X-ray spectral modelling of the AGN obscuring region in the CDFS: Bayesian model selection and catalogue

Abstract

AGN are known to have complex X-ray spectra that depend on both the properties of the accreting SMBH (e.g. mass, accretion rate) and the distribution of obscuring material in its vicinity ("torus"). Often however, simple and even unphysical models are adopted to represent the X-ray spectra of AGN. In the case of blank field surveys in particular, this should have an impact on e.g. the determination of the AGN luminosity function, the inferred accretion history of the Universe and also on our understanding of the relation between AGN and their host galaxies. We develop a Bayesian framework for model comparison and parameter estimation of X-ray spectra. We take into account uncertainties associated with X-ray data and photometric redshifts. We also demonstrate how Bayesian model comparison can be used to select among ten different physically motivated X-ray spectral models the one that provides a better representation of the observations. Despite the use of low-count spectra, our methodology is able to draw strong inferences on the geometry of the torus. For a sample of 350 AGN in the 4 Ms Chandra Deep Field South field, our analysis identifies four components needed to represent the diversity of the observed X-ray spectra: (abridged). Simpler models are ruled out with decisive evidence in favour of a geometrically extended structure with significant Compton scattering. Regarding the geometry of the obscurer, there is strong evidence against both a completely closed or entirely open toroidal geometry, in favour of an intermediate case. The additional Compton reflection required by data over that predicted by toroidal geometry models, may be a sign of a density gradient in the torus or reflection off the accretion disk. Finally, we release a catalogue with estimated parameters such as the accretion luminosity in the 2-10 keV band and the column density, $N_H$, of the obscurer.

28 pages, 18 figures, catalogue available from https://www.mpe.mpg.de/~jbuchner/agn_torus/analysis/cdfs4Ms_cat/, software available from https://github.com/JohannesBuchner/BXA

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• Into the UV: The Atmosphere of the Hot Jupiter HAT-P-41b Revealed
• Evidence that the Hot Jupiter WASP-77 A b Formed Beyond Its Parent Protoplanetary Disk's H2O Ice Line
• TOI-481 b & TOI-892 b: Two long period hot Jupiters from the Transiting Exoplanet Survey Satellite
• Simultaneous Inference of Neutron Star Equation of State and the Hubble Constant with a Population of Merging Neutron Stars
• NGC 300 ULX1: A test case for accretion torque theory
• Bayesian Evidences for Dark Energy models in light of current obsevational data
• Early Insights for Atmospheric Retrievals of Exoplanets using JWST Transit Spectroscopy
• The Hubble WFC3 Emission Spectrum of the Extremely-Hot Jupiter, KELT-9b
• Retrieving the C and O Abundances of HR 7672~AB: a Solar-Type Primary Star with a Benchmark Brown Dwarf
• Bayesian constraints on the origin and geology of exo-planetary material using a population of externally polluted white dwarfs
• Global Fit of Modified Quark Couplings to EW Gauge Bosons and Vector-Like Quarks in Light of the Cabibbo Angle Anomaly
• 15NH3 in the atmosphere of a cool brown dwarf
• Dust attenuation evolution in $z\sim 2$-$12$ JWST galaxies
• Synchrotron Radiation Dominates the Extremely Bright GRB 221009A
• Bayesian Model Comparison and Analysis of the Galactic Disk Population of Gamma-Ray Millisecond Pulsars
• The XXL Survey: VI. The 1000 brightest X-ray point sources
• Cosmological perturbations in the Tsallis holographic dark energy scenarios
• First constraints on the AGN X-ray luminosity function at $z\sim 6$ from an eROSITA-detected quasar
• The Magellan-TESS Survey I: Survey Description and Mid-Survey Results
• Towards rapid transient identification and characterization of kilonovae
• The CARMENES search for exoplanets around M dwarfs. Characterization of the nearby ultra-compact multiplanetary system YZ Ceti
• On the contamination of the global 21~cm signal from polarized foregrounds
• New perspectives on the BOSS small-scale lensing discrepancy for the Planck $\Lambda$CDM Cosmology
• The Star Formation History of the Milky Way's Nuclear Star Cluster
• Asymmetric spatial distribution of sub-solar metallicity stars in the Milky Way nuclear star cluster
• New binary black hole mergers in the LIGO-Virgo O3b data
• Illuminating the past 8 billion years of cold gas towards two gravitationally lensed quasars
• Neutrino Mass Priors for Cosmology from Random Matrices
• Constraining the Properties of the Thermonuclear Burst Oscillation Source XTE J1814-338 Through Pulse Profile Modelling
• Assessment of Supervised Machine Learning for Atmospheric Retrieval of Exoplanets
• An independent analysis of the Spitzer/IRAC phase curves of WASP43 b
• Strong lensing reveals jets in a sub-microJy radio quiet quasar
• On the Chemical Abundance of HR 8799 and the Planet c
• Extragalactic FXT Candidates Discovered by Chandra (2014-2022)
• X-ray constraints on the fraction of obscured AGN at high accretion luminosities
• On the halo-mass and radial scale dependence of the lensing is low effect
• The MAVERIC Survey: Chandra/ACIS Catalog of Faint X-ray sources in 38 Galactic globular clusters
• Updated Results on the Galaxy-Halo Connection from Satellite Kinematics in SDSS
• Transmission spectroscopy for the warm sub-Neptune HD3167c: evidence for molecular absorption and a possible high metallicity atmosphere
• XZ: Deriving redshifts from X-ray spectra of obscured AGN
• Retrieving C and O Abundance of HR 8799 c by Combining High- and Low-Resolution Data
• The stellar metallicities of massive quiescent galaxies at 1.0 < z < 1.3 from KMOS+VANDELS
• Probing Quarkyonic Matter in Neutron Stars with the Bayesian Nuclear-Physics Multi-Messenger Astrophysics Framework
• HST PanCET Program: A Complete Near-UV to Infrared Transmission Spectrum for the Hot Jupiter WASP-79b
• On velocity-dependent dark matter annihilations in dwarf satellites
• Black hole spectroscopy horizons for current and future gravitational wave detectors
• Eccentric Companions to Kepler-448b and Kepler-693b: Clues to the Formation of Warm Jupiters
• A direct measurement of tomographic lensing power spectra from CFHTLenS
• JADES: Primaeval Lyman-$\alpha$ emitting galaxies reveal early sites of reionisation out to redshift $z\sim 9$
• Exomoon Candidates from Transit Timing Variations: Eight Kepler systems with TTVs explainable by photometrically unseen exomoons
• Investigating photometric and spectroscopic variability in the multiply-imaged Little Red Dot A2744-QSO1
• Isotropy of low redshift type Ia Supernovae: A Bayesian analysis
• Detection and timing of gamma-ray pulsations from the $707$ Hz pulsar J0952$-$0607
• Bayesian inference of signatures of hyperons inside neutron stars
• A warm Jupiter transiting an M dwarf: A TESS single transit event confirmed with the Habitable-zone Planet Finder
• Exploring the GRB population: Robust afterglow modelling
• The GAPS Programme at TNG XXVII. Reassessment of a young planetary system with HARPS-N: is the hot Jupiter V830 Tau b really there?
• Asymmetric Surface Brightness Structure of Caustic Crossing Arc in SDSS J1226+2152: A Case for Dark Matter Substructure
• TOI-269 b: An eccentric sub-Neptune transiting a M2 dwarf revisited with ExTrA
• Gaussian Process Regression for foreground removal in HI intensity mapping experiments
• Superplot: a graphical interface for plotting and analysing MultiNest output
• A Highly Eccentric Warm Jupiter Orbiting TIC 237913194
• Survey of ortho-H${}_2$D${}^{+}$ in high-mass star-forming regions
• Constraints on $S_8$ from a full-scale and full-shape analysis of redshift-space clustering and galaxy-galaxy lensing in BOSS
• Escaping Helium and a Highly Muted Spectrum Suggest a Metal-Enriched Atmosphere on Sub-Neptune GJ3090b from JWST Transit Spectroscopy
• Priors on Lagrangian bias parameters from galaxy formation modelling
• The vertical structure of debris disks and the impact of gas
• A Comprehensive Analysis of WASP-17b's Transmission Spectrum from Space-Based Observations
• Physically motivated X-ray obscurer models
• Exploring and Validating Exoplanet Atmospheric Retrievals with Solar System Analog Observations
• Considerations for Atmospheric Retrieval of High-Precision Brown Dwarf Spectra
• Exploring the likelihood of the 21-cm power spectrum with simulation-based inference
• The ESO SupJup Survey I: Chemical and isotopic characterisation of the late L-dwarf DENIS J0255-4700 with CRIRES${}^{+}$
• A direct comparison of X-ray spectral models for tori in active galactic nuclei
• The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
• The Swift Bulge Survey: Motivation, Strategy, and First X-ray Results
• PyAutoFit: A Classy Probabilistic Programming Language for Model Composition and Fitting
• The ESO SupJup Survey III: Confirmation of 13CO in YSES 1 b and Atmospheric Detection of YSES 1 c with CRIRES+
• Inferring gas-phase metallicity gradients of galaxies at the seeing limit: A forward modelling approach
• The First Large Absorption Survey in HI (FLASH): I. Science Goals and Survey Design
• Aura-3D: A Three-dimensional Atmospheric Retrieval Framework for Exoplanet Transmission Spectra
• Testing the disk-corona interplay in radiatively-efficient broad-line AGN
• Differentiating Modern and Prebiotic Earth Scenarios for TRAPPIST-1e: High-resolution Transmission Spectra and Predictions for JWST
• A Sensitive Search for Supernova Emission Associated with the Extremely Energetic and Nearby GRB 221009A
• Is the atmosphere of the ultra-hot Jupiter WASP-121b variable?
• Spectral energy distribution and radio halo of NGC 253 at low radio frequencies
• A sub-Neptune and a non-transiting Neptune-mass companion unveiled by ESPRESSO around the bright late-F dwarf HD 5278 (TOI-130)
• A New Measurement of the Spectral Lag of Gamma-Ray Bursts and its Implications for Spectral Evolution Behaviors
• Implications of hidden gauged $U(1)$ model for $B$ anomalies
• High-precision search for dark photon dark matter with the Parkes Pulsar Timing Array
• Retrieval study of cool, directly imaged exoplanet 51 Eri b
• TESS Reveals a Short-period Sub-Neptune Sibling (HD 86226c) to a Known Long-period Giant Planet
• The Optical/Near-Infrared Extinction Law In Highly Reddened Regions
• An Unusual Transmission Spectrum for the Sub-Saturn KELT-11b Suggestive of a Sub-Solar Water Abundance
• The VANDELS survey: A strong correlation between Ly$\alpha$ equivalent width and stellar metallicity at $3\le \mathbf{z}\le 5$
• Triggering the Untriggered: The First Einstein Probe-Detected Gamma-Ray Burst 240219A and Its Implications
• Observational Constraints on Axion(s) Dark Energy with a Cosmological Constant
• Constraining short gamma-ray burst jet properties with gravitational waves and gamma rays
• An exploration of model degeneracies with a unified phase curve retrieval analysis: The light and dark sides of WASP-43 b
• Bayesian reconstruction of nuclear matter parameters from the equation of state of neutron star matter
• The Tucana dwarf spheroidal galaxy: not such a massive failure after all
• On the moment of inertia of PSR J0737-3039 A from LIGO/Virgo and NICER
• The Galactic Center: Improved Relative Astrometry for Velocities, Accelerations, and Orbits near the Supermassive Black Hole
• Near-infrared transmission spectrum of TRAPPIST-1 h using Hubble WFC3 G141 observations
• Atmospheric Effects on Neutron Star Parameter Constraints with NICER
• The challenge of measuring the phase function of debris disks. Application to HR\,4796
• The eROSITA Final Equatorial-Depth Survey (eFEDS): A multiwavelength view of WISE mid-infrared galaxies/active galactic nuclei
• The MOPYS project: A survey of 70 planets in search of extended He I and H atmospheres. No evidence of enhanced evaporation in young planets
• Spectropolarimetric variability in the repeating fast radio burst source FRB 20180301A
• Low frequency view of GRB 190114C reveals time varying shock micro-physics
• JWST/NIRCam discovery of the first Y+Y brown dwarf binary: WISE J033605.05$-$014350.4
• Multimessenger parameter estimation of GW170817: from jet structure to the Hubble constant
• Community targets for JWST's early release science program: evaluation of WASP-63b
• Inflation Model Selection meets Dark Radiation
• Nearly model-independent constraints on dense matter equation of state in a Bayesian approach
• Systematic errors induced by the elliptical power-law model in galaxy-galaxy strong lens modeling
• HD 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone
• Investigating ULX accretion flows and cyclotron resonance in NGC 300 ULX1
• NPTFit: A code package for Non-Poissonian Template Fitting
• Spectropolarimetric analysis of an active region filament. I. Magnetic and dynamical properties from single component inversions
• ExoReL${}^{\Re }$: A Bayesian Inverse Retrieval Framework For Exoplanetary Reflected Light Spectra
• Measuring the mass of the black widow PSR J1555-2908
• Sulfur Chemistry in L1157-B1
• The MUSE-Faint survey. II. The dark matter-density profile of the ultra-faint dwarf galaxy Eridanus 2
• Brightest galaxies as halo centre tracers in SDSS DR7
• Cosmological Evidence Modelling: a new simulation-based approach to constrain cosmology on non-linear scales
• Multiple Clues for Dayside Aerosols and Temperature Gradients in WASP-69 b from a Panchromatic JWST Emission Spectrum
• How Much Information Does the Sodium Doublet Encode? Retrieval Analysis of Non-LTE Sodium Lines at Low and High Spectral Resolutions
• Detecting the proposed CH4-CO2 biosignature pair with the James Webb Space Telescope: TRAPPIST-1e and the effect of cloud/haze
• K2-231 b: A sub-Neptune exoplanet transiting a solar twin in Ruprecht 147
• Dark energy reconstruction based on the PADE approximation; an expansion around the $\Lambda$CDM
• H- and Dissociation in Ultra-hot Jupiters: A Retrieval Case Study of WASP-18b
• Systematic analysis of the impacts of symmetry energy parameters on neutron star properties
• Cloud-by-cloud, multiphase, Bayesian modeling: Application to four weak, low ionization absorbers
• Warm and Cold Molecular Gas Conditions Modeled in 87 Galaxies Observed by the Herschel SPIRE Fourier Transform Spectrometer
• Narrowing down the possible explanations of cosmic acceleration with geometric probes
• ACCESS: A Visual to Near-infrared Spectrum of the Hot Jupiter WASP-43b with Evidence of ${\mathrm{H}}_2\mathrm{O}$, but no evidence of Na or K
• Detection of Na in WASP-21b's lower and upper atmosphere
• The Cosmic Ultraviolet Baryon Survey (CUBS) IV: The Complex Multiphase Circumgalactic Medium as Revealed by Partial Lyman Limit Systems
• Five young $\delta$ Scuti stars in the Pleiades seen with Kepler/K2
• Dim but not entirely dark: Extracting the Galactic Center Excess' source-count distribution with neural nets
• Apprentice for Event Generator Tuning
• Source properties of the lowest signal-to-noise-ratio binary black hole detections
• The Gaia-ESO Survey: Dynamical models of flattened, rotating globular clusters
• Binary companions of nearby supernova remnants found with Gaia
• Leptonic Unitarity Triangles
• The demographics of obscured AGN from X-ray spectroscopy guided by multiwavelength information
• Observing Supermassive Black Holes across cosmic time: from phenomenology to physics
• HST/STIS transmission spectrum of the ultra-hot Jupiter WASP-76 b confirms the presence of sodium in its atmosphere
• Parameter estimation for strong phase transitions in supranuclear matter using gravitational-wave astronomy
• Probing Early Universe Supercooled Phase Transitions with Gravitational Wave Data
• Bayesian Analysis of Molecular Emission and Dust Continuum of Protoplanetary Disks
• Effects of type Ia supernovae absolute magnitude priors on the Hubble constant value
• TOI-1231 b: A Temperate, Neptune-Sized Planet Transiting the Nearby M3 Dwarf NLTT 24399
• Hubble Space Telescope Observations of [O~III] Emission in Nearby QSO2s: Physical Properties of the Ionised Outflows
• Discovery of a disrupting open cluster far into the Milky Way halo: a recent star formation event in the leading arm of the Magellanic stream?
• DAMPE squib? Significance of the 1.4 TeV DAMPE excess
• Growth of matter perturbations in the extended viscous dark energy models
• The eROSITA Final Equatorial Depth Survey (eFEDS): Complex absorption and soft excesses in hard X-ray--selected active galactic nuclei
• Integrating light-curve and atmospheric modelling of transiting exoplanets
• An Infrared Search for Kilonovae with the WINTER Telescope. I. Binary Neutron Star Mergers
• Spitzer Reveals Evidence of Molecular Absorption in the Atmosphere of the Hot Neptune LTT 9979b
• How Does Thermal Scattering Shape the Infrared Spectra of Cloudy Exoplanets? A Theoretical Framework and Consequences for Atmospheric Retrievals in the JWST era
• Gamma-ray emission from the impulsive phase of the 2017 September 06 X9.3 flare
• The Detectability and Constraints of Biosignature Gases in the Near & Mid-Infrared from Transit Transmission Spectroscopy
• The space density of Compton-thick AGN at z~0.8 in the zCOSMOS-Bright Survey
• TOI-150b and TOI-163b: two transiting hot Jupiters, one eccentric and one inflated, revealed by TESS near and at the edge of the JWST CVZ
• Long-term and multi-wavelength evolution of a changing-look AGN Mrk 1018
• Ticking away: the long-term X-ray timing and spectral evolution of eRO-QPE2
• GJ357: A low-mass planetary system uncovered by precision radial-velocities and dynamical simulations
• Detection of a high-redshift molecular outflow in a primeval hyperstarburst galaxy
• XXL-HSC: The link between AGN activity and star formation in the Early Universe ($z⩾3.5$)
• A comparative study of WASP-67b and HAT-P-38b from WFC3 data
• LBT transmission spectroscopy of HAT-P-12b: confirmation of a cloudy atmosphere with no significant alkali features
• Charming Dark Matter
• The population of tidal disruption events discovered with eROSITA
• GRAVITY K-band spectroscopy of HD 206893 B: brown dwarf or exoplanet
• A Physical Background Model for the Fermi Gamma-ray Burst Monitor
• Collapsars as Sites of r-process Nucleosynthesis: Systematic Near-Infrared Follow-up of Type Ic-BL Supernovae
• HATS-54b-HATS-58Ab: five new transiting hot Jupiters including one with a possible temperate companion
• Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars
• An External Shock Origin of GRB $\text{141028A}$
• Silicate clouds and a circumplanetary disk in the YSES-1 exoplanet system
• Three new brown dwarfs and a massive hot Jupiter revealed by TESS around early-type stars
• Naturalness of the relaxion mechanism
• ACCESS: Ground-based Optical Transmission Spectroscopy of the Hot Jupiter WASP-4b
• An exquisitely deep view of quenching galaxies through the gravitational lens: Stellar population, morphology, and ionized gas
• Water depletion and 15NH3 in the atmosphere of the coldest brown dwarf observed with JWST/MIRI
• TOI-2257 b: A highly eccentric long-period sub-Neptune transiting a nearby M dwarf
• The HD 137496 system: A dense, hot super-Mercury and a cold Jupiter
• Is Spectral Width a Reliable Measure of GRB Emission Physics?
• A transmission spectrum of the sub-Earth planet L98-59~b in 1.1-1.7 $\mu$m
• Radiative Driving of the AGN Outflows in the Narrow-Line Seyfert 1 Galaxy NGC 4051
• Using High-Energy Neutrinos As Cosmic Magnetometers
• The seven sisters DANCe IV. Bayesian hierarchical model
• MIGHTEE-HI: The first MeerKAT HI mass function from an untargeted interferometric survey
• Discovery of the luminous X-ray ignition eRASSt J234402.9$-$352640; I. Tidal disruption event or a rapid increase in accretion in an active galactic nucleus?
• Probing the Physics of Star-Formation (ProPStar): II. The first systematic search for streamers toward protostars
• Quintessential Cosmological Tensions
• Planetary system around LTT 1445A unveiled by ESPRESSO: Multiple planets in a triple M-dwarf system
• A model for redistributing heat over the surface of irradiated spider companions
• Tentative Evidence for Water Vapor in the Atmosphere of the Neptune-Size Exoplanet HD 106315 c
• Nested sampling cross-checks using order statistics
• Incorporating Astrochemistry into Molecular Line Modelling via Emulation
• Exoplanet Interior Retrievals: core masses and metallicities from atmospheric abundances
• Bayesian comparison of nonstandard cosmologies using type Ia supernovae and BAO data
• The Quintuplet Cluster: Extended Structure and Tidal Radius
• Mapping the Likelihood of GW190521 with Diverse Mass and Spin Priors
• A 62-minute orbital period black widow binary in a wide hierarchical triple
• Supernovae evidence for foundational change to cosmological models
• The quadrupole in the local Hubble parameter: first constraints using Type Ia supernova data and forecasts for future surveys
• Evidence of a Clear Atmosphere for WASP-62b: the Only Known Transiting Gas Giant in the JWST Continuous Viewing Zone
• HADES RV program with HARPS-N at TNG. IX. A super-Earth around the M dwarf Gl686
• A Bayesian quantification of consistency in correlated datasets
• X-ray redshifts for obscured AGN: a case study in the J1030 deep field
• Decoding Neutron Star Observations: Revealing Composition through Bayesian Neural Networks
• The cosmic evolution of the stellar mass$-$velocity dispersion relation of early-type galaxies
• BOWIE-ALIGN: JWST reveals hints of planetesimal accretion and complex sulphur chemistry in the atmosphere of the misaligned hot Jupiter WASP-15b
• Investigating the Narrow Line Region Dynamics in Nearby Active Galaxies
• Strong constraints on a simple self-interacting neutrino cosmology
• Hubble WFC3 Spectroscopy of the Terrestrial Planets L~98-59~c \& d: No Evidence for a Clear Hydrogen Dominated Primary Atmosphere
• Confirmation of an He I evaporating atmosphere around the 650-Myr-old sub-Neptune HD235088 b (TOI-1430 b) with CARMENES
• Transmission spectroscopy of the ultra-hot Jupiter MASCARA-4 b: Disentangling the hydrostatic and exospheric regimes of ultra-hot Jupiters
• Probabilistic detection of spectral line components
• Dark Matter Density Profiles in Dwarf Galaxies: Linking Jeans Modeling Systematics and Observation
• The GAPS Programme at TNG XLII. A characterisation study of the multi-planet system around the 400 Myr-old star HD 63433 (TOI-1726)
• 7.1 keV sterile neutrino constraints from X-ray observations of 33 clusters of galaxies with Chandra ACIS
• Planet Formation around Super Massive Black Holes in the Active Galactic Nuclei
• A retrieval challenge exercise for the Ariel mission
• Across the Green Valley with HST grisms: colour evolution, crossing time-scales and the growth of the red sequence at $z=1.0-1.8$
• On spectroscopic phase-curve retrievals: H2 dissociation and thermal inversion in the atmosphere of the ultra-hot Jupiter WASP-103 b
• Hubble WFC3 Spectroscopy of the Rocky Planet L 98-59 b: No Evidence for a Cloud-Free Primordial Atmosphere
• JWST-TST High Contrast: Living on the Wedge, or, NIRCam Bar Coronagraphy Reveals CO${}_2$ in the HR 8799 and 51 Eri Exoplanets' Atmospheres
• Euclid: Effect of sample covariance on the number counts of galaxy clusters
• Self-calibration and robust propagation of photometric redshift distribution uncertainties in weak gravitational lensing
• A Complex Multiphase DLA Associated with a Compact Group at z=2.431 Traces Accretion, Outflows, and Tidal Streams
• Do Radio Active Galactic Nuclei Reflect X-ray Binary Spectral States?
• Orbital alignment of the eccentric warm Jupiter TOI-677 b
• Decomposition of galactic X-ray emission with Phox: Contributions from hot gas and XRBs
• An enhanced slope in the transmission spectrum of the hot Jupiter WASP-104b
• ACCESS: Confirmation of a Clear Atmosphere for WASP-96b and a Comparison of Light Curve Detrending Techniques
• Insufficient evidence for DMS and DMDS in the atmosphere of K2-18 b. From a joint analysis of JWST NIRISS, NIRSpec, and MIRI observations
• Euclid preparation. XLI. Galaxy power spectrum modelling in real space
• JWST-TST DREAMS: A Precise Water Abundance for Hot Jupiter WASP-17b from the NIRISS SOSS Transmission Spectrum
• Analysing the SEDs of protoplanetary disks with machine learning
• Recovering the Physical Properties of Molecular Gas in Galaxies from CO SLED Modeling
• Three-dimensional structure of the Sagittarius dSph core from RR Lyrae
• jetsimpy: A Highly Efficient Hydrodynamic Code for Gamma-ray Burst Afterglow
• AGN X-ray luminosity function and absorption function in the Early Universe ($3\le z\le 6$)
• Bayesian model comparison for simulation-based inference
• GRB 140102A: Insight into Prompt Spectral Evolution and Early Optical Afterglow Emission
• Extended $\Lambda$CDM model
• KiDS-1000 Cosmology: machine learning -- accelerated constraints on Interacting Dark Energy with COSMOPOWER
• Detection of Paschen $\beta$ absorption in the atmosphere of KELT-9 b: A new window into the atmospheres of ultra-hot Jupiters
• Characterising Atmospheres of Cloudy Temperate Mini-Neptunes with JWST
• Accretion History of AGN II: Constraints on AGN Spectral Parameters using the Cosmic X-ray Background
• Discovery and origins of giant optical nebulae surrounding quasar PKS 0454-22
• Challenges in the detection of gases in exoplanet atmospheres
• Large Interferometer For Exoplanets (LIFE): XIII. The Value of Combining Thermal Emission and Reflected Light for the Characterization of Earth Twins
• EXPRES. III. Revealing the Stellar Activity Radial Velocity Signature of $\epsilon$ Eridani with Photometry and Interferometry
• Stellar Spins in the Pleiades, Praesepe, and M35 Open Clusters
• Evidence for SiO cloud nucleation in the rogue planet PSO J318
• Constraining neutron star properties with a new equation of state insensitive approach
• Detecting Galaxy Groups and AGNs populating the local Universe in the eROSITA era
• Cosmological foundations revisited with Pantheon+
• Large Interferometer For Exoplanets (LIFE): IX. Assessing the Impact of Clouds on Atmospheric Retrievals at Mid-Infrared Wavelengths with a Venus-Twin Exoplanet
• HYMALAIA: A Hybrid Lagrangian Model for Intrinsic Alignments
• eROSITA cluster cosmology forecasts: cluster temperature substructure bias
• ACCESS: Confirmation of no potassium in the atmosphere of WASP-31b
• A Mirage or an Oasis? Water Vapor in the Atmosphere of the Warm Neptune TOI-674 b
• Nodal Precession and Tidal Evolution of Two Hot-Jupiters: WASP-33 b and KELT-9 b
• A quarter century of spectroscopic monitoring of the nearby M dwarf Gl 514. A super-Earth on an eccentric orbit moving in and out of the habitable zone
• Joint Observations of Space-based Gravitational-wave Detectors: Source Localization and Implication for Parity-violating gravity
• SPECIES II. Stellar parameters of the EXPRESS program giant star sample
• Multivariate Rational Approximation
• BAT AGN Spectroscopic Survey-XXIII. A New Mid-Infrared Diagnostic for Absorption in Active Galactic Nuclei
• Evidence for TiO in the atmosphere of the hot Jupiter HAT-P-65 b
• Maturing Satellite Kinematics into a Competitive Probe of the Galaxy-Halo Connection
• Extended $\Lambda$CDM model and viscous dark energy: A Bayesian analysis
• A binning-free method reveals a continuous relationship between galaxies' AGN power and offset from main sequence
• X-PSI Parameter Recovery for Temperature Map Configurations Inspired by PSR J0030+0451
• A Simplified Photodynamical Model for Planetary Mass Determination in Low-Eccentricity Multi-Transiting Systems
• The Fast X-ray Transient XRT 210423 and its Host Galaxy
• A Dissection of Spatially Resolved AGN Feedback across the Electromagnetic Spectrum
• MIGHTEE-HI: The HI mass-stellar mass relation over the last billion years
• A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE). VIII. Modeling ram pressure stripping of diffuse gas in the Virgo cluster spiral galaxy NGC 4330
• PdBI U/LIRG Survey (PULS): Dense Molecular Gas in Arp 220 and NGC 6240
• 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
• Beyond Simple AGN Unification with Chandra-observed 3CRR Sources
• GJ 806 (TOI-4481): A bright nearby multi-planetary system with a transiting hot, low-density super-Earth
• Four Jovian planets around low-luminosity giant stars observed by the EXPRESS and PPPS
• Optical follow-up of the tick-tock massive black hole binary candidate
• Stellar Populations in the Transition Region of Nuclear Star Cluster and Nuclear Stellar Disc
• A search for lensed gamma-ray bursts in 11 years of observations by Fermi GBM
• ALMA [N ıı] 205 μm Imaging Spectroscopy of the Lensed Submillimeter galaxy ID 141 at redshift 4.24
• Accretion properties of X-ray AGN: Evidence for radiation-regulated obscuration with redshift-dependent host galaxy contribution
• The transmission spectrum of WASP-17 b from the optical to the near-infrared wavelengths: combining STIS, WFC3 and IRAC datasets
• Detecting Biosignatures in the Atmospheres of Gas Dwarf Planets with the James Webb Space Telescope
• Constrains on the electric charges of the binary black holes with GWTC-1 events
• Inferring the morphology of AGN torus using X-ray spectra: A reliability study
• Detecting Globular Cluster Tidal Extensions with Bayesian Inference: I. Analysis of $\omega$ Centauri with Gaia EDR3
• Bayesian Inference of Reaction Rates in Icy Mantles
• A High Fraction of Heavily X-ray Obscured Active Galactic Nuclei
• JWST-TST High Contrast: JWST/NIRCam observations of the young giant planet $\beta$ Pic b
• Optical photometry of two transitional millisecond pulsars in the radio pulsar state
• Astrophysical interpretation of the anisotropies in the unresolved gamma-ray background
• Resolving phase transition properties of dense matter through tidal-excited g-mode from inspiralling neutron stars
• A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113
• A New Emulated Monte Carlo Radiative Transfer Disk-Wind Model: X-Ray Accretion Disk-wind Emulator -- XRADE
• A bottom-up search for Lyman-continuum leakage in the Hubble Ultra Deep Field
• Feasibility of dark matter admixed neutron star based on recent observational constraints
• TKS V. Twin sub-Neptunes Transiting the Nearby G Star HD 63935
• A simple parametrisation for coupled dark energy
• LESSER: A Catalogue of Spectroscopically selected sample of Lyman-$\alpha$ Emitters Lensed By Galaxies
• Relativistic accretion disk reflection in AGN X-ray spectra at z=0.5--4: a study of four \textit{Chandra} deep fields
• Impact of quasi-periodic and steep-spectrum timing noise on the measurement of pulsar timing parameters
• Transmission spectroscopy with VLT FORS2: a featureless spectrum for the low-density transiting exoplanet WASP-88b
• So close, so different: characterization of the K2-36 planetary system with HARPS-N
• eRASSt J074426.3+291606: prompt accretion disc formation in a 'faint and slow' tidal disruption event
• In Search of the Edge: A Bayesian Exploration of the Detectability of Red Edges in Exoplanet Reflection Spectra
• Chemical evolution of local post-starburst galaxies: Implications for the mass-metallicity relation
• X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z=6.56
• Featureless transmission spectra of 12 giant exoplanets observed by GTC/OSIRIS
• Super-Nyquist ultralight dark matter searches with broadband atom gradiometers
• Constraining the Gravitational-Wave Afterglow From a Binary Neutron Star Coalescence
• Spatially Resolved Outflows in a Seyfert Galaxy at z = 2.39
• TOI-179: a young system with a transiting compact Neptune-mass planet and a low-mass companion in outer orbit
• Simulation and physical model based gamma-ray burst afterglow analysis
• Black Hole Mass Function of Coalescing Binary Black Hole Systems: Is There a Pulsational Pair Instability Mass Cutoff?
• The Intrabinary Shock and Companion Star of Redback Pulsar J2215+5135
• An investigation of the circumgalactic medium around z~2.2 AGN with ACA and ALMA
• Forecasts on interacting dark energy with standard sirens
• Kinematic and metallicity properties od the Aquarius dwarf galaxy from FORS2 MXU spectroscopy
• JWST Observations of the Enigmatic Y Dwarf WISE 1828+2650: I. Limits to a Binary Companion
• Resolving the blazar CGRaBS J0809+5341 in the presence of telescope systematics
• Discovery and Timing of Millisecond Pulsars in the Globular Cluster M5 (NGC 5904) with FAST and Arecibo
• Time-resolved Hubble Space Telescope UV observations of an X-ray quasi-periodic eruption source
• Asteroseismology of $\delta$ Scuti stars: emulating model grids using a neural network
• Signs of Higher Multipoles and Orbital Precession in GW151226
• Time Resolved Absorption of Six Chemical Species With MAROON-X Points to Strong Drag in the Ultra Hot Jupiter TOI-1518 b
• Estimating the local dark matter density in a non-axisymmetric wobbling disc
• The Seven Sisters DANCe III: Projected spatial distribution
• Bayesian Comparison of the Cosmic Duality Scenarios
• Resolved Molecular Gas Observations of MaNGA Post-starbursts Reveal a Tumultuous Past
• The Sensitivity of Future Gamma-Ray Telescopes to Primordial Black Holes
• Blazar jet evolution revealed by multi-epoch broadband radio polarimetry
• Exploration of Parameter Spaces Assisted by Machine Learning
• Rainbow Cosmic Shear: Optimisation of Tomographic Bins
• EP241021a: a months-duration X-ray transient with luminous optical and radio emission
• Equation of state of nuclear matter and neutron stars: Quark mean-field model versus relativistic mean-field model
• A formally motivated retrieval framework applied to the high resolution transmission spectrum of HD 189733 b
• The JWST Weather Report: retrieving temperature variations, auroral heating, and static cloud coverage on SIMP-0136
• Probing fermionic asymmetric dark matter cores using global neutron star properties
• Fitting covariance matrix models to simulations
• Targeted search for the stochastic gravitational-wave background from the galactic millisecond pulsar population
• VVV-WIT-08: the giant star that blinked
• TOI-150: A transiting hot Jupiter in the TESS southern CVZ
• The effect of spin mismodeling on gravitational-wave measurements of the binary neutron star mass distribution
• WASP-121b's transmission spectrum observed with JWST/NIRSpec G395H reveals thermal dissociation and SiO in the atmosphere
• Hot planets around cool stars -- two short-period mini-Neptunes transiting the late K-dwarf TOI-1260
• Measuring the Orbits of the Arches and Quintuplet Clusters using HST and Gaia: Exploring Scenarios for Star Formation Near the Galactic Center
• Titanium chemistry of WASP-121 b with ESPRESSO in 4-UT mode
• Identification of a turnover in the initial mass function of a young stellar cluster down to 0.5 M${}_J$
• Atmospheric characterization of the super-Jupiter HIP 99770 b with KPIC
• Vertical wind structure in an X-ray binary revealed by a precessing accretion disk
• VLTI/GRAVITY Observations and Characterization of the Brown Dwarf Companion HD 72946 B
• A Bayesian Approach to the Vertical Structure of the Disk of the Milky Way
• A statistical measurement of the HI spin temperature in DLAs at cosmological distances
• Biases in retrieving planetary signals in the presence of quasi-periodic stellar activity
• A new software implementation of the Oslo method with rigorous statistical uncertainty propagation
• UNCOVERing the High-redshift AGN Population among Extreme UV Line Emitters
• Nonperturbative infrared finiteness in super-renormalisable scalar quantum field theory
• Far beyond stacking: Fully bayesian constraints on sub-microJy radio source populations over the XMM-LSS-VIDEO field
• Evidence for extended gaseous reservoirs around AGN at cosmic noon from ALMA CO(3-2) observations
• The SRG/eROSITA All-Sky Survey: X-ray beacons at late cosmic dawn
• Constraints on the dense matter equation of state and neutron star properties from NICER's mass-radius estimate of PSR J0740+6620 and multimessenger observations
• A Study of Stellar Spins in 15 Open Clusters
• Cross-Comparison of Sampling Algorithms for Pulse Profile Modeling of PSR J0740+6620
• Detection of TiO and VO in the atmosphere of WASP-121b and Evidence for its temporal variation
• Reflected spectroscopy of small exoplanets III: probing the UV band to measure biosignature gasses
• Footprints of population III stars in the gravitational-wave background
• Evidence for stellar contamination in the transmission spectra of HAT-P-12b
• Terminus: A Versatile Simulator for Space-based Telescopes
• Accelerating Bayesian microseismic event location with deep learning
• On the origin of the gamma-ray emission from Omega Centauri: Milisecond pulsars and dark matter annihilation
• Probing the physicochemical properties of the Leo Ring and the Leo I group
• Measuring the HI mass function below the detection threshold
• Bayesian model selection for GRB 211211A through multi-wavelength analyses
• A systematic validation of hot Neptunes in TESS data
• Knobs and dials of retrieving JWST transmission spectra. I. The importance of p-T profile complexity
• Ultra-deep ATCA imaging of 47 Tucanae reveals a central compact radio source
• Nonparametric Representation of Neutron Star Equation of State Using Variational Autoencoder
• The Exceptional X-ray Evolution of SN1996cr in High Resolution
• On the cosmic distance duality relation and the strong gravitational lens power law density profile
• A 5% measurement of the gravitational constant in the Large Magellanic Cloud
• The ESO SupJup Survey VII: Clouds and line asymmetries in CRIRES${}^{+}$ J-band spectra of the Luhman 16 binary
• Semi-analytic spectral fitting: simultaneously modelling the mass accumulation and chemical evolution in MaNGA spiral galaxies
• The optically-selected 1.4-GHz quasar luminosity function below 1 mJy
• Spectral Hardening Reveals Afterglow Emergence in Long-Duration Fast X-ray Transients: A Case Study of GRB 250404A/EP250404a
• A dense mini-Neptune orbiting the bright young star HD 18599
• The Most Obscured AGNs in the XMM-SERVS Fields
• K2-113b: A dense hot-Jupiter transiting a solar analogue
• Galaxy clustering from the bottom up: A Streaming Model emulator I
• Investigating subphotospheric dissipation in gamma-ray bursts using joint Fermi-Swift observations
• A multi-planetary system orbiting the early-M dwarf TOI-1238
• Establishing connection between neutron star properties and nuclear matter parameters through a comprehensive multivariate analysis
• The eROSITA Final Equatorial-Depth Survey (eFEDS): The first archetypal Quasar in the feedback phase discovered by eROSITA
• Improvement of the Helioseismic and Magnetic Imager (HMI) Vector Magnetic Field Inversion Code
• Tracing the formation and migration history: molecular signatures in the atmosphere of misaligned hot Jupiter WASP-94Ab using JWST NIRSpec/G395H
• Differences Between the Pierre Auger Observatory and Telescope Array Spectra: Systematic Effects or Indication of a Local Source of Ultra-High-Energy Cosmic Rays?
• Highly structured inner planetary system debris around the intermediate age Sun-like star TYC 8830 410 1
• EXPRES. II. Searching for Planets Around Active Stars: A Case Study of HD 101501
• MIRI-LRS spectrum of a cold exoplanet around a white dwarf: water, ammonia, and methane measurements
• A new approach to modelling gamma-ray burst afterglows: Using Gaussian processes to account for the systematics
• Do stellar-mass and super-massive black holes have similar dining habits?
• Testing the growth rate in homogeneous and inhomogeneous interacting vacuum models
• EDEN Survey: Small Transiting Planet Detection Limits and Constraints on the Occurrence Rates for Late M Dwarfs within 15 pc
• A Search for Neutrino Point-Source Populations in 7 Years of IceCube Data with Neutrino-count Statistics
• Scaling relations of z~0.25-1.5 galaxies in various environments from the morpho-kinematic analysis of the MAGIC sample
• The first look at Narrow-Line Seyfert 1 Galaxies with eROSITA
• The compositions of the HR 8799 planets reflect accretion of both solids and metal-enriched gas
• The SRG/eROSITA all-sky survey. X-ray emission from the warm-hot phase gas in long cosmic filaments
• Uncovering the Invisible: A Study of Gaia18ajz, a Candidate Black Hole Revealed by Microlensing
• Nambu-Jona-Lasinio description of hadronic matter from a Bayesian approach
• EasyScan_HEP: a tool for connecting programs to scan the parameter space of physics models
• Flavor constraints for a Vector-like quark of Nelson-Barr type
• The impact of neutron star spin on X-ray spectra
• Revisiting the Transit Timing Variations in the TrES-3 and Qatar-1 systems with TESS data
• Jupiter-like uniform metal enrichment in a system of multiple giant exoplanets
• The puzzle of the formation of T8 dwarf Ross 458c
• A Circumplanetary Dust Ring May Explain the Extreme Spectral Slope of the 10 Myr Young Exoplanet K2-33b
• The eROSITA Final Equatorial Depth Survey (eFEDS): the hard X-ray selected sample
• Fundamental Physics with ESPRESSO, Constraining a simple parametrisation for varying $\alpha$
• Monitoring clumpy wind accretion in supergiant fast X-ray transients with XMM-Newto
• One Fits All: A Unified Synchrotron Model Explains GRBs with FRED-Shaped Pulses
• The Chemical Composition of Extreme-Velocity Stars
• Estimation of singly-transiting K2 planet periods with Gaia parallaxes
• Obscuration properties of mid-IR selected AGN
• The multi-epoch X-ray tale of I Zwicky 1 outflows
• Discovery of two promising isolated neutron star candidates in the SRG/eROSITA All-Sky Survey
• AGN in the CALIFA survey: X-ray detection of nuclear sources
• Prospects for Distinguishing Dark Matter Models Using Annual Modulation
• IGRINS observations of WASP-127 b: H${}_2$O, CO, and super-Solar atmospheric metallicity in the inflated sub-Saturn
• A deep radio view of the evolution of the cosmic star-formation rate density from a stellar-mass selected sample in VLA-COSMOS
• ACCESS: An optical transmission spectrum of the high-gravity, hot Jupiter HAT-P-23b
• RV-exoplanet eccentricities: Good, Beta, and Best
• The eROSITA Final Equatorial-Depth Survey (eFEDS): An X-ray bright, extremely luminous infrared galaxy at z = 1.87
• The effect of inhomogeneities on dark energy constraints
• Unrecognized Astrometric Confusion in the Galactic Centre
• KiDS+VIKING-450: An internal-consistency test for cosmic shear tomography with a colour-based split of source galaxies
• Detection of Na and K in the atmosphere of the hot Jupiter HAT-P-1b with P200/DBSP
• X-ray diagnostics of Cassiopeia A's "Green Monster": evidence for dense shocked circumstellar plasma
• PRIMER & JADES reveal an abundance of massive quiescent galaxies at 2 < z < 5
• Impacts of high-contrast image processing on atmospheric retrievals
• Polarized radiation from an accretion shock in accreting millisecond pulsars using exact Compton scattering formalism
• TD-CARMA: Painless, accurate, and scalable estimates of gravitational-lens time delays with flexible CARMA processes
• The Global Magneto-Ionic Medium Survey (GMIMS): The brightest polarized region in the Southern sky at 75cm and its implications for Radio Loop II
• New JWST redshifts for the host galaxies of CDF-S XT1 and XT2: understanding their nature
• WASP-35 and HAT-P-30/WASP-51: re-analysis using TESS and ground-based transit photometry
• A precise blue-optical transmission spectrum from the ground: Evidence for haze in the atmosphere of WASP-74b
• Demographics of the M-star Multiple Population in the Orion Nebula Cluster
• The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) V: Comparison between scattered light and thermal emission
• Additional JWST/NIRSpec Transits of the Rocky M Dwarf Exoplanet GJ 1132 b Reveal a Featureless Spectrum
• Ground-Based Transmission Spectroscopy with VLT FORS2: Evidence for faculae and clouds in the optical spectrum of the warm Saturn WASP-110b
• Evidence for thermal X-ray emission from the synchrotron dominated shocks in Tycho's supernova remnant
• The EDGES measurement disfavors an excess radio background during the cosmic dawn
• Multi-colour optical light curves of the companion star to the millisecond pulsar PSR J2051-0827
• Tentative detection of titanium oxide in the atmosphere of WASP-69 b with a 4m ground-based telescope
• Detection of the 2175Å UV Bump at z>7: Evidence for Rapid Dust Evolution in a Merging Reionisation-Era Galaxy
• Earth as an Exoplanet. III. Using Empirical Thermal Emission Spectra as an Input for Atmospheric Retrieval of an Earth-twin Exoplanet
• Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background
• Detailed stellar activity analysis and modelling of GJ 832: Reassessment of the putative habitable zone planet GJ 832c
• Exploring Fermionic Dark Matter Admixed Neutron Stars in the Light of Astrophysical Observations
• Bayesian inferences on covariant density functionals from multimessenger astrophysical data: Nucleonic models
• Another look at the dayside spectra of WASP-43b and HD 209458b: are there scattering clouds?
• Rotational and radio emission properties of PSR J0738-4042 over half a century
• Pulse Profile Modelling of Thermonuclear Burst Oscillations II: Handling variability
• Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars
• The viability of ultralight bosonic dark matter in dwarf galaxies
• The hot interstellar medium towards 4U 1820-30: a Bayesian analysis
• Thermal Emission from the hot Jupiter WASP-103b in J and Ks Bands
• Investigating time variability of X-ray absorption in Swift GRBs
• An Empirical Bayesian Approach to Limb-darkening in Modeling WASP-121b Transit Light Curves
• A MeerKAT view of the double pulsar eclipses -- Geodetic precession of pulsar B and system geometry
• Gas and Star Formation from HD and Dust Emission in a Strongly Lensed Galaxy
• Formation of "Blanets" from Dust Grains around the Supermassive Black Holes in Galaxies
• Nuclear Level Density and $\gamma$-ray Strength Function of ${}^{67}\mathrm{Ni}$ and the impact on the i-process
• Unraveling the global behavior of equation of state by explicit finite nuclei constraints
• Measuring the baryonic Tully-Fisher relation below the detection threshold
• Dark lens candidates from Gaia Data Release 3
• LRG-BEASTS: Evidence for clouds in the transmission spectrum of HATS-46 b
• Thermodynamic Constraints on the Dark Sector
• Probing the physical properties of the intergalactic medium using gamma-ray bursts
• Inferring the Equation of State from Neutron Star Observables via Machine Learning
• TOI-837 b: characterisation, formation and evolutionary history of an infant warm Saturn-mass planet
• Detecting and Characterizing Water Vapor in the Atmospheres of Earth Analogs through Observation of the 0.94 Micron Feature in Reflected Light
• The multi-planet system TOI-421 -- A warm Neptune and a super puffy mini-Neptune transiting a G9 V star in a visual binary
• Multi-Peaked Non-Thermal Light Curves from Magnetar-Powered Gamma-Ray Bursts
• Refractory and Volatile Species in the UV-to-IR Transmission Spectrum of Ultra-hot Jupiter WASP-178b with HST and JWST
• TESS and HARPS reveal two sub-Neptunes around TOI 1062
• A spectroscopic map of the Galactic centre -- Observations and resolved stars
• Detecting Dark Compact Objects in Gaia DR4: A Data Analysis Pipeline for Transient Astrometric Lensing Searches
• NGC 1266: Characterization of the Nuclear Molecular Gas in an Unusual SB0 Galaxy
• Analyzing the dense matter equation of states in the light of the compact object HESS J1731-347
• Gravitational-Wave Geodesy: A New Tool for Validating Detection of the Stochastic Gravitational-Wave Background
• Enabling Robust Exoplanet Atmospheric Retrievals with Gaussian Processes
• The Critical Role of LIGO-India in the Era of Next-Generation Observatories
• Rocks, Water and Noble Liquids: Unfolding the Flavor Contents of Supernova Neutrinos
• LEvEL: Low-Energy Neutrino Experiment at the LHC
• Observational Evidence of a Centi-parsec Supermassive Black Hole Binary Existing in the Nearby Galaxy M81
• MIGHTEE-HI: Discovery of an HI-rich galaxy group at z = 0.044 with MeerKAT
• Towards fast machine-learning-assisted Bayesian posterior inference of microseismic event location and source mechanism
• Entanglement masquerading in the CMB
• A highly mutually-inclined, compact warm-Jupiter system KOI-984 ?
• Constraints on circum-galactic media from Sunyaev-Zel'dovich effects and X-ray data
• Deep Learning and genetic algorithms for cosmological Bayesian inference speed-up
• A search for X-ray absorbed sources in the 3XMM catalogue, using photometric redshifts and Bayesian spectral fits
• The independent discovery of planet candidates around low mass stars and astrophysical false positives from the first two TESS sectors
• Pursuing Truth: Improving Retrievals on Mid-Infrared Exo-Earth Spectra with Physically Motivated Water Abundance Profiles and Cloud Models
• Extreme winds on the emerging dayside of an ultrahot Jupiter
• Flow Matching for Atmospheric Retrieval of Exoplanets: Where Reliability meets Adaptive Noise Levels
• BASS. XLIX. Characterization of highly luminous and obscured AGNs: local X-ray and [NeV]$\lambda$3426 emission in comparison with the high-redshift Universe
• The ESO SupJup Survey VIII. Chemical fingerprints of young L dwarf twins
• $\pi$ Earth: a 3.14-day Earth-sized Planet from $\text{K2}$'s Kitchen Served Warm by the SPECULOOS Team
• Benchmark tests of transmission spectroscopy using transiting white dwarfs
• Revisiting the Architecture of the KOI-89 System
• Dark skies of the slightly eccentric WASP-18 b from its optical-to-infrared dayside emission
• Parameterizing pressure-temperature profiles of exoplanet atmospheres with neural networks
• Compton-thick active galactic nuclei from the 7 Ms observation in the Chandra Deep Field South
• A Population Analysis of 20 Exoplanets Observed from the Optical to the Near-infrared Wavelengths with HST: Evidence for Widespread Stellar Contamination
• Unveiling non-gray surface of cloudy exoplanets: the influence of wavelength-dependent surface albedo and cloud scattering properties on retrieval solutions
• The peculiar physics of GRB 170817A and their implications for short GRBs
• Model-independent determination of cosmic curvature based on Padé approximation
• MIRACLES: atmospheric characterization of directly imaged planets and substellar companions at 4-5 $\mu$m. II. Constraints on the mass and radius of the enshrouded planet PDS 70 b
• Two-Point Separation Functions for Modeling Wide Binary Systems in Nearby Dwarf Galaxies
• The 3D Kinematics of the Orion Nebula Cluster II: Mass-dependent Kinematics of the Inner Cluster
• eRO-ExTra: eROSITA extragalactic non-AGN X-ray transients and variables in eRASS1 and eRASS2
• Is there evidence for CIDER in the Universe?
• An HST Transmission Spectrum of the Closest M-Dwarf Transiting Rocky Planet LTT 1445Ab
• X-SHYNE: X-Shooter spectra of young exoplanet analogs II. Presentation and analysis of the full library
• XMM-Newton and NuSTAR Observations of an Optically Quiescent Quasar
• Discovery of a cold giant planet and mass measurement of a hot super-Earth in the multi-planetary system WASP-132
• A population of Optically Quiescent Quasars from WISE and SDSS
• ATMOSPHERIX: III- Estimating the C/O ratio and molecular dynamics at the limbs of WASP-76 b with SPIRou
• Comparing transit spectroscopy pipelines at the catalogue level: evidence for systematic differences
• LTD064402+245919: A Subgiant with a 1-3 M${}_{\odot }$ Undetected Companion Identified from LAMOST-TD Data
• The Tianlin Mission: a 6m UV/Opt/IR space telescope to explore the habitable worlds and the universe
• TIC~257060897b: an inflated, low-density, hot-Jupiter transiting a rapidly evolving subgiant star
• Perturbation theory models for LSST-era galaxy clustering: tests with sub-percent mock catalog measurements in Fourier and configuration space
• Accretion Disc Evolution in GRO J1655-40 and LMC X-3 with Relativistic and Non-Relativistic Disc Models
• More on Emergent Dark Energy from Unparticles
• The intrinsic X-ray luminosity distribution of an optically-selected SDSS quasar population
• The 31-year Rotation History of the Millisecond Pulsar J1939+2134 (B1937+21)
• LEGA-C: analysis of dynamical masses from ionized gas and stellar kinematics at z~0.8
• CROCODILE \\ Incorporating medium-resolution spectroscopy of close-in directly imaged exoplanets into atmospheric retrievals via cross-correlation
• Retrieving planet formation parameters of WASP-77Ab using SimAb
• The curse of clouds
• Cloudy mornings and clear evenings on a gas giant exoplanet
• NICMOS Kernel-Phase Interferometry I: Catalogue of Brown Dwarfs Observed in F110W and F170M
• Time delay interferometry with minimal null frequencies
• Spitzer's View of the Candidate Cluster and Protocluster Catalog (CCPC)
• Cosmological simulations of the same spiral galaxy: connecting the dark matter distribution of the host halo with the subgrid baryonic physics
• The ExoGRAVITY survey: A K-band spectral library of giant exoplanet and brown dwarf companions
• Coordinated X-ray and UV absorption within the accretion disk wind of the active galactic nucleus PG 1126-041
• New transient Galactic bulge intermediate polar candidate XMMU J175035.2-293557
• Two neighbours of the ultra-short-period Earth-sized planet K2-157 b in the warm Neptunian savanna
• A UV to X-ray view of soft excess in type 1 AGNs: I. sample selection and spectral profile
• A hard look at the X-ray spectral variability of NGC 7582
• HST Transmission Spectra of the Hot-Neptune HD 219666 b: Detection of Water and the Challenge of Constraining Both Water and Methane
• Spatially resolving polycyclic aromatic hydrocarbons in Herbig Ae disks with VISIR-NEAR at the VLT
• The first X-ray look at SMSS J114447.77-430859.3: the most luminous quasar in the last 9 Gyr
• GEMS JWST: Transmission spectroscopy of TOI-5205b reveals significant stellar contamination and a metal-poor atmosphere
• DeepGlow: an efficient neural-network emulator of physical afterglow models for gamma-ray bursts and gravitational-wave events
• Inferring small neutron star spins with neutron star-black hole mergers
• Stage IV baryonic feedback correction for non-Gaussianity inference
• Small scale clustering of BOSS galaxies: dependence on luminosity, color, age, stellar mass, specific star formation rate and other properties
• A grand-design spiral galaxy 1.5 billion years after the Big Bang with JWST
• JWST/MIRI observations of the young TWA 27 system: hydrocarbon disk chemistry, silicate clouds, evidence for a CPD
• Evidence of Titanate Clouds in the Day-side Atmosphere of the Ultra-Hot Jupiter WASP-121b
• Unveiling Multiple Physical Processes on a Cluster Galaxy at z=0.3 Using JWST
• ACCESS: Tentative detection of H${}_2$O in the ground-based optical transmission spectrum of the low-density hot Saturn HATS-5b
• The effect of spectroscopic binning on atmospheric retrievals
• Coupling quintessence kinetics to electromagnetism
• A Multiwavelength Machine-learning Approach to Classifying X-ray Sources in the Fields of Unidentified 4FGL-DR4 sources
• Horizontal and vertical exoplanet thermal structure from a JWST spectroscopic eclipse map
• Neutron star equation of state: identifying hadronic matter characteristics
• Enhancing noise characterization with robust time delay interferometry combination
• In-depth characterization of the Kepler-10 three-planet system with HARPS-N radial velocities and Kepler transit timing variations
• The GALAH Survey: Improving our understanding of confirmed and candidate planetary systems with large stellar surveys
• Discovery and characterisation of two Neptune-mass planets orbiting HD 212729 with TESS
• NEOSSat Observations of Three Transiting Hot Jupiters
• Accelerating Bayesian Sampling for Massive Black Hole Binaries with Prior Constraints from Conditional Variational Autoencoder
• Bayesian insights in Tycho supernova remnant : a detailed mapping of ejecta properties
• Application of hydrostatic local thermodynamic equilibrium atmosphere models to interpretations of supersoft X-ray source spectra
• X-ray variability of the triplet star system LTT1445 and evaporation history of the exoplanets around its A component
• Simultaneous multicolour transit photometry of hot Jupiters HAT-P-19b, HAT-P-51b, HAT-P-55b, and HAT-P-65b
• A Detailed Investigation of HD 209458 b HST & JWST Transmission Spectra with SANSAR
• Impostor Among $\nu$s: Dark Radiation Masquerading as Self-Interacting Neutrinos
• DESI Mock Challenge: Constructing DESI galaxy catalogues based on FastPM simulations
• Osiris revisited: Confirming a solar metallicity and low C/O in HD 209458b
• The GAPS programme at TNG XLIII. A massive brown dwarf orbiting the active M dwarf TOI-5375
• The Cherenkov Telescope Array Will Test Whether Pulsars Generate the Galactic Center Gamma-Ray Excess
• NuSTAR observations of a heavily X-ray obscured AGN in the dwarf galaxy J144013+024744
• Testing time-delayed cosmology
• Cosmic Void Baryon Acoustic Oscillation Measurement: Evaluation of Sensitivity to Selection Effects
• Detectability of Polycyclic Aromatic Hydrocarbons in the Atmosphere of WASP-6 b with JWST NIRSpec PRISM
• The role of cloud particle properties on WASP-39b transmission spectrum based on JWST/NIRSpec observations
• Lessons from Hubble and Spitzer: 1D Self-Consistent Model Grids for 19 Hot Jupiter Emission Spectra
• A reanalysis of the LHS 1140 b atmosphere observed with the Hubble Space Telescope
• Gravitational Microlensing Event Statistics for the Zwicky Transient Facility
• The Similar Seven: A set of very-alike exoplanets to test correlations between system parameters and atmospheric properties
• Improving pulsar-timing solutions through dynamic pulse fitting
• HADES RV programme with HARPS-N at TNG XIV. A candidate super-Earth orbiting the M-dwarf GJ 9689 with a period close to half the stellar rotation period
• Inferring properties of neutron stars born in short gamma-ray bursts with a plerion-like X-ray plateau
• Can Dark Stars account for the star formation efficiency excess at very high redshifts?
• A New Planet in the Kepler-159 System From Transit Timing Variations
• Helium escaping from the atmosphere of a nearby rocky exoplanet orbiting in a habitable zone
• Modelling polarized X-ray pulses from accreting millisecond pulsars with X-PSI, using different hot spot locations and shapes
• X-Ray Redshifts of Obscured Chandra Source Catalog AGN
• SAFARI I: A SPHERE discovery of a super metal-rich M dwarf companion to the star HD 86006
• archNEMESIS: an open-source Python package for analysis of planetary atmospheric spectra
• A forward-modelling method to infer the dark matter particle mass from strong gravitational lenses
• A 1% accurate method to include baryonic effects in galaxy-galaxy lensing models
• The Compton-thick AGN luminosity function in the local Universe: A robust estimate combining BAT detections and NuSTAR spectra
• jaxspec : a fast and robust Python library for X-ray spectral fitting
• Constraining a Model of the Radio Sky Below 6 MHz Using the Parker Solar Probe/FIELDS Instrument in Preparation for Upcoming Lunar-based Experiments
• Retrieving interior properties of hot Jupiters with Love numbers and atmospheric measurements
• On a possible cosmological evolution of galaxy cluster $Y_{\mathrm{X}}-Y_{\mathrm{SZE}}$ scaling relation
• Atmospheric retrievals for LIFE and other future space missions: the importance of mitigating systematic effects
• Winds of change: the nuclear and galaxy-scale outflows and the X-ray variability of 2MASS 0918+2117
• A web portal for hydrodynamical, cosmological simulations
• A Transiting Super-Earth in the Radius Valley and An Outer Planet Candidate Around HD 307842
• Simplifying asteroseismic analysis of solar-like oscillators: An application of principal component analysis for dimensionality reduction
• A re-analysis of equilibrium chemistry in five hot Jupiters
• Retrieving the transmission spectrum of HD 209458b using CHOCOLATE: A new chromatic Doppler tomography technique
• Dark Matter Freeze-out during $\mathrm{SU}(2{)}_{\mathrm{L}}$ Confinement
• A Comprehensive Analysis of the Panchromatic Transmission Spectrum of the Hot-Saturn WASP-96 b: Nondetection of Haze, Possible Sodium Limb Asymmetry, Stellar Characterization, and Formation History
• Data Analysis and Phenomenological Cosmology
• Studying dark matter with MadDM 3.1: a short user guide
• Unveiling a universal relationship between the f(R) parameter and neutron star properties
• Detection of Na in the atmosphere of the hot Jupiter HAT-P-55b
• The incidence of X-ray AGN and non-AGN galaxies in the far-infrared: insights into host galaxy properties and AGN obscuration
• Effect of Centrifugal Force on Transmission Spectroscopy of Exoplanet Atmospheres
• The SRG/eROSITA all-sky survey: Hard X-ray selected Active Galactic Nuclei
• The eROSITA DR1 variability catalogue
• New Constraints on Anisotropic Expansion from Supernovae Type Ia
• Aerosols and hydrocarbons in the atmosphere of a white dwarf planet
• Complementarity of direct detection experiments in search of light Dark Matter
• Is the high-energy environment of K2-18b special?
• Bayesian WIMP detection with the Cherenkov Telescope Array
• Doomed Worlds II: Reassessing Suggestions of Orbital Decay for TrES-5 b
• The Reliability of Accretion Disk Inclination Derived from X-ray Spectroscopy of Active Galaxies
• The GAPS Programme at TNG -- XXIII. HD 164922 d: a close-in super-Earth discovered with HARPS-N in a system with a long-period Saturn mass companion
• Expectations for the confirmation of Proxima c from a long-term radial velocity follow-up
• J01020100-7122208: an accreted evolved blue straggler that wasn't ejected from a supermassive black hole
• Impact sculpting of the early martian atmosphere
• Star formation histories of massive red spiral galaxies in the local universe
• Chandra Follow-up Observations of Swift-BAT-selected AGNs III
• A Venus in the Making? Predictions for JWST Observations of the Ultracool M-Dwarf planet LP 890-9 c
• A MUSE view of the multiple interacting system HCG 31
• The CHEOPS view on the climate of WASP-3 b
• Reconstructing AGN X-ray spectral parameter distributions with Bayesian methods II: Population inference
• Detection of CO${}_2$, CO, and H${}_2$O in the atmosphere of the warm sub-Saturn HAT-P-12b
• A new Bowen Fluorescence Flare and Extreme Coronal Line Emitter discovered by SRG/eROSITA
• Iron K-alpha echoes from the circumnuclear disk orbiting Sgr A*
• The GAPS Programme at TNG. LIX. A characterisation study of the $\sim$300 Myr old multi-planetary system orbiting the star BD+40 2790 (TOI-2076)
• The diverse quenching pathways of post-starburst galaxies in SDSS-IV MaNGA
• Robust parameter estimation from pulsar timing data
• HST/WFC3 Constraints on the Abundances of OH and FeH in the Atmosphere of the Ultra-Hot Neptune LTT-9779 b
• A Two-limb Explanation for the Optical-to-infrared Transmission Spectrum of the Hot Jupiter HAT-P-32Ab
• Soft X-ray emission from the classical nova AT 2018bej
• The COSMOS Wall at z$\sim$0.73: star-forming galaxies and their evolution in different environments
• YSES 2b is a background star: Differential astrometric M-dwarf measurements in time
• Association of Optical, Ultraviolet and Soft X-ray excess Emissions in AGNs
• Radio Galaxy Detection in the Visibility Domain
• Reconstructing AGN X-ray spectral parameter distributions with Bayesian methods I: Spectral analysis
• Interpreting the atmospheric composition of exoplanets: sensitivity to planet formation assumptions
• New $H(z)$ measurement at Redshift = 0.12 with DESI Data Release 1
• Simulation-efficient marginal posterior estimation with swyft: stop wasting your precious time
• Knobs and dials of retrieving JWST transmission spectra. II. Impacts of pipeline-level differences on retrieval posteriors
• XSNAP: An X-ray Supernova Analysis Pipeline with Application to the Type II Supernova 2024ggi
• Harnessing the XMM-Newton data: X-ray spectral modelling of 4XMM-DR11 detections and 4XMM-DR11s sources
• The very faint X-ray transient Swift J174610-290018 at the Galactic center
• Euclid: Early Release Observations -- The star cluster systems of the Local Group dwarf galaxies IC 10 and NGC 6822
• Impact of Accretion Assumptions on Pulse Profile Modelling of Superburst Oscillations in 4U 1636-536
• Flares in the Changing Look AGN Mrk 590. II: Deep X-ray observations reveal a Comptonizing inner accretion flow
• Scaling relations for the uncertainty in neutron star radius inferred from pulse profile modelling: the effect of spin rate
• Ultra High-Redshift or Closer-by, Dust-Obscured Galaxies? Deciphering the Nature of Faint, Previously Missed F200W-Dropouts in CEERS
• ZTF SN~Ia DR2: Cosmology-independent constraints on Type Ia supernova standardisation from supernova siblings
• Joint Inference of Population, Cosmology, and Neutron Star Equation of State from Gravitational Waves of Dark Binary Neutron Stars
• Time delay interferometry with minimal null frequencies and shortened time span
• Parameter constraints for accreting millisecond pulsars with synthetic NICER data
• Enhanced AGN Activity in Overdense Galactic Environments at $2<z<4$
• A Preference for Cold Dark Matter over Superfluid Dark Matter in Local Milky Way Data
• Direct Images of CO2 Absorption in the Atmosphere of a Super-Jupiter: Enhanced Metallicity Suggestive of Formation in a Disk
• Retrieving the Red Edge on Earth-like Planets with Heterogeneous Clouds and Surfaces
• Revisiting the atmosphere of HAT-P-70b with CARMENES high-resolution transmission spectroscopy
• Probing chromatic onsets of gravitational wave overtones
• Kinematic analysis of an Ultra-Strong MgII absorber at z~1.13 linking to Circumgalactic Gas Structures
• Detectability of massive binary black holes with sub-mHz gravitational wave missions
• Kilonova Light Curve Parameter Estimation Using Likelihood-Free Inference
• Detection of a Millisecond Periodicity in BATSE Short Gamma-Ray Bursts
• A new look into the atmospheric composition of WASP-39 b
• Pulse profile modelling of the accretion-powered millisecond pulsar SAX J1808.4-3658 using NICER data from its 2019 and 2022 outbursts
• The Multi-parameter Test of Gravitational Wave Dispersion with Principal Component Analysis
• From gas to stars: MUSEings on the internal evolution of IC 1613
• Evidence of the association of repeating fast-radio-burst sources with fast-spinning super-twisted magnetars
• OrbDot: A Python package for studying the secular evolution of exoplanet orbits
• Examining the evolution of the Supersoft X-ray Source RX J0513.9-6951
• A Measurement of the Water Abundance in the Atmosphere of the Hot Jupiter WASP-43b with High-resolution Cross-correlation Spectroscopy
• Re-examining the Bayesian colour excess estimation for the local star-forming galaxies observed in the HETDEX Pilot Survey
• The influence of tight binaries on proto-planetary disk masses
• Two unseen massive white dwarf candidates in close binaries
• Barrett: out-of-core processing of MultiNest output
• Measuring Hubble Constant with Dark Neutron Star-Black Hole Mergers
• Structure and Dynamics of the Young Massive Star Cluster Westerlund 1
• Discovery of a transiting hot water-world candidate orbiting Ross 176 with TESS and CARMENES
• AGN obscuration in optical and X-rays: Host properties and the interplay of nuclear and galactic gas and dust in a combined SDSS-XMM sample
• Kinematics of the Sagittarius Dwarf Spheroidal core: A 5D Analysis for a 6D Methodology with Gaia DR3
• Horizontal transport as a source of disequilibrium chemistry on the nightside of a hot exoplanet
• Obscured and unobscured X-ray AGNs I: Host galaxy properties
• Multi-epoch afterglow rebrightenings in GRB 250129A: Evidence for successive shock interactions
• Thermal emission spectra of the ultra-hot Jupiter WASP-33 b
• Evidence for stellar contamination and water absorption in NGTS-5b's transmission spectra with GTC/OSIRIS
• HyDRo: Atmospheric Retrieval of Rocky Exoplanets in Thermal Emission
• Misidentification of Short GRBs as Magnetars in Nearby Galaxies
• Dense gas linked to star-forming regions photoionised by embedded gamma-ray bursts
• Methane on the temperate exo-Saturn TOI-199b
• Kilonova and progenitor properties of merger-driven gamma-ray bursts
• Probing the anomalous positron fraction origin with fully leptonic decaying gravitino dark matter candidates
• X-ray analysis of the Planck-detected triplet-cluster system PLCK G334.8-38
• KRONOS I: The $1-2.8\mu$m JWST Transmission Spectrum of the 23 Myr V1298 Tau c
• Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study
• Bayes Factors via Savage-Dickey Supermodels
• Piercing through the Haze: Characterizing Titan-like terrestrial exoplanets with JWST
• Reflected spectroscopy of small exoplanets I: determining the atmospheric composition of sub-Neptunes planets
• Joint Optical-HI mock catalogues and prospects for upcoming HI surveys
• Planets or asteroids? A geochemical method to constrain the masses of White Dwarf pollutants
• Redshift Evolution of the HII Galaxy $L$-$\sigma$ Relation: Gaussian Process Analysis and Cosmological Implications
• A Near-Earth Object Model Calibrated to Earth Impactors
• Multicolour Validation of Two Temperate Mini-Neptunes Around M-dwarf Habitable Zones
• Information content on Venusian aerosols in VIRTIS-M infrared data
• Extragalactic Searches for Dark Matter Annihilation
• Inferring the nuclear symmetry energy at supra saturation density from neutrino cooling
• The $N_H$ Distribution of Hard X-ray Selected AGN in the NEP Field
• A constant pressure model for the warm absorber in Mrk 509
• Rapid Orbital Decay in the Ultracompact Double-degenerate Binary eRASSU J060839.5$-$704014
• iid2022: A Workshop on Statistical Methods for Event Data in Astronomy
• Potential sublimating exocomets around the young star PDS 70
• MINDS: The very low-mass star and brown dwarf sample II. Probing disk settling, dust properties, and dust-gas interplay with JWST/MIRI
• Time-resolved JWST Retrieval Analysis of the Coldest Brown Dwarf: Temperature and Chemical Variations in WISE 0855-07
• Contrasting evolutionary pathways of fast- and slow-rotating galaxies in the green valley
• Joint analysis of EDGES $21$-cm line observations with standard candles and rulers in $\Lambda$CDM and non-adiabatic gCg models
• The HUSTLE Program: The UV to Near-IR Transmission Spectrum of the Hot Jupiter KELT-7b
• Gravitational-Wave Geodesy: Defining False Alarm Probabilities with Respect to Correlated Noise
• Hiding behind a curtain of dust: Gas and dust properties of an ultra-luminous strongly-lensed z = 3.75 galaxy behind the Milky Way disk
• The X-ray statistical properties of dust-obscured galaxies detected by eROSITA
• Experimental Inference of Neutral and Impurity Transport in Alcator C-Mod Using High-Resolution X-Ray and Ultra-Violet Spectra
• Discovery of a multi-planetary system orbiting the aged Sun-like star HD 224018
• X-ray spectral fitting with Monte Carlo Dropout Neural Networks
• The thermodynamic structure and large-scale structure filament in MACS J0717.5+3745
• PAStar: a model for stellar surface from the Sun to active stars
• BayesEoR: Bayesian 21-cm Power Spectrum Estimation from Interferometric Visibilities
• Discovery and Characterization of White Dwarf-FGK Main-Sequence Binaries within the Optical Main-Sequence Locus
• Multi-messenger parameter inference of gravitational-wave and electromagnetic observations of white dwarf binaries
• Disentangling auroral, cloud and magnetic spot driven variability in three early L-dwarfs with HST/WFC3
• Magnetic-field Order in the Southwestern Rim of RCW 86 Constrained Using X-Ray Polarimetry
• Bayesian Inference of Neutron Star Properties in $f(Q)$ Gravity Using NICER Observations
• Using Statistical Emulation and Knowledge of Grain-Surface Diffusion for Bayesian Inference of Reaction Rate Parameters: An Application to a Glycine Network
• Medium effects on light clusters from heavy-ion collisions within a relativistic mean-field description
• New Dynamical Measurements from a Lensed Quasar Sample: Joint Analysis Constrains the Mass Profile Evolution of Lens Galaxies
• The effect of JWST/NIRSpec data reduction on the retrieval of WASP-39b atmospheric properties
• Atmospheric characterization of HIP 67522 b with VLT/CRIRES+. VLT/CRIRES+ suggests a heavier planet and hints at deuterium fractionation
• The Double-Burst Nature and Early Afterglow Evolution of Long GRB 110801A