dynesty: A Dynamic Nested Sampling Package for Estimating Bayesian Posteriors and Evidences

Abstract

We present dynesty, a public, open-source, Python package to estimate Bayesian posteriors and evidences (marginal likelihoods) using Dynamic Nested Sampling. By adaptively allocating samples based on posterior structure, Dynamic Nested Sampling has the benefits of Markov Chain Monte Carlo algorithms that focus exclusively on posterior estimation while retaining Nested Sampling's ability to estimate evidences and sample from complex, multi-modal distributions. We provide an overview of Nested Sampling, its extension to Dynamic Nested Sampling, the algorithmic challenges involved, and the various approaches taken to solve them. We then examine dynesty's performance on a variety of toy problems along with several astronomical applications. We find in particular problems dynesty can provide substantial improvements in sampling efficiency compared to popular MCMC approaches in the astronomical literature. More detailed statistical results related to Nested Sampling are also included in the Appendix.

28 pages, 12 figures, submitted to MNRAS; code available at https://github.com/joshspeagle/dynesty

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• GA-NIFS: Early-stage feedback in a heavily obscured AGN at $z=4.76$
• Measuring the properties of active galactic nuclei disks with gravitational waves
• Keck/KPIC Emission Spectroscopy of WASP-33b
• TOI-269 b: An eccentric sub-Neptune transiting a M2 dwarf revisited with ExTrA
• JWST reveals a rapid and strong day side variability of 55 Cancri e
• Poking Holes: Looking for Gaps in LIGO/Virgo's Black Hole Population
• Revisiting bright delta Scuti stars and their period-luminosity relation with TESS and Gaia DR3
• Optical Transmission Spectroscopy of the Terrestrial Exoplanet LHS 3844b from 13 Ground-Based Transit Observations
• Reconstructing the Assembly of Massive Galaxies. I: The Importance of the Progenitor Effect in the Observed Properties of Quiescent Galaxies at $z\approx 2$
• The Magnificent Five Images of Supernova Refsdal: Time Delay and Magnification Measurements
• Performance forecasts for the primordial gravitational wave detection pipelines for AliCPT-1
• Search for the birefringence of gravitational waves with the third observing run of Advanced LIGO-Virgo
• Inspiral-merger-ringdown waveforms in Einstein-scalar-Gauss-Bonnet gravity within the effective-one-body formalism
• A super-massive Neptune-sized planet
• Escaping Helium and a Highly Muted Spectrum Suggest a Metal-Enriched Atmosphere on Sub-Neptune GJ3090b from JWST Transit Spectroscopy
• How narrow is the M87* ring? II. A new geometric model
• The GTC exoplanet transit spectroscopy survey XI. Possible detection of Rayleigh scattering in the atmosphere of the Saturn-mass planet WASP-69b
• The CARMENES search for exoplanets around M dwarfs: Stable radial-velocity variations at the rotation period of AD~Leonis -- A test case study of current limitations to treating stellar activity
• The stellar populations of quiescent ultra-diffuse galaxies from optical to mid-infrared spectral energy distribution fitting
• Photometric detection at $7.7\mu \mathrm{m}$ of a galaxy beyond redshift $14$ with JWST/MIRI
• PyAutoFit: A Classy Probabilistic Programming Language for Model Composition and Fitting
• An Early-Time Optical and Ultraviolet Excess in the type-Ic SN 2020oi
• The Radcliffe Wave is Oscillating
• A Search for Gravitational Waves from Binary Mergers with a Single Observatory
• The dynamic magnetosphere of Swift J1818.0$-$1607
• Multi-waveform inference of gravitational waves
• Evidence for a correlation between binary black hole mass ratio and black-hole spins
• The K2-3 system revisited: testing photoevaporation and core-powered mass loss with three small planets spanning the radius valley
• Searching for anisotropy in the distribution of binary black hole mergers
• Mapping the Gravitational-wave Sky with LISA: A Bayesian Spherical Harmonic Approach
• Abell 1201: Detection of an Ultramassive Black Hole in a Strong Gravitational Lens
• Toward the unambiguous identification of supermassive binary black holes through Bayesian inference
• Correlations in gravitational-wave reconstructions from eccentric binaries: A case study with GW151226 and GW170608
• The Importance of Priors on LIGO-Virgo Parameter Estimation: the Case of Primordial Black Holes
• Bayesian Inference of the Dense Matter Equation of State built upon Covariant Density Functionals
• TESS Reveals a Short-period Sub-Neptune Sibling (HD 86226c) to a Known Long-period Giant Planet
• The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc
• On the Detection of Exomoons Transiting Isolated Planetary-Mass Objects
• Evidence for profile changes in PSR J1713+0747 using the uGMRT
• GW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-Spin Black Hole Coalescence
• The Contribution of In-situ and Ex-situ Star Formation in Early-Type Galaxies: MaNGA versus IllustrisTNG
• Detection and parameter estimation challenges of Type-II lensed binary black hole signals
• Discovery of the Magellanic Stellar Stream Out to 100 Kiloparsecs
• Constraining short gamma-ray burst jet properties with gravitational waves and gamma rays
• First semi-empirical test of the white dwarf mass-radius relationship using a single white dwarf via astrometric microlensing
• At least one in a dozen stars exhibits evidence of planetary ingestion
• Where intermediate-mass black holes could hide in the Galactic Centre: A full parameter study with the S2 orbit
• Deep Synoptic Array science: A massive elliptical host among two galaxy-cluster fast radio bursts
• Resonant tides in binary neutron star mergers: analytical-numerical relativity study
• An exploration of model degeneracies with a unified phase curve retrieval analysis: The light and dark sides of WASP-43 b
• PHANGS-MUSE: Detection and Bayesian classification of ~40000 ionised nebulae in nearby spiral galaxies
• A strong He II $\lambda$1640 emitter with extremely blue UV spectral slope at $z=8.16$: presence of Pop III stars?
• The unluckiest star: A spectroscopically confirmed repeated partial tidal disruption event AT 2022dbl
• Early JWST imaging reveals strong optical and NIR color gradients in galaxies at $z\sim 2$ driven mostly by dust
• AT 2020wey and the class of faint and fast Tidal Disruption Events
• A pair of warm giant planets near the 2:1 mean motion resonance around the K-dwarf star TOI-2202
• Detection and parameter estimation of binary neutron star merger remnants
• {\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning
• The geometric albedo of the hot Jupiter HD 189733b measured with CHEOPS
• A super-Earth and a mini-Neptune near the 2:1 MMR straddling the radius valley around the nearby mid-M dwarf TOI-2096
• Betelgeuse fainter in the sub-millimetre too: an analysis of JCMT and APEX monitoring during the recent optical minimum
• Gravitational waves from binary black hole mergers surrounded by scalar field clouds: Numerical simulations and observational implications
• Beyond the bulge-halo conspiracy? Density profiles of Early-type galaxies from extended-source strong lensing
• Planet Engulfment Detections are Rare According to Observations and Stellar Modeling
• A Bayesian Population Model for the Observed Dust Attenuation in Galaxies
• Exploring the Impact of Microlensing on Gravitational Wave Signals: Biases, Population Characteristics, and Prospects for Detection
• Neural network reconstructions for the Hubble parameter, growth rate and distance modulus
• 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
• TOI-2525 b and c: A pair of massive warm giant planets with a strong transit timing variations revealed by TESS
• Kalkayotl: A cluster distance inference code
• A 1.55 R${}_{\oplus }$ habitable-zone planet hosted by TOI-715, an M4 star near the ecliptic South Pole
• Systematic Biases in Estimating the Properties of Black Holes Due to Inaccurate Gravitational-Wave Models
• Systematic errors induced by the elliptical power-law model in galaxy-galaxy strong lens modeling
• Constraint on phase transition with the multimessenger data of neutron stars
• Testing strong lensing subhalo detection with a cosmological simulation
• The CARMENES search for exoplanets around M dwarfs, Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass star
• VARAHA: A Fast Non-Markovian sampler for estimating Gravitational-Wave posteriors
• SBI++: Flexible, Ultra-fast Likelihood-free Inference Customized for Astronomical Applications
• HD 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone
• Spectroscopic r-Process Abundance Retrieval for Kilonovae I: The Inferred Abundance Pattern of Early Emission from GW170817
• Hot Rocks Survey I : A possible shallow eclipse for LHS 1478 b
• TOI-3884 b: A rare 6-R${}_{\oplus }$ planet that transits a low-mass star with a giant and likely polar spot
• NANOGrav hints for first-order confinement-deconfinement phase transition in different QCD-matter scenarios
• Probing lens-induced gravitational-wave birefringence as a test of general relativity
• Lorentz Invariance Violation Limits from the Spectral Lag Transition of GRB~190114C
• On the detectability of higher harmonics with LISA
• Multiple Clues for Dayside Aerosols and Temperature Gradients in WASP-69 b from a Panchromatic JWST Emission Spectrum
• GW190521: Search for Echoes due to Stimulated Hawking Radiation from Black Holes
• GRB 200716C: Evidence for a Short Burst Being Lensed
• LRG-BEASTS: sodium absorption and Rayleigh scattering in the atmosphere of WASP-94A b using NTT/EFOSC2
• Population Properties of Gravitational-Wave Neutron Star--Black Hole Mergers
• Asteroseismic Signatures of Core Magnetism and Rotation in Hundreds of Low-Luminosity Red Giants
• A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics
• Direct Constraints on the Extremely Metal-Poor Massive Stars Underlying Nebular C IV Emission from Ultra-Deep HST/COS Ultraviolet Spectroscopy
• A Solar System formation analogue in the Ophiuchus star-forming complex
• Discovery of the optical afterglow and host galaxy of short GRB181123B at $z=1.754$: Implications for Delay Time Distributions
• Finding binary black holes in the Milky Way with LISA
• TOI-132 b: A short-period planet in the Neptune desert transiting a $V=11.3$ G-type star
• The Dusty Heart of NGC 4151 Revealed by $\lambda \sim$1-40 $\mu$m Reverberation Mapping and Variability: A Challenge to Current Clumpy Torus Models
• Numerical-Relativity-Informed Effective-One-Body model for Black-Hole-Neutron-Star Mergers with Higher Modes and Spin Precession
• Simultaneous Optical Transmission Spectroscopy of a Terrestrial, Habitable-Zone Exoplanet with Two Ground-Based Multi-Object Spectrographs
• Exploring the Hubble tension with a late time Modified Gravity scenario
• Deep Hubble Space Telescope Observations of GW170817: Complete Light Curves and the Properties of the Galaxy Merger of NGC 4993
• Planet Engulfment Signatures in Twin Stars
• Low-latency gravitational wave alert products and their performance at the time of the fourth LIGO-Virgo-KAGRA observing run
• Parameterised population models of transient non-Gaussian noise in the LIGO gravitational-wave detectors
• Combining effective-one-body accuracy and reduced-order-quadrature speed for binary neutron star merger parameter estimation with machine learning
• Quality over Quantity: Optimizing pulsar timing array analysis for stochastic and continuous gravitational wave signals
• The Aligned Orbit of the Eccentric Proto Hot Jupiter TOI-3362b
• First constraint on the dissipative tidal deformability of neutron stars
• The Circumgalactic Medium of Extreme Emission Line Galaxies at z ~ 2: Resolved Spectroscopy and Radiative Transfer Modeling of Spatially Extended Lyman-alpha Emission in the KBSS-KCWI Survey
• Practical approaches to analyzing PTA data: Cosmic strings with six pulsars
• pygwb: Python-based library for gravitational-wave background searches
• The cool brown dwarf Gliese 229 B is a close binary
• TOI-1231 b: A Temperate, Neptune-Sized Planet Transiting the Nearby M3 Dwarf NLTT 24399
• Gravitational-Wave Data Analysis with High-Precision Numerical Relativity Simulations of Boson Star mergers
• Testing Lorentz Invariance of Gravity in the Standard Model Extension with GWTC-3
• How Well Can We Measure Galaxy Dust Attenuation Curves? The Impact of the Assumed Star-Dust Geometry Model in SED Fitting
• Waltzing binaries: Probing line-of-sight acceleration of merging compact objects with gravitational waves
• TOI-1468: A system of two transiting planets, a super-Earth and a mini-Neptune, on opposite sides of the radius valley
• Spitzer Reveals Evidence of Molecular Absorption in the Atmosphere of the Hot Neptune LTT 9979b
• Forward Modeling of Double Neutron Stars: Insights from Highly-Offset Short Gamma-Ray Bursts
• Constraining the Gravitational Potential from the Projected Morphology of Extragalactic Tidal Streams
• Gravitational-wave population inference at past time infinity
• Template bank for compact binary mergers in the fourth observing run of Advanced LIGO, Advanced Virgo, and KAGRA
• Interplay of spin-precession and higher harmonics in the parameter estimation of binary black holes
• Frequency-Domain Analysis of Black-Hole Ringdowns
• Measuring properties of primordial black hole mergers at cosmological distances: effect of higher order modes in gravitational waves
• Reconstructing the Genealogy of LIGO-Virgo Black Holes
• Still at Odds with Conventional Galaxy Evolution: The Star Formation History of Ultra-Diffuse Galaxy Dragonfly 44
• Hyper Suprime-Cam Low Surface Brightness Galaxies II: A Hubble Space Telescope Study of the Globular Cluster Systems of Ultra-Diffuse Galaxies in Groups
• Inferring the population properties of binary black holes from unresolved gravitational waves
• Ground-based Optical Transmission Spectroscopy of the Nearby Terrestrial Exoplanet LTT 1445Ab
• Can Assembly Bias Explain the Lensing Amplitude of the BOSS CMASS Sample in a Planck Cosmology?
• Eccentricity-induced systematic error on parametrized tests of general relativity: Hierarchical Bayesian inference applied to a binary black hole population
• A sub-Earth-mass planet orbiting Barnard's star
• Systematic biases due to waveform mismodeling in parametrized post-Einsteinian tests of general relativity: The impact of neglecting spin precession and higher modes
• Analysis of a subsolar-mass compact binary candidate from the second observing run of Advanced LIGO
• A study of the Inspiral-Merger-Ringdown Consistency Test with gravitational-wave signals from compact binaries in eccentric orbits
• Dark matter profiles of SPARC galaxies: a challenge to fuzzy dark matter
• Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars
• An M dwarf accompanied by a close-in giant orbiter with SPECULOOS
• A transiting, temperate mini-Neptune orbiting the M dwarf TOI-1759 unveiled by TESS
• A Generalized Semi-Analytic Model for Magnetar-Driven Supernovae
• Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures
• Interpreting the X-ray afterglows of gamma-ray bursts with radiative losses and millisecond magnetars
• TOI-2257 b: A highly eccentric long-period sub-Neptune transiting a nearby M dwarf
• The population of merging compact binaries inferred using gravitational waves through GWTC-3
• Adiabatically compressed wave dark matter halo and intermediate-mass ratio inspirals
• Model exploration in gravitational-wave astronomy with the maximum population likelihood
• Impact of updated Multipole Love numbers and f-Love Universal Relations in the context of Binary Neutron Stars
• Three new brown dwarfs and a massive hot Jupiter revealed by TESS around early-type stars
• Re-Envisioning Numerical Information Field Theory (NIFTy.re): A Library for Gaussian Processes and Variational Inference
• The distant, galaxy cluster environment of the short GRB 161104A at $z\sim 0.8$ and a comparison to the short GRB host population
• Molecular Gas Reservoirs in Massive Quiescent Galaxies at $\mathrm{z}\sim 0.7$ Linked to Late Time Star Formation
• Compact Starburst Galaxies with Fast Outflows: Central Escape Velocities and Stellar Mass Surface Densities from Multi-band Hubble Space Telescope Imaging
• Minutes-duration Optical Flares with Supernova Luminosities
• The Issues of Mismodelling Gravitational-Wave Data for Parameter Estimation
• Bayesian model selection on Scalar $\epsilon$-Field Dark Energy
• TOI-3984 A b and TOI-5293 A b: two temperate gas giants transiting mid-M dwarfs in wide binary systems
• Accelerating Multi-Model Bayesian Inference, Model Selection and Systematic Studies for Gravitational Wave Astronomy
• Constraining spontaneous black hole scalarization in scalar-tensor-Gauss-Bonnet theories with current gravitational-wave data
• Search for Lorentz Invariance Violation from stacked Gamma-Ray Burst spectral lag data
• Kernel Selection for Gaussian Process in Cosmology: with Approximate Bayesian Computation Rejection and Nested Sampling
• Tentative Evidence for Water Vapor in the Atmosphere of the Neptune-Size Exoplanet HD 106315 c
• Flux density variability of 286 radio pulsars from a decade of monitoring
• Nested sampling cross-checks using order statistics
• The Magellan/PFS Exoplanet Search: A 55-day period dense Neptune transiting the bright ($V=8.6$) star HD 95338
• The TREX Survey: Kinematical Complexity Throughout M33's Stellar Disk and Evidence for a Stellar Halo
• TOI-1728b: The Habitable-zone Planet Finder confirms a warm super Neptune orbiting an M dwarf host
• The late afterglow of GW170817/GRB170817A: a large viewing angle and the shift of the Hubble constant to a value more consistent with the local measurements
• Starlight-polarization-based tomography of the magnetized interstellar medium: PASIPHAE's line-of-sight inversion method
• Measurability of precession and eccentricity for heavy binary-black-hole mergers
• DESI Dark Energy Time Evolution is Recovered by Cosmologically Coupled Black Holes
• Kinetic Model for Dark Energy - Dark Matter Interaction: Scenario for the Hubble Tension
• Testing an oscillatory behavior of dark energy
• Bayesian inference of multimessenger astrophysical data: Joint and coherent inference of gravitational waves and kilonovae
• Measuring tidal effects with the Einstein Telescope: A design study
• JWST-TST DREAMS: NIRSpec/PRISM Transmission Spectroscopy of the Habitable Zone Planet TRAPPIST-1 e
• Discovery and mass measurement of the hot, transiting, Earth-sized planet GJ 3929 b
• An environmental analysis of the fast transient AT2018cow and implications for its progenitor and late-time brightness
• Unraveling information about supranuclear-dense matter from the complete binary neutron star coalescence process using future gravitational-wave detector networks
• Constructing high-fidelity halo merger trees in AbacusSummit
• Bayesian Accretion Modeling: Axisymmetric Equatorial Emission in the Kerr Spacetime
• Supernova SN 2020faa -- an iPTF14hls look-alike?
• Which black hole is spinning? Probing the origin of black-hole spin with gravitational waves
• No-go guide for the Hubble tension: late-time or local-scale new physics
• Bioverse: The Habitable Zone Inner Edge Discontinuity as an Imprint of Runaway Greenhouse Climates on Exoplanet Demographics
• Revisiting the Gas Kinematics in SSA22 Lyman-$\alpha$ Blob 1 with Radiative Transfer Modeling in a Multiphase, Clumpy Medium
• Planets larger than Neptune have elevated eccentricities
• New Gravitational Wave Discoveries Enabled by Machine Learning
• J0107a: A Barred Spiral Dusty Star-forming Galaxy at $z=2.467$
• Fitting the light curves of Sagittarius A* with a hot-spot model
• MiMO: Mixture Model for Open Clusters in Color-Magnitude Diagrams
• A search for planetary companions around 800 pulsars from the Jodrell Bank pulsar timing programme
• Three long period transiting giant planets from TESS
• Improved analysis of GW190412 with a precessing numerical relativity surrogate waveform model
• The Cosmic Dipole in the Quaia Sample of Quasars: A Bayesian Analysis
• The cosmic build-up of dust and metals. Accurate abundances from GRB-selected star-forming galaxies at $1.7<z<6.3$
• An eccentric Brown Dwarf eclipsing an M dwarf
• A hidden active galactic nucleus powering bright [O III] nebulae in a protocluster at $z=4.5$ revealed by JWST
• Multimass modelling of Milky Way globular clusters -- I. Implications on their stellar initial mass function above 1 M${}_{\odot }$
• Confirmation of an He I evaporating atmosphere around the 650-Myr-old sub-Neptune HD235088 b (TOI-1430 b) with CARMENES
• BOWIE-ALIGN: JWST reveals hints of planetesimal accretion and complex sulphur chemistry in the atmosphere of the misaligned hot Jupiter WASP-15b
• Simple and statistically sound recommendations for analysing physical theories
• Linear to circular conversion in the polarized radio emission of a magnetar
• Identification of Gravitational-waves from Extreme Mass Ratio Inspirals
• Fast and robust Bayesian Inference using Gaussian Processes with GPry
• The first degree-scale starlight-polarization-based tomography map of the magnetized interstellar medium
• Detecting the stochastic gravitational wave background with the TianQin detector
• HD 28109 hosts a trio of transiting Neptunian planets including a near-resonant pair, confirmed by ASTEP from Antarctica
• The Return of GOLUM: Improving Distributed Joint Parameter Estimation for Strongly-Lensed Gravitational Waves
• Searching for quasi-periodic oscillations in astrophysical transients using Gaussian processes
• Adapting to noise distribution shifts in flow-based gravitational-wave inference
• The Habitable-zone Planet Finder Detects a Terrestrial-mass Planet Candidate Closely Orbiting Gliese 1151: The Likely Source of Coherent Low-frequency Radio Emission from an Inactive Star
• Fast Parameter Estimation of Binary Mergers for Multimessenger Followup
• Orbital eccentricity in a neutron star - black hole merger
• Coupled Multi Scalar Field Dark Energy
• Radio jet precession in M81*
• Fast likelihood evaluation using meshfree approximations for reconstructing compact binary sources
• LISA stellar-mass black hole searches with semicoherent and particle-swarm methods
• Improving Detection of Gravitational wave Microlensing Using Repeated Signals Induced by Strong Lensing
• Barry and the BAO Model Comparison
• LRG-BEASTS: Ground-based Detection of Sodium and a Steep Optical Slope in the Atmosphere of the Highly Inflated Hot-Saturn WASP-21b
• The MASSIVE Survey -- XVII. A Triaxial Orbit-based Determination of the Black Hole Mass and Intrinsic Shape of Elliptical Galaxy NGC 2693
• The anti-aligned spin of GW191109: glitch mitigation and its implications
• Applications of machine learning in gravitational wave research with current interferometric detectors
• Exploring over 700 massive quiescent galaxies at z = 2-7: Demographics and stellar mass functions
• Gaussian processes for radial velocity modeling Better rotation periods and planetary parameters with the quasi-periodic kernel and constrained priors
• Constraining the Distance to the North Polar Spur with Gaia DR2
• Across the Green Valley with HST grisms: colour evolution, crossing time-scales and the growth of the red sequence at $z=1.0-1.8$
• The ALMA-CRISTAL survey. Discovery of a 15 kpc-long gas plume in a $z=4.54$ Lyman-$\alpha$ blob
• The Detection of Transiting Exoplanets by Gaia
• SN 2020bqj: a Type Ibn supernova with a long lasting peak plateau
• Testing No-Hair Theorem by Quasi-Periodic Oscillations: the quadrupole of GRO J1655$-$40
• TESS discovery of a sub-Neptune orbiting a mid-M dwarf TOI-2136
• Bioverse: a simulation framework to assess the statistical power of future biosignature surveys
• Radial Velocity Survey for Planets around Young stars (RVSPY) A transiting warm super-Jovian planet around HD 114082, a young star with a debris disk
• A New Method For Studying Exoplanet Atmospheres Using Planetary Infrared Excess
• Efficient parameter inference for gravitational wave signals in the presence of transient noises using temporal and time-spectral fusion normalizing flow
• ACCESS: Confirmation of a Clear Atmosphere for WASP-96b and a Comparison of Light Curve Detrending Techniques
• TOI-969: a late-K dwarf with a hot mini-Neptune in the desert and an eccentric cold Jupiter
• JWST-TST DREAMS: A Precise Water Abundance for Hot Jupiter WASP-17b from the NIRISS SOSS Transmission Spectrum
• Complex Modulation of Rapidly Rotating Young M Dwarfs: Adding Pieces to the Puzzle
• The Aemulus Project VI: Emulation of beyond-standard galaxy clustering statistics to improve cosmological constraints
• The Galactic Distribution of Phosphorus: A Survey of 163 Disk and Halo Stars
• An ALMA Gas-dynamical Mass Measurement of the Supermassive Black Hole in the Local Compact Galaxy UGC 2698
• Parameter estimation methods for analyzing overlapping gravitational wave signals in the third-generation detector era
• The curious case of EP241021a: Unraveling the mystery of its exceptional rebrightening
• Revising the Giant Planet Mass-Metallicity Relation: Deciphering the Formation Sequence of Giant Planets
• Gravitational waves carry information beyond effective spin parameters but it is hard to extract
• Evidence of wind signatures in the gas velocity profiles of Red Geysers
• Characterization of a set of small planets with TESS and CHEOPS and an analysis of photometric performance
• A proper motion catalogue for the Milky Way's nuclear stellar disc
• HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
• Pitfalls of periodograms: The non-stationarity bias in the analysis of quasi-periodic oscillations
• On the LISA science performance in observations of short-lived signals from massive black hole binary coalescences
• Ordering the confusion: A study of the impact of lens models on gravitational-wave lensing detection capabilities
• A Method To Characterize the Wide-Angle Point Spread Function of Astronomical Images
• Stellar Populations in the Central 0.5 pc of Our Galaxy III: The Dynamical Sub-structures
• TOI-1268b: the youngest, hot, Saturn-mass transiting exoplanet
• Prospects for Taiji to detect a gravitational-wave background from cosmic strings
• Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?
• Sub-stellar Companions of Intermediate-mass Stars with CoRoT: CoRoT-34b, CoRoT-35b, and CoRoT-36b
• Systematic bias due to eccentricity in parameter estimation for merging binary neutron stars
• Kepler-90: Giant transit-timing variations reveal a super-puff
• Rapid parameter estimation of a two-component neutron star model with spin wandering using a Kalman filter
• A general approach to maximise information density in neutron reflectometry analysis
• Hints of spin-orbit resonances in the binary black hole population
• HATS-38 b and WASP-139 b join a growing group of hot Neptunes on polar orbits
• Constraints on parity and Lorentz violations in gravity from GWTC-3 through a parametrization of modified gravitational wave propagations
• Assessing and Mitigating the Impact of Glitches on Gravitational-Wave Parameter Estimation: a Model Agnostic Approach
• Using Equation of State Constraints to Classify Low-Mass Compact Binary Mergers
• ACCESS: Confirmation of no potassium in the atmosphere of WASP-31b
• Multiple Peaks and a Long Precursor in the Type IIn Supernova 2021qqp: An Energetic Explosion in a Complex Circumstellar Environment
• Computing Tools for Effective Field Theories
• Model systematics in time domain tests of binary black hole evolution
• Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits
• alpha-Deep Probabilistic Inference (alpha-DPI): efficient uncertainty quantification from exoplanet astrometry to black hole feature extraction
• Cloud Parameterizations and their Effect on Retrievals of Exoplanet Reflection Spectroscopy
• Understanding binary neutron star collisions with hypermodels
• Transmission spectroscopy of WASP-52 b with JWST NIRISS: Water and helium atmospheric absorption, alongside prominent star-spot crossings
• Inferring the Intermediate Mass Black Hole Number Density from Gravitational Wave Lensing Statistics
• A new method to measure the spectra of transiting exoplanet atmospheres using multi-object spectroscopy
• Effect of Noise Estimation in Time-Domain Ringdown Analysis: A Case Study with GW150914
• Importance of Sample Selection in Exoplanet Atmosphere Population Studies
• Rapid parameter estimation for an all-sky continuous gravitational wave search using conditional varitational auto-encoders
• General relativistic effects and the near-infrared and X-ray variability of Sgr A* I
• Rotation and Abundances of the Benchmark Brown Dwarf HD 33632 Ab from Keck/KPIC High-resolution Spectroscopy
• The galaxy-halo connection of disc galaxies over six orders of magnitude in stellar mass
• NGTS-14Ab: a Neptune-sized transiting planet in the desert
• TESS discovery of a super-Earth and three sub-Neptunes hosted by the bright, Sun-like star HD 108236
• TOI-1842b: A Transiting Warm Saturn Undergoing Re-Inflation around an Evolving Subgiant
• Precise mass determination for the keystone sub-Neptune planet transiting the mid-type M dwarf G 9-40
• Eccentricity signatures in LIGO-Virgo-KAGRA's BNS and NSBH binaries
• GJ 3090 b: one of the most favourable mini-Neptune for atmospheric characterisation
• Measuring angular N-point correlations of binary black hole merger gravitational-wave events with hierarchical Bayesian inference
• Where Outflows Meet Inflows: Gas Kinematics in SSA22 Lyman-$\alpha$ Blob 2 Decoded by Advanced Radiative Transfer Modelling
• Deciphering the unusual stellar progenitor of GRB 210704A
• ESPRESSO observations of Gaia BH1: high-precision orbital constraints and no evidence for an inner binary
• The GAPS program at TNG XLVII: The unusual formation history of V1298 Tau
• Dark-ages Reionization and Galaxy Formation Simulation -- XIX: Predictions of infrared excess and cosmic star formation rate density from UV observations
• Unveiling Microlensing Biases in Testing General Relativity with Gravitational Waves
• Characterizing Astrophysical Binary Neutron Stars with Gravitational Waves
• Bayesian estimate of the superfluid moments of inertia from the 2016 glitch in the Vela pulsar
• A Stimulating Explanation of the Extragalactic Radio Background
• A microlensing search of 700 million VVV light curves
• Microlensing and the type Ia supernova iPTF16geu
• Search for continuous gravitational waves from known pulsars in the first part of the fourth LIGO-Virgo-KAGRA observing run
• Efficient Reduced Order Quadrature Construction Algorithms for Fast Gravitational Wave Inference
• eRASSt J074426.3+291606: prompt accretion disc formation in a 'faint and slow' tidal disruption event
• TOI-1075 b: A Dense, Massive, Ultra-Short Period Hot Super-Earth Straddling the Radius Gap
• A candidate relativistic tidal disruption event at 340 Mpc
• Constraints on the Galactic Centre environment from \textit{Gaia} hypervelocity stars III: Insights on a possible companion to Sgr A*
• Probing hadron-quark phase transition in twin stars using $f$-modes
• A Phantom Menace: On the Morphology of the Galactic Center Excess
• Toward a better understanding of supernova environments: a study of SNe 2004dg and 2012P in NGC 5806 with HST and MUSE
• GW230529_181500: A Potential Primordial Binary Black Hole Merger in the Mass Gap
• Fresh view of the hot brown dwarf HD 984 B through high-resolution spectroscopy
• Pulsar Timing Arrays require hierarchical models
• Compact Binary Coalescences in Dense Gaseous Environments Can Pose as ones in Vacuum
• Signatures of inflowing gas in red geyser galaxies hosting radio-AGN
• BOWIE-ALIGN: A JWST comparative survey of aligned vs misaligned hot Jupiters to test the dependence of atmospheric composition on migration history
• The fast transient AT 2023clx in the nearby LINER galaxy NGC 3799 as a tidal disruption of a very low-mass star
• Impact of ringdown higher-order modes on black-hole mergers in dense environments: the scalar field case, detectability and parameter biases
• Modeling Radial Velocity Data of Resonant Planets to Infer Migration Histories
• Parameter estimation with the current generation of phenomenological waveform models applied to the black hole mergers of GWTC-1
• Asteroseismology of $\delta$ Scuti stars: emulating model grids using a neural network
• Tidal Disruption Events through the Lens of the Cooling Envelope Model
• HOD-Dependent Systematics for Luminous Red Galaxies in the DESI 2024 BAO Analysis
• The Spin-Orbit Alignment of 8 Warm Gas Giant Systems
• Hot-spots around Sagittarius A*: Joint fits to astrometry and polarimetry
• The interplay of astrophysics and nuclear physics in determining the properties of neutron stars
• The GAPS Programme at TNG XL: A puffy and warm Neptune-sized planet and an outer Neptune-mass candidate orbiting the solar-type star TOI-1422
• Three super-Earths and a possible water world from TESS and ESPRESSO
• Does the speed of gravitational waves depend on the source velocity?
• A comprehensive revisit of select Galileo/NIMS observations of Europa
• Spin Doctors: How to diagnose a hierarchical merger origin
• KilonovaNet: Surrogate Models of Kilonova Spectra with Conditional Variational Autoencoders
• Full forward model of galaxy clustering statistics with AbacusSummit lightcones
• A full transit of ${\nu }^2$ Lupi d and the search for an exomoon in its Hill sphere with CHEOPS
• New gravitational waveform model for precessing binary neutron stars with double-spin effects
• Espresso observations of HE 0107$-$5240 and other CEMP-no stars with $[Fe/H]\le -4.5$
• Evidence for a milliparsec-separation Supermassive Binary Black Hole with quasar microlensing
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• Modelling stellar activity with Gaussian process regression networks
• A massive hot Jupiter orbiting a metal-rich early-M star discovered in the TESS full frame images
• Hierarchical Bayesian Atmospheric Retrieval Modeling for Population Studies of Exoplanet Atmospheres: A Case Study on the Habitable Zone
• Noise analysis of the Indian Pulsar Timing Array data release I
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• Targeted search for the stochastic gravitational-wave background from the galactic millisecond pulsar population
• Modelling high-resolution ALMA observations of strongly lensed dustystar forming galaxies detected by Herschel
• Pandora: A fast open-source exomoon transit detection algorithm
• Mean shift cluster recognition method implementation in the nested sampling algorithm
• VVV-WIT-08: the giant star that blinked
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• High-energy spectra of LTT 1445A and GJ 486 reveal flares and activity
• A stochastic search for intermittent gravitational-wave backgrounds
• Population-level Hypothesis Testing with Rocky Planet Emission Data: A Tentative Trend in the Brightness Temperatures of M-Earths
• Multimessenger astronomy with a kHz-band gravitational-wave observatory
• Breaking bad degeneracies with Love relations: Improving gravitational-wave measurements through universal relations
• Three low-mass companions around aged stars discovered by TESS
• Incorporation of model accuracy in gravitational wave Bayesian inference
• A 2:1 Mean-Motion Resonance Super-Jovian pair revealed by TESS, FEROS, and HARPS
• Time-dependent visibility modelling of a relativistic jet in the X-ray binary MAXI J1803-298
• First Comparative Exoplanetology Within a Transiting Multi-planet System: Comparing the atmospheres of V1298 Tau b and c
• All-Sky Kinematics of the Distant Halo: The Reflex Response to the LMC
• NEID Reveals that The Young Warm Neptune TOI-2076 b Has a Low Obliquity
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• Hot planets around cool stars -- two short-period mini-Neptunes transiting the late K-dwarf TOI-1260
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• The astrophysical odds of GW151216
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• An eclipsing M-dwarf close to the hydrogen burning limit from NGTS
• Can we distinguish the adiabatic fluctuations and isocurvature fluctuations with pulsar timing arrays?
• Model-Independent Determination of $H_0$ and ${\Omega }_{K,0}$ using Time-Delay Galaxy Lenses and Gamma-Ray Bursts
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• SN 2021adxl: A luminous nearby interacting supernova in an extremely low metallicity environment
• Multiwavelength view of SPT-CL J2106-5844. The radio galaxies and the thermal and relativistic plasmas in a massive galaxy cluster merger at z~1.13
• Gravitational-wave constraints on scalar-tensor gravity from a neutron star and black-hole binary GW200115
• Parametrized spin-precessing inspiral-merger-ringdown waveform model for tests of general relativity
• Analysis of GWTC-3 with fully precessing numerical relativity surrogate models
• The Merian Survey: Design, Construction, and Characterization of a Filter Set Optimized to Find Dwarf Galaxies and Measure their Dark Matter Halo Properties with Weak Lensing
• ALMA resolves the first strongly-lensed Optical/NIR-dark galaxy
• Mimicking Mergers: Mistaking Black Hole Captures as Mergers
• Overscreening and Underscreening in Solid-Electrolyte Grain Boundary Space-Charge Layers
• Determining the maximum information gain and optimising experimental design in neutron reflectometry using the Fisher information
• Localization of binary neutron star mergers with a single Cosmic Explorer
• First eccentric inspiral-merger-ringdown analysis of neutron star-black hole mergers
• Linear vs. nonlinear modeling of black hole ringdowns
• Gravitational-wave parameter inference with the Newman-Penrose scalar ${\psi }_4$
• Feeding and feedback processes in the Spiderweb proto-intracluster medium
• GRB 220426A: A Thermal Radiation-Dominated Gamma-Ray Burst
• Measuring quasi-normal mode amplitudes with misaligned binary black hole ringdowns
• Three Warm Jupiters around Solar-analog stars detected with TESS
• Possible binary neutron star merger history of the primary of GW230529
• Light-Curve Structure and Halpha Line Formation in the Tidal Disruption Event AT 2019azh
• Footprints of population III stars in the gravitational-wave background
• Evidence of the pair instability gap from black hole masses
• Bayesian modelling of scattered light in the LIGO interferometers
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• The Cosmic Evolution of Fast Radio Bursts Inferred from the CHIME/FRB Baseband Catalog 1
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• New constraints on the central mass contents of Omega Centauri from combined stellar kinematics and pulsar timing
• Nested sampling with plateaus
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• Dark lenses through the dust: parallax microlensing events in the VVV
• CLEAR: The Morphological Evolution of Galaxies in the Green Valley
• A Statistical Detection of Wide Binary Systems in the Ultra-Faint Dwarf Galaxy Reticulum II
• Uncovering dark matter density profiles in dwarf galaxies with graph neural networks
• A dense mini-Neptune orbiting the bright young star HD 18599
• Effect of double spin-precession and higher harmonics on spin-induced quadrupole moment measurements
• The Type Ibn Supernova 2019kbj -- Indications for Diversity in Type Ibn Supernova Progenitors
• Tracing the formation and migration history: molecular signatures in the atmosphere of misaligned hot Jupiter WASP-94Ab using JWST NIRSpec/G395H
• A systematic validation of hot Neptunes in TESS data
• The COSMOS-Web Lens Survey (COWLS) I: Discovery of >100 high redshift strong lenses in contiguous JWST imaging
• The OATMEAL Survey. I. Low Stellar Obliquity in the Transiting Brown Dwarf System GPX-1
• Prompt sky localization of compact binary sources using a meshfree approximation
• Advice on describing Bayesian analysis of neutron and X-ray reflectometry
• An updated glitch rate law inferred from radio pulsars
• First Space-VLBI Observations of Sagittarius A*
• Transiting exoplanets with the Mid-InfraRed Instrument on board the James Webb Space Telescope: From simulations to observations
• Inflow of low-metallicity cool gas in the halo of the Andromeda galaxy
• 2D k-th nearest neighbor statistics: a highly informative probe of galaxy clustering
• A GPU-accelerated semi-coherent hierarchical search for stellar-mass binary inspiral signals in LISA
• Optical polarization and spectral properties of the H-poor superluminous supernovae SN 2021bnw and SN 2021fpl
• binary_c-python: A Python-based stellar population synthesis tool and interface to binary_c
• The nascent milliquasar VT J154843.06+220812.6: tidal disruption event or extreme accretion-state change?
• Revisiting the multi-planetary system of the nearby star HD 20794: Confirmation of a low-mass planet in the habitable zone of a nearby G-dwarf
• TESS and CHEOPS Discover Two Warm Sub-Neptunes Transiting the Bright K-dwarf HD 15906
• Using gravitational waves to distinguish between neutron stars and black holes in compact binary mergers
• Gravitational-wave Observations Suggest Most Black Hole Mergers Form in Triples
• Memory Effect or Cosmic String? Classifying Gravitational-Wave Bursts with Bayesian Inference
• Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
• Extending the Fisher Information Matrix in Gravitational-wave Data Analysis
• Compactness peaks: An astrophysical interpretation of the mass distribution of merging binary black holes
• Isolated pulsar population synthesis with simulation-based inference
• Post maximum light and late time optical imaging polarimetry of type I superluminous supernova 2020znr
• Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes
• A likely magnetic activity cycle for the exoplanet host M dwarf GJ 3512
• Search for a gravitational wave background from primordial black hole binaries using data from the first three LIGO-Virgo-KAGRA observing runs
• XLSSC 122 caught in the act of growing up: Spatially resolved SZ observations of a z=1.98 galaxy cluster
• Flexible Models for Galaxy Star Formation Histories Both Shift and Scramble the Optical Color-M/L Relationship
• Spectroscopy for asymmetric binary black hole mergers
• Potential biases and prospects for the Hubble constant estimation via electromagnetic and gravitational-wave joint analyses
• Distance to the Brick cloud using stellar kinematics
• Allesfitter: Flexible Star and Exoplanet Inference From Photometry and Radial Velocity
• Uncovering the Invisible: A Study of Gaia18ajz, a Candidate Black Hole Revealed by Microlensing
• Decoding Long-duration Gravitational Waves from Binary Neutron Stars with Machine Learning: Parameter Estimation and Equations of State
• pop-cosmos: Scaleable inference of galaxy properties and redshifts with a data-driven population model
• A comparison of Bayesian sampling algorithms for high-dimensional particle physics and cosmology applications
• Towards Studying Hierarchical Assembly in Real Time: A Milky Way Progenitor Galaxy at z = 2.36 under the Microscope
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• Do we need wavelets in the late Universe?
• Implications of GWTC-3 on primordial black holes from vacuum bubbles
• The EBLM Project XII. An eccentric, long-period eclipsing binary with a companion near the hydrogen-burning limit
• A 16 Hour Transit of Kepler-167 e Observed by the Ground-based Unistellar Telescope Network
• NGTS 15b, 16b, 17b and 18b: four hot Jupiters from the Next Generation Transit Survey
• Sky marginalization in black hole spectroscopy and tests of the area theorem
• The ultra narrow FRB20191107B, and the origins of FRB scattering
• Structure and Skewness of the Effective Inspiral Spin Distribution of Binary Black Hole Mergers
• An Unexplained Origin for the Unusual Globular Cluster System in the Ultra-diffuse Galaxy FCC 224
• Gravitational wave echoes search with combs
• Diving into the planetary system of Proxima with NIRPS -- Breaking the metre per second barrier in the infrared
• Neural post-Einsteinian framework for efficient theory-agnostic tests of general relativity with gravitational waves
• Unravelling the mass spectrum of destroyed dwarf galaxies with the metallicity distribution function
• Population properties of neutron stars in the coalescing compact binaries
• Dynamical masses of two young transiting sub-Neptunes orbiting HD 63433
• Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR
• CHEOPS and TESS view of the ultra-short period super-Earth TOI-561 b
• Hiding in plain sight: observing planet-starspot crossings with the James Webb Space Telescope
• Possibility of primordial black holes as the source of gravitational wave events in the advanced LIGO detector
• GWDALI: A Fisher-matrix based software for gravitational wave parameter-estimation beyond Gaussian approximation
• Detecting Planetary Oblateness in the Era of JWST: A Case Study of Kepler-167e
• TOI-1296b and TOI-1298b observed with TESS and SOPHIE: Two hot Saturn-mass exoplanets with different densities around metal-rich stars
• Analysis of the ionized interstellar medium and orbital dynamics of PSR~J1909-3744 using scintillation arcs
• 183 GHz water megamasers in active galactic nuclei: a new accretion disk tracer
• The unusual M-dwarf Warm Jupiter TOI-1899~b: Refinement of orbital and planetary parameters
• Searching for candidates of coalescing binary black holes formed through chemically homogeneous evolution in GWTC-3
• Be careful in multi-messenger inference of the Hubble constant: A path forward for robust inference
• A matched-filter approach to radio variability and transients: searching for orphan afterglows in the VAST Pilot Survey
• Accounting for numerical-relativity calibration uncertainty in gravitational-wave modeling and inference
• JADES Ultra-red Flattened Objects: Morphologies and Spatial Gradients in Color and Stellar Populations
• JWST-TST DREAMS: Non-Uniform Dayside Emission for WASP-17b from MIRI/LRS
• Towards a complete picture of the Sco-Cen outflow
• Planetary companions orbiting the M dwarfs GJ 724 and GJ 3988. A CARMENES and IRD collaboration
• Bayesian fitting of multi-Gaussian expansion models to galaxy images
• A hot Mars-sized exoplanet transiting an M dwarf
• Rapid inference and comparison of gravitational-wave population models with neural variational posteriors
• Search for Coincident Gravitational-wave and Fast Radio Burst Events from 4-OGC and the First CHIME/FRB Catalog
• Dust Buried Compact Sources in the Dwarf Galaxy NGC 4449
• A precise blue-optical transmission spectrum from the ground: Evidence for haze in the atmosphere of WASP-74b
• The CARMENES search for exoplanets around M dwarfs. Revisiting the GJ 581 multi-planetary system with new Doppler measurements from CARMENES, HARPS, and HIRES
• TOI-4504: Exceptionally large Transit Timing Variations induced by two resonant warm gas giants in a three planet system
• The First Spin-Orbit Obliquity of an M dwarf/brown dwarf System: An eccentric and aligned TOI-2119 b
• Additional JWST/NIRSpec Transits of the Rocky M Dwarf Exoplanet GJ 1132 b Reveal a Featureless Spectrum
• Decay of $f(R)$ quintessence into dark matter: mitigating the Hubble tension?
• Do both black holes spin in merging binaries? Evidence from GWTC-4 and astrophysical implications
• Improved parametrized test of general relativity using the IMRPhenomX waveform family: Including higher harmonics and precession
• Discriminating among cosmological models by data-driven methods
• Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
• Robust inference of gravitational wave source parameters in the presence of noise transients using normalizing flows
• Dark energy reconstruction analysis with artificial neural networks: Application on simulated Supernova Ia data from Rubin Observatory
• On the initial spin period distribution of neutron stars
• Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars
• An ESPRESSO view of HD 189733 system. Broadband transmission spectrum, differential rotation, and system architecture
• Cold Deuterium Fractionation in the Nearest Planet-Forming Disk
• White dwarf binary modulation can help stochastic gravitational wave background search
• Joint analysis of gravitational-wave and electromagnetic data of mergers: breaking an afterglow model degeneracy in GW170817 and in future events
• Spinning up a Daze: TESS Uncovers a Hot Jupiter orbiting the Rapid-Rotator TOI-778
• DESI Survey Validation Spectra Reveal an Increasing Fraction of Recently Quenched Galaxies at $z\sim 1$
• Characterization of the HD 108236 system with CHEOPS and TESS. Confirmation of a fifth transiting planet
• The Transit Timing and Atmosphere of Hot Jupiter HAT-P-37b
• Realizing the potential of deep neural network for analyzing neutron star observables and dense matter equation of state
• Rotational Variation Allows for Narrow Age Spread in the Extended Main Sequence Turnoff of Massive Cluster NGC 1846
• Physical Properties of the Host Galaxies of Ca-rich Transients
• A fully precessing higher-mode surrogate model of effective-one-body waveforms
• 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
• Prospects for measuring off-axis spins of binary black holes with Plus-era gravitational-wave detectors
• Quasinormal-modes of the Kerr-Newman black hole: GW150914 and fundamental physics implications
• Revisiting the HD 21749 Planetary System with Stellar Activity Modeling
• A Unified Spectroscopic and Photometric Model to Infer Surface Inhomogeneity: Application to Luhman 16B
• BASS XLVII: 22 GHz Radio Atlas of Swift-BAT Selected AGN
• Mapping the Skies of Ultracool Worlds: Detecting Storms and Spots with Extremely Large Telescopes
• Numerical relativity surrogate models for exotic compact objects: the case of head-on mergers of equal-mass Proca stars
• TESS and HARPS reveal two sub-Neptunes around TOI 1062
• The steep redshift evolution of the hierarchical binary black hole merger rate may cause the $z$-${\chi }_{\mathrm{eff}}$ correlation
• Missed opportunities: GRB 211211A and the case for continual gravitational-wave coverage with a single observatory
• Probing the Circumstellar Environment of highly luminous type IIn SN ASASSN-14il
• Reanalyzing the ringdown signal of GW150914 using the F-statistic method
• Prospects of Gravitational Wave Follow-up Through a Wide-field Ultra-violet Satellite: a Dorado Case Study
• GPU-accelerated LISA parameter estimation with full time domain response
• Tracking hidden magnetospheric fluctuations in accretion-powered pulsars with a Kalman filter
• Can a binary neutron star merger in the vicinity of a supermassive black hole enable a detection of a post-merger gravitational wave signal?
• Bayesian parameter estimation for targeted anisotropic gravitational-wave background
• Optimising experimental design in neutron reflectometry
• Importance of eccentricities in parameter estimation of compact binary inspirals with decihertz gravitational-wave detectors
• What is the nature of GW230529? An exploration of the gravitational lensing hypothesis
• A Stochastic Gravitational Wave Background in LISA from Unresolved White Dwarf Binaries in the Large Magellanic Cloud
• Cosmology and nuclear-physics implications of a subsolar gravitational-wave event
• Constraining $|V_{cs}|$ and physics beyond the Standard Model from exclusive (semi)leptonic charm decays
• Bayesian $\mathcal{F}$-statistic-based parameter estimation of continuous gravitational waves from known pulsars
• Very-High-Energy Gamma-Ray Afterglows of GRB 201015A and GRB 201216C
• BEBOP VII. SOPHIE discovery of BEBOP-3b, a circumbinary giant planet on an eccentric orbit
• Search for Lorentz Invariance Violation using Bayesian model comparison applied to Xiao et al. GRB spectral lag catalog
• Nuclear physics with gravitational waves from neutron stars disrupted by black holes
• GalaPy, the highly optimised C++/Python spectral modelling tool for galaxies -- I. Library presentation and photometric fitting
• Three Warm Jupiters orbiting TOI-6628, TOI-3837, TOI-5027 and one sub-Saturn orbiting TOI-2328
• Constraints on Non-Gaussian primordial curvature perturbation from the LIGO-Virgo-KAGRA third observing run
• Detecting Baryon Acoustic Oscillations with third generation gravitational wave observatories
• Secondary spins of extreme mass ratio inspirals: A probe to the formation channels
• Constraints on Inflation with Null Energy Condition Violation from Advanced LIGO and Advanced Virgo's First Three Observing Runs
• Uniform Modelling of the Stellar Density of Thirteen Tidal Streams within the Galactic Halo
• No evidence for a dip in the binary black hole mass spectrum
• Inferring the Astrophysical Population of Gravitational Wave Sources in the Presence of Noise Transients
• Exploring the Gas-Phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
• Characterizing the 3D Kinematics of Young Stars in the Radcliffe Wave
• SN 2022joj: A Peculiar Type Ia Supernova Possibly Driven by an Asymmetric Helium-shell Double Detonation
• Flow Matching for Atmospheric Retrieval of Exoplanets: Where Reliability meets Adaptive Noise Levels
• Impact of higher harmonics of gravitational radiation on the population inference of binary black holes
• $\mu$-GLANCE: A Novel Technique to Detect Chromatically and Achromatically Lensed Gravitational Wave Signals
• Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object
• Constraining string cosmology with the gravitational-wave background using the NANOGrav 15-year data set
• Conditional Noise Deep Learning for Parameter Estimation of Gravitational Wave Events
• Two warm Earth-sized exoplanets and an Earth-sized candidate in the M5V-M6V binary system TOI-2267
• Discovery of the variable optical counterpart of the redback pulsar PSR J2055+1545
• Gravitational wave ringdown analysis using the $\mathcal{F}$-statistic
• The Orbit and Companion of PSR J1622-0315: Variable Asymmetry and a Massive Neutron Star
• Comparison of Step Samplers for Nested Sampling
• Massive stars exploding in a He-rich circumstellar medium. XI. Diverse evolution of five Ibn SNe 2020nxt, 2020taz, 2021bbv, 2023utc and 2024aej
• Ensemble noise properties of the European Pulsar Timing Array
• High-precision source characterization of intermediate mass-ratio black hole coalescences with gravitational waves: The importance of higher-order multipoles
• Detecting Low-Mass Perturbers in Cluster Lenses using Curved Arc Bases
• Comparison between time-domain and frequency-domain Bayesian inferences to inspiral-merger-ringdown gravitational-wave signals
• Double Trouble: Two spectroscopically confirmed low-mass quiescent galaxies at z>5 in overdensities
• The Radius of PSR J0437-4715 from NICER Data
• HD 183579b: A Warm Sub-Neptune Transiting a Solar Twin Detected by TESS
• Testing the Cosmological Principle: On the Time Dilation of Distant Sources
• Brackett-$\gamma$ as a Gold-standard Test of Star Formation Rates Derived from SED Fitting
• Differential Interferometric Signatures of Close Binaries of Supermassive Black Holes in Active Galactic Nuclei: II. Merged Broad Line Regions
• Waveform systematics in identifying strongly gravitationally lensed gravitational waves: Posterior overlap method
• Unveiling a 36 Billion Solar Mass Black Hole at the Centre of the Cosmic Horseshoe Gravitational Lens
• Diversity in the haziness and chemistry of temperate sub-Neptunes
• The proper motion of stars in dwarf galaxies: distinguishing central density cusps from cores
• TOI-5108 b and TOI 5786 b: Two transiting sub-Saturns detected and characterized with TESS, MaHPS and SOPHIE
• Pinpointing coalescing binary neutron star sources with the IGWN, including LIGO-Aundha
• A Population Analysis of 20 Exoplanets Observed from the Optical to the Near-infrared Wavelengths with HST: Evidence for Widespread Stellar Contamination
• Confronting general relativity with principal component analysis: Simulations and results from GWTC-3 events
• PDS 70b Shows Stellar-like Carbon-to-oxygen Ratio
• Deep learning to detect gravitational waves from binary close encounters: Fast parameter estimation using normalizing flows
• TOI-4336 A b: A temperate sub-Neptune ripe for atmospheric characterization in a nearby triple M-dwarf system
• The discovery of three hot Jupiters, NGTS-23b, 24b and 25b, and updated parameters for HATS-54b from the Next Generation Transit Survey
• Dark skies of the slightly eccentric WASP-18 b from its optical-to-infrared dayside emission
• Simulation-based inference of galaxy properties from JWST pixels
• Deep Learning and genetic algorithms for cosmological Bayesian inference speed-up
• The Frequency and Mass-Ratio Distribution of Binaries in Clusters I: Description of the method and application to M67
• Measuring Star Formation Histories, Distances, and Metallicities with Pixel Color-Magnitude Diagrams II: Applications to Nearby Elliptical Galaxies
• Normalizing Constant Estimation with Gaussianized Bridge Sampling
• On Dark Gravitational Wave Standard Sirens as Cosmological Inference and Forecasting the Constraint on Hubble Constant using Binary Black Holes Detected by Deci-hertz Observatory
• The TESS-Keck Survey. XIII. An Eccentric Hot Neptune with a Similar-Mass Outer Companion around TOI-1272
• Exploiting the transit timing capabilities of Ariel
• Bayesian Analysis of the ${}^{70}$Zn$(d{,}^3\text{He}{)}^{69}$Cu Transfer Reaction
• A Gap in the Densities of Small Planets Orbiting M Dwarfs: Rigorous Statistical Confirmation Using the Open-source Code RhoPop
• Spectroscopic AGN survey at $z$ $\sim$ 2 with NTT/SOFI for GRAVITY+ observations
• RUBIES spectroscopically confirms the high number density of quiescent galaxies from $2<\mathbf{z}<5$
• Searching for orbital decay in a heartbeat star system KIC 3766353
• Distinguishing binary black hole precessional morphologies with gravitational wave observations
• Detecting a Gravitational-Wave Background from Inflation with Null Energy Condition Violation: Prospects for Taiji
• Discovery of a radio jet in the Cloverleaf Quasar at z = 2.56
• TIC~257060897b: an inflated, low-density, hot-Jupiter transiting a rapidly evolving subgiant star
• Bounds on the charge of the graviton using gravitational wave observations
• The Origin of the Cluster of Local Interstellar Clouds
• Efficient Bayesian inference and model selection for continuous gravitational waves in pulsar timing array data
• Non-Kerr Constraints using Binary Black Hole inspirals considering phase modifications up to 4 PN order
• An extremely low-density exoplanet spins slow
• Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins
• Anomalously low-mass core-He-burning star in NGC 6819 as a post-common-envelope phase product
• Black Hole Gravitational Potential Enhanced Fallback Accretion onto the Nascent Lighter Compact Object: Tentative Evidence in the O3 Run Data of LIGO/Virgo
• Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset
• Bayesian Model Selection of Lithium-Ion Battery Models via Bayesian Quadrature
• Constraints on peculiar velocity distribution of binary black holes using gravitational waves with GWTC-3
• Search for stochastic gravitational-wave background from string cosmology with Advanced LIGO and Virgo's O1$\sim$O3 data
• Effective chirp mass captures the inspiral frequency evolution of the non-spinning eccentric compact binary
• SN 2020zbf: A fast-rising hydrogen-poor superluminous supernova with strong carbon lines
• Methodology for constraining ultralight vector bosons with gravitational wave searches targeting merger remnant black holes
• LitePIG: A Lite Parameter Inference system for the Gravitational wave in the millihertz band
• Modelling Einstein cluster using Einasto profile
• Analysis of the public HARPS/ESO spectroscopic archive -- Jupiter-like planets around HD 103891 and HD 105779
• Accelerating Tests of General Relativity with Gravitational-Wave Signals using Hybrid Sampling
• Modified gravitational wave propagations in linearized gravity with Lorentz and diffeomorphism violations and their gravitational wave constraints
• Retrieving Exoplanet Atmospheres using Planetary Infrared Excess: Prospects for the Nightside of WASP-43 b and other Hot Jupiters
• Validating Sequential Monte Carlo for Gravitational-Wave Inference
• Simulation-based Inference for Gravitational-waves from Intermediate-Mass Binary Black Holes in Real Noise
• The magnetic field of the Radcliffe Wave: starlight polarization at nearest approach to the Sun
• Modeling matter(s) in SEOBNRv5THM: Generating fast and accurate effective-one-body waveforms for spin-aligned binary neutron stars
• Bayesian Search of Massive Scalar Fields from LIGO-Virgo-KAGRA Binaries
• Atmospheric abundances and bulk properties of the binary brown dwarf Gliese 229 Bab from JWST/MIRI spectroscopy
• Observability of spin precession in the presence of a black-hole remnant kick
• Probing intractable beyond-standard-model parameter spaces armed with Machine Learning
• PACMAN: A pipeline to reduce and analyze Hubble Wide Field Camera 3 IR Grism data
• Catalog variance of testing general relativity with gravitational-wave data
• Hierarchical triple mergers: testing Hawking's area theorem with the inspiral signals
• Evidence of Titanate Clouds in the Day-side Atmosphere of the Ultra-Hot Jupiter WASP-121b
• Eccentricity evolution consistency test to distinguish eccentric gravitational-wave signals from eccentricity mimickers
• The CARMENES search for exoplanets around M dwarfs. A sub-Neptunian mass planet in the habitable zone of HN Lib
• Assessing the systematic errors of extreme-mass-ratio inspirals waveforms for testing general relativity
• Mapping the Distant and Metal-Poor Milky Way with SDSS-V
• Two neighbours of the ultra-short-period Earth-sized planet K2-157 b in the warm Neptunian savanna
• Resolved Gas Temperatures and 12C/13C ratios in SVS13A from ALMA Observations of CH3CN and CH3-13-CN
• SN 2019odp: A Massive Oxygen-Rich Type Ib Supernova
• Measuring the magnetic dipole moment and magnetospheric fluctuations of SXP 18.3 with a Kalman filter
• Inferring small neutron star spins with neutron star-black hole mergers
• Empirical Dust Attenuation Model Leads to More Realistic UVJ Diagram for TNG100 Galaxies
• Evidence for evolving dark energy from DESI DR2 BAO and Pantheon${}^{+}$, DES-Dovekie, and Union3
• NGTS-21b: An Inflated Super-Jupiter Orbiting a Metal-poor K dwarf
• Probing the Spin-Induced Quadrupole Moment of Massive Black Holes with the Inspiral of Binary Black Holes
• New Constraints on Sodium Production in Globular Clusters From the ${}^{23}$Na${(}^3$He$,\text{d}{)}^{24}$Mg Reaction
• Biased parameter inference of eccentric, spin-precessing binary black holes
• Spatially Resolved Circumgalactic Medium around a Star-Forming Galaxy Driving a Galactic Outflow at $z\approx 0.8$
• RadioSED I: Bayesian inference of radio SEDs from inhomogeneous surveys
• GEMS JWST: Transmission spectroscopy of TOI-5205b reveals significant stellar contamination and a metal-poor atmosphere
• Extended mass distribution of PBHs during QCD phase transition: SGWB and mini-EMRIs
• Low-Frequency Turnover Star Forming Galaxies I: Radio Continuum Observations and Global Properties
• A Bayesian inference and model selection algorithm with an optimisation scheme to infer the model noise power
• A Detection of Red Noise in PSR J1824$-$2452A and Projections for PSR B1937+21 using NICER X-ray Timing Data
• The JWST EXCELS Survey: gas-phase metallicity evolution at 2 < z < 8
• Which is which? Identification of the two compact objects in gravitational-wave binaries
• Constraints on Bianchi-I type universe with SH0ES anchored Pantheon+ SNIa data
• Searching for double-peak and doubly broken gravitational-wave spectra from Advanced LIGO-Virgo's first three observing runs
• Accelerating Bayesian Sampling for Massive Black Hole Binaries with Prior Constraints from Conditional Variational Autoencoder
• Comparing measures of the Hubble and BAO tensions in $\Lambda$CDM and possible solutions in $f(Q)$ gravity
• Nested Sampling for Non-Gaussian Inference in SLAM Factor Graphs
• Beyond GWTC-3: Analysing and verifying new gravitational-wave events from community catalogues
• SN 2019hcc: A Type II Supernova Displaying Early O II Lines
• Fast and faithful interpolation of numerical relativity surrogate waveforms using meshfree approximation
• Search for Coincident Gravitational Wave and Long Gamma-Ray Bursts from 4-OGC and the Fermi-GBM/Swift-BAT Catalog
• The Similar Seven: A set of very-alike exoplanets to test correlations between system parameters and atmospheric properties
• A complete measurement of a black-hole recoil through higher-order gravitational-wave modes
• Next-generation global gravitational-wave detector network: Impact of detector orientation on compact binary coalescence and stochastic gravitational-wave background searches
• Cosmological Parameter Estimation with a Joint-Likelihood Analysis of the Cosmic Microwave Background and Big Bang Nucleosynthesis
• Quasi-Periodic Peak Energy Oscillations in X-ray Bursts from SGR J1935+2154
• Eruptive mass loss less than a year before the explosion of superluminous supernovae: I. The cases of SN 2020xga and SN 2022xgc
• Accelerated parameter estimation of supermassive black hole binaries in LISA using a meshfree approximation
• The Way of Water: ALMA resolves H2O emission lines in a strongly lensed dusty star-forming galaxy at z $\sim$ 3.1
• Where has all the $r$-process gone? Timescales for GRB-Kilonovae to Enrich their Host Galaxies
• Radiative Transfer and Inversion codes for characterizing planetary atmospheres: an overview
• GausSN: Bayesian Time-Delay Estimation for Strongly Lensed Supernovae
• Constraining parity and Lorentz violations in gravity with future ground- and space-based gravitational wave detectors
• Dark Matter Substructure or Source Model Systematics? A Case Study of Cluster Lens Abell S1063
• Tidal dissipation in binary neutron star inspirals from hyperon bulk viscosity: Phase modeling and parameter estimation bias
• An independent search for annual modulation and its significance in ANAIS-112 data
• Fast and accurate parameter estimation of high-redshift sources with the Einstein Telescope
• The soft X-ray transient EP241021a: A cosmic explosion with a complex off-axis jet and cocoon from a massive progenitor
• Testing Ghasemi-Nodehi-Bambi metric parameters with quasi-periodic oscillations
• The Performance of Photometric Reverberation Mapping at High Redshift and the Reliability of Damped Random Walk Models
• Waging a Campaign: Results from an Injection-Recovery Study involving 35 numerical Relativity Simulations and three Waveform Models
• NGTS-EB-7, an eccentric, long-period, low-mass eclipsing binary
• The GAPS Programme at TNG. LXV. Precise density measurement of TOI-1430 b, a young planet with an evaporating atmosphere
• Modeling Star Formation Histories of Changing-Look AGN Host Galaxies with Prospector
• Asteroseismology with PBjam 2.0: measuring dipole mode frequencies in coupling regimes from main sequence to low-luminosity red giant stars
• A Transiting Giant on a 7.7-Year Orbit Revealed by TTVs in the TOI-201 System
• NIRPS and TESS reveal a peculiar system around the M dwarf TOI-756: A transiting sub-Neptune and a cold eccentric giant
• The SPACE Program. I. The featureless spectrum of HD 86226 c challenges sub-Neptune atmosphere trends
• A Stringent Upper Limit on Dark Matter Self-Interaction Cross Section from Cluster Strong Lensing
• Model-independent search for the quasinormal modes of gravitational wave echoes
• Detecting episodes of star formation using Bayesian model selection
• Impact of Bayesian Priors on the Inferred Masses of Quasi-Circular Intermediate-Mass Black Hole Binaries
• GravSphere2: A higher-order Jeans method for mass-modeling spherical stellar systems
• The impact of waveform systematics and Gaussian noise on the interpretation of GW231123
• Probing General Relativity in galactic scales at z $\sim 0.3$
• The changing transit shape of TOI-3884 b
• Unveiling the existence of nontensorial gravitational-wave polarizations from individual supermassive black hole binaries with pulsar timing arrays
• Accelerated inference of binary black-hole populations from the stochastic gravitational-wave background
• Vacuum birefringence and the polarized X-ray emission from a radio magnetar
• Cosmology on a Gravitational Wave Background
• Inferring spin tilts of binary black holes at formation with plus-era gravitational wave detectors
• Angular power spectrum of gravitational-wave transient sources as a probe of the large-scale structure
• A homogeneous TTV investigation of all TESS systems with a confirmed single transiting planet
• Marginalised Gaussian Processes with Nested Sampling
• Determination of Hubble constant from Megamaser Cosmology Project using Profile Likelihood
• Scalar fields around black hole binaries in LIGO-Virgo-KAGRA
• GRB 201104A: A "Repetitive" Short Gamma-Ray Burst?
• A Machine Learning Approach to Integral Field Unit Spectroscopy Observations: III. Disentangling Multiple Components in Hii regions
• A follow-up on intermediate-mass black hole candidates in the second LIGO-Virgo observing run with the Bayes Coherence Ratio
• TOI-3288 b and TOI-4666 b: two gas giants transiting low-mass stars characterised by NIRPS
• A massive quiescent galaxy confirmed in a protocluster at z=3.09
• Probing black hole `charge' from the binary black hole inspiral
• Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. VI: Confirmation of a Long-Period Giant Planet Discovered with a Single TESS Transit
• Distinct Rotational Evolution of Giant Planets and Brown Dwarf Companions
• Kinematic scaling relations of disc galaxies from ionised gas at $z\sim 1$ and their connection with dark matter haloes
• eROSITA-RU Tidal Disruption Events with Keck-I/LRIS: Sample Selection, Optical Properties, and Host Galaxy Demographics
• Observing Rayleigh-Taylor stable and unstable accretion through a Kalman filter analysis of X-ray pulsars in the Small Magellanic Cloud
• Unveiling the nature of HE 0107-5240
• Accurate and efficient photo-eccentric transit modeling
• Verification of the Black Hole Area Law with GW230814
• Luminous, rapidly declining supernovae as stripped transitional objects in low metallicity environments: the case of SN 2022lxg
• Population synthesis and parameter estimation of neutron stars with continuous gravitational waves and third-generation detectors
• A New Brown Dwarf Orbiting an M star and An Investigation on the Eccentricity Distribution of Transiting Long-Period Brown Dwarfs
• Simplifying asteroseismic analysis of solar-like oscillators: An application of principal component analysis for dimensionality reduction
• Informed total-error-minimizing priors: Interpretable cosmological parameter constraints despite complex nuisance effects
• Measuring the magnetic dipole moment and magnetospheric fluctuations of accretion-powered pulsars in the Small Magellanic Cloud with an unscented Kalman filter
• The ORT and the uGMRT Pulsar Monitoring Program : Pulsar Timing Irregularities & the Gaussian Process Realization
• Pixel-level modelling of group-scale strong lens CASSOWARY 19
• Active Galactic Nuclei in the Green Valley at z$\sim$0.7
• Detectability of Gravitational-Wave Memory with LISA: A Bayesian Approach
• Optimized localization for gravitational-waves from merging binaries
• Modeling Strong Lenses from Wide-Field Ground-Based Observations in KiDS and GAMA
• Anomalies in Hadronic $B$ Decays: an Update
• NLTE atmospheric modelling of the ultra-hot Jupiter WASP-178b and comparison with UV and optical observations
• Exploring the Evolution of Nonlinear Electrodynamics in the Universe: A Dynamical Systems Approach
• When Dark Matter Heats Up: A Model-Independent Search for Non-Cold Behavior
• Sensitivity to Sub-Io-sized Exosatellite Transits in the MIRI LRS Lightcurve of the Nearest Substellar Worlds
• Testing black hole space-times with the S2 star orbit: a Bayesian comparison
• TESS and HARPS-N unveil two planets transiting TOI-1453. A super-Earth and one of the lowest mass sub-Neptunes
• On the Binary Nature of the Progenitor of SN2015ap: Insights from Its Light Curve and Spectral Evolution
• Effects of Environment on the Size Evolution of Quiescent Galaxies: Comparing Galaxies in Clusters and in the Field at Two Rest-frame Wavelengths
• Modern Bayesian Sampling Methods for Cosmological Inference: A Comparative Study
• Leveraging cross-detector parameter consistency measures to enhance sensitivities of gravitational wave searches
• CMB constraints on monodromy inflation at strong coupling
• Probing Spin-Orbit Resonances with the Binary Black Hole Population
• Gravitational waves from eccentric binary neutron star mergers: Systematic biases and inadequacy of quasicircular templates
• Einstein@Home Searches for Gamma-ray Pulsars in the Inner Galaxy
• The "Little Dark Dot": Evidence for Self-interacting Dark Matter in the Strong Lens SDSS J0946+1006?
• Constraining the Stellar Masses and Origin of the Protostellar VLA 1623 System
• Robust parameter estimation from pulsar timing data
• MANGOS II: Five new giant planets orbiting low-mass stars
• Accounting for the Known Unknowns: A Parametric Framework to Incorporate Systematic Waveform Errors in Gravitational-Wave Parameter Estimation
• Mapping atmospheric features of the planetary-mass brown dwarf SIMP 0136 with JWST NIRISS
• Robust and fast parameter estimation for gravitational waves from binary neutron star merger remnants
• Inferring the spins of merging black holes in the presence of data-quality issues
• A joint effort to discover and characterize two resonant mini Neptunes around TOI-1803 with TESS, HARPS-N and CHEOPS
• Evidence for Three Subpopulations of Merging Binary Black Holes at Different Primary Masses
• Validation of TOI-1221 b: A warm sub-Neptune exhibiting TTVs around a Sun-like star
• A Mini-Neptune and a Venus-Zone Planet in the Radius Valley Orbiting the Nearby M2-dwarf TOI-1266: Validation with the Habitable-zone Planet Finder
• Along the Primary Curve: Simultaneous Source and Lens Reconstruction of Bright Arcs in Cluster Lenses
• Robust, Rapid, and Simple Gravitational-wave Parameter Estimation
• Characterization of low-mass companions to $\text{Kepler}$ objects of interest observed with APOGEE-N
• Direct Inference of Nuclear Equation-of-State Parameters from Gravitational-Wave Observations
• Parameter estimation of binary black holes in the endpoint of the up-down instability
• Probing populations of dark stellar remnants in the globular clusters 47 Tuc and Terzan 5 using pulsar timing
• Probing Cosmology with Baryon Acoustic Oscillations using Gravitational Waves
• A sub-Neptune transiting the young field star HD 18599 at 40 pc
• Gravitational lensing aided luminosity distance estimation for compact binary coalescences
• Impact on $L$-observables of a new combined analysis of $B_{d,s}\to K^{(\ast )}$ form factors
• 28 Years of Sun-as-a-star Extreme Ultraviolet Light Curves from SOHO EIT
• Are all models wrong? Falsifying binary formation models in gravitational-wave astronomy
• Testing modified gravity with the eccentric neutron star--black hole merger GW200105
• Probing magneto-ionic microstructure towards the Vela pulsar using a prototype SKA-Low station
• Gravitational-wave model for neutron star merger remnants with supervised learning
• Precise radial velocities of giant stars -- XVII. Distinguishing planets from intrinsically induced radial velocity signals in evolved stars
• Separated twins or just siblings? A multi-planet system around an M dwarf including a cool sub-Neptune
• Discovery of Volatile Gas in the Giant Impact Disk around the 150-Myr old HD 23514
• Equivalence of Dark Energy Models: A Theoretical and Bayesian Perspective
• A Moderate Albedo from Reflecting Aerosols on the Dayside of WASP-80 b Revealed by JWST/NIRISS Eclipse Spectroscopy
• Beyond LambdaCDM: How the Hubble tension challenges early universe physics
• GW231123: Overlapping Gravitational Wave Signals?
• Study of pulsar flux density and its variability with Parkes data archive
• Bayesian WIMP detection with the Cherenkov Telescope Array
• Constraining the modified friction in gravitational wave propagation with precessing black hole binaries
• Effects of calibration uncertainties on the detection and parameter estimation of isotropic gravitational-wave backgrounds
• TOI-2322: two transiting rocky planets close to the stellar rotation period and its first harmonic
• Evidence for a Nonzero Eccentricity Superpuff Exoplanet WASP-107 b Using JWST Occultation Observation
• BD-14 3065b (TOI-4987b): from giant planet to brown dwarf: evidence for deuterium burning in old age?
• Confronting primordial black holes with LIGO-Virgo-KAGRA and the Einstein Telescope
• HD 143811 AB b: A Directly Imaged Planet Orbiting a Spectroscopic Binary in Sco-Cen
• Dynamical Architectures of S-type Transiting Planets in Binaries II: A Dichotomy in Orbital Alignment of Small Planets in Close Binary Systems
• Evidence for an Atmosphere on the Ultra-Short Period super-Earth HD 3167 b
• Meet the Neighbors: Gas Rich "Buddy Galaxies" are Common Around Recently Quenched Massive Galaxies in the SQuIGG$\vec{L}$E Survey
• Searching for topological dark matter in LIGO data
• Multi-parameter Tests of General Relativity Using Bayesian Parameter Estimation with Principal Component Analysis for LISA
• Self-consistent treatment of thermal effects in neutron-star post-mergers: observational implications for third-generation gravitational-wave detectors
• Unmasking noise transients masquerading as intermediate-mass black hole binaries
• Comparison of $\Lambda$CDM and $R_h=ct$ with updated galaxy cluster $f_{gas}$ measurements using Bayesian inference
• Is PSR J0514$-$4002E in a PBH-NS binary?
• Candidate strongly lensed type Ia supernovae in the Zwicky Transient Facility archive
• Joint Inference of Population, Cosmology, and Neutron Star Equation of State from Gravitational Waves of Dark Binary Neutron Stars
• The Impact of $\text{CLEAN}$ing on Strong Gravitational Lens Modelling
• Enhancing gravitational-wave host localization with SKYFAST: rapid volume and inclination angle reconstruction
• Search for a Gravitational-Wave Background from Sound Speed Resonance from Advanced LIGO and Advanced Virgo's First Three Observing Runs
• STAR NRE: Solving supernova selection effects with set-based truncated auto-regressive neural ratio estimation
• A sub-Earth-mass planet orbiting Barnard's star: No evidence of transits in TESS photometry
• Can Neutron Star Tidal Effects Obscure Deviations from General Relativity?
• Inferring jet physics from neutron star - black hole mergers with gravitational waves
• Phase consistency test to identify type II strongly lensed gravitational wave signals using a single event
• Sky localization of gravitational waves from eccentric binaries
• AGN in the ULIRG HE 0435-5304
• Limits on the existence of totally reflective exotic compact objects with current and future gravitational-wave detectors
• Constraining Cubic Curvature Corrections to General Relativity with Quasi-Periodic Oscillations
• Gaussian discriminators between $\Lambda$CDM and wCDM cosmologies using expansion data
• A pipeline to search for signatures of line-of-sight acceleration in gravitational wave signals produced by compact binary coalescences
• Overlapping signals in next-generation gravitational wave observatories: A recipe for selecting the best parameter estimation technique
• Granulation signatures in 3D hydrodynamical simulations: evaluating background model performance using a Bayesian nested sampling framework
• Einstein@Home all-sky "bucket" search for continuous gravitational waves in LIGO O3 public data
• The Case for Space: Estimating Precise Time Delays from Ground- and Space-Based Observations of Lensed Supernovae with Glimpse
• Discovery of a Nearby Habitable Zone Super-Earth Candidate Amenable to Direct Imaging
• A long-duration gamma-ray burst of dynamical origin from the nucleus of an ancient galaxy
• Ten years of extreme gravity tests of general theory of relativity with gravitational-wave observations
• Testing general relativity with gravitational waves -- improving and extending Modified Dispersion Relation tests
• Accelerated inference of microlensed gravitational waves with machine learning
• Searching for a Galactic component in the IceCube track-like neutrino events
• Testing general relativity with amplitudes of subdominant gravitational-wave modes
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• The Indian Pulsar Timing Array Data Release 2: II. Customised Single-Pulsar Noise Analysis and Noise Budget
• NF-iSAM: Incremental Smoothing and Mapping via Normalizing Flows
• A Bayesian Inference Framework for Gamma-Ray Burst Afterglow Properties
• Arbitrary Marginal Neural Ratio Estimation for Simulation-based Inference
• Discovery of Galactic center ejected star in DESI DR1
• ${\tau }^9$ Eri: A bright pulsating magnetic Bp star in a 5.95-day double-lined spectroscopic binary
• YSES 2b is a background star: Differential astrometric M-dwarf measurements in time
• RedDots: Planetary masses in the GJ1061 system from planet-planet interaction
• A transiting rocky super-Earth and a non-transiting sub-Neptune orbiting the M dwarf TOI-771
• An Assessment of Organics Detection and Characterization on the Surface of Europa with Infrared Spectroscopy
• Unveiling the Dark Side of UV/Optical Bright Galaxies: Optically Thick Dust Absorption
• Detecting non-thermal emission in a solar microflare using nested sampling
• Planet Hunters NGTS: New Planet Candidates from a Citizen Science Search of the Next Generation Transit Survey Public Data
• Confronting compositional confusion through the characterisation of the sub-Neptune orbiting HD 77946
• Measurability of neutron star tidal deformability from merging neutron star-black hole binaries
• Using Strong Lensing to Detect Subhalos with Steep Inner Density Profiles
• Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog
• 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)
• Reverse-time analysis uncovers universality classes in directional biological dynamics
• Galaxy-galaxy strong lens perturbations: line-of-sight haloes versus lens subhaloes
• Fermi-GBM Observations of GRB 210812A: Signatures of a Million Solar Mass Gravitational Lens
• Time delay measurements with Broken Power Law model
• Characterizing the host galaxies and delay times of Ca-rich gap transients vs 91bg-like SNe and normal Type Ia SNe
• Decameter-sized Earth Impactors -- II: A Bayesian Inference Approach to Meteoroid Ablation Modeling
• Constraints on gravitational waves from the 2024 Vela pulsar glitch
• Closing the Evidence Gap: reddemcee, a Fast Adaptive Parallel Tempering Sampler
• The asymmetric structure of the inner disc around HD 142527 A with VLTI/MATISSE
• Measurement prospects for the pair-instability mass cutoff with gravitational waves
• An Archival Optical Counterpart Search for Extragalactic Fast X-Ray Transients Discovered by Einstein Probe
• Granulation signatures as seen by Kepler short-cadence data. I. A decoupling between granulation and oscillation timescales for dwarfs
• Gas-depleted planet formation occurred in the four-planet system around the red dwarf LHS 1903
• Illuminating the Mass Gap Through Deep Optical Constraint on a Neutron Star Merger Candidate S250206dm
• A distant brown dwarf coplanar to a warm Jupiter and a hot super-Earth
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• Atmospheric asymmetries in WASP-121 b revealed by rotational transits detected with JWST
• Discovery of a Barred-Spiral Galaxy at $z_{spec}$ = 3.16 II. The Star Formation History
• ASTEP confirmation of a pair of long-period Jupiter-sized planets with extremely low densities transiting TOI-791
• An Adolescent and Near-Resonant Planetary System Near the End of Photoevaporation
• Observational bounds on Dark Matter Admixed Neutron Stars from Gravitational Wave Data
• The Hubble PanCET Program: A Featureless Transmission Spectrum for WASP-29b and Evidence of Enhanced Atmospheric Metallicity on WASP-80b
• Dynamical masses of young stellar objects with the VLBA: DYNAMO-VLBA: Radio binary stars in Orion
• The dark and featureless surface of rocky exoplanet LHS 3844 b from JWST mid-infrared spectroscopy
• Photometric Constraints on Intermediate-mass Black Holes in the Galactic Centre
• Bayesian Framework to Follow-up Continuous Gravitational Wave Candidates from Deep Surveys
• TESS phase curve of ultra-hot Jupiter WASP-189 b
• Challenging a binary neutron star merger interpretation of GW230529
• Can Big Black Holes Merge with the Smallest Black Holes?
• The RoPES project with HARPS and HARPS-N II. A third planet in the multi-planet system HD 176986
• Assessing robustness and bias in 1D retrievals of 3D Global Circulation Models at high spectral resolution: a WASP-76 b simulation case study in emission
• First Results from WINERED: Detection of Emission Lines from Neutral Iron and a Combined Set of Trace Species on the Dayside of WASP-189 b
• A Bayesian approach to time-domain Photonic Doppler Velocimetry
• Bayesian Analysis of the ${}^{86}$Sr$(\alpha ,\alpha )$ Reaction to Constrain the ${}^{86}$Sr$(\alpha ,n)$ Cross Section at Astrophysical Energies
• Discovery of a transiting hot water-world candidate orbiting Ross 176 with TESS and CARMENES
• Systematics in ETG Mass Profile Modelling: Strong Lensing & Stellar Dynamics
• NGTS-EB-8: A double-lined eclipsing M+M binary discovered by citizen scientists
• Using overlap of sky localization probability maps for filtering potentially lensed pairs of gravitational-wave signals
• Beetroots: spatially-regularized Bayesian inference of physical parameter maps -- Application to Orion
• Characterizing CO Emitters in the SSA22-AzTEC26 Field
• Search for giant planets in M67 V: a warm Jupiter orbiting the turn-off star S1429
• A Gaussian process framework for testing general relativity with gravitational waves
• Characterizing Compact-object Binaries in the Lower Mass Gap with Gravitational Waves
• Kilohertz Gravitational Waves from Binary Neutron Star Mergers: Full Spectrum Analyses and High-density Constraints on Neutron Star Matter
• Accelerating gravitational-wave parameterized tests of General Relativity using a multiband decomposition of likelihood
• Three Hot Jupiters transiting K-dwarfs with a significant heavy element mass
• Deep follow-up for gravitational-wave inference: a case study with GW151226
• An independent search for Jovian neutrinos using BOREXINO data
• Simulations of astrometric planet detection in Alpha Centauri by intensity interferometry
• Inferring Evidence from Nested Sampling Data via Information Field Theory
• Significant challenges for astrophysical inference with next-generation gravitational-wave observatories
• Measuring Hubble Constant with Dark Neutron Star-Black Hole Mergers
• A gating-and-inpainting perspective on GW150914 ringdown overtone: understanding the data analysis systematics
• A new third planet and the dynamical architecture of the HD33142 planetary system
• The impact of precession and higher-order multipoles for gravitational wave cosmological inference
• Methane on the temperate exo-Saturn TOI-199b
• Statistical biases in parametrized searches for gravitational-wave polarizations
• Evidence of large recoil velocity from a black hole merger signal
• Reducing systematic uncertainties in gravitational-wave population analyses by increasing the detection threshold
• The DESI DR1 Peculiar Velocity Survey: global zero-point and $H_0$ constraints
• TOI-1201 b: A mini-Neptune transiting a bright and moderately young M dwarf
• Improving exoplanet mass characterisation with Bayesian model selection using the Learned Harmonic Mean Estimator
• Spin-Orbit Geometry of AU Mic b and c from Back-to-Back Transits Observed Contemporaneously with Magellan PFS, LCOGT, and CHEOPS
• The Longest-period Young Transiting Exoplanets. A Duo of Puffy Giants inside a Debris Disk
• Constraining the orbit of the retrograde planet in the $\nu$ Octantis system
• Sector-Resolved Bayesian Model Averaging for DESI-Era Cosmology
• Dynamical analysis of the 5:1 mean-motion resonance of the HD 202206 system
• Persistence of post-Newtonian amplitude structure in binary black hole mergers
• Modifying $\Lambda$CDM dynamics via out-of-equilibrium axions: reconciling SH0ES and DESI $H_0$ values
• A restless supermassive black hole in the galaxy J0437+2456
• Evidence for Dynamical Filtering: High Binary Fraction, Hard-binary Excess, and Unresolved Triples in the Surviving Core of NGC 6791
• Discovery and Characterization of Three New High-amplitude delta Scuti Stars from TESS Observations
• Search for Annual Modulation in Combined ANAIS 112 and COSINE 100 Data using Bayesian Model Comparison
• Probing the peak of star formation with the stochastic background of binary black hole mergers
• Detection of periodic transit timing variations in warm sub-Saturn HD 332231 b
• Exploring the surface of HD 189733 via Doppler shadow analysis of planetary transits
• Toward a Unified Understanding of the Dense Matter Equation of State
• Black-box density function estimation using recursive partitioning
• Waveform model for the $(\ell =2,m=0)$ spherical harmonic and the displacement memory contribution from precessing binary black holes
• A Warm Massive Pair of Planets around TOI-1232 Revealed with Transit-timing Variations and Doppler Spectroscopy
• Bayesian Model Comparison of $R_h=ct$ versus $\Lambda$CDM using HII galaxy Hubble diagram
• Comparative Bayesian SED Fitting of PEARLSDG
• Optimizing Gaussian Process Kernels Using Nested Sampling and ABC Rejection for H(z) Reconstruction
• MatBYIB: A Matlab-based code for Bayesian inference of extreme mass-ratio inspiral binary with arbitrary eccentricity
• TOI-333b: A Neptune Desert planet around a F7V star
• TRIShUL: Technique for Reconstructing magnetic Interstellar Structure Using starLight polarization
• Measuring the crust-superfluid coupling time-scale for 105 UTMOST pulsars with a Kalman filter
• Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data
• Confirmation of SRGt 062340.2-265751 as a nova-like cataclysmic variable with a possible magnetic nature
• Probing the disk-jet coupling in M87
• Assessment of normalizing flows for parameter estimation on time-frequency representations of gravitational-wave data
• Constraining the selection corrected luminosity function and total pulse count for radio transients
• Prospects for Measuring Black Hole Masses using TDEs with the Vera C. Rubin Observatory
• A Radio-selected Population of Dark, Long Gamma-ray Bursts: Comparison to the Long Gamma-ray Burst Population and Implications for Host Dust Distributions
• The maximum mass and rotational kinetic energy of rapidly rotating neutron stars
• Oxyster: A Circumgalactic Low-ionization Oxygen Nebula next to a Starburst Galaxy at $z\sim 1$
• Lightweight posterior construction for gravitational-wave catalogs with the Kolmogorov-Arnold network
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• Constraining Scalar Charge in Neutron Stars through Gravitational Wave Signals from NSBH Mergers
• Revisiting the secondary eclipses of KELT-1b using TESS observations
• SQuIGGLE: Studying Quenching in Intermediate-z Galaxies -- Gas, AnguLar Momentum, and Evolution
• The Progenitor Systems of Classical Novae in M31
• How narrow is the M87* ring? I. The choice of closure likelihood function
• Probing Dark Matter with Strong Gravitational Lensing through an Effective Density Slope
• Model-agnostic search of gravitational wave echoes in LVK data
• Applicability of multi-component study on Bayesian searches for targeted anisotropic stochastic gravitational-wave background
• Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing?
• Two Rings and a Marginally Resolved, 5 AU, Disk Around LkCa 15 Identified Via Near Infrared Sparse Aperture Masking Interferometry
• Mapping the 3D Kinematical Structure of the Gas Disk of HD 169142
• Constraining the gravitational-wave emission of core-collapse supernovae with ground-based detectors
• Simulation-calibrated Bayesian inference for progenitor properties of the microquasar SS 433
• Hybrid waveforms for precessing quasi-circular binary systems
• APES: Approximate Posterior Ensemble Sampler
• XMM-Newton follow-up of two eROSITA X-ray binary candidates
• A Pearl in the Shell: an ultra-compact dwarf within the tidal debris surrounding spiral galaxy NGC 7531
• Investigating the extent of bladed terrain on Pluto via photometric surface roughness
• The MWA Long Baseline Epoch of Reionisation Survey: I. Improved Source Catalogue for the EoR 0 field
• Bayesian vs Frequentist: Comparing Bayesian model selection with a frequentist approach using the iterative smoothing method
• Parameter estimation for space-based gravitational wave detectors with ringdown signals
• Impact of Variable Photospheric Radius on Exoplanet Atmospheric Retrievals
• Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses
• Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension
• The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope
• Constraining the population of dark matter halo shapes using hierarchical inference with extragalactic stellar streams
• The Sequential Monte Carlo goes NUTS: Boosting Gravitational-Wave Inference
• Short gamma-ray burst progenitors have short delay times
• Systematic bias due to eccentricity in parameter estimation for merging binary neutron stars : Spinning case
• Probing missing physics from inspiralling compact binaries via time-frequency tracks
• A new method to correct for host star variability in multi-epoch observations of exoplanet transmission spectra
• Plunge-Merger-Ringdown Tests of General Relativity with GW250114
• Constraints on AvERA Cosmologies from Cosmic Chronometers and Type Ia Supernovae
• A VLA View of the Flared, Asymmetric Disk Around the Class 0 Protostar L1527 IRS
• Hidden Gems in TESS: sherlock finds two new rocky planets around nearby M dwarfs
• Characterization of merging black holes with two precessing spins
• Applying higher-modes consistency test on GW190814 : lessons on no-hair theorem, nature of the secondary compact object and waveform modeling
• Circular Mystery: Exploring Diffuse Emission Surrounding a Radio Galaxy with uGMRT and VLA Multiwavelength Observations
• Uncovering subdominant multipole asymmetries in binary black-hole mergers
• Cosmology with Love: Measuring the Hubble constant using neutron star universal relations
• How Holographic is the Dark Energy? A Spline Nodal reconstruction approach
• False Alarm Rate based Statistical Detection Limit for Astronomical Photon Detectors
• The Missing Multipole Problem: Investigating biases from model starting frequency in gravitational-wave analyses
• Identifying Host Galaxies of Binary Black Hole Mergers with Next-Generation Gravitational Wave Detector Networks
• Probing the partition function for temperature-dependent potentials with nested sampling
• Detection of the stochastic gravitational wave background with the space-borne gravitational-wave detector network
• Characterizing Binary Black Hole Subpopulations in GWTC-4 with Binned Gaussian Processes: On the Origins of the $35M_{\odot }$ Peak
• NIRPS tightens the mass estimate of GJ 3090 b and detects a planet near the stellar rotation period
• The GAPS Programme at the TNG: LXX. TOI-5734b: A hot sub-Neptune orbiting a relatively young K dwarf with an Earth-like density
• Towards a Field Based Bayesian Evidence Inference from Nested Sampling Data
• Extending Ground-Based Gravitational-Wave Sensitivity to 5 Hz
• Information content of JWST transmission spectroscopy of the exoplanet HAT-P-12b from the optical to the mid-infrared
• Blowing Star Formation Away in AGN Hosts (BAH) -- III. Serendipitous discovery of a $z\sim 2.9$ star-forming galaxy lensed by the galactic bulge of CGCG 012-070 using JWST NIRSpec
• Improved Constraints on Non-Kerr Deviations from Binary Black Hole Inspirals Using GWTC-4 Data
• Sibling Sub-Neptunes Around Sibling M Dwarfs: TOI-521 and TOI-912
• Gravitational-wave astronomy requires population-informed parameter estimation
• No model-independent evidence for a peak in binary black hole spin (mis)alignments
• Prospects for distinguishing dynamical tides in inspiralling binary neutron stars with third generation gravitational-wave detectors
• Determination of the best dark matter profile for the Milky Way with Gaia DR3 using Bayesian Model Comparison
• Constraints on the gravitational potential from DESI DR2 BAO and its implications for the local void scenario
• POSEIDON II: The Anti-Aligned Orbit of the Warm Neptune TOI-1710 A b
• Constraining Early Dark Energy cosmological models with Big Bang Nucleosynthesis
• Observational Biases and Improved Modelling of Off-axis Relativistic Jets
• Improved characterization of the TOI-2141 system: a dense sub-Neptune with non-transiting inner and outer companions
• Low-efficiency long gamma-ray bursts: A case study with AT2020blt
• High-frequency continuous gravitational waves searched in LIGO O3 public data with Einstein@Home
• JWST-TST High Contrast: First Direct Spectroscopy of GJ 504 b reveals Clouds and Possible Metal Enrichment
• MINDS survey of silicates in T Tauri disks: Correlation between dust and gas