolutionary Status of Red Giants in the Open Cluster NGC 752
• Implications of solar wind measurements for solar models and composition
• KODIAQ-Z: Metals and Baryons in the Cool Intergalactic and Circumgalactic Gas at 2.2<z<3.6
• Stellar Coronae, Solar Flares: a Detailed Comparison of sigma Gem, HR 1099, and the Sun in High-resolution X-rays
• Modeling ionized gas in low-metallicity environments: the Local Group dwarf galaxy IC10
• A comparison of UV and optical metallicities in star-forming galaxies
• The physical drivers of the atomic hydrogen-halo mass relation
• Visual and ultraviolet flux variability of the bright CP star $\theta$ Aur
• The Herschel Exploitation of Local Galaxy Andromeda (HELGA). VI. The distribution and properties of molecular cloud associations in M31
• Mixing matters
• Integrated-light analyses vs. colour-magnitude diagrams - II. Leo A, an extremely young dwarf in the Local Group
• Binary evolution along the Red Giant Branch with BINSTAR: The barium star perspective
• Observational properties of massive black hole binary progenitors
• Massive black hole assembly in nuclear star clusters
• Phase-resolved NuSTAR and Swift-XRT Observations of Magnetar 4U 0142+61
• Stellar laboratories. IX. New Se V, Sr IV - VII, Te VI, and I VI oscillator strengths and the Se, Sr, Te, and I abundances in the hot white dwarfs G191-B2B and RE 0503-289
• Evolution of the Thermodynamic Properties of Clusters of Galaxies out to Redshift of 1.8
• Spatially resolved hard X-ray polarization in solar flares: effects of Compton scattering and bremsstrahlung
• On the sdOB primary of the post common-envelope binary AA Doradus (LB 3459)
• The Araucaria Project. Accurate stellar parameters and distance to evolved eclipsing binary ASAS J180057-2333.8 in Sagittarius Arm
• Asteroseismology of massive stars with the TESS mission: the runaway Beta Cep pulsator PHL 346 = HN Aqr
• Star formation law in the EoR from [CII] and CIII] lines
• Multi-wavelength variability of the young solar analog iota Hor. X-ray cycle, star spots, flares, and UV emission
• Tracking the evolution of lithium in giants using asteroseismology: Super-Li-rich stars are almost exclusively young red-clump stars
• Two spotted and magnetic early B-type stars in the young open cluster NGC2264 discovered by MOST and ESPaDOnS
• Detection of Na in WASP-21b's lower and upper atmosphere
• Five young $\delta$ Scuti stars in the Pleiades seen with Kepler/K2
• The circumstellar matter of supernova 2014J and the core-degenerate scenario
• Higher metal abundances do not solve the solar problem
• Chemical Abundances for the Outer Halo Cluster Pal 4 from Co-added High-Resolution Spectroscopy
• RR Lyrae-based Distances for 39 Nearby Dwarf Galaxies Calibrated to Gaia eDR3
• Solar Flare Composition and Thermodynamics from RESIK X-ray Spectra
• Chemical Cartography. II. The Assembly History of the Galactic Stellar Halo Traced by Carbon-Enhanced Metal-Poor Stars
• Volatility of Sodium in Carbonaceous Chondrites at Temperatures Consistent with Low-Perihelia Asteroids
• Spatially resolved physical conditions of molecular gas and potential star formation tracers in M83, revealed by the Herschel SPIRE FTS
• The Gaia-ESO Survey: the N/O abundance ratio in the Milky Way
• Discovery and characterization of the exoplanets WASP-148b and c. A transiting system with two interacting giant planets
• Chemical Compositions of Field and Globular Cluster RR Lyrae Stars: I. NGC 3201
• Understanding the strong intervening OVI absorber at z${}_{abs}$ ~0.93 towards PG1206+459
• Probing the low-redshift star formation rate as a function of metallicity through the local environments of type II supernovae
• The HD 98800 quadruple pre-main sequence system. Towards full orbital characterisation using long-baseline infrared interferometry
• A peculiar Of star in the Local Group galaxy IC 1613
• Sixty Years of Element Abundance Measurements in Solar Energetic Particles
• Chemulator: Fast, accurate thermochemistry for dynamical models through emulation
• Primordial nucleosynthesis with varying fundamental constants: Solutions to the Lithium problem and the Deuterium discrepancy
• Global 3D Radiation Hydrodynamic Simulations of Proto-Jupiter's Convective Envelope
• The very low mass multiple system LHS\,1070 -- a testbed for model atmospheres for the lower end of the main sequence
• A new and homogeneous metallicity scale for Galactic classical Cepheids II. The abundance of iron and alpha elements
• Very deep spectroscopy of the bright Saturn Nebula NGC 7009 - II. Analysis of the rich optical recombination spectrum
• Stripped-Envelope Stars in Different Metallicity Environments I. Evolutionary Phases, Classification and Populations
• Information content of JWST-NIRSPEC transmission spectra of warm Neptunes
• Two long-period transiting exoplanets on eccentric orbits: NGTS-20 b (TOI-5152 b) and TOI-5153 b
• sMILES SSPs: A Library of Semi-Empirical MILES Stellar Population Models with Variable [$\alpha$/Fe] Abundances
• AT2018kzr: the merger of an oxygen-neon white dwarf and a neutron star or black hole
• Enriching inner discs and giant planets with heavy elements
• Galactic and Cosmic Type Ia SN rates: is it possible to impose constraints on SNIa progenitors?
• Water in Star and Planet Forming Regions
• SN 2018gjx reveals that some SNe Ibn are SNe IIb exploding in dense circumstellar material
• Supervised Machine Learning for Intercomparison of Model Grids of Brown Dwarfs: Application to GJ 570D and the Epsilon Indi B Binary System
• Dilution in elliptical galaxies: Implications for the relation between metallicity, stellar mass and star formation rate
• On the necessity of composition-dependent low-temperature opacity in metal-poor AGB stars
• Infrared Spectroscopy of Comet 73P/Schwassmann-Wachmann 3 using the Spitzer Space Telescope
• Infrared Spectroscopy of Symbiotic Stars. XII. The Neutron Star SyXB System 4U 1700+24 = V934 Herculis
• An ALMA view of CS and SiS around oxygen-rich AGB stars
• The EUV spectrum of the Sun: quiet and active Sun irradiances and chemical composition
• An HST/COS legacy survey of intervening SiIII absorption in the extended gaseous halos of low-redshift galaxies
• Single stars in the Hyades open cluster. Fiducial sequence for testing stellar and atmospheric models
• Study of galaxies in the Eridanus void. Sample and oxygen abundances
• The dust content of damped Lyman-alpha systems in the Sloan Digital Sky Survey
• First solar models with OPAS opacity tables
• The Chemical Abundances of Stars in the Halo (CASH) Project. III. A New Classification Scheme for Carbon-Enhanced Metal-poor Stars with S-process Element Enhancement
• KIC 9821622: An interesting lithium-rich giant in the Kepler field
• Spectroscopic survey of Kepler stars. II. FIES/NOT observations of A- and F-type stars
• CHEX-MATE: Robust reconstruction of temperature profiles in galaxy clusters with XMM-Newton
• Galaxies with grains: unraveling dust evolution and extinction curves with hydrodynamical simulations
• The X-ray light curve of the massive colliding wind Wolf-Rayet + O binary WR21a
• Asteroseismology of 19 low-luminosity red giant stars from Kepler
• Migration in the shearing sheet and estimates for young open cluster migration
• Surface-effect corrections for the solar model
• Element abundances in X-ray emitting plasmas in stars
• Lithium in CEMP-no stars: A new constraint on the lithium depletion mechanism in the early universe
• Multi-wavelength campaign on NGC7469 I. The rich 640 ks RGS spectrum
• Growing evidence that SNe Iax are not a one-parameter family: the case of PS1-12bwh
• SN 2012aa - a transient between Type Ibc core-collapse and superluminous supernovae
• WASP-92b, WASP-93b and WASP-118b: Three new transiting close-in giant planets
• The importance of preventive feedback: inference from observations of the stellar masses and metallicities of Milky Way dwarf galaxies
• Ammonia Abundance Derived from Juno MWR and VLA Observations of Jupiter
• Chemo-Dynamically Tagged Groups of CEMP Stars in the Halo of the Milky Way. I. Untangling the Origins of CEMP-$s$ and CEMP-no Stars
• Calibration of neutron star natal kick velocities to isolated pulsar observations
• The metal rich abundance pattern - spectroscopic properties and abundances for 107 main-sequence stars
• Exploring metallicity-dependent rates of Type Ia supernovae and their impact on galaxy formation
• Aluminium-26 from massive binary stars II. Rotating single stars up to core-collapse and their impact on the early Solar System
• Correlations of r-Process Elements in Very Metal-Poor Stars as Clues to their Nucleosynthesis Sites
• Neutron-Capture elements in planetary nebulae: first detections of near-Infrared [Te III] and [Br V] emission lines
• R-process-rich stellar streams in the Milky Way
• Probing core overshooting using subgiant asteroseismology: the case of KIC10273246
• Indications for very high metallicity and absence of methane for the eccentric exo-Saturn WASP-117b
• HST/STIS transmission spectrum of the ultra-hot Jupiter WASP-76 b confirms the presence of sodium in its atmosphere
• On the hydrostatic stratification of the solar tachocline
• On the (Lack of) Evolution of the Stellar Mass Function of Massive Galaxies from $z$=1.5 to 0.4
• Oxygen and zinc abundances in 417 Galactic bulge red giants
• Stellar ages and masses in the solar neighbourhood: Bayesian analysis using spectroscopy and Gaia DR1 parallaxes
• Spatially resolved X-ray study of supernova remnants that host magnetars: Implication of their fossil field origin
• The photospheric solar oxygen project: III. Investigation of the centre-to-limb variation of the 630nm [OI]-NiI blend
• Stellar Photospheric Abundances as a Probe of Disks and Planets
• Geoneutrinos in Large Direct Detection Experiments
• Chemistry of the High-Mass Protostellar Molecular Clump IRAS 16562-3959
• The Influence of Beta Decay Rates on r-Process Observables
• The R-Process Alliance: Chemo-Dynamically Tagged Groups II. An Extended Sample of Halo $r$-Process-Enhanced Stars
• Chemical abundances in the extremely Carbon and Xenon-rich halo planetary nebula H4-1
• Chemical abundances in Sgr A East: evidence for a Type Iax supernova remnant
• A deep X-ray view of the bare AGN Ark 120. I. Revealing the Soft X-ray Line Emission
• VINTERGATAN-GM: The cosmological imprints of early mergers on Milky-Way-mass galaxies
• Carbon and nitrogen abundances of individual stars in the Sculptor dwarf spheroidal galaxy
• Deep Learning Applied to the Asteroseismic Modeling of Stars with Coherent Oscillation Modes
• AstroSat and Chandra view of the high soft state of 4U 1630-47 (4U 1630-472): evidence of the disk wind and a rapidly spinning black hole
• Measuring the shock-heating rate in the winds of O stars using X-ray line spectra
• Ionizing stellar population in the disk of NGC 3310 $-$ I. The impact of a minor merger on galaxy evolution
• HD 24355 observed by the Kepler K2 mission: A rapidly oscillating Ap star pulsating in a distorted quadrupole mode
• SN 2020kyg and the rates of faint Iax Supernovae from ATLAS
• Near Infrared Spectroscopy of M Dwarfs. I. CO Molecule as an Abundance Indicator of Carbon
• Si K Edge Structure and Variability in Galactic X-Ray Binaries
• Chemical Compositions of Evolved Stars From Near-Infrared IGRINS High-Resolution Spectra. I. Abundances in Three Red Horizontal Branch Stars
• Asteroseismology of the young open cluster NGC 2516 I: Photometric and spectroscopic observations
• The Dual Nature of GHZ9: Coexisting Active Galactic Nuclei and Star Formation Activity in a Remote X-ray Source at z = 10.145
• KIC 4150611: a rare multi-eclipsing quintuple with a hybrid pulsator
• Small-scale structure in the interstellar medium: time-varying interstellar absorption towards κ Velorum
• Solar-to-supersolar sodium and oxygen absolute abundances for a "hot Saturn" orbiting a metal-rich star
• The Slow Demise of the Long-Lived SN 2005ip
• Local stellar formation history from the 40 pc white dwarf sample
• Self-consistent modelling of line-driven hot-star winds with Monte Carlo radiation hydrodynamics
• Synthetic observables for electron-capture supernovae and low-mass core collapse supernovae
• Kepler-167e as a Probe of the Formation Histories of Cold Giants with Inner Super-Earths
• The SAMI Galaxy Survey: the drivers of gas and stellar metallicity differences in galaxies
• Low-metallicity Young Clusters in the Outer Galaxy. II. Sh 2-208
• Young, Star-forming Galaxies and their local Counterparts: the Evolving Relationship of Mass-SFR-Metallicity since z ~ 2.1
• Chemical evolution of disc galaxies from cosmological simulations
• Constraining The Single-Degenerate Channel of Type Ia Supernovae With Stable Iron-Group Elements in SNR 3C 397
• Constraining Big Bang lithium production with recent solar neutrino data
• XMP gas-rich dwarfs in nearby voids: results of BTA spectroscopy
• New $\beta$ Cep pulsators discovered with K2 space photometry
• Perspectives on Intracluster Enrichment and the Stellar Initial Mass Function in Elliptical Galaxies
• Thermal Pressures in the Interstellar Medium of the Magellanic Clouds
• Helium enrichment in intermediate-age Magellanic Clouds clusters: towards an ubiquity of multiple stellar populations?
• The WAGGS project - II. The reliability of the calcium triplet as a metallicity indicator in integrated stellar light
• The effects of surface fossil magnetic fields on massive star evolution: IV. Grids of models at Solar, LMC, and SMC metallicities
• 3D non-LTE corrections for Li abundance and 6Li/7Li isotopic ratio in solar-type stars I. Application to HD 207129 and HD 95456
• The IGIMF and other IMFs in dSphs: the case of Sagittarius
• Elemental Abundances in M31: Alpha and Iron Element Abundances from Low-Resolution Resolved Stellar Spectroscopy in the Stellar Halo
• Discovery and Rapid Follow-up Observations of the Unusual Type II SN 2018ivc in NGC 1068
• [CII] halos in ALPINE galaxies: smoking-gun of galactic outflows?
• Galaxy counterparts of intervening high-z sub-DLAs/DLAs and MgII absorbers towards gamma-ray bursts
• The X-ray emission of Be+stripped star binaries
• Consistent Iron Abundances Derived from Neutral and Singly-Ionized Iron Lines in Ultraviolet and Optical Spectra of Six Warm Metal-Poor Stars
• Still at Odds with Conventional Galaxy Evolution: The Star Formation History of Ultra-Diffuse Galaxy Dragonfly 44
• The first nova eruption in a novalike variable: YZ Ret as seen in X-rays and gamma-rays
• Metals and dust in the neutral ISM: the Galaxy, Magellanic Clouds, and damped Lyman-α absorbers
• Subaru/HDS study of CH stars: elemental abundances for stellar neutron-capture process studies
• Convective overshoot mixing in stellar interior models
• Mitigating the mass dependence in the $\Delta \nu$ scaling relation of red-giant stars
• Atomic diffusion and turbulent mixing in solar-like stars: Impact on the fundamental properties of FG-type stars
• Galactic Chemical Evolution and the Oxygen Isotopic Composition of the Solar System
• HD 65949: Rosetta Stone or Red Herring
• Do high-spin high-mass X-ray binaries contribute to the population of merging binary black holes?
• Serendipitous discovery of the faint solar twin Inti 1
• Detailed Chemical Abundances of Four Stars in the Unusual Globular Cluster, Palomar 1
• A global study of the HII region M43 and its ionizing star (I. Stellar parameters and nebular empirical analysis)
• Spectroscopy on the $A^1\Pi \leftarrow X^1{\Sigma }^{+}$ Transition of Buffer-Gas Cooled AlCl
• Solar models in light of new high metallicity measurements from solar wind data
• On the structure and evolution of planets and their host stars $-$ effects of various heating mechanisms on the size of giant gas planets
• Chemical abundances of fast-rotating massive stars. I. Description of the methods and individual results
• Enrichment of Heavy Elements in the red giant S15-19 in the Sextans Dwarf Spheroidal Galaxy
• Chemical abundances in the protoplanetary disk LV2 (Orion): clues to the causes of the abundance anomaly in HII regions
• The MOSDEF Survey: First Measurement of Nebular Oxygen Abundance at $z>4$
• Can 1D radiative equilibrium models of faculae be used for calculating contamination of transmission spectra?
• NuSTAR view of the black hole wind in the galaxy merger IRAS F11119$+$3257
• Light Element Nucleosynthesis in a Molecular Cloud Interacting with a Supernova Remnant and the Origin of Beryllium-10 in the Protosolar Nebula
• Mass effect on the lithium abundance evolution of open clusters: Hyades, NGC 752, and M67
• Physical properties and transmission spectrum of the WASP-74 planetary system from multi-band photometry
• Stromlo Stellar Tracks: non-solar scaled abundances for massive stars
• From the CMD of Omega Centauri and (super-)AGB stellar models to a Galactic plane passage gas purging chemical evolution scenario
• From Carbon to Cobalt: Chemical compositions and ages of $z\sim 0.7$ quiescent galaxies
• X-Ray Absorption Analysis of MCG-6-30-15: Discerning Three Kinematic Systems
• Stellar laboratories. VIII. New Zr IV - VII, Xe IV - V, and Xe VII oscillator strengths and the Al, Zr, and Xe abundances in the hot white dwarfs G191-B2B and RE0503-289
• The magnetic field and spectral variability of the He-weak star HR 2949
• Age Determination of Galaxy Merger Remnant Stars using Asteroseismology
• Search for cold and hot gas in the ram pressure stripped Virgo dwarf galaxy IC3418
• Atomic data for neutron-capture elements II. Photoionization and recombination properties of low-charge krypton ions
• Mass-Metallicity Relation from Cosmological Hydrodynamical Simulations and X-ray Observations of Galaxy Groups and Clusters
• Hu1-2: a metal-poor bipolar planetary nebula with fast collimated outflows
• Identification of a Group III CEMP-no Star in the Dwarf Spheroidal Galaxy Canes Venatici I
• Evidence for Radiation Pressure Compression in the X-ray Narrow Line Region of Seyfert galaxies
• In-situ star formation in accretion disk and explanation for correlation between black hole mass and metallicity in AGNs
• Constraining the parameter space for the Solar Nebula
• Shadows, gaps, and ring-like structures in protoplanetary disks
• sMILES: A Library of Semi-Empirical MILES Stellar Spectra with Variable [$\alpha$/Fe] Abundances
• Joint XMM-Newton and Chandra Observations of the NGC 1407/1400 Complex: a Tail of an Early-Type Galaxy and a Tale of a Nearby Merging Group
• Inverse-Compton scattering in the resolved jet of the high-redshift quasar PKS J1421-0643
• On the internal pollution mechanisms in the globular cluster NGC 6121 (M4): heavy-element abundances and AGB models
• The Age of the Old Metal-Poor Globular Cluster NGC6397 Using WFC3/IR Photometry
• Solar Models with Revised Abundance
• Phosphorus Abundances in FGK Stars
• Abundance anomalies in pre-main-sequence stars: Stellar evolution models with mass loss
• Hunting the Parent of the Orphan Stream II: The First High-Resolution Spectroscopic Study
• Heavy metals in a light white dwarf: Abundances of the metal-rich, extremely low-mass GALEX J1717+6757
• Chemical Compositions of Field and Globular Cluster RR~Lyrae Stars: II. omega Centauri
• Solar Flare Ribbon Fronts I: Constraining flare energy deposition with IRIS spectroscopy
• The Galactic Chemical Evolution of phosphorus observed with IGRINS
• Partial mixing and the formation of 13C pockets in AGB stars: effects on the s-process elements
• Evolution and nucleosynthesis of helium-rich asymptotic giant branch models
• X-ray Spectroscopy of the gamma-ray Brightest Nova V906 Car (ASASSN-18fv)
• The magnetic field of the double-lined spectroscopic binary system HD 5550
• The puzzle of metallicity and multiple stellar populations in the Globular Clusters in Fornax
• Constraining Non-Standard Interactions of the Neutrino with Borexino
• The Solar Flare Iron Abundance
• Probing the mid-layer structure of red giants I. Mixed-mode coupling factor as a seismic diagnosis
• Chemo-kinematic ages of eccentric-planet-hosting M dwarf stars
• The Origin of the Dust Extinction Curve in Milky Way-like Galaxies
• The First Extensive Spectroscopic Study of Young Stars in the North America and Pelican Nebulae Region
• The Faint Host Galaxies of C IV Absorbers at z > 5
• Chemical pre-processing of cluster galaxies over the past 10 billion years in the IllustrisTNG simulations
• The Herschel Virgo Cluster Survey. XVIII. Star-forming dwarf galaxies in a cluster environment
• Theoretical uncertainties on the radius of low- and very-low mass stars
• The Mantis Network II: Examining the 3D high-resolution observable properties of the UHJs WASP-121b and WASP-189b through GCM modelling
• Diversity of Abundance Patterns of Light Neutron-capture Elements in Very-metal-poor Stars
• The impact of (n,$\gamma$) reaction rate uncertainties of unstable isotopes on the i-process nucleosynthesis of the elements from Ba to W
• Local associations and the barium puzzle
• Metal abundances in hot white dwarfs with signatures of a superionized wind
• Chandra Observations of SNR RCW 103
• The synthesis of Ti44 and Ni56 in massive stars
• Dynamically Tagged Groups of Metal-Poor Stars II. The Radial Velocity Experiment Data Release 6
• Survey of Extremely High-velocity Outflows in Sloan Digital Sky Survey Quasars
• Chandra High Energy Transmission Gratings Spectra of V3890 Sgr
• A Fresh Look at AGB stars in Galactic Open Clusters with Gaia: Impact on Stellar Models and the Initial-Final Mass Relation
• Anatomy of a z=6 Lyman-α emitter down to parsec scales: extreme UV slopes, metal-poor regions and possibly leaking star clusters
• A solar-type star polluted by calcium-rich supernova ejecta inside the supernova remnant RCW 86
• The impact of very massive stars on the chemical evolution of extremely metal-poor galaxies
• Is helium the key parameter in the extended color spread of the first generation stars in M3?
• Revealing the Ionization Properties of the Magellanic Stream using Optical Emission
• Evolution of lithium abundance in the Sun and solar twins
• The GAPS programme at TNG XXX. Atmospheric Rossiter-McLaughlin effect and atmospheric dynamics of KELT-20b
• Spatially resolved spectroscopy and chemical history of star-forming galaxies in the Hercules cluster: the effects of the environment
• The molecular gas mass of M33
• An exquisitely deep view of quenching galaxies through the gravitational lens: Stellar population, morphology, and ionized gas
• Wind inhibition by X-ray irradiation in HMXBs: the influence of clumping and the final X-ray luminosity
• On Neutron Star Mergers as the Source of r-process Enhanced Metal Poor Stars in the Milky Way
• CASSOWARY 20: a Wide Separation Einstein Cross Identified with the X-shooter Spectrograph
• A possible cyclotron resonance scattering feature near 0.7 keV in X1822-371
• On the age of Galactic bulge microlensed dwarf and subgiant stars
• Bayesian calibration of the mixing length parameter ${\alpha }_{ML}$ and of the helium-to-metal enrichment ratio $\Delta Y/\Delta Z$ with open clusters: the Hyades test-bed
• IC 4663: The first unambiguous [WN] Wolf-Rayet central star of a planetary nebula
• The nature of damped HI absorbers probed by cosmological simulations: satellite accretion and outflows
• Angular momentum transport by magnetic fields in main sequence stars with Gamma Doradus pulsators
• Spectroscopic Studies of Extremely Metal-Poor Stars with the Subaru High Dispersion Spectrograph. V. The Zn-Enhanced Metal-Poor Star BS 16920-017
• On a new and homogeneous metallicity scale for Galactic classical Cepheids - I. Physical parameters
• Very Low-Mass Stellar and Substellar Companions to Solar-Like Stars from MARVELS I: A Low Mass Ratio Stellar Companion to TYC 4110-01037-1 in a 79-day Orbit
• The kinetic temperature in a damped Lyman-alpha absorption system in Q2206-199 - an example of the warm neutral medium
• NGC 741 - Mergers and AGN feedback on galaxy group scale
• Physical properties of extreme emission-line galaxies at $z\sim 4-9$ from the JWST CEERS survey
• Detection of extragalactic CF+ toward PKS1830-211 -- Chemical differentiation in the absorbing gas
• The Interplay of Kinetic and Radiative Feedback in Galaxy Clusters
• The origin of the relation between metallicity and size in star-forming galaxies
• Observational identification of a sample of likely recent Common-Envelope Events
• The host-galaxy response to the afterglow of GRB 100901A
• DEVILS: Cosmic evolution of SED-derived metallicities and their connection to star-formation histories
• Investigating the Potential Dilution of the Metal Content of Hot Gas in Early-Type Galaxies by Accreted Cold Gas
• Chemical Abundances and Dust in the Halo Planetary Nebula K648 in M15: Its Origin and Evolution based on an Analysis of Multiwavelength Data
• Orbital parameters, chemical composition, and magnetic field of the Ap binary HD 98088
• Neutral chlorine and molecular hydrogen at high redshift
• Nitrogen oxide in protostellar envelopes and shocks: the ASAI survey
• Chemical abundances in the outskirts of nearby galaxy groups measured with joint Suzaku and Chandra observations
• X-ray properties of early-type stars in the Tarantula Nebula from T-ReX
• A bound on the 12C/13C ratio in near-pristine gas with ESPRESSO
• Orbital and spectral characterization of the benchmark T-type brown dwarf HD 19467B
• Peculiar double-periodic pulsation in RR Lyrae stars of the OGLE collection. I. Long-period stars with dominant radial fundamental mode
• Low luminosity Type II supernovae III. SN 2018hwm, a faint event with an unusually long plateau
• Stellar laboratories. VII. New Kr IV - VII oscillator strengths and an improved spectral analysis of the hot, hydrogen-deficient DO-type white dwarf RE0503-289
• X-ray analysis of JWST's first galaxy cluster lens SMACS J0723.3-7327
• Modelling the chemical evolution of the Galaxy halo
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• Forbidden line diagnostics of photoevaporative disc winds
• SN 2022ann: A type Icn supernova from a dwarf galaxy that reveals helium in its circumstellar environment
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• Exploring Chemical Homogeneity in Dwarf Galaxies: A VLT-MUSE study of JKB 18
• Axion global fits with Peccei-Quinn symmetry breaking before inflation using GAMBIT
• High resolution spectroscopy of the extended narrow-line region of IC 5063 and NGC 7212
• Clouds form on the hot Saturn JWST ERO target WASP-96b
• Machine learning detects multiplicity of the first stars in stellar archaeology data
• Unresolved versus resolved: testing the validity of young simple stellar population models with VLT/MUSE observations of NGC 3603
• Observational signatures of past mass-exchange episodes in massive binaries: The case of HD 149 404
• Magnetic and Rotational Evolution of $\rho$ CrB from Asteroseismology with TESS
• A NLTE analysis of the hot subdwarf O star Bd+28 4211. I. The UV spectrum
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• Tango of celestial dancers: A sample of detached eclipsing binary systems containing g-mode pulsating components. A case study of KIC9850387
• Characterizing the companion AGBs using surface chemical composition of barium stars
• Asteroseismic modelling of solar-type stars: A deeper look at the treatment of initial helium abundance
• Clumping and X-Rays in cooler B supergiant stars
• Gemini Planet Imager Spectroscopy of the Dusty Substellar Companion HD 206893 B
• Targeting Bright Metal-poor Stars in the Disk and Halo Systems of the Galaxy
• Kron 3: a fourth intermediate age cluster in the SMC with evidence of multiple populations
• Absolute dimensions of detached eclipsing binaries. III. The metallic-lined system YZ Cassiopeiae
• Dust masses and grain size distributions of a sample of Galactic pulsar wind nebulae
• X-ray spectroscopy of the z=6.4 quasar J1148+5251
• Silicate clouds and a circumplanetary disk in the YSES-1 exoplanet system
• Accretion in the detached post-common-envelope binary LTT 560
• Lithium in stellar atmospheres: observations and theory
• Oxygen and Neon Abundances of B-Type Stars in Comparison with the Sun
• Characterization of the Praesepe Star Cluster by Photometry and Proper Motions with 2MASS, PPMXL, and Pan-STARRS
• Reflection geometries in absorbed and unabsorbed AGN
• On the origin of central abundance drops in the intracluster medium of galaxy groups and clusters
• Intermediate-mass asymptotic giant branch stars and sources of ${}^{26}$Al, ${}^{60}$Fe, ${}^{107}$Pd, and ${}^{182}$Hf in the solar system
• Determining the metallicity of the solar envelope using seismic inversion techniques
• The impact of natal kicks on galactic r-process enrichment by neutron star mergers
• GARROTXA Cosmological Simulations of Milky Way-sized Galaxies: General Properties, Hot Gas Distribution, and Missing Baryons
• Down-the-barrel and transverse observations of the Large Magellanic Cloud: evidence for a symmetrical galactic wind on the near and far sides of the galaxy
• Seismic modelling of early B-type pulsators observed by BRITE: I. $\theta$ Ophiuchi
• Photoionization Emission Models for the Cyg X-3 X-ray Spectrum
• Constraining FeLoBAL outflows from absorption line variability
• The Abundance of Helium in the Source Plasma of Solar Energetic Particles
• Forming planets around stars with non-solar elemental composition
• Pulsational instability in B-type supergiant stars
• Magnetic geometry and surface differential rotation of the bright Am star Alhena A
• Overshooting calibration and age determination from evolved binary system
• Evidence of First Stars-enriched Gas in High-redshift Absorbers
• Catalog of Chromium, Cobalt, and Nickel Abundances in Globular Clusters and Dwarf Galaxies
• The eROSITA view of the Abell 3391/95 field: The Northern Clump. The largest infalling structure in the longest known gas filament observed with eROSITA, XMM-Newton, and Chandra
• The CARMENES search for exoplanets around M dwarfs: Not-so-fine hyperfine-split vanadium lines in cool star spectra
• The effects of near-core convective shells on the gravity modes of the subdwarf B pulsator KIC 10553698A
• Ionization structure and chemical abundances of the Wolf-Rayet nebula NGC6888 with integral field spectroscopy
• Chemical analysis of early-type stars with planets
• The Sun and stars as the primary energy input in planetary atmospheres
• Exploring the origins of a new, apparently metal-free gas cloud at z = 4.4
• How does accretion of planet-forming disks influence stellar abundances?
• High resolution modeling of [CII], [CI], [OIII] and CO line emission from the ISM and CGM of a star forming galaxy at z ~ 6.5
• Modeling H$\alpha$ and He 10830 transmission spectrum of WASP-52b
• Measuring the atomic composition of planetary building blocks
• The true stellar parameters of the Kepler target list
• Effect of electromagnetic dipole dark matter on energy transport in the solar interior
• Stellar laboratories II. New Zn IV and Zn V oscillator strengths and their validation in the hot white dwarfs G191-B2B and RE0503-289
• Characterizing circumgalactic gas around massive ellipticals at z~0.4 III. The galactic environment of a chemically-pristine Lyman limit absorber
• Imprint of planet formation in the deep interior of the Sun
• Evidence of a signature of planet formation processes from solar neutrino fluxes
• Effective Temperatures of Low-Mass Stars from High-Resolution H-band Spectroscopy
• Testing the cores of first ascent red-giant stars using the period spacing of g modes
• Empirical Constraints on the Nucleosynthesis of Nitrogen
• Sphinx measurements of the 2009 solar minimum x-ray emission
• Apsidal motion in the massive binary HD152218
• Ground-state ammonia and water in absorption towards Sgr B2
• The $\beta$ Cep/SPB star 12 Lacertae: extended mode identification and complex seismic modelling
• The 21cm "Outer Arm" and the Outer-Galaxy High-Velocity Clouds: Connected by Kinematics, Metallicity, and Distance
• Laboratory oscillator strengths of Sc I in the near-infrared region for astrophysical applications
• Semi-empirical model atmospheres for the chromosphere of the sunspot penumbra and umbral flashes
• The nitrogen carrier in protoplanetary disks
• Thorough characterisation of the 16 Cygni system Part I: Forward seismic modelling with WhoSGlAd
• Bolometric corrections of stellar oscillation amplitudes as observed by the Kepler, CoRoT, and TESS missions
• Radiative transfer of ionizing radiation through gas and dust: stellar source case
• XMM-Newton and Suzaku X-ray Shadowing Measurements of the Solar Wind Charge Exchange, Local Bubble, and Galactic Halo Emission
• Incorporating Astrochemistry into Molecular Line Modelling via Emulation
• Seismic modeling of a very young SPB star -- KIC8264293
• Towards a photometric metallicity scale for open clusters
• Mono-enriched stars and Galactic chemical evolution -- Possible biases in observations and theory
• Hydrodynamical modeling of the light curves of core collapse supernovae with HYPERION. I. The mass range 13-25 Msun, the metallicities -3<=[Fe/H]<=0 and the case of SN1999em
• HORuS transmission spectroscopy of 55 Cnc e
• The Mg II 2797, 2803 emission in low-metallicity star-forming galaxies from the SDSS
• The MgI line: a new probe of the atmospheres of evaporating exoplanets
• Nonthermal phenomena in the center of Abell 1775: An 800 kpc head-tail, revived fossil plasma and slingshot radio halo
• Spectral Shapes of the Lya Emission from Galaxies. II. the influence of stellar properties and nebular conditions on the emergent Lya profiles
• ATHOS: On-the-fly stellar parameter determination of FGK stars based on flux ratios from optical spectra
• X-Ray Absorption Analysis of NGC3516: Appearance of Fast Components with Increased Source Flux
• The GAPS Programme at TNG -- XXV. Stellar atmospheric parameters and chemical composition through GIARPS optical and near-infrared spectra
• Birth of a Be star: an APOGEE search for Be stars forming through binary mass transfer
• Sensitivity to neutrinos from the solar CNO cycle in Borexino
• On the effects of the Initial Mass Function on Galactic chemical enrichment
• The spectroscopic properties of the nebulae around seven Galactic and LMC Wolf-Rayet stars
• The multi-wavelength view of shocks in the fastest nova V1674 Her
• The Atacama Cosmology Telescope: High-Resolution Sunyaev-Zel'dovich Array Observations of ACT SZE-selected Clusters from the Equatorial Strip
• First detection of bromine and antimony in hot stars
• Nuclear processes in Astrophysics: Recent progress
• Dust evolution with MUPPI in cosmological volumes
• The IACOB project X. Large-scale quantitative spectroscopic analysis of Galactic luminous blue stars
• How different are the Liège and Hamburg atlases of the solar spectrum?
• On the redshift evolution of the baryon and gas fraction in simulated groups and clusters of galaxies
• Interstellar Silicon Depletion and the Ultraviolet Extinction
• Evaporation Barrier for Dark Matter in Celestial Bodies
• Evolution of the reservoirs of volatiles in the protosolar nebula
• 12C/13C isotopic ratios in red-giant stars of the open cluster NGC 6791
• Rapidly rotating Population III stellar models as a source of primary nitrogen
• Magnetic braking with MESA evolutionary models in the single star and LMXB regimes
• X-shooter spectroscopy of young stellar objects in Lupus: Lithium, iron, and barium elemental abundances
• The Ionizing Spectra of Extremely Metal-Poor O Stars: Constraints from the Only HII Region in Leo P
• Accelerated Fitting of Stellar Spectra
• An environmental analysis of the fast transient AT2018cow and implications for its progenitor and late-time brightness
• The impact of spatial fluctuations in the ultra-violet background on intergalactic carbon and silicon
• Low-metallicity Young Clusters in the Outer Galaxy I. Sh 2-207
• Far-UV spectroscopy of the planet-hosting star WASP-13: high-energy irradiance, distance, age, planetary mass-loss rate, and circumstellar environment
• Explodability criteria for the neutrino-driven supernova mechanism
• Searching for dark energy with the Sun
• Chemical Abundances of Planetary Nebulae in the Substructures of M31
• Probing Wolf-Rayet Winds: Chandra/HETG X-Ray Spectra of WR 6
• Solar Neutrino Spectroscopy
• Extended X-ray study of M49: the frontier of the Virgo Cluster
• The relationship between age, metallicity, and abundances for disk stars in a simulated Milky Way galaxy
• Unexplored outflows in nearby low luminosity AGNs: the case of NGC 1052
• Burned to ashes: How the thermal decomposition of refractory organics in the inner protoplanetary disc impacts the gas-phase C/O ratio
• The molecular gas properties in local Seyfert 2 galaxies
• ALMA Observations of Molecular Complexity in the Large Magellanic Cloud: The N105 Star-Forming Region
• X-ray to NIR emission from AA Tauri during the dim state - Occultation of the inner disk and gas-to-dust ratio of the absorber
• The Slowly Varying Corona: I --- Daily Differential Emission Measure Distributions Derived from EVE Spectra
• Variations in solar wind fractionation as seen by ACE/SWICS over a solar cycle and the implications for Genesis Mission results
• Using the Multi-Object Adaptive Optics demonstrator RAVEN to observe metal-poor stars in and towards the Galactic Centre
• A ghostly damped Ly$\alpha$ system revealed by metal absorption lines
• Kinematics of Extremely Metal-poor Galaxies: Evidence for Stellar Feedback
• Cosmological evolution of the Nitrogen abundance
• Metal-Rich SX Phe stars in the Kepler Field
• NLTE analysis of copper lines in different stellar populations
• CNO Neutrino Grand Prix: The race to solve the solar metallicity problem
• The Solar Flare Chlorine Abundance from RESIK X-ray Spectra
• The First Metallicity Study of M83 using the integrated UV light of Star Clusters
• The Enigmatic (Almost) Dark Galaxy Coma P: Distance Measurement and Stellar Populations from HST Imaging
• Abundances in the Herbig Ae star HD 101412: Abundance anomalies; Lambda Boo-Vega characteristics?
• A new procedure for defining a homogenous line-list for solar-type stars
• A metallicity study of F, G, K and M dwarfs in the Coma Berenices open cluster from the APOGEE survey
• XMP gas-rich dwarfs in Nearby Voids: results of SALT spectroscopy
• Constraints on Self Interacting Dark Matter from IceCube Results
• The GALAH Survey: Temporal Chemical Enrichment of the Galactic Disk
• Exploring the chemical link between local ellipticals and their high-redshift progenitors
• Relic neutrinos at accelerator experiments
• Discovery of a 6.4 h black hole binary in NGC 4490
• On the nature of WO stars: a quantitative analysis of the WO3 star DR1 in IC 1613
• SCExAO/MEC and CHARIS Discovery of a Low Mass, 6 AU-Separation Companion to HIP 109427 using Stochastic Speckle Discrimination and High-Contrast Spectroscopy
• A Dusty Locale: Evolution of Galactic Dust Populations from Milky Way to Dwarf-Mass Galaxies
• Super-adiabatic Temperature Gradient at Jupiter's Equatorial Zone and Implications for the Water Abundance
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• Effective temperatures of red supergiants estimated from line-depth ratios of iron lines in the YJ bands, 0.97--1.32 micron
• The Hubble PanCET Program: A Metal-rich Atmosphere for the Inflated Hot Jupiter HAT-P-41b
• Supernova 2018cuf: A Type IIP supernova with a slow fall from plateau
• High Dispersion Spectroscopy of the Superflare Star KIC6934317
• High-resolution emission spectroscopy retrievals of MASCARA-1b with CRIRES+: Strong detections of CO, H${}_2$O and Fe emission lines and a C$/$O consistent with solar
• The energy distribution of the first supernovae
• X-ray Absorption of High Redshift Quasars
• On the impact of the structural surface effect on global stellar properties and asteroseismic analyses
• Supernova SN 2020faa -- an iPTF14hls look-alike?
• Oxygen depletion in giant planets with different formation histories
• Criteria for Dynamical Timescale Mass Transfer of Metal-poor Intermediate-mass Stars
• WIYN Open Cluster Study LXII: Comparison of Isochrone Systems using Deep Multi-Band Photometry of M35
• Star Formation Timescales of the Halo Populations from Asteroseismology and Chemical Abundances
• The atomic-to-molecular hydrogen transition in the TNG50 simulation: Using realistic UV fields to create spatially resolved HI maps
• On the use of the index N2 to derive the metallicity in metal-poor galaxie
• Three long period transiting giant planets from TESS
• 3D1D hydro-nucleosynthesis simulations. I. Advective-reactive post-processing method and its application to H ingestion into He-shell flash convection in rapidly accreting white dwarfs
• Directly comparing coronal and solar wind elemental fractionation
• Linking the Sun to the Heliosphere Using Composition Data and Modelling. A Test Case with a Coronal Jet
• Co-spatial Long-slit UV/Optical Spectra of Ten Galactic Planetary Nebulae with HST/STIS I. Description of the Observations, Global Emission-line Measurements, and CNO Abundances
• The Great Flare of 2021 November 19 on AD Leo. Simultaneous XMM-Newton and TESS observations
• Neutrino Constraints on Inelastic Dark Matter after CDMS II
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• Chlorine-bearing molecules in molecular absorbers at intermediate redshifts
• An Updated Formalism For Line-Driven Radiative Acceleration and Implications for Stellar Mass Loss
• IR SED and Dust Masses of Sub-solar Metallicity Galaxies at z~2.3
• The chemical composition of $\alpha$ Cen AB revisited
• Exoplanetary Monte Carlo Radiative Transfer with Correlated-k I. Benchmarking Transit and Emission Observables
• Hierarchically modelling Kepler dwarfs and subgiants to improve inference of stellar properties with asteroseismology
• Dark Molecular Gas in Simulations of z~0 Disc Galaxies
• The 2175 Å extinction feature in the optical afterglow spectrum of GRB 180325A at z=2.25
• Evidence of a Clear Atmosphere for WASP-62b: the Only Known Transiting Gas Giant in the JWST Continuous Viewing Zone
• Theoretical oscillation frequencies for solar-type dwarfs from stellar models with $⟨3\mathrm{D}⟩$-atmospheres
• Early metal enrichment of gas-rich galaxies at z~5
• Moist adiabats with multiple condensing species: A new theory with application to giant planet atmospheres
• Searching for Dust around Hyper Metal-Poor Stars
• LSQ13ddu: A rapidly-evolving stripped-envelope supernova with early circumstellar interaction signatures
• Optical/near-infrared observations of the Fried Egg Nebula: Multiple shell ejections on a 100 yr timescale from a massive yellow hypergiant
• Chemical enrichment of stars due to accretion from ISM during the Galaxy's assembly
• On the contribution of the X-ray source to the extended nebular HeII emission in IZw18
• Detailed Iron-Peak Element Abundances in Three Very Metal-Poor Stars
• To Be or not to Be: the role of rotation in modeling Galactic Be X-ray Binaries
• Chemical abundances in the nuclear region of nearby galaxies from the Palomar Survey
• Modeling overcontact binaries, I. The effect of tidal deformation
• The effect of mass loss in models of red supergiants in the Small Magellanic Cloud
• Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
• Observational evidence of third dredge-up occurrence in S-type stars with initial masses around 1 Msun
• The nature of the 2014-2015 dim state of RW Aur revealed by X-ray, optical, and NIR observations
• High Resolution Optical Spectroscopy of the F Supergiant Proto-Planetary Nebula V887 Her=IRAS 18095+2704
• On Graphene in the Interstellar Medium
• The Mean Absorption Line Spectra of a Selection of Luminous z~6 Lyman Break Galaxies
• Looking for imprints of the first stellar generations in metal-poor bulge field stars
• Rotational spectra of vibrationally excited AlO and TiO in oxygen rich stars
• Searches for HCl and HF in comets 103P/Hartley 2 and C/2009 P1 (Garradd) with the Herschel space observatory
• The GALAH survey: Chemical homogeneity of the Orion complex
• On the use of Sulphur as a tracer for abundances in galaxies
• Energy function, formation rate and low-metallicity environment of fast radio bursts
• Resolved molecular line observations reveal an inherited molecular layer in the young disk around TMC1A
• Exploring the Milky Way Circumgalactic Medium in a Cosmological Context with a Semi-Analytic Model
• Synergising semi-analytical models and hydrodynamical simulations to interpret JWST data from the first billion years
• Modelling the chemical enrichment of Population III supernovae: The origin of the metals in near-pristine gas clouds
• BOWIE-ALIGN: JWST reveals hints of planetesimal accretion and complex sulphur chemistry in the atmosphere of the misaligned hot Jupiter WASP-15b
• Fundamental properties of nearby stars and the consequences on DeltaY/DeltaZ
• NuSTAR view of Swift/BAT AGN: The $R$-$\Gamma$ correlation
• Probing Red Supergiant dynamics through photo-center displacements measured by Gaia
• Astrophysical Sources of Statistical Uncertainty in Precision Radial Velocities and Their Approximations
• The effect of the centrifugal acceleration on period spacings of gravito-inertial modes in intermediate-mass stars
• On the Fe abundance peak formation in cool-core clusters of galaxies: hints from cluster WARPJ1415.1+3612 at z=1.03
• CLEAR: Survey Overview, Data Analysis and Products
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• Pulsational instability of pre-main sequence models from accreting protostars. I. Constraining the input physics for accretion with spectroscopic parameters and stellar pulsations
• A Bright Short Period M-M Eclipsing Binary from the KELT Survey: Magnetic Activity and the Mass-Radius Relationship for M-dwarfs
• The afterglow and host galaxy of GRB 090205: evidence for a Ly-alpha emitter at z=4.65
• Magnetic Doppler imaging of the chemically peculiar star HD 125248
• Calibrating the updated overshoot mixing model on eclipsing binary stars: HY Vir, YZ Cas, X2 Hya & VV Crv
• The HST large programme on $\omega$ Centauri -- V. Exploring the Ultracool Dwarf Population with Stellar Atmosphere and Evolutionary Modelling
• Evidence for a [WR] or WEL-type binary nucleus in the bipolar planetary nebula Vy 1-2
• The impact of multi-fluid effects in the solar chromosphere on the ponderomotive force under LTE and NEQ ionization conditions
• The R-Process Alliance: Discovery of a low-alpha, r-Process-Enhanced Metal-Poor Star in the Galactic Halo
• Si iv Column Densities Predicted from Non-Equilibrium Ionization Simulations of Turbulent Mixing Layers and High-Velocity Clouds
• Measuring Chemical Abundances with Infrared Nebular Lines: HII-Chi-mistry-IR
• A Lyman limit system associated with galactic winds
• An empirical prediction for stellar metallicity distributions in nearby galaxies
• Cold gas in the early Universe. Survey for neutral atomic-carbon in GRB host galaxies at 1 < z < 6 from optical afterglow spectroscopy
• Disruption of a planet spiralling into its host star
• Stellar Evolution in Real Time: Models Consistent with Direct Observation of Thermal Pulse in T Ursae Minoris
• Milky Way archaeology using RR Lyrae and type II Cepheids II. High velocity RR Lyrae stars, and mass of the Milky Way
• A chemo-dynamical link between the Gjöll stream and NGC 3201
• Seeding the second star -- II. CEMP star formation enriched from faint supernovae
• Grain Destruction in a Supernova Remnant Shock Wave
• The Effect of Bi-conical Outflows on Ly$\alpha$ Escape From Green Peas
• Extreme r-process enhanced stars at high metallicity in Fornax
• RESIK Solar X-ray flare element abundances on a non-isothermal assumption
• KIC 10736223: An Algol-type eclipsing binary just undergone the rapid mass-transfer stage
• Tol 2240-384 - a new low-metallicity AGN candidate
• On Stellar Evolution In A Neutrino Hertzsprung-Russell Diagram
• The impact of two massive early accretion events in a Milky Way-like galaxy: repercussions for the buildup of the stellar disc and halo
• 2D condensation model for the inner Solar Nebula: an enstatite-rich environment
• The SRG/eROSITA All-Sky Survey: SRG/eROSITA cross-calibration with Chandra and XMM-Newton using galaxy cluster gas temperatures
• Suzaku Observations of the Outskirts of the Galaxy Cluster Abell 3395 including a Filament toward Abell 3391
• Constraints on the Distance Moduli, Helium and Metal Abundances, and Ages of Globular Clusters From Their RR Lyrae and Non-Variable Horizontal-Branch Stars. III. M55 and NGC 6362
• Trans-iron Ge, As, Se, and heavier elements in the dwarf metal-poor stars, HD~19445, HD~84937, HD~94028, HD~140283, and HD~160617
• Applications of the $k$-$\omega$ model in stellar evolutionary models
• The stellar beta-decay rate of 134Cs and its impact on the Barium nucleosynthesis in the s process
• Absorption and emission features of ${}^7$Be{\sc II} in the outburst spectra of V838 Her (Nova Her 1991)
• The recondite intricacies of Zeeman Doppler mapping
• Verifying reddening and extinction for Gaia DR1 TGAS giants
• The R-Process Alliance: Fifth Data Release from the Search for R-Process-Enhanced Metal-poor Stars in the Galactic Halo with the GTC
• Trends in Nuclear Astrophysics
• The effects of surface fossil magnetic fields on massive star evolution: III. The case of $\tau$ Sco
• Grid-based estimates of stellar ages in binary systems. SCEPtER: Stellar CharactEristics Pisa Estimation gRid
• Surprises in the simultaneous X-ray and optical monitoring of pi Aqr
• Carbon Abundances in Starburst Galaxies of the Local Universe
• Flare activity and photospheric analysis of Proxima Centauri
• The XMM Cluster Survey: new evidence for the 3.5 keV feature in clusters is inconsistent with a dark matter origin
• More insights into bar quenching. Multi-wavelength analysis of four barred galaxies
• Clues on the rejuvenation of the S0 galaxy NGC 404 from the chemical abundance of its outer disk
• LAMOST J2217+2104: a new member of carbon-enhanced extremely metal-poor stars with excesses of Mg and Si
• Cosmic Galaxy-IGM HI Relation at $z\sim 2-3$ Probed in the COSMOS/UltraVISTA $1.6$ deg${}^2$ Field
• A search for the afterglows, kilonovae, and host galaxies of two short GRBs: GRB 211106A and GRB 211227A
• Galactic restrictions on iron production by various Types of supernovae
• Equilibrium Star Formation In A Constant Q Disk: Model Optimisation and Initial Tests
• Heavy-metal enrichment of intermediate He-sdOB stars: the pulsators Feige 46 and LS IV -14 116 revisited
• Gaia18aen: First symbiotic star discovered by Gaia
• The Most Metal-poor Stars in the Inner Bulge
• Surface correction of main sequence solar-like oscillators with the $Kepler$ LEGACY sample
• CHEX-MATE: Characterization of the intra-cluster medium temperature distribution
• ASASSN-14dq: A fast-declining type II-P Supernova in a low-luminosity host galaxy
• NGC 6705 a young $\alpha$-enhanced Open Cluster from OCCASO data
• Connecting turbulent velocities and magnetic fields in galaxy cluster simulations with active galactic nuclei jets
• Spectroscopic study of two new super Li rich red clump K giants
• Asteroseismic modelling of the subgiant μ Herculis using SONG data: lifting the degeneracy between age and model input parameters
• A disturbing FABLE of mergers, feedback, turbulence, and mass biases in simulated galaxy clusters
• MgII Absorption at 2 < z < 6 with Magellan / FIRE. II: A Longitudinal Study of HI, Metals, and Ionization in Galactic Haloes
• Masses, Oxygen and Carbon abundances in CHEPS dwarf stars
• The Evolution and Star Formation History of M33
• The metallicity distribution of HI systems in the EAGLE cosmological simulation
• LSQ13fn: A type II-Plateau supernova with a possibly low metallicity progenitor that breaks the standardised candle relation
• Discovery of the first tau Sco analogues: HD 66665 and HD 63425
• Multidimensional realistic modelling of Cepheid-like variables-II: Analysis of a Cepheid model
• First determination of s-process element abundances in pre-main sequence clusters: Y, Zr, La, and Ce in IC 2391, the Argus association and IC 2602
• Modelling ion populations in astrophysical plasmas: carbon in the solar transition region
• On the impact origin of Phobos and Deimos III: resulting composition from different impactors
• Discovery of technetium- and niobium-rich S stars: the case for bitrinsic stars
• Incidence of HI 21-cm absorption in strong FeII systems at $0.5<z<1.5$
• Aliphatic hydrocarbon content of the interstellar dust
• NGC 7469 as seen by MEGARA: new results from high-resolution IFU spectroscopy
• Evidence for chromium hydride in the atmosphere of Hot Jupiter WASP-31b
• First Co-spatial Comparison of Stellar, Neutral-, and Ionized-gas Metallicities in a metal-rich galaxy: M83
• Asteroseismology of evolved stars to constrain the internal transport of angular momentum. IV. Internal rotation of Kepler 56 from an MCMC analysis of the rotational splittings
• Helioseismic Measurements in the Solar Envelope Using Group Velocities of Surface Waves
• The First Dynamical Mass Determination of a Nitrogen-rich Wolf-Rayet Star using a Combined Visual and Spectroscopic Orbit
• Across the Green Valley with HST grisms: colour evolution, crossing time-scales and the growth of the red sequence at $z=1.0-1.8$
• Dust Condensation in Evolving Discs and the Composition of Planetary Building Blocks
• Gauged B-L Number and Neutron--Antineutron Oscillation: Long-range Forces Mediated by Baryophotons
• Coevolution of metallicity and star formation in galaxies to z=3.7: II. A theoretical model
• A theory of mass transfer in binary stars
• Depletion of chlorine into HCl ice in a protostellar core
• The Astrophysical Consequences of Intervening Galaxy Gas on Fast Radio Bursts
• High Resolution Optical Spectroscopy of Stars in the Sylgr Stellar Stream
• Present-day Galactic Evolution: Low-metallicity, Warm, Ionized Gas Inflow Associated with High-Velocity Cloud Complex A
• The Pristine survey -- XV. A CFHT ESPaDOnS view on the Milky Way halo and disc populations
• Axions as a probe of solar metals
• ExoMol photodissociation cross sections I: HCl and HF
• On the stability of bow shocks generated by red supergiants: the case of IRC-10414
• Carbon, Nitrogen and Oxygen Abundances in Atmospheres of the 5-11 M B-type Main Sequence Stars
• New candidates for extremely metal-poor emission-line galaxies in the SDSS/BOSS DR10
• The origin of circumstellar features in the spectra of hot DA white dwarfs
• Ray-tracing simulations and spectral models of X-ray radiation in dusty media
• A search for pulsations in the HgMn star HD 45975 with CoRoT photometry and ground-based spectroscopy
• Metallicity has followed local gravitational potential of galaxies since z=3
• gamma Doradus pulsation in two pre-main sequence stars discovered by CoRoT
• The metal enrichment of passive galaxies in cosmological simulations of galaxy formation
• Observations and numerical modelling of a convective disturbance in a large-scale cyclone in Jupiter's South Temperate Belt
• The Cosmic Evolution of Magnesium Isotopes
• Hubble WFC3 Spectroscopy of the Rocky Planet L 98-59 b: No Evidence for a Cloud-Free Primordial Atmosphere
• Chemical abundances of fast-rotating massive stars. II. Interpretation and comparison with evolutionary models
• Seismic inversion of the solar entropy: A case for improving the Standard Solar Model
• Detection of Two Intervening Ne VIII Absorbers Probing Warm Gas at z~0.6
• High-temperature ${}^{205}$Tl decay clarifies ${}^{205}$Pb dating in early Solar System
• Solar fusion III: New data and theory for hydrogen-burning stars
• HST survey of the Orion Nebula Cluster in the H${}_2$O 1.4 $\mu$m absorption band: II. The substellar IMF down to planetary masses
• Complex Organic Molecules in Star-Forming Regions of the Magellanic Clouds
• Planetary tidal interactions and the rotational evolution of low-mass stars. The Pleiades' anomaly
• Systematic Broad-band X-ray Study of super-Eddington Accretion onto Supermassive Black Holes. I. X-ray Continuum
• Continuum intensity and [O I] spectral line profiles in solar 3D photospheric models: the effect of magnetic fields
• Gas phase Elemental abundances in Molecular cloudS (GEMS) VI. A sulphur journey across star-forming regions: study of thioformaldehyde emission
• Realistic 3D hydrodynamics simulations find significant turbulent entrainment in massive stars
• The effect of the environment-dependent stellar initial mass function on the photometric properties of star-forming galaxies
• Benchmarking MESA isochrones against the Hyades single star sequence
• Discovery of a pre-merger shock in an intercluster filament in Abell 98
• Constraining the Milky Way assembly history with Galactic Archaeology. Ludwig Biermann Award Lecture 2015
• Bayesian Investigation of Isochrone Consistency Using the Old Open Cluster NGC 188
• The last 5 Gyr of Galactic chemical evolution based on H II region abundances derived from a temperature independent method
• GAME: GAlaxy Machine learning for Emission lines
• Measuring elemental abundance ratios in protoplanetary disks at millimeter wavelengths
• Bridging Optical and Far-Infrared Emission-Line Diagrams of Galaxies from Local to the Epoch of Reionization: Characteristic High [O III] 88 $\mu \mathrm{m}$/SFR at $z>6$
• Astrochemical Correlations in Molecular Clouds
• A New Approach to Convective Core Overshooting: Probabilistic Constraints from Color-Magnitude Diagrams of LMC Clusters
• Low-amplitude rotational modulation rather than pulsations in the CoRoT B-type supergiant HD 46769
• VLT/XShooter spectroscopy of Lyman Break Analogs: direct method O/H abundances and nitrogen enhancements
• MUSE-ALMA Haloes VIII: Statistical Study of Circumgalactic Medium Gas
• Comparative high-resolution spectroscopy of M dwarfs -- exploring non-LTE effects
• 3D stellar evolution: hydrodynamic simulations of a complete burning phase in a massive star
• GALEX J184559.8-413827: a new extreme helium star identified using SALT
• Carbon, isotopic ratio ${}^{12}$C/${}^{13}$C and nitrogen in solar twins: constraints for the chemical evolution of the local disc
• High Molecular Gas Masses in Absorption-selected Galaxies at $z\approx 2$
• Galaxy Lookback Evolution Models -- a Comparison with Magneticum Cosmological Simulations and Observations
• On the radial profile of gas-phase Fe/α ratio around distant galaxies
• Deep XMM-Newton Observations of the Most Distant SPT-SZ Galaxy Cluster
• Detection of carbon monoxide's 4.6 micron fundamental band structure in WASP-39b's atmosphere with JWST NIRSpec G395H
• Contamination in TESS light curves: The case of the Fast Yellow Pulsating Supergiants
• An ALMA view of SO and SO${}_2$ around oxygen-rich AGB stars
• ALMA observations of the nearby AGB star L${}_2$ Puppis. II. Gas disk properties derived from ${}^{12}$CO and ${}^{13}$CO $J=$3$-$2 emission
• Atmospheric composition of weak G band stars: CNO and Li abundances
• HST/ACS Photometry of Old Stars in NGC 1569: The Star Formation History of a Nearby Starburst
• HD 179821 (V1427 Aql, IRAS 19114+0002) -- A Massive Post-Red Supergiant Star?
• Modeling contact binaries, II. The effect of energy transfer
• The low-luminosity type II SN\,2016aqf: A well-monitored spectral evolution of the Ni/Fe abundance ratio
• Non-Standard Models, Solar Neutrinos, and Large θ_{13}
• Coronal Elemental Abundances during A-class Solar Flares Observed by Chandrayaan-2 XSM
• Water isotopologues in the circumstellar envelopes of M-type AGB stars
• SPYGLASS. II. The Multi-Generational and Multi-Origin Star Formation History of Cepheus Far North
• Stellar Population Diagnostics of the Massive Star Binary Fraction
• Isotope Anomalies in the Fe-group Elements in Meteorites and Connection to Nucleosynthesis in AGB Stars
• The detailed chemical composition of the terrestrial planet host Kepler-10
• Large Interferometer For Exoplanets (LIFE): VIII. Where is the phosphine? Observing exoplanetary PH3 with a space based MIR nulling interferometer
• Metal and dust evolution in ALMA REBELS galaxies: insights for future JWST observations
• An extremely fast halo hot subdwarf star in a wide binary system
• PopIII signatures in the spectra of PopII/I GRBs
• Investigation of coronal properties of X-ray bright G-dwarf stars based on the solar surface magnetic field -- corona relation
• Optical studies of two stripped envelope supernovae SN 2015ap (Type Ib) and SN 2016P (Type Ic)
• How the first stars shaped the faintest gas-dominated dwarf galaxies
• An in-depth reanalysis of the alleged type Ia supernova progenitor Henize 2-428
• The density-bounded twilight of starbursts in the early Universe
• Probing Structure in Cold Gas at $z\lesssim 1$ with Gravitationally Lensed Quasar Sight Lines
• The GALAH Survey: Accreted stars also inhabit the Spite Plateau
• Type II-P Supernova Progenitor Star Initial Masses and SN 2020jfo: Direct Detection, Light Curve Properties, Nebular Spectroscopy, and Local Environment
• Elliptical accretion disk as a model for tidal disruption events
• N/O abundance ratios in gamma-ray burst and supernova host galaxies at z<4. Comparison with AGN, starburst and HII regions
• H-ATLAS/GAMA: The nature and characteristics of optically red galaxies detected at submillimetre wavelengths
• 3D-HST Emission Line Galaxies at z ~ 2: Discrepancies in the Optical/UV Star Formation Rates
• A theoretical framework of BL Her stars. I. Effect of metallicity and convection parameters on period-luminosity and period-radius relations
• Absolute Calibration of Cepheid Period-Luminosity Relations in NGC 4258
• DZ Cha: a bona fide photoevaporating disc
• Two NIRCam channels are Better than One: How JWST Can Do More Science with NIRCam's Short-Wavelength Dispersed Hartmann Sensor
• Atmospheric parameters and carbon abundance for hot DB white dwarfs
• Atmospheric properties of AF Lep b with forward modeling
• Five-Year Optical and Near Infrared Observations of the Extremely Slow Nova V1280 Scorpii
• A Detailed Study of the Most Relaxed SPT-Selected Galaxy Clusters: Cool Core and Central Galaxy Properties
• JWST COMPASS: NIRSpec/G395H Transmission Observations of the Super-Earth TOI-776b
• A Deep Near-Infrared [Fe II]+[Si I] Emission Line Image of the Supernova Remnant Cassiopeia A
• Observational evidence for composite grains in an AGB outflow: MgS in the extreme carbon star LL Peg
• Experimental study of the removal of excited state phosphorus atoms by H${}_2$O and H${}_2$: implications for the formation of PO in stellar winds
• HD 41641: A classical $\delta$ Sct-type pulsator with chemical signatures of an Ap star
• The Metallicity of the Monoceros Stream
• Relationship between the Elemental Abundances and the Kinematics of Galactic-Field RR Lyrae Stars
• Neutron-capture element abundances in the planetary nebula NGC 5315 from deep optical and near-infrared spectrophotometry
• On the Optical-to-Silicate Extinction Ratio as a Probe of the Dust Size in Active Galactic Nuclei
• Deep secrets of intermediate-mass giants and supergiants: Models with rotation seem to overestimate mixing effects on the surface abundances of C, N, and Na
• Tidal migration of hot Jupiters: introducing the impact of gravity wave dissipation
• Spectroscopic evolution of massive stars near the main sequence at low metallicity
• Probing Population III Initial Mass Functions with He II/H$\alpha$ Intensity Mapping
• Extended theoretical transition data in C I - IV
• SN2020qlb: A hydrogen-poor superluminous supernova with well-characterized light curve undulations
• Evolutionary status of Polaris
• Hydrogen and the Abundances of Elements in Impulsive Solar Energetic-Particle Events
• AB Aur, a Rosetta stone for studies of planet formation (II): H${}_2$S detection and sulfur budget
• Auto-consistent metallicity and star formation history of the nearest blue compact dwarf galaxy NGC 6789
• A Multi-Phase Suzaku Study of X-rays from tau Sco
• Dusty wind of W Hya. Multi-wavelength modelling of the present-day and recent mass-loss
• CEMP stars: possible hosts to carbon planets in the early universe
• Modelling low charge ions in the solar atmosphere
• An outburst scenario for the X-ray spectral variability in 3C 111
• SIMBA-C: An updated chemical enrichment model for galactic chemical evolution in the SIMBA simulation
• Revealing Efficient Dust-Formation at Low Metallicity in Extragalactic Carbon-Rich Wolf-Rayet Binaries
• Extended Ly$\alpha$ emission around quasars with eclipsing damped Ly$\alpha$ systems
• ATOMIUM: Halide molecules around the S-type AGB star W Aquilae
• New hydrodynamic solutions for line-driven winds of hot massive stars using Lambert $W$-function
• Chemical abundance analysis of symbiotic giants - III. Metallicity and CNO abundance patterns in 24 southern systems
• Characterising Atmospheres of Cloudy Temperate Mini-Neptunes with JWST
• Theoretical tidal evolution constants for stellar models from the pre-main sequence to the white dwarf stage Apsidal motion constants, moment of inertia, and gravitational potential energy
• Ly-alpha emission in low-redshift most metal-deficient compact star-forming galaxies
• Nebular and global properties of the gravitationally lensed galaxy "the 8 o'clock arc"
• Chemical Abundance Evidence of Enduring High Star Formation Rates in an Early Type Galaxy: High [Ca/Fe] in NGC 5128 Globular Clusters
• Updated constraints on velocity and momentum-dependent asymmetric dark matter
• The s-Process Enrichment of the Globular Clusters M4 and M22
• Statistical analysis of roAp, He-weak and He-rich stars
• On the Optimal Choice of Nucleosynthetic Yields, IMF and Number of SNe Ia for Chemical Evolution Modelling
• Bootstrapping dielectronic recombination from second-row elements and the Orion Nebula
• Isochrone fitting to the open cluster M67 in the era of Gaia and improved model physics
• A Chandra study of Abell 795 -- a sloshing cluster with a FR0 radio galaxy at its center
• The Galactic Distribution of Phosphorus: A Survey of 163 Disk and Halo Stars
• A hot X-ray filament associated with A3017 galaxy cluster
• Tracking Advanced Planetary Systems (TAPAS) with HARPS-N. VI. HD 238914 and TYC 3318-01333-1 - two more Li-rich giants with planets
• Abundance analysis of a CEMP-no star in the Carina dwarf spheroidal galaxy
• The first retrieval of a substellar subdwarf: A cloud-free SDSS J125637.13-022452.4
• Optical high-resolution spectroscopy of 14 young $\alpha$-rich stars
• Self-ionizing galactic winds
• Mass transfer and tidally tilted pulsation in the Algol-type system TZ Dra
• Apsidal motion in the massive binary HD 152248 -- Constraining the internal structure of the stars
• The influence of a top-heavy integrated galactic IMF and dust on the chemical evolution of high-redshift starbursts
• [OII] emitters in MultiDark-Galaxies and DEEP2
• Retrieving Neptune's aerosol properties from Keck OSIRIS observations. I. Dark regions
• Coronal Elemental Abundance: New Results from Soft X-ray Spectroscopy of the Sun
• Water and Methanol Ice in L1544
• X-ray luminosity function of high-mass X-ray binaries: Studying the signatures of different physical processes using detailed binary evolution calculations
• Modeling dust emission in PN IC 418
• An inflationary disk phase to explain extended protoplanetary dust disks
• Extending the FIP bias sample to magnetically active stars. Challenging the FIP bias paradigm?
• Diagnostic capabilities of spectropolarimetric observations for understanding solar phenomena I. Zeeman-sensitive photospheric lines
• The hot circumgalactic medium of the Milky-Way: new insights from XMM-Newton observations
• Lithium depletion in solar analogs: age and mass effects
• Asteroseismology of RR Lyrae stars with non-radial modes
• A MUSE view of the massive merging galaxy cluster ACT-CL J0102-4915 (El Gordo) at z = 0.87: robust strong lensing model and data release
• First discovery of trans-iron elements in a DAO-type white dwarf (BD$-22{}^{\circ }3467$)
• Sub-Chandrasekhar-mass detonations are in tension with the observed $t_0-M_{\text{Ni56}}$ relation of type Ia supernovae
• Broad-band spectral study of X-ray transient MAXI J1820+070 using Swift/XRT and NuSTAR
• The X-Ray Line Feature At 3.5 Kev In Galaxy Cluster Spectra
• High-mass eclipsing binaries: a testbed for models of interior structure and evolution -- Accurate fundamental properties and surface chemical composition for V1034 Sco, GL Car, V573 Car and V346 Cen
• ecCNO Solar Neutrinos: A Challenge for Gigantic Ultra-Pure Liquid Scintillator Detectors
• Mode identification in three pulsating hot subdwarfs observed with TESS satellite
• pi Aqr is another gamma-Cas object
• A quasar hiding behind two dusty absorbers. Quantifying the selection bias of metal-rich, damped Lyman-alpha absorption systems
• Helioseismology and Asteroseismology: Looking for Gravitational Waves in acoustic oscillations
• Observations and three-dimensional photoionization modelling of the Wolf-Rayet planetary nebula Abell 48
• Projection effects in galaxy cluster samples: insights from X-ray redshifts
• A Bayesian estimation of the helioseismic solar age
• The most metal-rich stars in the universe: chemical contributions of low and intermediate mass asymptotic giant branch stars with metallicities between $0.04\le Z\le \mathrm{0.10.}$
• Interstellar Extinction and Elemental Abundances
• Resolving Star Formation on Sub-Kiloparsec Scales in the High-Redshift Galaxy SDP.11 Using Gravitational Lensing
• On the absolute age of the metal-rich globular M71 (NGC 6838): I. optical photometry
• Neutrino Fluxes from NUHM LSP Annihilations in the Sun
• Self-consistent solutions for line-driven winds of hot massive stars. The m-CAK procedure
• EDGE: The emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations
• Hydrogen and the Abundances of Elements in Gradual Solar Energetic-Particle Events
• Rotating Solar Models with Low Metal Abundances as Good as Those with High Metal Abundances
• Far-Ultraviolet Spectra of Main-Sequence O Stars at Extremely Low Metallicity
• Spectral Evolution of the X-Ray Remnant of SN 1987A: A High-Resolution $Chandra$ HETG Study
• X-ray emission from the giant magnetosphere of the magnetic O-type star NGC 1624-2
• Comprehensive stellar seismic analysis : New method exploiting the glitches information in solar-like pulsators
• Chemical abundance analysis of 13 southern symbiotic giants from high-resolution spectra at ~1.56 μm
• Detailed Abundances of Planet-Hosting Wide Binaries. II. HD80606 + HD80607
• HST/COS Detection of Deuterated Molecular Hydrogen in a DLA at z = 0.18
• Steep extinction towards GRB 140506A reconciled from host galaxy observations: Evidence that steep reddening laws are local
• Extremely metal-poor stars in the Fornax and Carina dwarf spheroidal galaxies
• U Sco 2010 outburst: observational evidence of an underlying ONeMg white dwarf
• Evidence for conservative mass transfer in the classical Algol system $\delta$ Librae from its surface carbon-to-nitrogen abundance ratio
• Testing the Limits of Precise Subgiant Characterization with APOGEE and Gaia: Opening a Window to Unprecedented Astrophysical Studies
• Study of the polarization produced by the Zeeman effect in the solar Mg I b lines
• A solar twin in the eclipsing binary LL Aqr
• High N/O ratio at high redshift as a result of a strong burst of star formation and differential galactic winds
• What have we learned from helioseismology, what have we really learned, and what do we aspire to learn?
• Rubidium and zirconium abundances in massive Galactic asymptotic giant branch stars revisited
• Phosphorus Abundances in the Hyades and Galactic Disk
• A rare early-type star revealed in the Wing of the Small Magellanic Cloud
• X-Shooting ULLYSES: Massive Stars at low metallicity IX: Empirical constraints on mass-loss rates and clumping parameters for OB supergiants in the Large Magellanic Cloud
• Planet Mass and Metallicity: The Exoplanets and Solar System Connection
• Characterisation of 92 Southern TESS Candidate Planet Hosts and a New Photometric [Fe/H] Relation for Cool Dwarfs
• Predicting the COSIE-C Signal from the Outer Corona up to 3 Solar Radii
• Magnetic Field and Atmospheric Chemical Abundances of the Magnetic Ap Star HD 318107
• HOLISMOKES -- V. Microlensing of type II supernovae and time-delay inference through spectroscopic phase retrieval
• The impact of pre-main sequence stellar evolution on midplane snowline locations and C/O in planet forming discs
• A comparison between X-shooter spectra and PHOENIX models across the HR-diagram
• Intriguing X-ray and optical variations of the gamma Cas analog HD45314
• PAHs in protoplanetary disks: emission and X-ray destruction
• Metal-Enriched Neutral Gas Reservoir around a Strongly-lensed, Low-mass Galaxy at $z=4$ Identified by JWST/NIRISS and VLT/MUSE
• Absolute rate coefficients for photorecombination and electron-impact ionization of magnesium-like iron ions from measurements at a heavy-ion storage ring
• r-process Abundance Patterns in the Globular Cluster M92
• The Impact of Outflows driven by Active Galactic Nuclei on Metals in and around Galaxies
• PISN-explorer: hunting the descendants of very massive first stars
• Optimal Integrated Abundances for Chemical Tagging of Extragalactic Globular Clusters
• Quantitative spectroscopy of late O-type main-sequence stars with a hybrid non-LTE method
• Galaxy Ecosystems: gas contents, inflows and outflows
• Sensitivity of a low threshold directional detector to CNO-cycle solar neutrinos
• Tidal Dissipation Impact on the Eccentric Onset of Common Envelope Phases in Massive Binary Star Systems
• The high A_V Quasar Survey: A z=2.027 metal-rich damped Lyman-alpha absorber towards a red quasar at z=3.21
• Understanding the origin of CEMP-no stars through ultra-faint dwarfs
• Thermodynamic fluctuations in solar photospheric three-dimensional convection simulations and observations
• The mass-metallicity relation as a ruler for galaxy evolution: insights from the James Webb Space Telescope
• Detection of Solar-Like Oscillations, Observational Constraints, and Stellar Models for $\theta$ Cyg, the Brightest Star Observed by the {\it Kepler} Mission
• Abundances and Depletions of Neutron-Capture Elements in the Interstellar Medium
• Effects of density on the oxygen ionisation equilibrium in collisional plasmas
• Compact jets dominate the continuum emission in low-luminosity active galactic nuclei
• ALMA and VLA reveal the lukewarm chromospheres of the nearby red supergiants Antares and Betelgeuse
• Many Roads Lead to Lithium: Formation Pathways For Lithium-Rich Red Giants
• 3D magneto-hydrodynamical simulations of stellar convective noise for improved exoplanet detection. I. Case of regularly sampled radial velocity observations
• SN 2018hti: a nearby superluminous supernova discovered in a metal-poor galaxy
• Observations of the low-luminosity Type Iax supernova 2019gsc: a fainter clone of SN 2008ha?
• Evolution of massive stars with new hydrodynamic wind models
• Theoretically Modelling Photoionized Regions with Fractal Geometry in Three Dimensions
• Spatially Resolved Dust, Gas, and Star Formation in the Dwarf Magellanic Irregular NGC4449
• Near Infrared Spectroscopy of M Dwarfs. II. H2O Molecule as an Abundance Indicator of Oxygen
• Fundamental parameters of the close interacting binary HD170582 and its luminous accretion disc
• NLTE analysis of the methylidyne radical (CH) molecular lines in metal-poor stellar atmospheres
• Probing GRB environments with time variability: ULTRASPEC fast imaging of GRB 080210
• The Three Young Nuclear Super Star Clusters in NGC 5253
• The eROSITA view of the Abell 3391/95 field: Cluster Outskirts and Filaments
• Key Atmospheric Signatures for Identifying the Source Reservoirs of Volatiles in Uranus and Neptune
• Evidence of structural discontinuities in the inner core of red-giant stars
• Rossby numbers of fully and partially convective stars
• A Concise Treatise on Converting Stellar Mass Fractions to Abundances to Molar Ratios
• Water Formation During the Epoch of First Metal Enrichment
• The Pan-Pacific Planet Search V. Fundamental Parameters for 164 Evolved Stars
• High Dispersion Spectroscopy of Solar-type Superflare Stars. III. Lithium Abundances
• Non-detection of ${}^6$Li in Spite plateau stars with ESPRESSO
• SN 2008gz - most likely a normal type IIP event
• On the white dwarf cooling sequence with extremely large telescopes
• Determining the Elemental and Isotopic Composition of the preSolar Nebula from Genesis Data Analysis: The Case of Oxygen
• Overcoming the structural surface effect with a realistic treatment of turbulent convection in 1D stellar models
• Observational signature of circumstellar interaction and ${}^{56}$Ni-mixing in the Type II Supernova 2016gfy
• Modeling synthetic spectra for transiting extrasolar giant planets: detectability of H${}_2$S and PH${}_3$ with JWST
• Milky Way archaeology using RR Lyrae and type II Cepheids I. The Orphan stream in 7D using RR Lyrae stars
• Quasar 2175 Å dust absorbers I: metallicity, depletion pattern, and kinematics
• Hinode EIS line widths in the quiet corona up to 1.5 Rsun
• Solar microflares: a case study on temperatures and the Fe XVIII emission
• Messenger Monte-Carlo MAPPINGS V (M^3) -- A self-consistent three-dimensional photoionization code
• Ultraviolet Signatures of the Multiphase Intracluster and Circumgalactic Media in the RomulusC Simulation
• O18O and C18O observations of rho Oph A
• Predominantly Low Metallicities Measured in a Stratified Sample of Lyman Limit Systems at z=3.7
• Solar Dynamics, Rotation, Convection and Overshoot
• The eclipsing binary systems with $\delta$ Scuti component. I. KIC 10661783
• The SRG/eROSITA All-Sky Survey: Constraints on AGN Feedback in Galaxy Groups
• A study of the elements copper through uranium in Sirius A: Contributions from STIS and ground-based spectra
• On the correlation between the local dark matter and stellar velocities
• Optical dimming of RW Aur associated with an iron rich corona and exceptionally high absorbing column density
• The Star Formation Reference Survey-V: the effect of extinction, stellar mass, metallicity, and nuclear activity on star-formation rates based on H$\alpha$ emission
• Temperature and Density Structure of a Recurring Active Region Jet
• On the Emergence of Thousands of Absorption Lines in the Quasar PG1411+442: A Clumpy High-Column Density Outflow from the Broad Emission-Line Region?
• Radio Analysis of SN 2004C Reveals an Unusual CSM Density Profile as a Harbinger of Core Collapse
• The star-formation history of low-mass disk galaxies: a case study of NGC\,300
• TOI-1268b: the youngest, hot, Saturn-mass transiting exoplanet
• The Bimodal Absorption System Imaging Campaign (BASIC) I. A Dual Population of Low-metallicity Absorbers at z $<1$
• Gas Phase Metallicities of Local Ultra-Luminous Infrared Galaxies Follow Normal Star-Forming Galaxies
• Keck and VLT Observations of Super-damped Lyman-alpha Absorbers at z=2=2.5: Constraints on Chemical Compositions and Physical Conditions
• Sulphur abundances in halo giants from the [S I] line at 1082 nm and the S I triplet around 1045 nm
• Evidence for SiO cloud nucleation in the rogue planet PSO J318
• Challenges in the detection of gases in exoplanet atmospheres
• Hypercritical Accretion for Black Hole High Spin in Cygnus X-1
• Dust grains cannot grow to millimeter sizes in protostellar envelopes
• Planetary parameters, XUV environments and mass-loss rates for nearby gaseous planets with X-ray detected host-stars
• Filling the gap between synchronized and non-synchronized sdBs in short-period sdBV+dM binaries with TESS: TIC 137608661, a new system with a well defined rotational splitting
• FUSE, STIS, and Keck spectroscopic analysis of the UV-bright star vZ 1128 in M3 (NGC 5272)
• Spectroscopic and photometric oscillatory envelope variability during the S Doradus outburst of the Luminous Blue Variable R71
• Fluorine Abundances in the Galactic Disk
• Chemical Abundances Of Open Clusters From High-Resolution Infrared Spectra. II. NGC 752
• The changing UV and X-ray properties of the Of?p star CPD -28 2561
• Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. III. Dynamically Tagged Groups and Chemodynamical Properties
• Polycyclic Aromatic Hydrocarbons as Star Formation Rate Indicators
• Decoding the compositions of four bright $r$-process-enhanced stars
• The dust-to-gas mass ratio of luminous galaxies as a function of their metallicity at cosmic noon
• The evolution of lithium in FGK dwarf stars: The Li rotation connection and the Li desert
• A Hint of a Low-Energy Excess in Cosmic-Ray Fluorine
• A Comparison of Rest-frame Ultraviolet and Optical Emission-Line Diagnostics in the Lensed Galaxy SDSS J1723+3411 at Redshift z=1.3293
• Galactic Chemical Evolution of Radioactive Isotopes with an s-process Contribution
• Outflow vs. Infall in Spiral Galaxies: Metal Absorption in the Halo of NGC 891
• The blue supergiant MN18 and its bipolar circumstellar nebula
• Stirred but not shaken: a multi-wavelength view of HD 16743's debris disc
• Limb darkening measurements from TESS and Kepler light curves of transiting exoplanets
• e-MERLIN 21cm constraints on the mass-loss rates of OB stars in Cyg OB2
• Photospheric and coronal abundances in solar-type stars: the peculiar case of Tau Bootis
• The ramp-up of interstellar medium enrichment at z>4
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE).XII. Ionised gas emission in the inner regions of lenticular galaxies
• The Coronal Abundances of Mid-F Dwarfs
• Spectral energy distribution of M-subdwarfs: A study of their atmospheric properties
• New constraints on the nature and origin of the Leading Arm of the Magellanic Stream
• Observational predictions for Thorne-Żytkow objects
• Planet transit and stellar granulation detection with interferometry
• Suzaku X-ray Observations of the Nearest Non-Cool Core Cluster, Antlia: Dynamically Young but with Remarkably Relaxed Outskirts
• The warm Gaseous Disk and the Anisotropic Circumgalactic Medium of the Milky Way
• S stars and s-process in the Gaia era II. Constraining the luminosity of the third dredge-up with Tc-rich S stars
• An Exceptional Dimming Event for a Massive, Cool Supergiant in M51
• Reconstructing Masses of Merging Neutron Stars from Stellar $R$-Process Abundance Signatures
• Convective Excitation and Damping of Solar-like Oscillations
• Low-mass eclipsing binaries in the WFCAM Transit Survey: the persistence of the M-dwarf radius inflation problem
• Forecasting Chemical Abundance Precision for Extragalactic Stellar Archaeology
• Is the Young Star RZ Piscium Consuming Its Own (Planetary) Offspring?
• Sub-damped Lyman alpha systems in the XQ-100 survey I -- Identification and contribution to the cosmological HI budget
• A merger shock in Abell 1367
• Luminous solar neutrinos II: Mass-mixing portals
• On the impact of spectral template uncertainties in synthetic stellar populations
• Differential Modelling Systematics across the HR Diagram from Asteroseismic Surface Corrections
• Modelling the Central Constant Emission X-ray component of eta Carinae
• The Solar Flare Sulphur Abundance from RESIK Observations
• Uncertainties in stellar evolution models: convective overshoot
• Solar Wind Helium Abundance Heralds Solar Cycle Onset
• Comprehensive abundance analysis of red giants in the open clusters Stock 2, NGC 2168, 6475, 6991 and 7762
• The ionised gas outflow in the Circinus galaxy: kinematics and physical conditions
• Shock Heating Energy of Umbral Flashes Measured with Integral Field Unit Spectroscopy
• Silicon isotopic abundance toward evolved stars and its application for presolar grains
• XSHOOTER spectroscopy of the enigmatic planetary nebula Lin49 in the Small Magellanic Cloud
• The formation of barium giants via mass accretion in binary systems
• Empirical estimates of the Galactic halo contribution to the dispersion measures of extragalactic fast radio bursts using X-ray absorption
• The virtual observatory service TheoSSA: Establishing a database of synthetic stellar flux standards. II. NLTE spectral analysis of the OB-type subdwarf Feige 110
• Suppressed CO emission and high G/D ratios in z=2 galaxies with sub-solar gas-phase metallicity
• Small-scale dynamo in cool main sequence stars. II. The effect of metallicity
• The Invisible Majority? Evolution and Detection of Outer Planetary Systems without Gas Giants
• Formation of different isotopomers of chloronium in the interstellar medium
• Cooling flows around cold clouds in the circumgalactic medium: steady-state models & comparison with TNG50
• Very Large Telescope deep echelle spectroscopy of Galactic planetary nebulae NGC 6153, M 1-42 and Hf 2-2
• The Gaia-ESO Survey: The analysis of the hot-star spectra
• Statistical Approach on Differential EmissionMeasure of Coronal Holes using the CATCH Catalog
• Steamworlds: atmospheric structure and critical mass of planets accreting icy pebbles
• Detailed opacity calculations for astrophysical applications
• The Gaia-ESO Survey: Oxygen abundance in the Galactic thin and thick disks
• Evolution of the habitable zone of low-mass stars. Detailed stellar models and analytical relationships for different masses and chemical compositions
• Late-time cosmic evolution of dust: solving the puzzle
• Extending the Chemical Reach of the H3 Survey: Detailed Abundances of the Dwarf-galaxy Stellar Stream Wukong/LMS-1
• Coronal Plasma Characterization via Coordinated Infrared and Extreme Ultraviolet Observations of a Total Solar Eclipse
• Radiative levitation in carbon-enhanced metal-poor stars with s-process enrichment
• Enrichment of the Galactic disc with neutron capture elements: Sr
• Enrichment of Jupiter's atmosphere by late planetesimal bombardment
• Tracing CNO exposed layers in the Algol-type binary system u Her
• Detailed chemical compositions of planet-hosting stars: II. Exploration of the interiors of terrestrial-type exoplanets
• A systematic study of super-Eddington layers in the envelopes of massive stars
• Removing Cool Cores and Central Metallicity Peaks in Galaxy Clusters with Powerful AGN Outbursts
• Chandrasekhar and sub-Chandrasekhar models for the X-ray emission of Type Ia supernova remnants (I): Bulk properties
• Convective storms and atmospheric vertical structure in Uranus and Neptune
• Status of Direct Determination of Solar Neutrino Fluxes after Borexino
• Dust Cooling in Supernova Remnants in the Large Magellanic Cloud
• Emission spectrum of ionized gas in the Irr galaxy Holmberg II
• Discovery of Galactic OIV and OV X-ray absorption due to transition temperature gas in the PKS 2155-304 spectrum
• Looking at the bright side - The story of AA Dor as revealed by its cool companion
• Quasi-equilibrium models of high-redshift disc galaxy evolution
• Chemical Evolution of Fluorine in the Milky Way
• A Comparison of Stellar and Gas-Phase Chemical Abundances in Dusty Early-Type Galaxies
• 3D NLTE modelling of Y and Eu. Centre-to-limb variation and solar abundances
• Super-Earth ingestion can explain the anomalously high metal abundances of M67 Y2235
• Determination of small-scale magnetic fields on Sun-like stars in the near-infrared using CRIRES${}^{+}$
• The origin of the 6.4 keV line emission and H${}_2$ ionization in the diffuse molecular gas of the Galactic center region
• $S^5$: The destruction of a bright dwarf galaxy as revealed by the chemistry of the Indus stellar stream
• The donor star of the X-ray pulsar X1908+075
• A New Precise Determination of the Primordial Abundance of Deuterium: Measurement in the metal-poor sub-DLA system at z=3.42 towards quasar J1332+0052
• Properties of the interstellar medium in star-forming galaxies at redshifts 2 < z < 5 from the VANDELS survey
• Mixing at young ages: Beryllium abundances in cool main-sequence stars of the open clusters IC 2391 and IC 2602
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray properties of Subaru optically-selected clusters
• High-resolution atmospheric retrievals of WASP-76b transmission spectroscopy with ESPRESSO: Monitoring limb asymmetries across multiple transits
• A constraint on the formation timescale of the young open cluster NGC 2264: Lithium abundance of pre-main sequence stars
• High-precision CoRoT space photometry and fundamental parameter determination of the B2.5V star HD 48977
• The mass-loss rates of red supergiants at low metallicity: Detection of rotational CO emission from two red supergiants in the Large Magellanic Cloud
• Asteroseismology of evolved stars to constrain the internal transport of angular momentum. V. Efficiency of the transport on the red giant branch and in the red clump
• A multi-wavelength study of a massive, active galaxy at $z\sim 2$: coupling the kinematics of the ionized and molecular gas
• A thin diffuse component of the Galactic Ridge X-ray emission and heating of the interstellar medium contributed by the radiation of Galactic X-ray binaries
• Constraining convective regions with asteroseismic linear structural inversions
• Measurement of 73Ge(n,g) cross sections and implications for stellar nucleosynthesis
• Kepler-93: a testbed for detailed seismic modelling and orbital evolution of super-earths around solar-like stars
• The atmospheric parameters of FGK stars using wavelet analysis of CORALIE spectra
• Inversions of the Ledoux discriminant: a closer look at the tachocline
• Testing abundance-age relations beyond solar analogues with Kepler LEGACY stars
• Dark dust II: Properties in the general field of the diffuse ISM
• A Spectroscopic and Photometric Investigation of the Mercury-Manganese Star KIC 6128830
• Analysis of first overtone bands of isotopologues of CO and SiO in stellar spectra
• Stellar wind models of central stars of planetary nebulae
• LLAMA: Stellar populations in the nuclei of ultra hard X-ray selected AGN and matched inactive galaxies
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• The Whisper of a Whimper of a Bang: 2400 Days of the Type Ia SN 2011fe Reveals the Decay of ${}^{55}$Fe
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• On the dearth of ultra-faint extremely metal poor galaxies
• Helium Suppression in Impulsive Solar Energetic-Particle Events
• Evidence of Pop~III stars' chemical signature in neutral gas at z~6. A study based on the E-XQR-30 spectroscopic sample
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• The amplitude of solar p-mode oscillations from three-dimensional convection simulations
• Spatial Distribution of Metals in the ICM: Evolution of the Iron Excess in Relaxed Galaxy Clusters
• Electron Energy Distributions in HII Regions and Planetary Nebulae: kappa-Distributions Do Not Apply
• HII regions in CALIFA survey: II. The relation between their physical properties and galaxy evolution
• Testing MURaM and MPS-ATLAS against the quiet solar spectrum
• Comparing the Effect of Radiative Transfer Schemes on Convection Simulations
• KSP-SN-2016kf: a long-rising H-rich Type II Supernova with unusually high ${}^{56}$Ni mass discovered in the KMTNet Supernova Program
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• Observations of Type Ia Supernova 2014J for Nearly 900 Days and Constraints on Its Progenitor System
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• The Concentration-Mass Relation of Massive, Dynamically Relaxed Galaxy Clusters: Agreement Between Observations and $\Lambda$CDM Simulations
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• The IACOB project XI. No increase of mass-loss rates over the bistability region
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• Extreme Ionizing Properties of Metal-Poor, Muv ~ -12 Star Complex in the first Gyr
• Aluminum-26 Enrichment in the Surface of Protostellar Disks Due to Protostellar Cosmic Rays
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• On the determination of the He abundance distribution in globular clusters from the width of the main sequence
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• The impact of (n,$\gamma$) reaction rate uncertainties on the predicted abundances of i-process elements with $32\le Z\le 48$ in the metal-poor star HD94028
• Measuring Tracers of Planet Formation in the Atmosphere of WASP-77A b: Sub-stellar O/H and C/H ratios, with a stellar C/O ratio and a potentially Super-stellar Ti/H ratio
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• FIRST, a fibered aperture masking instrument II. Spectroscopy of the Capella binary system at the diffraction limit
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• Leveraging HST with MUSE: I. Sodium abundance variations within the 2 Gyr-old cluster NGC 1978
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• On the possible noble gas deficiency of Pluto's atmosphere
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• Constraints on the Galactic Inner Halo Assembly History from the Age Gradient of Blue Horizontal-branch Stars
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• LIGO-Virgo-KAGRA's Oldest Black Holes: Probing star formation at cosmic noon with GWTC-3
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• A quantitative NLTE analysis of visual and ultraviolet spectra of four helium-rich subdwarf O stars
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• Effect of Photodesorption on Snow Line at the Surface of Optically Thick Circumstellar Disks around Herbig Ae/Be Stars
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• A Gemini/GMOS study of the physical conditions and kinematics of the blue compact dwarf galaxy Mrk 996
• A limit on variations in the fine-structure constant from spectra of nearby Sun-like stars
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• Probing the early Milky Way with GHOST spectra of an extremely metal-poor star in the Galactic disk
• The VLT/SPHERE view of the ATOMIUM cool evolved star sample. I. Overview: Sample characterization through polarization analysis
• The formation of the primitive star SDSS J102915+172927: effect of the dust mass and the grain-size distribution
• Dissecting the microphysics behind the metallicity-dependence of massive stars radii
• On the Habitability of Universes without Stable Deuterium
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• On the Anomalous Silicate Absorption Feature of the Prototypical Seyfert 2 Galaxy NGC 1068
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• Helium and Nitrogen Enrichment in Massive Main Sequence Stars: Mechanisms and Implications for the Origin of WNL Stars
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• A combined HST and XMM-Newton campaign for the magnetic O9.7 V star HD 54879: towards constraining the weak-wind problem of massive stars
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• The Morphological, Elastic, and Electric Properties of Dust Aggregates in Comets: A Close Look at COSIMA/Rosetta's Data on Dust in Comet 67P/Churyumov-Gerasimenko
• Thorough characterisation of the 16 Cygni system. Part II. Seismic inversions of the internal structure
• A Nucleosynthetic Origin for the Southwestern Fe-rich Structure in Kepler's Supernova Remnant
• Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. VII. Lithium
• Sub-damped Lyman alpha systems in the XQ-100 survey II -- Chemical evolution at 2.4<z<4.3
• Asteroseismology of the double-radial mode $\delta$ Scuti star BP Pegasi
• A study of methanol and silicon monoxide production through episodic explosions of grain mantles in the Central Molecular Zone
• Analytic solution of Chemical Evolution Models with Type Ia SNe
• Candidate LBV stars in galaxy NGC 7793 found via HST photometry + MUSE spectroscopy
• Highly Ionized Collimated Outflow from HE 0238 - 1904
• Molecular tracers of planet formation in the atmospheres of hot Jupiters
• Fundamental parameters and evolutionary status of the magnetic chemically peculiar stars HD 188041 (V1291 Aquilae), HD 111133 (EP Virginis), and HD 204411. Spectroscopy versus interferometry
• The Oxygen Abundance in the Solar Neighborhood
• Chemical Abundances of Planetary Nebulae in the Substructures of M31 -- II. The Extended Sample and A Comparison Study with the Outer-disk Group
• A Closer Look at Some Gas-Phase Depletions in the ISM: Trends for O, Ge, and Kr vs. $F_{\ast }$, $f({\mathrm{H}}_2)$, and Starlight Intensity
• CHIPS: Complete History of Interaction-Powered Supernovae
• The XUV irradiation and likely atmospheric escape of the super-Earth $\pi$ Men c
• Geoneutrinos and geoscience: an intriguing joint-venture
• Evidence of multithermal nature of spicular downflows. Impact on solar atmospheric heating
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• Solar Cycle Dependence of ICME Composition
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• AGN feedback and iron enrichment in the powerful radio galaxy, 4C+55.16
• Ground-based Spectroscopy of the Exoplanet XO-2b using a Systematic Wavelength Calibration
• Spectroscopic observations of active solar-analog stars having high X-ray luminosity, as a proxy of superflare stars
• Complete X-ray census of Mdwarfs in the solar Neighborhood I. GJ 745 AB: Coronal-hole Stars in the 10 pc Sample
• Convective settling in main sequence stars: Li and Be depletion
• Multi-wavelength campaign on NGC7469 II. Column densities and variability in the X-ray spectrum
• Fundamental stellar parameters and age-metallicity relation of Kepler red giants in comparison with theoretical evolutionary tracks
• Photon leaking or very hard ionizing radiation? Unveiling the nature of heII-emitters using the softness diagram
• An efficient method for determining the chemical evolution of gravitationally collapsing prestellar cores
• Chemical evolution of local post-starburst galaxies: Implications for the mass-metallicity relation
• The Cosmic Ultraviolet Baryon Survey (CUBS) II: Discovery of an H${}_2$-Bearing DLA in the Vicinity of an Early-Type Galaxy at z = 0.576
• Mg ii h&k spectra of an enhanced network region simulated with the MURaM-ChE code. Results using 1.5D synthesis
• Merging binary black holes formed through double-core evolution
• An asteroseismic age estimate of the open cluster NGC 6866 using Kepler and Gaia
• Spectroscopic Observations of Planetary Nebulae in the Northern Spur of M31
• Aluminium-26 from massive binary stars III. Binary stars up to core-collapse and their impact on the early Solar System
• Radiative properties of stellar plasmas and open challenges
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• A cosmic formation site of silicon and sulphur revealed by a new type of supernova explosion
• The mass--metallicity relation AKARI-FMOS infrared galaxies at $z\sim 0.88$ in the AKARI North Ecliptic Pole Deep Survey Field
• Planetary candidates transiting cool dwarf stars from Campaigns 12 to 15 of K2
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• Asteroseismology of evolved stars to constrain the internal transport of angular momentum. VI. Testing a parametric formulation for the azimuthal magneto-rotational instability
• Characteristics and applications of interplanetary coronal mass ejection composition
• Simulating extremely metal-poor gas and DLA metal content at redshift z=7
• {\it HST}/COS Observations of the Warm Ionized Gaseous Halo of NGC 891
• Chemical evolution of ${}^{26}$Al and ${}^{60}$Fe in the Milky Way
• Asteroseismology of $\delta$ Scuti stars: emulating model grids using a neural network
• The explosion energy of early stellar populations: The Fe-peak element ratios in low metallicity damped Lyman-alpha systems
• The supernova impostor PSN J09132750+7627410 and its progenitor
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• Chemical tracers of high-metallicity environments
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• Quasar 2175 Å dust absorbers II: Correlation analysis and relationship with other absorption line systems
• Emergence of small-scale magnetic flux in the quiet Sun
• Some glimpses from helioseismology at the dynamics of the deep solar interior
• Empirical mass-loss rates and clumping properties of O-type stars in the LMC
• Star Cluster Ages in the Gaia Era
• Stellar abundance of binary stars: their role in determining the formation location of super-Earths and ice giants
• Observational signatures of past mass-exchange episodes in massive binaries: The case of LSS 3074
• New constraints on the physical conditions in H${}_2$-bearing GRB-host damped Lyman-$\alpha$ absorbers
• Detection of Pristine Circumstellar Material of the Cassiopeia A Supernova
• Estimating dayside effective temperatures of hot Jupiters and associated uncertainties through Gaussian process regression
• Evolution and explosions of metal enriched supermassive stars: proton rich general relativistic instability supernovae
• Classifying AGN by X-ray Hardness Variability
• Metallicities in the Outer Regions of Spiral Galaxies
• Identification of Absorption Lines of Heavy Metals in the Wavelength Range 0.97--1.32 Micron
• The COS-legacy survey of C IV absorbers: properties and origins of the intervening systems
• Method and new tabulations for flux-weighted line-opacity and radiation line-force in supersonic media
• NLTE modelling of integrated light spectra. Abundances of barium, magnesium, and manganese in a metal-poor globular cluster
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• High spectral resolution spectroscopy of the SiO fundamental lines in red giants and red supergiants with VLT/VISIR
• Apsidal motion in massive eccentric binaries: The case of CPD-41${}^{\circ }$7742, and HD 152218 revisited
• Galactic structure in the outer disk: the field in the line of sight to the intermediate-age open cluster Tombaugh 1
• New Mn II energy levels from STIS-HST spectrum of the HgMn star HD 175640
• Coronal Densities, Temperatures and Abundances During the 2019 Total Solar Eclipse: The Role of Multi-Wavelength Observations in Coronal Plasma Characterization
• Chemical mixing in low mass stars: I. Rotation against atomic diffusion including radiative accelerations
• PHANGS-JWST First Results: A combined HST and JWST analysis of the nuclear star cluster in NGC 628
• CLASH-VLT: The inner slope of the MACS J1206.2-0847 dark matter density profile
• H${}_2$S observations in young stellar disks in Taurus
• The L1157-B1 astrochemical laboratory: testing the origin of DCN
• Keck HIRES Spectroscopy of SkyMapper Commissioning Survey Candidate Extremely Metal-Poor Stars
• Iron abundance in the prototype PG1159 star, GW Vir pulsator PG1159-035, and related objects
• Regular frequency patterns in the young delta Scuti star HD 261711 observed by the CoRoT and MOST satellites
• Probing Reionization and Early Cosmic Enrichment with the MgII Forest
• Carbon Abundances of Metal-Poor Star Determined from the C I 1.068-1.069 micron Lines
• A Critique of the Spite Plateau, and the Astration of Primordial Lithium
• What determines active region coronal plasma composition?
• Metal-enriched Galaxies in the First ~1 Billion Years: Evidence of a Smooth Metallicity Evolution at z ~ 5
• The atmosphere of WASP-17b: Optical high-resolution transmission spectroscopy
• Absolute dimensions of the metallic-line eclipsing binary V501 Monocerotis
• Deep near-IR observations of the Globular Cluster M4: Hunting for Brown Dwarfs
• Chlorine Abundances in Cool Stars
• MIRIS observation of near-infrared diffuse Galactic light
• The stochastic enrichment of Population II stars
• Abundance analysis of the outer halo globular cluster Palomar 14
• Evidence for a chemical enrichment coupling of globular clusters and field stars in the Fornax dSph
• X-shooter Observations of the Gravitational Lens System CASSOWARY 5
• HIP 10725: The First Solar Twin/Analogue Field Blue Straggler
• SOFIA-EXES Observations of Betelgeuse during the Great Dimming of 2019/2020
• The role of complex ionized absorber in the soft X-ray spectra of Intermediate Polars
• An extended and refined grid of 3D STAGGER model atmospheres. Processed snapshots for stellar spectroscopy
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• The surprisingly carbon-rich environment of the S-type star W Aql
• $Chempy$: A flexible chemical evolution model for abundance fitting - Do the Sun's abundances alone constrain chemical evolution models?
• High-redshift Damped Ly-alpha Absorbing Galaxy Model Reproducing the N(HI)-Z Distribution
• On the nature of the brightest globular cluster in M81
• The Atmospheres of Rocky Exoplanets II. Influence of surface composition on the diversity of cloud condensates
• Peering above the clouds of the warm Neptune GJ 436b with CRIRES+
• Probing O-enrichment in C-rich dust planetary nebulae
• Does magnetic field impact tidal dynamics inside the convective zone of low-mass stars along their evolution?
• X-ray spectroscopy in the microcalorimeter era 4: Optical depth effects on the soft X-rays studied with CLOUDY
• Deeply cooled core of the Phoenix galaxy cluster imaged by ALMA with the Sunyaev-Zel'dovich effect
• Origin of a massive hyper-runaway subgiant star LAMOST-HVS1 -- implication from Gaia and follow-up spectroscopy
• Carbon and Oxygen abundances across the Hertzsprung gap
• On line contribution functions and examining spectral line formation in 3D model stellar atmospheres
• Apsidal motion in the massive binary HD152248
• The Blue Supergiant Progenitor of the Supernova Imposter AT~2019krl
• Red Horizontal Branch stars: an asteroseismic perspective
• Numerical Models for the Diffuse Ionized Gas in Galaxies. II. Three-dimensional radiative transfer in inhomogeneous interstellar structures as a tool for analyzing the diffuse ionized gas
• PDRs4All. X. ALMA and JWST detection of neutral carbon in the externally irradiated disk d203-506: Undepleted gas-phase carbon
• The Enigma of the Open Cluster M29 (NGC 6913) Solved
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• PHL 417: a zirconium-rich pulsating hot subdwarf (V366 Aquarid) discovered in K2 data
• Galactic planetary nebulae with precise nebular abundances as a tool to understand the evolution of asymptotic giant branch stars
• BOWIE-ALIGN: A JWST comparative survey of aligned vs misaligned hot Jupiters to test the dependence of atmospheric composition on migration history
• The ultra-long GRB 220627A at z=3.08
• Influence of grain sizes and composition on the contraction rates of planetary envelopes and on planetary migration
• The large-scale magnetic field of the eccentric pre-main-sequence binary system V1878 Ori
• Fluorine Abundances in the Galactic Nuclear Star Cluster
• A coronagraphic absorbing cloud reveals the narrow-line region and extended Lyman-$\alpha$ emission of QSO J0823+0529
• Constraints on the Galactic Centre environment from Gaia hypervelocity stars II: The evolved population
• Addressing the acoustic tachocline anomaly and the lithium depletion problem at the same time
• Influence of XUV radiation on Pv ionization fraction in hot star winds
• Changing disc compositions via internal photoevaporation I: Solar-mass stars
• X-raying the AU Microscopii debris disk
• Atmospheric NLTE-Models for the Spectroscopic Analysis of Blue Stars with Winds. III. X-ray emission from wind-embedded shocks
• Radiative Turbulent Mixing Layers and the Survival of Magellanic Debris
• Pulsational instability of pre-main-sequence models from accreting protostars II. Modelling echelle diagrams of $\delta$ Scuti stars without rotational splitting
• The Belgian repository of fundamental atomic data and stellar spectra (BRASS). I. Cross-matching atomic databases of astrophysical interest
• Astrophysical parameters and orbital solution of the peculiar X-ray transient IGR J00370+6122
• MgII 2797, 2803 emission in a large sample of low-metallicity star-forming galaxies from SDSS DR14
• Light Element Abundances and Multiple Populations in M10
• Properties of the Umbral Filament Observed in Active Region NOAA 12529
• The role of gas kinematics in setting metallicity gradients at high redshift
• POPSTAR Evolutionary Synthesis Models III: Photometric properties of young star clusters and mixed populations
• Small-spatial scale variations of nebular properties and the abundance discrepancy in three Galactic HII regions
• Spectral analysis of four surprisingly similar hot hydrogen-rich subdwarf O stars
• Stellar models with self-consistent Rosseland opacities
• IRAS\,11472-0800: an extremely depleted pulsating binary post-AGB star
• Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. II. Discovery of a Failed Hot Jupiter on a 2.7 Year, Highly Eccentric Orbit
• Synthetic photometry of OB star clusters with stochastically sampled IMFs: analysis of models and HST observations
• Mergers of neutron stars and black holes with cores of giant stars: a population synthesis study
• A hot gaseous galaxy halo candidate with Mg X absorption
• The quadruple-lined, doubly-eclipsing system V482 Persei
• Properties of a Polar Coronal Hole During the Solar Minimum in 2007
• HAT-TR-318-007: a double-lined M-dwarf binary with total secondary eclipses discovered by HATNet and observed by K2
• Suzaku Monitoring of Hard X-ray Emission from Eta Carinae over a Single Binary Orbital Cycle
• Using cosmological simulations and synthetic absorption spectra to assess the accuracy of observationally derived CGM metallicities
• Calculation of molecular line intensity in stellar atmospheres
• New X-ray detections of magnetic period-bounce cataclysmic variables from XMM-Newton and SRG/eROSITA
• Quasars with PV broad absorption in BOSS data release 9
• ALMA Observations of Giant Molecular Clouds in the Starburst Dwarf Galaxy Henize 2-10
• Heavy element abundances in P-rich stars: A new site for the s-process?
• A Long Stream of Metal-Poor Cool Gas around a Massive Starburst Galaxy at z = 2.67
• Modeling the Infrared Extinction toward the Galactic Center
• Outer regions of the merging system Arp 270
• Global Analysis of KOI-977: Spectroscopy, Asteroseismology, and Phase-curve Analysis
• Astrophysical implications of the proton-proton cross section updates
• A Photodissociation Region study of NGC 4038
• A chemical signature from fast-rotating low-metallicity massive stars: ROA 276 in omega Centauri
• Asteroseismic analysis of two alpha-enhanced stars KIC 7976303 and KIC 8694723
• Analysis of the linear approximation of seismic inversions for various structural pairs
• The IACOB project: IV. New predictions for high-degree non-radial mode instability domains in massive stars and connection with macroturbulent broadening
• Constraining the final fates of massive stars by oxygen and iron enrichment history in the Galaxy
• Discovery of a Metal-poor, Luminous Post-AGB Star that Failed the Third Dredge-up
• Metallicities of Young Massive Clusters in NGC 5236 (M83)
• Detailed chemical abundance analysis of the thick disk star cluster Gaia 1
• Infrared Spectroscopy of HR 4796A's Bright Outer Cometary Ring + Tenuous Inner Hot Dust Cloud
• Re-awakening of GRS 1716--249 after 23 years, observed by {\it Swift}/XRT and {\it NuSTAR}
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• A Dynamical Study of Extraplanar Diffuse Ionized Gas in NGC 5775
• The dynamical state of Abell 2399: a bullet-like cluster
• An improved parametric method for evaluating radiative accelerations in stellar interiors
• A chemical study of carbon fractionation in external galaxies
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• Inverted metallicity gradients in two Virgo cluster star-forming dwarf galaxies: evidence of recent merging?
• ALMA observations of CS in NGC 1068: chemistry and excitation
• Discovery of High-Velocity H$\alpha$ Emission in the Direction of the Fermi Bubble
• The H${}_2$O Spectrum of the Massive Protostar AFGL 2136 IRS 1 from 2 to 13 $\mu$m at High Resolution: Probing the Circumstellar Disk
• Stellar laboratories. X. New Cu IV - VII oscillator strengths and the first detection of copper and indium in hot white dwarfs
• High-cadence Dispersed Spectral Analysis of Supernova Remnant 1987A
• Diagnosing the interstellar medium of galaxies with far-infrared emission lines I. The [C II] 158 microns line at z~0
• The K2 M67 Study: Precise Mass for a Turnoff Star in the Old Open Cluster M67
• Evidence for galaxy quenching in the green valley caused by a lack of a circumgalactic medium
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• Spectral analysis of the low-mass X-ray pulsar 4U 1822-371: Reflection component in a high-inclination system
• Cloud-convection feedback in brown dwarfs atmosphere
• The ALPINE-ALMA [CII] Survey: Investigation of 10 Galaxies at $z\sim 4.5$ with [OII] and [CII] Line Emission $-$ ISM Properties and [OII]$-$SFR Relation
• Neural networks: solving the chemistry of the interstellar medium
• Modification of the radioactive heat budget of Earth-like exoplanets by the loss of primordial atmospheres
• The imprint of star formation on stellar pulsations
• The giants that were born swiftly -- Implications of the top-heavy stellar initial mass function on the birth conditions of globular clusters
• The effects of local stellar radiation and dust depletion on non-equilibrium interstellar chemistry
• Optical spectroscopy of the extremely metal-deficient star-forming galaxy HSC J1631+4426: a test of the strong-line method
• Cosmic Ray Interstellar Propagation Tool using Itô Calculus (criptic): software for simultaneous calculation of cosmic ray transport and observational signatures
• The Origin of Stars in the Inner 500 Parsecs in TNG50 Galaxies
• The chemical evolution of the solar neighbourhood for planet-hosting stars
• Latest Evolution of the X-Ray Remnant of SN 1987A: Beyond the Inner Ring
• Eta-Earth Revisited II: Deriving a Maximum Number of Earth-like Habitats in the Galactic Disk
• WASP-121b's transmission spectrum observed with JWST/NIRSpec G395H reveals thermal dissociation and SiO in the atmosphere
• PDRs4All. XII. FUV-driven formation of hydrocarbon radicals and their relation with PAHs
• The Formation of Black Holes in Non-interacting, Isolated Binaries. Gaia Black Holes as Calibrators of Stellar Winds From Massive Stars
• Boron depletion in Galactic early B-type stars reveals two different main sequence star populations
• CAI formation in the early Solar System
• The cold interstellar medium of a normal sub-$L^{\star }$ galaxy at the end of reionization
• Chemical Diagnostics to Unveil Environments Enriched by First Stars
• The SRG/eROSITA All-Sky Survey: View of the Virgo Cluster
• Trading oxygen for iron I: the [O/Fe] -- specific star formation rate relation of galaxies
• The Great Dimming of the hypergiant star RW Cephei: CHARA Array images and spectral analysis
• Probing the hot circumgalactic medium of external galaxies in X-ray absorption II: a luminous spiral galaxy at $z\approx 0.225$
• Dynamical He Flashes in Double White Dwarf Binaries
• Evidence for multiple nucleosynthetic processes from carbon enhanced metal-poor stars in the Carina dwarf spheroidal galaxy
• Production of $p$-nuclei from $r$-process seeds: the $\nu r$-process
• Iron-Peak Element Abundances in Warm Very Metal-Poor Stars
• A Glimpse of the Stellar Populations and Elemental Abundances of Gravitationally Lensed, Quiescent Galaxies at $z\gtrsim 1$ with Keck Deep Spectroscopy
• Mass function of a young cluster in a low-metallicity environment. Sh 2-209
• The EBLM project X. Benchmark masses, radii and temperatures for two fully convective M-dwarfs using K2
• New Detections of Phosphorus Molecules towards Solar-type Protostars
• How do Spitzer IRAC Fluxes Compare to HST CALSPEC
• The peculiar chemical pattern of the WASP-160 binary system: signatures of planetary formation and evolution?
• Longitudinally Resolved Spectral Retrieval (ReSpect) of WASP-43b
• Fundamental properties of a selected sample of Ap stars: Inferences from interferometric and asteroseismic constraints
• Wind suppression by X-rays in Cygnus X-3
• The Mass Budget Necessary to Explain `Oumuamua as a Nitrogen Iceberg
• Absorption-selected galaxies trace the low-mass, late-type, star-forming population at $z\sim 2-3$
• Coupled Day-Night Models of Exoplanetary Atmospheres
• Seismic analysis of the double-mode radial pulsator SX Phoenicis
• VALES VII: Molecular and ionized gas properties in pressure balanced interstellar medium of starburst galaxies at z ~ 0.15
• The M dwarf problem: Fe and Ti abundances in a volume-limited sample of M dwarf stars
• Simulating Solar Flare Irradiance with Multithreaded Models of Flare Arcades
• Forming one of the most massive objects in the Universe: The quadruple merger in Abell 1758
• Metallicity, temperature, and gravity scales of M subdwarfs
• The GALAH Survey: Lithium-strong KM dwarfs
• G7.7-3.7: a young supernova remnant probably associated with the guest star in 386 CE (SN 386)
• Metal Pollution of Low-Mass Population III Stars through Accretion of Interstellar Objects like `Oumuamua
• $\alpha$ Centauri A as a potential stellar model calibrator: establishing the nature of its core
• Chemical composition of two bright extremely metal-poor stars from the SDSS MARVELS pre-survey
• Discovery of a new classical nova shell around a nova-like cataclysmic variable
• Stellar parameters for the central star of the planetary nebula PRTM 1 using the German Astrophysical Virtual Observatory service TheoSSA
• On the deuterium abundance and the importance of stellar mass loss in the interstellar and intergalactic medium
• Physical conditions of the molecular gas in metal-poor galaxies
• Asteroseismic inversions in the Kepler era: application to the Kepler Legacy sample
• A Quintuple Star System Containing Two Eclipsing Binaries
• The chemical composition of red giants in 47 Tucanae. II. Magnesium isotopes and pollution scenarios
• Lithium in Open Cluster Red Giants Hosting Substellar Companions
• WASP-135b: a highly irradiated, inflated hot Jupiter orbiting a G5V star
• Near infrared spectroscopy of M dwarfs. III. Carbon and oxygen abundances in late M dwarfs including the dusty rapid rotator 2MASSI J1835379+325954
• HE 0017+0055 : A probable pulsating CEMP-rs star and long-period binary
• The far-ultraviolet spectra of "cool" PG1159 stars
• Overshooting by convective settling
• The [alpha/Fe] ratios of very metal-poor stars within the IGIMF theory
• What produces the extended LINER-type emission in the NUGA galaxy NGC 5850?
• Evolution of the Mass-Metallicity relations in passive and star-forming galaxies from SPH-cosmological simulations
• Abundance study of the two solar-analogue CoRoT targets HD 42618 and HD 43587 from HARPS spectroscopy
• Density Functional Theory Approach to Nuclear Fission
• Chemical abundances in Orion protoplanetary discs: integral field spectroscopy and photoevaporation models of HST 10
• A complete X-ray spectral coverage of the 2010 May-June outbursts of Circinus X-1
• Electron Distribution in the Galactic Disk - Results From a Non-Equilibrium Ionization Model of the ISM
• SGAS 143845.1+145407: A Big, Cool Starburst at Redshift 0.816
• Cosmic star formation rate: a theoretical approach
• CNO and F abundances in the barium star HD 123396
• The effect of the regular solution model in the condensation of protoplanetary dust
• Theoretical and experimental activities on opacities for a good interpretation of seismic stellar probes
• Gas absorption and dust extinction towards the Orion Nebula Cluster
• Multicomponent H2 in DLA at zabs = 2.05: physical conditions through observations and numerical models
• Mixed Modes and Asteroseismic Surface Effects: II. Subgiant Systematics
• Soft X-ray Spectral Diagnostics of Multi-thermal Plasma in Solar Flares with Chandrayaan-2 XSM
• Model Atmospheres for X-ray Bursting Neutron Stars
• A candidate planetary-mass object with a photoevaporating disk in Orion
• The sulphur species in hot rocky exoplanet atmospheres
• Mixing of materials in magnetised core-collapse supernova remnants
• Deeply Buried Nuclei in the Infrared-Luminous Galaxies NGC 4418 and Arp 220: I. ALMA Observations at $\lambda =$1.4-0.4 mm and Continuum Analysis
• Photospheric carbon and oxygen abundances of F-G type stars in the Pleiades cluster
• Neutron-Capture Element Abundances in Magellanic Cloud Planetary Nebulae
• The ESO UVES Advanced Data Products Quasar Sample - IV. On the deficiency of Argon in DLA systems
• Asteroseismology of $\beta$ Cephei stars: The stellar inferences tested in hare and hound exercises
• Lyman-alpha radiation pressure: an analytical exploration
• Constraining the ${}^7$Be($p,\gamma$)${}^8$B $S$-factor with the new precise ${}^7$Be solar neutrino flux from Borexino
• Search for Extremely Metal-Poor Stars with GEMINI-N/GRACES I. Chemical-Abundance Analysis
• Plasma opacity calculations using the Starrett and Saumon average-atom model with ion correlations
• Using realistic host galaxy metallicities to improve the GRB X-ray equivalent total hydrogen column density and constrain the intergalactic medium density
• Novel bounds on decaying axionlike particle dark matter from the cosmic background
• Neon Abundances of B-stars in the Solar Neighborhood
• Co-spatial Long-slit UV/Optical Spectra of Ten Galactic Planetary Nebulae with HST/STIS II. Nebular Models, Central Star Properties and He+CNO Synthesis
• The dynamical mass and evolutionary status of the type-II Cepheid in the eclipsing binary system OGLE-LMC-T2CEP-211 with a double-ring disk
• An Expanded Set of Los Alamos OPLIB Tables in MESA: Type-1 Rosseland-mean Opacities and Solar Models
• Diagnostics of Parameters for the X-ray Jets of SS 433 from High-Resolution Chandra Spectroscopy
• Optimal Celestial Bodies for Dark Matter Detection
• Optical interferometry and Gaia measurement uncertainties reveal the physics of asymptotic giant branch stars
• Simulation of energy transport by dark matter scattering in stars
• Gas sloshing and cold fronts in pre-merging galaxy cluster Abell 98
• High velocity blue-shifted FeII absorption in the dwarf star-forming galaxy PHL293B: Evidence for a wind driven supershell?
• K-CLASH: Strangulation and Ram Pressure Stripping in Galaxy Cluster Members at 0.3 < z < 0.6
• The inner circumstellar dust of the red supergiant Antares as seen with VLT/SPHERE/ZIMPOL
• Quasar outflow energetics from broad absorption line variability
• Dust Extinction Law in Nearby Star-Resolved Galaxies. I. M31 Traced by Supergiants
• disnht: modeling X-ray absorption from distributed column densities
• New orbital ephemerides for the dipping source 4U 1323-619: constraining the distance to the source
• On the production of He${}^{+}$ of solar origin in the solar wind
• Carbon line formation and spectroscopy in O-type stars
• Locked In Ice: how Pebble Drift and Volatile Entrapment can Significantly Impact Carbon and Oxygen Ratios in Evolving Protoplanetary Discs
• Super lithium-rich K giant with low ${}^{12}\mathrm{C}$ to ${}^{13}\mathrm{C}$ ratio
• Developing the physical understanding of intermediate polars: an X-ray study of TV Col and V2731 Oph
• Apsidal motion in massive eccentric binaries in NGC 6231: The case of HD 152219
• The first all-sky survey of star-forming galaxies with eROSITA: Scaling relations and a population of X-ray luminous starbursts
• The metallicity and star formation activity of long gamma-ray burst hosts for z$<$3: insights from the Illustris simulation
• Galactic Constraints on Supernova Progenitor Models
• Modelling of the B-type binaries CW Cep and U Oph: A critical view on dynamical masses, core boundary mixing, and core mass
• Comprehensive UV and Optical spectral analysis of Cygnus X-1: Stellar and wind parameters, abundances, and evolutionary implications
• Spatially resolved analysis of Superluminous Supernovae PTF~11hrq and PTF~12dam host galaxies
• Asteroseismic and orbital analysis of the triple star system HD 188753 observed by Kepler
• The magnetised and thermally unstable tails of jellyfish galaxies
• The impact of composition choices on solar evolution: age, helio- and asteroseismology, and neutrinos
• Redshift evolution of the hot intracluster gas metallicity in the C-EAGLE cluster simulations
• An X-ray Census of Fast Radio Burst Host Galaxies: Constraints on AGN and X-ray Counterparts
• Deep Narrowband Photometry of the M101 Group: Strong-Line Abundances of 720 HII Regions
• The effect of radiation pressure on spatial distribution of dust inside HII regions
• Metal enrichment signatures of the first stars on high-z DLAs
• Search for planets around stars with wide brown dwarfs
• The Helium Abundance in the Ejecta of U Scorpii
• From the stellar properties of HD219134 to the internal compositions of its transiting exoplanets
• Ab initio Study of Ground-State CS Photodissociation Via Highly Excited Electronic States
• An abundance analysis from the STIS-HST UV spectrum of the non-magnetic Bp star HR 6000
• CCD $UBV(RI{)}_C$ Photometry of Twenty Open Clusters
• Supernova 2020wnt: An Atypical Superluminous Supernova with a Hidden Central Engine
• Discovery of a magnetic field in the early B-type star sigma Lupi
• On the Nitrogen variation in ~2 Gyr old massive star clusters in the Large Magellanic Cloud
• The polluted atmosphere of the white dwarf NLTT 25792 and the diversity of circumstellar environments
• Hidden IR structures in NGC 40: signpost of an ancient born-again event
• Planetary influence on the young Sun's evolution: the solar neutrino probe
• Two Planets Straddling the Habitable Zone of The Nearby K Dwarf Gl 414A
• Exploring mutual information between IRIS spectral lines. II. Calculating the most probable response in all spectral windows
• Exploring the convective core of the hybrid $\delta$ Scuti-$\gamma$ Doradus star CoRoT 100866999 with asteroseismology
• Probing the Sun's inner core using solar neutrinos: a new diagnostic method
• AREPO White Dwarf merger simulations resulting in edge-lit detonation and run-away hypervelocity companion
• Understanding the progenitor formation galaxies of merging binary black holes
• Non-parametric Morphologies of Mergers in the Illustris Simulation
• Quantitative spectral analysis of the sdB star HD 188112: a helium-core white dwarf progenitor
• Chandra grating spectroscopy of embedded wind shock X-ray emission from O stars shows low plasma temperatures and significant wind absorption
• Asymmetry of line profiles of stellar oscillations measured by Kepler for ensembles of solar-like oscillators: impact on mode frequencies and dependence on effective temperature
• Resolved and Integrated Stellar Masses in the SDSS-IV/MaNGA Survey, Paper I: PCA spectral fitting & stellar mass-to-light ratio estimates
• Light bosons and photospheric solutions to the solar abundance problem
• Oxygen abundance and the N/C vs N/O relation for AFG supergiants and bright giants
• KIC 7955301: a hierarchical triple system with eclipse timing variations and an oscillating red giant
• The ionizing and heating power of ultraluminous X-ray sources under the geometrical beaming model
• Magma ocean interactions can explain JWST observations of the sub-Neptune TOI-270 d
• Annihilation of NMSSM neutralinos in the Sun and neutrino telescope limits
• An X-ray and SZ bright diffuse source toward M31: a Local Hot Bridge
• Measurement of neutrino flux from the primary proton--proton fusion process in the Sun with Borexino detector
• HD molecules at high redshift: cosmic-ray ionization rate in the diffuse interstellar medium
• Modeling the quantum interference signatures of the Ba II D2 4554 A line in the second solar spectrum
• Unveiling the interplay between the GASP jellyfish galaxy JO194 and its environment with Chandra
• Stellar population astrophysics (SPA) with the TNG -- The Arcturus Lab
• In Situ and Ex Situ Formation Models of Kepler 11 Planets
• Investigating the physical properties of galaxies in the Epoch of Reionization with MIRI/JWST spectroscopy
• Fundamental Vibrational Transitions of HCl Detected in CRL 2136
• Axion Helioscopes as Solar Thermometers
• Self-consistent Modelling of Gamma-Ray Spectra from Solar Flares with the Monte Carlo Simulation Package FLUKA
• Multiple Populations in Integrated Light Spectroscopy of Intermediate Age Clusters
• Calibrated, cosmological hydrodynamical simulations with variable IMFs II: Correlations between the IMF and global galaxy properties
• X-Ray Studies of the Abell 3158 Galaxy Cluster with eROSITA
• Pulsations in B-type supergiants with masses $M<20M_{\odot }$ before and after core helium ignition
• The GAPS programme at TNG: TBD. Studies of atmospheric FeII winds in ultra-hot Jupiters KELT-9b and KELT-20b using HARPS-N spectrograph
• Difference in chemical composition between the bright and faint red clump stars in the Milky Way bulge
• Probing Protoplanetary Disk Winds with C II Absorption
• Tentative Detection of the Circumgalactic Medium of the Isolated Low-Mass Dwarf Galaxy WLM
• Semi-analytic spectral fitting: simultaneously modelling the mass accumulation and chemical evolution in MaNGA spiral galaxies
• Kinetic tomography of the Galactic plane within 1.25 kiloparsecs from the Sun. The interstellar flows revealed by HI and CO line emission and 3D dust
• Light chemical elements in stars: mysteries and unsolved problems
• A rapidly evolving high-amplitude $\delta$ Scuti star crossing the Hertzsprung Gap
• Reanalysis of neutron-capture elements in the benchmark r-rich star CS 31082-001
• A High-Metallicity High Velocity Cloud along the MRK 421 Sight Line: A Tracer of Complex M?
• A changing wind collision
• ExoLyn: a golden mean approach to multi-species cloud modelling in atmospheric retrieval
• Evolution of the UV slope of galaxies at cosmic morning (z > 4): the properties of extremely blue galaxies
• Neutrino Backgrounds in Future Liquid Noble Element Dark Matter Direct Detection Experiments
• Down-the-barrel observations of a multiphase quasar outflow at high redshift: VLT/X-shooter spectroscopy of the proximate molecular absorber at z=2.631 towards SDSS J001514+184212
• HCT/HESP study of two carbon stars from the LAMOST survey
• Abundances of neutron-capture elements in G 24-25. A halo-population CH subgiant
• The impact of carbon and oxygen abundances on the metal-poor initial mass function
• Oscillation modes in the rapidly rotating Slowly Pulsating B-type star $\bmu$ Eridani
• The relationship between photometric and spectroscopic oscillation amplitudes from 3D stellar atmosphere simulations
• ALMA observations of molecular gas in the host galaxy of AT2018cow
• Galactic archaeology at high redshift: inferring the nature of GRB host galaxies from abundances
• Seismic Solar Models from Ledoux discriminant inversions
• Low-metallicity Young Clusters in the Outer Galaxy. III. Sh 2-127
• Quantitative spectroscopy of extreme helium stars - Model atmospheres and a non-LTE abundance analysis of BD+10${}^{\circ }$2179?
• Physical Conditions and Extension of the Coronal Line Region in IC 5063
• Excitation and charge transfer in low-energy hydrogen atom collisions with neutral carbon and nitrogen
• Interferometry of chemically peculiar stars: theoretical predictions vs. modern observing facilities
• Do the close binaries HD 22128 and HD 56495 contain Ap or Am stars?
• Interstellar Dust Close to the Sun
• Spectroscopic and asteroseismic analysis of the remarkable main-sequence A star KIC 11145123
• AGC 226178 and NGVS 3543: Two deceptive dwarfs towards Virgo
• Spatially Resolved Gas Flows Around the Milky Way
• On the [$\alpha$/Fe]-[Fe/H] relations in early-type galaxies
• A Dusty Dawn: Galactic Dust Buildup at $z\gtrsim 5$
• Tracing the formation and migration history: molecular signatures in the atmosphere of misaligned hot Jupiter WASP-94Ab using JWST NIRSpec/G395H
• The GALAH Survey: Using Galactic Archaeology to Refine our Knowledge of TESS Target Stars
• The diffuse radio emission in the high-redshift cluster PSZ2 G091.83+26.11: total intensity and polarisation analysis with Very Large Array 1-4 GHz observations
• Lithium abundance in a sample of solar-like stars
• Stellar migration in the Auriga simulations
• Rest-frame UV and optical emission line diagnostics of ionised gas properties: a test case in a star-forming knot of a lensed galaxy at z~1.7
• Evolution of rotating massive stars with new hydrodynamic wind models
• The pristine nature of SMSS 1605$-$1443 revealed by ESPRESSO
• Multiple stellar populations at less evolved stages: detection of chemical variations among main-sequence dwarfs in NGC 1978
• Orbital and atmospheric parameters of two wide O-type subdwarf binaries: BD$-$11${}^{\mathrm{o}}$162 and Feige 80
• Helioseismic and Neutrino Data Driven Reconstruction of Solar Properties
• Spectroscopy of hot Gamma Doradus and A-F hybrid Kepler candidates close to the hot border of the Delta Scuti instability strip
• Gas Accretion and Star Formation Rates
• Carbon-to-Oxygen Ratios in M dwarfs and Solar-type stars
• The Physical Parameters of Four WC-type Wolf-Rayet Stars in the Large Magellanic Cloud: Evidence of Evolution
• Chemical analysis of two extremely metal-poor stars HE 2148-2039 and HE 2155-2043
• Properties of the Hyades, the eclipsing binary HD27130, and the oscillating red giant $\epsilon$ Tau
• On the X-ray Spectral Energy Distributions of Star-Forming Galaxies: the 0.3-30 keV Spectrum of the Low-Metallicity Starburst Galaxy VV 114
• Composite Stellar Populations and Element by Element Abundances in the Milky Way Bulge and Elliptical Galaxies
• Optical Transmission Spectra of Hot-Jupiters: Effects of Scattering
• Magnetic field of the eclipsing binary UV Piscium
• Cosmic Ray-Driven Galactic Winds with Resolved ISM and Ion-Neutral Damping
• G306.3-0.9: A newly discovered young galactic supernova remnant
• Fundamental properties of solar-like oscillating stars from frequencies of minimum $\Delta \nu$: I. Model computations for solar composition
• Inflow of low-metallicity cool gas in the halo of the Andromeda galaxy
• The long X-ray tail in Zwicky 8338
• Optical tweezers in a dusty universe
• Probing the Warm-Hot Circumgalactic Medium with broad OVI and X-rays
• Modeling of multimode radially pulsating High-Amplitude Delta Scuti stars from the OGLE Galactic bulge sample
• Electron-impact excitation of diatomic hydride cations II: OH${}^{+}$ and SH${}^{+}$
• Massive stars in the Sagittarius Dwarf Irregular Galaxy
• Production of secondary particles in heavy nuclei interactions in supernova remnants
• The hot white dwarf in the peculiar binary nucleus of the planetary nebula EGB6
• The Solar Neighborhood XLVII: Comparing M Dwarf Models with Hubble Space Telescope Dynamical Masses and Spectroscopy
• Atomic Transition Probabilities for Transitions of Si I and Si II and the Silicon Abundances of Several Very Metal-Poor Stars
• Discovery of an $[Fe/H]\sim -4.8$ Star in $Gaia$ XP Spectra
• Multi-wavelength observations by XSM, Hinode and SDO of an active region. Chemical abundances and temperatures
• HD/H${}_2$ ratio in the diffuse interstellar medium
• Uncovering the physical origin of the prominent Lyman-$\alpha$ emission and absorption in GS9422 at $z=5.943$
• The Dwarf Starburst Host Galaxy of a Type Ia SN at z = 1.55 from CANDELS
• A Deep Exposure in High Resolution X-Rays Reveals the Hottest Plasma in the $\zeta$Puppis Wind
• Observations of Outflowing UV Absorbers in NGC 4051 with the Cosmic Origins Spectrograph
• The solar photospheric abundance of zirconium
• The VANDELS Survey: New constraints on the high-mass X-ray binary populations in normal star-forming galaxies at 3 < z < 5.5
• Revisiting the fundamental properties of Cepheid Polaris using detailed stellar evolution models
• Magnetic field topology and chemical spot distributions of the Ap star HD119419
• Chemical Evolution of R-process Elements in Stars (CERES): IV. An observational run-up of the third r-process peak with Hf, Os, Ir, and Pt
• Revisiting Delta Y/Delta Z from multiple main sequences in Globular Clusters: insight from nearby stars
• Stellar evolution models with entropy-calibrated mixing-length parameter: application to red giants
• Revisiting the hardening of the stellar ionizing radiation in galaxy disks
• The Trace of the CNO Cycle in the Ring Nebula NGC6888
• Photometric and spectroscopic evolution of the peculiar Type IIn SN 2012ab
• Metallicity and X-ray luminosity variations in NGC 922
• Feeding and feedback in the powerful radio galaxy 3C 120
• Empirical derivation of the metallicity evolution with time and radius using TNG50 Milky Way/Andromeda analogues
• Out-of-Transit Refracted Light in the Atmospheres of Transiting and Non-Transiting Exoplanets
• The First Billion Years project: gamma-ray bursts at z>5
• Bisectors of the HARPS Cross-Correlation-Function. The dependence on stellar atmospheric parameters
• Infrared dust arcs around the stars: I. effect of the radiation pressure
• Galaxy chemical evolution models: The role of molecular gas formation
• Sr and Ba abundance determinations: comparing machine-learning with star-by-star analyses -- High-resolution re-analysis of suspected LAMOST barium stars
• Quantitative comparison of opacities calculated using the $R$-matrix and Distorted-Wave methods: Fe XVII
• Thermal emission from bow shocks II: 3D magnetohydrodynamic models of Zeta Ophiuchi
• A Solar System Test of Self-Interacting Dark Matter
• First Light II: Emission Line Extinction, Population III Stars, and X-ray Binaries
• The Occurrence and Impact of Carbon-Oxygen Shell Mergers in Massive Stars
• Dust Extinction Law in Nearby Star-Resolved Galaxies. II. M33 Traced by Supergiants
• Detection of Dust in High-Velocity Cloud Complex C -- Enriched Gas Accreting onto the Milky Way
• Can GW231123 have a stellar origin?
• Characterizing the Rapid Hydrogen Disappearance in SN2022crv: Evidence of a Continuum between Type Ib and IIb Supernova Properties
• Properties of M31. III: Candidate Beat Cepheids from PS1 PAndromeda Data and Their Implication on Metallicity Gradient
• Binaries discovered by the MUCHFUSS project; FBS 0117+396: An sdB+dM binary with a pulsating primary
• Mid-infrared extinction and fresh silicate dust towards the Galactic Center
• Towards ultra metal-poor DLAs: linking the chemistry of the most metal-poor DLA to the first stars
• Constraining IGM enrichment and metallicity with the C IV forest correlation function
• Unravelling the Dust Attenuation Scaling Relations and their Evolution
• Explaining the ${}^{12}\text{C}{/}^{13}\text{C}$ ratio in the Galactic halo: the contribution from shell mergers in primordial massive stars
• The effect of including molecular opacities of variable composition on the evolution of intermediate-mass AGB stars
• SN 2020udy: a SN Iax with strict limits on interaction consistent with a helium-star companion
• On the dust properties of high redshift molecular clouds and the connection to the 2175 Å extinction bump
• A benchmark study of atomic models for the transition region against quiet Sun observations
• Galactic Pal-eontology: Abundance Analysis of the Disrupting Globular Cluster Palomar 5
• PARSEC V2.0: Rotating tracks and isochrones for seven addtional metallicities in the range Z=0.0001-0.03
• Combining Hipparcos and Gaia data for the study of binaries: the BINARYS tool
• Experimentally constrained ${}^{165,166}\text{Ho}(n,\gamma )$ rates and implications for the $s$ process
• Gaia-assisted selection of a quasar reddened by dust in an extremely-strong Damped Lyman-α Absorber at z=2.226
• The brightest GRB ever detected: GRB 221009A as a highly luminous event at z = 0.151
• Evolution of Dust-Obscured Star Formation and Gas to z=2.2 from HiZELS
• GalCEM I -- An Open-Source Detailed Isotopic Chemical Evolution Code
• Chemical abundances in the protoplanetary disk LV2 (Orion) - II: High dispersion VLT observations and microjet properties
• MusE GAs FLOw and Wind (MEGAFLOW) IX. The impact of gas flows on the relations between the mass, star formation rate and metallicity of galaxies
• A need to revise stellar opacities from asteroseismology of $\delta$ Scuti stars
• Li-rich and super Li-rich giants produced by element diffusion
• Combined Effects of Disk Winds and Turbulence-Driven Accretion on Planet Populations
• The Imprint of Element Abundance Patterns on Quiescent Galaxy SEDs
• Small-scale loops heated to transition region temperatures and their chromospheric signatures in the simulated solar atmosphere
• Measuring the Local ISM along the Sight Lines of the Two Voyager Spacecraft with HST/STIS
• The Extraplanar Type II Supernova ASASSN-14jb in the Nearby Edge-on Galaxy ESO 467-G051
• The compositions of the HR 8799 planets reflect accretion of both solids and metal-enriched gas
• Magellan LDSS3 emission confirmation of galaxies hosting metal-rich Lyman-alpha absorption systems
• Diverse metallicities of Fermi bubble clouds indicate dual origins in the disk and halo
• The X-ray Properties of the Cometary Blue Compact Dwarf galaxies Mrk 59 and Mrk 71
• A multispectral analysis of the northeastern shell of IC 443
• The Herbig Ae SB2 System HD 104237
• Tracking the ice mantle history in the Solar-type Protostars of NGC 1333 IRAS 4
• Cold parsec-scale gas in a zabs~0.1 sub-DLA with disparate H2 and 21-cm absorption
• Chemical abundance of LINER galaxies -- Metallicity calibrations based on SDSS-IV MaNGA
• Cold gas in hot star clusters: the wind from the red supergiant W26 in Westerlund 1
• Relative Abundance Measurements in Plumes and Interplumes
• Hubble Space Telescope Spectroscopy of a Planetary Nebula in an M31 Open Cluster: Hot-Bottom Burning at $3.4M_{\odot }$
• Relativistic electron impact ionization cross sections of carbon ions and application to an optically thin plasma
• Silicon abundance from RESIK solar flare observations
• Cloud and Haze Parameterization in Atmospheric Retrievals: Insights from Titan's Cassini Data and JWST Observations of Hot Jupiters
• The extended atmosphere and circumstellar environment of the cool evolved star VX Sagittarii as seen by MATISSE
• Selected topics in the evolution of low-mass stars
• Gemini spectroscopy of the outer disk star cluster BH176
• Chemical abundance analysis of extremely metal-poor stars in the Sextans dwarf spheroidal galaxy
• Detection of deuterated molecules, but not of lithium hydride, in the z=0.89 absorber toward PKS1830-211
• Stellar models of Betelgeuse constrained using observed surface conditions
• The peculiar chemical abundance of the transitional millisecond pulsar PSR J1023+0038 -- Li enhancement
• SO2 and OCS toward high-mass protostars: A comparative study between ice and gas
• The nature of the high Galactic latitude O-star HD93521: new results from X-ray and optical spectroscopy
• The diffusive overshooting approach on Li abundance in clusters
• Lyman continuum leaker candidates among highly ionised, low-redshift dwarf galaxies selected from HeII
• New self-consistent wind parameters fitting optical spectra of O-type stars observed with HERMES spectrograph
• Solar System chemical abundances corrected for systematics
• MIRI-LRS spectrum of a cold exoplanet around a white dwarf: water, ammonia, and methane measurements
• Metallicity estimation of MW, SMC and LMC classical Cepheids from the shape of the $V$- and $I$-band light curves
• An In-Depth Study of the Abundance Pattern in the Hot Interstellar Medium in NGC 4649
• Europium as a lodestar: diagnosis of radiogenic heat production in terrestrial exoplanets
• The infrared echo of SN2010jl and its implications for shock breakout characteristics
• Constraining SN feedback: a tug of war between reionization and the Milky Way satellites
• Pulsations of Pre-White Dwarfs with Hydrogen-dominated Atmospheres
• Detection of ${}^7$Be II in the Classical Nova V5669 Sgr (Nova Sagittarii 2015 No.3)
• Probing the hidden atomic gas in Class I jets with SOFIA
• Lithium in red giants: the roles of the He-core flash and the luminosity bump
• Jupiter-like uniform metal enrichment in a system of multiple giant exoplanets
• Multiple Stokes I inversions to infer magnetic fields in the spectral range around Cr I 5782 Å
• How many explosions does one need? -- Quantifying supernovae in globular clusters from iron abundance spreads
• Nucleosynthesis signatures of neutrino-driven winds from proto-neutron stars: a perspective from chemical evolution models
• The solar abundance problem: the effect of the turbulent kinetic flux on the solar envelope model
• The MOSDEF-LRIS Survey: Probing ISM/CGM Structure of Star-Forming Galaxies at z~2 Using Rest-UV Spectroscopy
• ALMA ACA study of the H${}_2$S/OCS ratio in low-mass protostars
• Zinc abundances of planetary nebulae
• Constraints on the properties of macroscopic transport in the Sun from combined lithium and beryllium depletion
• Spectropolarimetric Constraints on the Nature of Interstellar Grains
• Coronal Diagnostics from Narrowband Images around 30.4 nm
• Modelling chemical clocks -- Theoretical evidences of the space and time evolution of [s/alpha] in the Galactic disc with Gaia-ESO survey
• GA-NIFS: The highly overdense system BR1202-0725 at z $\sim$ 4.7. A double AGN with fast outflows plus eight companion galaxies
• First Identification and Chemical Modeling of New Thiol ($-$SH) Bearing Molecule in the Interstellar Medium: Dithioformic Acid
• VLT/UVES observations of peculiar alpha abundances in a sub-DLA at z ~ 1.8 towards the quasar B1101-26
• Evolution of the radial ISM metallicity gradient in the Milky Way disk since redshift $\approx 3$
• Chemical analysis of eight giant stars of the globular cluster NGC 6366
• Evidence of a non-conservative mass transfer in the ultra-compact X-ray source XB 1916-053
• Matter accretion in metal-poor stars down to extremely metal-poor stars and the lithium problem
• A Comprehensive Analysis of the Magnetic Standard Star HD 94660: Host of a Massive Compact Companion?
• Heavy elements unveil the non primordial origin of the giant HI ring in Leo
• Probing dark energy via galaxy cluster outskirts
• Detection of new eruptions in the Magellanic Clouds LBVs R 40 and R 110
• AlFoCS + F3D II: unexpectedly low gas-to-dust ratios in the Fornax galaxy cluster
• The energetic particle environment of a GJ 436 b-like planet
• Abundances of disk and bulge giants from hi-res optical spectra: I. O, Mg, Ca, and Ti in the Solar neighborhood and Kepler field samples
• The influence of photo-induced processes and charge transfer on carbon and oxygen in the lower solar atmosphere
• SDSS-IV MaNGA: A serendipitous observation of a potential gas accretion event
• Tidal Dissipation in Evolved Low and Intermediate Mass Stars
• Time-series Doppler images and surface differential rotation of the effectively-single rapidly-rotating K-giant KU Pegasi
• New Limits on Thermally annihilating Dark Matter from Neutrino Telescopes
• The far-ultraviolet spectra of two hot PG1159 stars
• Estimation of physical conditions in the cold phase of the ISM in the sub-DLA system at z = 2.06 in the spectrum of the quasar J2123-0050
• Study of Chemically Peculiar Stars-I : High-resolution Spectroscopy and K2 Photometry of Am Stars in the Region of M44
• Deciphering stellar metallicities in the early Universe: Case study of a young galaxy at z = 4.77 in the MUSE eXtremely Deep Field
• Models for Metal-Poor Stars with Different Initial Abundances of C, N, O, Mg, and Si. II. Application to the Colour-Magnitude Diagrams of the Globular Clusters 47 Tuc, NGC 6362, M5, M3, M55, and M92
• Models of Metal-Poor Stars with Different Initial Abundances of C, N, O, Mg, and Si. I. Bolometric Corrections Derived from New MARCS Synthetic Spectra and Their Implications for Observed Colour-Magnitude Diagrams
• Cobalt and copper abundances in 56 Galactic bulge red giants
• Comparison of Helium Abundance between ICMEs and Solar Wind near 1 AU
• The Timescales of Star Cluster Emergence: The Case of NGC 4449
• Evolution of rotating massive stars adopting a newer, self-consistent wind prescription at SMC metallicity
• Nature of the DLA towards Q0528-250: High pressure and strong UV field revealed by excitation of CI, H2 and SiII
• Herschel dust emission as a probe of starless cores mass: MCLD 123.5+24.9 of the Polaris Flare
• A high coverage view of the thermodynamics and metal abundance in the outskirts of the nearby galaxy cluster Abell 2199
• Constraining the near-core rotation of the gamma Doradus star 43 Cygni using BRITE-Constellation data
• Surface abundance and the hunt for stratification in chemically peculiar hot subdwarfs: PG 0909+276 and UVO 0512-08
• Determining the large-scale environmental dependence of gas-phase metallicity in dwarf galaxies
• Isotopic ratios in the red giant component of the recurrent nova T Coronae Borealis
• On the use of the main sequence knee (saddle) to measure globular cluster ages
• An upper limit on the spins of merging binary black holes formed through binary evolution
• A Detailed Study of Giants and Horizontal Branch Stars in M68: Atmospheric Parameters and Chemical Abundances
• Photodissociation and induced chemical asymmetries on ultra-hot gas giants. A case study of HCN on WASP-76 b
• Hot subdwarf wind models with accurate abundances I. Hydrogen dominated stars HD 49798 and BD+18${}^{\circ }$2647
• Observations of the Ultraviolet-Bright Star Y453 in the Globular Cluster M4 (NGC 6121)
• SHOTGLAS II. MUSE spectroscopy of blue horizontal branch stars in the core of $\omega$ Centauri and NGC 6752
• Optical properties of non-stoichiometric amorphous silicates with application to circumstellar dust extinction
• A Flat-Spectrum Radio Transient at 122 Mpc consistent with an Emerging Pulsar Wind Nebula
• The solar disk at high energies
• Cerium features in kilonova near-infrared spectra: implication from a chemically peculiar star
• The deep oxygen abundance in Solar System Giant Planets, with a new derivation for Saturn
• Temperature-chemistry coupling in the evolution of gas giant atmospheres driven by stellar flares
• Revisiting inelastic Cu+H collisions and the non-LTE Galactic evolution of copper
• On the Origin of Metal-poor Stars in the Solar Neighborhood
• Age and metal gradients in massive quiescent galaxies at $0.6\lesssim z\lesssim 1.0$: implications for quenching and assembly histories
• LAMA: LAMOST Medium-Resolution Spectral Analysis Pipeline
• The Pristine Inner Galaxy Survey (PIGS) IX. The largest detailed chemical analysis of very metal-poor stars in the Sagittarius dwarf galaxy
• Ariel stellar characterisation II. Chemical abundances of carbon, nitrogen, and oxygen for 181 planet-host FGK dwarf stars
• Star-formation rates of two GRB host galaxies at z~2 and a [CII] deficit observed with ALMA
• Improving 1D stellar atmosphere models with insights from multi-dimensional simulations I. 1D vs 2D stratifications and spectral comparison for O stars
• Homogeneous Stellar Atmospheric Parameters and 22 Elemental Abundances for FGK Stars Derived From LAMOST Low-resolution Spectra with DD-Payne
• Ages and metallicities of quiescent galaxies: confronting broadband ($UVJ$) colours with stellar absorption lines
• Helioseismic inference of the solar radiative opacity
• STEREO/HI and Optical Observations of the Classical Nova V5583 Sagittarii
• Modelling galaxy spectra at redshifts 0.2<z<2.3 by the [OII]/Hb and [OIII]/Hb line ratios
• NLTE spectroscopic analysis of the ${}^3$He anomaly in subluminous B-type stars
• The Chemical Evolution of Iron-Peak Elements with Hypernovae
• Understanding Physical Properties of Young M-dwarfs: NIR spectroscopic studies
• Uncertainties and biases in modelling 16 Cyg A and B
• Neutron-capture elements in dwarf galaxies III: A homogenized analysis of 13 dwarf spheroidal and ultra-faint galaxies
• The YNEV stellar evolution and oscillation code
• FLUKA Simulations of Pion Decay Gamma-radiation from Energetic Flare Ions
• An extremely hot white dwarf with a rapidly rotating K-type subgiant companion: UCAC2 46706450
• Searching for r-process-enhanced stars in the LAMOST Survey I: The Method
• Misclassified B stars in the Kepler field
• Wolf-Rayet stars in the Antennae unveiled by MUSE
• Pre-supernova feedback mechanisms drive the destruction of molecular clouds in nearby star-forming disc galaxies
• On the Mass Loading of AGN-Driven Outflows in Elliptical Galaxies and Clusters
• Chemical analysis of three barium stars: HD 51959, HD 88035, HD 121447
• AME - Asteroseismology Made Easy. Estimating stellar properties by use of scaled models
• Chemical abundance analysis of symbiotic giants. I. RW Hya and SY Mus
• A Wideband Self-Consistent Disk-Averaged Spectrum of Jupiter Near 30 GHz and Its Implications for NH${}_3$ Saturation in the Upper Troposphere
• Circumgalactic gas at its extreme: tidal gas streams around the Whale galaxy NGC 4631 explored with HST/COS
• Standard solar models: a perspective from updated solar neutrino fluxes and the gravity-mode period spacing
• Kennicutt-Schmidt relation variety and star-forming cloud fraction
• Chemical Abundance of the LINER galaxy UGC 4805 with SDSS-IV MaNGA
• Nitrogen Enrichment in Atmospheres of A- and F- Type Supergiants
• Constraining Progenitors of Observed LMXBs Using CARB Magnetic Braking
• The dynamic chromosphere: pushing the boundaries of observations and models
• The peculiar abundances of HE 1005-1439. A carbon-enhanced extremely metal-poor star contaminated with products of both s-and i-process nucleosynthesis
• Spatially Resolved X-ray Study of Supernova Remnant G306.3$-$0.9 with Unusually High Calcium Abundance
• Periodic optical variability and debris accretion in white dwarfs: a test for a causal connection
• Modelling emission lines in star forming galaxies
• The Gaia-ESO Survey: Matching Chemo-Dynamical Simulations to Observations of the Milky Way
• Probing star formation and feedback in dwarf galaxies. Integral field view of the blue compact galaxy Tololo 1937-423
• Non-Local Thermodynamic Equilibrium abundance analyses of the extreme helium stars: V652 Her and HD 144941
• Pulsar wind nebulae of runaway massive stars
• Constraints on interstellar dust models from extinction and spectro-polarimetry
• Effect of interstellar objects on metallicity of low-mass first stars formed in a cosmological model
• A Comparison of the Chemical Composition of Main Sequence and Giant Stars in the Open Cluster NCC 752
• Nitrogen Fractionation in External Galaxies
• The extent of intergalactic metal enrichment from galactic winds during the Cosmic Dawn
• Critical Metallicity of Cool Supergiant Formation. I. Effects on Stellar Mass Loss and Feedback
• Corotating Shock Waves and the Solar-Wind Source of Energetic Ion Abundances: Power Laws in A/Q
• Four Metal-poor Stars in the Sagittarius Dwarf Spheroidal Galaxy
• A Universal Relation of Dust Obscuration Across Cosmic Time
• Dark matter imprint on ${}^8$B neutrino spectrum
• Quantifying How Density Gradients and Front Curvature Affect Carbon Detonation Strength During Type Ia Supernovae
• SALT revisits DY Cen: a rapidly-evolving strontium-rich single helium star
• AGN feedback in the FR II galaxy 3C 220.1
• Physical properties of the fluorine and neutron-capture element-rich PN Jonckheere 900
• Searching for narrow absorption and emission lines in XMM-Newton spectra of gamma-ray bursts
• The Nucleosynthesis and Reaction Rates of Fluorine 19 (${}^{19}F$) in the Sun
• Chemical evolution of ultra-faint dwarf galaxies: testing the IGIMF
• Asteroseismic modelling strategies in the PLATO era I. Mean density inversions and direct treatment of the seismic information
• An X-ray Detection of Star Formation In a Highly Magnified Giant Arc
• CHEX-MATE: CLUster Multi-Probes in Three Dimensions (CLUMP-3D), I. Gas Analysis Method using X-ray and Sunyaev-Zel'dovich Effect Data
• Revisiting equilibrium condensation and rocky planet compositions: Introducing the ECCOplanets code
• Dust depletion of Ca and Ti in QSO absorption line systems
• Variations on a theme -- the puzzling behaviour of Schulte 12
• Physical Conditions of Five O VI Absorption Systems Towards PG $1522+101$
• Fluorescent Fe K line emission of gamma Cas stars I. Do gamma Cas stars host propelling neutron stars?
• Are Lithium-Rich Giants Binaries? A Radial Velocity Variability Analysis of 1,400 Giants
• Highly ionized Calcium and Argon X-ray spectra from a large solar flare
• Variability of the adiabatic parameter in monoatomic thermal and non-thermal plasmas
• HI imaging of dwarf star-forming galaxies: Masses, morphologies and gas deficiencies
• Disentangling the origin of chemical differences using GHOST
• A nearby GRB host galaxy: VLT/X-shooter observations of HG 031203
• Formation of GW230529 from Isolated Binary Evolution
• Constraining the formation of WASP-39b using JWST transit spectroscopy
• A distinct halo population revealed from 3D non-LTE magnesium abundances
• Solar chameleons: Novel channels
• The earliest phases of CNO enrichment in galaxies
• WASP-157b, a Transiting Hot Jupiter Observed with K2
• HERMES spectroscopy of normal A and Am stars
• NGTS 15b, 16b, 17b and 18b: four hot Jupiters from the Next Generation Transit Survey
• Empirical determination of atomic line parameters of the 1.5 $\mu$m spectral region
• Exoplanet accretion monitoring spectroscopic survey (ENTROPY) I. Evidence for magnetospheric accretion in the young isolated planetary-mass object 2MASS J11151597+1937266
• Explosive nucleosynthesis of a metal-deficient star as the source of a distinct odd-even effect in the solar twin HIP 11915
• Breaking the degeneracy between gas inflow and outflows with stellar metallicity: Insights on M101
• A spectroscopically confirmed Gaia-selected sample of 318 new young stars within $\sim$200 pc
• M Subdwarf Research. II. Atmospheric Parameters and Kinematics
• New X-ray detections of known Wolf-Rayet stars
• Modeling contact binaries, III. Properties of a population of close, massive binaries
• The Massive M31 Cluster G1: Detailed Chemical Abundances from Integrated Light Spectroscopy
• The hot gas mass fraction in halos. From Milky Way-like groups to massive clusters
• HD144941: The most extreme helium-strong star
• Stellar convective cores as dark matter probes
• TOI-1296b and TOI-1298b observed with TESS and SOPHIE: Two hot Saturn-mass exoplanets with different densities around metal-rich stars
• Extremely weak CO emission in IZw 18
• Detection of an extremely strong magnetic field in the double-degenerate binary merger product HD 144941
• Outside-in stellar formation in the spiral galaxy M33?
• WD 1145+017: Alternative models of the atmosphere, dust clouds, and gas rings
• Pulsation Frequencies and Modes of Giant Exoplanets
• Scenarios to explain extreme Be depletion in solar-like stars: accretion or rotation effects ?
• A holistic approach to understand Helium enrichment in Interplanetary coronal mass ejections: New insights
• X-ray response to disk evolution in two gamma-Cas stars
• Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
• Maximum Temperatures in Evolving Protoplanetary Discs and Composition of Planetary Building Blocks
• Coronae of Stars with Super Solar Elemental Abundances
• The first transition Wolf-Rayet WN/C star in M31
• Discovery of a new bona fide luminous blue variable in Norma
• Diversity of low-mass planet atmospheres in the C-H-O-N-S-Cl system with interior dissolution, nonideality, and condensation: Application to TRAPPIST-1e and sub-Neptunes
• Detection of Na and K in the atmosphere of the hot Jupiter HAT-P-1b with P200/DBSP
• Spectroscopic study of four metal-poor carbon stars from the Hamburg/ESO Survey: On confirming the low-mass nature of their companions
• SDSS-IV MaNGA: the chemical co-evolution of gas and stars in spiral galaxies
• High-resolution near-infrared spectroscopy of globular cluster and field stars toward the Galactic bulge
• SCExAO and Keck Direct Imaging Discovery of a Low-Mass Companion Around the Accelerating F5 Star HIP 5319
• The Demographics of Binary Companions to Stripped-Envelope Supernovae: Confronting Observations with Population Synthesis
• Bayesian Seismology of the Sun
• A Pristine Star-Forming Complex at z=4.19
• Red Supergiants in the JWST Era. I: Near-IR Photometric Diagnostics
• Revisiting the Red-giant Branch Hosts KOI-3886 and $\iota$ Draconis. Detailed Asteroseismic Modeling and Consolidated Stellar Parameters
• Integral field spectroscopy of M1-67. A Wolf-Rayet nebula with LBVN appearance
• The puzzle of the formation of T8 dwarf Ross 458c
• Solar center-to-limb variation in Rossiter-McLaughlin and exoplanet transmission spectroscopy
• Core-collapse supernova inside the core of a young massive star cluster: 3D MHD simulations
• M67 Blue Stragglers with High-resolution Infrared Spectroscopy
• CHEOPS and TESS view of the ultra-short period super-Earth TOI-561 b
• The 2003-4 multisite photometric campaign for the Beta Cephei and eclipsing star 16 (EN) Lacertae with an Appendix on 2 Andromedae, the variable comparison star
• Chemical abundance analysis of symbiotic giants. Metallicity and CNO abundance patterns in 14 northern S-type systems
• An investigation of the line of sight towards QSO PKS 0237-233
• A spectroscopic study of the open cluster NGC 6250
• Exploring Spatially-Resolved Metallicities, Dynamics and Outflows in Low-Mass Galaxies at $z\sim 7.6$
• A Comparative L-dwarf Sample Exploring the Interplay Between Atmospheric Assumptions and Data Properties
• An old warm Jupiter orbiting the metal-poor G-dwarf TOI-5542
• A Holistic and Probabilistic Approach to the Ground-based Data of HAT-P-19 System
• Dissociative recombination measurements of NH${}^{+}$ using an ion storage ring
• Chemical Compositions of Red Giant Stars from Habitable Zone Planet Finder Spectroscopy
• Neon, sulphur and argon abundances of planetary nebulae in the sub-solar metallicity Galactic anti-centre
• A statistical test on the reliability of the non-coevality of stars in binary systems
• Exploring the Correlation between $\mathrm{H}\alpha$-to-UV Ratio and Burstiness for Typical Star-forming Galaxies at $z\sim 2$
• The IAG Solar Flux Atlas: Telluric Correction With a Semi-Empirical Model
• Discovery of large scale shock fronts correlated with the radio halo and radio relic in the A2163 galaxy cluster
• Hubble Space Telescope ultraviolet spectroscopy of the hottest known helium-rich pre-white dwarf KPD0005+5106
• Asymmetric capture of Dirac dark matter by the Sun
• Elimination of the Blue Loops in the Evolution of Intermediate-mass Stars by the Neutrino Magnetic Moment and Large Extra Dimensions
• Hybrid-chimes: A model for radiative cooling and the abundances of ions and molecules in simulations of galaxy formation
• A metal-rich elongated structure in the core of the group NGC4325
• GK Car and GZ Nor: Two low-luminous, depleted RV Tauri stars
• Potassium detection and Lithium depletion in comets C/2011 L4 (Panstarrs) and C/1965 S1 (Ikeya-Seki)
• The SCUBA-2 Web Survey: I. Observations of CO(3-2) in hyper-luminous QSO fields
• The connection between stellar mass, age and quenching timescale in massive quiescent galaxies at $z\simeq 1$
• Why Are Some Gamma-Ray Bursts Hosted by Oxygen-rich Galaxies?
• The high-velocity clouds above the disk of the outer Milky Way: misty precipitating gas in a region roiled by stellar streams
• Mapping the ionized gas of the metal-poor HII galaxy PHL 293B with MEGARA
• Interstellar bromine abundance is consistent with cometary ices from Rosetta
• A simple scheme to implement a nonlocal turbulent convection model for the convective overshoot mixing
• Physical properties of the very young PN Hen3-1357 (Stingray Nebula) based on multiwavelength observations
• Coralie radial-velocity search for companions around evolved stars (CASCADES) III. A new Jupiter host-star: in-depth analysis of HD 29399 using TESS data
• The Impacts of Neutron-Star Structure and Base Heating on Type I X-Ray Bursts and Code Comparison
• Probing the atmosphere of HD189733b with the Na I and K I lines
• Wide Integral-Field Infrared Spectroscopy of the Bright [Fe II] Shell in the Young Supernova Remnant G11.2-0.3
• Radiation feedback in dusty clouds
• TIC-320687387 B: a long-period eclipsing M-dwarf close to the hydrogen burning limit
• On the binary helium star DY Centauri: Chemical composition and evolutionary state
• KELT-17: a chemically peculiar Am star and a hot-Jupiter planet
• Optical and NIR data and modelling of nova V5668 Sgr
• Small-scale magnetic fields of the spectroscopic binary T Tauri stars V1878 Ori and V4046 Sir
• Stellar population synthesis models with a physically varying IMF
• Goodness-of-fit test for isochrone fitting in the Gaia era. Statistical assessment of the error distribution
• Chemistry and physical properties of the born-again planetary nebula HuBi 1
• Chandra View of Magnetically Confined Wind in HD191612: Theory versus Observations
• Rotational Variation Allows for Narrow Age Spread in the Extended Main Sequence Turnoff of Massive Cluster NGC 1846
• The 300km/s stellar stream near Segue 1: Insights From high-resolution spectroscopy of its brightest star
• Signatures of the impact of flare ejected plasma on the photosphere of a sunspot light-bridge
• On asymmetric dark matter constraints from the asteroseismology of a subgiant star
• Evolutionary Constraints on the Long-period Subdwarf B Binary PG 1018-047
• Dust Buried Compact Sources in the Dwarf Galaxy NGC 4449
• Chemical Evolution of R-process Elements in Stars (CERES). III. Chemical abundances of neutron capture elements from Ba to Eu
• The giant HII region NGC 588 as a benchmark for 2D photoionisation models
• Chemical Abundances in the PN Wray16-423 in the Sagittarius Dwarf Spheroidal Galaxy: Constraining the Dust Composition
• Properties of the open cluster Tombaugh 1 from high resolution spectroscopy and uvbyCaH$\beta$ photometry
• Neutral and Ionized Hydrides in Star-forming Regions -- Observations with Herschel/HIFI
• Discovery of a young pre-intermediate polar
• The Disturbed and Globular Cluster-Rich Ultra-diffuse Galaxy UGC 9050-Dw1
• The SRG/eROSITA all-sky survey: The morphologies of clusters of galaxies I: A catalogue of morphological parameters
• Cool and Data-Driven: An Exploration of Optical Cool Dwarf Chemistry with Both Data-Driven and Physical Models
• Envelope Overshooting in Low Metallicity Intermediate- and High-mass Stars: a test with the Sagittarius Dwarf Irregular Galaxy
• Chemical evolution models: GRB host identification and cosmic dust predictions
• Ionized Gas in the First 10 Kiloparsecs of the Interstellar Galactic Halo: Metal Ion Fractions
• The O I] 1641A line as a probe of symbiotic star winds
• Chemical enrichment and host galaxies of extremely-strong intervening DLAs towards quasars
• Herschel-PACS Measurements of Nitrogen Enrichment in Nebulae around Wolf-Rayet Stars
• AstroSat Soft X-ray observations of the symbiotic recurrent nova V3890 Sgr during its 2019 outburst
• Spatially-Resolved Study of Recombining Plasma in W49B Using XMM-Newton
• A probable pre-main sequence chemically peculiar star in the open cluster Stock 16
• The luminous, massive and solar metallicity galaxy hosting the Swift gamma-ray burst, GRB 160804A at z = 0.737
• Formation of Planetary Populations III: Core Composition & Atmospheric Evaporation
• Close to the Dredge: Precise X-ray C and N Abundances in lambda Andromeda and its Precocious RGB Mixing Problem
• Possible Overionization of C II, N II, and O II Ions in the Atmospheres of Early B- and Late O-Type Stars
• Non-local thermodynamic equilibrium spectral analysis of five hot, hydrogen-deficient pre-white dwarfs
• HD 51844: An Am delta Scuti in a binary showing periastron brightening
• Detection of Metal-Rich, Cool-Warm Gas in the Outskirts of Galaxy Clusters
• Three Saturn-mass planets transiting F-type stars revealed with TESS and HARPS
• Fundamental parameters of massive stars in multiple systems: The cases of HD17505A and HD206267A
• Tracing the evolutionary pathways of dust and cold gas in high-z quiescent galaxies with SIMBA
• A binary with a $\delta$~Scuti star and an oscillating red giant: orbit and asteroseismology of KIC9773821
• Magnetic fields in gaps surrounding giant protoplanets
• The dust and gas content of carbon stars toward the Galactic Halo
• IPOPv2 online service for the generation of opacity tables
• [Fe II] 1.64 um Features of Jets and Outflows from Young Stellar Objects in the Carina Nebula
• High-ion absorption in the proximate damped Lyman-alpha system toward Q0841+129
• Probing IGM accretion onto faint Lyα emitters at z~2.8
• Stormy weather in 3C 196.1: nuclear outbursts and merger events shape the environment of the hybrid radio galaxy 3C 196.1
• Spatially-resolved UV diagnostics of AGN feedback: radiation pressure dominates in a prototypical quasar-driven superwind
• Detection of Low Metallicity Warm Plasma in a Galaxy Overdensity Environment at z ~ 0.2
• Zoom-in cosmological hydrodynamical simulation of a star-forming barred, spiral galaxy at redshift z=2
• Untangling the Sources of Abundance Dispersion in Low-Metallicity Stars
• Near infrared spectroscopy of M dwarfs. IV. A preliminary survey on the carbon isotopic ratios in M dwarfs
• Stellar Neutrino Emission Across The Mass-Metallicity Plane
• Neon Insights from Old Solar X-rays: a Plasma Temperature Dependence of the Coronal Neon Content
• Does the i-process operate at nearly solar metallicity?
• Spitzer observations of extragalactic H II regions - III. NGC 6822 and the hot star, H II region connection
• Chemodynamical study of two CEMP-no stars from the Hamburg/ESO Survey
• Bayesian inference of stellar parameters based on 1D stellar models coupled with 3D envelopes
• Barium stars as tracers of s-process nucleosynthesis in AGB stars III. Systematic deviations from the AGB models
• Rotational mixing in carbon-enhanced metal-poor stars with s-process enrichment
• Magnetic Field Geometry and Composition Variation in Slow Solar Winds: The Case of Sulfur
• Open issues in probing interiors of solar-like oscillating main sequence stars 1. From the Sun to nearly suns
• Constraints on planetary tidal dissipation from a detailed study of Kepler 91b
• NLTE Analysis of Copper Abundances in the Galactic Bulge Stars
• Halpha imaging survey of Wolf-Rayet galaxies: morphologies and star formation rates
• Scl-1013644: a CEMP-s star in the Sculptor Dwarf Spheroidal Galaxy
• Protostellar accretion in low mass metal poor stars and the cosmological lithium problem
• pySTARBURST99: The Next Generation of STARBURST99
• Excess H, Suppressed He, and the Abundances of Elements in Solar Energetic Particles
• On Carbon Nanotubes in the Interstellar Medium
• Chemical enrichment of the planet forming region as probed by accretion
• Thermohaline mixing in extremely metal-poor stars
• Investigating cannibalistic millisecond pulsar binaries using MESA: New constraints from pulsar spin and mass evolution
• VV 655 and NGC 4418: Implications of an interaction for the evolution of a LIRG
• Optical Appearance of Eccentric Tidal Disruption Events
• BRITE observations of $\nu$ Centauri and $\gamma$ Lupi, the first non-eclipsing members of the new class of nascent binaries
• Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. III. Detection of lithium in the metal-poor bulge dwarf MOA-2010-BLG-285S
• A novel approach to investigate chemical inhomogeneities in GRB host galaxies: The $Z_{\mathrm{abs}}-Z_{\mathrm{emiss}}$ relation
• Rotational Dynamics and Star Formation in the Nearby Dwarf Galaxy NGC 5238
• How do supernova remnants cool? -- I. Morphology, optical emission lines, and shocks
• Assessing the capability of a model-based stellar XUV estimation
• On the Cosmic Evolution of Fe/Mg in QSO Absorption Line Systems
• The optical properties of three type II supernovae: 2014cx, 2014cy and 2015cz
• First VLT/X-shooter spectroscopy of early-type stars outside the Local Group
• The Impact of Wind Scalings on Stellar Growth and the Baryon Cycle in Cosmological Simulations
• $i(cm)z$, a semi-analytic model for the thermodynamic properties in galaxy clusters: calibrations with mass and redshift, and implication for the hydrostatic bias
• Quantifying the Influence of Key Physical Processes on the Formation of Emission Lines Observed by IRIS: I. Non-Equilibrium Ionization and Density-Dependent Rates
• The open cluster NGC 7142: interstellar extinction, distance and age
• Properties of the ionisation glitch: I. Modelling the ionisation region
• Radial Velocity Monitoring of the Young Star Hubble 4: Disentangling Starspot Lifetimes from Orbital Motion
• Direct observation of the Broad Line Region in X-rays during the low state of NGC4051
• Ionized gas in the Scutum spiral arm as traced in [N II] and [C II]
• Consistent transport properties in multicomponent two-temperature magnetized plasmas:
• The Efficiency of Noble Gas Trapping in Astrophysical Environments
• Lightning generation in moist convective clouds and constraints on the water abundance in Jupiter
• A sub-Neptune planet around TOI-1695 discovered and characterized with SPIRou and TESS
• Observations of the Ultraviolet-Bright Star Barnard 29 in the Globular Cluster M13 (NGC 6205)
• Metal-Poor Stars Observed with the Southern African Large Telescope II. An Extended Sample
• Influence of the Void Environment on Chemical Abundances in Dwarf Galaxies and Implications for Connecting Star Formation and Halo Mass
• Mid-infrared evidence for iron-rich dust in the multi-ringed inner disk of HD 144432
• A semi-analytical perspective on massive galaxies at $z\sim 0.55$
• Where are the extremely metal-poor stars in the Milky Way and Andromeda? Expectations from TNG50
• Two's company, three's a crowd: SALT reveals the likely triple nature of the nucleus of the extreme abundance discrepancy factor planetary nebula Sp 3
• Delayed Development of Cool Plasmas in X-ray Flares from kappa1 Ceti
• Carbon-enhanced metal-poor stars in the SDSS-APOGEE database
• Evolution of Chemistry in the envelope of Hot Corinos (ECHOS). I. Extremely young sulphur chemistry in the isolated Class 0 object B335
• The Detection of Deuterated Water in the Large Magellanic Cloud with ALMA
• Chemical Abundances of the Typhon Stellar Stream
• Infall and Disk Processes - the Message from Meteorites
• HD66051, an eclipsing binary hosting a highly peculiar, HgMn-related star
• Analysis of eclipsing binaries in multiple stellar systems: the case of V1200 Centauri
• Exploring the nature of ultra-luminous X-ray sources across stellar population ages using detailed binary evolution calculations
• Tracing the 10${}^7$K Warm-Hot Intergalactic Medium with UV absorption lines
• Does the ${\nu }_{\max }$ scaling relation depend on metallicity? Insights from 3D convection simulations
• X-ray Properties of Young Early Type Galaxies: II. Abundance Ratio in the Hot ISM
• Leveraging HST with MUSE: II. Na-abundance variations in intermediate age star clusters
• Suzaku and Chandra observations of the galaxy cluster RXC J1053.7+5453 with a radio relic
• HST Detection of Extended Neutral Hydrogen in a Massive Elliptical at z = 0.4
• Constraints on galactic wind models
• A comparative study of two 47 Tuc giant stars with different s-process enrichment
• Charting Circumstellar Chemistry of Carbon-rich AGB Stars: I. ALMA 3 mm spectral surveys
• Infrared fine-structure lines at high redshift
• Absorption-based Circumgalactic Medium Line Emission Estimates
• Exploring the connection between atmosphere models and evolution models of very massive stars
• Molecular gas scaling relations for local star-forming galaxies in the low-$M_{\ast }$ regime
• Constraints on the frequency and mass content of r-process events derived from turbulent mixing in galactic disks
• Insight into the solar plage chromosphere with DKIST
• A Search for Boron in Damped Lyα Systems
• A coherent view of Li depletion and angular momentum transport to explain the Li plateau -- from Population II to Population I stars
• An X-ray view of HD166734, a massive supergiant system
• RW Aur B: a modest UX Ori type companion of the famous primary
• The GAPS Programme at TNG. XXX: Characterization of the low-density gas giant HAT-P-67 b with GIARPS
• The first spectroscopic verification of an extragalactic classical chemically peculiar star
• Efficient numerical treatment of ambipolar and Hall drift as hyperbolic system
• Damped Lyman-$\alpha$ absorbers and atomic hydrogen in galaxies: the view of the GAEA model
• Multiple components in the molecular outflow of the red supergiant NML Cyg
• Ages and Masses of Star Clusters in M33: a Multi-wavelength Study
• Solar Models with dynamic screening and early mass loss tested by helioseismic, astrophysical, and planetary constraints
• Revisiting the Chandra Observation on the Region of PSR J1809-1917: Indication of an X-ray Halo and Implication for the Origin of HESS J1809-193
• The host of the Type I SLSN 2017egm: A young, sub-solar metallicity environment in a massive spiral galaxy
• Tidal bridge and tidal dwarf candidates in the interacting system Arp194
• He abundance of Dense Circumstellar Clumps in the Cassiopeia A Supernova Remnant
• Glitches in solar-like oscillating F-type stars: Theoretical signature of the base of the convective envelope on the ratios $r_{010}$
• A Coordinated X-ray and Optical Campaign on the Nearest Massive Eclipsing Binary, Delta Ori Aa: I. Overview of the X-ray Spectrum
• Probing Velocity Dependent Self-Interacting Dark Matter with Neutrino Telescopes
• Neutrino-driven Core-collapse Supernova Yields in Galactic Chemical Evolution
• Spectropolarimetric Inversion in Four Dimensions with Deep Learning (SPIn4D): I. Overview, Magnetohydrodynamic Modeling, and Stokes Profile Synthesis
• North Polar Spur: gaseous plume(s) from star-forming regions at $\sim$3-5 kpc from Galactic Center?
• Collision-induced mass loss and mass gain on an extremely massive star. An analytical approach and a static proto-globular cluster test-case
• Probing the Dragonfish star-forming complex: the ionizing population of the young massive cluster Mercer 30
• Oxygen abundance determination of B-type stars with the OI 7771-5A lines
• Non-LTE radiation hydrodynamics in PLUTO
• Probing the physical properties of the intergalactic medium using gamma-ray bursts
• The Baltimore Oriole's Nest: Cool Winds from the Inner and Outer Parts of a Star-Forming Galaxy at z=1.3
• Detached Eclipsing Binaries in Compact Hierarchical Triples: Triple-lined systems BD+44 2258 and KIC 06525196
• A High-Resolution Spectroscopic Survey of Directly Imaged Companion Hosts: I. Determination of diagnostic stellar abundances for planet formation and composition
• Large-scale environmental dependence of the abundance ratio of nitrogen to oxygen in blue, star-forming galaxies fainter than L*
• Empirical Constraints on Core Collapse Supernova Yields using Very Metal Poor Damped Lyman Alpha Absorbers
• Breaking degeneracies in exoplanetary parameters through self-consistent atmosphere-interior modelling
• Uncertainties in the solar photospheric oxygen abundance
• EROSITA Spectro-Imaging Analysis of the Abell 3408 Galaxy Cluster
• Development of convective envelopes in massive stars: Implications for gravitational wave sources
• Assessing the processes behind planet engulfment and its imprints
• Solar polarimetry in the K I $D_2$ line: A novel possibility for a stratospheric balloon
• Seismic modelling of the rotating, slowly pulsating B-type star HD 21071
• Cosmic Ray Ionization of Low-Excitation Lines in Active Galactic Nuclei and Starburst Galaxies
• The ionizing photon production efficiency of star-forming galaxies at $z\sim 4-10$
• Multi-frequency high spectral resolution observations of HCN toward the circumstellar envelope of Y CVn
• Mode identification and seismic study of $\delta$ Scuti, the prototype of a class of pulsating stars
• Revealing Thermal Comptonization of accretion-disk photons in IC4329A with AstroSat
• Amplitude of solar gravity modes generated by penetrative plumes
• Measuring solar neutrinos over Gigayear timescales with Paleo Detectors
• Elemental gas-phase abundances of intermediate redshift type Ia supernova star-forming host galaxies
• The Relative Supernovae Contribution to the Chemical Enrichment History of Abell 1837
• Asteroseismic age estimates of RGB stars in open clusters. A statistical investigation of different estimation methods
• Stability Analysis of Strange-Modes in Hot Massive Stars with Time-Dependent Convection
• Phase resolved X-ray spectroscopy of HDE228766: Probing the wind of an extreme Of+/WNLha star
• Constraining the magnetic vector in the quiet solar photosphere and the impact of instrumental degradation
• The K2 M67 Study: A Curiously Young Star in an Eclipsing Binary in an Old Open Cluster
• The long-period massive binary HD~54662 revisited
• Prompt stellar and binary black hole mergers in tight triples: Insights from chemically homogeneous evolution
• The collimated propagation causes of astrophysical and laboratory jets
• Impact of measurement errors on the inferred stellar asteroseismic ages. Statistical models for intermediate age main sequence and red giant branch stars
• Spatially resolved measurements of the solar photospheric oxygen abundance
• Tomography of cool giant and supergiant star atmospheres III. Validation of the method on VLTI/AMBER observations of the Mira star S Ori
• Metallicity Estimation of Core-Collapse Supernova HII Regions in Galaxies within 30 Mpc
• Metallicity dependence of the CO-to-H${}_2$ and the [CI]-to-H${}_2$ conversion factors in galaxies
• Abundance analysis, spectral variability, and search for the presence of a magnetic field in the typical PGa star HD19400
• Investigating the superorbital modulations in 4U 1909+07, IGR J16418-4532 and IGR J16479-4514 with Swift XRT, BAT and NuSTAR observations
• Oxygen-rich dust production in IC 10
• Grids of stellar models including second harmonic and colours: Solar composition
• Can Galactic chemical evolution explain the oxygen isotopic variations in the Solar System?
• Etching glass in the early Universe: Luminous HF and water emission in a QSO-SMG pair at z=4.7
• Seimei KOOLS-IFU Mapping of the Gas and Dust Distributions in Galactic Planetary Nebulae: the Case of IC2165
• Kpc-scale properties of dust temperature in terms of dust mass and star formation activity
• An XMM-Newton view of the M17 nebula
• Limits on Intergalactic Dust During Reionization
• Heavy elements in old very metal-rich stars
• A high-resolution spectroscopic study of two new Na- and Al-rich field giants -- likely globular cluster escapees in the Galactic halo
• Novae: An Important Source of Lithium in the Galaxy
• Spectroscopic Determination of Stellar Parameters and Oxygen Abundances for Hyades/Field G-K Dwarfs
• Metal abundances in the MACER simulations of the hot interstellar medium
• The Aquarius Co-Moving Group is Not a Disrupted Classical Globular Cluster
• Hα Dots: Direct-Method Metal Abundances of Low-Luminosity Star-Forming Systems
• The chemical compositions of multiple stellar populations in the globular cluster NGC 2808
• FIT{\it spec}: a new algorithm for the automated fit of synthetic stellar spectra for OB stars
• Evolution of grain size distribution with enhanced abundance of small carbonaceous grains in galactic environments
• Stellar population analysis of MaNGA early-type galaxies: IMF dependence and systematic effects
• HII Region Metallicity Constraints Near the Site of the Strongly Lensed Supernova "SN Refsdal" at Redshift 1.49
• Chemical abundance analysis of symbiotic giants - II. AE Ara, BX Mon, KX TrA, and CL Sco
• Age determination of galactic B-type stars in double-lined eclipsing binaries
• Recovery of the low- and high-mass end slopes of the IMF in massive early-type galaxies using detailed elemental abundances
• Ups!... I did it again: unveiling the hidden companion in Upsilon Sagittarii, a unique binary system at a second mass transfer stage
• A novel inversion method to determine the coronal magnetic field including the impact of bound-free absorption
• A Compact High Velocity Cloud near the Magellanic Stream: Metallicity and Small-Scale Structure
• To clump or not to clump The impact of wind inhomogeneities on the optical and NIR spectroscopic analysis of massive OB stars
• Metal Enrichment in the Fermi Bubbles as a Probe of Their Origin
• Are spectral and timing correlations similar in different spectral states in black hole X-ray binaries?
• Particle acceleration, escape and non-thermal emission from core-collapse supernovae inside non-identical wind-blown bubbles
• A formation timescale of the Galactic halo from Mg isotopes in dwarf stars
• A Monte Carlo based simulation of the galactic chemical evolution of the Milky Way galaxy
• Spectroscopic study of Ba and CEMP-s stars: Mass distribution of AGB progenitors
• Observational properties of a Type Ib Supernova MASTER OT J120451.50+265946.6 in NGC 4080
• Is the post-AGB star SAO 40039 mildly H-deficient?
• The evolution of the galaxy and the birth of the solar system: The short-lived nuclides connection
• Implications of a non-universal IMF from C, N, and O abundances in very metal-poor Galactic stars and damped Lyman-alpha absorbers
• Distorted surfaces of magnetic helium-peculiar stars: An application to a Cen
• Multipole vector dark matter below the GeV-scale
• On the origin of the absorption and emission line components in the spectra of PHL 293B
• High-resolution spectroscopy of the high velocity hot post-AGB star IRAS 18379-1707 (LS 5112)
• Surrogate forward models for population inference on compact binary mergers
• Masses and ages for metal-poor stars: a pilot program combining asteroseismology and high-resolution spectroscopic follow-up of RAVE halo stars
• Chemical evolution of galaxies: emerging dust and the different gas phases in a new multiphase code
• Sulphur in the metal poor globular cluster NGC 6397
• Star formation in outer rings of S0 galaxies. IV. NGC 254 -- a double-ringed S0 with gas counter-rotation
• CO-Dark Star Formation and Black Hole Activity in 3C 368 at z = 1.131: Coeval Growth of Stellar and Supermassive Black Hole Masses
• Relevance of the small frequency separation for asteroseismic stellar age, mass, and radius. A statistical investigation for main-sequence low-mass stars
• Ice origins of OCS and chemistry of CS2-bearing ice mantles
• A Hyperactive FRB Pinpointed in an SMC-Like Satellite Host Galaxy
• Humps and bumps: The effects of shocks on the optical light curves of fundamental-mode RR Lyrae stars
• Europium, we have a problem. Modelling r-process enrichment across Local Group galaxies
• Connecting the growth of galaxies to the large-scale environment in a massive node of the Cosmic Web at z~3
• Studying the Warm Hot Intergalactic Medium in emission: a reprise
• A new view on exoplanet transits: Transit of Venus described using three-dimensional solar atmosphere Stagger-grid simulations
• Metal-enriched Pair-instability supernovae: Effects of rotation
• Elemental abundances of intermediate age open cluster NGC 3680
• X-ray Line Diagnostics of Ion Temperature at Cosmic-Ray Accelerating Collisionless Shocks
• Chandra X-ray Measurement of Gas-phase Heavy Element Abundances in the Central Parsec of the Galaxy
• RR Lyrae stars as probes of the outer Galactic halo: Chemical and kinematic analysis of a pilot sample
• Dust Emission as a Function of Stellar Population Age in the Nearby Galaxy M33
• Probing the nucleosynthetic contribution of low-metallicity, low-mass star companions of CEMP stars
• Synthetic IRIS spectra of the solar transition region: Effect of high-energy tails
• The discovery of three hot Jupiters, NGTS-23b, 24b and 25b, and updated parameters for HATS-54b from the Next Generation Transit Survey
• Fundamental effective temperature measurements for eclipsing binary stars -- II. The detached F-type eclipsing binary CPD-54 810
• Multiple origins for the DLA at $z_{\mathrm{abs}}=0.313$ toward PKS 1127$-$145 indicated by a complex dust depletion pattern of Ca, Ti, and Mn
• Revising the evolutionary stage of HD 163899: the effects of convective overshooting and rotation
• Rotating Solar Models in Agreement with Helioseismic Results and Updated Neutrino Fluxes
• SWIFT J0503.7-2819: A nearly synchronous intermediate polar below the period gap?
• Impact of asteroseismology on improving stellar ages determination
• Impact of central mixing scheme and nuclear reaction network on the extent of convective cores
• Simulations of pre-supernova feedback in spherical clouds
• Revised surface abundances of R Coronae Borealis stars
• An uncertainty principle for star formation -- V. The influence of dust extinction on star formation rate tracer lifetimes and the inferred molecular cloud lifecycle
• A hot Jupiter transiting a mid-K dwarf found in the pre-OmegaCam Transit Survey
• Search for gas accretion imprints in voids: I. Sample selection and results for NGC 428
• On the validity of the spectroscopic age indicators [Y/Mg], [Y/Al], [Y/Si], [Y/Ca], and [Y/Ti] for giant stars
• Enrichment of the Galactic disc with neutron-capture elements: Gd, Dy, and Th
• How external photo-evaporation changes the chemical composition of the inner disc
• Ultraviolet spectroscopy of the supernova Ia hypervelocity runaway white dwarf J0927-6335
• The luminosity constraint in the era of precision solar physics
• Supernovae from stellar mergers and accretors of binary mass transfer: Implications for Type IIP, 1987A-like and interacting supernovae
• Cloud-cloud collisions triggering star formation in galaxy simulations
• Modeling Dust Production, Growth, and Destruction in Reionization-Era Galaxies with the CROC Simulations: Methods and Parameter Exploration
• Real-time spectroscopy of solar pp neutrinos using Nd-150
• Modeling stellar abundance patterns resulting from the addition of earthlike planetary material
• A method for identifying metal-poor stars with Gaia BP/RP spectra
• Element Abundances of Solar Energetic Particles and the Photosphere, the Corona, and the Solar Wind
• Surface chemical composition of single WNh stars
• Resolution criteria to avoid artificial clumping in Lagrangian hydrodynamic simulations with a multi-phase interstellar medium
• Population of excited levels of Fe+, Ni+ and Cr+ in exocomets gaseous tails
• The magnetic field of the chemically peculiar star V352Peg
• High-resolution spectroscopy and abundance analysis of Delta Scuti stars near the Gamma Doradus instability strip
• The Impact of Tidal Migration of Hot Jupiters on the Rotation of Sun-like Main-sequence Stars
• HORuS transmission spectroscopy and revised planetary parameters of KELT-7b
• The Galactic Chemical Evolution of Chlorine
• Nucleosynthetic Yields from Neutron Stars Accreting in Binary Common Envelopes
• AGB subpopulations in the nearby globular cluster NGC 6397
• Adding a Suite of Chemical Abundances to the MACER Code for the Evolution of Massive Elliptical Galaxies
• B stars seen at high resolution by XMM-Newton
• Exploring the shell model of high-velocity features of Type Ia supernovae using TARDIS
• Probing the dynamical state, baryon content, and multiphase nature of galaxy clusters with bright background QSOs
• Effect of NLTE model atmospheres on photometric amplitudes and phases of early B-type pulsating stars
• Dust Extinction towards the Type Ia Supernova 2012cu in NGC 4772
• HST/WFPC2 imaging analysis and Cloudy modelling of the multiple shell planetary nebulae NGC 3242, NGC 6826 and NGC 7662
• Lambda Bootis stars in the SuperWASP survey
• Polycyclic aromatic hydrocarbons destruction in star-forming regions across 42 nearby galaxies
• Measuring titanium isotope ratios in exoplanet atmospheres
• The partial ionisation zone of heavy elements in F-stars: a study on how it correlates with rotation
• The ortho-to-para ratio of interstellar NH${}_2$: Quasi-classical trajectory calculations and new simulations
• Accelerating Galaxy Winds During the Big Bang of Starbursts
• The carbon-rich type Ic supernova 2016adj in the iconic dust lane of Centaurus A: signatures of interaction with circumstellar hydrogen?
• Gravitationally Lensed Quasar SDSS J1442+4055: Redshifts of Lensing Galaxies, Time Delay, Microlensing Variability, and Intervening Metal System at z ~ 2
• Evolution of Hen\,3-1357, the Stingray Nebula
• Exploring the Interstellar Medium Using an Asymmetric X-ray Dust Scattering Halo
• 1RXH J082623.6-505741: a new long-period cataclysmic variable with an evolved donor and a low mass transfer rate
• CD -24_17504 revisited: a new comprehensive element abundance analysis
• Infrared multiple-angle incidence resolution spectrometry for vapor-deposited amorphous water
• Helium Enhancement in the Metal Rich Red Giants of Omega Centauri
• Detailed Chemical Abundances of Star Clusters in the Large Magellanic Cloud
• Close, bright and boxy: the superluminous SN 2018hti
• The solar abundance problem and eMSTOs in clusters
• The role of environment on the star formation history of disc galaxies
• Creating and using large grids of precalculated model atmospheres for a rapid analysis of stellar spectra
• Identification of pulsational modes in rotating slowly pulsating B-type stars
• MIRACLE I.: Unveiling the Multi-Phase, Multi-Scale physical properties of the Active Galaxy NGC 424 with MIRI, MUSE, and ALMA
• SDSS-IV MaNGA: Constraints on the Conditions for Star Formation in Galaxy Discs
• Absolute rate coefficients for photorecombination of berylliumlike and boronlike silicon ions
• Vertical Convection in Turbulent Accretion Disks and Light Curves of the A0620-00 1975 Outburst
• On the chemical abundances of Miras in clusters: V1 in the metal-rich globular NGC 5927
• Metallicity of the globular cluster NGC 6388 from high resolution spectra of more than 160 giant stars
• Spatially resolved [CII]-gas conversion factor in early galaxies
• Theoretical predictions of surface light element abundances in protostellar and pre-Main Sequence phase
• High-Resolution Chemical Abundances of the Nyx Stream
• Density Conversion between 1-D and 3-D Stellar Models with 1D-MESA2HYDRO-3D
• Highly Ionized Sodium X-ray Line Emission from the Solar Corona and the Abundance of Sodium
• Anticipating the Sun's heavy-element abundance
• Improved determination of the atmospheric parameters of the pulsating sdB star Feige 48
• Modelling stars with Gaussian Process Regression: Augmenting Stellar Model Grid
• New perspectives on MASCARA-1b: A combined analysis of pre- and post-eclipse emission data using CRIRES+
• Analysis of absorption lines in the high resolution spectra of five hot post-AGB candidates
• How the cool-core population transitions from galaxy groups to massive clusters: A comparison of the largest Magneticum simulation with eROSITA, XMM-Newton, Chandra and LOFAR observations
• Non-Equilibrium Spectrum Formation Affecting Solar Irradiance
• MAGIS (Measuring Abundances of red super Giants with Infrared Spectroscopy) project I. Establishment of an abundance analysis procedure for red supergiants and its evaluation with nearby stars
• L-GALAXIES 2020: The formation and chemical evolution of stellar haloes in Milky Way Analogues and galaxy clusters
• The VLT-FLAMES Tarantula Survey XXXII. Low-luminosity late O-type stars -- classification, main physical parameters, and silicon abundances
• Exploring the mysterious high-ionization source powering [Ne V] in high-z analog SBS0335-052 E with JWST/MIRI
• Joint inference of the Milky Way star formation history and IMF from Gaia all-sky $G<13$ data
• Searching for star-forming dwarf galaxies in the Antlia cluster
• Hydride ion continuum hides absorption signatures in the NIRPS near-infrared transmission spectrum of the ultra-hot gas giant WASP-189b
• Chemical abundances and deviations from the solar S/O ratio in the gas-phase ISM of galaxies based on infrared emission lines
• Coronal Loops with Different Metallicities and Generalized RTV Scaling Laws
• CHEX-MATE: pressure profiles of 6 galaxy clusters as seen by SPT and Planck
• Structure and dynamics of the internetwork solar chromosphere: results of a small-scale dynamo simulation
• RV variable, hot post-AGB stars from the MUCHFUSS project - Classification, atmospheric parameters, formation scenarios
• Discovery of an Extremely r-process-enhanced Thin-disk Star with [Eu/H] = +0.78
• Chemical composition of stars with massive planets
• $\text{Herschel}$ Photometric Observations of $\mathrm{L}\mathrm{ITTLE}$ $\mathrm{T}\mathrm{HINGS}$ Dwarf Galaxies
• Investigating the observational properties of Type Ib supernova SN 2017iro
• Recommended conventions for reporting results from direct dark matter searches
• A puzzling non-detection of [O III] and [C II] from a $z\approx 7.7$ galaxy observed with ALMA
• Local heating due to convective overshooting and the solar modelling problem
• Accurate stellar parameters and distance to two evolved eclipsing binary systems, OGLE-BLG-ECL-123903 and OGLE-BLG-ECL-296596, towards the Galactic bulge
• Physical and chemical properties of Wolf-Rayet planetary nebulae
• A neutron star candidate in the long-period binary 56 UMa
• Probing the physical properties of the intergalactic medium using blazars
• HST STIS UV Spectroscopic Observations of the Protoplanetary Nebula Hen3-1475
• Modelling of integrated-light spectra from the optical to the near-infrared: the globular cluster G280 in M31
• NOEMA Observations of a Molecular Cloud in the low-metallicity Galaxy Kiso 5639
• Suzaku observation of Jupiter's X-rays around solar maximum
• Elemental abundances in the remnant of the ancient eruption of CK Vulpeculae
• Young stellar clumps in the interacting systems: Arp305
• CO and Fine-Structure Lines Reveal Low Metallicity in a Stellar-Mass-Rich Galaxy at z ~ 1?
• A broadband X-ray view of the NLSy1 1E 0754.6+392.8
• MUSE observations of NGC330 in the Small Magellanic Cloud. Helium abundance of bright main sequence stars
• From "universal" profiles to "universal" scaling laws in X-ray galaxy clusters
• Variability of Disk Emission in Pre-Main Sequence and related Stars. V. Occultation Events from the innermost disk region of the Herbig Ae Star HD 163296
• A partial Lyman limit system tracing intragroup gas at $z\approx 0.8$ towards HE1003+0149
• Thermal WIMPs and the Scale of New Physics: Global Fits of Dirac Dark Matter Effective Field Theories
• The XMM Cluster Survey: An independent demonstration of the fidelity of the eFEDS galaxy cluster data products and implications for future studies
• Predictions for Complex Distributions of Stellar Elemental Abundances in Low-Mass Galaxies
• Abundance of zirconium in the globular cluster 47 Tuc: a possible Zr-Na correlation?
• Chemical enrichment in groups and clusters
• The role of low-lying resonances for ${}^{10}$Be(p,$\alpha$) reaction rate and implications for the formation of the Solar System
• A binary origin for the first isolated stellar-mass black hole detected with astrometric microlensing
• Decoding the X-ray flare from MAXI J0709-159 using optical spectroscopy and multi-epoch photometry
• LOTUS: A (non-)LTE Optimization Tool for Uniform derivation of Stellar atmospheric parameters
• Galaxy clusters at z~1 imaged by ALMA with the Sunyaev-Zel'dovich effect
• A survey for variable young stars with small telescopes: VII -- Spot Properties on YSOs in IC5070
• Sub-stellar engulfment by a main sequence star: where is the lithium?
• Chasing ICM cooling and AGN feedback from the macro to the meso scales in the galaxy cluster ZwCl 235
• Evidence for a Dusty Dark Dwarf Galaxy in the Quadruple Lens MG0414+0534
• Are Milky-Way-like galaxies like the Milky Way? A view from SDSS-IV/MaNGA
• The softness diagram for MaNGA star-forming regions: diffuse ionized gas contamination or local HOLMES predominance?
• The solar photospheric silicon abundance according to CO5BOLD: Investigating line broadening, magnetic fields, and model effects
• The properties of small magnetic flux ropes inside the solar wind come from coronal holes, active regions, and quiet Sun
• Statistics of Magrathea exoplanets beyond the Main Sequence. Simulating the long-term evolution of circumbinary giant planets with TRES
• Asteroseismic investigation on KIC 10526294 to probe convective core overshoot mixing
• Long-rising Type II Supernovae in the Zwicky Transient Facility Census of the Local Universe
• The correlations between galaxy properties in different environments of the cosmic web
• A study of the capabilities for inferring atmospheric information from high-spatial-resolution simulations
• Physical conditions and element abundances in SN and GRB host galaxies at different redshifts
• Prospects on the Detection of Solar Dark Photons by the International Axion Observatory
• Vanadium oxide clusters in substellar atmospheres: A quantum chemical study
• Braving the Storm: Quantifying Disk-wide Ionized Outflows in the Large Magellanic Cloud with ULLYSES
• Observational signatures of the dust size evolution in isolated galaxy simulations
• ATMOSPHERIX: III- Estimating the C/O ratio and molecular dynamics at the limbs of WASP-76 b with SPIRou
• The clumpy torus around type II AGN as revealed by X-ray fluorescent lines
• The $\gamma$-process nucleosynthesis in core-collapse supernovae II. Effect of the explosive recipe
• Anomalously low-mass core-He-burning star in NGC 6819 as a post-common-envelope phase product
• Recovering Injected Astrophysics from the LISA Galactic Double White Dwarf Binaries
• The nature of the late B-type stars HD 67044 and HD 42035
• Stable Case BB/BC Mass Transfer to Form GW190425-like Massive Binary Neutron Star Mergers
• CHEX-MATE: the intracluster medium entropy distribution in the gravity-dominated regime
• The perils of stacking optically selected groups in eROSITA data. The Magneticum perspective
• The initial mass-remnant mass relation for core collapse supernovae
• Ariel stellar characterisation III. Fast rotators and new FGK stars in the Ariel Mission Candidate Sample
• HD 163296 and its Giant Planets: Creation of Exo-comets, Interstellar Objects and Transport of Volatile Material
• X-Shooting ULLYSES: massive stars at low metallicity: XII. The clumped winds of O-type (super)giants in the Large Magellanic Cloud
• Spatiotemporal Low FIP Abundance: A Catalyst for Coronal Condensation
• Insights on Metal Enrichment and Environmental Effect at $z\approx 5-7$ with JWST ASPIRE/EIGER and Chemical Evolution Model
• Advancing accuracy in age determinations of old-disk stars using an oscillating red giant in an eclipsing binary
• Cloudy mornings and clear evenings on a gas giant exoplanet
• The MUSE view of the Sculptor galaxy: survey overview and the planetary nebulae luminosity function
• Multi-frequency observations of PDS 70c: Radio emission mechanisms in the circum-planetary environment
• Molecular line formation in the extremely metal-poor star BD+44 493
• Bayesian Statistics as a New Tool for Spectral Analysis: I. Application for the Determination of Basic Parameters of Massive Stars
• LMC S63: a historical reappraisal of the outburst behaviour of a deeply eclipsing Magellanic symbiotic star
• Modelling the chemical evolution of molecular clouds as a function of metallicity
• SN 2022acko: a low-luminosity SNe IIP with signs of early circumstellar interaction
• The cosmological lithium problem
• Possible Evidence for the Presence of Volatiles on the Warm Super-Earth TOI-270 b
• Abundances of refractory ions in Beta Pictoris exocomets
• On the manifest link between Terzan 5 and the Galactic bulge
• Stripping of nitrogen-rich AGB ejecta from interacting dwarf irregular galaxies
• Metallicity beats sSFR: The connection between superluminous supernova host galaxy environments and the importance of metallicity for their production
• Retrieving planet formation parameters of WASP-77Ab using SimAb
• VPNEP: Detailed characterization of TESS targets around the Northern Ecliptic Pole
• Estimating the Oblateness Of Dark Matter Halos Using Neutral Hydrogen Velocity Dispersion
• Effects of dust grain size distribution on the abundances of CO and H${}_2$ in galaxy evolution
• Simulating nearly edge-on sloshing in the galaxy cluster Abell 2199
• Abundance stratification in type Ia supernovae -- VI: the peculiar slow decliner SN\,1999aa
• Spectroscopic analysis of BPS CS 22940-0009: connecting evolved helium stars
• Models for Metal-Poor Stars with Different Initial Abundances of C, N, O, Mg, and Si. III. Grids of Isochrones for $-2.5\le$ [Fe/H] $\le -0.5$ and Helium Abundances $Y=0.25$ and $0.29$ at Each Metallicity
• Kinematic signatures of impulsive supernova feedback in dwarf galaxies
• Can scallop-shell stars trap dust in their magnetic fields?
• Stellar population astrophysics (SPA) with the TNG -- The chemical content of the red supergiant population in the Perseus complex
• Investigation of the Prompt SNe Ia progenitor nature through the analysis of the chemical composition of globular clusters and circumgalactic clouds
• The Environments of CO Cores and Star Formation in the Dwarf Irregular Galaxy WLM
• Ionization of heavy elements and the adiabatic exponent in the solar plasma
• Detection of the S(1) Rotational Line of H2 toward IRC+10216: A Simultaneous Measurement of Mass-Loss Rate and CO Abundance
• Doppler shifts of spectral lines formed in the solar transition region and corona
• Core overshoot constrained by the absence of a solar convective core and some solar-like stars
• The XXL Survey: XLVIII; X-ray follow-up of distant XXL clusters: Masses, scaling relations and AGN contamination
• Optical and NIR spectroscopy of cool CEMP stars to probe the nucleosynthesis in low mass AGB binary system
• The BIG X-ray tail
• Polycyclic aromatic hydrocarbons and the ionized gas
• V772 Cas: an ellipsoidal HgMn star in an eclipsing binary
• LAMOST/HRS Spectroscopic Analysis of Two New Li-rich Giants
• Modelling the composition of a young star cluster ejecta
• Revealing Ionization Conditions of Sz 102 with Spatially Resolved [Ne III] Microjets
• A new model for the origin of very metal poor stars and their chemical composition
• The X-ray emission of the Seyfert 2 galaxy MCG-01-24-12
• Dynamic screening in solar and stellar nuclear reactions
• Unbiased Spectroscopic Study of the Cygnus Loop with LAMOST. I. Optical Properties of Emission Lines and the Global Spectrum
• The Solar Photospheric-to-Coronal Fe abundance from X-ray Fluorescence Lines
• Binary evolution leading to the formation of the very massive neutron star in the J0740+6620 binary system
• Does the structure of Pop III supernova ejecta affect the elemental abundance of extremely metal-poor stars?
• A Carbon-enhanced Lyman Limit System: Signature of the First Generation of Stars?
• A study of extragalactic planetary nebulae populations based on spectroscopy. I. Data compilation and first findings
• Non-Detection of the Putative Substellar Companion to HD 149382
• OGLE-GAL-ACEP-091 -- The First Known Multi-Mode Anomalous Cepheid
• The Slowly Varying Corona. II. The Components of F ${}_{10.7}$ and Their Use in EUV Proxies
• Atmospheric Characterization and Further Orbital Modeling of $\kappa$ And b
• A method for mapping the aliphatic hydrocarbon content of interstellar dust towards the Galactic Centre
• A Sub-Damped Ly$\alpha$ Absorber with Unusual Abundances: Evidence of Gas Recycling in a Low-Redshift Galaxy Group
• Two's a crowd? Characterising the effect of photometric contamination on the extraction of the global asteroseismic parameter ${\nu }_{\text{max}}$ in red-giant binaries
• Ultraviolet extinction properties of the 30 Dor Nebula and interpreting observations of starburst clusters
• Carbon Isotope Ratios in M10 Giants
• The LLAGN in the centre of the Galaxy
• The First Candidate Colliding-Wind Binary in M33
• The Homogenous Study of Transiting Systems (HoSTS). II. The influence of the line list on stellar parameters
• Type Ia supernovae with and without blueshifted narrow Na I D lines - how different is their structure?
• 3D photoionization models of nova V723 Cas
• Arp 202: a TDG formed in a parent's extended dark matter halo?
• Distribution of star formation rates during the rapid assembly of NGC 1399 as deduced from its globular cluster system
• Does the chemical signature of TYC 8442-1036-1 originate from a rotating massive star that died in a faint explosion?
• The nature of the light variability of magnetic Of?p star HD 191612
• Evolutionary history of four binary blue stragglers from the globular clusters ωCen, M55, 47 Tuc and NGC 6752
• Contribution of the first galaxies to the cosmic far-infrared/sub-millimeter background - I. Mean background level
• Metallicities in long GRB host galaxies at z$<$0.5 calculated by the detailed modelling of optical and infrared line ratios
• New neutrino physics and the altered shapes of solar neutrino spectra
• Refining the asteroseismic model for the young delta Scuti star HD 144277 using HARPS spectroscopy
• Effect of rotational mixing and metallicity on the hot star wind mass-loss rates
• Unravelling the Mysteries of the Leo Ring: An Absorption Line Study of an Unusual Gas Cloud
• Helium abundance in giant planets and the local interstellar medium
• High resolution spectroscopy of the relatively hydrogen-poor metal rich giants in the globular cluster Omega Centauri
• PACS and SPIRE range spectroscopy of cool, evolved stars
• A formation pathway for terrestrial planets with moderate water content involving atmospheric-volatile recycling
• Ionized Carbon in Galaxies: The [C II] 158 $\mu$m Line as a Total Molecular Gas Mass Tracer Revisited
• High-precision photometric and high-resolution spectroscopic characterisation of HD 180347
• An extended low-density atmosphere around the Jupiter-sized planet WASP-193 b
• Testing a non-local 1-equation turbulent convection model: A solar model
• The effects of individual metal contents on isochrones for C, N, O, Na, Mg, Al, Si, and Fe
• Hot Gas Outflow Properties of the Starburst Galaxy NGC 4945
• A negative stellar mass$-$gaseous metallicity gradient relation of dwarf galaxies modulated by stellar feedback
• Transitions in magnetic behavior at the substellar boundary
• A chemodynamical analysis of bright metal-poor stars from the HESP-GOMPA survey -- Indications of a non-prevailing site for light r-process elements
• Newly discovered Ca II absorbers in the early universe: statistics, element abundances and dust
• X-ray irradiation of the stellar wind in HMXBs with B supergiants: Implications for ULXs
• Very massive stars at low metallicity: evolution, synthetic spectroscopy, and impact on the integrated light of starbursts
• Abundance Discrepancy Factors in high density planetary nebulae
• Role of magnetic arcades in explaining the puzzle of the gamma-ray emission from the solar disk
• The absorption and emission spectrum of the magnetic Herbig Ae star HD 190073
• Spectroscopic survey of faint planetary-nebula nuclei III. A [WC] central star and two new PG1159 nuclei
• SN 2023zaw: an ultra-stripped, nickel-poor supernova from a low-mass progenitor
• ALMA Observations of the Molecular Clouds in NGC 625
• Computation of atomic astrophysical opacities
• Influence of galactic arm scale dynamics on the molecular composition of the cold and dense ISM III. Elemental depletion and shortcomings of the current physico-chemical models
• Formation and Thermodynamic Evolution of plasmoids in active region jets
• Surface density: a new parameter in the fundamental metallicity relation of star-forming galaxies
• Ultraviolet Spectral Synthesis of Iota Herculis
• The escape of hydrogen-rich atmosphere of exoplanet: Mass loss rates and the absorptions of stellar Lyman $\alpha$
• $\text{globin}$: A spectropolarimetric inversion code for the coupled inference of atomic line parameters
• Characterising the AGB bump and its potential to constrain mixing processes in stellar interiors
• Theoretical X-ray light curves of young SNe II: the example of SN 2013ej
• On the Contribution of Very Massive Stars to the Sulfur Abundance in Star-Forming Galaxies: the Role of PISN
• Soft X-ray absorption excess in gamma-ray burst afterglow spectra: Absorption by turbulent ISM
• The Differential Assembly History of the Centers and Outskirts of Main Sequence Galaxies at $z\sim 2.3$
• Carbon-rich Sub-Neptune Interiors Are Compatible with JWST Observations
• Convective Mixing: The Formation Channel of Li-rich Giants
• Understanding the rotational variability of K2 targets. HgMn star KIC 250152017 and blue horizontal branch star KIC 249660366
• The oldest stars with low neutron-capture element abundances and origins in ancient dwarf galaxies
• Spectroscopic Determination of Capella's Photospheric Abundances: Possible Influence of Stellar Activity
• AstroSat view of spectral transition in the changing-look active galaxy NGC1566 during the declining phase of the 2018 outburst
• s-process Enriched Evolved Binaries in the Galaxy and the Magellanic Clouds
• Constraints on the gas-phase C/O ratio of DR Tau's outer disk from CS, SO, and C${}_2$H observations
• The C/N ratio from FUV spectroscopy as a constraint upon the past evolution of HS0218+3229
• Ionization chemistry in the inner disc: a combined treatment of ionic and thermionic emission and arbitrary grain size distributions
• A public grid of radiative transfer simulations for Lyman-alpha and metal lines in idealised galactic outflows
• Massive stars exploding in a He-rich circumstellar medium $-$ X. Flash spectral features in the Type Ibn SN 2019cj and observations of SN 2018jmt
• New nickel opacities and their impact on stellar models
• Substructure analysis of the RXCJ0232.2-4420 galaxy cluster
• Impact of newly measured 26Al(n, p)26Mg and 26Al(n, α)23Na reaction rates on the nucleosynthesis of 26Al in stars
• Angular momentum and lithium transport from main sequence to sub-giant and red giant low-mass stars
• High-resolution SOFIA/EXES Spectroscopy of Water Absorption Lines in the Massive Young Binary W3 IRS 5
• Two Channels of Metal-Rich Compact Stellar System Formation: Starbursts under High Ram Pressure versus Tidal Stripping
• Unveiling Multiple Physical Processes on a Cluster Galaxy at z=0.3 Using JWST
• Reconciling the Results of the z~2 MOSDEF and KBSS-MOSFIRE Surveys
• Chemical Abundances of a Sample of Oxygen-dominated Galaxies
• NLTE 1.5D Modeling of Red Giant Stars
• To Grow Old and Peculiar: A Survey of Anomalous Variable Stars in M80 and Age Determination using K2 and Gaia
• On the nature of the core of $\alpha$ Centauri A: the impact of the metallicity mixture
• Mean opacities of a strongly magnetized high temperature plasma
• Computational Estimation of the Binding Energies of POx and HPOx (x=2,3) Species
• Mapping the aliphatic hydrocarbon content of interstellar dust in the Galactic plane
• Natal kicks of compact objects
• Solar neutrino with Borexino: results and perspectives
• R-matrix electron-impact excitation data for the H- and He-like ions with Z=6-30
• WASP 0639-32: a new F-type subgiant/K-type main-sequence detached eclipsing binary from the WASP project
• Connecting planet formation and astrochemistry: C/O and N/O of warm giant planets and Jupiter-analogs
• Stellar model calibrations with the Ai Phe binary system. Open questions about the robustness of the fit
• PRUSSIC II -- ALMA imaging of dense-gas tracers in SDP.81: Evidence for low mechanical heating and a sub-solar metallicity in a z=3.04 dusty galaxy
• The warm-hot intergalactic medium in inter-cluster filaments -- A forecast for HUBS observations based on eRASS1 superclusters
• Solar Flare Ion Temperatures
• Detection of high-degree prograde sectoral mode sequences in the A-star KIC 8054146?
• The Sun: Light Dark Matter and Sterile Neutrinos
• Multi-fluid Simulation of Solar Chromospheric Turbulence and Heating Due to the Thermal Farley-Buneman Instability
• Observations of Ly$\alpha$ Emitters at High Redshift
• The properties and environment of very young galaxies in the local Universe
• Under the magnifying glass: A combined 3D model applied to cloudy warm Saturn type exoplanets around M-dwarfs
• The [C II] line emission as an interstellar medium probe in the MARIGOLD galaxies
• Comprehensive spectroscopic and photometric study of pulsating eclipsing binary star AI Hya
• Potential contributions of Pop III and intermediate-mass Pop II stars to cosmic chemical enrichment
• Stellar abundances of beryllium and CUBES
• The interstellar medium in Andromeda's dwarf spheroidal galaxies: II. Multi-phase gas content and ISM conditions
• First detection of [N II] 205 micrometer absorption in interstellar gas
• On possible explanations of pulsations in Maia stars
• Determining the evolutionary stage of the delta Scuti star HIP 80088 with asteroseismology
• COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
• Metallicity-PAH Relation of MIR-selected Star-forming Galaxies in AKARI North Ecliptic Pole-wide Survey
• Water Ice Deposition and Growth in Molecular Clouds
• Chemical compositions of giants in the Hyades And Sirius superclusters
• TESS Asteroseismic Analysis of HD 76920: The Giant Star Hosting An Extremely Eccentric Exoplanet
• Inner and outer star forming regions over the disks of spiral galaxies. II. A comparative of physical properties and evolutionary stages
• Spectroscopic determination of C, N, and O abundances of solar-analog stars based on the lines of hydride molecules
• A Grid of Synthetic Spectra for Subdwarfs: Non-LTE line-blanketed atmosphere models
• Computation of the transmitted and polarized scattered fluxes by the exoplanet HD 189733b in X-rays
• Advancements in solar neutrino physics
• Confirmation of two magnetic cataclysmic variables as polars: 1RXS J174320.1-042953 and YY Sex
• Multiverse Predictions for Habitability: Element Abundances
• A Tale of Three Galaxies: Deciphering the Infrared Emission of the Spectroscopically Anomalous Galaxies IRAS F10398+1455, IRAS F21013-0739 and SDSS J0808+3948
• Stellar Populations in type Ia supernova host galaxies at intermediate-high redshift: Star formation and metallicity enrichment histories
• Is planetary inward migration responsible for GJ 504's fast rotation and bright X-ray luminosity? New constraints from eROSITA
• CII*/CII ratio in high-redshift DLAs: ISM phase separation drives the observed bimodality of [CII] cooling rates
• Modeling of two CoRoT solar analogues constrained by seismic and spectroscopic analysis
• High-resolution spectroscopy of the extremely iron-poor post-AGB star CC Lyr
• Inference for Stellar Opacities from Seismic Studies of the Hybrid $\beta$ Cep/SPB pulsators
• Understanding star formation and feedback in small galaxies. The case of the blue compact dwarf Mrk 900
• Chemodynamics of metal-poor wide binaries in the Galactic halo: Association with the Sequoia event
• Common envelope jets supernova with thermonuclear outburst progenitor for the enigmatic supernova remnant W49B
• Validating Stellar Abundance Measurements from Multi-Resolution Spectroscopy
• The EBLM project -- XIV. TESS light curves for eclipsing binaries with very low mass companions
• Phase-resolved X-ray spectroscopy and spectral energy distribution of the X-ray soft polar RS Caeli
• Gemini-GRACES high-quality spectra of Kepler evolved stars with transiting planets I. Detailed characterization of multi-planet systems Kepler-278 and Kepler-391
• New Constraints on Sodium Production in Globular Clusters From the ${}^{23}$Na${(}^3$He$,\text{d}{)}^{24}$Mg Reaction
• The Ages of Optically Bright Sub-Clusters in the Serpens Star-Forming Region
• Uncovering the ultimate planet impostor. An eclipsing brown dwarf in a hierarchical triple with two evolved stars
• Measuring Dust Attenuation Curves of SINGS/KINGFISH Galaxies Using Swift/UVOT Photometry
• Effect of planet ingestion on low-mass stars evolution: the case of 2MASS J08095427--4721419 star in the Gamma Velorum cluster
• Circumstellar CO J = 3-2 detected around the evolving metal-poor ([Fe/H] ~ -1.15 dex) AGB star RU Vulpeculae
• Exploring Damped Lyman-$\alpha$ System Host Galaxies using Gamma-ray Bursts
• Abundance analysis of s-process enhanced barium stars
• Molecular gas in super spiral galaxies
• Detections of [C II] 158 $\mu$m and [O III] 88 $\mu$m in a Local Lyman Continuum Emitter, Mrk 54, and its Implications to High-redshift ALMA Studies
• Discovery of a pair of very metal-poor stars enriched in neutron-capture elements: The proto-disk r-II star BPS CS 29529-0089 and the Gaia-Sausage-Enceladus r-I star TYC 9219-2422-1
• Star forming brightest cluster galaxies at $z\sim 0.4$ in KiDS. Further studies of cold gas and stellar properties
• Slow Magnetoacoustic Oscillations in Stellar Coronal Loops
• The Origin of the X-ray Emission from the High-velocity Cloud MS30.7-81.4-118
• Stellar Population Astrophysics (SPA) with the TNG. alpha-elements, lithium, sodium and aluminum in 16 open clusters
• Metallicity in the merger Seyfert galaxy NGC 6240
• Ages for exoplanet host stars
• Calibrating chemical mixing induced by internal gravity waves based on hydrodynamical simulations; The chemical evolution of OB-type stars
• Atmospheric Escape by Magnetically Driven Wind from Gaseous Planets II --Effects of Magnetic Diffusion--
• New insight into the massive eccentric binary HD 165052: self-consistent orbital solution, apsidal motion, and fundamental parameters
• From order to chaos: the blurred out metallicity gradient of the Gaia-Enceladus/Sausage progenitor
• Combining Astrometry and Elemental Abundances: The Case of the Candidate Pre-Gaia Halo Moving Groups G03-37, G18-39, and G21-22
• Evidence for a hot galactic halo around the Andromeda Galaxy using fast radio bursts along two sightlines
• Asteroseismology of the young open cluster NGC 2516 II. Constraining cluster age using gravity-mode pulsators
• Tighter constraints on the atmosphere of GJ 436 b from combined high-resolution CARMENES and CRIRES${}^{+}$ observations
• A Semi-Analytical Computation of the Theoretical Uncertainties of the Solar Neutrino Flux
• MUSE spectroscopic observations of the Young Massive Cluster NGC1850
• Major mergers with small galaxies - the discovery of a Magellanic-type galaxy at z=0.12
• Be, V and Cu in the halo star CS 31082-001 from near-UV spectroscopy
• The Noctua Suite of Simulations -- The Difficulty of Growing Massive Black Holes in Low-Mass Dwarf Galaxies
• Age and convective core overshooting calibrations in CPD-54 810 binary system. Statistical investigation on the solution robustness
• A Detailed Investigation of HD 209458 b HST & JWST Transmission Spectra with SANSAR
• Physical cool-core condensation radius in massive galaxy clusters
• Helium abundance (and $H_0$) in X-COP galaxy clusters
• Neutron-Capture Element Signatures in Globular Clusters: Insights from the Gaia-ESO Survey
• Changing disc compositions via internal photoevaporation II: M dwarf systems
• Coralie radial velocity search for companions around evolved stars (CASCADES) II. Seismic masses for three red giants orbited by long-period massive planets
• Asteroseismology of the G8 subgiant beta Aquilae with SONG-Tenerife, SONG-Australia and TESS
• VLT/MUSE and ATCA observations of the host galaxy of the short GRB 080905A at z=0.122
• KELT-9 and its ultra-hot Jupiter: stellar parameters, composition, and planetary pollution
• Uncertainties in models of stellar structure and evolution
• Detection of cesium in the atmosphere of the hot He-rich white dwarf HD 149499B
• Modelling of the scandium abundance evolution in AmFm stars
• Duration and properties of the embedded phase of star formation in 37 nearby galaxies from PHANGS-JWST
• Element Abundances and Source Plasma Temperatures of Solar Energetic Particles
• Modelling $\delta$ Scuti pulsations: A new grid of p, g, and f modes across pre-main-sequence to post-main-sequence evolution
• Stellar Population Astrophysics (SPA) with the TNG: NLTE atmospheric parameters and abundances of giant stars in 33 Open Clusters
• The Impact of Inelastic Collisions with Hydrogen on NLTE Copper Abundances in Metal-Poor Stars
• PRODIGE VI -- Envelope to Disk with NOEMA: VI. The Missing Sulfur Problem
• Direct determination of oxygen abundances in line emitting star-forming galaxies at intermediate redshift
• Fluctuations of the intergalactic ionization field at redshift z ~ 2
• Pushing the boundaries of asteroseismic individual frequency modelling: unveiling two evolved very-low metallicity red giants
• Numerical integral of resistance coefficients in diffusion
• A comprehensive study of the relations between the properties of planetary systems and the chemical compositions of their host stars
• Disc fragmentation and oligarchic growth of protostellar systems in low-metallicity gas clouds
• First models of s process in AGB stars of solar metallicity for the stellar evolutionary code ATON with a novel stable explicit numerical solver
• An Actinide-boost Star Discovered in the Gaia-Sausage-Enceladus
• The Warm Gas in the MW: the Kinematical Model of C IV and its Connection with Si IV
• Influence of the C/O ratio on titanium and vanadium oxides in protoplanetary disks
• The New Astronomical Frontier of Interstellar Objects
• Canonical X-Ray Fluorescence Line Intensities as Column Density Indicators
• Impact of Newly Measured Nuclear Reaction Rates on ${}^{26}$Al Ejected Yields from Massive Stars
• Geoastronomy: Rocky planets as the Lavosier-Lomonosov Bridge from the non-living to the living world
• 3xmm j181923.7$-$170616: an x-ray binary with a 408s pulsar
• Accelerated growth of seed black holes by dust in the early universe
• Multiple populations within globular clusters in Early-type galaxies Exploring their effect on stellar initial mass function estimates
• Metals at the surface of last scatter
• Observing EAGLE galaxies with JWST: predictions for Milky Way progenitors and their building blocks
• Metal distribution in the ICM - a comprehensive numerical study of twelve galaxy clusters
• First detection of HS2 in a cold dark cloud
• The SPACE Program. I. The featureless spectrum of HD 86226 c challenges sub-Neptune atmosphere trends
• Baryon Pasting the Uchuu Lightcone Simulation
• Abundances in Galactic Bulge planetary nebulae from optical, ultraviolet and infrared observations
• Probing cosmic chemical enrichment with next-generation gravitational-wave observatories
• Hot-star wind models with magnetically split line blanketing
• Tracing the origin of moving groups I. The γ Leo moving group with high resolution spectra from the Subaru Telescope
• XMM-Newton RGS observations of the Cat's Eye Nebula
• Organic matter in interstellar dust lost at the approach to the heliosphere: Exothermic chemical reactions of free radicals ignited by the Sun
• The Solar X-ray Limb
• Chemical composition of the outer halo globular cluster Palomar 15
• XMM-Newton observations of the X-ray soft polar QS Telescopii
• Discovery of a Metal-Poor Red Giant Star with the Highest Ultra-Lithium Enhancement
• A revisit to the enigmatic variable star 21 Comae
• Carbon Abundance Inhomogeneities and Deep Mixing Rates in Galactic Globular Clusters
• Exploring the convective core of the high-amplitude $\delta$ Scuti star TIC 120857354 with asteroseismology
• An impact-free mechanism to deliver water to terrestrial planets and exoplanets
• The ALPINE-ALMA [CII] Survey: Unveiling the baryon evolution in the ISM of $z\sim 5$ star-forming galaxies
• Evolved Eclipsing Binaries and the Age of the Open Cluster NGC 752
• Spectral analysis of the barium central star of the planetary nebula Hen 2-39
• Does radiative feedback make faint z>6 galaxies look small?
• s-process Enriched Post-AGB Star J003643.94-723722.1 in the SMC with an Extreme C/O Ratio and the First Precise Detection of Lead
• Solar-Metallicity Gas in the Extended Halo of a Galaxy at $z\sim 0.12$
• Modified Gravity (MOG) and its test on galaxy clusters
• Mapping the Active Galactic Nucleus Effects on the Stellar and Gas Properties of NGC 5806
• Precise Age for the Binary Star System 12 Com in the Coma Berenices Cluster
• Triangulum-Andromeda overdensity: a region with a complex stellar population
• The true nature of HE0057-5959, the most metal-poor Li-rich star
• Detection and characterization of detached tidal dwarf galaxies
• A super-Earth and a mini-Neptune around Kepler-59
• XMM-Newton --NuSTAR monitoring campaign of the Seyfert 1 galaxy IC 4329A
• Generic energy transport solutions to the solar abundance problem -- a hint of new physics
• Rotational modulation and single g-mode pulsation in the B9pSi star HD174356?
• An Intercomparison Study of Two Proximate Damped Ly$\alpha$ Systems with Residual Flux upon the Ly$\alpha$ Absorption Trough toward Quasars
• A Sub-solar Fe/O, logT~7.5 Gas Component Permeating the Milky Way's CGM
• The Stellar Population and Orbit of the Galactic Globular Cluster Palomar 3
• Weighing stars from birth to death: mass determination methods across the HRD
• The SRG/eROSITA All-Sky Survey: Large-scale view of the Centaurus cluster
• Spatially resolving the chemical composition of the planet building blocks
• Metal line emission around z<1 galaxies
• Recent Advances in Modeling Stellar Interiors
• CO radial gradients in the bulge of M31
• Benchmarking the effective temperature scale of red giant branch stellar models: the case of the metal-poor halo giant HD 122563
• First result of the experimental search for the 9.4 keV solar axion reactions with Kr-83 in the copper proportional counter
• Understanding the thermal and magnetic properties of a X-class flare in the low solar atmosphere
• Spectropolarimetric follow-up of 8 rapidly rotating, X-ray bright FK Comae candidates
• Hunt for Starspots in HARPS Spectra of G and K Stars
• Detection of the actinide Th in an r-process-enhanced star with accretion origin
• Growth and disruption in the Lyra complex
• Origin of Black Hole Spin in Lower-Mass-Gap Black Hole-Neutron Star Binaries
• Significant H I and Metal Differences around the z = 0.83 Lens Galaxy Towards the Doubly Lensed Quasar SBS 0909+532
• Pair Lines of Sight Observations of Multiphase Gas Bearing O VI in a Galaxy Environment
• The Cool Giant HD 77361 - A Super Li-Rich Star
• Unveiling the evolutionary state of three B supergiant stars: PU Gem, $\epsilon$ CMa and $\eta$ CMa
• A survey of extremely metal-poor gas at cosmic noon: evidence of elevated [O/Fe]
• Ionization degree and magnetic diffusivity in star-forming clouds with different metallicities
• Asteroseismology of double-mode radial $\delta$ Scuti stars: AE Ursae Majoris and RV Arietis
• On the origin of the $10^7$ K hot emitting gas in the Circumgalactic medium of the Milky Way
• Ultra-faint [CII] emission in a redshift = 2 gravitationally-lensed metal-poor dwarf galaxy
• Stellar Migration and Chemical Enrichment in the Milky Way Disc: A Hybrid Model
• X-Shooting ULLYSES: Massive Stars at Low Metallicity X. Physical Parameters and Feedback of Massive Stars in the LMC N11 B Star-Forming Region
• Refined Telluric Absorption Correction for Low-Resolution Ground-Based Spectroscopy: Resolution and Radial Velocity Effects in the O2 A-Band for Exoplanets and K I Emission Lines
• BD+30${}^{\circ }$549: young helium-weak silicon star in NGC 1333 star-forming region
• Chemical abundances of the high-latitude Herbig Ae Star PDS2
• Upper Limits on the Mass of Cool Gas in the Circumgalactic Medium of Dwarf Galaxies
• Asteroseismology of the heartbeat star KIC 5006817
• [Fe II] 1.64 um Imaging Observations of the Outflow Features around Ultracompact H II Regions in the 1st Galactic Quadrant
• CO emissions from optically selected galaxies at z~0.1-0.2: Tight anti-correlation between molecular gas fraction and 4000 Åbreak strength
• Assessing model-based carbon and oxygen abundance derivation from ultraviolet emission lines in AGNs
• Probing the origins. I. Generalised Additive Model inference of birth radii for Milky Way stars in the solar vicinity
• Representation of s-process abundances for comparison to data from bulk meteorites
• Diving into the magnetosphere of the Of?p star HD108
• Double progenitor origin of the S-star cluster
• The CoRoT target HD49933: a possible seismic signature of heavy elements ionization in the deep convective zone
• The survey of planetary nebulae in Andromeda (M31) VII. Predictions of a major merger simulation model compared with chemodynamical data of the disc and inner halo substructures
• Asteroseismic analysis of eight solar-like oscillating evolved stars in the open cluster NGC 6811
• Looking for nebular He II emission south of the multiple-massive star system, HD 5980
• SN 2019hcc: A Type II Supernova Displaying Early O II Lines
• The GALAH survey: Improving chemical abundances using star clusters
• Are Am stars and hot-Jupiter planets related?
• Mixing due to internal gravity waves can explain the CNO surface abundances of B-type detached eclipsing binaries and single stars
• Binary stellar evolution yields in galactic chemical evolution calculations
• The evolutionary and asteroseismic imprints of mass accretion. The 10 M${}_{\odot }$ $\beta$ Cep case study
• Migration and Evolution of giant ExoPlanets (MEEP) II: Super-Jupiters and Lithium-rich Host Stars
• Three-dimensional modeling of ionized gas. II. Spectral energy distributions of massive and very massive stars in stationary and time-dependent modeling of the ionization of metals in HII regions
• Exploring the hardness of the ionizing radiation with the infrared softness diagram. II. Bimodal distributions in both the ionizing continuum slope and the excitation in active galactic nuclei
• Solar Neutrino Detection Sensitivity in DARWIN via Electron Scattering
• A [CII]-158-micron Survey of DLA galaxies at z~4: Observations of Dense and Metal-Enriched Neutral Gas within the Circumgalactic Medium of Star-Forming Galaxies
• X-ray Properties of Low-Mass Pre-Main Sequence Stars in the Orion Trapezium Cluster
• Discovery of resonating integration modes in triple-mode high-amplitude $\delta$ Scuti stars: A new evolutionary phase indicator
• Quasar radiation transforms the gas in a merging companion galaxy
• Wind shear and the role of eddy vapor transport in driving water convection on Jupiter
• Detection of pure warm-hot intergalactic medium emission from a $7.2$ Mpc long filament in the Shapley supercluster using X-ray spectroscopy
• A new pathway to SO${}_2$: Revealing the NUV driven sulfur chemistry in hot gas giants
• The robustness of inferred envelope and core rotation rates of red-giant stars from asteroseismology
• Cocoon shock, X-ray cavities and extended Inverse Compton emission in Hercules A: clues from Chandra observations
• How disc initial conditions sculpt the atmospheric composition of giant planets
• Yields from massive stars in binaries. Chemical evolution of the Milky Way disk
• A theoretical framework for BL Her stars III. A case study: Robust light curve optimisation in the LMC
• An Updated Line List for Spectroscopic Investigation of G Stars II: Refined Solar Abundances via Extended Wavelength Coverage to 10 000 Å
• Kinetic and photochemical disequilibrium in the potentially carbon-rich atmosphere of the warm-Jupiter WASP-69b
• KBSS-InCLOSE I: Design and First Results from the Inner CGM of QSO Line Of Sight Emitting Galaxies at z~2-3
• Multi-wavelength spectroscopic analysis of the ULX Holmberg II X-1 and its nebula suggests the presence of a heavy black hole accreting from a B-type donor
• Neutral carbon in diffuse interstellar medium: abundance matching with H2 for DLAs at high redshifts
• Detecting gravity modes in the solar ${}^{8}B$ neutrino flux
• A detached double X-ray tail in the merging galaxy cluster Z8338 with a large double tail
• Experimental Investigation of the Photochemical Production of Hydrocarbons in Warm Gas Giant Exoplanet Atmospheres
• The multi-zone chemical evolution of the Galactic bulge: predicting abundances for different radial zones
• Uncertainties in asteroseismic grid-based estimates of the ages of halo stars
• A quest for sulfur-bearing refractory species. Identification of CaS in the interstellar medium
• Neutron-capture elements in NGC 6752 multiple populations
• Collisional- and photo-excitations of Ca IV including strong 3.2 $\mu$m emission line
• Complex asteroseismology of the hybrid B-type pulsator $\gamma$ Pegasi: a test of stellar opacities
• Proto-planetary disk composition-dependent element volatility in the context of rocky planet formation
• The solar sulphur abundance in view of large-scale atomic structure calculations and 3D non-LTE models
• Unravelling optical and X-ray properties of the disc-dominated intermediate polar IGR J15094-6649
• Assessing stellar yields in Galaxy chemical evolution: observational stellar abundance patterns
• Arcsecond-Scale X-ray Imaging and Spectroscopy of SS 433 with Chandra HETG
• How does the chemical composition of solids influence the formation of planetesimals?
• The quasar luminosity function at $z\sim 5$ via deep learning and Bayesian information criterion
• Asteroseismic Investigations of the Binary System HD176465
• The planetary-mass-limit VLT/SINFONI library: Spectral extraction and atmospheric characterization via forward modeling
• Revisiting the Perseus Cluster I: Resolving the Si/S/Ar/Ca ratios by Stellar Convection
• Parametric models of core-helium-burning stars: structural glitches near the core
• $L$-band Spectra of Young Brown Dwarfs
• Constraints on stellar parameters of the SPB star HD182255 from complex asteroseismology
• First release of PLATO consortium stellar limb-darkening coefficients
• Modelling the selection of galaxy groups with end to end simulations
• X-ray confirmation of the intermediate polar IGR J16547-1916
• The Milky Way in context: The formation of galactic discs and chemical sequences from a cosmological perspective
• NLTE atmospheric modelling of the ultra-hot Jupiter WASP-178b and comparison with UV and optical observations
• Extremely strong DLAs at high redshift: Gas cooling and H${}_2$ formation
• Modeling the progenitors of low-mass post-accretion binaries
• Abundance of zinc in the red giants of Galactic globular cluster 47 Tucanae
• M dwarfs and the fraction of high carbon-to-oxygen stars in the solar neighbourhood
• An extremely metal-poor Lyman $\alpha$ emitter candidate at $z=6$ revealed through absorption spectroscopy
• The impact of wind mass loss on nucleosynthesis and yields of very massive stars at low metallicity
• Discovery of a damped Ly$\alpha$ absorber originating in a spectacular interacting dwarf galaxy pair at $z=0.026$
• An on-the-fly line-driven-wind iterative mass-loss estimator (LIME) for hot, massive stars of arbitrary chemical compositions
• The nature of the Cygnus extreme B-supergiant 2MASS J20395358+4222505
• Testing Model Atmospheres for Young Very Low Mass Stars and Brown Dwarfs in the Infrared: Evidence for Significantly Underestimated Dust Opacities
• CHEX-MATE: Multi-probe analysis of Abell 1689
• Calculating Opacity in Hot, Dense Matter using Second-Order Electron-Photon and Two-Photon Transitions to Approximate Line Broadening
• Solar abundances and 3D model atmospheres
• Prospects of measuring a metallicity trend and spread in globular clusters from low-resolution spectroscopy
• Extremely iron-poor O-type stars in the Magellanic Bridge
• MAISTEP -- a new grid-based machine learning tool for inferring stellar parameters I. Ages of giant-planet host stars
• Axion spectra and the associated x-ray spectra of low-mass stars
• Diagnostics from solar and stellar glitches
• Boron Abundances in the Galactic Disk
• The First SRG/eROSITA All-Sky Survey. Characterization of clusters of galaxies misclassified in the eRASS1 point source catalog
• CRexit: how different cosmic ray transport modes affect thermal instability in the circumgalactic medium
• Cloudy-Maraston: Integrating nebular continuum and line emission with the Maraston stellar population synthesis models
• Three nearby K-giants with planets: Accurate determination of basic parameters, including an analysis of metallicity based on Fe I lines
• The PICS Project. I. The impact of metallicity and helium abundance on the bright end of the planetary nebula luminosity function
• Thermal emission from bow shocks. III. Variable diffuse X-ray emission from stellar-wind bow shocks driven by dynamical instabilities
• An H$\alpha$ kinematic survey of the $Herschel$ Reference Survey -- I. Fabry-Perot observations with the 1.93m telescope at OHP
• Misty, patchy, and turbulent: constraining the cool circumgalactic medium with mCC
• The Outcome of Collisions between Gaseous Clumps formed by Disk Instability
• Secrets in the shadow: High precision stellar abundances of fast-rotating A-type exoplanet host stars through transit spectroscopy
• Neutron Tagging Can Greatly Reduce Spallation Backgrounds in Super-Kamiokande
• A global view on the colliding-wind binary WR 147
• Omega Centauri: weak MgH-band in red giants directly trace the helium content
• The Puzzling Spectrum of HD 94509
• The evolutionary status of chemically peculiar eclipsing binary star DV Boo
• Constraining the helium-to-metal enrichment ratio $\Delta Y/\Delta Z$ from main sequence binary stars. Theoretical analysis of the accuracy and precision of the age and helium abundance estimates
• Revisiting Kepler-444 Part I. Seismic modelling and inversions of stellar structure
• Spectroscopy of Eclipsing Compact Hierarchical Triples I
• Solar Models and Astrophysical S-factors Constrained by Helioseismic Results and Updated Neutrino Fluxes
• On the incidence rate of RR Lyrae stars with non-radial modes
• Upper Limit on Star Formation and Metal Enrichment in Minihalos
• The Mystery of Alpha and the Isotopes
• DLA and sub-DLA metallicity evolution: A case study of absorbers towards Q0338-0005
• Planetary system architectures with low-mass inner planets: Direct imaging exploration of mature systems beyond 1 au
• Infrared spectra of TiO2 clusters for hot Jupiter atmospheres
• The unusual ISM in Blue and Dusty Gas Rich Galaxies (BADGRS)
• A rare case of FR I interaction with a hot X-ray bridge in the A2384 galaxy cluster
• On the Metallicities and Kinematics of the Circumgalactic Media of Damped Ly$\alpha$ Systems at $z\sim 2.5$
• Near-Infrared Spectroscopy of Dense Ejecta Knots in the Outer Eastern Area of the Cassiopeia A Supernova Remnant
• Residual eccentricity of an Earth-like planet orbiting a red giant Sun
• On the chemistry of hydrides of N atoms and O${}^{+}$ ions
• Sardinia Radio Telescope observations of Local Group dwarf galaxies -- I. The cases of NGC6822, IC1613, and WLM
• Exploring AGN - starburst coexistence in galaxies at z$\sim$ 0.8 by the [OIII]4959+5007/[OIII]4363 line ratio
• Evolution of dwarf galaxy observable parameters
• Revisiting the iron abundance in the hyper iron-poor star HE 1327-2326 with UV COS/$HST$ data
• Deciphering the period spacing pattern in the oscillation spectrum of the SPB star KIC 7760680
• SAFARI I: A SPHERE discovery of a super metal-rich M dwarf companion to the star HD 86006
• Identification of Large Equivalent Width Dusty Galaxies at 4 $<$ z $<$ 6 from Sub-mm Colours
• X-ray Activity Variations and Coronal Abundances of the Star-Planet Interaction candidate HD 179949
• A study on missing lines in the synthetic solar spectrum near the Ca triplet
• Theoretical evaluation of solar proton-proton fusion reaction rate and its uncertainties
• Examining the Properties of Low-Luminosity Hosts of Type Ia Supernovae from ASAS-SN
• Two merging galaxy clusters with very hot shock fronts observed shortly before pericentric passage
• Solid Accretion onto Neptune-Mass Planets I: In-Situ Accretion and Constraints from the metallicity of Uranus and Neptune
• Diversity of dwarf galaxy IR-submm emission patterns: CLUES from hydrodynamical simulations
• Lithium detection in red supergiant stars of the Perseus complex
• Spectroscopy of high proper motion stars in the ground--based UV
• An astrometric and spectroscopic study of the $\delta$ Scuti variable HD21190 and its wide companion CPD -83${}^{\circ }$ 64B
• Non-relativistic free-free emission due to $n-$distribution of electrons - Radiative cooling and thermally averaged and total Gaunt factors
• Discovery of faint double-peak Halpha emission in the halo of low redshift galaxies
• Candidate exoplanet host HD131399A: a nascent Am star
• Cluster outskirts and their connection to the cosmic web
• A detailed X-ray investigation of zeta Puppis IV. Further characterization of the variability
• Stellar Inversion Techniques
• XMM-Newton X-ray and HST weak gravitational lensing study of the extremely X-ray luminous galaxy cluster ClJ120958.9+495352 ($z=0.902$)
• Stellar evolution and modelling stars
• Analysis of Co-spatial UV-optical STIS Spectra of Planetary Nebula NGC 3242
• On the relationship between metallicity distributions of globular clusters and of circumgalactic gas
• Fundamental parameters and abundance analysis of the components in the SB2 system HD 60803
• The symbiotic binary St 2-22: Orbital and stellar parameters and jet evolution following its 2019 outburst
• The extraordinary frequency pattern variation in δ Scuti stars
• Quasar Host Galaxies and the $M_{SMBH}$ - ${\sigma }_{\ast }$ Relation
• Chemical abundances of three new Ba stars from the Keck/HIRES spectra
• Seismological challenges for stellar structure
• First Star Survivors as Metal-Rich Halo Stars that Experienced Supernova Explosions in Binary Systems
• DECam Survey for Low-Mass Stars and Substellar Objects in the UCL and LCC Subgroups of the Sco-Cen OB Association (SCOCENSUS)
• Rubidium abundances in solar metallicity stars
• From cool to hot F-stars: the influence of two ionization regions in the acoustic oscillations
• Planetary host stars: Evaluating uncertainties in ultra-cool model atmospheres
• Spatial Distribution of OVI Covering Fractions in the Simulated Circumgalactic Medium
• A headless tadpole galaxy: the high gas-phase metallicity of the ultra-diffuse galaxy UGC 2162
• A census of H$\alpha$ emitters in the intergalactic medium of the NGC 2865 system
• Helium escaping from the atmosphere of a nearby rocky exoplanet orbiting in a habitable zone
• Formation of millisecond pulsar-helium star binaries
• The strongly irradiated planets in Praesepe
• A full reconstruction of two galaxy clusters intra-cluster medium with strong gravitational lensing
• Structure of crystalline water ice formed through neon matrix sublimation under cryogenic and vacuum conditions
• Properties of observable mixed inertial and gravito-inertial modes in γ Doradus stars
• Detection of infrared fluorescence of carbon dioxide in R Leonis with SOFIA/EXES
• Iron abundance in the atmosphere of Arcturus
• Peculiarities of Abundances of Selected Elements in Metal-Rich Field RR Lyrae Stars
• Resolving high-z Galaxy Cluster properties through joint X-ray and Millimeter analysis: a case study of SPT-CLJ0615-5746
• JADES Dark Horse: demonstrating high-multiplex observations with JWST/NIRSpec dense-shutter spectroscopy in the JADES Origins Field
• Chandra's X-ray study confirms that the magnetic standard Ap star KQ Vel hosts a neutron star companion
• Calibrating the metallicity of M dwarfs in wide physical binaries with F-, G-, and K-primaries -- II: Carbon, oxygen, and odd-Z iron-peak abundances of the primary stars
• Synthetic stellar spectra to study multiple populations in globular clusters: an extended grid and the effects on the integrated light
• Tracing bulk elemental ratios in exoplanetary atmospheres with TiO chemistry
• Muon g-2, Long-Range Muon Spin Force, and Neutrino Oscillations
• NLTE spectral analysis of the intermediate helium-rich subdwarf B star CPD-20°1123
• Population synthesis of Thorne-Żytkow objects: Rejuvenated donors and unexplored progenitors in the common envelope formation channel
• 3D and Some Other Things Missing from the Theory of Massive Star Evolution
• Twenty years of observations of PM 1-188: Its chemical abundances and extraordinary kinematics
• The Sun. A typical star in the solar neighborhood?
• Probing the soft state evolution of 4U 1543-47 during its 2021 outburst using AstroSat
• Indicators of Mass in Spherical Stellar Atmospheres
• Exploring magnetic loops and serpentine fields in the quiet Sun with the GRIS-IFU
• The R-Process Alliance: Exploring the cosmic scatter among ten r-process sites with stellar abundances
• A High-Resolution Spectroscopic Survey of Directly Imaged Companion Hosts: II. Diversity in C/O Ratios among Host Stars
• Linking solar bosonic dark matter halos and active neutrinos
• Radiative acceleration calculation methods and abundance anomalies in Am stars
• The diverse quenching pathways of post-starburst galaxies in SDSS-IV MaNGA
• The $i$-processes nucleosynthesis during the formation of He-rich hot-subdwarf stars
• The recurrent nova V3890~Sgr: a near-infrared and optical study of the red giant component and its environment
• Frequency separation ratios do not suppress magnetic activity effects in solar-like stars
• On the evolutionary status of high-latitude variable V534 Lyr
• The R-Process Alliance: Hunting for gold in the near-UV spectrum of 2MASS J05383296-5904280
• Introduction to Astronomy with Radioactivity
• The Impact of Neutrino Magnetic Moments on the Evolution of the Helium Flash and Lithium-Rich Red Clump Stars
• TYC 8606-2025-1: a mild barium star surrounded by the ejecta of a very late thermal pulse
• Observations of AR Sco with $Chandra$ and $AstroSat$ Soft X-ray Telescope
• Searching for lambda Boo stars in binary systems
• Heavy-element Rydberg transition line emission from the post-giant-evolution star HD101584
• Search for Interstellar LiH in the Milky Way
• The N/O ratio in early B-type main sequence stars as an indicator of their evolution
• Detection and characterisation of a 106-day transiting Jupiter : TOI-2449 b / NGTS-36 b
• Analogs of primeval galaxies two billion years after the Big Bang
• Forming the local starburst galaxy Haro 11 through hydrodynamical merger simulations
• Unveiling the nature of the Einstein Probe transient EP 241021a
• Detection of a Star Forming Galaxy in the Center of a Low-Mass Galaxy Cluster
• Reassessing the Spin of Second-born Black Holes in Coalescing Binary Black Holes and Its Connection to the chi_eff-q Correlation
• Carbon from massive binary-stripped stars over cosmic time: effect of metallicity
• Chemical analysis of a carbon-enhanced very metal-poor star: CD-27 14351
• Optical/X-ray/radio view of Abell 1213: A galaxy cluster with anomalous diffuse radio emission
• SDSS J1059+4251, a highly magnified z ~ 2.8 star-forming galaxy: ESI observations of the rest-frame UV spectrum
• Ca ii 854.2 nm in an enhanced network region simulated with MURaM-ChE
• X-ray polarization in SN 1006 southwest shows spatial variations and differences with the radio band
• Astrophysics with radioactive isotopes
• The Sonora Brown Dwarf Atmosphere and Evolution Models I. Model Description and Application to Cloudless Atmospheres in Rainout Chemical Equilibrium
• Fundamental relation in isolated galaxies, pairs, and triplets in the local universe
• Solar cycle observations of the Neon abundance in the Sun-as-a-star
• The iron and oxygen content of LMC Classical Cepheids and its implications for the Extragalactic Distance Scale and Hubble constant
• NuSTAR view of heavily absorbed AGN: The $R-N_{\text{H}}$ correlation
• Improving 1D stellar atmosphere models with insights from multi-dimensional simulations II. 1D versus 3D hydrodynamically consistent model comparison for WR stars
• Inhomogeneous magnetic coupling in exoplanets: the stop & go of WASP-18 b's atmospheric flows
• A Fast, Hot Wind from a Nuclear Starburst
• Excess Galactic molecular absorption toward the radio galaxy 3C 111
• The uneven sisters I, NGC 4388 - a strongly constrained ram pressure stripping event
• Simulations of facular magnetic fields on cool stars I: Main sequence stars with solar metallicity
• Properties of the giant HII regions and bar in the nearby spiral galaxy NGC5430
• A Theoretical Study of the Outer Layers of Eight Kepler F-stars: The Relevance of Ionization Processes
• Off-centre convective zones in mass accreting stellar models
• Semi-analytic modelling of the europium production by neutron star mergers in the halo of the Milky Way
• K2 Observations of 95 Vir: delta Scuti Pulsations in a Chromospherically Active Star
• Deep Chandra Observations of the z = 1.16 Relaxed, Cool-core Galaxy Cluster SPT-CL J2215-3537
• Nucleosynthesis in advective disc and outflow: possible explanation for overabundances in winds from X-ray binaries
• Modelling dust extinction in the Magellanic Clouds
• Deep Chandra observations of PLCKG287.0+32.9: a clear detection of a shock front in a heated former cool core
• Multi-Object and Long-Slit Spectroscopy of Very Low Mass Brown Dwarfs in Orion Nebular Cluster
• A Spectroscopic Study of Weak Metallic Emission Lines in a B3V Star iota Her
• Activity of Selected Solar Twins
• Extreme AGN feedback in the fossil galaxy group SDSSTG 4436
• Super-Earth masses and stellar abundances from NIRPS reveal tentative evidence for water-rich formation around M dwarfs
• Tree-based solvers for adaptive mesh refinement code FLASH -- IV: An X-ray radiation scheme to couple discrete and diffuse X-ray emission sources to the thermochemistry of the interstellar medium
• A Recent Starbust in the Low Surface Brightness Galaxy UGC 628
• The ionic composition of the local absorber towards 3C 273
• Core to Cosmic Edge: SIMBA-C's New Take on Abundance Profiles in the Intragroup Medium at z = 0
• The NGC 346 massive star census: Nitrogen abundances for apparently single, narrow lined, hydrogen core burning B-type stars
• On the Size and Mass of Photo-ionized Clouds in Extended Spiral Galaxy Halos
• Solar models with protosolar accretion and turbulent mixing
• On the Application of Differential Evolution to the Analysis of X-Ray Spectra
• ALMA Datacubes and Continuum Maps of the Irradiated Western Wall in Carina
• Detection of CO${}_2$, CO, and H${}_2$O in the atmosphere of the warm sub-Saturn HAT-P-12b
• Dependence of the Sr-to-Ba and Sr-to-Eu Ratio on the Nuclear Equation of State in Metal Poor Halo Stars
• Quantifying stochasticity-driven uncertainties in H II region metallicities
• Physical conditions in the gas phases of the giant HII region LMC-N11: II. Origin of [CII] and fraction of CO-dark gas
• Inferring Galactic Parameters from Chemical Abundances: A Multi-Star Approach
• Physical properties of circumnuclear ionising clusters. I. NGC 7742
• Physically motivated modeling of LyC escape fraction during reionization
• Chemical evolution of the bulge of M31: predictions about abundance ratios
• Cosmic-ray impact on optical and mid-infrared emission line diagnostics in NGC 5728
• Build-up and survival of the disc: From numerical models of galaxy formation to the Milky Way
• Spectroscopic abundance analyses of the 3He stars HD 185330 and 3 Cen A
• Abundance sensitive points of line profiles in the stellar spectra
• The evolved pulsating CEMP star HD112869
• LAMOST J045019.27+394758.7, with peculiar abundances of N, Na, V, Zn, is possibly a Sculptor dwarf galaxy escapee
• Relighting the fire in Hickson Compact Group (HCG) 15: magnetised fossil plasma revealed by the SKA Pathfinders & Precursors
• Bright [CII]158$\mu$m Streamers as a Beacon for Giant Galaxy Formation in SPT2349$-$56 at $z=4.3$
• 3D non-LTE Ca II line formation in metal-poor FGK stars. I. Abundance corrections, radial velocity corrections, and synthetic spectra
• Impact of $\text{T}$- and $\rho$-dependent decay rates and new (n,$\gamma$) cross sections on the $\text{s}$ process in low-mass AGB stars
• The Chemical Composition of the Solar Surface
• The Origin of the Large Magellanic Cloud Globular Cluster NGC 2005
• A Compact Group of Galaxies at z = 2.48 hosting an AGN-Driven Outflow
• Creating and using large grids of pre-calculated model atmospheres for rapid analysis of stellar spectra
• Intermediate-luminosity red transients: Spectrophotometric properties and connection to electron-capture supernova explosions
• Échelle Spectroscopy of the Chemically Peculiar Star ${\theta }^1$ Ori F
• Modelling the impact of circumbinary disk accretion on post-AGB binary evolution and surface chemistry
• Abundance analysis of a nitrogen-rich extreme-helium hot subdwarf from the SALT survey
• The JCMT Nearby Galaxies Legacy Survey: SCUBA-2 observations of nearby galaxies
• Reliability of 1D radiative-convective photochemical-equilibrium retrievals on transit spectra of WASP-107b
• Asteroseismology of low-mass stars: the balance between partial ionisation and Coulomb interactions
• A theoretical framework for BL Her stars IV. New period-luminosity relations in the Rubin-LSST filters
• X-ray irradiation of three planets around Hyades star K2-136
• Metals and a Search for Molecules in the Distant Universe: Magellan MIKE Observations of sub-DLAs at 2<z<3
• Challenges in Forming Millisecond Pulsar-Black Holes from Isolated Binaries
• Interpreting Millimeter Emission from IMEGIN galaxies NGC 2146 and NGC 2976
• Updated Models for the Creation of a Low-z QSO Absorber by a Dwarf Galaxy Wind
• Asteroseismology of sz lyn using multi-band high time resolution photometry from ground and space
• Linear Solar Models: a simple tool to investigate the properties of solar interior
• Aluminium-26 production in low- and intermediate-mass binary systems
• Fluorescent Fe K line emission of gamma Cas stars II. Predictions for magnetic interactions and white-dwarf accretion scenarios
• Using Binary Population Synthesis to Calculate the Yields of Low- and Intermediate-Mass Binary Populations at Low Metallicity
• Can supernova from runaway stars mimic the signs of absorbing `super-virial' gas?
• The oscillation properties of the Blue Large Amplitude Pulsators (BLAPs): relative change rate of periods, excitations, and period relations
• A multi-ion non-equilibrium solver for ionised astrophysical plasmas with arbitrary elemental abundances
• Combustion Toolbox: An open-source thermochemical code for gas- and condensed-phase problems involving chemical equilibrium
• Numerical simulations of line-profile variation beyond a single-surface approximation for oscillations in roAp stars
• Chemodynamic evidence of pristine gas accretion in the void galaxy VGS 12
• Hertzsprung gap stars in nearby galaxies and the Quest for Luminous Red Novae Progenitors
• Infrared Properties of a Complete Sample of Star-Forming Dwarf Galaxies
• XSNAP: An X-ray Supernova Analysis Pipeline with Application to the Type II Supernova 2024ggi
• Confronting compositional confusion through the characterisation of the sub-Neptune orbiting HD 77946
• A high-redshift quasar absorber without CIV - a galactic outflow caught in the act?
• Realising efficient computation of individual frequencies for red-giant models
• The Calibration of Polycyclic Aromatic Hydrocarbon Dust Emission as a Star Formation Rate Indicator in the AKARI NEP Survey
• Helium Abundance of the Sun: A Spectroscopic Analysis
• An updated discussion of the solar abundance problem
• Impact of cosmic web on galaxy properties and their correlations: Insights from Principal Component Analysis
• Asteroseismic modelling of main-sequence solar-like stars and Kepler exoplanet host stars with the FICO procedure I. Catalogue of fundamental stellar properties
• Evolution of stars with 60 and 200 Msun: predictions for WNh stars in the Milky Way
• Towards Understanding the Nature of Young Detached Binary System HD 350731
• Typing supernova remnant G352.7$-$0.1 using XMM-Newton X-ray observations
• Spectroscopic and Photometric Behaviour of LP Ori
• Study of the effects of magnetic braking on the lithium abundances of the Sun and solar-type stars
• Soft X-ray emission from the classical nova AT 2018bej
• The dark days are overcast: Iron-bearing clouds on HD 209458 b and WASP-43 b can explain low dayside albedos
• Investigation of [KSF2015] 1381-19L, a WC9-type star in the high extinction Galactic region
• On the Origin of Intracluster Light based on the High-resolution Simulation, NewCluster
• The stellar to sub-stellar masses transition in 47 Tuc
• Dark Matter in Stars
• Chameleon fields and solar physics
• The Vertical Structure and Asymmetry of Mg ii-enriched Gas in the Milky Way Disk
• The fluxes of CN neutrinos from the Sun in case of mixing in a spherical layer in the solar core
• Physical properties of circumnuclear ionising clusters. II. NGC 7469
• An Observationally Driven Multifield Approach for Probing the Circum-Galactic Medium with Convolutional Neural Networks
• Nuclear Reactions in Evolving Stars
• Photometric determination of rotation axis inclination, rotation rate, and mass of rapidly rotating intermediate-mass stars
• Ultraviolet spectroscopy reveals a hot and luminous companion to the Be star+black hole candidate MWC 656
• Simulating the Escaping Atmosphere of GJ 436 b with Two-fluid Magnetohydrodynamic Models
• The influence of atomic alignment on absorption and emission spectroscopy
• The Cliff: A Metal-Poor Little Red Dot Hosting an Overmassive Black Hole at $z=3.55$
• NLTE abundances of Cr in the Sun and metal-poor stars
• Differential abundance analysis of Procyon and Theta Sculptoris: Comparison with abundance patterns of solar-like pairs
• Nitrogen enhancement of GN-z11 by metal pollution from supermassive stars
• From Exoplanets to Quasars: Detection of Potential Damped Lyman Alpha Absorbing Galaxies Using Angular Differential Imaging
• Global Chemistry and Thermal Structure Models for the Hot Jupiter WASP-43b and Predictions for JWST
• Contributions of supernovae type II & Ib/c to the galactic chemical evolution
• The Compositional Dimension of Planet Formation
• On the age of the magnetically active WW Psa and TX Psa members of the beta Pictoris association
• The Sterile-Active Neutrino Flavor Model: the Imprint of Dark Matter on the Electron Neutrino Spectra
• An XMM-Newton look at the strongly variable radio-weak BL Lac Fermi J1544-0639
• Searches for Extremely Metal Poor Galaxies using ALFALFA-selected Dwarf Galaxies
• Constraining galactic baryon cycle using the galaxy stellar-to-halo mass relations
• Detection of Enhanced Germanium in a New Cool Extreme Helium Star A 980: Insights and Implications
• Dynamically consistent analysis of Galactic WN4b stars
• CO-to-H${}_2$ conversion factor and grain size distribution through the analysis of ${\alpha }_{\mathrm{CO}}$-$q_{\mathrm{PAH}}$ relation
• Hypothesis about Enrichment of Solar System
• The molecular-gas properties in the gravitationally lensed merger HATLAS J142935.3-002836
• KIC 4150611: A quadruply eclipsing heptuple star system with a g-mode period-spacing pattern Asteroseismic modelling of the g-mode period-spacing pattern
• Unequivocal detection of the tidal deformation of a red giant in a binary system via interferometry
• Non-Local Thermodynamic Equilibrium inversions of the Si I 10827 A spectral line
• Investigating the Efficiency of Explosion Chemistry as a Source of Complex Organic Molecules in TMC-1
• High-temperature dust formation in carbon-rich astrophysical environments
• The Discovery and Origin of A Very-High Velocity Cloud Toward M33
• Radioactive Decay
• The LEGARE Project. I. Chemical evolution model of the Nuclear Stellar Disc in a Bayesian framework
• Star formation in low density HI gas around the Elliptical Galaxy NGC2865
• Evolutionary tracks of binary neutron star progenitors across cosmic times
• The MOSDEF Survey: A New View of a Remarkable z=1.89 Merger
• Physical Conditions and Chemical Abundances of the Variable Planetary Nebula IC 4997
• Toward a Comprehensive Grid of Cepheid Models with MESA. III. Evolutionary and Pulsation Relations for Models with Core and Envelope Overshooting
• Solar Model Independent Constraints on the Sterile Neutrino Interpretation of the Gallium Anomaly
• Multiple Absorption-Line Spectroscopy of the Intergalactic Medium. I. Model
• Main-sequence Turnoff Stars as Probes of the Ancient Galactic Relic: Chemo-dynamical Analysis of a Pilot Sample
• Interpreting the atmospheric composition of exoplanets: sensitivity to planet formation assumptions
• The X-ray and Radio Loud Fast Blue Optical Transient AT2020mrf: Implications for an Emerging Class of Engine-Driven Massive Star Explosions
• HST/WFC3 Constraints on the Abundances of OH and FeH in the Atmosphere of the Ultra-Hot Neptune LTT-9779 b
• Lanthanides and other spectral oddities in a Centauri
• Toward a Comprehensive Grid of Cepheid Models with MESA II. Impact of Physical and Numerical Assumptions on Elemental Abundances
• Measurements of 4He in Metal-Poor Extragalactic HII Regions: the Primordial Helium Abundance and the Delta Y / Delta O Ratio
• PEPSI Investigation, Retrieval, and Atlas of Numerous Giant Atmospheres (PIRANGA). IV. High-Resolution Phased-Resolved Spectroscopy of The Ultra Hot Jupiter KELT-20 b
• Optical Observations and Modeling of the Superluminous Supernova 2018lfe
• A comprehensive chemical abundance analysis of the extremely metal poor Leoncino Dwarf galaxy (AGC 198691)
• The metal-poorest tail of the Galactic halo: hypothesis on its origin from precise spectral analysis
• Modeling the H$\alpha$ Emission Surrounding Spica using the Lyman Continuum from a Gravity-darkened Central Star
• The impact of the transport of chemicals and electronic screening on helioseismic and neutrino observations in solar models
• Exploring the habitability and interior composition of exoplanets lying within the extended habitable zone
• On the Chemistry of the Young Massive Protostellar core NGC 2264 CMM3
• Molecules and Chemistry in Red Supergiants
• MIRACLE II: Unveiling the multi-phase gas interplay in the circumnuclear region of NGC 1365 via multi-cloud modeling
• Chemical templates of the Central Molecular Zone. Shock and protostellar object signatures under Galactic Center conditions
• Accelerating exoplanet climate modelling: A machine learning approach to complement 3D GCM grid simulations
• Is there a unique asteroseismic interior model for the solar-like oscillating KIC 7747078?
• Exploring the probing power of gamma-Dor's inertial dip for core magnetism: case of a toroidal field
• Metallic species in interstellar medium: Astrochemical modeling
• An improved model for the effect of correlated Si-III absorption on the one-dimensional Lyman-$\alpha$ forest power spectrum
• Does the Fe L-shell blend bias abundance measurements in intermediate-temperature clusters?
• Photometric stellar parameters for asteroseismology and Galactic studies
• Near-Eddington mass loss of hydrogen-rich Wolf-Rayet stars
• A new view of the solar interface region from the Interface Region Imaging Spectrograph (IRIS)
• Technetium-rich M Stars: Prime diagnostics of recent third dredge-up events on the Asymptotic Giant Branch
• Near-pristine gas at high redshifts: a window on early nucleosynthesis
• The SDSS-HET Survey of Kepler Eclipsing Binaries. A Sample of Four Benchmark Binaries
• Galaxy cluster count cosmology with simulation-based inference
• UNITSIM-Galaxies: data release and clustering of emission-line galaxies
• GMRT H I mapping of mid-infrared bright Blue Compact Dwarf Galaxies W1016+3754 & W2326+0608
• OASIS Survey Direct Imaging and Astrometric Discovery of HIP 71618 B: A Substellar Companion Suitable for the Roman Coronagraph Technology Demonstration
• Winds of Massive Stars: High Resolution X-ray Spectra of Stars in NGC 3603
• Glitch analysis and asteroseismic modelling of subgiant $\mu$ Herculis: confirming and interpreting the ${\Gamma }_1$ peak as the helium glitch
• Impact of the latest 22Ne+α reaction rates on nucleosynthesis in massive stars and galactic chemical evolution
• GRB 180325A: dust grain-size distribution and interstellar iron nanoparticles contribution
• EUROnu-WP6 2010 Report
• On the Relationship between Solar Spicules and Propagating Coronal Disturbances: The Role of Shocks
• Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
• Age and chemical composition of the globular cluster NGC 6652
• Winds versus jets: a comparison between black hole feedback modes in simulations of idealized galaxy groups and clusters
• Abundances of Disk Planetary Nebulae in M31 and the Radial Oxygen Gradient
• A New Member of the Fast and Furious Family: A Relativistic and Time-Variable UV Outflow in a Luminous Quasar
• HE0144-4657: A Carbon-Enhanced Ultra Metal-Poor Star ([Fe/H] ~ -4.1) from the Helmi Stream Disrupted Dwarf Galaxy
• Extrasolar enigmas: from disintegrating exoplanets to exoasteroids
• Accelerated particle beams in a 3D simulation of the quiet Sun. Lower atmospheric spectral diagnostics
• The curious conundrum regarding sulfur and oxygen abundances in planetary nebulae
• Reduce, Reuse, Recycle: Planetary Nebulae as Green Galactic Citizens
• Stellar granulation and interferometry
• MUSE Study of Two Giant Low-surface-brightness Galaxies with Compact Satellites
• GLIMPSE-D: Metallicity Decline in Faint Galaxies: Implications for [O III]+Hb Luminosity Function and Reionisation Budget
• Upper Limits for Emissions in the Coma of Comet 67P/Churyumov-Gerasimenko Near Perihelion as Measured by Rosetta's Alice Far-Ultraviolet Spectrograph
• On the Habitability of Our Universe
• Scaling relations and baryonic cycling in local star-forming galaxies: I. The sample
• Testing microphysics data
• KRONOS I: The $1-2.8\mu$m JWST Transmission Spectrum of the 23 Myr V1298 Tau c
• Concluding remarks on Solar and Stellar Activities and related planets
• Fluorine Abundances in Local Stellar Populations
• Abundant hydrocarbons in a buried galactic nucleus with signs of carbonaceous grain and polycyclic aromatic hydrocarbon processing
• Accretion process, magnetic fields, and apsidal motion in the pre-main sequence binary DQ Tau
• Exploring circumstellar chemistry in X-ray emitting AGB stars
• Preliminary Evidence That Protoplanetary Disks Eject More Mass Than They Retain
• Atomic Data and Neutron-Capture Element Abundances in Planetary Nebulae
• Impact of MgII interstellar medium absorption on near-ultraviolet exoplanet transit measurements
• Star formation quenching precedes morphological transformation in COSMOS-WEB's richest galaxy groups
• A new look into the atmospheric composition of WASP-39 b
• Open clusters in the outer disc studied with MEGARA@GTC Auner 1 and Berkeley 102
• Suppression of lithium depletion in young low-mass stars from fast rotation
• HR-GO II: chemical abundances of low-$E$ retrograde dynamically-tagged-groups: Revealing Thamnos as a very metal-poor substructure
• First joint absorption and T${}_e$-based metallicity measured in a GRB host galaxy at $z=4.28$ using JWST/NIRSpec
• Exploring the Small-scale Magnetic Fields in the Atmosphere of HD 49385 by Asteroseismic Analysis
• Chemical enrichment in LINERs from MaNGA. I. Tracing Oxygen and Nitrogen Nuclear Abundances in LINERs with Varied Ionizing Sources
• First detection of sign-reversed linear polarization from the forbidden [O I] 630.03 nm line
• Neutrinos from stars in the Milky Way
• The survey of Planetary Nebulae in Andromeda (M31): I. Imaging the disk and halo with MegaCam@CFHT
• Asteroseismic analysis of red giants in eclipsing binaries using two methods: implications for scaling relations and chemical composition
• A machine-learning photometric classifier for massive stars in nearby galaxies II. The catalog
• Uncertainties in asteroseismic grid-based estimates of stellar ages. SCEPtER: Stellar CharactEristics Pisa Estimation gRid
• The ALPINE-CRISTAL-JWST Survey: Gas-phase abundance gradients of main sequence star-forming galaxies and their kinematics at $4<z<6$
• The Stellar Chemical Abundances of Simulated Massive Galaxies at $z=2$
• The Warm-Hot Disk-Halo Interface Below the Perseus Spiral Arm
• Growing in number, passive in nature: tracing the evolution of the most massive quiescent galaxies since z ~ 0.8 with BOSS and DESI
• Analysis of TESS field eclipsing binary star V948 Her: a pulsating or non-pulsating star?
• Beryllium: The smoking gun of a rejuvenated star
• Revisiting the BE99 method for the study of outflowing gas in protostellar jets
• The Astronomical Hub: A Unified Ecosystem for Modern Astronomical Research
• Mixing-length estimates from binary systems. A theoretical investigation on the estimation errors
• The shocking features in the closest rich galaxy cluster Norma
• The Modulating Optical Depth of Photoelectric Absorption Edge with Pulse Phase in Accretion-Powered X-ray Pulsars
• Progress in global helioseismology: a new light on the solar modelling problem and its implications for solar-like stars
• Confirmation of the hot super-Neptune TOI-672 b with NIRPS and HARPS and Insights into the Neptunian desert around M dwarfs
• On SH Molecules in Umbral Spectra
• Probing the Diversity of Type Ia Supernova Remnants in 3-D Hydrodynamic Simulations with X-ray Spectral Synthesis
• Dependence of pulsation mode of Cepheids on metallicity
• Stellar age determination using deep neural networks: Isochrone ages for 1.3 million stars, based on BaSTI, MIST, PARSEC, Dartmouth and SYCLIST evolutionary grids
• Charting circumstellar chemistry of carbon-rich asymptotic giant branch stars. II. Abundances and spatial distributions of CS
• TOI-4552 b: A new ultra-short period rocky world revealed by NIRPS and TESS
• Nuclear astrophysics
• Dark matter scattering in astrophysical media: collective effects
• Detecting PAHs in high-z galaxies in proxy: Modelling physical conditions in an extremely strong damped Lyman-alpha absorber towards QSO SDSS J1143+1420 at z=2.323
• Fine-tuning the complex organic molecule formation: sulfur and CO ice as regulators of surface chemistry
• Hazy blue worlds: A holistic aerosol model for Uranus and Neptune, including Dark Spots
• The light elements in the light of 3D and non-LTE effects
• Stellar population modelling of neutron stars and black holes: spatially-resolved graveyards in MaNGA/SDSS-IV galaxies
• MUSEQuBES: Physical conditions, origins, and multi-element abundances of the circumgalactic medium of an isolated, star-forming dwarf galaxy at z=0.57
• What is Neptune's D/H ratio really telling us about its water abundance ?
• Deuterium Chemistry in the Young Massive Protostellar Core NGC 2264 CMM3
• Impact of near-degeneracy effects on linear rotational inversions for red-giant stars
• Impact on Astrophysics and Elementary Particle Physics of recent and future solar neutrino data
• The asymmetry of white dwarf double detonations and the observed scatter around the Phillips relation
• TULIPS: a Tool for Understanding the Lives, Interiors, and Physics of Stars
• Study of Integrated Spectra of Four Globular Clusters in M31
• Self-consistent numerical simulations for the formation and dynamics of solar prominences
• The odd bunch: chrono-chemo-dynamics of sixteen unusual stars from Kepler
• Discovery of lambda Boo stars in open clusters
• Th/Eu abundance ratio of red giants in the Kepler Field
• 50 Dra: Am-type twins with additional variability in a non-eclipsing system
• Multi-wavelength properties of $z\gtrsim 6$ LISA detectable events
• Neutral-Gas-Phase Metal Abundances in ZnII-Selected Quasar Absorption Line Systems near Redshift $z=1.2$
• Mixing in two magnetic OB stars discovered by the MiMeS collaboration
• Constraints on Weak Supernova Kicks from Observed Pulsar Velocities
• Molecules with ALMA at Planet-forming Scales (MAPS) XII: Inferring the C/O and S/H ratios in Protoplanetary Disks with Sulfur Molecules
• Measurement of the Electric Dipole Moment of AlCl by Stark Level Spectroscopy
• Granulation signatures as seen by Kepler short-cadence data. I. A decoupling between granulation and oscillation timescales for dwarfs
• Measuring the HI content of individual galaxies out to the epoch of reionization with [CII]
• Properties of Interstellar Medium in the S0 Galaxy NGC 1222: Evidence for Shocked-enhanced Line Emission
• Densities of small planets around the M dwarfs TOI-4336 A and TOI-4342 with ESPRESSO: Three sub-Neptunes, one super-Earth, and a Neptune-mass candidate
• $\delta$ Circini: A massive hierarchical triple system with an eclipsing binary
• Testing Evolutionary Models with Red Supergiant and Wolf-Rayet Populations
• The metallicity dependence of long-duration gamma-ray bursts
• A study of the electrostatic properties of the interiors of low-mass stars: Possible implications for the observed rotational properties
• A New Model For Including Galactic Winds in Simulations of Galaxy Formation II: Implementation of PhEW in Cosmological Simulations
• Violent mergers can explain the inflated state of some of the fastest stars in the Galaxy
• A Low Metallicity Massive Contact Binary Star System Candidate in WLM identified by Hubble and James Webb Space Telescope imaging
• Dense gas linked to star-forming regions photoionised by embedded gamma-ray bursts
• Magnetic fields and internal mixing of main sequence B stars
• Challenges and Advances in Modeling of the Solar Atmosphere: A White Paper of Findings and Recommendations
• Comparative study of low-temperature opacities with GARSTEC models
• Modeling HMI observables for the study of solar oscillations
• Discovery of the First Octupole Pulsation Mode in a delta Scuti Star: A Stationary l = 3 Sectoral Mode
• Nucleosynthesis: what direct reactions can do for it?
• The Multi-Epoch Jet Outbursts in Abell 496: synchrotron ageing and buoyant X-ray cavities draped by warm gas filaments
• RXCJ1111.6+4050 galaxy cluster: the observational evidence of a transitional fossil group
• Abundances of neutron-capture elements in CH and Carbon-Enhanced Metal-Poor (CEMP) stars
• True Unicorns and False Positives: Simulated Probabilities of Dark Massive Companions to Bright Stars
• Icy Volatile Enhancements in Evolving Protoplanetary Disks
• Matching seismic masses for RR Lyrae-type and oscillating red horizontal-branch stars in M4
• How leaky? A large parameter study of leaky dust traps to quantify the transport of pebbles and ice in protoplanetary discs
• Evolution and star formation history of NGC300 from a chemical evolution model with radial gas inflows
• SILCC -- IX. The multi-phase interstellar medium at low metallicity
• The influence of rotation and metallicity on the explodability of massive stars
• X-Shooting ULLYSES: Massive stars at low metallicity XV. On the metallicity dependence of B-supergiant mass-loss rates
• The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The UV Photometric Catalog and Stripped Star Candidate Selection
• Modeling the near-UV band of GK stars, Paper III: Dependence on abundance pattern
• Methane on the temperate exo-Saturn TOI-199b
• Discovery of a hot post-AGB star in Galactic globular cluster E3
• "In-System" Fission-Events: An Insight into Puzzles of Exoplanets and Stars?
• Blueberry and Green Pea galaxies live in low density environments
• The Evolution and Internal Structure of Neptunes and Sub-Neptunes: The importance of thermal conductivity in non-convective regions
• Searching for intergalactic star forming regions in Stephan's Quintet with SITELLE: II. Physical properties and metallicity
• The Predicted Properties of Helium-Enriched Globular Cluster Progenitors at High Redshift
• Spectroscopic and asteroseismic analysis of the secondary clump red giant HD 226808
• Using Stellar Spectral Energy Distributions to Measure Exoplanet Parameters
• Abundance stratification in type Ia supernovae -- VII. The peculiar, C-rich iPTF16abc: highlighting diversity among luminous events
• Stars on the ascending helium giant branch I. From white dwarf merger to helium giant: the evolutionary state of the rapidly rotating hot subdwarf HE 1518-0948
• Discovery of new N-emitters over a wide redshift range
• The Observed O VI is Just the Tip of the Iceberg: Estimating the Hidden Material in Circumgalactic and Intergalactic Clouds
• A compositional link between rocky exoplanets and their host stars
• Hunting for Planetary Nebulae toward the Galactic Center
• Intensities of the hydrogen Balmer lines of solar-like stars revealed by the LAMOST spectroscopic surveys
• The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray stacking analysis of Subaru's optically selected clusters spanning low richness regime
• A sensitivity analysis of interstellar ice chemistry in astrochemical models
• From gas to stars: MUSEings on the internal evolution of IC 1613
• On the Observability of Optically Thin Coronal Hyperfine Structure Lines
• Dust in brown dwarfs and extra-solar planets VI. Assessing seed formation across the brown dwarf and exoplanet regimes
• RR Lyrae stars with variable mean magnitudes
• Self-consistent Conditions for ${}^{26}$Al Injection into Protosolar Disk from a Nearby Supernova
• Lyman-alpha at Cosmic Noon II: The relationship between kinematics and Lyman-alpha in z~2-3 Lyman Break Galaxies
• Low Energy Neutrino Measurements
• Detailed properties of gravitational-wave mergers from flyby perturbations of wide binary black holes in the field
• The interplay between AGN feedback and precipitation of the intracluster medium in simulations of galaxy groups and clusters
• Hidden Gems in TESS: sherlock finds two new rocky planets around nearby M dwarfs
• The processing of radiation by dust in galaxies
• 3D elemental abundances of stars at formation across the histories of Milky Way-mass galaxies in the FIRE simulations
• Carbon measurements in two ultra-faint dwarf galaxies: Grus II and Tucana IV
• Asteroseismology of iota Draconis and Discovery of an Additional Long-Period Companion
• Gravitational Instability of Gas-Dust Circumnuclear Disks in Galaxies
• Matter Effects of Sterile Neutrino in Light of Renormalization-Group Equations
• A new shock in the pre-merging cluster pair 1E2215-2216
• Detection horizon for the neutrino burst from the stellar helium flash
• The mmax-Mecl relation in the LEGUS clusters
• Prospects for studying million-degree gas in the Milky Way halo using the forbidden optical [FeX] and [FeXIV] intersystem lines
• Purveyors of fine halos III. Chemical abundance analysis of a potential omega Cen associate
• Predictions for the X-ray circumgalactic medium of edge-on discs and spheroids
• Resolved molecular gas and star-formation in massive unquenched spirals : I. UGC 8179
• Detailed theoretical analysis of core Helium-burning stars: Mixed mode patterns I. Impact of the He-flash discontinuity and of induced semi-convection
• M^3D: Mosaicking M33 with MUSE datacubes I. Unveiling the diversity of HII regions in M33 with MUSE
• Metallicities in M dwarfs: Investigating different determination techniques
• Out of oxygen: Extremely metal-poor galaxy candidates identified at $2.5<z<6.5$ with deep JADES medium-band imaging
• Noble gases Neon and argon: a role for the chemical patterns of multiple populations in globular clusters?
• KIC 3868420: A high-amplitude $\delta$ Scuti-$\gamma$ Dor hybrid star crossing the Hertzsprung gap
• A hybrid SLAM-Payne framework for atmospheric parameter and abundance determination of early-type Stars from LAMOST DR9 low-resolution Spectra
• UVES analysis of red giants in the bulge globular cluster NGC 6522
• Intermediate-mass stars and the origin of the gas-giant planet-metallicity correlation
• Spitzer's perspective of polycyclic aromatic hydrocarbons in galaxies
• Interstellar Hydrocarbons: Degradation Chemistry in Diffuse Clouds
• Resonance locking and tidal evolution in rotating γ-Doradus binaries
• Discerning internal conditions of pulsating hot subdwarf B stars. Modelling multiple trapped modes in KIC 10001893
• CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
• SN 2019va: A Type IIP Supernova with Large Influence of Nickel-56 Decay on the Plateau-phase Light Curve
• Dynamic Photometric Variability in Three Young Brown Dwarfs in Taurus: Detection of Optical Flares with TESS data
• The SAPP pipeline for the determination of stellar abundances and atmospheric parameters of stars in the core program of the PLATO mission
• A comprehensive study of $\delta$ Scuti-type pulsators in eclipsing binaries: oscillating eclipsing Algols
• The extreme properties of the nearby hyper-Eddington accreting Active Galactic Nucleus in IRAS 04416+1215
• Revisiting the X-ray Emission of the Asynchronous Polar V1432 Aql
• A Near-Infrared and Optical Study of NGC 5822: An Open Cluster Hosting Barium-stars and Lithium-Enriched Giant Stars
• PISP: Projected-Space Inference of Stellar Parameters
• Detailed Abundances of Planet-Hosting Open Clusters. The Praesepe (Beehive) Cluster
• Heavy element enrichment of gas in surface-accretion disks: A possible origin of the mass-metallicity anti-correlation in exoplanets
• Ruminations Upon the Modeling of X-ray Foregrounds, Backgrounds and Faint Sources
• Three Puzzles from Nuclear Astrophysics
• The Metallicity Distribution Function in Outer Halo Fields of Simulated Elliptical Galaxies Compared to Observations of NGC 5128
• The importance of the way in which supernova energy is distributed around young stellar populations in simulations of galaxies
• Subaru/FOCAS IFU revealed the metallicity gradient of a local extremely metal-poor galaxy
• The Halo21 Absorption Modeling Challenge: Lessons From "Observing" Synthetic Circumgalactic Absorption Spectra
• Probing Quadratically Coupled Ultralight Dark Matter with Pulsar Timing Arrays
• Bound or blown: the fate of hot gas in galaxy groups
• LYRA II: Cosmological dwarf galaxy formation with inhomogeneous Population III enrichment
• Formation of Water-rich Giant Planet Satellites at Decretion Disk Ice Lines
• Chemical Abundance Analysis of Moving Group W11450 (Latham 1)
• The impact of metallicity-dependent dust destruction on the dust-to-metals ratio in galaxies
• The relationship between warm and hot gas-phase metallicity in massive elliptical galaxies and the influence of AGN feedback
• Sensitivity of the g-mode frequencies to pulsation codes and their parameters
• Asteroseismology of stars on the upper main sequence
• Evolution of Massive Main-sequence Stars in Rapid Population Synthesis. I. Framework and Implementation
• Thermomagnetic Ettingshausen-Nernst effect in tachocline, magnetic reconnection phenomenon in lower layers, axion mechanism of solar luminosity variations, coronal heating problem solution and mechanism of ADM variations around BH
• The ionization structure and chemical history in isolated H ii regions of dwarf galaxies with VIMOS/IFU II. The Leo A galaxy
• Detection of stellar-like abundance anomalies in the slow solar wind
• Planetary Formation and Evolution Revealed with a Saturn Entry Probe: The Importance of Noble Gases
• Origin and evolution of the Galactic inventories of interstellar dust and its composition
• Fundamental properties of two rapidly rotating stars: Rasalhague and Alkaid
• Carbon Abundances in Compact Galactic Planetary Nebulae: An Ultraviolet spectroscopic study with the Space Telescope Imaging Spectrograph (STIS)
• Advanced asteroseismic modelling: breaking the degeneracy between stellar mass and initial helium abundance
• The solar carbon, nitrogen, and oxygen abundances from a 3D LTE analysis of molecular lines
• On the Formation of Deuterated Methyl Formate in Hot Corinos
• Diagnosing the Properties and Evolutionary Fates of Black Hole and Wolf-Rayet X-ray Binaries as Potential Gravitational Wave Sources for the LIGO-Virgo-KAGRA Network
• Expectation for the MeV Gamma-Ray Emission from Pair-Instability Supernovae
• Chemical Elements Abundance in the Universe and the Origin of Life
• Spatially Resolved Properties of Extraplanar Diffuse Ionized Gas in NGC3511 and NGC3513
• Impact of the low solar abundance on the ages of globular clusters
• Extreme equivalent width-selected low-mass starbursts at $z=4-9$: insights into their role in cosmic reionization
• A Main Sequence CH-star in the globular cluster M55 (NGC 6809)
• The breaking of cold traps and onset of titanium in ultra-hot Jupiter atmospheres: WASP-189b in context
• Chemical compositions of semi-regular variable red giants
• The fate of Earth during the Sun's giant phases: New constraints from ab initio tidal modelling and AGB mass loss
• A comparative study of O, Ne, Cl, and Ar in Hii regions and PNe of the Galactic disk: Temporal evolution of radial gradients?
• Type Iax supernovae from deflagrations in Chandrasekhar mass white dwarfs
• A comparison of dust content and properties in GAMA/G10-COSMOS/3D-HST and SIMBA cosmological simulations
• An Outlook on Nuclear Physics
• Improved hydrodynamic pulsation models for the pulsating extreme helium star V652 Herculis
• Global Helioseismology
• Non-LTE Abundances in OB stars: Preliminary Results for 5 Stars in the Outer Galactic Disk
• New scaling relations from MESA models for mass and radius of subgiant stars: application to Kepler targets
• In medio stat virtus: enrichment history in poor galaxy clusters
• NIRPS tightens the mass estimate of GJ 3090 b and detects a planet near the stellar rotation period
• Modelling the formation of the first two neutron star-black hole mergers, GW200105 and GW200115: metallicity, chirp masses and merger remnant spins
• On the Galactic chemical evolution of sulphur. Sulphur abundances from the [S i] 1082 nm line in giants
• Is the nitrogen-rich source PN K4-47 a true planetary nebula?
• The contribution of stars, dust, neutral gas and supermassive black holes in galaxies to the cosmic baryon inventory
• Chemical composition and ages of four globular clusters in M31 from the analysis of their integrated-light spectra
• Spectroscopy of a sample of RV Tauri stars without IR excess
• Apsidal motion and proximity effects in the massive binary BD+60 497
• Uncertainty in predicting the stochastic gravitational wave background from compact binary coalescences
• SDSS-IV MaStar: Determination of Stellar Parameters Using Bayesian Averaging
• Condensation sequence of circumstellar cluster seeds (CSCCS)
• The optical constants and grain sizes of interstellar dust measured directly using the dust scattered x-ray halo of GRB 221009A
• A Multiband Catalog of Infrared-Excess Sources in the Vela-Carina Region: VVVX, DECaPS, and GLIMPSE
• Time-resolved JWST Retrieval Analysis of the Coldest Brown Dwarf: Temperature and Chemical Variations in WISE 0855-07
• The SOL $\text{(Solar Origin and Life)}$ Project: Detailed characterization of candidates for the ZAMS and Subgiant stages
• Radial differential rotation leading to dipole collapse in pre-main-sequence stars
• Viability of novae as sources of Galactic lithium
• Pulsation and Rotation of the EL CVn-type Eclipsing Binary 1SWASP J024743.37-251549.2
• The mixing of internal gravity waves and lithium production in intermediate-mass AGB stars
• A spatially-resolved large cavity of the J0337 protoplanetary disk in Perseus
• The effect of carbon grain destruction on the chemical structure of protoplanetary disks
• Discovery of Galaxy Clusters and a Head-Tail Radio Galaxy in the Direction of Globular Cluster NGC 6752
• Pulsations of blue supergiants before and after helium core ignition
• SAGA: Stellar Abundances for Galactic Archaeology
• Co-existence of Internal Gravity Waves and Tayler-Spruit Magnetic Fields in the Radiative Core of Low-mass Stars
• SDSS-IV MaNGA: Data-Model Discrepancy in Temperature-sensitive Line Ratios for Star-forming Galaxies
• Simulating Jellyfish Galaxies: A Case Study for a Gas-Rich Dwarf Galaxy
• Nitrogen abundances in star-forming galaxies 2.2 Gyr after the Big Bang are not elevated
• Investigating AGN feedback in H$\alpha$-luminous galaxy clusters: first Chandra X-ray analysis of Abell 2009
• Lithium abundance evolution in open clusters: Hyades, NGC752, and M67
• Weak CS Emission in an Extremely Metal-poor Galaxy DDO 70
• Effects of metallicity on mode switching in Cepheids
• GalSBI-SPS: a stellar population synthesis-based galaxy population model for cosmology and galaxy evolution applications
• Mixing-length calibration from field stars. An investigation on statistical errors, systematic biases, and spurious metallicity trends
• Revisiting the Evolutionary Status of Massive Stars at the central parsec of the Milky Way
• Attempting an accurate age estimate of the open cluster NGC 6633 using CoRoT and Gaia
• Atmospheric Signatures of Common Envelope Evolution in White Dwarf Planets
• The Tarantula massive binary monitoring VII. The nature of the eccentric O+BH binary candidate VFTS 812
• A Census of Sun's Ancestors and their Contributions to the Solar System Chemical Composition
• A model for the emission line galaxy luminosity function and flux ratios at high-redshifts
• Neutron star atmospheres composed of fusion ashes
• Towards understanding stellar variability at the sub m/s level: granulation-induced variability across the optical spectrum
• Photometric and Spectroscopic Analysis of Five Am Stars
• A semi-analytical perspective on massive red galaxies: I. Assembly history, environment & redshift evolution
• [$\alpha$/Fe] traced by H ii regions from the CALIFA survey: The connection between morphology and chemical abundance patterns
• Discovery and Characterization of Three New High-amplitude delta Scuti Stars from TESS Observations
• A rare phosphorus-rich star in an eclipsing binary from TESS
• Atomic Transition Probabilities of Neutral Calcium
• Toward a Comprehensive Grid of Cepheid Models with MESA. IV. Modest Effects of Rotation on Blue Loops
• Constraining the Metallicities of Damped Ly$\alpha$ Systems Using Extinction Curves
• Seed of Life in Space (SOLIS) XI. First measurement of nitrogen fractionation in shocked clumps of the L1157 protostellar outflow
• Gas and dust from extremely metal-poor AGB stars
• The Chemical and Thermal Structure of the Hot Atmosphere of the Elliptical Galaxy NGC 5813
• Citations to Australian Astronomy: 5 and 10 Year Benchmarks
• Chemical diversity of the atmospheres and interiors of sub-Neptunes: a case study of GJ 436 b
• The temperature and emission measure distribution in the quiet and active solar corona: a Bayesian approach
• The MAGIC project. III. Radial and azimuthal Galactic abundance gradients using classical Cepheids
• OO Dra: an Algol-type binary formed through an extremely helium-poor mass accretion revealed by asteroseismology
• Influence of radiative pumping on the HD rotational level populations in diffuse molecular clouds of the interstellar medium
• Revisiting the exoplanet radius valley with host stars from SWEET-Cat
• A multi-wavelength view of the open cluster NGC 2527: Discovery of active stars
• Mixing of CNO-cycled matter in massive stars
• The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- I. A golden thread through time and space
• Multiwavelength Characterization of a Dynamically Relaxed Cool Core Galaxy Cluster at $z=1.5$
• Towards solar measurements of nuclear reaction rates
• Spectroscopic Modeling of Luminous Transients Powered by H-Rich and He-Rich Circumstellar Interaction
• Constraints on Fermionic Dark Matter Absorption from Radiochemical Solar-Neutrino Measurements
• Testing the 3-equation Kuhfuss Convection Model using the Sun
• Does the solar oxygen abundance change over the solar cycle? An investigation into activity-induced variations of the O I infrared triplet
• Young, blue, and isolated stellar systems in the Virgo Cluster. II. A new class of stellar system
• The Nova Synthetic Data Base: A Principal Component/AI Analysis of Novae Synoptic Spectra
• Exploratory scenarios for the differential nuclear and tidal evolution of TZ Fornacis
• Applied Nanofabrication for X-ray Grating Spectroscopy
• Galaxy formation and chemical evolution
• Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars
• EC 22536-5304: a lead-rich and metal-poor long-period binary
• High-precision K2/TESS Photometry and HERMES Spectroscopy of Four Bright Field Stars
• Silicon and Strontium abundances of very metal-poor stars determined from near-infrared spectra
• Can UVB variations reconcile simulated quasar absorption lines at high redshift?
• The impact of disk-locking on convective turnover times of low-mass pre-main sequence and main sequence stars
• Next-generation Exo-REM atmospheric models: application to VHS 1256 b to emulate patchy clouds
• Exploring nonstandard quark interactions through solar neutrino studies
• The cosmic journey of dust grains -- from nucleation to planetary system
• Beyond the [OIII]$\lambda$4363 auroral line: [NeIII]$\lambda$3868 as a direct tracer of electron temperature
• An Improved Pair Method to Probe the Dust Extinction Law
• The Effects of Cosmic-Ray Diffusion and Radiative Cooling on the Galactic Wind from the Milky Way
• Spectroscopic long-term monitoring of RZ Cas -- Part I: Basic stellar and system parameters
• Stellar Bounds on a Model with Photon-Photino Oscillation
• A Chandra view of SPT-CL J0217-5014: a massive galaxy cluster at a cosmic intersection at z=0.53
• Relative evolution of eclipsing binaries: A tool to measure globular cluster ages and He abundances
• Black Hole Survival Guide: Searching for Stars in the Galactic Center That Endure Partial Tidal Disruption
• Detection of a Superluminous Spiral Galaxy in the Heart of a Massive Galaxy Cluster
• Contrasting evolutionary pathways of fast- and slow-rotating galaxies in the green valley
• An ancient system hidden in the Galactic plane?
• LRPayne: Stellar parameters and abundances from low-resolution spectra
• Galactic evolution of D, 3He and 4He
• Probing stellar cores from inversions of frequency separation ratios
• The R-Process Alliance: A Nearly Complete R-Process Abundance Template Derived from Ultraviolet Spectroscopy of the R-Process-Enhanced Metal-Poor Star HD 222925
• Linking atmospheric chemistry of the hot Jupiter HD 209458b to its formation location through infrared transmission and emission spectra
• Thermal Comptonization in a changing corona in the changing-look active galaxy NGC 1566
• Discovery of O stars in the tidal Magellanic Bridge: Stellar parameters, abundances, and feedback of the nearest metal-poor massive stars and their implication for the Magellanic System ecology
• Modelling the host galaxies of binary compact object mergers with observational scaling relations
• Evidence for the Late Arrival of Hot Jupiters in Systems with High Host-star Obliquities