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.

arXiv comment28 pages, 12 figures, submitted to MNRAS; code available at https://github.com/joshspeagle/dynesty

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• Caught in the Act: Core-powered Mass-loss Predictions for Observing Atmospheric Escape
• Heavy double neutron stars: birth, mid-life and death
• Spin it as you like: the (lack of a) measurement of the spin tilt distribution with LIGO-Virgo-KAGRA binary black holes
• Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA
• Dynamical dark energy models in the light of Gravitational-Wave Transient Catalogues
• Parameter Estimation Bias From Overlapping Binary Black Hole Events In Second Generation Interferometers
• Model Comparison of $\Lambda$CDM vs $R_h=ct$ using Cosmic Chronometers
• Blind spots and biases: the dangers of ignoring eccentricity in gravitational-wave signals from binary black holes
• Constraints on the phase transition and nuclear symmetry parameters from PSR $\mathrm{J}0740+6620$ and multimessenger data of other neutron stars
• Fast, faithful, frequency-domain effective-one-body waveforms for compact binary coalescences
• Constraints on warm dark matter from UV luminosity functions of high-z galaxies with Bayesian model comparison
• The Diverse Molecular Gas Content of Massive Galaxies Undergoing Quenching at z~1
• Improved post-Newtonian waveform model for inspiralling precessing-eccentric compact binaries
• HST PanCET Program: A Complete Near-UV to Infrared Transmission Spectrum for the Hot Jupiter WASP-79b
• Measuring binary black hole orbital-plane spin orientations
• Swift J1727.8-1613 has the Largest Resolved Continuous Jet Ever Seen in an X-ray Binary
• JADES + JEMS: A Detailed Look at the Buildup of Central Stellar Cores and Suppression of Star Formation in Galaxies at Redshifts 3 < z < 4.5
• Model selection applied to reconstructions of the Dark Energy
• Probing the speed of scalar-induced gravitational waves with pulsar timing arrays
• Measuring the properties of active galactic nuclei disks with gravitational waves
• JWST reveals a rapid and strong day side variability of 55 Cancri e
• GA-NIFS: Early-stage feedback in a heavily obscured AGN at $z=4.76$
• TOI-269 b: An eccentric sub-Neptune transiting a M2 dwarf revisited with ExTrA
• 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
• Keck/KPIC Emission Spectroscopy of WASP-33b
• Keck Integral-Field Spectroscopy of M87 Reveals an Intrinsically Triaxial Galaxy and a Revised Black Hole Mass
• 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
• The Magnificent Five Images of Supernova Refsdal: Time Delay and Magnification Measurements
• 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
• Reconstructing the Assembly of Massive Galaxies. I: The Importance of the Progenitor Effect in the Observed Properties of Quiescent Galaxies at $z\approx 2$
• Optical Transmission Spectroscopy of the Terrestrial Exoplanet LHS 3844b from 13 Ground-Based Transit Observations
• The dynamic magnetosphere of Swift J1818.0$-$1607
• How narrow is the M87* ring? II. A new geometric model
• An Early-Time Optical and Ultraviolet Excess in the type-Ic SN 2020oi
• The stellar populations of quiescent ultra-diffuse galaxies from optical to mid-infrared spectral energy distribution fitting
• PyAutoFit: A Classy Probabilistic Programming Language for Model Composition and Fitting
• The K2-3 system revisited: testing photoevaporation and core-powered mass loss with three small planets spanning the radius valley
• A Search for Gravitational Waves from Binary Mergers with a Single Observatory
• Toward the unambiguous identification of supermassive binary black holes through Bayesian inference
• Mapping the Gravitational-wave Sky with LISA: A Bayesian Spherical Harmonic Approach
• Evidence for a correlation between binary black hole mass ratio and black-hole spins
• The GTC exoplanet transit spectroscopy survey XI. Possible detection of Rayleigh scattering in the atmosphere of the Saturn-mass planet WASP-69b
• The Radcliffe Wave is Oscillating
• Multi-waveform inference of gravitational waves
• Searching for anisotropy in the distribution of binary black hole mergers
• 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
• Photometric detection at $7.7\mu \mathrm{m}$ of a galaxy beyond redshift $14$ with JWST/MIRI
• Abell 1201: Detection of an Ultramassive Black Hole in a Strong Gravitational Lens
• On the Detection of Exomoons Transiting Isolated Planetary-Mass Objects
• Evidence for profile changes in PSR J1713+0747 using the uGMRT
• TESS Reveals a Short-period Sub-Neptune Sibling (HD 86226c) to a Known Long-period Giant Planet
• 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
• The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc
• Correlations in gravitational-wave reconstructions from eccentric binaries: A case study with GW151226 and GW170608
• 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
• Where intermediate-mass black holes could hide in the Galactic Centre: A full parameter study with the S2 orbit
• Constraining short gamma-ray burst jet properties with gravitational waves and gamma rays
• PHANGS-MUSE: Detection and Bayesian classification of ~40000 ionised nebulae in nearby spiral galaxies
• A pair of warm giant planets near the 2:1 mean motion resonance around the K-dwarf star TOI-2202
• Detection and parameter estimation challenges of Type-II lensed binary black hole signals
• A strong He II $\lambda$1640 emitter with extremely blue UV spectral slope at $z=8.16$: presence of Pop III stars?
• Discovery of the Magellanic Stellar Stream Out to 100 Kiloparsecs
• Resonant tides in binary neutron star mergers: analytical-numerical relativity study
• The unluckiest star: A spectroscopically confirmed repeated partial tidal disruption event AT 2022dbl
• Deep Synoptic Array science: A massive elliptical host among two galaxy-cluster fast radio bursts
• Early JWST imaging reveals strong optical and NIR color gradients in galaxies at $z\sim 2$ driven mostly by dust
• At least one in a dozen stars exhibits evidence of planetary ingestion
• An exploration of model degeneracies with a unified phase curve retrieval analysis: The light and dark sides of WASP-43 b
• AT 2020wey and the class of faint and fast Tidal Disruption Events
• First semi-empirical test of the white dwarf mass-radius relationship using a single white dwarf via astrometric microlensing
• A super-Earth and a mini-Neptune near the 2:1 MMR straddling the radius valley around the nearby mid-M dwarf TOI-2096
• Gravitational waves from binary black hole mergers surrounded by scalar field clouds: Numerical simulations and observational implications
• Kalkayotl: A cluster distance inference code
• Beyond the bulge-halo conspiracy? Density profiles of Early-type galaxies from extended-source strong lensing
• The geometric albedo of the hot Jupiter HD 189733b measured with CHEOPS
• Neural network reconstructions for the Hubble parameter, growth rate and distance modulus
• TOI-2525 b and c: A pair of massive warm giant planets with a strong transit timing variations revealed by TESS
• Planet Engulfment Detections are Rare According to Observations and Stellar Modeling
• 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
• A Bayesian Population Model for the Observed Dust Attenuation in Galaxies
• Betelgeuse fainter in the sub-millimetre too: an analysis of JCMT and APEX monitoring during the recent optical minimum
• Exploring the Impact of Microlensing on Gravitational Wave Signals: Biases, Population Characteristics, and Prospects for Detection
• Detection and parameter estimation of binary neutron star merger remnants
• {\sc mirkwood:} Fast and Accurate SED Modeling Using Machine Learning
• Testing strong lensing subhalo detection with a cosmological simulation
• NANOGrav hints for first-order confinement-deconfinement phase transition in different QCD-matter scenarios
• TOI-3884 b: A rare 6-R${}_{\oplus }$ planet that transits a low-mass star with a giant and likely polar spot
• 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
• Probing lens-induced gravitational-wave birefringence as a test of general relativity
• VARAHA: A Fast Non-Markovian sampler for estimating Gravitational-Wave posteriors
• Spectroscopic r-Process Abundance Retrieval for Kilonovae I: The Inferred Abundance Pattern of Early Emission from GW170817
• Systematic errors induced by the elliptical power-law model in galaxy-galaxy strong lens modeling
• Lorentz Invariance Violation Limits from the Spectral Lag Transition of GRB~190114C
• Hot Rocks Survey I : A possible shallow eclipse for LHS 1478 b
• SBI++: Flexible, Ultra-fast Likelihood-free Inference Customized for Astronomical Applications
• Constraint on phase transition with the multimessenger data of neutron stars
• 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
• HD 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone
• Finding binary black holes in the Milky Way with LISA
• GW190521: Search for Echoes due to Stimulated Hawking Radiation from Black Holes
• Direct Constraints on the Extremely Metal-Poor Massive Stars Underlying Nebular C IV Emission from Ultra-Deep HST/COS Ultraviolet Spectroscopy
• On the detectability of higher harmonics with LISA
• GRB 200716C: Evidence for a Short Burst Being Lensed
• Asteroseismic Signatures of Core Magnetism and Rotation in Hundreds of Low-Luminosity Red Giants
• A Solar System formation analogue in the Ophiuchus star-forming complex
• Multiple Clues for Dayside Aerosols and Temperature Gradients in WASP-69 b from a Panchromatic JWST Emission Spectrum
• A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics
• Discovery of the optical afterglow and host galaxy of short GRB181123B at $z=1.754$: Implications for Delay Time Distributions
• Population Properties of Gravitational-Wave Neutron Star--Black Hole Mergers
• LRG-BEASTS: sodium absorption and Rayleigh scattering in the atmosphere of WASP-94A b using NTT/EFOSC2
• Simultaneous Optical Transmission Spectroscopy of a Terrestrial, Habitable-Zone Exoplanet with Two Ground-Based Multi-Object Spectrographs
• TOI-132 b: A short-period planet in the Neptune desert transiting a $V=11.3$ G-type star
• Low-latency gravitational wave alert products and their performance at the time of the fourth LIGO-Virgo-KAGRA observing run
• Numerical-Relativity-Informed Effective-One-Body model for Black-Hole-Neutron-Star Mergers with Higher Modes and Spin Precession
• Exploring the Hubble tension with a late time Modified Gravity scenario
• 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
• Planet Engulfment Signatures in Twin Stars
• Deep Hubble Space Telescope Observations of GW170817: Complete Light Curves and the Properties of the Galaxy Merger of NGC 4993
• pygwb: Python-based library for gravitational-wave background searches
• How Well Can We Measure Galaxy Dust Attenuation Curves? The Impact of the Assumed Star-Dust Geometry Model in SED Fitting
• The Aligned Orbit of the Eccentric Proto Hot Jupiter TOI-3362b
• 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
• 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
• Parameterised population models of transient non-Gaussian noise in the LIGO gravitational-wave detectors
• Quality over Quantity: Optimizing pulsar timing array analysis for stochastic and continuous gravitational wave signals
• First constraint on the dissipative tidal deformability of neutron stars
• 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
• Testing Lorentz Invariance of Gravity in the Standard Model Extension with GWTC-3
• Combining effective-one-body accuracy and reduced-order-quadrature speed for binary neutron star merger parameter estimation with machine learning
• Gravitational-wave population inference at past time infinity
• Constraining the Gravitational Potential from the Projected Morphology of Extragalactic Tidal Streams
• Inferring the population properties of binary black holes from unresolved gravitational waves
• Can Assembly Bias Explain the Lensing Amplitude of the BOSS CMASS Sample in a Planck Cosmology?
• Forward Modeling of Double Neutron Stars: Insights from Highly-Offset Short Gamma-Ray Bursts
• 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
• Spitzer Reveals Evidence of Molecular Absorption in the Atmosphere of the Hot Neptune LTT 9979b
• Frequency-Domain Analysis of Black-Hole Ringdowns
• Interplay of spin-precession and higher harmonics in the parameter estimation of binary black holes
• Ground-based Optical Transmission Spectroscopy of the Nearby Terrestrial Exoplanet LTT 1445Ab
• Reconstructing the Genealogy of LIGO-Virgo Black Holes
• Measuring properties of primordial black hole mergers at cosmological distances: effect of higher order modes in gravitational waves
• Template bank for compact binary mergers in the fourth observing run of Advanced LIGO, Advanced Virgo, and KAGRA
• Eccentricity-induced systematic error on parametrized tests of general relativity: Hierarchical Bayesian inference applied to a binary black hole population
• Constraining nuclear parameters using Gravitational waves from f-mode Oscillations in Neutron Stars
• Interpreting the X-ray afterglows of gamma-ray bursts with radiative losses and millisecond magnetars
• Analysis of a subsolar-mass compact binary candidate from the second observing run of Advanced LIGO
• A sub-Earth-mass planet orbiting Barnard's star
• Eccentric or circular? A reanalysis of binary black hole gravitational wave events for orbital eccentricity signatures
• A transiting, temperate mini-Neptune orbiting the M dwarf TOI-1759 unveiled by TESS
• Dark matter profiles of SPARC galaxies: a challenge to fuzzy dark matter
• A study of the Inspiral-Merger-Ringdown Consistency Test with gravitational-wave signals from compact binaries in eccentric orbits
• Systematic biases due to waveform mismodeling in parametrized post-Einsteinian tests of general relativity: The impact of neglecting spin precession and higher modes
• An M dwarf accompanied by a close-in giant orbiter with SPECULOOS
• A Generalized Semi-Analytic Model for Magnetar-Driven Supernovae
• Constraining spontaneous black hole scalarization in scalar-tensor-Gauss-Bonnet theories with current gravitational-wave data
• Model exploration in gravitational-wave astronomy with the maximum population likelihood
• Minutes-duration Optical Flares with Supernova Luminosities
• 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
• TOI-3984 A b and TOI-5293 A b: two temperate gas giants transiting mid-M dwarfs in wide binary systems
• The Issues of Mismodelling Gravitational-Wave Data for Parameter Estimation
• Search for Lorentz Invariance Violation from stacked Gamma-Ray Burst spectral lag data
• TOI-2257 b: A highly eccentric long-period sub-Neptune transiting a nearby M dwarf
• Accelerating Multi-Model Bayesian Inference, Model Selection and Systematic Studies for Gravitational Wave Astronomy
• Compact Starburst Galaxies with Fast Outflows: Central Escape Velocities and Stellar Mass Surface Densities from Multi-band Hubble Space Telescope Imaging
• Molecular Gas Reservoirs in Massive Quiescent Galaxies at $\mathrm{z}\sim 0.7$ Linked to Late Time Star Formation
• Bayesian model selection on Scalar $\epsilon$-Field Dark Energy
• The distant, galaxy cluster environment of the short GRB 161104A at $z\sim 0.8$ and a comparison to the short GRB host population
• Impact of updated Multipole Love numbers and f-Love Universal Relations in the context of Binary Neutron Stars
• Adiabatically compressed wave dark matter halo and intermediate-mass ratio inspirals
• The population of merging compact binaries inferred using gravitational waves through GWTC-3
• TOI-1728b: The Habitable-zone Planet Finder confirms a warm super Neptune orbiting an M dwarf host
• DESI Dark Energy Time Evolution is Recovered by Cosmologically Coupled Black Holes
• JWST-TST DREAMS: NIRSpec/PRISM Transmission Spectroscopy of the Habitable Zone Planet TRAPPIST-1 e
• Kernel Selection for Gaussian Process in Cosmology: with Approximate Bayesian Computation Rejection and Nested Sampling
• Measurability of precession and eccentricity for heavy binary-black-hole mergers
• 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
• Nested sampling cross-checks using order statistics
• 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
• Starlight-polarization-based tomography of the magnetized interstellar medium: PASIPHAE's line-of-sight inversion method
• 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
• Measuring tidal effects with the Einstein Telescope: A design study
• 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
• Variational Inference as an alternative to MCMC for parameter estimation and model selection
• No-go guide for the Hubble tension: late-time or local-scale new physics
• Planets larger than Neptune have elevated eccentricities
• The Cosmic Dipole in the Quaia Sample of Quasars: A Bayesian Analysis
• New Gravitational Wave Discoveries Enabled by Machine Learning
• Discovery and mass measurement of the hot, transiting, Earth-sized planet GJ 3929 b
• Revisiting the Gas Kinematics in SSA22 Lyman-$\alpha$ Blob 1 with Radiative Transfer Modeling in a Multiphase, Clumpy Medium
• J0107a: A Barred Spiral Dusty Star-forming Galaxy at $z=2.467$
• Unraveling information about supranuclear-dense matter from the complete binary neutron star coalescence process using future gravitational-wave detector networks
• Three long period transiting giant planets from TESS
• MiMO: Mixture Model for Open Clusters in Color-Magnitude Diagrams
• Constructing high-fidelity halo merger trees in AbacusSummit
• Which black hole is spinning? Probing the origin of black-hole spin with gravitational waves
• A search for planetary companions around 800 pulsars from the Jodrell Bank pulsar timing programme
• Bioverse: The Habitable Zone Inner Edge Discontinuity as an Imprint of Runaway Greenhouse Climates on Exoplanet Demographics
• Supernova SN 2020faa -- an iPTF14hls look-alike?
• Improved analysis of GW190412 with a precessing numerical relativity surrogate waveform model
• An environmental analysis of the fast transient AT2018cow and implications for its progenitor and late-time brightness
• Bayesian Accretion Modeling: Axisymmetric Equatorial Emission in the Kerr Spacetime
• Fitting the light curves of Sagittarius A* with a hot-spot model
• The cosmic build-up of dust and metals. Accurate abundances from GRB-selected star-forming galaxies at $1.7<z<6.3$
• Identification of Gravitational-waves from Extreme Mass Ratio Inspirals
• Confirmation of an He I evaporating atmosphere around the 650-Myr-old sub-Neptune HD235088 b (TOI-1430 b) with CARMENES
• The first degree-scale starlight-polarization-based tomography map of the magnetized interstellar medium
• A hidden active galactic nucleus powering bright [O III] nebulae in a protocluster at $z=4.5$ revealed by JWST
• BOWIE-ALIGN: JWST reveals hints of planetesimal accretion and complex sulphur chemistry in the atmosphere of the misaligned hot Jupiter WASP-15b
• The Return of GOLUM: Improving Distributed Joint Parameter Estimation for Strongly-Lensed Gravitational Waves
• An eccentric Brown Dwarf eclipsing an M dwarf
• Fast and robust Bayesian Inference using Gaussian Processes with GPry
• Linear to circular conversion in the polarized radio emission of a magnetar
• 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
• Simple and statistically sound recommendations for analysing physical theories
• Multimass modelling of Milky Way globular clusters -- I. Implications on their stellar initial mass function above 1 M${}_{\odot }$
• Constraining the Distance to the North Polar Spur with Gaia DR2
• Radio jet precession in M81*
• Gaussian processes for radial velocity modeling Better rotation periods and planetary parameters with the quasi-periodic kernel and constrained priors
• Exploring over 700 massive quiescent galaxies at z = 2-7: Demographics and stellar mass functions
• 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
• The MASSIVE Survey -- XVII. A Triaxial Orbit-based Determination of the Black Hole Mass and Intrinsic Shape of Elliptical Galaxy NGC 2693
• Searching for quasi-periodic oscillations in astrophysical transients using Gaussian processes
• Orbital eccentricity in a neutron star - black hole merger
• Across the Green Valley with HST grisms: colour evolution, crossing time-scales and the growth of the red sequence at $z=1.0-1.8$
• LRG-BEASTS: Ground-based Detection of Sodium and a Steep Optical Slope in the Atmosphere of the Highly Inflated Hot-Saturn WASP-21b
• Fast Parameter Estimation of Binary Mergers for Multimessenger Followup
• Applications of machine learning in gravitational wave research with current interferometric detectors
• Barry and the BAO Model Comparison
• The anti-aligned spin of GW191109: glitch mitigation and its implications
• The ALMA-CRISTAL survey. Discovery of a 15 kpc-long gas plume in a $z=4.54$ Lyman-$\alpha$ blob
• Coupled Multi Scalar Field Dark Energy
• Improving Detection of Gravitational wave Microlensing Using Repeated Signals Induced by Strong Lensing
• Fast likelihood evaluation using meshfree approximations for reconstructing compact binary sources
• LISA stellar-mass black hole searches with semicoherent and particle-swarm methods
• Adapting to noise distribution shifts in flow-based gravitational-wave inference
• Evidence of wind signatures in the gas velocity profiles of Red Geysers
• 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
• Testing No-Hair Theorem by Quasi-Periodic Oscillations: the quadrupole of GRO J1655$-$40
• SN 2020bqj: a Type Ibn supernova with a long lasting peak plateau
• Bioverse: a simulation framework to assess the statistical power of future biosignature surveys
• The Galactic Distribution of Phosphorus: A Survey of 163 Disk and Halo Stars
• TESS discovery of a sub-Neptune orbiting a mid-M dwarf TOI-2136
• The Detection of Transiting Exoplanets by Gaia
• The curious case of EP241021a: Unraveling the mystery of its exceptional rebrightening
• TOI-969: a late-K dwarf with a hot mini-Neptune in the desert and an eccentric cold Jupiter
• A New Method For Studying Exoplanet Atmospheres Using Planetary Infrared Excess
• The Aemulus Project VI: Emulation of beyond-standard galaxy clustering statistics to improve cosmological constraints
• Parameter estimation methods for analyzing overlapping gravitational wave signals in the third-generation detector era
• Gravitational waves carry information beyond effective spin parameters but it is hard to extract
• ACCESS: Confirmation of a Clear Atmosphere for WASP-96b and a Comparison of Light Curve Detrending Techniques
• An ALMA Gas-dynamical Mass Measurement of the Supermassive Black Hole in the Local Compact Galaxy UGC 2698
• Revising the Giant Planet Mass-Metallicity Relation: Deciphering the Formation Sequence of Giant Planets
• 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
• Efficient parameter inference for gravitational wave signals in the presence of transient noises using temporal and time-spectral fusion normalizing flow
• Prospects for Taiji to detect a gravitational-wave background from cosmic strings
• Characterization of a set of small planets with TESS and CHEOPS and an analysis of photometric performance
• Ordering the confusion: A study of the impact of lens models on gravitational-wave lensing detection capabilities
• Sub-stellar Companions of Intermediate-mass Stars with CoRoT: CoRoT-34b, CoRoT-35b, and CoRoT-36b
• On the LISA science performance in observations of short-lived signals from massive black hole binary coalescences
• Rapid parameter estimation of a two-component neutron star model with spin wandering using a Kalman filter
• A Method To Characterize the Wide-Angle Point Spread Function of Astronomical Images
• Kepler-90: Giant transit-timing variations reveal a super-puff
• Assessing and Mitigating the Impact of Glitches on Gravitational-Wave Parameter Estimation: a Model Agnostic Approach
• TOI-1268b: the youngest, hot, Saturn-mass transiting exoplanet
• Hints of spin-orbit resonances in the binary black hole population
• A proper motion catalogue for the Milky Way's nuclear stellar disc
• Pitfalls of periodograms: The non-stationarity bias in the analysis of quasi-periodic oscillations
• Does non-stationary noise in LIGO and Virgo affect the estimation of $H_0$?
• HOD-Dependent Systematics in Emission Line Galaxies for the DESI 2024 BAO analysis
• 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
• Stellar Populations in the Central 0.5 pc of Our Galaxy III: The Dynamical Sub-structures
• Systematic bias due to eccentricity in parameter estimation for merging binary neutron stars
• A general approach to maximise information density in neutron reflectometry analysis
• Transmission spectroscopy of WASP-52 b with JWST NIRISS: Water and helium atmospheric absorption, alongside prominent star-spot crossings
• A new method to measure the spectra of transiting exoplanet atmospheres using multi-object spectroscopy
• ACCESS: Confirmation of no potassium in the atmosphere of WASP-31b
• Rapid parameter estimation for an all-sky continuous gravitational wave search using conditional varitational auto-encoders
• Inferring the Intermediate Mass Black Hole Number Density from Gravitational Wave Lensing Statistics
• Time-domain phenomenological multipolar waveforms for aligned-spin binary black holes in elliptical orbits
• Computing Tools for Effective Field Theories
• alpha-Deep Probabilistic Inference (alpha-DPI): efficient uncertainty quantification from exoplanet astrometry to black hole feature extraction
• Multiple Peaks and a Long Precursor in the Type IIn Supernova 2021qqp: An Energetic Explosion in a Complex Circumstellar Environment
• Effect of Noise Estimation in Time-Domain Ringdown Analysis: A Case Study with GW150914
• Importance of Sample Selection in Exoplanet Atmosphere Population Studies
• Understanding binary neutron star collisions with hypermodels
• Cloud Parameterizations and their Effect on Retrievals of Exoplanet Reflection Spectroscopy
• General relativistic effects and the near-infrared and X-ray variability of Sgr A* I
• Using Equation of State Constraints to Classify Low-Mass Compact Binary Mergers
• Model systematics in time domain tests of binary black hole evolution
• Measuring angular N-point correlations of binary black hole merger gravitational-wave events with hierarchical Bayesian inference
• Bayesian estimate of the superfluid moments of inertia from the 2016 glitch in the Vela pulsar
• TESS discovery of a super-Earth and three sub-Neptunes hosted by the bright, Sun-like star HD 108236
• Precise mass determination for the keystone sub-Neptune planet transiting the mid-type M dwarf G 9-40
• Deciphering the unusual stellar progenitor of GRB 210704A
• GJ 3090 b: one of the most favourable mini-Neptune for atmospheric characterisation
• ESPRESSO observations of Gaia BH1: high-precision orbital constraints and no evidence for an inner binary
• TOI-1842b: A Transiting Warm Saturn Undergoing Re-Inflation around an Evolving Subgiant
• Where Outflows Meet Inflows: Gas Kinematics in SSA22 Lyman-$\alpha$ Blob 2 Decoded by Advanced Radiative Transfer Modelling
• The galaxy-halo connection of disc galaxies over six orders of magnitude in stellar mass
• Unveiling Microlensing Biases in Testing General Relativity with Gravitational Waves
• Characterizing Astrophysical Binary Neutron Stars with Gravitational Waves
• NGTS-14Ab: a Neptune-sized transiting planet in the desert
• Rotation and Abundances of the Benchmark Brown Dwarf HD 33632 Ab from Keck/KPIC High-resolution Spectroscopy
• Dark-ages Reionization and Galaxy Formation Simulation -- XIX: Predictions of infrared excess and cosmic star formation rate density from UV observations
• Eccentricity signatures in LIGO-Virgo-KAGRA's BNS and NSBH binaries
• The GAPS program at TNG XLVII: The unusual formation history of V1298 Tau
• Toward a better understanding of supernova environments: a study of SNe 2004dg and 2012P in NGC 5806 with HST and MUSE
• Compact Binary Coalescences in Dense Gaseous Environments Can Pose as ones in Vacuum
• Search for continuous gravitational waves from known pulsars in the first part of the fourth LIGO-Virgo-KAGRA observing run
• 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
• A Phantom Menace: On the Morphology of the Galactic Center Excess
• Efficient Reduced Order Quadrature Construction Algorithms for Fast Gravitational Wave Inference
• Probing hadron-quark phase transition in twin stars using $f$-modes
• Constraints on the Galactic Centre environment from \textit{Gaia} hypervelocity stars III: Insights on a possible companion to Sgr A*
• GW230529_181500: A Potential Primordial Binary Black Hole Merger in the Mass Gap
• eRASSt J074426.3+291606: prompt accretion disc formation in a 'faint and slow' tidal disruption event
• Signatures of inflowing gas in red geyser galaxies hosting radio-AGN
• Fresh view of the hot brown dwarf HD 984 B through high-resolution spectroscopy
• A microlensing search of 700 million VVV light curves
• Pulsar Timing Arrays require hierarchical models
• A Stimulating Explanation of the Extragalactic Radio Background
• Microlensing and the type Ia supernova iPTF16geu
• Three super-Earths and a possible water world from TESS and ESPRESSO
• Metallicity Distribution Function of the Eridanus~II Ultra-Faint Dwarf Galaxy from Hubble Space Telescope Narrow-band Imaging
• Full forward model of galaxy clustering statistics with AbacusSummit lightcones
• Modeling Radial Velocity Data of Resonant Planets to Infer Migration Histories
• Tidal Disruption Events through the Lens of the Cooling Envelope Model
• The fast transient AT 2023clx in the nearby LINER galaxy NGC 3799 as a tidal disruption of a very low-mass star
• 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
• The interplay of astrophysics and nuclear physics in determining the properties of neutron stars
• Hot-spots around Sagittarius A*: Joint fits to astrometry and polarimetry
• 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
• Impact of ringdown higher-order modes on black-hole mergers in dense environments: the scalar field case, detectability and parameter biases
• The Spin-Orbit Alignment of 8 Warm Gas Giant Systems
• A comprehensive revisit of select Galileo/NIMS observations of Europa
• 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
• Does the speed of gravitational waves depend on the source velocity?
• 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
• 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
• Spin Doctors: How to diagnose a hierarchical merger origin
• HOD-Dependent Systematics for Luminous Red Galaxies in the DESI 2024 BAO Analysis
• BOWIE-ALIGN: A JWST comparative survey of aligned vs misaligned hot Jupiters to test the dependence of atmospheric composition on migration history
• Hierarchical Bayesian Atmospheric Retrieval Modeling for Population Studies of Exoplanet Atmospheres: A Case Study on the Habitable Zone
• KilonovaNet: Surrogate Models of Kilonova Spectra with Conditional Variational Autoencoders
• High-energy spectra of LTT 1445A and GJ 486 reveal flares and activity
• Modelling high-resolution ALMA observations of strongly lensed dustystar forming galaxies detected by Herschel
• The effect of spin mismodeling on gravitational-wave measurements of the binary neutron star mass distribution
• Multimessenger astronomy with a kHz-band gravitational-wave observatory
• An eclipsing M-dwarf close to the hydrogen burning limit from NGTS
• Adding equatorial-asymmetric effects for spin-precessing binaries into the SEOBNRv5PHM waveform model
• Hot planets around cool stars -- two short-period mini-Neptunes transiting the late K-dwarf TOI-1260
• Targeted search for the stochastic gravitational-wave background from the galactic millisecond pulsar population
• 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
• Parametrized spin-precessing inspiral-merger-ringdown waveform model for tests of general relativity
• WASP-121b's transmission spectrum observed with JWST/NIRSpec G395H reveals thermal dissociation and SiO in the atmosphere
• Population-level Hypothesis Testing with Rocky Planet Emission Data: A Tentative Trend in the Brightness Temperatures of M-Earths
• Incorporation of model accuracy in gravitational wave Bayesian inference
• Breaking bad degeneracies with Love relations: Improving gravitational-wave measurements through universal relations
• First Comparative Exoplanetology Within a Transiting Multi-planet System: Comparing the atmospheres of V1298 Tau b and c
• Three low-mass companions around aged stars discovered by TESS
• A stochastic search for intermittent gravitational-wave backgrounds
• All-Sky Kinematics of the Distant Halo: The Reflex Response to the LMC
• A 2:1 Mean-Motion Resonance Super-Jovian pair revealed by TESS, FEROS, and HARPS
• PSR~J1910$-$5959A: A rare gravitational laboratory for testing white dwarf models
• Time-dependent visibility modelling of a relativistic jet in the X-ray binary MAXI J1803-298
• Dynamical modelling and origin of gas turbulence in z $\sim$ 4.5 galaxies
• Can we distinguish the adiabatic fluctuations and isocurvature fluctuations with pulsar timing arrays?
• NEID Reveals that The Young Warm Neptune TOI-2076 b Has a Low Obliquity
• SN 2021adxl: A luminous nearby interacting supernova in an extremely low metallicity environment
• A Glimpse of the Stellar Populations and Elemental Abundances of Gravitationally Lensed, Quiescent Galaxies at $z\gtrsim 1$ with Keck Deep Spectroscopy
• Gravitational-wave constraints on scalar-tensor gravity from a neutron star and black-hole binary GW200115
• Mean shift cluster recognition method implementation in the nested sampling algorithm
• Analysis of GWTC-3 with fully precessing numerical relativity surrogate models
• Pandora: A fast open-source exomoon transit detection algorithm
• VVV-WIT-08: the giant star that blinked
• Model-Independent Determination of $H_0$ and ${\Omega }_{K,0}$ using Time-Delay Galaxy Lenses and Gamma-Ray Bursts
• Noise analysis of the Indian Pulsar Timing Array data release I
• The astrophysical odds of GW151216
• 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
• Measuring quasi-normal mode amplitudes with misaligned binary black hole ringdowns
• Evidence of the pair instability gap from black hole masses
• Localization of binary neutron star mergers with a single Cosmic Explorer
• Linear vs. nonlinear modeling of black hole ringdowns
• Toward a complete description of $b\to u{\ell }^{-}\bar{\nu }$ decays within the Weak Effective Theory
• Feeding and feedback processes in the Spiderweb proto-intracluster medium
• Gravitational-wave parameter inference with the Newman-Penrose scalar ${\psi }_4$
• Light-Curve Structure and Halpha Line Formation in the Tidal Disruption Event AT 2019azh
• Bayesian modelling of scattered light in the LIGO interferometers
• The Cosmic Evolution of Fast Radio Bursts Inferred from the CHIME/FRB Baseband Catalog 1
• Photodynamical analysis of the nearly resonant planetary system WASP-148: Accurate transit-timing variations and mutual orbital inclination
• Dark lenses through the dust: parallax microlensing events in the VVV
• Footprints of population III stars in the gravitational-wave background
• Inferring physical properties of stellar collapse by third-generation gravitational-wave detectors
• Nested sampling with plateaus
• Two Planets Straddling the Habitable Zone of The Nearby K Dwarf Gl 414A
• ALMA resolves the first strongly-lensed Optical/NIR-dark galaxy
• GRB 220426A: A Thermal Radiation-Dominated Gamma-Ray Burst
• Determining the maximum information gain and optimising experimental design in neutron reflectometry using the Fisher information
• Overscreening and Underscreening in Solid-Electrolyte Grain Boundary Space-Charge Layers
• Mimicking Mergers: Mistaking Black Hole Captures as Mergers
• New constraints on the central mass contents of Omega Centauri from combined stellar kinematics and pulsar timing
• First eccentric inspiral-merger-ringdown analysis of neutron star-black hole mergers
• Possible binary neutron star merger history of the primary of GW230529
• Three Warm Jupiters around Solar-analog stars detected with TESS
• First Space-VLBI Observations of Sagittarius A*
• Tracing the formation and migration history: molecular signatures in the atmosphere of misaligned hot Jupiter WASP-94Ab using JWST NIRSpec/G395H
• Advice on describing Bayesian analysis of neutron and X-ray reflectometry
• An updated glitch rate law inferred from radio pulsars
• Transiting exoplanets with the Mid-InfraRed Instrument on board the James Webb Space Telescope: From simulations to observations
• The COSMOS-Web Lens Survey (COWLS) I: Discovery of >100 high redshift strong lenses in contiguous JWST imaging
• Prompt sky localization of compact binary sources using a meshfree approximation
• A dense mini-Neptune orbiting the bright young star HD 18599
• 2D k-th nearest neighbor statistics: a highly informative probe of galaxy clustering
• CLEAR: The Morphological Evolution of Galaxies in the Green Valley
• The nascent milliquasar VT J154843.06+220812.6: tidal disruption event or extreme accretion-state change?
• Uncovering dark matter density profiles in dwarf galaxies with graph neural networks
• The OATMEAL Survey. I. Low Stellar Obliquity in the Transiting Brown Dwarf System GPX-1
• A systematic validation of hot Neptunes in TESS data
• A Statistical Detection of Wide Binary Systems in the Ultra-Faint Dwarf Galaxy Reticulum II
• Inflow of low-metallicity cool gas in the halo of the Andromeda galaxy
• The Type Ibn Supernova 2019kbj -- Indications for Diversity in Type Ibn Supernova Progenitors
• A GPU-accelerated semi-coherent hierarchical search for stellar-mass binary inspiral signals in LISA
• Effect of double spin-precession and higher harmonics on spin-induced quadrupole moment measurements
• 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
• Rarity of precession and higher-order multipoles in gravitational waves from merging binary black holes
• Using gravitational waves to distinguish between neutron stars and black holes in compact binary mergers
• Distance to the Brick cloud using stellar kinematics
• Memory Effect or Cosmic String? Classifying Gravitational-Wave Bursts with Bayesian Inference
• 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
• Potential biases and prospects for the Hubble constant estimation via electromagnetic and gravitational-wave joint analyses
• 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
• Allesfitter: Flexible Star and Exoplanet Inference From Photometry and Radial Velocity
• Spectroscopy for asymmetric binary black hole mergers
• Isolated pulsar population synthesis with simulation-based inference
• Bayesian framework to infer the Hubble constant from the cross-correlation of individual gravitational wave events with galaxies
• Search for a gravitational wave background from primordial black hole binaries using data from the first three LIGO-Virgo-KAGRA observing runs
• Extending the Fisher Information Matrix in Gravitational-wave Data Analysis
• TESS and CHEOPS Discover Two Warm Sub-Neptunes Transiting the Bright K-dwarf HD 15906
• Uncovering the Invisible: A Study of Gaia18ajz, a Candidate Black Hole Revealed by Microlensing
• Post maximum light and late time optical imaging polarimetry of type I superluminous supernova 2020znr
• Gravitational-wave Observations Suggest Most Black Hole Mergers Form in Triples
• Compactness peaks: An astrophysical interpretation of the mass distribution of merging binary black holes
• A likely magnetic activity cycle for the exoplanet host M dwarf GJ 3512
• An Unexplained Origin for the Unusual Globular Cluster System in the Ultra-diffuse Galaxy FCC 224
• pop-cosmos: Scaleable inference of galaxy properties and redshifts with a data-driven population model
• Be careful in multi-messenger inference of the Hubble constant: A path forward for robust inference
• Detecting Planetary Oblateness in the Era of JWST: A Case Study of Kepler-167e
• Towards Studying Hierarchical Assembly in Real Time: A Milky Way Progenitor Galaxy at z = 2.36 under the Microscope
• The ultra narrow FRB20191107B, and the origins of FRB scattering
• CHEOPS and TESS view of the ultra-short period super-Earth TOI-561 b
• Do we need wavelets in the late Universe?
• Analysis of the ionized interstellar medium and orbital dynamics of PSR~J1909-3744 using scintillation arcs
• A 16 Hour Transit of Kepler-167 e Observed by the Ground-based Unistellar Telescope Network
• A comparison of Bayesian sampling algorithms for high-dimensional particle physics and cosmology applications
• Sky marginalization in black hole spectroscopy and tests of the area theorem
• The EBLM Project XII. An eccentric, long-period eclipsing binary with a companion near the hydrogen-burning limit
• JADES Ultra-red Flattened Objects: Morphologies and Spatial Gradients in Color and Stellar Populations
• Towards a complete picture of the Sco-Cen outflow
• Accounting for numerical-relativity calibration uncertainty in gravitational-wave modeling and inference
• JWST-TST DREAMS: Non-Uniform Dayside Emission for WASP-17b from MIRI/LRS
• Decoding Long-duration Gravitational Waves from Binary Neutron Stars with Machine Learning: Parameter Estimation and Equations of State
• Planetary companions orbiting the M dwarfs GJ 724 and GJ 3988. A CARMENES and IRD collaboration
• A hot Mars-sized exoplanet transiting an M dwarf
• Structure and Skewness of the Effective Inspiral Spin Distribution of Binary Black Hole Mergers
• 183 GHz water megamasers in active galactic nuclei: a new accretion disk tracer
• Rapid inference and comparison of gravitational-wave population models with neural variational posteriors
• Searching for candidates of coalescing binary black holes formed through chemically homogeneous evolution in GWTC-3
• 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
• The unusual M-dwarf Warm Jupiter TOI-1899~b: Refinement of orbital and planetary parameters
• Diving into the planetary system of Proxima with NIRPS -- Breaking the metre per second barrier in the infrared
• Bayesian fitting of multi-Gaussian expansion models to galaxy images
• GWDALI: A Fisher-matrix based software for gravitational wave parameter-estimation beyond Gaussian approximation
• TOI-1296b and TOI-1298b observed with TESS and SOPHIE: Two hot Saturn-mass exoplanets with different densities around metal-rich stars
• Possibility of primordial black holes as the source of gravitational wave events in the advanced LIGO detector
• NGTS 15b, 16b, 17b and 18b: four hot Jupiters from the Next Generation Transit Survey
• Search for lensing signatures in the gravitational-wave observations from the first half of LIGO-Virgo's third observing run
• Population properties of neutron stars in the coalescing compact binaries
• Hiding in plain sight: observing planet-starspot crossings with the James Webb Space Telescope
• Gravitational wave echoes search with combs
• Dynamical masses of two young transiting sub-Neptunes orbiting HD 63433
• Neural post-Einsteinian framework for efficient theory-agnostic tests of general relativity with gravitational waves
• A matched-filter approach to radio variability and transients: searching for orphan afterglows in the VAST Pilot Survey
• Unravelling the mass spectrum of destroyed dwarf galaxies with the metallicity distribution function
• Implications of GWTC-3 on primordial black holes from vacuum bubbles
• A fully precessing higher-mode surrogate model of effective-one-body waveforms
• An ESPRESSO view of HD 189733 system. Broadband transmission spectrum, differential rotation, and system architecture
• Search for Coincident Gravitational-wave and Fast Radio Burst Events from 4-OGC and the First CHIME/FRB Catalog
• Revisiting the HD 21749 Planetary System with Stellar Activity Modeling
• Cost of inferred nuclear parameters towards the f-mode dynamical tide in binary neutron stars
• Joint analysis of gravitational-wave and electromagnetic data of mergers: breaking an afterglow model degeneracy in GW170817 and in future events
• Quasinormal-modes of the Kerr-Newman black hole: GW150914 and fundamental physics implications
• Cold Deuterium Fractionation in the Nearest Planet-Forming Disk
• Robust inference of gravitational wave source parameters in the presence of noise transients using normalizing flows
• On the initial spin period distribution of neutron stars
• The CARMENES search for exoplanets around M dwarfs. Revisiting the GJ 581 multi-planetary system with new Doppler measurements from CARMENES, HARPS, and HIRES
• 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
• Phenomenological model of gravitational self-force enhanced tides in inspiralling binary neutron stars
• Realizing the potential of deep neural network for analyzing neutron star observables and dense matter equation of state
• 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
• 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 $z\sim 1$
• Prospects for measuring off-axis spins of binary black holes with Plus-era gravitational-wave detectors
• Do both black holes spin in merging binaries? Evidence from GWTC-4 and astrophysical implications
• 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?
• 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
• Dark energy reconstruction analysis with artificial neural networks: Application on simulated Supernova Ia data from Rubin Observatory
• Improved parametrized test of general relativity using the IMRPhenomX waveform family: Including higher harmonics and precession
• Characterization of the HD 108236 system with CHEOPS and TESS. Confirmation of a fifth transiting planet
• The First Spin-Orbit Obliquity of an M dwarf/brown dwarf System: An eccentric and aligned TOI-2119 b
• Discriminating among cosmological models by data-driven methods
• TOI-4504: Exceptionally large Transit Timing Variations induced by two resonant warm gas giants in a three planet system
• The Transit Timing and Atmosphere of Hot Jupiter HAT-P-37b
• White dwarf binary modulation can help stochastic gravitational wave background search
• TESS and HARPS reveal two sub-Neptunes around TOI 1062
• Can a binary neutron star merger in the vicinity of a supermassive black hole enable a detection of a post-merger gravitational wave signal?
• Missed opportunities: GRB 211211A and the case for continual gravitational-wave coverage with a single observatory
• Nuclear physics with gravitational waves from neutron stars disrupted by black holes
• Exploring the Gas-Phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
• Bayesian $\mathcal{F}$-statistic-based parameter estimation of continuous gravitational waves from known pulsars
• Three Warm Jupiters orbiting TOI-6628, TOI-3837, TOI-5027 and one sub-Saturn orbiting TOI-2328
• The steep redshift evolution of the hierarchical binary black hole merger rate may cause the $z$-${\chi }_{\mathrm{eff}}$ correlation
• BEBOP VII. SOPHIE discovery of BEBOP-3b, a circumbinary giant planet on an eccentric orbit
• BASS XLVII: 22 GHz Radio Atlas of Swift-BAT Selected AGN
• Secondary spins of extreme mass ratio inspirals: A probe to the formation channels
• GPU-accelerated LISA parameter estimation with full time domain response
• Reanalyzing the ringdown signal of GW150914 using the F-statistic method
• What is the nature of GW230529? An exploration of the gravitational lensing hypothesis
• 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
• No evidence for a dip in the binary black hole mass spectrum
• Constraints on Inflation with Null Energy Condition Violation from Advanced LIGO and Advanced Virgo's First Three Observing Runs
• Probing the Circumstellar Environment of highly luminous type IIn SN ASASSN-14il
• Numerical relativity surrogate models for exotic compact objects: the case of head-on mergers of equal-mass Proca stars
• GalaPy, the highly optimised C++/Python spectral modelling tool for galaxies -- I. Library presentation and photometric fitting
• Constraints on Non-Gaussian primordial curvature perturbation from the LIGO-Virgo-KAGRA third observing run
• A Stochastic Gravitational Wave Background in LISA from Unresolved White Dwarf Binaries in the Large Magellanic Cloud
• Very-High-Energy Gamma-Ray Afterglows of GRB 201015A and GRB 201216C
• Mapping the Skies of Ultracool Worlds: Detecting Storms and Spots with Extremely Large Telescopes
• Inferring the Astrophysical Population of Gravitational Wave Sources in the Presence of Noise Transients
• Tracking hidden magnetospheric fluctuations in accretion-powered pulsars with a Kalman filter
• Importance of eccentricities in parameter estimation of compact binary inspirals with decihertz gravitational-wave detectors
• Bayesian parameter estimation for targeted anisotropic gravitational-wave background
• Prospects of Gravitational Wave Follow-up Through a Wide-field Ultra-violet Satellite: a Dorado Case Study
• Uniform Modelling of the Stellar Density of Thirteen Tidal Streams within the Galactic Halo
• A Unified Spectroscopic and Photometric Model to Infer Surface Inhomogeneity: Application to Luhman 16B
• Search for Lorentz Invariance Violation using Bayesian model comparison applied to Xiao et al. GRB spectral lag catalog
• Detecting Baryon Acoustic Oscillations with third generation gravitational wave observatories
• Optimising experimental design in neutron reflectometry
• Two warm Earth-sized exoplanets and an Earth-sized candidate in the M5V-M6V binary system TOI-2267
• Double Trouble: Two spectroscopically confirmed low-mass quiescent galaxies at z>5 in overdensities
• Discovery of the variable optical counterpart of the redback pulsar PSR J2055+1545
• A Population Analysis of 20 Exoplanets Observed from the Optical to the Near-infrared Wavelengths with HST: Evidence for Widespread Stellar Contamination
• Massive stars exploding in a He-rich circumstellar medium. XI. Diverse evolution of five Ibn SNe 2020nxt, 2020taz, 2021bbv, 2023utc and 2024aej
• Brackett-$\gamma$ as a Gold-standard Test of Star Formation Rates Derived from SED Fitting
• Gravitational wave ringdown analysis using the $\mathcal{F}$-statistic
• Impact of higher harmonics of gravitational radiation on the population inference of binary black holes
• Comparison of Step Samplers for Nested Sampling
• 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
• Pinpointing coalescing binary neutron star sources with the IGWN, including LIGO-Aundha
• Deep Learning and genetic algorithms for cosmological Bayesian inference speed-up
• The proper motion of stars in dwarf galaxies: distinguishing central density cusps from cores
• Waveform systematics in identifying strongly gravitationally lensed gravitational waves: Posterior overlap method
• SN 2022joj: A Peculiar Type Ia Supernova Possibly Driven by an Asymmetric Helium-shell Double Detonation
• Unveiling a 36 Billion Solar Mass Black Hole at the Centre of the Cosmic Horseshoe Gravitational Lens
• Characterizing the 3D Kinematics of Young Stars in the Radcliffe Wave
• 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
• Measuring Star Formation Histories, Distances, and Metallicities with Pixel Color-Magnitude Diagrams II: Applications to Nearby Elliptical Galaxies
• Testing the Cosmological Principle: On the Time Dilation of Distant Sources
• Ensemble noise properties of the European Pulsar Timing Array
• The Frequency and Mass-Ratio Distribution of Binaries in Clusters I: Description of the method and application to M67
• Detecting Low-Mass Perturbers in Cluster Lenses using Curved Arc Bases
• $\mu$-GLANCE: A Novel Technique to Detect Chromatically and Achromatically Lensed Gravitational Wave Signals
• High-precision source characterization of intermediate mass-ratio black hole coalescences with gravitational waves: The importance of higher-order multipoles
• 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
• PDS 70b Shows Stellar-like Carbon-to-oxygen Ratio
• TOI-5108 b and TOI 5786 b: Two transiting sub-Saturns detected and characterized with TESS, MaHPS and SOPHIE
• The Radius of PSR J0437-4715 from NICER Data
• Flow Matching for Atmospheric Retrieval of Exoplanets: Where Reliability meets Adaptive Noise Levels
• Diversity in the haziness and chemistry of temperate sub-Neptunes
• Comparison between time-domain and frequency-domain Bayesian inferences to inspiral-merger-ringdown gravitational-wave signals
• The Orbit and Companion of PSR J1622-0315: Variable Asymmetry and a Massive Neutron Star
• Simulation-based inference of galaxy properties from JWST pixels
• Differential Interferometric Signatures of Close Binaries of Supermassive Black Holes in Active Galactic Nuclei: II. Merged Broad Line Regions
• Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object
• Confronting general relativity with principal component analysis: Simulations and results from GWTC-3 events
• HD 183579b: A Warm Sub-Neptune Transiting a Solar Twin Detected by TESS
• Discovery of a radio jet in the Cloverleaf Quasar at z = 2.56
• Who Ordered That? Unequal-Mass Binary Black Hole Mergers Have Larger Effective Spins
• Signatures of a subpopulation of hierarchical mergers in the GWTC-4 gravitational-wave dataset
• Analysis of the public HARPS/ESO spectroscopic archive -- Jupiter-like planets around HD 103891 and HD 105779
• Bayesian Analysis of the ${}^{70}$Zn$(d{,}^3\text{He}{)}^{69}$Cu Transfer Reaction
• 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
• Spectroscopic AGN survey at $z$ $\sim$ 2 with NTT/SOFI for GRAVITY+ observations
• An extremely low-density exoplanet spins slow
• Black Hole Gravitational Potential Enhanced Fallback Accretion onto the Nascent Lighter Compact Object: Tentative Evidence in the O3 Run Data of LIGO/Virgo
• Effective chirp mass captures the inspiral frequency evolution of the non-spinning eccentric compact binary
• RUBIES spectroscopically confirms the high number density of quiescent galaxies from $2<\mathbf{z}<5$
• The Origin of the Cluster of Local Interstellar Clouds
• Detecting a Gravitational-Wave Background from Inflation with Null Energy Condition Violation: Prospects for Taiji
• A Gap in the Densities of Small Planets Orbiting M Dwarfs: Rigorous Statistical Confirmation Using the Open-source Code RhoPop
• Bounds on the charge of the graviton using gravitational wave observations
• Efficient Bayesian inference and model selection for continuous gravitational waves in pulsar timing array data
• SN 2020zbf: A fast-rising hydrogen-poor superluminous supernova with strong carbon lines
• Bayesian Model Selection of Lithium-Ion Battery Models via Bayesian Quadrature
• Non-Kerr Constraints using Binary Black Hole inspirals considering phase modifications up to 4 PN order
• Anomalously low-mass core-He-burning star in NGC 6819 as a post-common-envelope phase product
• Search for stochastic gravitational-wave background from string cosmology with Advanced LIGO and Virgo's O1$\sim$O3 data
• Constraints on peculiar velocity distribution of binary black holes using gravitational waves with GWTC-3
• Exploiting the transit timing capabilities of Ariel
• LitePIG: A Lite Parameter Inference system for the Gravitational wave in the millihertz band
• The TESS-Keck Survey. XIII. An Eccentric Hot Neptune with a Similar-Mass Outer Companion around TOI-1272
• Accelerating Tests of General Relativity with Gravitational-Wave Signals using Hybrid Sampling
• Distinguishing binary black hole precessional morphologies with gravitational wave observations
• Modelling Einstein cluster using Einasto profile
• Retrieving Exoplanet Atmospheres using Planetary Infrared Excess: Prospects for the Nightside of WASP-43 b and other Hot Jupiters
• Methodology for constraining ultralight vector bosons with gravitational wave searches targeting merger remnant black holes
• TIC~257060897b: an inflated, low-density, hot-Jupiter transiting a rapidly evolving subgiant star
• Modified gravitational wave propagations in linearized gravity with Lorentz and diffeomorphism violations and their gravitational wave constraints
• Searching for orbital decay in a heartbeat star system KIC 3766353
• 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
• GEMS JWST: Transmission spectroscopy of TOI-5205b reveals significant stellar contamination and a metal-poor atmosphere
• New Constraints on Sodium Production in Globular Clusters From the ${}^{23}$Na${(}^3$He$,\text{d}{)}^{24}$Mg Reaction
• Mapping the Distant and Metal-Poor Milky Way with SDSS-V
• Atmospheric abundances and bulk properties of the binary brown dwarf Gliese 229 Bab from JWST/MIRI spectroscopy
• Hierarchical triple mergers: testing Hawking's area theorem with the inspiral signals
• The CARMENES search for exoplanets around M dwarfs. A sub-Neptunian mass planet in the habitable zone of HN Lib
• Constraints on Bianchi-I type universe with SH0ES anchored Pantheon+ SNIa data
• Catalog variance of testing general relativity with gravitational-wave data
• Spatially Resolved Circumgalactic Medium around a Star-Forming Galaxy Driving a Galactic Outflow at $z\approx 0.8$
• Modeling matter(s) in SEOBNRv5THM: Generating fast and accurate effective-one-body waveforms for spin-aligned binary neutron stars
• Probing the Spin-Induced Quadrupole Moment of Massive Black Holes with the Inspiral of Binary Black Holes
• Which is which? Identification of the two compact objects in gravitational-wave binaries
• NGTS-21b: An Inflated Super-Jupiter Orbiting a Metal-poor K dwarf
• Resolved Gas Temperatures and 12C/13C ratios in SVS13A from ALMA Observations of CH3CN and CH3-13-CN
• A Detection of Red Noise in PSR J1824$-$2452A and Projections for PSR B1937+21 using NICER X-ray Timing Data
• The JWST EXCELS Survey: gas-phase metallicity evolution at 2 < z < 8
• Bayesian Search of Massive Scalar Fields from LIGO-Virgo-KAGRA Binaries
• Observability of spin precession in the presence of a black-hole remnant kick
• Probing intractable beyond-standard-model parameter spaces armed with Machine Learning
• Validating Sequential Monte Carlo for Gravitational-Wave Inference
• Searching for double-peak and doubly broken gravitational-wave spectra from Advanced LIGO-Virgo's first three observing runs
• Biased parameter inference of eccentric, spin-precessing binary black holes
• Two neighbours of the ultra-short-period Earth-sized planet K2-157 b in the warm Neptunian savanna
• The magnetic field of the Radcliffe Wave: starlight polarization at nearest approach to the Sun
• Evidence for evolving dark energy from DESI DR2 BAO and Pantheon${}^{+}$, DES-Dovekie, and Union3
• Simulation-based Inference for Gravitational-waves from Intermediate-Mass Binary Black Holes in Real Noise
• 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
• SN 2019odp: A Massive Oxygen-Rich Type Ib Supernova
• 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
• Assessing the systematic errors of extreme-mass-ratio inspirals waveforms for testing general relativity
• PACMAN: A pipeline to reduce and analyze Hubble Wide Field Camera 3 IR Grism data
• RadioSED I: Bayesian inference of radio SEDs from inhomogeneous surveys
• Radiative Transfer and Inversion codes for characterizing planetary atmospheres: an overview
• Nested Sampling for Non-Gaussian Inference in SLAM Factor Graphs
• The impact of waveform systematics and Gaussian noise on the interpretation of GW231123
• Beyond GWTC-3: Analysing and verifying new gravitational-wave events from community catalogues
• Fast and faithful interpolation of numerical relativity surrogate waveforms using meshfree approximation
• The Way of Water: ALMA resolves H2O emission lines in a strongly lensed dusty star-forming galaxy at z $\sim$ 3.1
• A complete measurement of a black-hole recoil through higher-order gravitational-wave modes
• Model-independent search for the quasinormal modes of gravitational wave echoes
• Impact of Bayesian Priors on the Inferred Masses of Quasi-Circular Intermediate-Mass Black Hole Binaries
• 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
• 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
• Detecting episodes of star formation using Bayesian model selection
• Where has all the $r$-process gone? Timescales for GRB-Kilonovae to Enrich their Host Galaxies
• Quasi-Periodic Peak Energy Oscillations in X-ray Bursts from SGR J1935+2154
• Accelerating Bayesian Sampling for Massive Black Hole Binaries with Prior Constraints from Conditional Variational Autoencoder
• 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
• Testing Ghasemi-Nodehi-Bambi metric parameters with quasi-periodic oscillations
• SN 2019hcc: A Type II Supernova Displaying Early O II Lines
• 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
• Search for Coincident Gravitational Wave and Long Gamma-Ray Bursts from 4-OGC and the Fermi-GBM/Swift-BAT Catalog
• Waging a Campaign: Results from an Injection-Recovery Study involving 35 numerical Relativity Simulations and three Waveform Models
• Modeling Star Formation Histories of Changing-Look AGN Host Galaxies with Prospector
• The Similar Seven: A set of very-alike exoplanets to test correlations between system parameters and atmospheric properties
• A Transiting Giant on a 7.7-Year Orbit Revealed by TTVs in the TOI-201 System
• GausSN: Bayesian Time-Delay Estimation for Strongly Lensed Supernovae
• 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
• Asteroseismology with PBjam 2.0: measuring dipole mode frequencies in coupling regimes from main sequence to low-luminosity red giant stars
• GravSphere2: A higher-order Jeans method for mass-modeling spherical stellar systems
• 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
• Comparing measures of the Hubble and BAO tensions in $\Lambda$CDM and possible solutions in $f(Q)$ gravity
• The Performance of Photometric Reverberation Mapping at High Redshift and the Reliability of Damped Random Walk Models
• A follow-up on intermediate-mass black hole candidates in the second LIGO-Virgo observing run with the Bayes Coherence Ratio
• Detectability of Gravitational-Wave Memory with LISA: A Bayesian Approach
• Marginalised Gaussian Processes with Nested Sampling
• NLTE atmospheric modelling of the ultra-hot Jupiter WASP-178b and comparison with UV and optical observations
• Probing General Relativity in galactic scales at z $\sim 0.3$
• Inferring spin tilts of binary black holes at formation with plus-era gravitational wave detectors
• The changing transit shape of TOI-3884 b
• Kinematic scaling relations of disc galaxies from ionised gas at $z\sim 1$ and their connection with dark matter haloes
• Informed total-error-minimizing priors: Interpretable cosmological parameter constraints despite complex nuisance effects
• Accelerated inference of binary black-hole populations from the stochastic gravitational-wave background
• A homogeneous TTV investigation of all TESS systems with a confirmed single transiting planet
• Scalar fields around black hole binaries in LIGO-Virgo-KAGRA
• Accurate and efficient photo-eccentric transit modeling
• Optimized localization for gravitational-waves from merging binaries
• Unveiling the nature of HE 0107-5240
• The ORT and the uGMRT Pulsar Monitoring Program : Pulsar Timing Irregularities & the Gaussian Process Realization
• Simplifying asteroseismic analysis of solar-like oscillators: An application of principal component analysis for dimensionality reduction
• Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. VI: Confirmation of a Long-Period Giant Planet Discovered with a Single TESS Transit
• Measuring the magnetic dipole moment and magnetospheric fluctuations of accretion-powered pulsars in the Small Magellanic Cloud with an unscented Kalman filter
• TOI-3288 b and TOI-4666 b: two gas giants transiting low-mass stars characterised by NIRPS
• When Dark Matter Heats Up: A Model-Independent Search for Non-Cold Behavior
• Active Galactic Nuclei in the Green Valley at z$\sim$0.7
• Vacuum birefringence and the polarized X-ray emission from a radio magnetar
• Angular power spectrum of gravitational-wave transient sources as a probe of the large-scale structure
• A Machine Learning Approach to Integral Field Unit Spectroscopy Observations: III. Disentangling Multiple Components in Hii regions
• Cosmology on a Gravitational Wave Background
• A New Brown Dwarf Orbiting an M star and An Investigation on the Eccentricity Distribution of Transiting Long-Period Brown Dwarfs
• Observing Rayleigh-Taylor stable and unstable accretion through a Kalman filter analysis of X-ray pulsars in the Small Magellanic Cloud
• A massive quiescent galaxy confirmed in a protocluster at z=3.09
• Luminous, rapidly declining supernovae as stripped transitional objects in low metallicity environments: the case of SN 2022lxg
• Exploring the Evolution of Nonlinear Electrodynamics in the Universe: A Dynamical Systems Approach
• Unveiling the existence of nontensorial gravitational-wave polarizations from individual supermassive black hole binaries with pulsar timing arrays
• Modeling Strong Lenses from Wide-Field Ground-Based Observations in KiDS and GAMA
• GRB 201104A: A "Repetitive" Short Gamma-Ray Burst?
• Pixel-level modelling of group-scale strong lens CASSOWARY 19
• Population synthesis and parameter estimation of neutron stars with continuous gravitational waves and third-generation detectors
• Probing black hole `charge' from the binary black hole inspiral
• eROSITA-RU Tidal Disruption Events with Keck-I/LRIS: Sample Selection, Optical Properties, and Host Galaxy Demographics
• Verification of the Black Hole Area Law with GW230814
• Distinct Rotational Evolution of Giant Planets and Brown Dwarf Companions
• Determination of Hubble constant from Megamaser Cosmology Project using Profile Likelihood
• Anomalies in Hadronic $B$ Decays: an Update
• Evidence for an Atmosphere on the Ultra-Short Period super-Earth HD 3167 b
• 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
• CMB constraints on monodromy inflation at strong coupling
• TESS and HARPS-N unveil two planets transiting TOI-1453. A super-Earth and one of the lowest mass sub-Neptunes
• Modern Bayesian Sampling Methods for Cosmological Inference: A Comparative Study
• Probing Spin-Orbit Resonances with the Binary Black Hole Population
• Leveraging cross-detector parameter consistency measures to enhance sensitivities of gravitational wave searches
• Gravitational waves from eccentric binary neutron star mergers: Systematic biases and inadequacy of quasicircular templates
• 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
• Robust parameter estimation from pulsar timing data
• Accounting for the Known Unknowns: A Parametric Framework to Incorporate Systematic Waveform Errors in Gravitational-Wave Parameter Estimation
• 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?
• Robust and fast parameter estimation for gravitational waves from binary neutron star merger remnants
• Equivalence of Dark Energy Models: A Theoretical and Bayesian Perspective
• A joint effort to discover and characterize two resonant mini Neptunes around TOI-1803 with TESS, HARPS-N and CHEOPS
• A Moderate Albedo from Reflecting Aerosols on the Dayside of WASP-80 b Revealed by JWST/NIRISS Eclipse Spectroscopy
• Separated twins or just siblings? A multi-planet system around an M dwarf including a cool sub-Neptune
• Along the Primary Curve: Simultaneous Source and Lens Reconstruction of Bright Arcs in Cluster Lenses
• Robust, Rapid, and Simple Gravitational-wave Parameter Estimation
• Validation of TOI-1221 b: A warm sub-Neptune exhibiting TTVs around a Sun-like star
• Probing populations of dark stellar remnants in the globular clusters 47 Tuc and Terzan 5 using pulsar timing
• Gravitational lensing aided luminosity distance estimation for compact binary coalescences
• Direct Inference of Nuclear Equation-of-State Parameters from Gravitational-Wave Observations
• Probing Cosmology with Baryon Acoustic Oscillations using Gravitational Waves
• Characterization of low-mass companions to $\text{Kepler}$ objects of interest observed with APOGEE-N
• Effects of calibration uncertainties on the detection and parameter estimation of isotropic gravitational-wave backgrounds
• Impact on $L$-observables of a new combined analysis of $B_{d,s}\to K^{(\ast )}$ form factors
• Study of pulsar flux density and its variability with Parkes data archive
• Are all models wrong? Falsifying binary formation models in gravitational-wave astronomy
• Gravitational-wave model for neutron star merger remnants with supervised learning
• 28 Years of Sun-as-a-star Extreme Ultraviolet Light Curves from SOHO EIT
• Testing modified gravity with the eccentric neutron star--black hole merger GW200105
• A sub-Neptune transiting the young field star HD 18599 at 40 pc
• Constraining the modified friction in gravitational wave propagation with precessing black hole binaries
• Discovery of Volatile Gas in the Giant Impact Disk around the 150-Myr old HD 23514
• Constraining the Stellar Masses and Origin of the Protostellar VLA 1623 System
• Beyond LambdaCDM: How the Hubble tension challenges early universe physics
• TOI-2322: two transiting rocky planets close to the stellar rotation period and its first harmonic
• Inferring the spins of merging black holes in the presence of data-quality issues
• BD-14 3065b (TOI-4987b): from giant planet to brown dwarf: evidence for deuterium burning in old age?
• Bayesian WIMP detection with the Cherenkov Telescope Array
• Confronting primordial black holes with LIGO-Virgo-KAGRA and the Einstein Telescope
• GW231123: Overlapping Gravitational Wave Signals?
• MANGOS II: Five new giant planets orbiting low-mass stars
• Testing black hole space-times with the S2 star orbit: a Bayesian comparison
• Parameter estimation of binary black holes in the endpoint of the up-down instability
• Probing magneto-ionic microstructure towards the Vela pulsar using a prototype SKA-Low station
• HD 143811 AB b: A Directly Imaged Planet Orbiting a Spectroscopic Binary in Sco-Cen
• Sensitivity to Sub-Io-sized Exosatellite Transits in the MIRI LRS Lightcurve of the Nearest Substellar Worlds
• Dynamical Architectures of S-type Transiting Planets in Binaries II: A Dichotomy in Orbital Alignment of Small Planets in Close Binary Systems
• Evidence for a Nonzero Eccentricity Superpuff Exoplanet WASP-107 b Using JWST Occultation Observation
• Mapping atmospheric features of the planetary-mass brown dwarf SIMP 0136 with JWST NIRISS
• Precise radial velocities of giant stars -- XVII. Distinguishing planets from intrinsically induced radial velocity signals in evolved stars
• Evidence for Three Subpopulations of Merging Binary Black Holes at Different Primary Masses
• Planet Hunters NGTS: New Planet Candidates from a Citizen Science Search of the Next Generation Transit Survey Public Data
• 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
• ${\tau }^9$ Eri: A bright pulsating magnetic Bp star in a 5.95-day double-lined spectroscopic binary
• 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
• 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
• 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
• Testing general relativity with amplitudes of subdominant gravitational-wave modes
• The Indian Pulsar Timing Array Data Release 2: II. Customised Single-Pulsar Noise Analysis and Noise Budget
• Mapping the cosmic expansion history from LIGO-Virgo-KAGRA in synergy with DESI and SPHEREx
• NF-iSAM: Incremental Smoothing and Mapping via Normalizing Flows
• Discovery of Galactic center ejected star in DESI DR1
• Meet the Neighbors: Gas Rich "Buddy Galaxies" are Common Around Recently Quenched Massive Galaxies in the SQuIGG$\vec{L}$E Survey
• 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
• Confronting compositional confusion through the characterisation of the sub-Neptune orbiting HD 77946
• A long-duration gamma-ray burst of dynamical origin from the nucleus of an ancient galaxy
• Measurability of neutron star tidal deformability from merging neutron star-black hole binaries
• AGN in the ULIRG HE 0435-5304
• Searching for a Galactic component in the IceCube track-like neutrino events
• A Bayesian Inference Framework for Gamma-Ray Burst Afterglow Properties
• Arbitrary Marginal Neural Ratio Estimation for Simulation-based Inference
• 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)
• 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
• Granulation signatures as seen by Kepler short-cadence data. I. A decoupling between granulation and oscillation timescales for dwarfs
• 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
• Systematics in ETG Mass Profile Modelling: Strong Lensing & Stellar Dynamics
• 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
• A Bayesian approach to time-domain Photonic Doppler Velocimetry
• Fermi-GBM Observations of GRB 210812A: Signatures of a Million Solar Mass Gravitational Lens
• Three Hot Jupiters transiting K-dwarfs with a significant heavy element mass
• A distant brown dwarf coplanar to a warm Jupiter and a hot super-Earth
• Deep follow-up for gravitational-wave inference: a case study with GW151226
• An independent search for Jovian neutrinos using BOREXINO data
• Search for giant planets in M67 V: a warm Jupiter orbiting the turn-off star S1429
• Bayesian Analysis of the ${}^{86}$Sr$(\alpha ,\alpha )$ Reaction to Constrain the ${}^{86}$Sr$(\alpha ,n)$ Cross Section at Astrophysical Energies
• Atmospheric asymmetries in WASP-121 b revealed by rotational transits detected with JWST
• 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
• The Hubble PanCET Program: A Featureless Transmission Spectrum for WASP-29b and Evidence of Enhanced Atmospheric Metallicity on WASP-80b
• Constraints on gravitational waves from the 2024 Vela pulsar glitch
• NGTS-EB-8: A double-lined eclipsing M+M binary discovered by citizen scientists
• Measuring Hubble Constant with Dark Neutron Star-Black Hole Mergers
• Reducing systematic uncertainties in gravitational-wave population analyses by increasing the detection threshold
• Accelerating gravitational-wave parameterized tests of General Relativity using a multiband decomposition of likelihood
• Simulations of astrometric planet detection in Alpha Centauri by intensity interferometry
• Gas-depleted planet formation occurred in the four-planet system around the red dwarf LHS 1903
• Inferring Evidence from Nested Sampling Data via Information Field Theory
• Discovery of a Barred-Spiral Galaxy at $z_{spec}$ = 3.16 II. The Star Formation History
• Illuminating the Mass Gap Through Deep Optical Constraint on a Neutron Star Merger Candidate S250206dm
• Beetroots: spatially-regularized Bayesian inference of physical parameter maps -- Application to Orion
• Characterizing the host galaxies and delay times of Ca-rich gap transients vs 91bg-like SNe and normal Type Ia SNe
• Evidence of large recoil velocity from a black hole merger signal
• Reverse-time analysis uncovers universality classes in directional biological dynamics
• Dynamical masses of young stellar objects with the VLBA: DYNAMO-VLBA: Radio binary stars in Orion
• Significant challenges for astrophysical inference with next-generation gravitational-wave observatories
• Characterizing CO Emitters in the SSA22-AzTEC26 Field
• The dark and featureless surface of rocky exoplanet LHS 3844 b from JWST mid-infrared spectroscopy
• The asymmetric structure of the inner disc around HD 142527 A with VLTI/MATISSE
• Closing the Evidence Gap: reddemcee, a Fast Adaptive Parallel Tempering Sampler
• Photometric Constraints on Intermediate-mass Black Holes in the Galactic Centre
• Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
• A new third planet and the dynamical architecture of the HD33142 planetary system
• Using Strong Lensing to Detect Subhalos with Steep Inner Density Profiles
• A gating-and-inpainting perspective on GW150914 ringdown overtone: understanding the data analysis systematics
• Measurement prospects for the pair-instability mass cutoff with gravitational waves
• The DESI DR1 Peculiar Velocity Survey: global zero-point and $H_0$ constraints
• Decameter-sized Earth Impactors -- II: A Bayesian Inference Approach to Meteoroid Ablation Modeling
• Statistical biases in parametrized searches for gravitational-wave polarizations
• TESS phase curve of ultra-hot Jupiter WASP-189 b
• Observational bounds on Dark Matter Admixed Neutron Stars from Gravitational Wave Data
• Time delay measurements with Broken Power Law model
• Bayesian Framework to Follow-up Continuous Gravitational Wave Candidates from Deep Surveys
• Challenging a binary neutron star merger interpretation of GW230529
• Can Big Black Holes Merge with the Smallest Black Holes?
• Neural Post-Einsteinian Test of General Relativity with the Third Gravitational-Wave Transient Catalog
• Methane on the temperate exo-Saturn TOI-199b
• An Archival Optical Counterpart Search for Extragalactic Fast X-Ray Transients Discovered by Einstein Probe
• The impact of precession and higher-order multipoles for gravitational wave cosmological inference
• Discovery of a transiting hot water-world candidate orbiting Ross 176 with TESS and CARMENES
• Galaxy-galaxy strong lens perturbations: line-of-sight haloes versus lens subhaloes
• Using overlap of sky localization probability maps for filtering potentially lensed pairs of gravitational-wave signals
• APES: Approximate Posterior Ensemble Sampler
• SQuIGGLE: Studying Quenching in Intermediate-z Galaxies -- Gas, AnguLar Momentum, and Evolution
• Lightweight posterior construction for gravitational-wave catalogs with the Kolmogorov-Arnold network
• Constraining the selection corrected luminosity function and total pulse count for radio transients
• XMM-Newton follow-up of two eROSITA X-ray binary candidates
• Investigating the extent of bladed terrain on Pluto via photometric surface roughness
• Towards a Field Based Bayesian Evidence Inference from Nested Sampling Data
• Probing missing physics from inspiralling compact binaries via time-frequency tracks
• How Holographic is the Dark Energy? A Spline Nodal reconstruction approach
• 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
• Prospects for distinguishing dynamical tides in inspiralling binary neutron stars with third generation gravitational-wave detectors
• Probing the peak of star formation with the stochastic background of binary black hole mergers
• Waveform model for the $(\ell =2,m=0)$ spherical harmonic and the displacement memory contribution from precessing binary black holes
• Optimizing Gaussian Process Kernels Using Nested Sampling and ABC Rejection for H(z) Reconstruction
• A VLA View of the Flared, Asymmetric Disk Around the Class 0 Protostar L1527 IRS
• MatBYIB: A Matlab-based code for Bayesian inference of extreme mass-ratio inspiral binary with arbitrary eccentricity
• Characterization of merging black holes with two precessing spins
• A new method to correct for host star variability in multi-epoch observations of exoplanet transmission spectra
• Assessment of normalizing flows for parameter estimation on time-frequency representations of gravitational-wave data
• Which black hole formed first? Mass-ratio reversal in massive binary stars from gravitational-wave data
• The maximum mass and rotational kinetic energy of rapidly rotating neutron stars
• A Radio-selected Population of Dark, Long Gamma-ray Bursts: Comparison to the Long Gamma-ray Burst Population and Implications for Host Dust Distributions
• Oxyster: A Circumgalactic Low-ionization Oxygen Nebula next to a Starburst Galaxy at $z\sim 1$
• Constraining Scalar Charge in Neutron Stars through Gravitational Wave Signals from NSBH Mergers
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• Impact of Variable Photospheric Radius on Exoplanet Atmospheric Retrievals
• Two Rings and a Marginally Resolved, 5 AU, Disk Around LkCa 15 Identified Via Near Infrared Sparse Aperture Masking Interferometry
• Revisiting the secondary eclipses of KELT-1b using TESS observations
• Constraints on AvERA Cosmologies from Cosmic Chronometers and Type Ia Supernovae
• Cosmology with Love: Measuring the Hubble constant using neutron star universal relations
• Probing Dark Matter with Strong Gravitational Lensing through an Effective Density Slope
• Detection of the stochastic gravitational wave background with the space-borne gravitational-wave detector network
• Can Eccentric Binary Black Hole Signals Mimic Gravitational-Wave Microlensing?
• Model-agnostic search of gravitational wave echoes in LVK data
• How narrow is the M87* ring? I. The choice of closure likelihood function
• Search for Annual Modulation in Combined ANAIS 112 and COSINE 100 Data using Bayesian Model Comparison
• ExoEcho: Exoplanet Ephemerides Change Observations. III. A JWST Survey for Transit Timing Variations of 37 Exoplanets
• Systematic bias due to eccentricity in parameter estimation for merging binary neutron stars : Spinning case
• 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
• Low-efficiency long gamma-ray bursts: A case study with AT2020blt
• 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
• Mapping the 3D Kinematical Structure of the Gas Disk of HD 169142
• Characterizing Binary Black Hole Subpopulations in GWTC-4 with Binned Gaussian Processes: On the Origins of the $35M_{\odot }$ Peak
• Plunge-Merger-Ringdown Tests of General Relativity with GW250114
• Hidden Gems in TESS: sherlock finds two new rocky planets around nearby M dwarfs
• Uncovering subdominant multipole asymmetries in binary black-hole mergers
• Toward a Unified Understanding of the Dense Matter Equation of State
• TRIShUL: Technique for Reconstructing magnetic Interstellar Structure Using starLight polarization
• TOI-1201 b: A mini-Neptune transiting a bright and moderately young M dwarf
• Parameter estimation for space-based gravitational wave detectors with ringdown signals
• Identifying Host Galaxies of Binary Black Hole Mergers with Next-Generation Gravitational Wave Detector Networks
• 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
• A restless supermassive black hole in the galaxy J0437+2456
• 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
• Improved Constraints on Non-Kerr Deviations from Binary Black Hole Inspirals Using GWTC-4 Data
• The Missing Multipole Problem: Investigating biases from model starting frequency in gravitational-wave analyses
• Gravitational-wave astronomy requires population-informed parameter estimation
• No model-independent evidence for a peak in binary black hole spin (mis)alignments
• 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
• 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
• 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
• Modifying $\Lambda$CDM dynamics via out-of-equilibrium axions: reconciling SH0ES and DESI $H_0$ values
• 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
• 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
• 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
• TOI-333b: A Neptune Desert planet around a F7V star
• Measuring the crust-superfluid coupling time-scale for 105 UTMOST pulsars with a Kalman filter
• Confirmation of SRGt 062340.2-265751 as a nova-like cataclysmic variable with a possible magnetic nature
• Probing the disk-jet coupling in M87
• Prospects for Measuring Black Hole Masses using TDEs with the Vera C. Rubin Observatory
• Constraining the gravitational-wave emission of core-collapse supernovae with ground-based detectors
• The MWA Long Baseline Epoch of Reionisation Survey: I. Improved Source Catalogue for the EoR 0 field
• Simulation-calibrated Bayesian inference for progenitor properties of the microquasar SS 433
• Black-box density function estimation using recursive partitioning
• The Progenitor Systems of Classical Novae in M31
• Applicability of multi-component study on Bayesian searches for targeted anisotropic stochastic gravitational-wave background
• Bayesian vs Frequentist: Comparing Bayesian model selection with a frequentist approach using the iterative smoothing method
• The Nearby Evolved Stars Survey II: Constructing a volume-limited sample and first results from the James Clerk Maxwell Telescope
• Hybrid waveforms for precessing quasi-circular binary systems
• A Pearl in the Shell: an ultra-compact dwarf within the tidal debris surrounding spiral galaxy NGC 7531
• Applying higher-modes consistency test on GW190814 : lessons on no-hair theorem, nature of the secondary compact object and waveform modeling
• False Alarm Rate based Statistical Detection Limit for Astronomical Photon Detectors
• Circular Mystery: Exploring Diffuse Emission Surrounding a Radio Galaxy with uGMRT and VLA Multiwavelength Observations
• Probing the partition function for temperature-dependent potentials with nested sampling
• Sibling Sub-Neptunes Around Sibling M Dwarfs: TOI-521 and TOI-912
• Improved characterization of the TOI-2141 system: a dense sub-Neptune with non-transiting inner and outer companions
• High-frequency continuous gravitational waves searched in LIGO O3 public data with Einstein@Home
• Persistence of post-Newtonian amplitude structure in binary black hole mergers