The James Webb Space Telescope

Abstract

The James Webb Space Telescope (JWST) is a large (6.6m), cold (50K), infrared-optimized space observatory that will be launched early in the next decade. The observatory will have four instruments: a near-infrared camera, a near-infrared multi-object spectrograph, and a tunable filter imager will cover the wavelength range, 0.6 to 5.0 microns, while the mid-infrared instrument will do both imaging and spectroscopy from 5.0 to 29 microns. The JWST science goals are divided into four themes. The End of the Dark Ages: First Light and Reionization theme seeks to identify the first luminous sources to form and to determine the ionization history of the early universe. The Assembly of Galaxies theme seeks to determine how galaxies and the dark matter, gas, stars, metals, morphological structures, and active nuclei within them evolved from the epoch of reionization to the present day. The Birth of Stars and Protoplanetary Systems theme seeks to unravel the birth and early evolution of stars, from infall on to dust-enshrouded protostars to the genesis of planetary systems. The Planetary Systems and the Origins of Life theme seeks to determine the physical and chemical properties of planetary systems including our own, and investigate the potential for the origins of life in those systems. To enable these observations, JWST consists of a telescope, an instrument package, a spacecraft and a sunshield. The telescope consists of 18 beryllium segments, some of which are deployed. The segments will be brought into optical alignment on-orbit through a process of periodic wavefront sensing and control. The JWST operations plan is based on that used for previous space observatories, and the majority of JWST observing time will be allocated to the international astronomical community through annual peer-reviewed proposal opportunities.

96 pages, including 48 figures and 15 tables, accepted by Space Science Reviews

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• The mass-radius relation of exoplanets, revisited
• The baryon content of groups and clusters of galaxies in the FABLE simulations
• Expanding the Y Dwarf Census with Spitzer Follow-up of the Coldest CatWISE Solar Neighborhood Discoveries
• Tidal Inflation Reconciles Low-Density Sub-Saturns with Core Accretion
• New Roads to the Small-Scale Universe: Measurements of the Clustering of Matter with the High-Redshift UV Galaxy Luminosity Function
• Tracking Down the Source Population Responsible for the Unresolved Cosmic 6-8 keV Background
• Unidirectional Imaging using Deep Learning-Designed Materials
• The Clustering of High-Redshift (2.9 $\le$ z $\le$ 5.1) Quasars in SDSS Stripe 82
• unTimely: a Full-sky, Time-Domain unWISE Catalog
• ASTRI Mini-Array Core Science at the Observatorio del Teide
• Gravitational Wave Astronomy With TianQin
• Probing the Neutral Fraction of the IGM with GRBs during the Epoch of Reionization
• Detectable molecular features above hydrocarbon haze via transmission spectroscopy with JWST: Case studies of GJ 1214b-, GJ 436b-, HD 97658b-, and Kepler-51b-like planets
• Tables of phase functions, opacities, albedos, equilibrium temperatures, and radiative accelerations of dust grains in exoplanets
• New Candidate Extreme T Subdwarfs from the Backyard Worlds: Planet 9 Citizen Science Project
• CEERS Key Paper III: The Resolved Host Properties of AGN at 3 < z < 5 with JWST
• Dark Photon Dark Matter in the Presence of Inhomogeneous Structure
• Planet-Planet Occultations in TRAPPIST-1 and Other Exoplanet Systems
• Large-Scale Structure Formation: from the first non-linear objects to massive galaxy clusters
• A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS
• The Blazar sequence and its Physical Understanding
• Chemical abundance scaling relations for multiple elements in z~2-3 star-forming galaxies
• Reheating neutron stars with the annihilation of self-interacting dark matter
• JWST reveals a possible $z\sim 11$ galaxy merger in triply-lensed MACS0647$-$JD
• The unstable CO2 feedback cycle on ocean planets
• Following the Cosmic Evolution of Pristine Gas II: The search for Pop III-Bright Galaxies
• High redshift JWST predictions from IllustrisTNG: II. Galaxy line and continuum spectral indices and dust attenuation curves
• Galactic cosmic ray induced radiation dose on terrestrial exoplanets
• HD2685 b: A Hot-Jupiter orbiting an early F-type star detected by TESS
• JWST MIRI/MRS in-flight absolute flux calibration and tailored fringe correction for unresolved sources
• The JWST Early Release Science Program for the Direct Imaging & Spectroscopy of Exoplanetary Systems
• Magnetic Fields in the Formation of the First Stars. I. Theory vs. Simulation
• Dissipative Evolution of Unequal Mass Binary-Single Interactions and its Relevance to Gravitational Wave Detections
• The first galaxies: simulating their feedback-regulated assembly
• The Breakthrough Listen Search for Intelligent Life: A 3.95-8.00 GHz Search for Radio Technosignatures in the Restricted Earth Transit Zone
• Lyman-alpha radiation hydrodynamics of galactic winds before cosmic reionization
• YSE-PZ: A Transient Survey Management Platform that Empowers the Human-in-the-Loop
• Emission-Line Galaxies from the HST PEARS Grism Survey I: The South Fields
• The Effect of Orbital Configuration on the Possible Climates and Habitability of Kepler-62f
• Duty Cycle and the Increasing Star Formation History of z>=6 Galaxies
• Phantom matter: a challenging solution to the cosmological tensions
• Detecting gravitationally lensed population III galaxies with the Hubble Space Telescope and the James Webb Space Telescope
• A New Statistical Model for Population III Supernova Rates: Discriminating Between $\Lambda$CDM and WDM Cosmologies
• Seven wonders of Cosmic Dawn: JWST confirms a high abundance of galaxies and AGNs at z $\simeq$ 9-11 in the GLASS field
• Semi-analytic forecasts for JWST -- V. AGN luminosity functions and helium reionization at z = 2-7
• Implementation of disequilibrium chemistry to spectral retrieval code ARCiS and application to sixteen exoplanet transmission spectra: Indication of disequilibrium chemistry for HD 209458b and WASP-39b
• Peering into cosmic reionization: the Ly$\alpha$ visibility evolution from galaxies at $z$ = 4.5-8.5 with JWST
• First results from the JWST Early Release Science Program Q3D: The Warm Ionized Gas Outflow in z ~ 1.6 Quasar XID 2028 and its Impact on the Host Galaxy
• Detectability of the First Cosmic Explosions
• EMPRESS. IV. Extremely Metal-Poor Galaxies (EMPGs) Including Very Low-Mass Primordial Systems with M*=10^4--10^5 M_sun and 2--3% (O/H)_sun: High (Fe/O) Suggestive of Metal Enrichment by Hypernovae/Pair-Instability Supernovae
• The Ultimately Large Telescope -- what kind of facility do we need to detect Population III stars?
• Spectroscopic time series performance of the Mid-Infrared Instrument on the JWST
• Probing the stellar initial mass function with high-$z$ supernovae
• A model-based approach to the spatial and spectral calibration of NIRSpec onboard JWST
• Confirming Variability in the Secondary Eclipse Depth of the Super-Earth 55 Cancri e
• The role of faint population III supernovae in forming CEMP stars in ultra-faint dwarf galaxies
• Shapes and alignments of dark matter haloes and their brightest cluster galaxies in 39 strong lensing clusters
• Direct evidence for Ly$\alpha$ depletion in the protocluster core
• MOA-2016-BLG-227Lb: A Massive Planet Characterized by Combining Lightcurve Analysis and Keck AO Imaging
• Rapidly growing primordial black holes as seeds of the massive high-redshift JWST Galaxies
• Morphology of the very inclined debris disk around HD 32297
• The 30-Year Search for the Compact Object in SN 1987A
• Exploring galaxies-gravitational waves cross-correlations as an astrophysical probe
• A search for transiting planets around FGKM dwarfs and sub-giants in the TESS Full Frame Images of the Southern ecliptic hemisphere
• Composite Dark Energy and the Cosmological Tensions
• Adding Context to JWST Surveys with Current and Future 21cm Radio Observations
• The dust content of the Crab Nebula
• The evolution of the size-mass relation at $z$=1-3 derived from the complete Hubble Frontier Fields data set
• Theoretical vs. observational uncertainties: composition of giant exoplanets
• Distinguishing between wet and dry atmospheres of TRAPPIST-1 e and f
• The First Habitable Zone Earth-Sized Planet From TESS II: $Spitzer$ Confirms TOI-700 d
• A False Positive For Ocean Glint on Exoplanets: the Latitude-Albedo Effect
• X-ray flux in the SED modelling: An application of X-CIGALE in the XMM-XXL field
• Small-scale Intensity Mapping: Extended Ly$\alpha$, H$\alpha$ and Continuum emission as a Probe of Halo Star Formation in High-redshift Galaxies
• Constraining the Frequency of Free-Floating Planets from a Synthesis of Microlensing, Radial Velocity, and Direct Imaging Survey Results
• Photometric redshift-aided classification using ensemble learning
• Supermassive Dark Star candidates seen by JWST?
• High redshift JWST predictions from IllustrisTNG: III. Infrared luminosity functions, obscured star formation and dust temperature of high-redshift galaxies
• The nature of point source fringes in mid-infrared spectra acquired with the James Webb Space Telescope
• The James Webb Space Telescope North Ecliptic Pole Time-Domain Field -- I: Field Selection of a JWST Community Field for Time-Domain Studies
• Metallicity of Galactic RR Lyrae from Optical and Infrared Light Curves: I. Period-Fourier-Metallicity Relations for Fundamental Mode RR Lyrae
• The JWST Weather Report from the Nearest Brown Dwarfs I: multi-period JWST NIRSpec + MIRI monitoring of the benchmark binary brown dwarf WISE 1049AB
• The Climates of Other Worlds: A Review of the Emerging Field of Exoplanet Climatology
• Detectability of High-Redshift Superluminous Supernovae with Upcoming Optical and Near-Infrared Surveys - II. Beyond z=6
• Photometry's bright future: Detecting Solar System analogues with future space telescopes
• Modelling the atmosphere of lava planet K2-141b: implications for low and high resolution spectroscopy
• HD 89345: a bright oscillating star hosting a transiting warm Saturn-sized planet observed by K2
• ASTRODEEP-JWST: NIRCam-HST multiband photometry and redshifts for half a million sources in six extragalactic deep fields
• General-relativistic neutrino-radiation magnetohydrodynamics simulation of seconds-long black hole-neutron star mergers: Dependence on initial magnetic field strength, configuration, and neutron-star equation of state
• Far-IR/Submillimeter Spectroscopic Cosmological Surveys: Predictions of Infrared Line Luminosity Functions for z<4 Galaxies
• Observing Dark Stars with JWST
• The Relationship between Mid-Infrared and Sub-Millimetre Variability of Deeply Embedded Protostars
• Cold or Warm? Constraining Dark Matter with Primeval Galaxies and Cosmic Reionization after Planck
• Gaia Data Release 3: A Golden Sample of Astrophysical Parameters
• TOI-3714 b and TOI-3629 b: Two gas giants transiting M dwarfs confirmed with HPF and NEID
• GALLUMI: A Galaxy Luminosity Function Pipeline for Cosmology and Astrophysics
• Photometry and Performance of SPECULOOS-South
• New Insights into Cosmic Ray induced Biosignature Chemistry in Earth-like Atmospheres
• Accelerated Bayesian SED Modeling using Amortized Neural Posterior Estimation
• Characterizing Atmospheres of Transiting Earth-like Exoplanets Orbiting M Dwarfs with James Webb Space Telescope
• Direct imaging of sub-Jupiter mass exoplanets with James Webb Space Telescope coronagraphy
• Simulating and interpreting deep observations in the Hubble Ultra Deep Field with the JWST/NIRSpec low-resolution 'prism'
• Swansong Biospheres II: The final signs of life on terrestrial planets near the end of their habitable lifetimes
• Scaling Relations for Galaxies Prior to Reionization
• Looking for Population III stars with He II line intensity mapping
• Mapping Directly Imaged Giant Exoplanets
• The TESS-Keck Survey: Science Goals and Target Selection
• Alfnoor: A Retrieval Simulation of the Ariel Target List
• TOI-674b: an oasis in the desert of exo-Neptunes transiting a nearby M dwarf
• Cosmic variance of $z>7$ galaxies: Prediction from BlueTides
• Ring Galaxies in the EAGLE Hydrodynamical Simulations
• The Photometric Properties of Galaxies in the Early Universe
• Synthetic Evolution Tracks of Giant Planets
• Observing planet-disk interaction in debris disks
• Thermal phase curves of non-transiting terrestrial exoplanets 2. Characterizing airless planets
• Modelling Galaxy and AGN Evolution in the IR: Black Hole Accretion versus Star-Formation Activity
• Cosmological Model Tests with JWST
• High-redshift supernova rates measured with the gravitational telescope A1689
• Multiwavelength characterization of faint Ultra Steep Spectrum radio sources : A search for high-redshift radio galaxies
• Star formation in the first galaxies - III. Formation, evolution, and characteristics of the first stellar cluster
• Aluminium oxide in the atmosphere of hot Jupiter WASP-43b
• Molecular mapping of the PDS70 system: No molecular absorption signatures from the forming planet PDS70 b
• The Carnegie Chicago Hubble Program: The Mid-Infrared Colours of Cepheids and the Effect of Metallicity on the CO Band-head at $4.6\mu$m
• The Demographics of Kepler's Earths and super-Earths into the Habitable Zone
• Exoplanet Spectroscopy with JWST NIRISS: Diagnostics and Case Studies
• Low Albedo Surfaces of Lava Worlds
• Search for Optically Dark Infrared Galaxies without Counterparts of Subaru Hyper Suprime-Cam in the AKARI North Ecliptic Pole Wide Survey Field
• The COMBS survey I: Chemical Origins of Metal-Poor Stars in the Galactic Bulge
• Early-type galaxies in the near-infrared: 1.5-2.4\mum spectroscopy
• Direct emission spectroscopy of exoplanets with the medium resolution imaging spectrometer on board JWST MIRI: I. Molecular mapping and sensitivity to instrumental effects
• A Word to the WISE: Confusion is Unavoidable for WISE-selected Infrared Excesses
• Stability analysis of supermassive primordial stars: a new mass range for general relativistic instability supernovae
• The Challenges of Identifying Population III Stars in the Early Universe
• Retrieval study of cool, directly imaged exoplanet 51 Eri b
• Following the Cosmic Evolution of Pristine Gas III: The Observational Consequences of the Unknown Properties of Population III Stars
• A System of Three Super Earths Transiting the Late K-Dwarf GJ 9827 at Thirty Parsecs
• Massive Black Hole Binaries from the TNG50-3 Simulation: I. Coalescence and LISA Detection Rates
• Assessment of Isoprene as a Possible Biosignature Gas in Exoplanets with Anoxic Atmospheres
• The future of astronomy with small satellites
• First semi-empirical test of the white dwarf mass-radius relationship using a single white dwarf via astrometric microlensing
• JWST NIRSpec observations of Supernova 1987A -- from the inner ejecta to the reverse shock
• The Lyman Continuum Escape Fraction of Galaxies and AGN in the GOODS Fields
• A cryogenic liquid-mirror telescope on the moon to study the early universe
• LHS 1815b: The First Thick-Disk Planet Detected By TESS
• Metal line emission from galaxy haloes at z~1
• Near-infrared emission line diagnostics for AGN from the local Universe to redshift 3
• SPECULOOS Northern Observatory: searching for red worlds in the northern skies
• The spectral energy distribution of the redshift 7.1 quasar ULAS J1120+0641
• Measuring the reionization optical depth without large-scale CMB polarization
• The Brightest Galaxies at Cosmic Dawn from Scatter in the Galaxy Luminosity versus Halo Mass Relation
• Hubble Space Telescope Wide Field Camera 3 Observations of Escaping Lyman Continuum Radiation from Galaxies and Weak AGN at Redshifts $z$$\simeq$2.3-4.1
• Mineral snowflakes on exoplanets and brown dwarfs: Effects of micro-porosity, size distributions, and particle shape
• A Measurement of the Cosmic Optical Background and Diffuse Galactic Light Scaling from the R < 50 AU New Horizons-LORRI Data
• Formation of the first stars
• X-ray binary accretion states in Active Galactic Nuclei? Sensing the accretion disc of supermassive black holes with mid-infrared nebular lines
• A New Method to Measure Star Formation Rates in Active Galaxies Using Mid-infrared Neon Emission Lines
• Climate Modeling of a Potential ExoVenus
• Seeing sharper and deeper: JWST's first glimpse of the photometric and spectroscopic properties of galaxies in the epoch of reionisation
• Properties of reionization-era galaxies from JWST luminosity functions and 21-cm interferometry
• Stability of Cool Cores During Galaxy Cluster Growth: A Joint $Chandra$/SPT Analysis of 67 Galaxy Clusters Along a Common Evolutionary Track Spanning 9 Gyr
• First Constraints on Small-Scale Non-Gaussianity from UV Galaxy Luminosity Functions
• Unbound Particles in Dark Matter Halos
• Simulating the effect of photoheating feedback during reionization
• Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys
• An ALMA survey of submillimetre galaxies in the COSMOS field: The extent of the radio-emitting region revealed by 3 GHz imaging with the Very Large Array
• Single site observations of \textit{TESS} single transit detections
• Photometric determination of the mass accretion rates of pre-main sequence stars. V. Recent star formation in the 30 Dor nebula
• TOI-3884 b: A rare 6-R${}_{\oplus }$ planet that transits a low-mass star with a giant and likely polar spot
• Gravitational Lensing - Einstein's Unfinished Symphony
• BASS XXVIII: Near-infrared Data Release 2, High-Ionization and Broad Lines in Active Galactic Nuclei
• Non-Equilibrium Chemistry and Destruction of CO by X-ray Flares
• An Hα Impression of Lyα Galaxies at $z\simeq 6$ with Deep JWST/NIRCam Imaging
• Neutron star observations of pseudoscalar-mediated dark matter
• Probing the $z\gtrsim 6$ quasars in a universe with IllustrisTNG physics: Impact of gas-based black hole seeding models
• Rivers of Gas I.: Unveiling The Properties of High Redshift Filaments
• Estimating the warm dark matter mass from strong lensing images with truncated marginal neural ratio estimation
• Value Added Catalog of physical properties of more than 1.3 million galaxies from the DESI Survey
• Transiting Exoplanet Monitoring Project (TEMP). VI. The Homogeneous Refinement of System Parameters for 39 Transiting Hot Jupiters with 127 New Light Curves
• Convolutional neural networks as an alternative to Bayesian retrievals
• Stellar winds and metal enrichment from fast-rotating Population III stars
• An Hα view of galaxy build-up in the first 2 Gyr: luminosity functions at z~4-6.5 from NIRCam/grism spectroscopy
• Warm Dark Matter and Cosmic Reionization
• Sky localization of complete inspiral-merger-ringdown signals for nonspinning massive black hole binaries
• Capture of Electroweak Multiplet Dark Matter in Neutron Stars
• ProFuse: Physical Multi-Band Structural Decomposition of Galaxies and the Mass-Size-Age Plane
• Analytic Scattering and Refraction Models for Exoplanet Transit Spectra
• Early Black Holes in Cosmological Simulations: Luminosity Functions and Clustering Behaviour
• Structures of Local Galaxies Compared to High Redshift Star-forming Galaxies
• Balmer Break Galaxy Candidates at $z\sim 6$: a Potential View on the Star-Formation Activity at $z\gtrsim 14$
• Inefficient water degassing inhibits ocean formation on rocky planets: An insight from self-consistent mantle degassing models
• Constraints from deuterium on the formation of icy bodies in the Jovian system and beyond
• Narrow-band surveys for very high redshift Lyman-alpha emitters
• Ultra deep AKARI observations of Abell 2218: resolving the 15 um extragalactic background light
• Stellar & Planetary Parameters for K2's Late Type Dwarf Systems from C1 to C5
• A Study of Flares in the Ultra-Cool Regime from SPECULOOS-South
• Decoding the giant extragalactic radio sources
• The host galaxies of z=7 quasars: predictions from the BlueTides simulation
• An empirical infrared transit spectrum of Earth: opacity windows and biosignatures
• NGTS-2b: An inflated hot-Jupiter transiting a bright F-dwarf
• Possible identification of massive and evolved galaxies At z > 5
• ALMA reveals large overdensity and strong clustering of galaxies in quasar environments at $z\sim 4$
• On the separation between RR Lyrae and Type II Cepheids and their importance for distance determination: the case of $\omega$ Cen
• Boosting Lya and HeII 1640A Line Fluxes from Pop III Galaxies: Stochastic IMF Sampling and Departures from Case-B
• Possibilities for an Aerial Biosphere in Temperate Sub Neptune-Sized Exoplanet Atmospheres
• Stellar versus Galactic: The intensity of cosmic rays at the evolving Earth and young exoplanets around Sun-like stars
• The PLATO field selection process. II. Characterization of LOPS2, the first long-pointing field
• Towards a new era in giant exoplanet characterisation
• CEERS: Spatially Resolved UV and mid-IR Star Formation in Galaxies at 0.2 < z < 2.5: The Picture from the Hubble and James Webb Space Telescopes
• Circular polarization of the CMB: Foregrounds and detection prospects
• Revealing the cosmic reionisation history with fast radio bursts in the era of Square Kilometre Array
• Measuring Elemental Abundances of JWST Target Stars for Exoplanet Characterization I. FGK Stars
• The Galactic cosmic ray intensity at the evolving Earth and young exoplanets
• The Colorado Ultraviolet Transit Experiment (CUTE) Mission Overview
• Associating Host Galaxy Candidates to Massive Black Hole Binaries resolved by Pulsar Timing Arrays
• The Impact of Interpixel Capacitance in CMOS Detectors on PSF shapes and Implications for WFIRST
• Physical properties of extreme emission-line galaxies at $z\sim 4-9$ from the JWST CEERS survey
• On the Detection of Supermassive Primordial Stars. II. Blue Supergiants
• The Space Infrared Interferometric Telescope (SPIRIT): High-resolution imaging and spectroscopy in the far-infrared
• Final Spitzer IRAC Observations of the Rise and Fall of SN 1987A
• Observational signatures of outbursting protostars - I: From hydrodynamic simulations to observations
• The Solar Neighborhood. XLVI. Revealing New M Dwarf Binaries and their Orbital Architectures
• Population III Star Clusters in the Reionized Universe
• The ultraviolet habitable zone of exoplanets
• A novel black-hole mass scaling relation based on coronal gas, and its dependence with the accretion disc
• Spitzer transit follow-up of planet candidates from the K2 mission
• CEERS: MIRI deciphers the spatial distribution of dust-obscured star formation in galaxies at $0.1<z<2.5$
• HORuS transmission spectroscopy of 55 Cnc e
• The Spitzer search for the transits of HARPS low-mass planets - I. No transit for the super-Earth HD 40307b
• Are WASP-107-like Systems Consistent with High-eccentricity Migration?
• Planetary system around LTT 1445A unveiled by ESPRESSO: Multiple planets in a triple M-dwarf system
• Discovery of WASP-65b and WASP-75b: Two Hot Jupiters Without Highly Inflated Radii
• Color Magnitude Relation and Morphology of Low-Redshift ULIRGs in SDSS
• Signature of the first galaxies in JWST deep field observations
• Placing High-Redshift Quasars in Perspective: a Catalog of Spectroscopic Properties from the Gemini Near Infrared Spectrograph -- Distant Quasar Survey
• Probing the atmosphere of a sub-Jovian planet orbiting a cool dwarf
• Cosmic metal density evolution in neutral gas: insights from observations and cosmological simulations
• Heating Neutron Stars with Inelastic Dark Matter and Relativistic Targets
• Gamma-ray bursts and Population III stars
• Small-scale Intensity Mapping: Extended Halos as a Probe of the Ionizing Escape Fraction and Faint Galaxy Populations during Reionization
• Convective Mixing in Gas Giant Planets with Primordial Composition Gradients
• Infrared luminosity functions based on 18 mid-infrared bands: revealing cosmic star formation history with AKARI and Hyper Suprime-Cam
• Fast infrared variability from the black-hole candidate MAXI J1535$-$571 and tight constraints on the modelling
• Discovery and mass measurement of the hot, transiting, Earth-sized planet GJ 3929 b
• Assessing potential cluster Cepheids from a new distance and reddening parameterization and 2MASS photometry
• Searching for New Physics in Ultradense Environment: a Review on Dark Matter Admixed Neutron Stars
• Gravitational waves from the remnants of the first stars in nuclear star clusters
• Implementing Tidal and Gravitational Wave Energy Losses in Few-body Codes: A Fast and Easy Drag Force Model
• Measuring Chemical Abundances with Infrared Nebular Lines: HII-Chi-mistry-IR
• Exploring the diversity and similarity of radially anisotropic Milky Way-like stellar haloes: implications for disrupted dwarf galaxy searches
• Dark matter powered stars: Constraints from the extragalactic background light
• The TESS View of LOFAR Radio-Emitting Stars
• Where are the magnetar binary companions? Candidates from a comparison with binary population synthesis predictions
• Impact of gas spin and Lyman-Werner flux on black hole seed formation in cosmological simulations: implications for direct collapse
• Revealing the Local Cosmic Web from Galaxies by Deep Learning
• Astrophysical Tests of Dark Matter Self-Interactions
• Satellite Relayed Global Quantum Communication without Quantum Memory
• The deep composition of Uranus and Neptune from in situ exploration and thermochemical modeling
• Ions in the Thermosphere of Exoplanets: Observable Constraints Revealed by Innovative Laboratory Experiments
• Detecting strongly lensed supernovae at z ~ 5-7 with LSST
• On the bio-habitability of M-dwarf planets
• Chandra probes the X-ray variability of M51 ULX-7: evidence of propeller transition and X-ray dips on orbital periods
• A frequency resolved atlas of the sky in continuous gravitational waves
• Direct Observation of Cosmic Strings via their Strong Gravitational Lensing Effect: II. Results from the HST/ACS Image Archive
• Properties of High-Redshift GRBs
• Simulating MOS science on the ELT: Ly$\alpha$ forest tomography
• Two super-Earths at the edge of the habitable zone of the nearby M dwarf TOI-2095
• Observing the host galaxies of high-redshift quasars with JWST: predictions from the BlueTides simulation
• Photochemical Runaway in Exoplanet Atmospheres: Implications for Biosignatures
• Jet-powered supernovae of $\sim 10^5{M}_{\odot }$ population III stars are observable by $Euclid$, $WFIRST$, $WISH$, and $JWST$
• Dark Matter Candidates and Searches
• Are the host galaxies of Long Gamma-Ray Bursts more compact than star-forming galaxies of the field?
• The Cosmic Microwave Background and the Stellar Initial Mass Function
• Observation uncertainty effects on the precision of interior planetary parameters
• Reionisation & Cosmic Dawn Astrophysics from the Square Kilometre Array: Impact of Observing Strategies
• A Multiwavelength Study of ELAN Environments (AMUSE${}^2$). Mass budget, satellites spin alignment and gas infall in a massive $z\sim 3$ quasar host halo
• Photonic ring resonator filters for astronomical OH suppression
• Quantifying the Influence of Jupiter on the Earth's Orbital Cycles
• Probing Population III Initial Mass Functions with He II/H$\alpha$ Intensity Mapping
• Mitigating stellar activity jitter with different line lists for least-squares deconvolution: analysis of a parametric and a randomised line selection
• Spatially Resolving the Kinematics of the <100 μas Quasar Broad Line Region using Spectroastrometry
• Identification of AKARI infrared sources by Deep HSC Optical Survey: Construction of New Band-Merged Catalogue in the NEP-Wide field
• On the Significance of Rare Objects at High Redshift: The Impact of Cosmic Variance
• ZELDA: fitting Lyman-alpha line profiles using deep learning
• On the Use of Field RR Lyrae as Galactic Probes. V. Optical and radial velocity curve templates
• Enhanced star formation in $z\sim 6$ quasar companions
• TESS discovery of a sub-Neptune orbiting a mid-M dwarf TOI-2136
• High Eddington quasars as discovery tools: current state and challenges
• TOI-969: a late-K dwarf with a hot mini-Neptune in the desert and an eccentric cold Jupiter
• Simulating JWST/NIRCam Color Selection of High-Redshift Galaxies
• Spitzer Photometry of ~1 Million Stars in M31 and 15 Other Galaxies
• Two NIRCam channels are Better than One: How JWST Can Do More Science with NIRCam's Short-Wavelength Dispersed Hartmann Sensor
• Hydrohalite Salt-albedo Feedback Could Cool M-dwarf Planets
• Exploiting synergies between JWST and cosmic 21-cm observations to uncover star formation in the early Universe
• Revisiting the Kepler field with TESS: Improved ephemerides using TESS 2min data
• The Size and Pervasiveness of Ly$\alpha$-UV Spatial Offsets in Star-Forming Galaxies at $z\sim 6$
• The KOSMA-$\tau$ PDR Model -- I. Recent updates to the numerical model of photo-dissociated regions
• SOFIA observations of far-IR fine-structure lines in galaxies to measure metallicity
• Evidence that Emission and Absorption Outflows in Quasars Are Related
• The K2 and TESS Synergy. I. Updated Ephemerides and Parameters for K2-114, K2-167, K2-237, and K2-261
• Star-formation rate and stellar mass calibrations based on infrared photometry and their dependence on stellar population age and extinction
• On the LISA science performance in observations of short-lived signals from massive black hole binary coalescences
• Astrophysical Observations of a Dark Matter-Baryon Fifth Force
• The Effect of Land Fraction and Host Star Spectral Energy Distribution on the Planetary Albedo of Terrestrial Worlds
• Source counts at 7.7 to 21 $\mu$m in CEERS field with James Webb Space Telescope
• Gap Transients Interacting with Circumstellar Medium
• Beyond the Local Volume. I. Surface Densities of Ultracool Dwarfs in Deep HST/WFC3 Parallel Fields
• The Effects of Radiative Feedback and Supernova Induced Turbulence on Early Galaxies
• Magnification Bias of Distant Galaxies in the Hubble Frontier Fields: Testing Wave vs. Particle Dark Matter Predictions
• Cooling of Neutron Stars admixed with Light Dark Matter: a case study
• Challenges in the detection of gases in exoplanet atmospheres
• Dusty Stellar Birth and Death in the Metal-Poor Galaxy NGC 6822
• Stellar Tidal Disruption Events by Direct Collapse Black Holes
• Compatibility of JWST results with exotic halos
• Dark Stars Powered by Self-Interacting Dark Matter
• Chemical Composition of Bright Stars in the Continuous Viewing Zone of the TESS Space Mission
• JexoSim: A time domain simulator of exoplanet transit spectroscopy with JWST
• On the stability of satellites at unstable libration points of sun-planet-moon systems
• Exoplanet Transits with Next-Generation Radio Telescopes
• The PLATO Simulator: modelling of high-precision high-cadence space-based imaging
• MADYS: the Manifold Age Determination for Young Stars
• A tiny host galaxy for the first giant black hole: $z=7.5$ quasar in BlueTides
• Large Interferometer For Exoplanets (LIFE). X. Detectability of currently known exoplanets and synergies with future IR/O/UV reflected-starlight imaging missions
• SPECULOOS: a network of robotic telescopes to hunt for terrestrial planets around the nearest ultracool dwarfs
• New Early Dark Energy as a solution to the $H_0$ and $S_8$ tensions
• The high-ionization IR fine-structure lines as bolometric indicators of the AGN power: study of the complete 12 micron AGN sample
• Expected performances of the Characterising Exoplanet Satellite (CHEOPS) II. The CHEOPS simulator
• Detectability of Wandering Intermediate-Mass Black Holes in the Milky Way Galaxy from Radio to X-rays
• Multiple measurements of gravitational waves acting as standard probes: model-independent constraints on the cosmic curvature with DECIGO
• Metallicity of Galactic RR Lyrae from Optical and Infrared Light Curves: II. Period-Fourier-Metallicity Relations for First Overtone RR Lyrae
• Gravitational waves from mergers of Population III binary black holes: roles played by two evolution channels
• JWST-TST High Contrast: JWST/NIRCam observations of the young giant planet $\beta$ Pic b
• A direct and robust method to observationally constrain the halo mass function via the submillimeter magnification bias: Proof of concept
• Direct-collapse supermassive black holes from relic particle decay
• The Impact of Redshift on Galaxy Morphometric Classification: case studies for SDSS, DES, LSST and HST with Morfometryka
• Parallaxes of Cool Objects with WISE: Filling in for Gaia
• Evolution of Spin Period and Magnetic Field of the Crab Pulsar: Decay of the Braking Index by the Particle Wind Flow Torque
• Galaxy source counts at 7.7 $\mu$m, 10 $\mu$m and 15 $\mu$m with the James Webb Space Telescope
• Probing the Timescale of the 1.4 GHz Radio emissions as a Star formation tracer
• The Dark Side of Using Dark Sirens to Constrain the Hubble-Lemaître Constant
• HD 20329b: An ultra-short-period planet around a solar-type star found by TESS
• GJ 3090 b: one of the most favourable mini-Neptune for atmospheric characterisation
• Prebiosignature Molecules Can Be Detected in Temperate Exoplanet Atmospheres with JWST
• A Mini-Neptune Orbiting the Metal-poor K Dwarf BD+29 2654
• Transmission spectroscopy with VLT FORS2: a featureless spectrum for the low-density transiting exoplanet WASP-88b
• Unveiling Luminous Ly$\alpha$ Emitters at $z\approx 6$ through JWST/NIRCam Imaging in the COSMOS Field
• The most massive Population III stars
• Machine-learning recovery of foreground wedge-removed 21-cm light cones for high-$z$ galaxy mapping
• VLBI observations of VIK J2318-3113, a quasar at z = 6.44
• HD207897 b: A dense sub-Neptune transiting a nearby and bright K-type star
• JWST's PEARLS: resolved study of the stellar and dust components in starburst galaxies at cosmic noon
• 3-D climate simulations for the detectability of Proxima Centauri b
• Electromagnetic Follow-up Observations of Binary Neutron Star Mergers with Early Warnings from Decihertz Gravitational-wave Observatories
• Reionization with Simba: How much does astrophysics matter in modeling cosmic reionization?
• The intermediate-ionization lines as virial broadening estimators for Population A quasars
• The Near Infrared Imager and Slitless Spectrograph for JWST -- V. Kernel Phase Imaging and Data Analysis
• Cosmic Reionization On Computers: The Galaxy-Halo Connection between $5\le z\le 10$
• Simulated JWST datasets for multispectral and hyperspectral image fusion
• Impact of EDGES 21cm Global Signal on Primordial Power Spectrum
• Universe opacity and CMB
• The NuSTAR Extragalactic Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain Field
• An 11 Earth-Mass, Long-Period Sub-Neptune Orbiting a Sun-like Star
• Analysis of Orbital Configurations for Millimetron Space Observatory
• Cosmology with the submillimetre galaxies magnification bias: Proof of concept
• High resolution science with high redshift galaxies
• Looking for Signatures of AGN Feedback in Radio-Quiet AGN
• Kernel-phase Detection Limits : Hypothesis Testing and the Example of JWST NIRISS Full Pupil Images
• Toward accurate thermal modeling of phase change material based photonic devices
• X-ray variability of HD 189733 across eight years of XMM-Newton observations
• Earth as an Exoplanet. II. Earth's Time-variable Thermal Emission and Its Atmospheric Seasonality of Bioindicators
• LADDER: Revisiting the Cosmic Distance Ladder with Deep Learning Approaches and Exploring its Applications
• Impact of gas based seeding on supermassive black hole populations at $z\ge 7$
• Giant exoplanet composition: Why do the hydrogen-helium equation of state and interior structure matter?
• Euclid detectability of pair instability supernovae in binary population synthesis models consistent with merging binary black holes
• Spitzer IRAC observations of JWST calibration stars
• The resolved chemical composition of the starburst dwarf galaxy CGCG007-025: Direct method versus photoionization model fitting
• SPICA and the Chemical Evolution of Galaxies: The Rise of Metals and Dust
• The Atmospheres of Rocky Exoplanets II. Influence of surface composition on the diversity of cloud condensates
• HOD modelling of high redshift galaxies using the BLUETIDES simulation
• The Stellar Kinematics of Void Dwarf Galaxies Using KCWI
• Observability of Forming Planets and their Circumplanetary Disks IV. -- with JWST & ELT
• Searching for supernovae in the multiply-imaged galaxies behind the gravitational telescope A370
• Scalable inference with Autoregressive Neural Ratio Estimation
• Multimessenger astronomy with a kHz-band gravitational-wave observatory
• YunMa: Enabling Spectral Retrievals of Exoplanetary Clouds
• Testing gravity with gravitational waves $\times$ electromagnetic probes cross-correlations
• Characterization of starspots on a young M-dwarf K2-25: multi-band observations of stellar photometric variability and planetary transits
• The TEMPO Survey I: Predicting Yields of the Transiting Exosatellites, Moons, and Planets from a 30-day Survey of Orion with the Nancy Grace Roman Space Telescope
• Inferring Chemical Disequilibrium Biosignatures for Proterozoic Earth-Like Exoplanets
• Enhanced Early Galaxy Formation in JWST from Axion Dark Matter?
• The Detectability of Kiloparsec Scale Dual AGNs: The Impact of Galactic Structure and Black Hole Orbital Properties
• Correlations between H$\alpha$ Equivalent Width and Galaxy Properties at $z=0.47$: Physical or Selection-driven?
• The Space Environment and Atmospheric Joule Heating of the Habitable Zone Exoplanet TOI700-d
• Massive spheroids can form in single minor mergers
• A methodology to select galaxies just after the quenching of star formation
• MOMO V. Effelsberg, Swift and Fermi study of the blazar and supermassive binary black hole candidate OJ 287 in a period of high activity
• Spectroscopy of the Supernova H0pe Host Galaxy at Redshift 1.78
• High-contrast observations of brown dwarf companion HR 2562 B with the vector Apodizing Phase Plate coronagraph
• Signatures of impact-driven atmospheric loss in large ensembles of exoplanets
• Formation of Compact Stellar Clusters by High-Redshift Galaxy Outflows II: Effect of Turbulence and Metal-Line Cooling
• Morphological Classification of Local Luminous Infrared Galaxies
• Cosmic Type Ia SN rate and constraints on SN Ia progenitors
• Identifying the progenitors of present-day early-type galaxies in observational surveys: correcting `progenitor bias' using the Horizon-AGN simulation
• Interior-atmosphere modelling to assess the observability of rocky planets with JWST
• Deblending Galaxies with Generative Adversarial Networks
• GRBs and fundamental physics
• Footprints of population III stars in the gravitational-wave background
• GJ 3929: High Precision Photometric and Doppler Characterization of an Exo-Venus and its Hot, Mini-Neptune-mass Companion
• Enlightening the dark ages with dark matter
• Observations of the High Redshift Universe
• The Evolution of AGN Activity in Brightest Cluster Galaxies
• The missing FeII bump in faint JWST AGN: possible evidence for metal-poor broad-line regions at early cosmic times
• Knobs and dials of retrieving JWST transmission spectra. I. The importance of p-T profile complexity
• Prospects for Detecting Signs of Life on Exoplanets in the JWST Era
• Gemini Near Infrared Spectrograph -- Distant Quasar Survey: Augmented Spectroscopic Catalog and a Prescription for Correcting UV-Based Quasar Redshifts
• A z=1.85 galaxy group in CEERS: evolved, dustless, massive intra-halo light and a brightest group galaxy in the making
• EOS-ESTM: A flexible climate model for habitable exoplanets
• The Simulated Catalogue of Optical Transients and Correlated Hosts (SCOTCH)
• Gaussian Process Reconstruction of Reionization History
• Dwarf satellites of high-z Lyman Break Galaxies: a free lunch for JWST
• PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-Domain Field II
• AGNs at the cosmic dawn: predictions for future surveys from a $\Lambda$CDM cosmological model
• MOA-bin-29b : A Microlensing Gas Giant Planet Orbiting a Low-mass Host Star
• Abundant Serendipitous Emission Line Sources with JWST/NIRSpec
• Galaxy Morphology Classification Using Multi-Scale Convolution Capsule Network
• Splitting the lentils: Clues to galaxy/black hole coevolution from the discovery of offset relations for non-dusty versus dusty (wet-merger-built) lenticular galaxies in the $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{spheroid}}$ diagram
• Exoplanet Modulation of Stellar Coronal Radio Emission
• Unveiling the main sequence of galaxies at $z\ge 5$ with the James Webb Space Telescope: predictions from simulations
• The Sparse Atmospheric MOdel Sampling Analysis (SAMOSA) intercomparison: Motivations and protocol version 1.0. A CUISINES model intercomparison project
• Was there an early reionization component in our universe?
• Spitzer mid-infrared point sources in the fields of nearby galaxies
• 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
• The Lyman Alpha Reference Sample. VIII. Characterizing Lyman-Alpha Scattering in Nearby Galaxies
• In-focus wavefront sensing using non-redundant mask-induced pupil diversity
• The MIRI Medium Resolution Spectrometer calibration pipeline
• The Search for Celestial Positronium via the Recombination Spectrum
• Wide-field adaptive optics performance in cosmological deep fields for multi-object spectroscopy with the European Extremely Large Telescope
• Searching for TESS Photometric Variability of Possible JWST Spectrophotometric Standard Stars
• Silicate Precursor Silane detected in Cold Low-Metallicity Brown Dwarf
• Habitable Zone and Atmosphere Retention Distance (HaZARD) Stellar-evolution-dependent loss models of secondary atmospheres
• Photometric Calibrations of M-dwarf Metallicity with Markov Chain Monte Carlo and Bayesian Inference
• 3D-DASH: The Widest Near-Infrared Hubble Space Telescope Survey
• The energetic particle environment of a GJ 436 b-like planet
• Theoretical investigation of the occurrence of tidally excited oscillations in massive eccentric binary systems
• Detection of multiple stellar populations in extragalactic massive clusters with JWST
• Quantifying the information impact of future searches for exoplanetary biosignatures
• Properties of globular clusters formed in dark matter mini-halos
• New-generation dust emission templates for star-forming galaxies
• Validation and atmospheric exploration of the sub-Neptune TOI-2136b around a nearby M3 dwarf
• Hundreds of TESS exoplanets might be larger than we thought
• Realistic Detection and Early Warning of Binary Neutron Stars with Decihertz Gravitational-wave Observatories
• Biosignature Surveys to Exoplanet Yields and Beyond
• Status of the Stratospheric Observatory for Infrared Astronomy (SOFIA)
• A feasibility study on the photometric detection of quiescent black hole X-ray binaries
• Cross-sections for heavy atmospheres: H${}_2$O self-broadening
• Competing chemical signatures in the atmosphere of TOI-270 d: Inference of sulfur and carbon chemistry
• Fires in the deep: The luminosity distribution of early-time gamma-ray-burst afterglows in light of the Gamow Explorer sensitivity requirements
• VaTEST II: Statistical Validation of 11 TESS-Detected Exoplanets Orbiting K-type Stars
• Maximising the power of deep extragalactic imaging surveys with the James Webb Space Telescope
• The Aromatic Features in Very Faint Dwarf Galaxies
• The K2 & TESS Synergy II: Revisiting 26 systems in the TESS Primary Mission
• Impacts of Water Latent Heat on the Thermal Structure of Ultra-Cool Objects: Brown Dwarfs and Free-Floating Planets
• Modelling emission lines in star forming galaxies
• Calibration of mid- to far-infrared spectral lines in galaxies
• Fully fluorinated non-carbon compounds NF3 and SF6 as ideal technosignature gases
• Developing a Drift Rate Distribution for Technosignature Searches of Exoplanets
• Finding Singularities in Gravitational Lensing
• Multiverse Predictions for Habitability: The Number of Stars and their Properties
• VISIONS: The VISTA Star Formation Atlas -- I. Survey overview
• SASHIMI-SIDM: Semi-analytical subhalo modelling for self-interacting dark matter at sub-galactic scales
• Dark Exoplanets
• Extreme Primordial Star Formation Enabled by High Redshift Quasars
• Toward a multidimensional analysis of transmission spectroscopy. Part III: Modelling 2D effects in retrievals with TauREx
• Detecting Planetary Oblateness in the Era of JWST: A Case Study of Kepler-167e
• Premature Black Hole Death of Population III Stars by Dark Matter
• Feeding plankton to whales: high-redshift supermassive black holes from tiny black hole explosions
• Characterizing WASP-43b's interior structure: unveiling tidal decay and apsidal motion
• Constraining the Minimum Luminosity of High Redshift Galaxies through Gravitational Lensing
• A Framework for Optimizing Exoplanet Target Selection for the James Webb Space Telescope
• Deep redshift topological lensing: strategies for the T^3 candidate
• AutoSourceID-Light. Fast Optical Source Localization via U-Net and Laplacian of Gaussian
• Dark energy reconstruction analysis with artificial neural networks: Application on simulated Supernova Ia data from Rubin Observatory
• Revisiting the HD 21749 Planetary System with Stellar Activity Modeling
• Repeated Cyclogenesis on Hot-Exoplanet Atmospheres with Deep Heating
• Observing Near-Earth Objects with the James Webb Space Telescope
• Detecting Population III Stars through Tidal Disruption Events in the Era of JWST and Roman
• Gravitational-wave event rates as a new probe for dark matter microphysics
• The Infrared Luminosity Function of AKARI 90$\mu$m Galaxies in the Local Universe
• A close outer companion to the ultra-hot Jupiter TOI-2109 b?
• The Ultramarine Simulation: properties of dark matter haloes before redshift 5.5
• Unraveling the origin of giant exoplanets: Observational implications of convective mixing
• From Dust to Nanodust: Resolving Circumstellar Dust from the Colliding-Wind Binary Wolf-Rayet (WR) 140
• Characterization of the HD 108236 system with CHEOPS and TESS. Confirmation of a fifth transiting planet
• Ozone Production in Electron Irradiated CO2:O2 Ices
• Prospects of calibrating afterglow modeling of short GRBs with gravitational wave inclination angle measurements and resolving the Hubble tension with a GW-GRB association event
• Salty ice and the dilemma of ocean exoplanet habitability
• New JWST redshifts for the host galaxies of CDF-S XT1 and XT2: understanding their nature
• Charting nearby stellar systems: The intensity of Galactic cosmic rays for a sample of solar-type stars
• Collisions of Terrestrial Worlds: The Occurrence of Extreme Mid-Infrared Excesses around Low-Mass Field Stars
• Follow the Water: Finding Water, Snow and Clouds on Terrestrial Exoplanets with Photometry and Machine Learning
• An Earth-sized Planet around an M5 Dwarf Star at 22 pc
• Variation of optical and infrared properties of galaxies with their surface brightness
• Exploring dark sector parameters in light of neutron star temperatures
• The Telltale Heartbeat: Detection and Characterization of Eccentric Orbiting Planets via Tides on their Host Star
• Theoretical compensation of static deformations of freeform multi mirror substrates
• Halfway to the Peak: The JWST MIRI 5.6 micron number counts and source population
• Probabilistic and progressive deblended far-infrared and sub-millimetre point source catalogues I. Methodology and first application in the COSMOS field
• Radial velocity confirmation of a hot super-Neptune discovered by TESS with a warm Saturn-mass companion
• Statistical tests of young radio pulsars with/without supernova remnants: implying two origins of neutron stars
• An interference-based method for the detection of strongly lensed gravitational waves
• JADES Data Release 4 Paper I: Sample Selection, Observing Strategy and Redshifts of the complete spectroscopic sample
• The strong suppression of Galactic cosmic rays reaching AU Mic b, c and Prox Cen b
• The ionizing photon production efficiency of star-forming galaxies at $z\sim 4-10$
• The duration of reionization constrains the ionizing sources
• Optical tracking of deep-space spacecraft in Halo L2 orbits and beyond: the Gaia mission as a pilot case
• Milankovitch Cycles for a Circumstellar Earth-analog within $\alpha$ Centauri-like Binaries
• Least response method to separate CMB spectral distortions from foregrounds
• Evolution of the Planetary Obliquity: The Eccentric Kozai-Lidov Mechanism Coupled with Tide
• HD 183579b: A Warm Sub-Neptune Transiting a Solar Twin Detected by TESS
• Early formation of supermassive black holes from the collapse of strongly self-interacting dark matter
• A power spectrum approach to the search for Axion-like Particles from resolved galaxy clusters using CMB as a backlight
• Environmental Effects on AGN activity via Extinction-free Mid-Infrared Census
• Dark skies of the slightly eccentric WASP-18 b from its optical-to-infrared dayside emission
• Rocks, Water and Noble Liquids: Unfolding the Flavor Contents of Supernova Neutrinos
• Cyber-Cosmos: A New Citizen Science Concept in A Dark Sky Destination
• Probing Na in giant exoplanets with ESPRESSO and 3D NLTE stellar spectra
• Probing Interstellar Dust with Infrared Echoes from the Cas A Supernova
• Discovery of Five Candidate Analogs for $\eta$Carinae in Nearby Galaxies
• Searching for Biosignatures in Exoplanetary Impact Ejecta
• Detectability of Rocky-Vapour Atmospheres on Super-Earths with Ariel
• PhoSim-NIRCam: Photon-by-photon image simulations of the James Webb Space Telescope's Near-Infrared Camera
• Brackett-$\gamma$ as a Gold-standard Test of Star Formation Rates Derived from SED Fitting
• Physical properties of strong 1 < z < 3 Balmer and Paschen lines emitters observed with JWST
• A study in scarlet -- I. Photometric properties of a sample of Intermediate Luminosity Red Transients
• TOI-1696 and TOI-2136: Constraining the Masses of Two Mini-Neptunes with HPF
• Analysis of the spatially-resolved $V$-3.6$\mu$m colors and dust extinction in 257 nearby NGC and IC galaxies
• Tidal Heating of Exomoons in Resonance and Implications for Detection
• Two transiting hot Jupiters from the WASP survey: WASP-150b and WASP-176b
• The Luminosity and Stellar Mass Functions of Red W1-W2 Galaxies
• Validation of a Third Planet in the LHS 1678 System
• PAC in DESI. I. Galaxy Stellar Mass Function into the $10^6{\mathrm{M}}_{\odot }$ Frontier
• Searching for galaxy-scale strong-lenses in galaxy clusters with deep networks -- I: methodology and network performance
• Dust emission, extinction, and scattering in LDN 1642
• On the nature of infrared-faint radio sources in the SXDF and VLA-VVDS fields
• JexoSim 2.0: End-to-End JWST Simulator for Exoplanet Spectroscopy -- Implementation and Case Studies
• MOA-2012-BLG-505Lb: A super-Earth mass planet probably in the Galactic bulge
• Observing Outer Planet Satellites (except Titan) with JWST: Science Justification and Observational Requirements
• TIC~257060897b: an inflated, low-density, hot-Jupiter transiting a rapidly evolving subgiant star
• Retrieving Exoplanet Atmospheres using Planetary Infrared Excess: Prospects for the Nightside of WASP-43 b and other Hot Jupiters
• Stability and pulsation of the first dark stars
• Predictions for Complex Distributions of Stellar Elemental Abundances in Low-Mass Galaxies
• Euclid preparation. Observational expectations for redshift z<7 active galactic nuclei in the Euclid Wide and Deep surveys
• PRIMER: JWST/MIRI reveals the evolution of star-forming structures in galaxies at z<2.5
• Potential Interior Structures and Habitability of Super-Earth Exoplanets LHS 1140 b, K2-18 b, TOI-1452 b and TOI-1468 c
• The NEID Earth Twin Survey. II. Dynamical Masses in Seven High-acceleration Star Systems
• Unveiling the Universe with Emerging Cosmological Probes
• Extragalactic Fields Optimized for Adaptive Optics
• The TRAPUM Large Magellanic Cloud pulsar survey with MeerKAT I: Survey setup and first seven pulsar discoveries
• ARES VI: Viability of one-dimensional retrieval models for transmission spectroscopy characterization of exo-atmospheres in the era of JWST and Ariel
• The Tianlin Mission: a 6m UV/Opt/IR space telescope to explore the habitable worlds and the universe
• Measuring the Temperature of Starspots from Multi-Filter Photometry
• Robustness of Gaian Feedbacks to Climate Perturbations
• Galactic cosmic ray propagation through M dwarf planetary systems
• RUBIES spectroscopically confirms the high number density of quiescent galaxies from $2<\mathbf{z}<5$
• Chemical evolution imprints in the rare isotopes of nearby M dwarfs
• Stellar Signals of a Baryon-Number-Violating Long-Range Force
• Multi-band, Multi-epoch Photometry of the Spot-crossing System TOI-3884: Refined System Geometry and Spot Properties
• Astrophysical signatures of leptonium
• From Gas to Stars Over Cosmic Time
• The Fine Structure Constant and Habitable Planets
• A systematic search for dormant galaxies at z~5-7 from the JWST NIRSpec archive
• Enhancing 3D Planetary Atmosphere Simulations with a Surrogate Radiative Transfer Model
• Constraints on a Non-thermal History from Galactic Dark Matter Spikes
• The recent star formation history of NGC 628 on resolved scales
• Validating Stellar Abundance Measurements from Multi-Resolution Spectroscopy
• Formation of the First Galaxies: Theory and Simulations
• Astrophysics with the Laser Interferometer Space Antenna
• HELLO project: High-$z$ Evolution of Large and Luminous Objects
• Exotic Image Formation in Strong Gravitational Lensing by Clusters of Galaxies -- IV. Elliptical NFW Lenses and Hyperbolic Umbilics
• Small-scale Effects of Thermal Inflation on Halo Abundance at High-$z$, Galaxy Substructure Abundance and 21-cm Power Spectrum
• Spectral variability studies in Active Galactic Nuclei: Exploring continuum and emission line regions in the age of LSST and JWST
• Principal Component Analysis of Up-the-ramp Sampled IR Array Data
• Theoretical Transmission Spectra of Exoplanet Atmospheres with Hydrocarbon Haze. II. Dependence on UV Irradiation Intensity, Metallicity, C/O Ratio, Eddy Diffusion Coefficient, and Temperature
• The Habitability of GJ 357 d : Possible Climates and Observability
• DAmodel: Hierarchical Bayesian Modelling of DA White Dwarfs for Spectrophotometric Calibration
• Two neighbours of the ultra-short-period Earth-sized planet K2-157 b in the warm Neptunian savanna
• Evidence of Titanate Clouds in the Day-side Atmosphere of the Ultra-Hot Jupiter WASP-121b
• Long-term 4.6$\mu$m Variability in Brown Dwarfs and a New Technique for Identifying Brown Dwarf Binary Candidates
• Quantum Radio Astronomy: Data Encodings and Quantum Image Processing
• COLIBRE: calibrating subgrid feedback in cosmological simulations that include a cold gas phase
• relensing: Reconstructing the mass profile of galaxy clusters from gravitational lensing
• Extended source fringe flats for the JWST MIRI Medium Resolution Spectrometer
• Searching for Hot Water World Candidates with CHEOPS: Refining the radii and analysing the internal structures and atmospheric lifetimes of TOI-238 b and TOI-1685 b
• An extended low-density atmosphere around the Jupiter-sized planet WASP-193 b
• Boosting Line Intensity Map Signal-to-Noise with the Ly-$\alpha$ Forest Cross-Correlation
• Foreground and sensitivity analysis for broad band (2D) 21cm--Ly-alpha and 21cm--H-alpha correlation experiments probing the Epoch of Reionization
• Emission Line Predictions for Mock Galaxy Catalogues: a New Differentiable and Empirical Mapping from DESI
• High-redshift quasar selection from the CFHQSIR survey
• Radii, masses, and transit-timing variations of the three-planet system orbiting the naked-eye star TOI-396
• Reconstructing Atmospheric Parameters of Exoplanets Using Deep Learning
• A reanalysis of the LHS 1140 b atmosphere observed with the Hubble Space Telescope
• Mysteries of Capotauro: investigating the puzzling nature of an extreme F356W-dropout
• Fluorescent C II* 1335A emission spectroscopically resolved in a galaxy at z = 5.754
• MEGADES: MEGARA Galaxy Discs Evolution Survey. Data Release I: central fields
• Gravitational Microlensing Event Statistics for the Zwicky Transient Facility
• N-body simulations of structure formation in thermal inflation cosmologies
• Identification of Intermediate-mass Black Hole Candidates Among a Sample of Sd Galaxies
• Exotic Image Formation in Strong Gravitational Lensing by Clusters of Galaxies. I: Cross-Section
• The GAPS programme at TNG XLIII. A massive brown dwarf orbiting the active M dwarf TOI-5375
• ALMA and Keck analysis of Fomalhaut field sources: JWST's Great Dust Cloud is a background object
• Spectrophotometric Redshifts In The Faint Infrared Grism Survey: Finding Overdensities Of Faint Galaxies
• PAH Spectral Diversity in NGC 7027 and the Evolution of Aromatic Carriers
• Tighter constraints on the atmosphere of GJ 436 b from combined high-resolution CARMENES and CRIRES${}^{+}$ observations
• Improvements to the Search for Cosmic Dawn Using the Long Wavelength Array
• CEMPlifying reionization
• Effects of chemically homogeneous evolution of the first stars on the 21-cm signal and reionization
• Cosmic reflections I: the structural diversity of simulated and observed low-mass galaxy analogues
• Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
• NIRPS and TESS reveal a peculiar system around the M dwarf TOI-756: A transiting sub-Neptune and a cold eccentric giant
• Exploring the evolution of star formation and dwarf galaxy properties with JWST/MIRI serendipitous spectroscopic surveys
• Troubles mounting for multipolar dark matter
• Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect
• Generating synthetic star catalogs from simulated data for next-gen observatories with py-ananke
• Planet Across Space and Time (PAST). VII. The origin and tidal evolution of hot Jupiters constrained by a broken age-frequency relation
• Detecting planetary mass companions near the water frost-line using JWST interferometry
• In Search of Extraterrestrial Artificial Intelligence Through Dyson Sphere-like structures around Primordial Black Holes
• An optimised survey strategy for the ERIS/NIX imager: searching for young giant exoplanets and very low mass brown dwarfs using the K-peak custom photometric filter
• Earth-like planets hosting systems: Architecture and properties
• TODDLERS: A New UV to Millimeter Emission Library for Star-Forming Regions. II. Star Formation Rate Indicators Using Auriga Zoom Simulations
• A rocky exoplanet classification method and its application to calculating surface pressure and surface temperature
• A CHEOPS Search for Massive, Long-Period Companions to the Warm Jupiter K2-139 b
• PM 1-322: new variable planetary nebula
• Can Isotopologues Be Used as Biosignature Gases in Exoplanet Atmospheres?
• X-ray properties of high-redshift Radio Loud and Radio Quiet Quasars observed by Chandra
• Reconciling PTA and JWST and preparing for LISA with POMPOCO: a Parametrisation Of the Massive black hole POpulation for Comparison to Observations
• A low-mass sub-Neptune planet transiting the bright active star HD 73344
• Infrared bubble recognition in the Milky Way and beyond using deep learning
• The changing transit shape of TOI-3884 b
• Machine Learning Classification of COSMOS2020 Galaxies: Quiescent vs. Star-Forming
• A Measurement of The Faint Source Correlation Function in the GOODS and UDF Survey
• Photometric properties of classical bulge and pseudo-bulge galaxies at $0.5\le z<1.0$
• Astronomical imaging Fourier spectroscopy at far-infrared wavelengths
• Primordial black holes save $R^2$ inflation
• Probing the earliest phases in the formation of massive galaxies with simulated HST+JWST imaging data from Illustris
• Cosmological Zoom-In Simulations of Milky Way Host Mass Dark Matter Halos with a Blue-Tilted Primordial Power Spectrum
• Can Carbon Fractionation Provide Evidence for Aerial Biospheres in the Atmospheres of Temperate Sub-Neptunes?
• Quantifying the Impact of Starspot-Crossing Events on Retrieved Parameters from Transit Lightcurves
• Shedding light on the star formation rate-halo accretion rate connection and halo quenching mechanism via DECODE, the Discrete statistical sEmi-empiriCal mODEl
• A One-Dimensional Energy Balance Model Parameterization for the Formation of CO2 Ice on the Surfaces of Eccentric Extrasolar Planets
• "Zombie" or active? An alternative explanation to the properties of star-forming galaxies at high redshift
• Wavelength Calibration and Resolving Power of the JWST MIRI Medium Resolution Spectrometer
• Host group degeneracy in gravitational lensing time delay determination of $H_0$
• Role of Future SNIa Data from Rubin LSST in Reinvestigating Cosmological Models
• Impact of Planetary Parameters on Water Clouds Microphysics
• Reconstructing the epoch of reionisation with Planck PR4
• Revealing the Warm and Hot Halo Baryons via Thomson Scattering of Quasar Light
• Evaluating the GeoSnap 13-$\mu$m Cut-Off HgCdTe Detector for mid-IR ground-based astronomy
• AGN -- host galaxy photometric decomposition using a fast, accurate and precise deep learning approach
• Inferring properties of dust in supernovae with neural networks
• Narrowing the discovery space of the cosmological 21-cm signal using multi-wavelength constraints
• Improved Treatment of Bosonic Dark Matter Dynamics in Neutron Stars: Consequences and Constraints
• Cosmic ray ionisation of a post-impact early Earth atmosphere: Solar cosmic ray ionisation must be considered in origin-of-life scenarios
• The Diversity of Exoplanetary Environments and the Search for Signs of Life Beyond Earth
• Exotic Image Formation in Strong Gravitational Lensing by Clusters of Galaxies -- II: Uncertainties
• From Large Telescopes to the MUltiplexed Survey Telescope (MUST)
• QSO MUSEUM III: the circumgalactic medium in Ly$\alpha$ emission around 120 $z\sim 3$ quasars covering the SDSS parameter space. Witnessing the instantaneous AGN feedback on halo scales
• Cloudy with a chance of starshine: Possible photometric signatures of nebular-dominated emission in $1.5<z<8.5$ JADES galaxies
• The black hole masses of extremely luminous radio-WISE selected galaxies
• Shedding the envelope: JWST reveals a kiloparsec-scale [OIII]-weak Balmer shell around a z=7.64 quasar
• On the parameter refinement of inflated exoplanets with large radius uncertainty based on TESS observations
• Cosmic X-ray surveys of Active Galactic Nuclei: synergy between X-ray and infrared observations
• The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization
• Clues from 4U 0142+61 on supernova fallback disc formation and precession
• Hot exozodiacal dust around Fomalhaut: The MATISSE perspective
• gaspery: Optimized Scheduling of Radial Velocity Follow-Up Observations for Active Host Stars
• Comprehensive analysis of TESS Full Orbital Phase Curve of WASP-121b
• SpectrAx: Spectral Search of Axion-Like Particles Using Multi-Band Observations of Galaxy Clusters from SKA, SO, CMB-S4 and eROSITA
• Supernovae at the cosmic dawn
• Reionization relics in the cross-correlation between the Ly$\alpha$ forest and 21 cm intensity mapping in the post-reionization era
• Analysis of the Intrinsic Mid-Infrared L-band to Visible--Near-Infrared Flux Ratios in Spectral Synthesis Models of Composite Stellar Populations
• Searching for signatures of chaos in gamma-ray light curves of selected Fermi-LAT blazars
• X-ray Unveiling Events in a z~1.6 Active Galactic Nucleus in the 7 Ms Chandra Deep Field-South
• L 363-38 b: a planet newly discovered with ESPRESSO orbiting a nearby M dwarf star
• Stellar activity and transits
• Rapid Spectral Parameter Prediction for Black Hole X-Ray Binaries using Physicalised Autoencoders
• Time Evolution of Mg II in SDSS J2320+0024: Implications for a Subparsec Binary Supermassive Black Hole System
• Classifying merger stages with adaptive deep learning and cosmological hydrodynamical simulations
• Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies
• Through the fog: a complementary optical galaxy classification scheme for 'intermediate' redshifts
• Search for Exoplanetary Ring Systems with TESS
• Cosmic wallflowers: the circumgalactic origins of isolated ultra-compact star clusters at $z>7$
• Ultra High-Redshift or Closer-by, Dust-Obscured Galaxies? Deciphering the Nature of Faint, Previously Missed F200W-Dropouts in CEERS
• SPECULOOS: five years hunting terrestrial planets around ultra-cool dwarfs
• Can the James Webb Space Telescope detect isolated population III stars?
• Unveiling the Dark Side of UV/Optical Bright Galaxies: Optically Thick Dust Absorption
• Detecting Bosonic Dark Matter with Neutron Stars
• Distinctive Electronic Characteristics and Ultra-high Thermoelectric Power Factor in Be-Fe Intermetallics
• Increased Surface Temperatures of Habitable White Dwarf Worlds Relative to Main-Sequence Exoplanets
• Planetary architectures under the influence of a stellar binary
• State Space Modelling for detecting and characterising Gravitational Waves afterglows
• Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
• High resolution Spectra of Earth-Like Planets Orbiting Red Giant Host Stars
• SPHEREx: Aromatics, Aliphatics and PAH Size across the Iris Nebula
• EDGES of the dark forest: A new absorption window into the composite dark matter and large scale structure
• On the long-term evolution of razor-thin galactic discs: Balescu-Lenard prediction and perspectives
• Rapid characterization of exoplanet atmospheres with the Exoplanet Transmission Spectroscopy Imager (ETSI)
• Testing Photometric Techniques for Measuring the Rest-Frame UV Spectral Slope Against JWST PRISM Spectroscopy
• Observing galaxy mergers at the epoch of reionization
• On possible life-dispersal patterns beyond the Earth
• From atomic physics, to upper-atmospheric chemistry, to cosmology: A "laser photometric ratio star" to calibrate telescopes at major observatories
• Galactic Component Mapping of Galaxy UGC 2885 by Machine Learning Classification
• An ACA 1mm survey of HzRGs in the ELAIS-S1: survey description and first results
• Mechanical cosmology: simulating scalar fluctuations in expanding Universes using synthetic mechanical lattices
• Star Formation for Predictive Primordial Galaxy Formation
• Cophasing multiple aperture telescopes with Linearized Analytic Phase Diversity (LAPD)
• Radiative Flux from a High-Resolution Atmospheric Dynamics Simulation of a Hot-Jupiter for JWST and Ariel
• Type Ia Supernovae from First-generation Stars
• Global climate by Rossby number in the Solar system planets
• Compact dust-obscured star-formation and the origin of the galaxy bimodality
• Exoplanets: Possible Biosignatures
• Direct measurement of ISM proper motion with image registration
• The impact of the free-floating planet (FFP) mass function on the event rate for the accurate microlensing parallax determination: application to Euclid and Roman parallax observation
• Cosmic Dragons: A Two-Component Mixture Model of COSMOS Galaxies
• "Observations" of simulated dwarf galaxies: Star-formation histories from color-magnitude diagrams
• Planetary Exploration Horizon 2061 Report, Chapter 4: From planetary exploration goals to technology requirements
• Peculiar black hole accretion rates in AGN with highest star formation rates in the universe
• An EUV Non-Linear Optics Based Approach to Study the Photochemical Processes of Titanś Atmosphere
• The fate of the progenitors of luminous red novae: Infrared detection of LRNe years after the outburst
• Discovery of a transiting hot water-world candidate orbiting Ross 176 with TESS and CARMENES
• The CHEOPS view of HD 95338b: refined transit parameters, and a search for exomoons
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• The dark and featureless surface of rocky exoplanet LHS 3844 b from JWST mid-infrared spectroscopy
• The GAPS programme at TNG LXXI. A sub-Neptune suitable for atmospheric characterization in a multiplanet and mutually inclined system orbiting the bright K dwarf TOI-5789 (HIP 99452)
• Using Strong Lensing to Detect Subhalos with Steep Inner Density Profiles
• Synergies between space telescopes in the photometric characterization of the atmospheres of Hot Jupiters
• The TESS-Keck Survey. XIX. A Warm Transiting Sub-Saturn Mass Planet and a non-Transiting Saturn Mass Planet Orbiting a Solar Analog
• Deep Inelastic Scattering in the Capture of Dark Matter by Neutron Stars
• Reflections on "Can AI Understand Our Universe?"
• Flexible Simulation Based Inference for Galaxy Photometric Fitting with Synthesizer
• Linear response of rotating and flattened stellar clusters: the oblate Kuzmin-Kutuzov Stäckel family
• High-Redshift Galactic Outflows: Orientation Effects, Kinematics, and Metallicity in TNG50 and SERRA
• The impact of lunar topography on the 21-cm power spectrum for grid-based arrays : Insights for the Dark-ages EXplorer (DEX)
• Serendipitous observation of a white dwarf companion to a JWST/MIRI coronagraphic calibrator
• The Herschel-SPIRE Dark Field I: The deepest Herschel image of the submillimetre Universe
• Exotic Image Formation in Strong Gravitational Lensing by Clusters of Galaxies -- III: Statistics with HUDF
• A Panchromatic JWST Spectrum of a Giant Starspot on the Fully Convective M-dwarf TOI-3884
• Ultra-compact X-ray Binaries: A Review
• The SNIa Runaway LP 398-9: Detection of Circumstellar Material and Surface Rotation
• TOI-4552 b: A new ultra-short period rocky world revealed by NIRPS and TESS
• Enhancing Ground-Based Observations of Trans-Neptunian Objects using a Single-Epoch Parallax Measurement from L2
• Hot Rocks Survey V: Secondary Eclipse Photometry of GJ 3473 b with JWST/MIRI
• A search for transit timing variations in the transiting hot Jupiter systems HIP 65, NGTS-6, NGTS-10 and WASP-173
• Direct Imaging Discovery of Giant Exoplanet $\beta$ Pictoris d: A Decade-Long Game of Hide-and-Seek
• The Detection Prospect of the Counter Jet Radiation in the Late Afterglow of GRB 170817A
• TOI-6884b: A low-mass brown dwarf transiting a slightly evolved star
• Enhancing Gravitational Lens Study with Deep Learning: A Study on Effects of Dropout Regularization
• Research on the Interstellar Medium and Star Formation in the Galaxy: An Indian Perspective
• $\text{Exoformer}$: Accelerating Bayesian atmospheric retrievals with transformer neural networks
• Nonlinear backstepping with saturation for low-thrust station-keeping of libration point orbits
• Towards the exploration of astrophysical datacubes through volumetric rendering within CARTA
• A machine learning approach to estimate mid-infrared fluxes from WISE data
• The Dyson Minds 2025 Workshop: SETI around Black Holes
• Studying the spectral properties of Active Galactic Nuclei in the JWST era
• Observing Planetary Rings with JWST: Science Justification and Observation Requirements
• Correlated Read Noise Reduction in Infrared Arrays Using Deep Learning
• Analytical transit light curves for arbitrary power-law limb darkening: a unified framework
• The James Webb Space Telescope Absolute Flux Calibration. I. Program Design and Calibrator Stars
• 3D models of the circumstellar environments of evolved stars: Formation of multiple spiral structures
• VIZSLA -- Versatile Ice Zigzag Sublimation Setup for Laboratory Astrochemistry
• The impact of the presence of water ice on the analysis of debris disk observations
• Low-dimensional platforms for single photon detection
• Predicting large scale cosmological structure evolution with generative adversarial network-based autoencoders
• Finding High-Redshift Galaxies with JWST
• Optimizing Foreground Modelling for Global 21cm Cosmology with GPU-Accelerated Nested Sampling
• The role of young and evolved stars in the heating of dust in local galaxies
• Dust and gas modelling in radiative transfer simulations of disc-dominated galaxies with RADMC-3D
• Everything Every Band All at Once I: A Global Morphology Catalog in Abell 2744 based on UNCOVER/MegaScience
• A novel sub-grid model for super-Eddington accretion of spinning black holes in galaxy-scale simulations
• Building A Field: The Future of Astronomy with Gravitational Waves, A State of The Profession Consideration for Astro2020
• Capability for detection of GW190521-like binary black holes with TianQin
• The Observational Effects and Signatures of Tidally Distorted Solid Exoplanets
• Future Architecture of the Interplanetary Internet
• Bouncing Cosmologies in modified gravity with space time torsion
• Spectral Map Making with SPHEREx
• H2 MAGIE: H2 as a Major Agent to Galaxy Interaction and Evolution
• Rapid and Predictive Planet Population Synthesis Model (RAPPS) I. Upgraded model and resulting synthetic populations
• Oxyster: A Circumgalactic Low-ionization Oxygen Nebula next to a Starburst Galaxy at $z\sim 1$
• Extreme equivalent width-selected low-mass starbursts at $z=4-9$: insights into their role in cosmic reionization
• Stellar flare-driven evolution of primordial early exo-Earth atmospheres: Insights from a Young M Dwarf Flare model
• Analysing the flux stability of stellar calibrator candidates with TESS
• Challenges in Stellar Population Studies
• Massive black holes in the first billion years with JWST
• Searching for technosignatures in exoplanetary systems with current and future missions
• Large Language Model-driven Analysis of General Coordinates Network (GCN) Circulars
• Spectral Hardness as the Primary Discriminator: Unveiling the Collapsar--Merger Boundary with a Gold-Standard Gamma-Ray Burst Sample
• A Simple Condition for Sustained Super-Eddington Black Hole Growth