Array Programming with NumPy

Abstract

Array programming provides a powerful, compact, expressive syntax for accessing, manipulating, and operating on data in vectors, matrices, and higher-dimensional arrays. NumPy is the primary array programming library for the Python language. It plays an essential role in research analysis pipelines in fields as diverse as physics, chemistry, astronomy, geoscience, biology, psychology, material science, engineering, finance, and economics. For example, in astronomy, NumPy was an important part of the software stack used in the discovery of gravitational waves and the first imaging of a black hole. Here we show how a few fundamental array concepts lead to a simple and powerful programming paradigm for organizing, exploring, and analyzing scientific data. NumPy is the foundation upon which the entire scientific Python universe is constructed. It is so pervasive that several projects, targeting audiences with specialized needs, have developed their own NumPy-like interfaces and array objects. Because of its central position in the ecosystem, NumPy increasingly plays the role of an interoperability layer between these new array computation libraries.

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• Electromagnetic Signatures from Supermassive Binary Black Holes Approaching Merger
• Formation of black holes in the pair-instability mass gap: evolution of a post-collision star
• The cumulative star-formation histories of dwarf galaxies with TNG50. I: Environment-driven diversity and connection to quenching
• Characterizing Undetected Stellar Companions with Combined Datasets
• Euclid: Cosmological forecasts from the void size function
• Image Subtraction in Fourier Space
• Two lensed star candidates at $z\simeq 4.8$ behind the galaxy cluster MACS J0647.7+7015
• The mass-radius relation of exoplanets, revisited
• MIDIS: Strong (Hb + [OIII]) and Ha emitters at redshift $z\simeq 7-8$ unveiled with JWST/NIRCam and MIRI imaging in the Hubble eXtreme Deep Field (XDF)
• The First JWST Spectral Energy Distribution of a Y dwarf
• ALMA Confirmation of an Obscured Hyperluminous Radio-Loud AGN at $z=6.853$ Associated with a Dusty Starburst in the 1.5 deg${}^2$ COSMOS Field
• Observability of Evaporating Lava Worlds
• Little red dots as young supermassive black holes in dense ionized cocoons
• Evidence for the volatile-rich composition of a 1.5-$R_{\oplus }$ planet
• Observability of signatures of transport-induced chemistry in clear atmospheres of hot gas giant exoplanets
• A circular polarisation survey for radio stars with the Australian SKA Pathfinder
• 3D Morphology of Open Clusters in the Solar Neighborhood with Gaia EDR3 II: Hierarchical Star Formation Revealed by Spatial and Kinematic Substructures
• Intensity Mapping as a Probe of Axion Dark Matter
• The massive relic galaxy NGC 1277 is dark matter deficient. From dynamical models of integral-field stellar kinematics out to five effective radii
• Bayesian parameter estimation of stellar-mass black-hole binaries with LISA
• Awesome SOSS: Atmospheric Characterisation of WASP-96 b using the JWST Early Release Observations
• Unified model for the LISA measurements and instrument simulations
• CONCERTO: High-fidelity simulation of millimeter line emissions of galaxies and [CII] intensity mapping
• Model-Parallel Fourier Neural Operators as Learned Surrogates for Large-Scale Parametric PDEs
• Common envelope evolution of eccentric binaries
• GRMHD simulations of neutron-star mergers with weak interactions: r-process nucleosynthesis and electromagnetic signatures of dynamical ejecta
• BubbleDet: A Python package to compute functional determinants for bubble nucleation
• CNN-Based Deep Learning in Solar Wind Forecasting
• Introducing piXedfit -- a Spectral Energy Distribution Fitting Code Designed for Resolved Sources
• Software and computing for Run 3 of the ATLAS experiment at the LHC
• Galaxy Zoo: Stronger bars facilitate quenching in star forming galaxies
• Pulse-level noisy quantum circuits with QuTiP
• An all-sky sample of intermediate- to high-mass OBA-type eclipsing binaries observed by TESS
• Simulating quantum repeater strategies for multiple satellites
• ExoClock project II: A large-scale integrated study with 180 updated exoplanet ephemerides
• The gas and stellar content of a metal-poor galaxy at $z=8.496$ as revealed by JWST and ALMA
• Microarcsecond Astrometry: Science Highlights from Gaia
• The TESS-Keck Survey IV: A Retrograde, Polar Orbit for the Ultra-Low-Density, Hot Super-Neptune WASP-107b
• Fast and Credible Likelihood-Free Cosmology with Truncated Marginal Neural Ratio Estimation
• Stellar surface inhomogeneities as a potential source of the atmospheric signal detected in the K2-18 b transmission spectrum
• A simple model for mixing and cooling in cloud-wind interactions
• Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies
• Gaussian Process Foreground Subtraction and Power Spectrum Estimation for 21 cm Cosmology
• IllustrisTNG in the HSC-SSP: image data release and the major role of mini mergers as drivers of asymmetry and star formation
• REFLACX, a dataset of reports and eye-tracking data for localization of abnormalities in chest x-rays
• Redback: A Bayesian inference software package for electromagnetic transients
• The JWST Advanced Deep Extragalactic Survey: Discovery of an Extreme Galaxy Overdensity at $z=5.4$ with JWST/NIRCam in GOODS-S
• QUIJOTE scientific results -- IV. A northern sky survey in intensity and polarization at 10-20GHz with the Multi-Frequency Instrument
• Star Formation Regulation and Self-Pollution by Stellar Wind Feedback
• Andromeda XXI -- a dwarf galaxy in a low density dark matter halo
• A new way to test the Cosmological Principle: measuring our peculiar velocity and the large scale anisotropy independently
• Circumstellar Interaction Powers the Light Curves of Luminous Rapidly Evolving Optical Transients
• Metal-enriched halo gas across galaxy overdensities over the last 10 billion years
• Physical constraints on the extended interstellar medium of the z=6.42 quasar J1148+5251: [CII] 158um, [NII] 205um and [OI] 146um observations
• Exhaustive Symbolic Regression
• Gravitational wave sources in our Galactic backyard: Predictions for BHBH, BHNS and NSNS binaries detectable with LISA
• Forecasting pulsar timing array sensitivity to anisotropy in the stochastic gravitational wave background
• Medical Imaging and Machine Learning
• TOI-1452 b: SPIRou and TESS reveal a super-Earth in a temperate orbit transiting an M4 dwarf
• Overfitting Affects the Reliability of Radial Velocity Mass Estimates of the V1298 Tau Planets
• MaNGA DynPop -- I. Quality-assessed stellar dynamical modelling from integral-field spectroscopy of 10K nearby galaxies: a catalogue of masses, mass-to-light ratios, density profiles and dark matter
• Stellar Abundance Maps of the Milky Way Disk
• Constraining mornings & evenings on distant worlds: a new semi-analytical approach and prospects with transmission spectroscopy
• Combined analysis of the 12.8 and 15 $\mu m$ JWST/MIRI eclipse observations of TRAPPIST-1 b
• Steady-state accretion in magnetized protoplanetary disks
• Variational quantum eigensolver for the Heisenberg antiferromagnet on the kagome lattice
• Limits on Millimeter Continuum Emission from Circumplanetary Material in the DSHARP Disks
• The time delay distribution and formation metallicity of LIGO-Virgo's binary black holes
• Cosmological constraints from the BOSS DR12 void size function
• The Diverse Properties of Type Icn Supernovae Point to Multiple Progenitor Channels
• Magnetic field evolution in cosmic filaments with LOFAR data
• TIC 168789840: A Sextuply-Eclipsing Sextuple Star System
• CHEOPS Precision Phase Curve of the Super-Earth 55 Cnc e
• COSMOS2020: Discovery of a protocluster of massive quiescent galaxies at $z=2.77$
• Waveform uncertainty quantification and interpretation for gravitational-wave astronomy
• Molecular Gas Properties and CO-to-H2 Conversion Factors in the Central Kiloparsec of NGC 3351
• The Pan-STARRS1 z>5.6 quasar survey II: Discovery of 55 Quasars at 5.6<z<6.5
• Stellar Disruption of Axion Miniclusters in the Milky Way
• Constraints on the intergalactic magnetic field using Fermi-LAT and H.E.S.S. blazar observations
• Lattice continuum-limit study of nucleon quasi-PDFs
• Gas-phase metallicity gradients in galaxies at $z\sim 6-8$
• PySME -- Spectroscopy Made Easier
• Outflows Driven by Direct and Reprocessed Radiation Pressure in Massive Star Clusters
• Solar Flare Effects on the Earth's Lower Ionosphere
• Ultraviolet spectra of extreme nearby star-forming regions: evidence for an overabundance of very massive stars
• Stellar Rotation of T Tauri stars in the Orion Star-Forming Complex
• Modelling the Ringdown from Precessing Black Hole Binaries
• Redox hysteresis of super-Earth exoplanets from magma ocean circulation
• YSE-PZ: A Transient Survey Management Platform that Empowers the Human-in-the-Loop
• The Physical Drivers and Observational Tracers of CO-to-H2 Conversion Factor Variations in Nearby Barred Galaxy Centers
• The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z=3.5
• EIGER III. JWST/NIRCam observations of the ultra-luminous high-redshift quasar J0100+2802
• A 4 Gyr M-dwarf Gyrochrone from CFHT/MegaPrime Monitoring of the Open Cluster M67
• An ALMA study of hub-filament systems I. On the clump mass concentration within the most massive cores
• Reconstructing the Extreme Ultraviolet Emission of Cool Dwarfs Using Differential Emission Measure Polynomials
• TOI-5205 b: A Short-period Jovian Planet Transiting a Mid-M Dwarf
• Exploring Changing-look Active Galactic Nuclei with the Sloan Digital Sky Survey V: First Year Results
• Distance-Weighted Graph Neural Networks on FPGAs for Real-Time Particle Reconstruction in High Energy Physics
• The Two-Dimensional Metallicity Distribution and Mixing Scales of Nearby Galaxies
• HETDEX Public Source Catalog 1: 220K Sources Including Over 50K Lyman Alpha Emitters from an Untargeted Wide-area Spectroscopic Survey
• JWST Thermal Emission of the Terrestrial Exoplanet GJ 1132b
• Constraining the Cosmic Baryon Distribution with Fast Radio Burst Foreground Mapping
• Quartz Clouds in the Dayside Atmosphere of the Quintessential Hot Jupiter HD 189733 b
• Phase-resolved spectroscopy of a quasi-periodic oscillation in the black hole X-ray binary GRS 1915+105 with NICER and NuSTAR
• The Atacama Cosmology Telescope: Cosmology from cross-correlations of unWISE galaxies and ACT DR6 CMB lensing
• To cool is to keep: Residual H/He atmospheres of super-Earths and sub-Neptunes
• Atmospheres as windows into sub-Neptune interiors: coupled chemistry and structure of hydrogen-silane-water envelopes
• Kartezio: Evolutionary Design of Explainable Pipelines for Biomedical Image Analysis
• Constraining scalar-tensor theories by neutron star-balck hole gravitational wave events
• Testing AGN outflow and accretion models with CIV and HeII emission line demographics in z=2 quasars
• Metallicity, ionization parameter, and pressure variations of HII regions in the TYPHOON spiral galaxies
• A Deep Learning Approach for Active Anomaly Detection of Extragalactic Transients
• Constraints on the Faint End of the Galaxy Stellar Mass Function at z ~ 4-8 from Deep JWST Data
• Implementation of disequilibrium chemistry to spectral retrieval code ARCiS and application to sixteen exoplanet transmission spectra: Indication of disequilibrium chemistry for HD 209458b and WASP-39b
• Uncertain Times: The Redshift-Time Relation from Cosmology and Stars
• TOI-2109b: An Ultrahot Gas Giant on a 16 hr Orbit
• Numerical relativity surrogate model with memory effects and post-Newtonian hybridization
• Appreciating mergers for understanding the non-linear $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{spheroid}}$ and $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{galaxy}}$ relations, updated herein, and the implications for the (reduced) role of AGN feedback
• A Spectral Survey of WASP-19b with ESPRESSO
• Linear and Nonlinear Dimensionality Reduction from Fluid Mechanics to Machine Learning
• Mapping the exo-Neptunian landscape. A ridge between the desert and savanna
• The strength and structure of the magnetic field in the galactic outflow of M82
• WISDOM Project -- X. The morphology of the molecular ISM in galaxy centres and its dependence on galaxy structure
• The SAMI Galaxy Survey: stellar population and structural trends across the Fundamental Plane
• Bioverse: A Comprehensive Assessment of the Capabilities of Extremely Large Telescopes to Probe Earth-like O${}_2$ Levels in Nearby Transiting Habitable Zone Exoplanets
• Discovery and characterization of five new eclipsing AM CVn systems
• Galaxy Mergers in the Epoch of Reionization I: A JWST Study of Pair Fractions, Merger Rates, and Stellar Mass Accretion Rates at $z=4.5-11.5$
• Gauge-equivariant flow models for sampling in lattice field theories with pseudofermions
• Confirmation of Iron Emission Lines and Non-detection of TiO on the Dayside of KELT-9b with MAROON-X
• First Light And Reionisation Epoch Simulations (FLARES) IV: The size evolution of galaxies at $z\ge 5$
• COSMOS2020: Exploring the dawn of quenching for massive galaxies at 3 < z < 5 with a new colour selection method
• The Low-redshift Lyman-continuum Survey: [S II]-deficiency and the leakage of ionizing radiation
• Recovery of TESS Stellar Rotation Periods Using Deep Learning
• Statistical properties of the nebular spectra of 103 stripped envelope core collapse supernovae
• Inference of the cosmic rest-frame from supernovae Ia
• The Mass of the Milky Way from the H3 Survey
• The Galactic Dust-Up: Modeling Dust Evolution in FIRE
• Cosmography with Supernova Refsdal through time-delay cluster lensing: independent measurements of the Hubble constant and geometry of the Universe
• KiDS & Euclid: Cosmological implications of a pseudo angular power spectrum analysis of KiDS-1000 cosmic shear tomography
• On the origin of the mass-metallicity gradient relation in the local Universe
• A novel way of measuring the gas disk mass of protoplanetary disks using N2H+ and C18O
• Spectroscopic time series performance of the Mid-Infrared Instrument on the JWST
• Symmetries, Safety, and Self-Supervision
• Artificial intelligence discovery of a charging protocol in a micromaser quantum battery
• Fractal aggregates of sub-micron-sized grains in the young planet-forming disk around IM Lup
• The importance of silicate vapor in determining the structure, radii, and envelope mass fractions of sub-Neptunes
• Variational quantum simulations of stochastic differential equations
• Gaia Data Release 3: Properties of the line broadening parameter derived with the Radial Velocity Spectrometer (RVS)
• The mass and size of Herbig disks as seen by ALMA
• First results from SMAUG: The need for preventative stellar feedback and improved baryon cycling in semi-analytic models of galaxy formation
• Mid-to-Late M Dwarfs Lack Jupiter Analogs
• Predicting the Exoplanet Yield of the TESS Prime and Extended Missions Through Years 1-7
• Toward a Better Understanding of Cosmic Chronometers: Stellar Population Properties of Passive Galaxies at Intermediate Redshift
• Weighing the Galactic disk using phase-space spirals II. Most stringent constraints to a thin dark disk using Gaia EDR3
• Signatures of mass ratio reversal in gravitational waves from merging binary black holes
• The halo mass function and filaments in full cosmological simulations with fuzzy dark matter
• Dynamical ejecta synchrotron emission as possible contributor to the changing behaviour of GRB170817A
• Detecting stochastic gravitational waves with binary resonance
• Comprehensive analysis of a dense sample of FRB 121102 bursts
• Flares, jets and quasi-periodic outbursts from neutron star merger remnants
• Jellyfish galaxies with the IllustrisTNG simulations -- When, where, and for how long does ram pressure stripping of cold gas occur?
• Exploring dark matter spike distribution around the Galactic centre with stellar orbits
• Substructure in the stellar halo near the Sun. I. Data-driven clustering in Integrals of Motion space
• A lensed radio jet at milli-arcsecond resolution I: Bayesian comparison of parametric lens models
• The Galaxy Progenitors of Stellar Streams around Milky Way-mass Galaxies in the FIRE Cosmological Simulations
• Lifelong Machine Learning Potentials
• Investigating Deep Learning Methods for Obtaining Photometric Redshift Estimations from Images
• The SAMI Galaxy Survey: a statistical approach to an optimal classification of stellar kinematics in galaxy surveys
• A Closer Look at Exoplanet Occurrence Rates: Considering the Multiplicity of Stars Without Detected Planets
• Galaxy And Mass Assembly (GAMA): The inferred mass--metallicity relation from z=0 to 3.5 via forensic SED fitting
• Stellar Escape from Globular Clusters. I. Escape Mechanisms and Properties at Ejection
• The Hawaii Infrared Parallax Program. V. New T-Dwarf Members and Candidate Members of Nearby Young Moving Groups
• physiCal: A physical approach to the marginalization of LIGO calibration uncertainties
• $\mathtt{bajes}$: Bayesian inference of multimessenger astrophysical data, methods and application to gravitational-waves
• CO or no CO? Narrowing the CO abundance constraint and recovering the H2O detection in the atmosphere of WASP-127 b using SPIRou
• The SAGA Survey. III. A Census of 101 Satellite Systems around Milky Way-mass Galaxies
• On the Application of Bayesian Leave-One-Out Cross-Validation to Exoplanet Atmospheric Analysis
• Setting the stage for the search for life with the Habitable Worlds Observatory: Properties of 164 promising planet survey targets
• Identification of High-Redshift Galaxy Overdensities in GOODS-N and GOODS-S
• Evidence that the Hot Jupiter WASP-77 A b Formed Beyond Its Parent Protoplanetary Disk's H2O Ice Line
• RUBIES: A Spectroscopic Census of Little Red Dots; All V-Shaped Point Sources Have Broad Lines
• Non-linear black hole dynamics and Carrollian fluids
• Gemini/GMOS Optical Transmission Spectroscopy of WASP-121b: signs of variability in an ultra-hot Jupiter?
• Probing Kilonova Ejecta Properties Using a Catalog of Short Gamma-Ray Burst Observations
• Flybys, orbits, splashback: subhalos and the importance of the halo boundary
• Using [Ne V]/[Ne III] to Understand the Nature of Extreme-Ionization Galaxies
• Quantum Machine-Learning for Eigenstate Filtration in Two-Dimensional Materials
• Dynamically constraining the length of the Milky Way bar
• Bayesian field-level inference of primordial non-Gaussianity using next-generation galaxy surveys
• pyerrors: a python framework for error analysis of Monte Carlo data
• High-resolution atmospheric retrievals of WASP-121b transmission spectroscopy with ESPRESSO: Consistent relative abundance constraints across multiple epochs and instruments
• A neural simulation-based inference approach for characterizing the Galactic Center $\gamma$-ray excess
• High [OIII]/[CII] surface brightness ratios trace early starburst galaxies
• VERTICO II: effects of HI-identified environmental mechanisms on molecular gas
• Can gravitational-wave memory help constrain binary black-hole parameters? A LISA case study
• Dark Matter Deficient Galaxies And Their Member Star Clusters Form Simultaneously During High-velocity Galaxy Collisions In 1.25 pc Resolution Simulations
• APPLESOSS: A Producer of ProfiLEs for SOSS. Application to the NIRISS SOSS Mode
• Warm Jupiters in TESS Full-Frame Images: A Catalog and Observed Eccentricity Distribution for Year 1
• On the discovery of stars, quasars, and galaxies in the Southern Hemisphere with S-PLUS DR2
• JWST near-infrared spectroscopy of the Lucy Jupiter Trojan flyby targets: Evidence for OH absorption, aliphatic organics, and CO${}_2$
• Scalable Uncertainty Quantification for Deep Operator Networks using Randomized Priors
• After The Fall: Resolving the Molecular Gas in Post-Starburst Galaxies
• The challenge of simultaneously matching the observed diversity of chemical abundance patterns in cosmological hydrodynamical simulations
• Stellar Metallicities from SkyMapper Photometry II: Precise photometric metallicities of $\sim$280,000 giant stars with [Fe/H] $<-0.75$ in the Milky Way
• The bursty star formation history of the Fornax dwarf spheroidal galaxy revealed with the HST
• Properties of the jet in M87 revealed by its helical structure imaged with the VLBA at 8 and 15 GHz
• Differentiable quantum chemistry with PySCF for molecules and materials at the mean-field level and beyond
• The challenge of simulating the star cluster population of dwarf galaxies with resolved interstellar medium
• Astrometric Accelerations as Dynamical Beacons: Discovery and Characterization of HIP 21152 B, the First T-Dwarf Companion in the Hyades
• An unusually low-density super-Earth transiting the bright early-type M-dwarf GJ 1018 (TOI-244)
• H-alpha and Ca II Infrared Triplet Variations During a Transit of the 23 Myr Planet V1298 Tau c
• The unpopular Package: a Data-driven Approach to De-trend TESS Full Frame Image Light Curves
• HST grism spectroscopy of z~3 massive quiescent galaxies: Approaching the metamorphosis
• Pythonic Black-box Electronic Structure Tool (PyBEST). An open-source Python platform for electronic structure calculations at the interface between chemistry and physics
• Generative Capacity of Probabilistic Protein Sequence Models
• Black Hole Polarimetry I: A Signature of Electromagnetic Energy Extraction
• Mining the Ultra-Hot Skies of HAT-P-70b: Detection of a Profusion of Neutral and Ionized Species
• The Spectroscopic Classification of Astronomical Transients (SCAT) Survey: Overview, Pipeline Description, Initial Results, and Future Plans
• Velocity structure functions in multiphase turbulence: interpreting kinematics of H$\alpha$ filaments in cool core clusters
• The integrated 3-point correlation function of cosmic shear
• The Mira Distance to M101 and a 4% Measurement of H0
• CRIRES+ and ESPRESSO reveal an atmosphere enriched in volatiles relative to refractories on the ultra-hot Jupiter WASP-121b
• Photometric segregation of dwarf and giant FGK stars using the SVO Filter Profile Service and photometric tools
• $\text{Mangrove}$: Learning Galaxy Properties from Merger Trees
• Milky Way Mass with K Giants and BHB Stars Using LAMOST, SDSS/SEGUE, and Gaia: 3D Spherical Jeans Equation and Tracer Mass Estimator
• SMARPs and SHARPs: Two Solar Cycles of Active Region Data
• Porous Dust Particles in Protoplanetary Disks: Application to the HL Tau Disk
• Blandford-Znajek jets in galaxy formation simulations: exploring the diversity of outflows produced by spin-driven AGN jets in Seyfert galaxies
• Towards efficient and accurate \emph{ab initio} solutions to periodic systems via transcorrelation and coupled cluster theory
• A Transient "Changing-look'' Active Galactic Nucleus Resolved on Month Timescales from First-year Sloan Digital Sky Survey V Data
• How merger-driven gas motions in galaxy clusters can turn AGN bubbles into radio relics
• The stellar metallicity gradients of Local Group dwarf galaxies
• Testing new physics models with global comparisons to collider measurements: the Contur toolkit
• Gravelamps: Gravitational Wave Lensing Mass Profile Model Selection
• PHANGS-JWST First Results: Duration of the early phase of massive star formation in NGC628
• Target Selection for the DESI Peculiar Velocity Survey
• Gaia pulsars and where to find them
• The NANOGrav 15-year Gravitational-Wave Background Methods
• On dust evolution in planet-forming discs in binary systems. I -- Theoretical and numerical modelling: radial drift is faster in binary discs
• Bridging the gap -- the disappearance of the intermediate period gap for fully convective stars, uncovered by new ZTF rotation periods
• Outflows from Super Star Clusters in the Central Starburst of NGC253
• The FRB20190520B Sightline Intersects Foreground Galaxy Clusters
• Roaring Storms in the Planetary-Mass Companion VHS 1256-1257 b: Hubble Space Telescope Multi-epoch Monitoring Reveals Vigorous Evolution in an Ultra-cool Atmosphere
• Signatures of the Many Supermassive Black Hole Mergers in a Cosmologically Forming Massive Early-Type Galaxy
• Gaia Data Release 3: A Golden Sample of Astrophysical Parameters
• A quasar-based supermassive black hole binary population model: implications for the gravitational-wave background
• Machine-learning classification of astronomical sources: estimating F1-score in the absence of ground truth
• Simultaneous Multiwavelength Flare Observations of EV Lacertae
• Complications in the ALMA Detection of Phosphine at Venus
• A galaxy-driven model of type Ia supernova luminosity variations
• A data-driven Reconstruction of Horndeski gravity via the Gaussian processes
• Gaia DR3 in 6D: The search for fast hypervelocity stars and constraints on the Galactic Centre environment
• Aemulus $\nu$: Precise Predictions for Matter and Biased Tracer Power Spectra in the Presence of Neutrinos
• The KBSS-KCWI Survey: The connection between extended Ly$\alpha$ halos and galaxy azimuthal angle at $z\sim 2-3$
• Do Central Compact Objects have Carbon Atmospheres?
• Measurement of the Open Magnetic Flux in the Inner Heliosphere down to 0.13AU
• Cosmological Implications of Axion-Matter Couplings
• PetroFit: A Python Package for Computing Petrosian Radii and Fitting Galaxy Light Profiles
• Three-dimensional Global Simulations of Type-II Planet-disk Interaction with a Magnetized Disk Wind: I. Magnetic Flux Concentration and Gap Properties
• The first large catalogue of spectroscopic redshifts in Webb's First Deep Field, SMACS J0723.3$-$7327
• Long-term Evolution of Binary Orbits Induced by Circumbinary Disks
• Dynamical Mass of the Young Substellar Companion HD 984 B
• The XQR-30 Metal Absorber Catalog: 778 Absorption Systems Spanning 2 < z < 6.5
• Characterization of Population III Stars with Stellar Atmosphere and Evolutionary Modeling and Predictions of their Observability with the James Webb Space Telescope
• Galaxy cluster strong lensing cosmography: cosmological constraints from a sample of regular galaxy clusters
• Obliquities of Exoplanet Host Stars: 19 New and Updated Measurements, and Trends in the Sample of 205 Measurements
• A Primer on Focused Solar Energetic Particle Transport: Basic physics and recent modelling results
• The Possibility of Modeling the Very High Energy Afterglow of GRB 221009A in a Wind Environment
• Quantum error correction with dissipatively stabilized squeezed cat qubits
• TOI-561 b: A Low Density Ultra-Short Period "Rocky" Planet around a Metal-Poor Star
• Photometric variability as a proxy for magnetic activity and its dependence on metallicity
• PHANGS-JWST First Results: Rapid Evolution of Star Formation in the Central Molecular Gas Ring of NGC1365
• The IGRINS YSO Survey I. Stellar parameters of pre-main sequence stars in Taurus-Auriga
• Cosmology with varying fundamental constants from hyperlight, coupled scalars
• Ginex: SSD-enabled Billion-scale Graph Neural Network Training on a Single Machine via Provably Optimal In-memory Caching
• A New Infrared Criterion for Selecting Active Galactic Nuclei to Lower Luminosities
• The Impact of Mixing Treatments on Cloud Modelling in 3D Simulations of Hot Jupiters
• Two-pole nature of the $\Lambda (1405)$ from lattice QCD
• Blind spots and biases: the dangers of ignoring eccentricity in gravitational-wave signals from binary black holes
• On the inconsistency of [C/Fe] abundances and the fractions of carbon-enhanced metal-poor stars among various stellar surveys
• Implicit Likelihood Inference of Reionization Parameters from the 21 cm Power Spectrum
• Fast simulation of bosonic qubits via Gaussian functions in phase space
• Tracing snowlines and C/O ratio in a planet-hosting disk: ALMA molecular line observations towards the HD169142 disk
• The Pan-STARRS1 $\mathbf{z}>5.6$ Quasar Survey: III. The $\mathbf{z}\approx 6$ Quasar Luminosity Function
• TOI-1278 B: SPIRou unveils a rare Brown Dwarf Companion in Close-In Orbit around an M dwarf
• Predictions of the LSST Solar System Yield: Near-Earth Objects, Main Belt Asteroids, Jupiter Trojans, and Trans-Neptunian Objects
• Accurate characterization of the stochastic gravitational-wave background with pulsar timing arrays by likelihood reweighting
• Unveiling the merger structure of black hole binaries in generic planar orbits
• The impact of spurious collisional heating on the morphological evolution of simulated galactic discs
• The Three-Phase Evolution of the Milky Way
• Lattice QCD study of $\pi \Sigma -\bar{K}N$ scattering and the $\Lambda (1405)$ resonance
• Swift J1727.8-1613 has the Largest Resolved Continuous Jet Ever Seen in an X-ray Binary
• SLAC Microresonator RF (SMuRF) Electronics: A tone-tracking readout system for superconducting microwave resonator arrays
• Calibrations of the Compton Spectrometer and Imager
• Graph Neural Networks for Charged Particle Tracking on FPGAs
• RC100: Rotation Curves of 100 Massive Star-Forming Galaxies at z=0.6-2.5 Reveal Little Dark Matter on Galactic Scales
• ALMA-IMF II -- investigating the origin of stellar masses: Continuum Images and Data Processing
• The Fornax3D project: Assembly histories of lenticular galaxies from a combined dynamical and population orbital analysis
• Digging into the Interior of Hot Cores with ALMA (DIHCA). I. Dissecting the High-mass Star-Forming Core G335.579-0.292 MM1
• A thermal-kinetic subgrid model for supernova feedback in simulations of galaxy formation
• The GAPS Programme at TNG XXXIX -- Multiple molecular species in the atmosphere of the warm giant planet WASP-80 b unveiled at high resolution with GIANO-B
• The star formation history of Eridanus II: on the role of SNe feedback in the quenching of ultra-faint dwarf galaxies
• Radial structure and formation of the Milky Way disc
• The origin of metal-poor stars on prograde disk orbits in FIRE simulations of Milky Way-mass galaxies
• Gaia Data Release 3: Hot-star radial velocities
• A Comparative Analysis of the Chemical Compositions of Gaia-Enceladus/Sausage and Milky Way Satellites using APOGEE
• Chasing rainbows and ocean glints: Inner working angle constraints for the Habitable Worlds Observatory
• Impact of noise transients on low latency gravitational-wave event localisation
• The CGM${}^2$ Survey: Circumgalactic O VI from dwarf to massive star-forming galaxies
• Towards Robust Expert Finding in Community Question Answering Platforms
• Evaluating the prevalence of spurious correlations in pulsar timing array datasets
• Poking Holes: Looking for Gaps in LIGO/Virgo's Black Hole Population
• Searching for ringdown higher modes with a numerical relativity-informed post-merger model
• Spin and Eccentricity Evolution in Triple Systems: from the Lidov-Kozai Interaction to the Final Merger of the Inner Binary
• Probabilistic Mass Mapping with Neural Score Estimation
• ParSNIP: Generative Models of Transient Light Curves with Physics-Enabled Deep Learning
• Measuring the properties of active galactic nuclei disks with gravitational waves
• Distant Relatives: The Chemical Homogeneity of Comoving Pairs Identified in Gaia
• Effects of UV stellar spectral uncertainty on the chemistry of terrestrial atmospheres
• Priors on red galaxy stochasticity from hybrid effective field theory
• Molecular photodissociation enabled by ultrafast plasmon decay
• X-ray Thomson scattering spectra from DFT-MD simulations based on a modified Chihara formula
• The TESS Grand Unified Hot Jupiter Survey. II. Twenty New Giant Planets
• Systematically Revisiting All NuSTAR Spins of Black Holes in X-Ray Binaries
• Flow-based sampling in the lattice Schwinger model at criticality
• Synthetic Evolution Tracks of Giant Planets
• Escaping Helium and a Highly Muted Spectrum Suggest a Metal-Enriched Atmosphere on Sub-Neptune GJ3090b from JWST Transit Spectroscopy
• Towards an open-source landscape for 3D CSEM modelling
• GALACTICNUCLEUS: A high-angular-resolution $JH{K}_s$ imaging survey of the Galactic centre. IV. Extinction maps and de-reddened photometry
• Data mining techniques on astronomical spectra data. II : Classification Analysis
• FLIMFLAM DR1: The First Constraints on the Cosmic Baryon Distribution from 8 FRB sightlines
• The vertical structure of debris disks and the impact of gas
• LEGWORK: A python package for computing the evolution and detectability of stellar-origin gravitational-wave sources with space-based detectors
• Uses of Complex Metrics in Cosmology
• A New Analysis of 8 Spitzer Phase Curves and Hot Jupiter Population Trends: Qatar-1b, Qatar-2b, WASP-52b, WASP-34b, and WASP-140b
• U(1) symmetric recurrent neural networks for quantum state reconstruction
• JWST Observations of Young protoStars (JOYS): Linked accretion and ejection in a Class I protobinary system
• The CubeSpec space mission. I. Asteroseismology of massive stars from time series optical spectroscopy: science requirements and target list prioritisation
• The SPIRou Legacy Survey Rotation period of quiet M dwarfs from circular polarization in near-infrared spectral lines: I. The SPIRou APERO analysis
• The MASSIVE SURVEY XVI. The Stellar Initial Mass Function in the Center of MASSIVE Early-Type Galaxies
• Deep learning approach for identification of HII regions during reionization in 21-cm observations
• AGN Feedback in SDSS-IV MaNGA: AGNs have Suppressed Central Star Formation Rates
• ATOCA: an algorithm to treat order contamination. Application to the NIRISS SOSS mode
• Ionized gas kinematics and chemical abundances of low-mass star-forming galaxies at $z\sim 3$
• The Quest for the Missing Dust: II -- Two Orders of Magnitude of Evolution in the Dust-to-Gas Ratio Resolved Within Local Group Galaxies
• Integrated Mass Loss of Evolved Stars in M4 using Asteroseismology
• exoALMA III: Line-intensity Modeling and System Property Extraction from Protoplanetary Disks
• Machine learning assisted phase and size-controlled synthesis of iron oxides
• agnpy: An open-source python package modelling the radiative processes of jetted active galactic nuclei
• The SAMI Galaxy Survey: flipping of the spin-filament alignment correlates most strongly with growth of the bulge
• Observational Signatures of Frame Dragging in Strong Gravity
• Deep Realistic Extragalactic Model (DREaM) Galaxy Catalogs: Predictions for a Roman Ultra-Deep Field
• How many quantum gates do gauge theories require?
• Constraints on the cosmic expansion rate at redshift 2.3 from the Lyman-$\alpha$ forest
• Modest dust settling in the IRAS04302+2247 Class I protoplanetary disk
• IDEFIX: a versatile performance-portable Godunov code for astrophysical flows
• JWST CEERS probes the role of stellar mass and morphology in obscuring galaxies
• Reducing the complexity of chemical networks via interpretable autoencoders
• Aura-3D: A Three-dimensional Atmospheric Retrieval Framework for Exoplanet Transmission Spectra
• A JWST Near- and Mid-Infrared Nebular Spectrum of the Type Ia Supernova 2021aefx
• A Near-Infrared Chemical Inventory of the Atmosphere of 55 Cancri e
• Direct emission spectroscopy of exoplanets with the medium resolution imaging spectrometer on board JWST MIRI: I. Molecular mapping and sensitivity to instrumental effects
• The dynamic magnetosphere of Swift J1818.0$-$1607
• Widespread Detection of Two Components in the Hot Circumgalactic Medium of the Milky Way
• The MUSE eXtremely Deep Field: Individual detections of Lyα haloes around rest-frame UV-selected galaxies at z~2.9-4.4
• RIGEL: Simulating dwarf galaxies at solar mass resolution with radiative transfer and feedback from individual massive stars
• Phases of Mass Transfer from Hot Subdwarfs to White Dwarf Companions and Their Photometric Properties
• PyAutoFit: A Classy Probabilistic Programming Language for Model Composition and Fitting
• Energetic Electron Distribution of the Coronal Acceleration Region: First results from Joint Microwave and Hard X-ray Imaging Spectroscopy
• A Late-Time Galaxy-Targeted Search for the Radio Counterpart of GW190814
• Simulated Bars May Be Shorter But Are Not Slower Than Observed: TNG50 vs. MaNGA
• Tailoring hot-carrier distributions of plasmonic nanostructures through surface alloying
• Disk Tearing Leads to Low and High Frequency Quasi Periodic Oscillations in a GRMHD Simulation of a Thin Accretion Disk
• Neutron star mass estimates from gamma-ray eclipses in spider millisecond pulsar binaries
• TESS observations of the Pleiades cluster: a nursery for delta Scuti stars
• Matrix decompositions in Quantum Optics: Takagi/Autonne, Bloch-Messiah/Euler, Iwasawa, and Williamson
• Outshining in the Spatially Resolved Analysis of a Strongly-Lensed Galaxy at z=6.072 with JWST NIRCam
• QCD constraints on isospin-dense matter and the nuclear equation of state
• Axion-like Particle Searches at DarkQuest
• Target Prioritization and Observing Strategies for the NEID Earth Twin Survey
• Modeling the kinematics of the decelerating jets from the black hole X-ray binary MAXI J1348$-$630
• The Fundamental Plane in the LEGA-C Survey: unraveling the $M/L$ variations of massive star-forming and quiescent galaxies at $z\sim 0.8$
• The ESO SupJup Survey III: Confirmation of 13CO in YSES 1 b and Atmospheric Detection of YSES 1 c with CRIRES+
• Revealing the Impact of Quasar Luminosity on Giant Ly$\alpha$ Nebulae
• Photometric detection at $7.7\mu \mathrm{m}$ of a galaxy beyond redshift $14$ with JWST/MIRI
• Detection of Ionized Calcium in the Atmosphere of the Ultra-Hot Jupiter WASP-76b
• Model-independent constraints on ${\Omega }_m$ and $H(z)$ from the link between geometry and growth
• The Gas Morphology of Nearby Star-Forming Galaxies
• Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys
• Revisiting the evidence for precession in GW200129 with machine learning noise mitigation
• Developing the Future of Gamma-ray Astrophysics with Monolithic Silicon Pixels
• Photochemical hazes dramatically alter temperature structure and atmospheric circulation in 3D simulations of hot Jupiters
• Fading AGN in Post-Starburst Galaxies
• Bayesian neural networks via MCMC: a Python-based tutorial
• Detection Limits of Low-mass, Long-period Exoplanets Using Gaussian Processes Applied to HARPS-N Solar RVs
• New Observations of Solar Wind 1/f Turbulence Spectrum from Parker Solar Probe
• Surface Brightness Profile of Lyman-$\alpha$ Halos out to 320 kpc in HETDEX
• COSMOS2020: Ubiquitous AGN Activity of Massive Quiescent Galaxies at $0<z<5$ Revealed by X-ray and Radio Stacking
• Numerical simulations of the random angular momentum in convection II: delayed explosions of red supergiants following "failed'' supernovae
• Chemical Feedbacks of Pebble Growth: Impacts on CO depletion and C/O ratios
• N-body simulations of dark matter with frequent self-interactions
• Beyond UVJ: Color Selection of Galaxies in the JWST Era
• MAGAZ3NE: High Stellar Velocity Dispersions for Ultra-Massive Quiescent Galaxies at $z\gtrsim 3$
• The growth and migration of massive planets under the influence of external photoevaporation
• The Gaia EDR3 view of Johnson-Kron-Cousins standard stars: the curated Landolt and Stetson collections
• The ${\chi }_{\mathrm{eff}}-z$ correlation of field binary black hole mergers and how 3G gravitational-wave detectors can constrain it
• System-reliability based multi-ensemble of GAN and one-class joint Gaussian distributions for unsupervised real-time structural health monitoring
• pyTDGL: Time-dependent Ginzburg-Landau in Python
• The ALMOND Survey: Molecular cloud properties and gas density tracers across 25 nearby spiral galaxies with ALMA
• From giant clumps to clouds -- III. The connection between star formation and turbulence in the ISM
• Multi-phase outflows in high redshift quasar host galaxies
• Undetected Binary Stars Cause an Observed Mass Dependent Age Gradient in Upper Scorpius
• Detection of nonlinear resonances among gravity modes of slowly pulsating B stars: results from five iterative prewhitening strategies
• Evidence for mass-dependent peculiar velocities in compact object binaries: Towards better constraints on natal kicks
• Computing solution space properties of combinatorial optimization problems via generic tensor networks
• Wave-driven mass loss of stripped envelope massive stars: progenitor-dependence, mass ejection, and supernovae
• Variational Monte Carlo with Large Patched Transformers
• Photometric Redshifts from SDSS Images with an Interpretable Deep Capsule Network
• Cosmological coupling of nonsingular black holes
• Identifying RR Lyrae Variable Stars in Six Years of the Dark Energy Survey
• Deep Synoptic Array science: A massive elliptical host among two galaxy-cluster fast radio bursts
• PHANGS-MUSE: Detection and Bayesian classification of ~40000 ionised nebulae in nearby spiral galaxies
• 97 Eclipsing Quadruple Star Candidates Discovered in TESS Full Frame Images
• MIGHTEE: Deep 1.4 GHz Source Counts and the Sky Temperature Contribution of Star Forming Galaxies and Active Galactic Nuclei
• Arkenstone I: A Novel Method for Robustly Capturing High Specific Energy Outflows In Cosmological Simulations
• Impact of extreme spins and mass ratios on the post-merger observables of high-mass binary neutron stars
• New minimal, median, and maximal propagation models for dark matter searches with Galactic cosmic rays
• Statistical Study of the Star Formation Efficiency in Bars: Is Star Formation Suppressed in Gas-Rich Bars?
• Discovery of the Magellanic Stellar Stream Out to 100 Kiloparsecs
• Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO & SFR data
• Still Brighter than Pre-Explosion, SN 2012Z Did Not Disappear: Comparing Hubble Space Telescope Observations a Decade Apart
• On the rise times in FU Orionis events
• Measurements of the Hubble Constant with a Two Rung Distance Ladder: Two Out of Three Ain't Bad
• Metal line emission from galaxy haloes at z~1
• The SAMI Galaxy Survey: Mass and Environment as Independent Drivers of Galaxy Dynamics
• Resolving the Complex Evolution of a Supermassive Black Hole Triplet in a Cosmological Simulation
• Self-Consistent Spin, Tidal and Dynamical Equations of Motion in the REBOUNDx Framework
• Detailed chemical abundances of stars in the outskirts of the Tucana II ultra-faint dwarf galaxy
• GW241011 and GW241110: Exploring Binary Formation and Fundamental Physics with Asymmetric, High-Spin Black Hole Coalescence
• LoTSS Jellyfish Galaxies IV: Enhanced Star Formation on the Leading Half of Cluster Galaxies and Gas Compression in IC3949
• Constraining galaxy overdensities around three z~6.5 quasars with ALMA and MUSE
• Stellar Obliquities in Long-period Exoplanet Systems (SOLES) I: The Spin-Orbit Alignment of K2-140 b
• Toward Robust Corrections for Stellar Contamination in JWST Exoplanet Transmission Spectra
• JWST Peers into the Class I Protostar TMC1A: Atomic Jet and Spatially Resolved Dissociative Shock Region
• The origins of Calcium-rich supernovae from disruptions of CO white-dwarfs by hybrid He-CO white-dwarfs
• Turbulence in Milky Way Star-Forming Regions Traced by Young Stars and Gas
• On the Correlation between Hot Jupiters and Stellar Clustering: High-eccentricity Migration Induced by Stellar Flybys
• Confusion noise from Galactic binaries for Taiji
• Pulsar Candidate Identification Using Semi-Supervised Generative Adversarial Networks
• Exploring the link between C IV outflow kinematics and sublimation-temperature dust in quasars
• Water Ice Cloud Variability & Multi-Epoch Transmission Spectra of TRAPPIST-1e
• The SIBELIUS Project: E Pluribus Unum
• Spectropolarimetric variability in the repeating fast radio burst source FRB 20180301A
• PHANGS-JWST First Results: The Dust Filament Network of NGC 628 and its Relation to Star Formation Activity
• Exploring the s-process history in the Galactic disk: Cerium abundances and gradients in Open Clusters from the OCCAM/APOGEE sample
• An orbital perspective on the starvation, stripping, and quenching of satellite galaxies in the EAGLE simulations
• Giant planet engulfment by evolved giant stars: light curves, asteroseismology, and survivability
• The Lightweaver Framework for NLTE Radiative Transfer in Python
• The global structure of magnetic fields and gas in simulated Milky Way-analogue galaxies
• Discovery of the local counterpart of disc galaxies at z > 4: The oldest thin disc of the Milky Way using Gaia-RVS
• Mapping Dark Matter with Extragalactic Stellar Streams: the Case of Centaurus A
• Revealing the physical properties of gas accreting to haloes in the EAGLE simulations
• Planet Engulfment Detections are Rare According to Observations and Stellar Modeling
• Focal Plane Wavefront Sensing using Machine Learning: Performance of Convolutional Neural Networks compared to Fundamental Limits
• ENERO: Efficient Real-Time WAN Routing Optimization with Deep Reinforcement Learning
• Tidal tails in the disintegrating open cluster NGC 752
• Cosmology and Astrophysics with Standard Sirens and Galaxy Catalogs in View of Future Gravitational Wave Observations
• Superposed metric for spinning black hole binaries approaching merger
• GIGA-Lens: Fast Bayesian Inference for Strong Gravitational Lens Modeling
• The 3-D Kinematics of the Orion Nebula Cluster: NIRSPEC-AO Radial Velocities of the Core Population
• Exploring the Impact of Microlensing on Gravitational Wave Signals: Biases, Population Characteristics, and Prospects for Detection
• Planetary Nebula Luminosity Function distances for 19 galaxies observed by PHANGS-MUSE
• netrd: A library for network reconstruction and graph distances
• Galaxy Clustering Analysis with SimBIG and the Wavelet Scattering Transform
• Constraints on Stellar Flare Energy Ratios in the NUV and Optical From a Multiwavelength Study of GALEX and Kepler Flare Stars
• Resolving desorption of complex organic molecules in a hot core: Transition from non-thermal to thermal desorption or two-step thermal desorption?
• Age-Dating Red Giant Stars Associated with Galactic Disk and Halo Substructures
• Cosmoglobe DR1 results. II. Constraints on isotropic cosmic birefringence from reprocessed WMAP and Planck LFI data
• A Systematic Search for Short-period Close White Dwarf Binary Candidates Based on Gaia EDR3 Catalog and Zwicky Transient Facility Data
• TOI-5005 b: A super-Neptune in the savanna near the ridge
• Probing new light gauge bosons with gravitational-wave interferometers using an adapted semi-coherent method
• A radio technosignature search towards Proxima Centauri resulting in a signal-of-interest
• Constraining nucleosynthesis in neutrino-driven winds: observations, simulations and nuclear physics
• On the design space between molecular mechanics and machine learning force fields
• JWST Observations of Young protoStars (JOYS). HH 211: the textbook case of a protostellar jet and outflow
• First search for ultralight dark matter with a space-based gravitational-wave antenna: LISA Pathfinder
• The Morpho-Kinematic Architecture of Super Star Clusters in the Center of NGC253
• Mass ejection in failed supernovae: equation of state and neutrino loss dependence
• Freely jointed chain models with extensible links
• The First Quiescent Galaxies in TNG300
• Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0
• Compton-Thick AGN in the NuSTAR era VIII: A joint NuSTAR-XMM-Newton monitoring of the changing-look Compton-thick AGN NGC 1358
• Planck constraints on cross-correlations between anisotropic cosmic birefringence and CMB polarization
• What it Takes to Measure Reionization with Fast Radio Bursts
• Transferring spectroscopic stellar labels to 217 million Gaia DR3 XP stars with SHBoost
• SporTran: a code to estimate transport coefficients from the cepstral analysis of (multivariate) current time series
• First frequency-domain phenomenological model of the multipole asymmetry in gravitational-wave signals from binary-black-hole coalescence
• Radio and Far-IR Emission Associated with a Massive Star-forming Galaxy Candidate at z$\simeq$6.8: A Radio-Loud AGN in the Reionization Era?
• The growth of H II regions around massive stars: the role of metallicity and dust
• Antenna beam characterisation for the global 21cm experiment LEDA and its impact on signal model parameter reconstruction
• Euclid preparation: XIII. Forecasts for galaxy morphology with the Euclid Survey using Deep Generative Models
• Circumstellar Medium Interaction in SN 2018lab, A Low-Luminosity II-P Supernova observed with TESS
• SBI++: Flexible, Ultra-fast Likelihood-free Inference Customized for Astronomical Applications
• The Effect of Jet-Ejecta Interaction on the Viewing Angle Dependence of Kilonova Light Curves
• Revisiting the Iconic Spitzer Phase Curve of 55 Cancri e: Hotter Dayside, Cooler Nightside and Smaller Phase Offset
• A Quasi-periodic Oscillation in the gamma-ray Emission from the Non-blazar Active Galactic Nucleus PKS 0521-36
• VARAHA: A Fast Non-Markovian sampler for estimating Gravitational-Wave posteriors
• Orbital decay in M82 X-2
• The locations of features in the mass distribution of merging binary black holes are robust against uncertainties in the metallicity-dependent cosmic star formation history
• Evaluating the Plausible Range of N2O Biosignatures on Exo-Earths: An Integrated Biogeochemical, Photochemical, and Spectral Modeling Approach
• Revisiting UV/optical continuum time lags in AGN
• Radiation shielding of protoplanetary discs in young star-forming regions
• A $Gaia$ EDR3 search for tidal tails in disintegrating open clusters
• Searching for flaring star-planet interactions in AU Mic TESS observations
• Formation of globular clusters in dwarf galaxies of the Local Group
• Data mining techniques on astronomical spectra data. I : Clustering Analysis
• ALMA observations of NGC 6334S. II. Subsonic and Transonic Narrow Filaments in a High-mass Star Formation Cloud
• KiDS-Legacy: Consistency of cosmic shear measurements and joint cosmological constraints with external probes
• The Impact of Black Hole Formation on Population Averaged Supernova Yields
• Theoretical systematics in testing the Cosmological Principle with the kinematic quasar dipole
• The Bright Extragalactic ALMA Redshift Survey (BEARS) I: redshifts of bright gravitationally-lensed galaxies from the Herschel ATLAS
• An Observationally-Derived Kick Distribution for Neutron Stars in Binary Systems
• Accurate predictions from small boxes: variance suppression via the Zel'dovich approximation
• The evolution of the Milky Way's thin disc radial metallicity gradient with K2 asteroseismic ages
• Measurement-induced transitions for interacting fermions
• The MUSE-Faint survey. II. The dark matter-density profile of the ultra-faint dwarf galaxy Eridanus 2
• Inductive Simulation of Calorimeter Showers with Normalizing Flows
• The fraction and kinematics of broad absorption line quasars across cosmic time
• Chandra, HST/STIS, NICER, Swift, and TESS Detail the Flare Evolution of the Repeating Nuclear Transient ASASSN-14ko
• Star Formation and Molecular Gas Diagnostics with Mid- and Far-Infrared Emission
• Dynamics of relativistic radio jets in asymmetric environments
• First Light And Reionisation Epoch Simulations (FLARES) VII: The Star Formation and Metal Enrichment Histories of Galaxies in the early Universe
• The deepest $Chandra$ view of RBS 797: evidence for two pairs of equidistant X-ray cavities
• The SNAD Viewer: Everything You Want to Know about Your Favorite ZTF Object
• Estimating the warm dark matter mass from strong lensing images with truncated marginal neural ratio estimation
• RMTable2023 and PolSpectra2023: standards for reporting polarization and Faraday rotation measurements of radio sources
• Fine structures of radio bursts from flare star AD Leo with FAST observations
• The photometric variability of massive stars due to gravity waves excited by core convection
• Is Open-Source There Yet? A Comparative Study on Commercial and Open-Source LLMs in Their Ability to Label Chest X-Ray Reports
• IQ Collaboratory II: The Quiescent Fraction of Isolated, Low Mass Galaxies Across Simulations and Observations
• Formation of star clusters and enrichment by massive stars in simulations of low-metallicity galaxies with a fully sampled initial stellar mass function
• The radial variation of the solar wind turbulence spectra near the kinetic break scale from Parker Solar Probe measurements
• Controlling Chaos Using Edge Computing Hardware
• Optimization of model independent gravitational wave search using machine learning
• Strong decay widths and mass spectra of charmed baryons
• Distant Echoes of the Milky Way's Last Major Merger
• Investigating Topological Order using Recurrent Neural Networks
• A multi-shock model for the density variance of anisotropic, highly-magnetised, supersonic turbulence
• KiDS-1000 cosmology: Combined second- and third-order shear statistics
• UOCS VII. Blue Straggler Populations of Open Cluster NGC 7789 with UVIT/AstroSat
• The Demographics of Terrestrial Planets in the Venus Zone
• JWST Observations of Young protoStars (JOYS). Overview of gaseous molecular emission and absorption in low-mass protostars
• Study of changes in the pulsation period of 148 Galactic Cepheid variables
• Mock data study for next-generation ground-based detectors: The performance loss of matched filtering due to correlated confusion noise
• Implications of the Milky Way travel velocity for dynamical mass estimates of the Local Group
• Investigating the relation between gravitational wave tests of general relativity
• Constraining SIDM with halo shapes: revisited predictions from realistic simulations of early-type galaxies
• Improved AI-generated Solar Farside Magnetograms by STEREO and SDO Data Sets and Their Release
• Turbulent diffusion of streaming cosmic rays in compressible, partially ionised plasma
• Efficient implementation of the single-reference algebraic diagrammatic construction theory for charged excitations: Applications to the TEMPO radical and DNA base pairs
• An upper limit on [OIII] 88 $\mu$m and 1.2 mm continuum emission from a JWST $z\approx 12-13$ galaxy candidate with ALMA
• Unveiling the contribution of Pop III stars in primeval galaxies at redshift $\ge 6$
• The Masses of a Sample of Radial-Velocity Exoplanets with Astrometric Measurements
• Collisional evolution of dust and water ice in protoplanetary discs during and after an accretion outburst
• On the formation of massive quiescent galaxies with diverse morphologies in the TNG50 simulation
• Environment-assisted quantum transport and mobility edges
• A geometric modelling framework to support the design of heterogeneous lattice structures with non-linearly varying geometry
• Planet Engulfment Signatures in Twin Stars
• Truncated atomic plane wave method for the subband structure calculations of Moiré systems
• Deep Investigation of Neutral Gas Origins (DINGO): HI stacking experiments with early science data
• CMB lensing power spectrum estimation without instrument noise bias
• Stellar masses, sizes, and radial profiles for 465 nearby early-type galaxies: an extension to the Spitzer Survey of Stellar Structure in Galaxies (S${}^4$G)
• Broad-band selection, spectroscopic identification, and physical properties of a population of extreme emission line galaxies at 3<z<3.7
• AGN impact on the molecular gas in galactic centers as probed by CO lines
• Zapped then Napped? A rapidly quenched remnant leaker candidate with a steep spectroscopic ${\beta }_{UV}$ slope at z=8.5
• Explosion analysis from images: Trinity and Beirut
• A Spatially-Resolved Survey of Distant Quasar Host Galaxies: I. Dynamics of galactic outflows
• Lexically-Accelerated Dense Retrieval
• Halo Formation from Yukawa Forces in the Very Early Universe
• TESS Data for Asteroseismology (T'DA) Stellar Variability Classification Pipeline: Set-Up and Application to the Kepler Q9 Data
• Beyond runaway: initiation of the post-runaway greenhouse state on rocky exoplanets
• The Sloan Digital Sky Survey Reverberation Mapping Project: The M_BH-Host Relations at 0.2<z<0.6 from Reverberation Mapping and Hubble Space Telescope Imaging
• Dynamical Accretion Flows -- ALMAGAL: Flows along filamentary structures in high-mass star-forming clusters
• PPDONet: Deep Operator Networks for Fast Prediction of Steady-State Solutions in Disk-Planet Systems
• Weak damping of propagating MHD kink waves in the quiescent corona
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• The influence of the environment on the spin evolution of low-mass stars. I. External photoevaporation of circumstellar disks
• Direct $N$-body simulations of satellite formation around small asteroids: insights from DART's encounter with the Didymos system
• Orbital Torus Imaging: Using Element Abundances to Map Orbits and Mass in the Milky Way
• Evolution of CIV Absorbers I. The Cosmic Incidence
• Quality over Quantity: Optimizing pulsar timing array analysis for stochastic and continuous gravitational wave signals
• Probing the Shock Breakout Signal of SN 2024ggi from the Transformation of Early Flash Spectroscopy
• Geometry-Induced Dynamics of Confined Chiral Active Matter
• JWST Low-Resolution MIRI Spectral Observations of SN~2021aefx: High-density Burning in a Type Ia Supernova
• Electromagnetic precursor flares from the late inspiral of neutron star binaries
• The Simons Observatory: pipeline comparison and validation for large-scale B-modes
• Connecting the Light Curves of Type IIP Supernovae to the Properties of their Progenitors
• Single-Particle Mobility Edge without Disorder
• Electromagnetic precursors to black hole - neutron star gravitational wave events: Flares and reconnection-powered fast-radio transients from the late inspiral
• Testing Self-Organized Criticality Across the Main Sequence using Stellar Flares from TESS
• The SAGA Survey. IV. The Star Formation Properties of 101 Satellite Systems around Milky Way-mass Galaxies
• On the Co-Orbitation of Satellite Galaxies Along the Great Plane of Andromeda: NGC 147, NGC 185, and Expectations from Cosmological Simulations
• Exploring metallicity-dependent rates of Type Ia supernovae and their impact on galaxy formation
• Stellar halos from The Dragonfly Edge-on Galaxies Survey
• Gas Accretion Can Drive Turbulence in Galaxies
• The Atacama Cosmology Telescope: Summary of DR4 and DR5 Data Products and Data Access
• Testing Lorentz Invariance of Gravity in the Standard Model Extension with GWTC-3
• Satellite Optical Brightness
• Unifying High- and Low-resolution Observations to Constrain the Dayside Atmosphere of KELT-20b/MASCARA-2b
• Semi-analytical covariance matrices for two-point correlation function for DESI 2024 data
• System-level fractionation of carbon from disk and planetesimal processing
• Random Forests as a viable method to select and discover high redshift quasars
• H.E.S.S. follow-up observations of GRB221009A
• Massive binary black holes from Population II and III stars
• The NANOGrav 12.5-Year Data Set: Polarimetry and Faraday Rotation Measures from Observations of Millisecond Pulsars with the Green Bank Telescope
• Detection of period-spacing patterns due to the gravity modes of rotating dwarfs in the TESS southern continuous viewing zone
• KiDS-SBI: Simulation-based inference analysis of KiDS-1000 cosmic shear
• The perspective of voids on rising cosmology tensions
• Extension of HOPS Out to 500 ParSecs (eHOPS). I. Identification and Modeling of Protostars in the Aquila Molecular Clouds
• A fast radio burst localized at detection to an edge-on galaxy using very-long-baseline interferometry
• Optical/$\gamma$-ray blazar flare correlations: understanding the high-energy emission process using ASAS-SN and Fermi light curves
• The formation and early evolution of embedded star clusters in spiral galaxies
• Sustained FU Orionis-type outbursts from colliding discs in stellar flybys
• Ringdown amplitudes of nonspinning eccentric binaries
• CLEAR: High-Ionization [Ne V] $\lambda$3426 Emission-line Galaxies at $1.4<z<2.3$
• Globular cluster numbers in dark matter haloes in a dual formation scenario: an empirical model within EMERGE
• Pinpointing the jet apex of 3C 84
• CHEX-MATE: Robust reconstruction of temperature profiles in galaxy clusters with XMM-Newton
• The nuclear star cluster and nuclear stellar disc of the Milky Way: Different stellar population and star formation history
• TREXIO: A File Format and Library for Quantum Chemistry
• The Hough Stream Spotter: A New Method for Detecting Linear Structure in Resolved Stars and Application to the Stellar Halo of M31
• Single-Shot Readout of a Superconducting Qubit Using a Thermal Detector
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• Stirring the Base of the Solar Wind: On Heat Transfer and Vortex Formation
• A dynamics-based density profile for dark haloes -- II. Fitting function
• CREIME: A Convolutional Recurrent model for Earthquake Identification and Magnitude Estimation
• Parameterised population models of transient non-Gaussian noise in the LIGO gravitational-wave detectors
• Archetype-Based Redshift Estimation for the Dark Energy Spectroscopic Instrument Survey
• Inner Planetary System Gap Complexity is a Predictor of Outer Giant Planets
• Fast high-fidelity gates for galvanically-coupled fluxonium qubits using strong flux modulation
• The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). VI. The core-scale CO-depletion
• A cosmic stream of atomic carbon gas connected to a massive radio galaxy at redshift 3.8
• Examining the orbital decay targets KELT-9 b, KELT-16 b and WASP-4 b, and the transit-timing variations of HD 97658 b
• Reconnection-powered fast radio transients from coalescing neutron star binaries
• Aerosols are not Spherical Cows: Using Discrete Dipole Approximation to Model the Properties of Fractal Particles
• A pulsar wind nebula origin of the LHAASO-detected UHE gamma-ray sources
• Stellar Cycles in Fully Convective Stars and a New Interpretation of Dynamo Evolution
• Membership lists for 431 open clusters in Gaia DR2 using extreme deconvolution gaussian mixture models
• Resolving the eccentricity of stellar mass binary black holes with next generation ground-based gravitational wave detectors
• The GOGREEN survey: Dependence of galaxy properties on halo mass at z > 1 and implications for environmental quenching
• Model-based cross-correlation search for gravitational waves from the low-mass X-ray binary Scorpius X-1 in LIGO O3 data
• The Star-forming Main Sequence of the Host Galaxies of Low-redshift Quasars
• A morphology-independent test of the mixed polarization content of gravitational wave signals from compact binary coalescences
• Periodic Radio Emission from the T8 Dwarf WISE J062309.94-045624.6
• GaiaHub: A method for combining data from the Gaia and Hubble space telescopes to derive improved proper motions for faint stars
• Forming Iron-rich Planets with Giant Impacts
• Nonlinear 3D Cosmic Web Simulation with Heavy-Tailed Generative Adversarial Networks
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• HiFAST: an HI data calibration and imaging pipeline for FAST
• Understanding how fast black holes spin by analysing data from the second gravitational-wave catalogue
• Forward Modeling of Double Neutron Stars: Insights from Highly-Offset Short Gamma-Ray Bursts
• GW190521: tracing imprints of spin-precession on the most massive black hole binary
• Data Combination: Interferometry and Single-dish Imaging in Radio Astronomy
• An Infrared Search for Kilonovae with the WINTER Telescope. I. Binary Neutron Star Mergers
• Quokka: A code for two-moment AMR radiation hydrodynamics on GPUs
• Infrared Radiation Feedback Does Not Regulate Star Cluster Formation
• SDSS-IV MaNGA: Stellar M/L gradients and the M/L-colour relation in galaxies
• Solar Anti-Hale Bipolar Magnetic Regions: A Distinct Population with Systematic Properties
• Carbon-Enhanced Metal-Poor star candidates from BP/RP Spectra in $Gaia$ DR3
• Asteroseismology of the young open cluster NGC 2516 I: Photometric and spectroscopic observations
• A New Approach to Electroweak Symmetry Non-Restoration
• Eccentricity-induced systematic error on parametrized tests of general relativity: Hierarchical Bayesian inference applied to a binary black hole population
• Training Data Augmentation for Deep Learning Radio Frequency Systems
• Correcting correlation functions for redshift-dependent interloper contamination
• A biconical ionised gas outflow and evidence for positive feedback in NGC 7172 uncovered by MIRI/JWST
• Mass Transfer and Stellar Evolution of the White Dwarfs in AM CVn Binaries
• Detection of Intracluster Globular Clusters in the First JWST Images of the Gravitational Lens Cluster SMACS J0723.3-7327 at z = 0.39
• Survival of ALMA Rings in the Absence of Pressure Maxima
• TESS spots a mini-neptune interior to a hot saturn in the TOI-2000 system
• Earth System Data Cubes: Avenues for advancing Earth system research
• Constraining the Gravitational Potential from the Projected Morphology of Extragalactic Tidal Streams
• oMEGACat I: MUSE spectroscopy of 300,000 stars within the half-light radius of $\omega$ Centauri
• High-ionization emission line ratios from quasar broad line regions: metallicity or density?
• Plasmoid Instability in the Multiphase Interstellar Medium
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• Your: Your Unified Reader
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• The Detection of Transiting Exoplanets by Gaia
• The origin of the [CII]-deficit in a simulated dwarf galaxies starburst
• Weak evidence for variable occultation depth of 55 Cnc e with TESS
• The Dark World: A Tale of WASP-43b in Reflected Light with HST WFC3/UVIS
• Measuring eccentricity and gas-induced perturbation from gravitational waves of LISA massive black hole binaries
• The hot circumgalactic medium of the Milky-Way: new insights from XMM-Newton observations
• TOI-969: a late-K dwarf with a hot mini-Neptune in the desert and an eccentric cold Jupiter
• Chemical footprints of giant planet formation. Role of planet accretion in shaping the C/O ratio of protoplanetary disks
• CLASS: Coronal Line Activity Spectroscopic Survey
• Modelling Populations of Kilonovae
• The water-ice feature in near-infrared disk-scattered light around HD 142527: Micron-sized icy grains lifted up to the disk surface?
• Rapid determination of LISA sensitivity to extreme mass ratio inspirals with machine learning
• An Effective Bias Expansion for 21 cm Cosmology in Redshift Space
• PyQMC: an all-Python real-space quantum Monte Carlo module in PySCF
• A Systematic Exploration of Kilonova Candidates from Neutron Star Mergers During the Third Gravitational Wave Observing Run
• Probing the speed of gravity with LVK, LISA, and joint observations
• First Light And Reionisation Epoch Simulations (FLARES) VI: The colour evolution of galaxies $z=5-15$
• The effect of interior heat flux on the atmospheric circulation of hot and ultra-hot Jupiters
• The influence of host star activity evolution on the population of super-Earths and mini-Neptunes
• Orbital alignment of the eccentric warm Jupiter TOI-677 b
• Angular momentum evolution can be predicted from cosmological initial conditions
• Transition to turbulence in nonuniform coronal loops driven by torsional Alfven waves
• An ALMA Gas-dynamical Mass Measurement of the Supermassive Black Hole in the Local Compact Galaxy UGC 2698
• Constraining the mass and redshift evolution of the hydrostatic mass bias using the gas mass fraction in galaxy clusters
• A cosmic-ray database update: CRDB v4.1
• ZELDA: fitting Lyman-alpha line profiles using deep learning
• A Bayesian estimation of the Milky Way's circular velocity curve using Gaia DR3
• Observing planet-driven dust spirals with ALMA
• Semi-regular red giants as distance indicators I. The period-luminosity relations of semi-regular variables revisited
• CosmoFlow: Python Package for Cosmological Correlators
• A Pilot Study of Nulling in 22 Pulsars Using Mixture Modeling
• TOI-1859b: A 64-Day Warm Jupiter on an Eccentric and Misaligned Orbit
• ThERESA: Three-Dimensional Eclipse Mapping with Application to Synthetic JWST Data
• Simulated performance of the molecular mapping for young giant exoplanets with the Medium Resolution Spectrometer of JWST/MIRI
• General relativistic hydrodynamic simulations of perturbed transonic accretion
• Stellar Parameters and Chemical Abundances Estimated from LAMOST-II DR8 MRS based on Cycle-StarNet
• Using the Gaia excess uncertainty as a proxy for stellar variability and age
• ALMA observations of the Extended Green Object G19.01$-$0.03: I. A Keplerian disc in a massive protostellar system
• Investigating the impact of vertically extended coronae on X-ray reverberation mapping
• Empirical quantification of predictive uncertainty due to model discrepancy by training with an ensemble of experimental designs: an application to ion channel kinetics
• Discovery of PSR J0523-7125 as a Circularly Polarized Variable Radio Source in the Large Magellanic Cloud
• Deciphering stellar chorus: apollinaire, a Python 3 module for Bayesian peakbagging in helio- and asteroseismology
• High-frequency wave power observed in the solar chromosphere with IBIS and ALMA
• ALP dark matter with non-periodic potentials: parametric resonance, halo formation and gravitational signatures
• GLoW: novel methods for wave-optics phenomena in gravitational lensing
• The new magnetar SGR J1830-0645 in outburst
• A kinematic study of central compact objects and their host supernova remnants
• Constraints on Cosmological Parameters with a Sample of Type Ia Supernovae from JWST
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• An Elusive Population of Massive Disk Galaxies Hosting Double-lobed Radio-loud AGNs
• Data Leakage and Evaluation Issues in Micro-Expression Analysis
• Reading the tea leaves in the $M_{\mathrm{bh}}$-$M_{\ast ,\mathrm{sph}}$ and $M_{\mathrm{bh}}$-$R_{\mathrm{e},\mathrm{sph}}$ diagrams: dry and gaseous mergers with remnant angular momentum
• Stellar Spins in the Pleiades, Praesepe, and M35 Open Clusters
• The dynamic centres of infrared-dark clouds and the formation of cores
• New Observations of the Eclipsing Binary System NY Vir and its Candidate Circumbinary Planets
• Far-Ultraviolet Spectra of Main-Sequence O Stars at Extremely Low Metallicity
• Coronal mass ejections and type II radio emission variability during a magnetic cycle on the solar-type star $\epsilon$ Eridani
• Many Roads Lead to Lithium: Formation Pathways For Lithium-Rich Red Giants
• Potential of the Julia programming language for high energy physics computing
• Boundary Layer Circumplanetary Accretion: How Fast Could an Unmagnetized Planet Spin Up Through Its Disk?
• The SRG/eROSITA All-Sky Survey: Constraints on AGN Feedback in Galaxy Groups
• Evidence of a Decreased Binary Fraction for Massive Stars Within 20 Milliparsecs of the Supermassive Black Hole at the Galactic Center
• The Dependence of the Hierarchical Distribution of Star Clusters on Galactic Environment
• Beyond the Local Volume. I. Surface Densities of Ultracool Dwarfs in Deep HST/WFC3 Parallel Fields
• Comparative Analysis of TRGBs (CATs) from Unsupervised, Multi-Halo-Field Measurements: Contrast is Key
• ASKAP observations of multiple rapid scintillators reveal a degrees-long plasma filament
• Gauge preheating with full general relativity
• Stellar multiplicity affects the correlation between proto-planetary disc masses and accretion rates: binaries explain high-accretors in Upper Sco
• Possible Ribose Synthesis in Carbonaceous Planetesimals
• Characterisation of 92 Southern TESS Candidate Planet Hosts and a New Photometric [Fe/H] Relation for Cool Dwarfs
• SPA${}^{\mathrm{H}}$M: the Spectrum of Approximated Hamiltonian Matrices representations
• Characterization of hot populations of Melotte 66 open cluster using Swift/UVOT
• Characterization of a set of small planets with TESS and CHEOPS and an analysis of photometric performance
• Efficiently Imaging Accreting Protoplanets from Space: Reference Star Differential Imaging of the PDS 70 Planetary System using the HST/WFC3 Archival PSF Library
• Photon shot-noise limited transient absorption soft X-ray spectroscopy at the European XFEL
• Plaskett 1.8 metre Observations of Starlink Satellites
• oMEGACat III. Multi-band photometry and metallicities reveal spatially well-mixed populations within $\omega$ Centauri's half-light radius
• Starspots Modelling and Flare Analysis on Selected MV Stars
• Slumping regime in lock-release turbidity currents
• EDGE: The emergence of dwarf galaxy scaling relations from cosmological radiation-hydrodynamics simulations
• Did the Milky Way just light up? The recent star formation history of the Galactic disc
• Detecting low-mass haloes with strong gravitational lensing II: constraints on the density profiles of two detected subhaloes
• Assembly of the Intracluster Light in the Horizon-AGN Simulation
• The Role of Adaptive Ray Tracing in Analyzing Black Hole Structure
• Determination of dynamical ages of open clusters through the A${}^{+}$ parameter -- I
• Constraints on Moon's orbit 3.2 billion years ago from tidal bundle data
• AGN-driven Cold Gas Outflow of NGC 1068 Characterized by Dissociation-Sensitive Molecules
• Gravitational Waves from Black-Hole Encounters: Prospects for Ground- and Galaxy-Based Observatories
• A Method To Characterize the Wide-Angle Point Spread Function of Astronomical Images
• The Effect of Dark Matter Halo Shape on Bar Buckling and Boxy/Peanut Bulges
• Barium stars as tracers of s-process nucleosynthesis in AGB stars II. Using machine learning techniques on 169 stars
• Tree boosting for learning EFT parameters
• A Lensing-Band Approach to Spacetime Constraints
• A Comparison of the Baryonic Tully-Fisher Relation in MaNGA and IllustrisTNG
• PHANGS-JWST First Results: Spurring on Star Formation: JWST Reveals Localised Star Formation in a Spiral Arm Spur of NGC 628
• Accretion rates in hierarchical triple systems with discs
• MINDS: The very low-mass star and brown dwarf sample -- Hidden water in carbon-dominated protoplanetary disks
• Surrogate modelling the Baryonic Universe II: on forward modelling the colours of individual and populations of galaxies
• Inferring host-galaxy properties of LIGO-Virgo-KAGRA's black holes
• HyperPCA: a Powerful Tool to Extract Elemental Maps from Noisy Data Obtained in LIBS Mapping of Materials
• AMICO galaxy clusters in KiDS-DR3: Measurement of the halo bias and power spectrum normalization from a stacked weak lensing analysis
• Frequentist versus Bayesian analyses: Cross-correlation as an (approximate) sufficient statistic for LIGO-Virgo stochastic background searches
• Photometric detection of internal gravity waves in upper main-sequence stars. III. Comparison of amplitude spectrum fitting and Gaussian process regression using celerite2
• ALMA/ACA CO Survey of the IC 1459 and NGC 4636 Groups: Environmental Effects on the Molecular Gas of Group Galaxies
• Modeling chemistry during star formation: Water deuteration in dynamic star-forming regions
• First Observations of the Brown Dwarf HD 19467 B with JWST
• Probing atmospheric escape through metastable He I triplet lines in 15 exoplanets observed with SPIRou
• The density distribution and physical origins of intermittency in supersonic, highly magnetised turbulence with diverse modes of driving
• Milky Way archaeology using RR Lyrae and type II Cepheids I. The Orphan stream in 7D using RR Lyrae stars
• EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies
• Mass-accretion, spectral, and photometric properties of T Tauri stars in Taurus based on TESS and LAMOST
• HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules -- I. Survey description and a first look toward W3(OH), W3 IRS5 and NGC 7538 IRS1
• Preparing to discover the unknown with Rubin LSST -- I: Time domain
• Galactic gamma-ray and neutrino emission from interacting cosmic-ray nuclei
• A jolt to the system: ram pressure on low-mass galaxies in simulations of the Local Group
• Mining S-PLUS for Metal-Poor Stars in the Milky Way
• A Lack of Variability Between Repeated Spitzer Phase Curves of WASP-43b
• Quantum AI simulator using a hybrid CPU-FPGA approach
• Massive galaxy formation caught in action at z~5 with JWST
• Disentangling Multiple Stochastic Gravitational Wave Background Sources in PTA Datasets
• The multifarious ionization sources and disturbed kinematics of extraplanar gas in five low-mass galaxies
• Constraints on parity and Lorentz violations in gravity from GWTC-3 through a parametrization of modified gravitational wave propagations
• The Cosmic Dispersion Measure in the EAGLE Simulations
• Exploring Proxies for the Supermassive Black Hole Mass Function: Implications for Pulsar Timing Arrays
• SN2017jgh - A high-cadence complete shock cooling lightcurve of a SN IIb with the Kepler telescope
• On the formation of solar wind & switchbacks, and quiet Sun heating
• The BINGO Project IV: Simulations for mission performance assessment and preliminary component separation steps
• Hot Rocks Survey III: A deep eclipse for LHS 1140c and a new Gaussian process method to account for correlated noise in individual pixels
• A Pseudo-Two-Dimensional (P2D) Model for FeS2 Conversion Cathode Batteries
• Chemical signatures of a warped protoplanetary disc
• The Response of Dark Matter Haloes to Gas Ejection: CuspCore II
• A 3D View of Orion: I. Barnard's Loop
• Constraining Reionization in Progress at z=5.7 with Lyman-$\alpha$ Emitters: Voids, Peaks, and Cosmic Variance
• The Time-Dependent Distribution of Optical Polarization Angle Changes in Blazars
• Stirred but not shaken: a multi-wavelength view of HD 16743's debris disc
• Decoding the compositions of four bright $r$-process-enhanced stars
• SN 2018gj: A Short-plateau Type II Supernova with Persistent Blue-shifted H-alpha Emission
• Variational quantum dynamics of two-dimensional rotor models
• VLA resolves unexpected radio structures in the Perseus cluster of galaxies
• Yang-Mills glueball masses from spectral reconstruction
• Differential Modelling Systematics across the HR Diagram from Asteroseismic Surface Corrections
• $\nu$DoBe -- A Python Tool for Neutrinoless Double Beta Decay
• The MUSE Ultra Deep Field (MUDF). III. Hubble Space Telescope WFC3 Grism Spectroscopy and Imaging
• Optimized pulsed sideband cooling and enhanced thermometry of trapped ions
• COMAP Early Science: VI. A First Look at the COMAP Galactic Plane Survey
• An absolute calibration of the near-infrared Period-Luminosity Relations of Type II Cepheids in the Milky Way and in the Large Magellanic Cloud
• Constraints on the (re-)orientation of star-disk systems through infall
• Inhomogeneous phases in the chirally imbalanced $2+1$-dimensional Gross-Neveu model and their absence in the continuum limit
• Multiwavelength Analysis of A1240, the Double Radio Relic Merging Galaxy Cluster Embedded in a ~80 Mpc-long Cosmic Filament
• JWST sighting of decameter main-belt asteroids and view on meteorite sources
• Extending relax-and-round combinatorial optimization solvers with quantum correlations
• PRAiSE: Resolved spectral evolution in simulated radio sources
• Computing Tools for Effective Field Theories
• Galactic winds and bubbles from nuclear starburst rings
• Identifying Host Galaxies of Supermassive Black Hole Binaries Found by PTAs
• The MeerKAT Pulsar Timing Array: Maps of the gravitational-wave sky with the 4.5 year data release
• The matter density PDF for modified gravity and dark energy with Large Deviations Theory
• Photometric and Structural Parameters of Newly Discovered Nuclear Star Clusters in Local Volume Galaxies
• Streamlined Lensed Quasar Identification in Multiband Images via Ensemble Networks
• An Integrated Analysis with Predictions on the Architecture of the tau Ceti Planetary System, Including a Habitable Zone Planet
• The minimum measurable eccentricity from gravitational waves of LISA massive black hole binaries
• The Milky Way as Seen by Classical Cepheids II: Spiral Structure
• Salt-bearing disk candidates around high-mass young stellar objects
• The dark side of FIRE: predicting the population of dark matter subhaloes around Milky Way-mass galaxies
• Towards realistic statistical models of the grid frequency
• The NANOGrav 15 yr Data Set: Looking for Signs of Discreteness in the Gravitational-wave Background
• Understanding binary neutron star collisions with hypermodels
• Numerical Challenges in Modeling Gravothermal Collapse in Self-Interacting Dark Matter Halos
• Disc cloaking: Establishing a lower limit to the number density of local compact massive spheroids/bulges and the potential fate of some high-z red nuggets
• Revisiting Rotation Measures from the Canadian Galactic Plane Survey: the Magnetic Field in the Disk of the Outer Galaxy
• The SRG/eROSITA diffuse soft X-ray background. I. The local hot bubble in the western Galactic hemisphere
• Dynamics of baryon ejection in magnetar giant flares: implications for radio afterglows, r-process nucleosynthesis, and fast radio bursts
• Quasar Factor Analysis -- An Unsupervised and Probabilistic Quasar Continuum Prediction Algorithm with Latent Factor Analysis
• The Spin-Orbit Misalignment of TOI-1842b: The First Measurement of the Rossiter-McLaughlin Effect for a Warm Sub-Saturn around a Massive Star
• Quantifying uncertainties in general relativistic magnetohydrodynamic codes
• The impact of selection biases on tests of general relativity with gravitational-wave inspirals
• Unified field theoretical approach to deep and recurrent neuronal networks
• Phase Retrieval and Design with Automatic Differentiation
• Resonant and Ultra-short-period Planet Systems are at Opposite Ends of the Exoplanet Age Distribution
• A portrait of the Vast Polar Structure as a young phenomenon: hints from its member satellites
• Differentiable Cosmological Simulation with Adjoint Method
• Shocking Sgr B2(N1) with its own outflow: A new perspective on segregation between O- and N-bearing molecules
• Alternative Methylated Biosignatures I: Methyl Bromide, A Capstone Biosignature
• Revealing the Field Sub-subgiant Population Using a Catalog of Active Giant Stars and Gaia EDR3
• Ubiquitous [OII] Emission in Quiescent Galaxies at z ~ 0.85
• Pulsating B stars in the Scorpius-Centaurus Association with TESS
• oMEGACat II -- Photometry and proper motions for 1.4 million stars in Omega Centauri and its rotation in the plane of the sky
• Hydrodynamics and survivability during post-main-sequence planetary engulfment
• Analysis of a Tau Neutrino Origin for the Near-Horizon Air Shower Events Observed by the Fourth Flight of the Antarctic Impulsive Transient Antenna (ANITA)
• Strategies for optimal sky subtraction in the low surface brightness regime
• Improved particle spray algorithm for modeling globular cluster streams
• A Dearth of Close-In Stellar Companions to M-dwarf TESS Objects of Interest
• Using the Sun to Measure the Primary Beam Response of the Canadian Hydrogen Intensity Mapping Experiment
• Characterising Tidal Features Around Galaxies in Cosmological Simulations
• The GRAVITY young stellar object survey -- XI. Probing the inner disk and magnetospheric accretion region of CI Tau
• Measuring ${\sigma }_8$ using DESI Legacy Imaging Surveys Emission-Line Galaxies and Planck CMB Lensing and the Impact of Dust on Parameter Inference
• PlatoSim: An end-to-end PLATO camera simulator for modelling high-precision space-based photometry
• An Isotropy Measurement with Gravitational Wave Observations
• Revisiting Radial Velocity Measurements of the K2-18 System with the Line-by-Line Framework
• Zwicky Transient Facility and Globular Clusters: The Period-Luminosity and Period-Wesenheit Relations for Type II Cepheids
• A new method to measure the spectra of transiting exoplanet atmospheres using multi-object spectroscopy
• Applications of Machine Learning to Detecting Fast Neutrino Flavor Instabilities in Core-Collapse Supernova and Neutron Star Merger Models
• Stellar Characterization and Radius Inflation of Hyades M Dwarf Stars From the APOGEE Survey
• Flashlights: An Off-Caustic Lensed Star at Redshift $z$ = 1.26 in Abell 370
• Impact of climate change on site characteristics of eight major astronomical observatories using high-resolution global climate projections until 2050
• Using Equation of State Constraints to Classify Low-Mass Compact Binary Mergers
• The large-scale 21-cm power spectrum from reionization
• Deep exploration for continuous gravitational waves at 171--172 Hz in LIGO second observing run data
• QUIJOTE scientific results -- VIII. Diffuse polarized foregrounds from component separation with QUIJOTE-MFI
• Photometric identification of compact galaxies, stars and quasars using multiple neural networks
• Optimization of the resonator-induced phase gate for superconducting qubits
• Mixed Modes and Asteroseismic Surface Effects: I. Analytic Treatment
• Gaussian RBF Centered Kernel Alignment (CKA) in the Large Bandwidth Limit
• Stellar Chromospheric Activity Database of Solar-like Stars Based on the LAMOST Low-Resolution Spectroscopic Survey
• The Influence of 10 Unique Chemical Elements in Shaping the Distribution of Kepler Planets
• Efficient Gravitational Wave Template Bank Generation with Differentiable Waveforms
• The Alcock-Paczyński effect from Lyman-$\alpha$ forest correlations: Analysis validation with synthetic data
• Mapping the "invisible" circumgalactic medium around a z $\sim$ 4.5 radio galaxy with MUSE
• Astraeus VI: Hierarchical assembly of AGN and their large-scale effect during the Epoch of Reionization
• Placing LOFAR-detected quasars in CIV emission space: implications for winds, jets and star formation
• The hot Neptune WASP-166 b with ESPRESSO III: A blue-shifted tentative water signal constrains the presence of clouds
• Induced earthquake source parameters, attenuation, and site effects from waveform envelopes in the Fennoscandian Shield
• Probing the large scale structure using gravitational-wave observations of binary black holes
• The Obscured Fraction of Quasars at Cosmic Noon
• BNNpriors: A library for Bayesian neural network inference with different prior distributions
• Discovery of a red backsplash galaxy candidate near M81
• One never walks alone: the effect of the perturber population on subhalo measurements in strong gravitational lenses
• TOI-4010: A System of Three Large Short-Period Planets With a Massive Long-Period Companion
• Effects of Multiphase Gas and Projection on X-ray Observables in Simulated Galaxy Clusters as Seen by eROSITA
• Where Outflows Meet Inflows: Gas Kinematics in SSA22 Lyman-$\alpha$ Blob 2 Decoded by Advanced Radiative Transfer Modelling
• Tracking Superharmonic Resonances for Nonlinear Vibration of Conservative and Hysteretic Single Degree of Freedom Systems
• Discovery of correlated evolution in solar noise storm source parameters: Insights on magnetic field dynamics during a microflare
• Nonperturbative structure in coupled axion sectors and implications for direct detection
• The ASAS-SN Bright Supernova Catalog -- V. 2018-2020
• High Resolution HST Imaging Survey of Local Star-Forming Galaxies I: Spatially-Resolved Obscured Star Formation with H$\alpha$ and Paschen-$\beta$ Recombination Lines
• Numerical challenges for energy conservation in N-body simulations of collapsing self-interacting dark matter halos
• Velocity Distribution of Dark Matter Spike around Schwarzschild Black Holes and Effects on Gravitational Waves from EMRIs
• Data Compression and Inference in Cosmology with Self-Supervised Machine Learning
• Direct-collapse supermassive black holes from relic particle decay
• Universal non-Debye low-frequency vibrations in sheared amorphous solids
• High-resolution atmospheric retrievals of WASP-76b transmission spectroscopy with ESPRESSO: Monitoring limb asymmetries across multiple transits
• Height-averaged Navier-Stokes solver for hydrodynamic lubrication
• JWST-TST High Contrast: JWST/NIRCam observations of the young giant planet $\beta$ Pic b
• Calibrating angular momentum transport in intermediate-mass stars from gravity-mode asteroseismology
• Relativistic corrections for measuring Hubble's constant to 1% using stellar standard candles
• A Near-infrared Variability Survey of Young Planetary-mass Objects
• A detailed look at the thermal and non-thermal X-ray emission from the Vela supernova remnant with SRG/eROSITA
• A weakly-parametric approach to stochastic background inference in LISA
• The HETDEX Survey: The Ly$\alpha$ Escape Fraction from 3D-HST Emission Line Galaxies at $z\sim 2$
• Unveiling Microlensing Biases in Testing General Relativity with Gravitational Waves
• The Galactic neutron star population I - an extragalactic view of the Milky Way and the implications for fast radio bursts
• The Variable Detection of Atmospheric Escape around the young, Hot Neptune AU Mic b
• Hypercubes of AGN Tori (HYPERCAT) -- I. Models and Image Morphology
• Exploring the possibility of Peter Pan discs across stellar mass
• Rotation and Abundances of the Benchmark Brown Dwarf HD 33632 Ab from Keck/KPIC High-resolution Spectroscopy
• Determination of small-scale magnetic fields on Sun-like stars in the near-infrared using CRIRES${}^{+}$
• Forest Fire Clustering for Single-cell Sequencing with Iterative Label Propagation and Parallelized Monte Carlo Simulation
• Gamma-ray detection of newly discovered Ancora SNR: G288.8-6.3
• Characterising coronal turbulence using snapshot imaging of radio bursts in 80-200 MHz
• Effects on the local dark matter distribution due to the Large Magellanic Cloud
• Dynamical generation of chiral $W$ and Greenberger-Horne-Zeilinger states in laser-controlled Rydberg-atom trimers
• MIGHTEE-HI: deep spectral line observations of the COSMOS field
• Kinematic analysis of the super-extended HI disk of the nearby spiral galaxy M83
• INSPIRE: INvestigating Stellar Population In RElics IV. The Initial Mass Function slope in relics
• MR. Estimator, a toolbox to determine intrinsic timescales from subsampled spiking activity
• Exploring the interaction between the MW and LMC with a large sample of blue horizontal branch stars from the DESI survey
• Evidence of an age gradient along the line of sight in the nuclear stellar disc of the Milky Way
• Search range in experimental quantum annealing
• Machine Learning Automated Approach for Enormous Synchrotron X-Ray Diffraction Data Interpretation
• A CHEOPS White Dwarf Transit Search
• The C-Band All-Sky Survey (C-BASS): Template Fitting of Diffuse Galactic Microwave Emission in the Northern Sky
• Linear Viscoelastic Response of the Vertex Model with Internal and External Dissipation: Normal Modes Analysis
• Runaway and Hypervelocity Stars from Compact Object Encounters in Globular Clusters
• Flares, Rotation, Activity Cycles and a Magnetic Star-Planet Interaction Hypothesis for the Far Ultraviolet Emission of GJ 436
• The role of baryons in self-interacting dark matter mergers
• TDCOSMO. XVI. Measurement of the Hubble Constant from the Lensed Quasar WGD2038$-$4008
• Tidally Tilted Pulsations in HD 265435, a subdwarf B Star with a Close White Dwarf Companion
• New insights into the rotational evolution of near-solar age stars from the open cluster M67
• The Triggerless Data Acquisition System of the XENONnT Experiment
• Multiple shock fronts in RBS 797: the Chandra window on shock heating in galaxy clusters
• Quantum advantage for differential equation analysis
• Sufficiency of a Gaussian power spectrum likelihood for accurate cosmology from upcoming weak lensing surveys
• Calibration of Transition-edge Sensor (TES) Bolometer Arrays with Application to CLASS
• Quantum chemical roots of machine-learning molecular similarity descriptors
• Joint reconstruction and segmentation of noisy velocity images as an inverse Navier-Stokes problem
• Fast and realistic large-scale structure from machine-learning-augmented random field simulations
• The impact of extragalactic foregrounds on internal delensing of CMB B-mode polarization
• Evolution of AM CVn binaries with WD donors
• Multiwavelength Vertical Structure in the AU Mic Debris Disk: Characterizing the Collisional Cascade
• Stellar winds and photoionization in a spiral arm
• A Composite Likelihood Approach for Inference under Photometric Redshift Uncertainty
• Kinematic Structure of the Large Magellanic Cloud Globular Cluster System from Gaia eDR3 and Hubble Space Telescope Proper Motions
• Non-ideal MHD simulations of subcritical prestellar cores with non-equilibrium chemistry
• LLWP -- A new Loomis-Wood Software at the Example of Acetone-13C1
• An old, metal-rich accreted stellar component in the Milky Way stellar disk
• Direct-imaging Discovery of a Substellar Companion Orbiting the Accelerating Variable Star, HIP 39017
• An Empirical Calibration of the Tip of the Red Giant Branch Distance Method in the Near Infrared. I. HST WFC3/IR F110W and F160W Filters
• Realistic synthetic integral field spectroscopy with RealSim-IFS
• Instrumental systematics biases in CMB lensing reconstruction: a simulation-based assessment
• Stellar angular momentum can be controlled from cosmological initial conditions
• Physics-informed compressed sensing for PC-MRI: an inverse Navier-Stokes problem
• Extragalactic Peaked-Spectrum Radio Sources at Low-Frequencies are Young Radio Galaxies
• Eruption of the Envelope of Massive Stars by Energy Injection with Finite Duration
• Migratory Outbursting Quasi-Hilda Object 282P/(323137) 2003 BM80
• enpheeph: A Fault Injection Framework for Spiking and Compressed Deep Neural Networks
• Lack-of-correlation anomaly in CMB large scale polarisation maps
• The Local Group's mass: probably no more than the sum of its parts
• Characterization of the variability in the O+B eclipsing binary HD 165246
• Data-driven equation for drug-membrane permeability across drugs and membranes
• Analytical Weak-lensing Shear Responses of Galaxy Properties and Galaxy Detection
• Analyzing black-hole ringdowns II: data conditioning
• MaNGA galaxy properties -- II. A detailed comparison of observed and simulated spiral galaxy scaling relations
• The SRG-eROSITA All-Sky Survey : Constraints on f(R) Gravity from Cluster Abundance
• A Spectroscopic Analysis of the California-Kepler Survey Sample: II. Correlations of Stellar Metallicities with Planetary Architectures
• HOLISMOKES -- IX. Neural network inference of strong-lens parameters and uncertainties from ground-based images
• Complex angular structure of three elliptical galaxies from high-resolution ALMA observations of strong gravitational lenses
• Lyα Halos around [O III]-Selected Galaxies in HETDEX
• The Galactic Underworld: The spatial distribution of compact remnants
• Exploring the Redshift-Space Peculiar Velocity Field and its Power Spectrum
• Early Planet Formation in Embedded Disks (eDisk) IX: High-resolution ALMA Observations of the Class 0 Protostar R CrA IRS5N and its surrounding
• X-Ray Constraints on Dark Photon Tridents
• Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey: I. Evidence for thermal energy anisotropy using oriented stacking
• High-resolution Emission Spectroscopy of the Ultrahot Jupiter KELT-9b: Little Variation in Day- and Nightside Emission Line Contrasts
• Signatures of Black Hole Spin and Plasma Acceleration in Jet Polarimetry
• Exploring the evolution of gravitational-wave emitters with efficient emulation: Constraining the origins of binary black holes using normalising flows
• LIGO-Virgo-KAGRA's Oldest Black Holes: Probing star formation at cosmic noon with GWTC-3
• Magnetically Arrested Circumbinary Accretion Flows
• Significant Molecular Gas Deficiencies in Star-forming Cluster Galaxies at $z\sim 1.4$
• Deep multi-task mining Calabi-Yau four-folds
• Sizing from the Smallest Scales: The Mass of the Milky Way
• Reconstruction Attack on Differential Private Trajectory Protection Mechanisms
• CHIPS: Complete History of Interaction-Powered Supernovae
• Compact Binary Coalescences in Dense Gaseous Environments Can Pose as ones in Vacuum
• Identify Light-Curve Signals with Deep Learning Based Object Detection Algorithm. I. Transit Detection
• Self-Interacting Dark Matter, Core Collapse and the Galaxy-Galaxy Strong Lensing Discrepancy
• Pulsar Timing Arrays require hierarchical models
• Enhancing ReaxFF for Molecular Dynamics Simulations of Lithium-Ion Batteries: An interactive reparameterization protocol
• A High Precision Survey of the D/H Ratio in the Nearby Interstellar Medium
• Learning to do multiframe wavefront sensing unsupervisedly: applications to blind deconvolution
• Precession and polar alignment of accretion discs in triple (or multiple) stellar systems
• Charactering instrumental noises and stochastic gravitational wave signals from combined time-delay interferometry
• Evidence for Variable Accretion onto PDS 70 c and Implications for Protoplanet Detections
• TeNeS: Tensor Network Solver for Quantum Lattice Systems
• Needle in a Bayes Stack: a Hierarchical Bayesian Method for Constraining the Neutron Star Equation of State with an Ensemble of Binary Neutron Star Post-merger Remnants
• Discovery of Super-Slow Rotating Asteroids with ATLAS and ZTF photometry
• Predicting the Timing of the the Solar Cycle 25 Polar Field Reversal
• Constraints on UHECR sources and extragalactic magnetic fields from directional anisotropies
• Outflow densities and ionisation mechanisms in the NLRs of the prototypical Seyfert galaxies NGC 1068 and NGC 4151
• Revisiting the [C II]${}_{158\mu \text{m}}$ line-intensity mapping power spectrum from the EoR using non-uniform line-luminosity scatter
• jVMC: Versatile and performant variational Monte Carlo leveraging automated differentiation and GPU acceleration
• Chemical evolution of local post-starburst galaxies: Implications for the mass-metallicity relation
• The SRG/eROSITA All-Sky Survey : Constraints on the structure growth from cluster number counts
• The MEGARA view of outflows in LINERs
• A search for radio afterglows from gamma-ray bursts with the Australian Square Kilometre Array Pathfinder
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• McFacts III: Compact binary mergers from AGN disks over an entire synthetic universe
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• Insights into the reionization epoch from cosmic-noon-CIV emitters in the VANDELS survey
• Atmosphere Loss in Oblique Super-Earth Impacts
• Characterizing the Circumgalactic Medium of the Lowest-Mass Galaxies: A Case Study of IC 1613
• Fast estimation of aperture mass statistics II: Detectability of higher order statistics in current and future surveys
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• Stellar proper motions in the outskirts of classical dwarf spheroidal galaxies with Gaia EDR3
• Rethinking data-driven point spread function modeling with a differentiable optical model
• It's a Breeze: The Circumgalactic Medium of a Dwarf Galaxy is Easy to Strip
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• The MAVERIC Survey: Variable Jet-Accretion Coupling in Luminous Accreting Neutron Stars in Galactic Globular Clusters
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• The SRG/eROSITA All-Sky Survey: Weak-Lensing of eRASS1 Galaxy Clusters in KiDS-1000 and Consistency Checks with DES Y3 & HSC-Y3
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• RABBITS -- I. The crucial role of nuclear star formation in driving the coalescence of supermassive black hole binaries
• Molecular Flows in Contemporary Active Galaxies and the Efficacy of Radio-Mechanical Feedback
• Eccentric Minidisks in Accreting Binaries
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• EDGE-INFERNO: Simulating every observable star in faint dwarf galaxies and their consequences for resolved-star photometric surveys
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• PHANGS-JWST First Results: A combined HST and JWST analysis of the nuclear star cluster in NGC 628
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• Interrelation of the environment of Ly$\alpha$ emitters and massive galaxies at $2<z<4.5$
• COOL-LAMPS III: Discovery of a 25".9 Separation Quasar Lensed by a Merging Galaxy Cluster
• Mixed-precision explicit stabilized Runge-Kutta methods for single- and multi-scale differential equations
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• On the detectability of strong lensing in near-infrared surveys
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• Resolving the Hot Dust Disk of ESO323-G77
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• Q${}^2$Chemistry: A quantum computation platform for quantum chemistry
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• The POKEMON Speckle Survey of Nearby M Dwarfs. I. New Discoveries
• The Maximum Mass-Loss Efficiency for a Photoionization-Driven Isothermal Parker Wind
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• The Tiered Radio Extragalactic Continuum (T-RECS) simulation II: HI emission and continuum-HI cross-correlation
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• The Linear Algebra Mapping Problem. Current state of linear algebra languages and libraries
• Late-time X-ray Observations of the Jetted Tidal Disruption Event AT2022cmc: The Relativistic Jet Shuts Off
• Spin Doctors: How to diagnose a hierarchical merger origin
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• The ALMA Survey of Gas Evolution of PROtoplanetary Disks (AGE-PRO): VIII. The impact of external photoevaporation on disk masses and radii in Upper Scorpius
• Modeling kilonova afterglows: Effects of the thermal electron population and interaction with GRB outflows
• AIRI: Predicting Retention Indices and their Uncertainties using Artificial Intelligence
• Entrainment of Hot Gas into Cold Streams: The Origin of Excessive Star-formation Rates at Cosmic Noon
• SUNRISE: The rich molecular inventory of high-redshift dusty galaxies revealed by broadband spectral line surveys
• MUSEQuBES: The relation between Ly$\alpha$ emitters and C IV absorbers at $z\approx 3.3$
• Cosmology from the integrated shear 3-point correlation function: simulated likelihood analyses with machine-learning emulators
• Local models of two-temperature accretion disc coronae. I. Structure, outflows, and energetics
• Spatio-temporal complexity of power-grid frequency fluctuations
• The Gaia-ESO Survey: Preparing the ground for 4MOST & WEAVE galactic surveys. Chemical evolution of lithium with machine learning
• Iterative Angular Differential Imaging (IADI): An exploration of recovering disk structures in scattered light with an iterative ADI approach
• Polarised emission from aligned dust grains in nearby galaxies: predictions from the Auriga simulations
• From molecular to multi-asperity contacts: how roughness bridges the friction scale gap
• The MAVERIC Survey: Simultaneous Chandra and VLA observations of the transitional millisecond pulsar candidate NGC 6652B
• Fishing for Planets: A Comparative Analysis of EPRV Survey Performance in the Presence of Correlated Noise
• The physical properties of Cluster Chains
• UVIT observations of the Small Magellanic Cloud: Point source catalogue
• Physical Parameters and Properties of 20 Cold Brown Dwarfs in JWST
• On the use of temporal filtering for mitigating galactic synchrotron calibration bias in 21 cm reionization observations
• Tidal disruption of star clusters in galaxy formation simulations
• Feature Guided Training and Rotational Standardisation for the Morphological Classification of Radio Galaxies
• A roadmap to cosmological parameter analysis with third-order shear statistics III: Efficient estimation of third-order shear correlation functions and an application to the KiDS-1000 data
• The Gaia-ESO Survey: Old super-metal-rich visitors from the inner Galaxy
• A Tale of a Tail: A Tidally-Disrupting Ultra-Diffuse Galaxy in the M81 Group
• Quantification of high dimensional non-Gaussianities and its implication to Fisher analysis in cosmology
• The diversity of spiral galaxies explained
• The Influence of Muons, Pions, and Trapped Neutrinos on Neutron Star Mergers
• Effects of Emerging Bipolar Magnetic Regions in Mean-field Dynamo Model of Solar Cycles 23 and 24
• Static Energy in ($2+1+1$)-Flavor Lattice QCD: Scale Setting and Charm Effects
• WASP-121b's transmission spectrum observed with JWST/NIRSpec G395H reveals thermal dissociation and SiO in the atmosphere
• Kernel Phase and Coronagraphy with Automatic Differentiation
• CLASS Survey Description: Coronal Line Needles in the SDSS Haystack
• Dust Budget Crisis in Little Red Dots
• Formation of proto-globular cluster candidates in cosmological simulations of dwarf galaxies at $z>4$
• Longitudinally Resolved Spectral Retrieval (ReSpect) of WASP-43b
• Atmospheric characterization of the super-Jupiter HIP 99770 b with KPIC
• Host Galaxies of Ultra Strong Mg II absorbers at z $\sim$ 0.5
• Late-Onset Circumstellar Medium Interactions are Rare: An Unbiased GALEX View of Type Ia Supernovae
• The most luminous, merger-free AGN show only marginal correlation with bar presence
• The first catalog of candidate white dwarf-main sequence binaries in open star clusters: A new window into common envelope evolution
• Unitary control of partially coherent waves. I. Absorption
• Galaxy quenching timescales from a forensic reconstruction of their colour evolution
• Wave-function-based emulation for nucleon-nucleon scattering in momentum space
• The Lyman Alpha Spectral Database (LASD)
• Unveiling $\delta$ Scuti and $\gamma$ Doradus Hybrid Pulsation of HD 53166 and HD 53349 Plus Rich Frequencies in HD 52788 -- Catalogs of 70552 $\delta$ Sct and 8080 $\gamma$ Dor
• PSR~J1910$-$5959A: A rare gravitational laboratory for testing white dwarf models
• Warped Disk Evolution in Grid-Based Simulations
• General relativistic magnetized Bondi-Hoyle-Lyttleton accretion with a spin-field misalignment: Jet nutation, polarity reversals, and Magnus drag
• Searching for a Hypervelocity White Dwarf Companion: A Proper Motion Survey of SN 1006
• On dust evolution in planet-forming discs in binary systems. II -- Comparison with Taurus and $\rho$ Ophiuchus (sub-)millimetre observations: discs in binaries have small dust sizes
• 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
• QoT estimation using EGN-assisted machine learning for multi-period network planning
• Hydrodynamic atmospheric escape in HD 189733 b: Signatures of carbon and hydrogen measured with the Hubble Space Telescope
• Hubble Space Telescope Proper Motion (HSTPROMO) Catalogs of Galactic Globular Clusters. VII. Energy Equipartition
• Introducing the Condor Array Telescope. 1. Motivation, Configuration, and Performance
• External or internal companion exciting the spiral arms in CQ Tau?
• Introducing the Condor Array Telescope: IV. A possible nova super-remnant surrounding the putative recurrent nova KT Eridani
• Relativistic Dynamical Stability Criterion of Multi-Planet Systems with a Distant Companion
• Predicting metallicities and carbon abundances from Gaia XP spectra for (carbon-enhanced) metal-poor stars
• Connecting Low- and High-Redshift Weak Emission-Line Quasars via HST Spectroscopy of Ly$\alpha$ Emission
• Trading oxygen for iron I: the [O/Fe] -- specific star formation rate relation of galaxies
• Pattern speed evolution of barred galaxies in TNG50
• Dust beyond the torus: Revealing the mid-infrared heart of local Seyfert ESO 428-G14 with JWST/MIRI
• No evidence that the binary black hole mass distribution evolves with redshift
• Strongly lensed supernovae as a self-sufficient probe of the distance duality relation
• What's the Difference? The potential for Convolutional Neural Networks for transient detection without template subtraction
• The impact of galaxy selection on the splashback boundaries of galaxy clusters
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• Global geomagnetic perturbation forecasting using Deep Learning
• Inflation: a Python library for classical and quantum causal compatibility
• Mapping the pressure-dependent day-night temperature contrast of a strongly irradiated atmosphere with HST spectroscopic phase curve
• 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
• On the choice of the most suitable indicator for the assembly state of dark matter haloes through cosmic time
• "Layer-by-layer" Unsupervised Clustering of Statistically Relevant Fluctuations in Noisy Time-series Data of Complex Dynamical Systems
• The CH radical at radio wavelengths: Revisiting emission in the 3.3GHz ground state lines
• X-Ray Luminous Supernovae: Threats to Terrestrial Biospheres
• Mass segregation and dynamics of primordial binaries in star clusters with a radially anisotropic velocity distribution
• Nuclear Activity in the Low Metallicity Dwarf Galaxy SDSS J0944-0038: A Glimpse into the Primordial Universe
• Scalable inference with Autoregressive Neural Ratio Estimation
• Systematics in tests of general relativity using LISA massive black hole binaries
• On the nature of LOFAR RMs and new constraints on magnetic fields in cosmic filaments and on magnetogenesis scenarios
• Interstellar Polarization Survey III: Relation Between Optical Polarization and Reddening in the General Interstellar Medium
• Classifications of Fermi-LAT unassociated sources in multiple machine learning methods
• The HI Column Density Distribution of the Galactic Disk and Halo
• Charting Galactic Accelerations with Stellar Streams and Machine Learning
• Calorimeter shower superresolution
• Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
• Discovery of $\sim$2200 new supernova remnants in 19 nearby star-forming galaxies with MUSE spectroscopy
• The Quenched Satellite Population Around Milky Way Analogs
• Optimal Fitting and Debiasing for Detectors Read Out Up-the-Ramp
• The Escape Velocity Profile of the Milky Way from Gaia DR3
• Titanium chemistry of WASP-121 b with ESPRESSO in 4-UT mode
• The impact of r-process heating on the dynamics of neutron star merger accretion disc winds and their electromagnetic radiation
• Consistent eccentricities for gravitational wave astronomy: Resolving discrepancies between astrophysical simulations and waveform models
• Effects of Planetesimal Scattering: Explaining the Observed Offsets from Period Ratios 3:2 and 2:1
• Estimating Magnetic Filling Factors From Simultaneous Spectroscopy and Photometry: Disentangling Spots, Plage, and Network
• Machine Learning for Conservative-to-Primitive in Relativistic Hydrodynamics
• The Radio Parallax of the Crab Pulsar: A First VLBI Measurement Calibrated with Giant Pulses
• Mode identification and ensemble asteroseismology of 119 $\beta$ Cep stars detected by Gaia light curves and monitored by TESS
• Not All Subhaloes Are Created Equal: Modelling the Diversity of Subhalo Density Profiles in TNG50
• Enhanced Star Formation Activity of Extreme Jellyfish Galaxies in Massive Clusters and the Role of Ram Pressure Stripping
• Submillimeter pulsations from the magnetar XTE J1810-197
• $\text{tdescore}$: An Accurate Photometric Classifier for Tidal Disruption Events
• Kinematics and Mass Distributions for Non-Spherical Deprojected Sérsic Density Profiles and Applications to Multi-Component Galactic Systems
• Cosmological Constraints on 4-Dimensional Einstein-Gauss-Bonnet Gravity
• Dynamical He Flashes in Double White Dwarf Binaries
• Cosmic Ray Interstellar Propagation Tool using Itô Calculus (criptic): software for simultaneous calculation of cosmic ray transport and observational signatures
• Phase mixing and the 1/f spectrum in the solar wind
• The Manhattan Suite: Accelerated galaxy evolution in the early Universe
• A Glimpse of the Stellar Populations and Elemental Abundances of Gravitationally Lensed, Quiescent Galaxies at $z\gtrsim 1$ with Keck Deep Spectroscopy
• Detecting the HI Power Spectrum in the Post-Reionization Universe with SKA-Low
• No Significant Correlation between Line-emission and Continuum Substructures in the Molecules with ALMA at Planet-forming Scales Program
• Family dispute: do Type IIP supernova siblings agree on their distance?
• FAST-ASKAP Synergy: Quantifying Coexistent Tidal and Ram Pressure Strippings in the NGC 4636 Group
• Magnetic field draping around clumpy high-velocity clouds in galactic halo
• Pandora: A fast open-source exomoon transit detection algorithm
• Sublimation of refractory minerals in the gas envelopes of accreting rocky planets
• Super-resolving Herschel imaging: a proof of concept using Deep Neural Networks
• Measuring the variability of directly imaged exoplanets using vector Apodizing Phase Plates combined with ground-based differential spectrophotometry
• The properties of magnetised cold filaments in a cool-core galaxy cluster
• JWST MIRI and NIRCam observations of NGC 891 and its circumgalactic medium
• Recovering the origins of the lenticular galaxy NGC 3115 using multi-band imaging
• Entangling Schrödinger's cat states by bridging discrete- and continuous-variable encoding
• Soft X-ray phase nano-microscopy of micrometre-thick magnets
• The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4<z<6
• 3D tomography of the giant Ly$\alpha$ nebulae of $z$$\approx$3--5 radio-loud AGN
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• All-Sky Kinematics of the Distant Halo: The Reflex Response to the LMC
• Variance Reduction and Noise Source Sampling Techniques for Monte Carlo Simulations of Neutron Noise Induced by Mechanical Vibrations
• JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z=5 to z=0.5
• On single crystal total scattering data reduction and correction protocols for analysis in direct space
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• Strong-lensing source reconstruction with variationally optimised Gaussian processes
• Broadband X-ray/UV/optical time-resolved spectroscopy of NGC 5548: The origin of the UV/optical variability in active galactic nuclei
• Tuning of extended state observer with neural network-based control performance assessment
• Mixed Modes and Asteroseismic Surface Effects: II. Subgiant Systematics
• Evidence of a Cloud-Cloud Collision from Overshooting Gas in the Galactic Center
• Data-driven study of composition-dependent phase compatibility in NiTi shape memory alloys
• A decade of radial-velocity monitoring of Vega and new limits on the presence of planets
• Simultaneous X-ray and radio observations of the transitional millisecond pulsar candidate CXOU J110926.4-650224. The discovery of a variable radio counterpart
• Investigation on the Orbital Period Variations of NN Ser: Implications for the Hypothetical Planets, the Applegate Mechanism and the Orbital Stability
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• Constraining Cosmic Inflation with Observations: Prospects for 2030
• Probing Hot Gas Components of Circumgalactic Medium in Cosmological Simulations with the Thermal Sunyaev-Zel'dovich Effect
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• Synthesizing Stellar Populations in South Pole Telescope Galaxy Clusters: I. Ages of Quiescent Member Galaxies at 0.3 < z < 1.4
• Automated SpectroPhotometric Image REDuction (ASPIRED)
• The Distance and Dynamical History of the Virgo Cluster Ultradiffuse Galaxy VCC 615
• Forbidden Line Emission from Type Ia Supernova Remnants Containing Balmer-Dominated Shells
• Membership analysis and 3D kinematics of the star-forming complex around Trumpler 37 using Gaia-DR3
• The cosmological simulation code $\mathrm{CO}N\mathrm{CEPT}1.0$
• Thermonuclear and Electron-Capture Supernovae from Stripped-Envelope Stars
• Emulation of the Cosmic Dawn 21-cm Power Spectrum and Classification of Excess Radio Models Using an Artificial Neural Network
• Testing protoplanetary disc evolution with CO fluxes. A proof of concept in Lupus and Upper Sco
• Search and identification of transient and variable radio sources using MeerKAT observations: a case study on the MAXI J1820+070 field
• Non-detection of Helium in the Hot Jupiter WASP-48b
• AREPO White Dwarf merger simulations resulting in edge-lit detonation and run-away hypervelocity companion
• MUSE-ALMA Halos XI: Gas flows in the circumgalactic medium
• Good and Proper: Self-similarity of N-body Simulations with Proper Force Softening
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• GRB 220426A: A Thermal Radiation-Dominated Gamma-Ray Burst
• Water observed in the atmosphere of τ Bootis Ab with CARMENES/CAHA
• Locked In Ice: how Pebble Drift and Volatile Entrapment can Significantly Impact Carbon and Oxygen Ratios in Evolving Protoplanetary Discs
• GJ 3929: High Precision Photometric and Doppler Characterization of an Exo-Venus and its Hot, Mini-Neptune-mass Companion
• Magma ocean interactions can explain JWST observations of the sub-Neptune TOI-270 d
• ULX pulsar Swift J0243.6+6124 observations with NuSTAR -- dominance of reflected emission in the super-Eddington state
• Unveiling the warm dense ISM in $z>6$ quasar host galaxies via water vapor emission
• Continuum source catalog for the first APERTIF data release
• Constraining the Densities of the Three Kepler-289 Planets with Transit Timing Variations
• Circumplanetary disk ices. I. Ice formation vs. viscous evolution and grain drift
• Stochastic excitation of internal gravity waves in rotating late F-type stars: A 3D simulation approach
• A pilot ASKAP survey for radio transients towards the Galactic Centre
• Signatures of impact-driven atmospheric loss in large ensembles of exoplanets
• A Reanalysis of the Composition of K2-106b: an Ultra-short Period Super-Mercury Candidate
• Searching for axion dark matter with MeerKAT Radio Telescope
• Classifying Astronomical Transients Using Only Host Galaxy Photometry
• Relativistic Signatures of Flux Eruption Events Near Black Holes
• DeepZipper: A Novel Deep Learning Architecture for Lensed Supernovae Identification
• First eccentric inspiral-merger-ringdown analysis of neutron star-black hole mergers
• Availability, outage, and capacity of spatially correlated, Australasian free-space optical networks
• Deep Narrowband Photometry of the M101 Group: Strong-Line Abundances of 720 HII Regions
• Investigating Clumpy Galaxies in the Sloan Digital Sky Survey Stripe 82 using the Galaxy Zoo
• A framework for structural shape optimization based on automatic differentiation, the adjoint method and accelerated linear algebra
• Path separation of dissipation-corrected targeted molecular dynamics simulations of protein-ligand unbinding
• The Cosmic Shoreline Revisited: A Metric for Atmospheric Retention Informed by Hydrodynamic Escape
• A multi-tracer empirically-driven approach to line-intensity mapping lightcones
• Unravelling the enigmatic ISM conditions in Minkowski's Object
• Does charge matter in high-energy collisions of black holes?
• The polarization of the synchrotron radiation from a recollimated jet: application to high-energy BL Lacs
• Which galaxy property is the best gauge of the oxygen abundance?
• Observable Primordial Gravitational Waves from Non-minimally Coupled $R^2$ Palatini Modified Gravity
• PauliComposer: Compute Tensor Products of Pauli Matrices Efficiently
• Characteristics of small protoplanetary disc warps in kinematic observations
• The H.E.S.S. Gravitational Wave Rapid Follow-up Program
• TiDES: The 4MOST Time Domain Extragalactic Survey
• Ripples spreading across the Galactic disc. Interplay of direct and indirect effects of the Sagittarius dwarf impact
• Unbinned Profiled Unfolding
• Measurement of the matter-radiation equality scale using the extended Baryon Oscillation Spectroscopic Survey Quasar Sample
• Late-time tails in nonlinear evolutions of merging black holes
• TOI-954 b and K2-329 b: Short-Period Saturn-Mass Planets that Test whether Irradiation Leads to Inflation
• Radio Afterglows from Compact Binary Coalescences: Prospects for Next-Generation Telescopes
• Stability and detectability of exomoons orbiting HIP 41378 f, a temperate Jovian planet with an anomalously low apparent density
• Investigating the amplitude and rotation of the phase spiral in the Milky Way outer disc
• Simulating image coaddition with the Nancy Grace Roman Space Telescope: I. Simulation methodology and general results
• Dense Molecular Gas Properties of the Central Kpc of Nearby Ultraluminous Infrared Galaxies Constrained by ALMA Three Transition-line Observations
• The impact of dust evolution on the dead zone outer edge in magnetized protoplanetary disks
• Localization of binary neutron star mergers with a single Cosmic Explorer
• Gray Two-moment Neutrino Transport: Comprehensive Tests and Improvements for Supernova Simulations
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• A Pristine-UNIONS view on the Galaxy: Kinematics of the distant spur feature of the Sagittarius stream traced by Blue Horizontal Branch stars
• Bounds on the charge of the graviton using gravitational wave observations
• The MUSE view of the Sculptor galaxy: survey overview and the planetary nebulae luminosity function
• Ariel stellar characterisation III. Fast rotators and new FGK stars in the Ariel Mission Candidate Sample
• Multimessenger hierarchical triple merger gravitational-wave event pair GW190514-GW190521 inside AGN J124942.3 + 344929
• On the origin of Jupiter's fuzzy core: constraints from N-body, impact and evolution simulations
• Trapping Interlayer Excitons in van der Waals Heterostructures by Potential Arrays
• A Diffused Background from Axion-like Particles in the Microwave Sky
• Initial sizes of star clusters: implications for cluster dissolution during galaxy evolution
• Three-dimensional simulations of the magnetorotational instability in eccentric disks
• Neural-network preconditioners for solving the Dirac equation in lattice gauge theory
• Cosmic dipole tensions: confronting the cosmic microwave background with infrared and radio populations of cosmological sources
• Cost-Efficient High-Resolution Linear Absorption Spectra Through Extrapolating the Dipole Moment from Real-Time Time-Dependent Electronic-Structure Theory
• Modelling the Track of the GD-1 Stellar Stream Inside a Host with a Fermionic Dark Matter Core-Halo Distribution
• A kinematically constrained kick distribution for isolated neutron stars
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• fSEAD: a Composable FPGA-based Streaming Ensemble Anomaly Detection Library
• Probing modified Newtonian dynamics with hypervelocity stars
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• The VMC survey -- LIV. The internal kinematics of the LMC with new VISTA observations
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• The hydrostatic-to-lensing mass bias from resolved X-ray and optical-IR data
• SIMPLE: Simple Intensity Map Producer for Line Emission
• Correction Formulas for the Mølmer-Sørensen Gate Under Strong Driving
• Observations of scattered light from exoplanet atmospheres
• Evidence for Primordial Alignment II: Insights from Stellar Obliquity Measurements for Hot Jupiters in Compact Multiplanet Systems
• Extreme Variability Quasars in Their Various States. II: Spectral Variation Revealed with Multi-epoch Spectra
• First VLBI detection of Fornax A
• The Relation between Solar Spicules and Magnetohydrodynamic Shocks
• High-Precision Redshifts for Type Ia Supernovae with the Nancy Grace Roman Space Telescope P127 Prism
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• Improving Black Hole Accretion Treatment in Hydrodynamical Simulations
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• A practical, effective calculation of gamma difference distributions with open data science tools
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• The Lyman-alpha and Continuum Origins Survey. I. Survey description and Ly$\alpha$ imaging
• The Dark Energy Camera Magellanic Clouds Emission-Line Survey
• Frenetic steering in a nonequilibrium graph
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• ATOMIUM: Continuum emission and evidence of dust enhancement from binary motion
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• Spectropolarimetric Radio Imaging of Faint Gyrosynchrotron Emission from a CME : A Possible Indication of the Insufficiency of Homogeneous Models
• A Dependable Distance Estimator to Black Hole Low-Mass X-ray Binaries
• First upper limits on the 21-cm signal power spectrum of neutral hydrogen at $z=9.16$ from the LOFAR 3C196 field
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• Seeking Self-Regulating Simulations of Idealized Milky Way-Like Galaxies
• CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation
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• The ones that got away: chemical tagging of globular cluster-origin stars with Gaia BP/RP spectra
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• Accurate Ground-based Astrometry of Naked-eye Stars: The United States Naval Observatory Bright-Star Astrometric Database
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• ACCESS: Tentative detection of H${}_2$O in the ground-based optical transmission spectrum of the low-density hot Saturn HATS-5b
• WALOP-South: A Four-Camera One-Shot Imaging Polarimeter for PASIPHAE Survey. Paper II -- Polarimetric Modelling and Calibration
• J-PLUS: Discovery and characterisation of ultracool dwarfs using Virtual Observatory tools II. Second data release and machine learning methodology
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• The first X-ray look at SMSS J114447.77-430859.3: the most luminous quasar in the last 9 Gyr
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• High-resolution SOFIA/EXES Spectroscopy of Water Absorption Lines in the Massive Young Binary W3 IRS 5
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• Revealing the hidden cosmic feast: A z=4.3 galaxy group hosting two optically dark, efficiently star-forming galaxies
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• Investigating the Growth of Little Red Dot Descendants at z<4 with the JWST
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• MIGHTEE-HI: The direct detection of neutral hydrogen in galaxies at $z>0.25$
• NOEMA${}^{3D}$: A first kpc resolution study of a $z\sim 1.5$ main sequence barred galaxy channeling gas into a growing bulge
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• The First Model-Independent Chromatic Microlensing Search: No Evidence in the Gravitational Wave Catalog of LIGO-Virgo-KAGRA
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• Revisiting X-ray Afterglows of Jetted Tidal Disruption Events with the External Reverse Shock
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• Simulating image coaddition with the Nancy Grace Roman Space Telescope: III. Software improvements and new linear algebra strategies
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• Milky Way-Like Gas Excitation in an Ultrabright Submillimeter Galaxy at $z=1.6$
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• Jellyfish galaxies with the IllustrisTNG simulations -- Supermassive black hole activity in dense environments with ram-pressure stripped satellites
• pop-cosmos: Insights from generative modeling of a deep, infrared-selected galaxy population
• Surrogate models for lightcurves and photosphere properties of Type II supernovae
• Simplifying asteroseismic analysis of solar-like oscillators: An application of principal component analysis for dimensionality reduction
• Informed total-error-minimizing priors: Interpretable cosmological parameter constraints despite complex nuisance effects
• Position-dependent Voronoi probability distribution functions for matter and halos
• STable AutoCorrelation Integral Estimator (STACIE): Robust and accurate transport properties from molecular dynamics simulations
• Tiny galaxies and dark substructures: exploring the "dark" subhaloes in TNG50
• Close contact restriction periods for patients who received iodine-131 therapy for differentiated thyroid cancer
• Comparing the Space Densities of Millisecond-Spin Magnetars and Fast X-Ray Transients
• VLBA astrometry of PSRs B0329+54 and B1133+16: Improved pulsar distances and comparison of global ionospheric models
• BLADE: An Automated Framework for Classifying Light Curves from the Center for Near-Earth Object Studies (CNEOS) Fireball Database
• A Bayesian approach to modelling spectrometer data chromaticity corrected using beam factors -- II. Model priors and posterior odds
• Towards nonlinear optics with Mössbauer nuclei using x-ray cavities
• Physical Conditions of the Ionized Superwind in NGC 253 with VLT/MUSE
• Revisiting the Perseus Cluster I: Resolving the Si/S/Ar/Ca ratios by Stellar Convection
• Primordial Black Hole Triggered Type Ia Supernovae I: Impact on Explosion Dynamics and Light Curves
• TMMax: High-performance modeling of multilayer thin-film structures using transfer matrix method with JAX
• Past the outer rim, into the unknown: structures beyond the Kuiper Cliff
• Cosmic Ray Rejection with Attention Augmented Deep Learning
• Companion Mass Limits for 17 Binary Systems Obtained with Binary Differential Imaging and MagAO/Clio
• Continued radio observations of the persistent radio source associated with FRB20190520B provides insights into its origin
• A photometric study of two contact binaries: CRTS J025408.1+265957 and CRTS J012111.1+272933
• Lazarus Stars: Numerical investigations of stellar evolution with star-lifting as a life extension strategy
• Metal-poor single Wolf-Rayet stars: The interplay of optically thick winds and rotation
• Transactional Python for Durable Machine Learning: Vision, Challenges, and Feasibility
• Data-Space Validation of High-Dimensional Models by Comparing Sample Quantiles
• planetMagFields: A Python package for analyzing and plotting planetary magnetic field data
• Towards a Machine-Learned Poisson Solver for Low-Temperature Plasma Simulations in Complex Geometries
• Compact Steep Spectrum Radio Sources with Enhanced Star Formation are Smaller than $10$kpc
• Resurgence of CO in a warm bubble around accreting protoplanets and its observability
• The Breakthrough Listen Search for Intelligent Life: Nearby Stars' Close Encounters with the Brightest Earth Transmissions
• On the Origins of Spontaneous Spherical Symmetry-Breaking in Open-Shell Atoms Through Polymer Self-Consistent Field Theory
• Finite-element assembly approach of optical quantum walk networks
• Symmetry breaking at a topological phase transition
• Dwarf-Dwarf interactions and their influence on star formation : Insights from post-merger galaxies
• A deep Search for Ethylene Glycol and Glycolonitrile in the V883 Ori Protoplanetary Disk
• Measuring neutrino mass and asymmetry with matter pairwise velocities
• Inferring Mbh-Mbulge Evolution from the Gravitational Wave Background
• Characterising galaxy clusters' completeness function in Planck with hydrodynamical simulations
• Circumplanetary disk ices II. Composition
• Image Classification by Throwing Quantum Kitchen Sinks at Tensor Networks
• The COS-Holes Survey: Connecting Galaxy Black Hole Mass with the State of the CGM
• The End of the Road for Far-infrared Reddening Maps? Evidence for Reddening Errors Driven by Changes in PAH Abundance
• New Active Asteroid 2015 VA108: A Citizen Science Discovery
• Singular spectrum analysis of time series data from low frequency radiometers, with an application to SITARA data
• The Ly$\alpha$ and Continuum Origins Survey. III. Investigating the Link between Galaxy Morphology, Merger Properties and LyC Escape
• Repeating versus Nonrepeating Fast Radio Bursts: A Deep Learning Approach to Morphological Characterization
• Understanding and predicting cadence effects in the characterization of exoplanet transits
• Survey for Distant Solar Twins (SDST) -- III. Identification of new solar twin and solar analogue stars
• The density of planar sets avoiding unit distances
• Planning Visual Inspection Tours for a 3D Dubins Airplane Model in an Urban Environment
• First results from the ENTOTO neutron monitor: Quantifying the waiting time distribution
• Vacillating about media bias: changing one's mind intermittently within a network of political allies and opponents
• A hierarchical Bayesian approach to point source analysis in high-energy neutrino telescopes
• Machine Learning Classification of COSMOS2020 Galaxies: Quiescent vs. Star-Forming
• Two-horn quiescent prominence observed in H-alpha and MgII h&k lines with THEMIS and IRIS
• X-ray properties of high-redshift Radio Loud and Radio Quiet Quasars observed by Chandra
• Polarization and variability of compact sources measured in Planck time-ordered data
• Early Growing Supermassive Black Holes Strengthen Bars and Boxy/Peanut Bulges
• Feeding the Dead: Neutral Gas Inflow in a Long-Quenched Ancient Massive Galaxy at $z\sim 2.7$ Observed with JWST/NIRSpec
• PLQ-Sim: A Computational Tool for Simulating Photoluminescence Quenching Dynamics in Organic Donor/Acceptor Blends
• Not all spacetime coordinates for general-relativistic ray tracing are created equal
• Scalar fields around black hole binaries in LIGO-Virgo-KAGRA
• Can quasi-circular mergers of charged black holes produce extremal black holes?
• The Boundary Element Method for Acoustic Transmission with Nonconforming Grids
• Potential impact of noise correlation in next-generation gravitational wave detectors
• Modeling Apsidal Motion in Eclipsing Binaries using ELC
• Associations Between Scattering Screens and Interstellar Medium Filaments
• Light Curve Classification with DistClassiPy: a new distance-based classifier
• StarStream: Automatic detection algorithm for stellar streams
• A novel radio imaging method for physical spectral index modelling
• MAGIC: Microlensing Analysis Guided by Intelligent Computation
• colorspace: A Python Toolbox for Manipulating and Assessing Colors and Palettes
• Discerning media bias within a network of political allies and opponents: Disruption by partisans
• Measuring the Substructure Mass Power Spectrum of 23 SLACS Strong Galaxy-Galaxy Lenses with Convolutional Neural Networks
• The $z\sim 2$ $[\mathrm{O}\mathrm{III}]$ Luminosity Function of Grism-selected Emission-line Galaxies
• Controlling stable Bloch points with electric currents
• Effects of CO-dark Gas on Measurements of Molecular Cloud Stability and the Size-Linewidth Relationship
• Evolution of MHD turbulence in the expanding solar wind: residual energy and intermittency
• Discovery of faint double-peak Halpha emission in the halo of low redshift galaxies
• Accurate and efficient photo-eccentric transit modeling
• Schmidt modes carrying orbital angular momentum generated by cascaded systems pumped with Laguerre-Gaussian beams
• Noise-aware variational eigensolvers: a dissipative route for lattice gauge theories
• Quantifying the Impact of Starspot-Crossing Events on Retrieved Parameters from Transit Lightcurves
• C2-GaMe: Classification of Cluster Galaxy Membership with Machine Learning
• ExoplaNeT accRetion mOnitoring sPectroscopic surveY (ENTROPY) - II. Time series of Balmer line profiles of Delorme 1(AB)b
• Application of the Eddington inversion method to constrain the dark matter halo of galaxies using only observed surface brightness profiles
• Asymmetries in asymptotic giant branch stars and their winds. I. From 3D RHD models to synthetic observables
• Optimising the shape of photometric redshift distributions with clustering cross-correlations
• Holographic Beam Measurements of the Canadian Hydrogen Intensity Mapping Experiment (CHIME)
• PyArmadillo: a streamlined linear algebra library for Python
• Distant probes of RM structure -- Where is the Faraday Rotation towards the Magellanic Leading Arm?
• VAMPyR -- A High-Level Python Library for Mathematical Operations in a Multiwavelets Representation
• TDCOSMO. XXIII. Measurement of the Hubble constant from the doubly lensed quasar HE1104-1805
• Multiphase gas in elliptical galaxies: the role of Type Ia supernovae
• GRB 201104A: A "Repetitive" Short Gamma-Ray Burst?
• RI$-$Calc: A User Friendly Software and Web Server for Refractive Index Calculation
• An HST/STIS View of Protoplanetary Disks in Upper Scorpius: Observations of Three Young M-Stars
• Merging White Dwarf Binaries Produce Type Ia Supernovae in Elliptical Galaxies
• Analytical Noise Bias Correction for Precise Weak Lensing Shear Inference
• A Galactic Transformation -- Understanding the SMC's Structural and Kinematic Disequilibrium
• Design and performance of a multi-terahertz Fourier transform spectrometer for axion dark matter experiments
• Globular clusters in \textsc{OrbIT}: complete dynamical characterisation of the globular cluster population of the Milky Way through updated orbital reconstruction
• The Simons Observatory: impact of bandpass, polarization angle and calibration uncertainties on small-scale power spectrum analysis
• Sphractal: Estimating the Fractal Dimension of Surfaces Computed from Precise Atomic Coordinates via Box-Counting Algorithm
• Shock-induced partial alignment in geometrically-thick tilted accretion disks around black holes
• The circular velocity and halo mass functions of galaxies in the nearby Universe
• Active Galactic Nuclei in the Green Valley at z$\sim$0.7
• KBSS-InCLOSE I: Design and First Results from the Inner CGM of QSO Line Of Sight Emitting Galaxies at z~2-3
• SOLAX: A Python solver for fermionic quantum systems with neural network support
• First Light And Reionisation Epoch Simulations (FLARES) XVI: Size Evolution of Massive Dusty Galaxies at Cosmic Dawn from UV to IR
• Euclid: Estimation of the impact of correlated readout noise for flux measurements with the Euclid NISP instrument
• Deepest limits on scattered light emission from the Epsilon Eridani inner debris disk with HST/STIS
• Distinct Rotational Evolution of Giant Planets and Brown Dwarf Companions
• The Emission and Suppression of Line Features in Luminous Transients
• The Galactic Center in Color: Measuring Extinction with High-Proper-Motion Stars
• A Close-in Planet Orbiting Giant Star HD 167768
• A self-supervised, physics-aware, Bayesian neural network architecture for modelling galaxy emission-line kinematics
• A Novel Solution for Resonant Scattering Using Self-Consistent Boundary Conditions
• Building spectral templates and reconstructing parameters for core collapse supernovae with CASTOR
• How do the dynamics of the Milky Way -- Large Magellanic Cloud system affect gamma-ray constraints on particle dark matter?
• The first r-process enhanced star confirmed to be a member of the Galactic bulge
• Ly$\alpha$ Emission from [OIII] Emitters Near Reionization: The role of environment in galaxy Ly$\alpha$ detection
• Chemical evolution of an evaporating lava pool
• FAST H I 21 cm study of blueberry galaxies
• Enhanced Small-Scale Structure in the Cosmic Dark Ages
• Stellar angular momentum of disk galaxies at z = 0.7 in the MAGIC survey I. Impact of the environment
• Cosmological prior for the $J$-factor estimation of dwarf spheroidal galaxies
• Active smectics on a sphere
• A dense dark matter core of the subhalo in the strong lensing system JVAS B1938+666
• Bayesian inference methodology for Primordial Power Spectrum reconstructions from Large Scale Structure
• Spitzer phase curve observations and circulation models of the inflated ultra-hot Jupiter WASP-76b
• Carbon from massive binary-stripped stars over cosmic time: effect of metallicity
• The Hierarchical Dynamical State of Molecular Gas from 3 to 300 pc in NGC 253
• Exploring magnetic loops and serpentine fields in the quiet Sun with the GRIS-IFU
• On Stellar Migration from Andromeda to the Milky Way
• The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios
• KiDS-Legacy: Constraints on Horndeski gravity from weak lensing combined with galaxy clustering and cosmic microwave background anisotropies
• Discrete Time Crystal Phase of Higher Dimensional Integrable Models
• K2, Spitzer, and TESS Transits of Four Sub-Neptune Exoplanets
• Accelerated Bayesian inference of plasma profiles with self-consistent MHD equilibria at W7-X via neural networks
• Nearly Full-Sky Low-Multipole Cosmic Microwave Background Temperature Anisotropy: III. CMB Temperature Anomalies
• Artificial Greenhouse Gases as Exoplanet Technosignatures
• Neural translation for Stokes inversion and synthesis
• HOLISMOKES -- XIV. Time-delay and differential dust extinction determination with lensed type II supernova color curves
• Cosmological perturbation theory using generalized Einstein de Sitter cosmologies
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• Sensitivity to Sub-Io-sized Exosatellite Transits in the MIRI LRS Lightcurve of the Nearest Substellar Worlds
• Adapting coherent-state superpositions in noisy channels
• Intrinsic alignment from multiple shear estimates: A first application to data and forecasts for Stage IV
• A new analytical model of the cosmic-ray energy flux for Galactic diffuse radio emission
• A New Tidal Stream Discovered in Gaia DR3
• The qspec Python package: A physics toolbox for laser spectroscopy
• The corona of a fully convective star with a near-polar flare
• VIRIS: Simulating indoor airborne transmission combining architectural design and people movement
• Principal Components for Model-Agnostic Modified Gravity with 3x2pt
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• The middle-aged pulsar PSR J1741-2054 and its bow-shock nebula in far ultraviolet
• QUIJOTE scientific results -- IX. Radio sources in the QUIJOTE-MFI wide survey maps
• Polarimetric differential imaging with VLT/NACO. A comprehensive PDI pipeline for NACO data (PIPPIN)
• Analyses of Hydrogen-stripped core-collapse supernovae using MOSFiT and MESA based tools
• OGHReS: Star formation in the Outer Galaxy II ($\ell =180^{\circ }$-$280^{\circ }$)
• A joint 1% calibration of the RR Lyrae & type-II Cepheid Leavitt laws yields homogeneous distances to 93 Galactic globular clusters
• Testing modified gravity with the eccentric neutron star--black hole merger GW200105
• A Bayesian neural network predicts the dissolution of compact planetary systems
• An Imaging Search for Post-Main-Sequence Planets of Sirius B
• Einstein@Home Searches for Gamma-ray Pulsars in the Inner Galaxy
• Deep Chandra observations of PLCKG287.0+32.9: a clear detection of a shock front in a heated former cool core
• Unexpected solar-cycle variation of acoustic mode power in Sun-as-a-star observations
• Reducing circuit depth with qubitwise diagonalization
• Isolating the extreme debris disc signature -- explorations of eccentric extreme debris discs formed by giant impacts
• CHEX-MATE: New detections and properties of the radio diffuse emission in massive clusters with MeerKAT
• Flaring Latitudes in Ensembles of Low Mass Stars
• Photometric calibration in u-band using blue halo stars
• A link between the size and composition of comets
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• The stellar population in the SARAO MeerKAT Galactic Plane Survey
• A Moderate Albedo from Reflecting Aerosols on the Dayside of WASP-80 b Revealed by JWST/NIRISS Eclipse Spectroscopy
• Precise determination of circumstellar disk lifetimes: Disk evolution in a single star-forming region
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• Detecting Intermediate-Mass Black Holes out to 20 Mpc with ELT/HARMONI: The Case of FCC 119
• Axion-Photon Conversion in Neutron Star Magnetospheres: The Role of the Plasma in the Goldreich-Julian Model
• An advanced pulse-avalanche stochastic model of long gamma-ray burst light curves
• Catalog-level blinding on the bispectrum for DESI-like galaxy surveys
• The Solar Neighborhood LII: M Dwarf Twin Binaries -- Presumed Identical Twins Appear Fraternal in Variability, Rotation, H$\alpha$, and X-rays
• Optimizing charge-balanced pulse stimulation for desynchronization
• Numerical Relativity Estimates of the Remnant Recoil Velocity in Binary Neutron Star Mergers
• SpectrAx: Spectral Search of Axion-Like Particles Using Multi-Band Observations of Galaxy Clusters from SKA, SO, CMB-S4 and eROSITA
• Searching for Protoplanets around MWC 758 and MWC 480 in Br-$\gamma$ using Kernel Phase and SCExAO/CHARIS
• Revisiting the Dragonfly Galaxy I. High-resolution ALMA and VLA Observations of the Radio Hotspots in a Hyper-luminous Infrared Galaxy at $z=1.92$
• The SRG/eROSITA all-sky survey: Hard X-ray selected Active Galactic Nuclei
• PSF Calibration of DAMPE for gamma-ray Observations
• Auriga Streams II: orbital properties of tidally disrupting satellites of Milky Way-mass galaxies
• Turnaround density evolution encodes cosmology in simulations
• The kinematics of young stellar population in the W5 region of the Cassiopeia OB6 association: implication on the formation process of stellar associations
• High-precision light curves of geostationary objects: The PHANTOM ECHOES 2 RPO campaign
• Connections between the cycle-to-cycle light curve and O-C variations of the non-Blazhko RR Lyrae stars
• The K2 Galactic Archaeology Program: Overview, target selection and survey properties
• The Correlation Between Dust and Gas Contents in Molecular Clouds
• Dynamics of star associations in an SMBH-IMBH system: The case of IRS13 in the Galactic centre
• Cosmic Census: Relative Distributions of Dark Matter, Galaxies and Diffuse Gas
• A Multi-wavelength Characterization of the 2023 Outburst of MAXI J1807+132: Manifestations of Disk Instability and Jet Emission
• Inferring Time-Dependent Distribution Functions from Kinematic Snapshots
• Geoff: The Generic Optimization Framework & Frontend for Particle Accelerator Controls
• Inferring the spins of merging black holes in the presence of data-quality issues
• Ultra-Faint Milky Way Satellites Discovered in Carina, Phoenix, and Telescopium with DELVE Data Release 3
• On the origin of the Hercules group: I. chemical signatures indicating the outer bar origin
• ForSE+: Simulating non-Gaussian CMB foregrounds at 3 arcminutes in a stochastic way based on a generative adversarial network
• Ultra-sensitive radon assay using an electrostatic chamber in a recirculating system
• HADES RV Programme with HARPS-N at TNG. XVI. A super-Earth in the habitable zone of the GJ 3998 multi-planet system
• Cosmology with Binary Neutron Stars: Does Mass-Redshift Correlation Matter?
• Out-of-focus holography at the Effelsberg telescope
• Scintillation Properties of PSR B1133+16 Measured with Very Long Baseline Interferometry
• A First-look at Spatially-resolved Infrared Supernova Remnants in M33 with JWST
• Relieving scale disparity in binary black hole simulations
• Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
• [CII] luminosity models and large-scale image cubes based on COSMOS 2020 and ALPINE-ALMA [CII] data back to the epoch of reionisation
• A direct measurement of the electron density turbulence parameter $C_1$ and implications for the emission size of the magnetar XTE J1810-197
• The cusp-halo relation
• Differencing and Coadding JWST Images with Matched Point Spread Function
• Brighter and More Massive Galaxies in the Vicinity of Lyman-alpha Nebulae
• Measuring galaxy abundance and clustering at high redshift from incomplete spectroscopic data: Tests on mock catalogs
• Beyond LambdaCDM: How the Hubble tension challenges early universe physics
• Bubbles in a box: Eliminating edge nucleation in cold-atom simulators of vacuum decay
• The disc origin of the Milky Way bulge: On the high velocity dispersion of metal-rich stars at low latitude
• Open cluster members in APOGEE DR17 I. Dynamics and star members
• Time Can Invalidate Algorithmic Recourse
• MADAS -- A Python framework for assessing similarity in materials-science data
• Tidally driven inertial waves enhance eccentricity damping and spin evolution in planets and stars
• Quasi-normal modes of slowly-rotating Johannsen black holes
• JWST Spectroscopy of a Blue Binary Cold Classical Kuiper Belt Object
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Validating the bright Gaia celestial reference frame with new VLBI astrometry of radio stars
• Filament formation due to diffusive instabilities in dusty protoplanetary disks
• Inflation from a chaotic potential with a step
• The Nature of Gravitational Wave Events with Host Environment Escape Velocities
• Fading in the Flow: Suppression of cold gas growth in expanding galactic outflows
• Using Giant Pulses to Measure the Impulse Response of the Interstellar Medium
• Assessment of Spatio-Temporal Predictors in the Presence of Missing and Heterogeneous Data
• Filtering in CMB data analysis with application to ACT DR4 and Planck observations
• Enhancing the detection of low-energy M dwarf flares: Wavelet-based denoising of CHEOPS data
• Raster Forge: Interactive Raster Manipulation Library and GUI for Python
• Fourier Domain
• Photometric Catalogue for Space and Ground Night-Time Remote-Sensing Calibration: RGB Synthetic Photometry from Gaia DR3 Spectrophotometry
• Application of the Green function formalism to the interplay between avalanche and multiphoton ionization induced by optical pulses
• Bayesian inference for near-field interferometric tests of collapse models
• Effects of Outer Giant Planets on In Situ Formation of Inner Super-Earths
• FALCO: a Foundation model of Astronomical Light Curves for time dOmain astronomy
• How Distance Affects GRB Prompt Emission Measurements
• Fundamental thresholds for computational and erasure errors via the coherent information
• The 3D Galactocentric velocities of Kepler stars: marginalizing over missing RVs
• Galaxy Correlation Function and Local Density from Photometric Redshifts Using the Stochastic Order Redshift Technique (SORT)
• Active Filaments on Curved Surfaces: From Single Filaments to Dilute Suspensions
• A Unified Perspective for Loss-Oriented Imbalanced Learning via Localization
• Weighing the Darkness III: How Gaia Could, but Probably Won't, Astrometrically Detect Free-Floating Black Holes
• Three young planets around the K-dwarf K2-198: High-energy environment, evaporation history and expected future
• Magnetic Field-Constrained Ensemble Image Segmentation of Coronal Holes in Chromospheric Observations
• ALAAMEE: Open-source software for fitting autologistic actor attribute models
• A Trio of Giant Planets Orbiting Evolved Star HD 184010
• Portable, heterogeneous ensemble workflows at scale using libEnsemble
• Galactic properties that favour star cluster formation: a statistical view
• Simulating realistic self-interacting dark matter models including small and large-angle scattering
• Testing the Surface Brightness Fluctuation Method on Dwarf Galaxies in the COSMOS Field
• Emulators for stellar profiles in binary population modeling
• Shear-gravity transition determines the steep velocity dispersion-size relation in molecular clouds: confronting analytical formula with observations
• First Detections of PN, PO, and PO+ toward a Shocked Low-mass Starless Core
• Testing the sources of the peculiar abundances in globular clusters
• Machine-learning Closure for Vlasov-Poisson Dynamics in Fourier-Hermite Space
• Delayed phase mixing in the self-gravitating Galactic disc
• Discovery of a Proto-White Dwarf with a Massive Unseen Companion
• Electromagnetic Follow-up to Gravitational Wave Events with the UltraViolet EXplorer (UVEX)
• Principled interpolation of Green's functions learned from data
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• Fisher matrix forecasts on the astrophysics of galaxies during the epoch of reionisation from the 21-cm power spectra
• Beyond the Nyquist frequency: Asteroseismic catalog of undersampled Kepler late subgiants and early red giants
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• A Unified Multi-Wavelength Data Analysis Workflow with gammapy. Constraining the Broadband Emission of FSRQ OP 313
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• The He I 10830 A line: Radiative transfer and differential illumination effects
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• Seismic detection of core magnetic fields in red giants using the gravity offset
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• The Host Galaxies of PTA Sources: Converting Supermassive BH Binary Parameters into EM Observables
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• JADES Dark Horse: demonstrating high-multiplex observations with JWST/NIRSpec dense-shutter spectroscopy in the JADES Origins Field
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• Molecules with ALMA at Planet-forming Scales (MAPS) XIX. Spiral Arms, a Tail, and Diffuse Structures Traced by CO around the GM Aur Disk
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• Modeling Tidal Streams and Tidal Tails around Galaxies Using Deep Wendelstein Imaging Data
• Stellar halos tracing the assembly of ultra-faint dwarf galaxies
• Boosting Performance Optimization with Interactive Data Movement Visualization
• KMT-2025-BLG-1616Lb: First Microlensing Bound Planet From DREAMS
• The Roles of Low-Noise Stations, Arrays and Ocean-Bottom Seismometers in Monitoring UK Offshore Seismicity associated with Subsurface Storage of Carbon Dioxide
• Approximating Higher-Order Derivative Tensors Using Secant Updates
• COOL-LAMPS IV: A Sample of Bright Strongly-Lensed Galaxies at $3<z<4$
• The Simons Observatory: Studies of Detector Yield and Readout Noise From the First Large-Scale Deployment of Microwave Multiplexing at the Large Aperture Telescope
• A three-dimensional model for the reversal in the local large-scale interstellar magnetic field
• CMB-PAInT: An inpainting tool for the cosmic microwave background
• Reionization relics in the cross-correlation between the Ly$\alpha$ forest and 21 cm intensity mapping in the post-reionization era
• Spatial variation in temperature and density in the IC 63 PDR from ${\mathrm{H}}_2$ Spectroscopy
• Comparing simulated Milky Way satellite galaxies with observations using unsupervised clustering
• Detection of a white dwarf orbiting a Carbon-Oxygen depleted blue straggler in 47 Tucanae
• Accelerating lensed quasar discovery and modeling with physics-informed variational autoencoders
• The AutoSPADA Platform: User-Friendly Edge Computing for Distributed Learning and Data Analytics in Connected Vehicles
• Close encounters with the Death Star: Interactions between collapsed bodies and the Solar System
• Planet Mass Function around M stars at 1-10 au: A Plethora of sub-Earth mass objects
• The Effect of Points Dispersion on the $k$-nn Search in Random Projection Forests
• Doomed Worlds II: Reassessing Suggestions of Orbital Decay for TrES-5 b
• Elemental Abundances of Kepler Objects of Interest in APOGEE DR17
• Probing magneto-ionic microstructure towards the Vela pulsar using a prototype SKA-Low station
• The Simons Observatory: Validation of reconstructed power spectra from simulated filtered maps for the Small Aperture Telescope survey
• SOFIA/HAWC+ Far-Infrared Polarimetric Large Area CMZ Exploration Survey. V. The Magnetic Field Strength and Morphology in the Sagittarius C Complex
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• Scalable and Robust Multiband Modeling of AGN Light Curves in Rubin-LSST
• Improved Gibbs samplers for Cosmic Microwave Background power spectrum estimation
• Mapping Parameter Correlations in Spinning Binary Black Hole Mergers
• The RSD Sorting Hat: Unmixing Radial Scales in Projection
• Enabling MPI communication within Numba/LLVM JIT-compiled Python code using numba-mpi v1.0
• The JWST Emission Line Survey (JELS): The sizes and merger fraction of star-forming galaxies during the Epoch of Reionization
• The diverse quenching pathways of post-starburst galaxies in SDSS-IV MaNGA
• The Type Ia Supernova and Asymptotic Giant Branch Stellar Ejecta-regulated Interstellar Medium of Massive Galaxies
• Inferring the density and membership of stellar streams with flexible models: The GD-1 stream in Gaia Data Release 3
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• Dust-UV offsets in high-redshift galaxies in the Cosmic Dawn III simulation
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• Weakly supervised anomaly detection for resonant new physics in the dijet final state using proton-proton collisions at $\sqrt{s}=13$ TeV with the ATLAS detector
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• The Outskirt Stellar Mass of Low-Redshift Massive Galaxies is an Excellent Halo Mass Proxy in Illustris/IllustrisTNG Simulations
• An improved algorithm for separating clock delays from ionospheric effects in radio astronomy
• The Multi-parameter Test of Gravitational Wave Dispersion with Principal Component Analysis
• ComPACT: ACT+Planck galaxy cluster catalogue
• Laser-pump-resistive-probe technique to study nanosecond-scale relaxation processes
• From gas to stars: MUSEings on the internal evolution of IC 1613
• A Blob Method for Mean Field Control With Terminal Constraints
• Refitting cosmological data with neutrino mass and degeneracy
• Randomized Approach to Matrix Completion: Applications in Recommendation Systems and Image Inpainting
• PyPartMC: A Pythonic interface to a particle-resolved, Monte Carlo aerosol simulation framework
• Generalized Hydrodynamics for the Volterra lattice: Ballistic and nonballistic behavior of correlation functions
• Sequential Federated Analysis of Early Outbreak Data Applied to Incubation Period Estimation
• X-ray polarimetric features of Gamma-ray Bursts across varied redshifts and hints for Axion-Like-Particles
• Adaptation of the Phase Distance Correlation Periodogram to Account for Measurement Uncertainties
• Brightening and Fading in the Youngest Galactic Supernova Remnant G1.9+0.3: 13 years of monitoring with the Chandra X-ray Observatory
• Characterizing the Spectral Structure of Weak Impulsive Narrowband Quiet Sun Emissions
• Deep Learning Calabi-Yau four folds with hybrid and recurrent neural network architectures
• Ecology, Spatial Structure, and Selection Pressure Induce Strong Signatures in Phylogenetic Structure
• Multiphase Powerful Outflows Detected in High-z Quasars
• Optimal bolometer transfer function deconvolution for CMB experiments through maximum likelihood mapmaking
• QPOML: A Machine Learning Approach to Detect and Characterize Quasi-Periodic Oscillations in X-ray Binaries
• Blueshifted hydrogen emission and shock wave of RR Lyrae variables in SDSS and LAMOST
• General relativistic self-gravitating equilibrium disks around rotating neutron stars
• Topology Estimation of Simulated 4D Image Data by Combining Downscaling and Convolutional Neural Networks
• STag II: Classification of Serendipitous Supernovae Observed by Galaxy Redshift Surveys
• Demonstrating Quantum Homomorphic Encryption Through Simulation
• Systematics in ETG Mass Profile Modelling: Strong Lensing & Stellar Dynamics
• Multipoles of the galaxy bispectrum on a light cone: wide-separation and relativistic corrections
• Pattern formation by advection-diffusion in new economic geography
• The Continuous Tensor Abstraction: Where Indices are Real
• The Pascal Matrix, Commuting Tridiagonal Operators and Fourier Algebras
• Modeling the Far-Infrared Polarization Spectrum of a High-Mass Star Forming Cloud
• The Angular Correlation Function as measured by the GLEAM-X Survey
• Probing the Morphology of Polarized Emission Induced by Fluctuation Dynamo using Minkowski Functionals
• New Coevolution Dynamic as an Optimization Strategy in Group Problem Solving
• When did the initial mass function become bottom-heavy?
• VoDEx: a Python library for time annotation and management of volumetric functional imaging data
• Intensity and Dimensionality-Dependent Dynamics of Laser-Proton Acceleration in 1D, 2D, and 3D Particle-in-Cell Simulations
• Physics-enhanced neural networks for equation-of-state calculations
• SPORES-HWO. II. Companion Mass Limits and Updated Planet Properties for 120 Future Exoplanet Imaging Targets from 35 yr of Precise Doppler Monitoring
• Robust optimal design of large-scale Bayesian nonlinear inverse problems
• Lossy Image Compression with Stochastic Quantization
• Constraints on Weak Supernova Kicks from Observed Pulsar Velocities
• Effects of the internal temperature on vertical mixing and on cloud structures in Ultra Hot Jupiters
• Complex-Phase Extensions of Szegedy Quantum Walk on Graphs
• Photonic Simulation of Localization Phenomena Using Boson Sampling
• A Low Metallicity Massive Contact Binary Star System Candidate in WLM identified by Hubble and James Webb Space Telescope imaging
• Proteome-wide prediction of mode of inheritance and molecular mechanism underlying genetic diseases using structural interactomics
• The Bouc-Wen Model for Binary Direct Collinear Collisions of Convex Viscoplastic Bodies
• Observability of 2HDM charged Higgs boson in a misaligned scenario
• Asymmetric Distribution of the Solar Photospheric Magnetic Field Values
• Evidence that Planets in the Radius Gap Do Not Resemble Their Neighbors
• The calibrations of DAMPE $\gamma$-ray effective area
• lintsampler: Easy random sampling via linear interpolation
• Further Evidence for Tidal Spin-Up of Hot Jupiter Host Stars
• Novel computational approaches for ratio distributions with an application to Hake's ratio in effect size measurement
• Starkiller: subtracting stars and other sources from IFU spectroscopic data through forward modeling
• Float Self-Tagging
• Outer Solar System spacecraft to probe the $\mu$Hz gravitational wave frontier
• Modelling the Center-to-Limb systematic in normal-mode-coupling measurements
• Goupil: A Monte Carlo engine for the backward transport of low-energy gamma-rays
• Solar Mean Magnetic Field of the Chromosphere
• Metallicity estimation of RR Lyrae stars from their I-band light curves
• On the detectability and parameterisation of binary stars through spectral energy distributions
• Mean-field dynamo due to spatiotemporal fluctuations of the turbulent kinetic energy
• On volume density and star formation in nearby molecular clouds
• On the Relation between the Inclination Angle of the Accretion Disk and the Broad-line Region in Active Galactic Nuclei
• CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform
• CoSTI: Consistency Models for (a faster) Spatio-Temporal Imputation
• An Independent Search for Small Long-period Planets in Kepler Data I: Detection Pipeline
• NutMaat: A Python package for stellar spectral classification on the MK system
• Cosmic ray transport and acceleration in an evolving shock landscape
• Characterizing CO Emitters in the SSA22-AzTEC26 Field
• H I absorption line and anomalous dispersion in the radio pulses of PSR B1937+21
• Contaminating Electromagnetic Transients in LISA Gravitational Wave Localization Volumes. I: The Intrinsic Rates
• A Search for Low-frequency Radio Pulses from Long Gamma-ray Bursts with the Murchison Widefield Array
• Can we constrain galaxy geometry parameters using spatially integrated SED fitting?
• The Parallel Ionizing Emissivity Survey (PIE). I. Survey design and selection of candidate Lyman Continuum leakers at 3.1<z<3.5
• Impact of multi-messenger spectral modelling on blazar-neutrino associations
• Tidal disruption events as the origin of the eROSITA and Fermi bubbles
• Precise Parameters from Bayesian SED Fitting Indicate Thermally-Driven Mass Loss Likely Driver of Radius Valley
• A lattice pairing-field approach to ultracold Fermi gases
• clusttraj: A Solvent-Informed Clustering Tool for Molecular Modeling
• Tidal phenomena in the Galactic Center: The curious case of X7
• Lightning activity on a tidally locked terrestrial exoplanet in storm-resolving simulations for a range of surface pressures
• Search for the Optical Counterpart of Einstein Probe Discovered Fast X-ray Transients from Lulin Observatory
• Modeling Atmospheric Ion Escape from Kepler-1649 b and c over Time
• HI 21-cm Absorption Associated with Foreground Galaxies on Top of Quasars
• Atacama Cosmology Telescope: Observations of supermassive black hole binary candidates. Strong sinusoidal variations at 95, 147 and 225 GHz in PKS 2131$-$021 and PKS J0805$-$0111
• On the dependence of galaxy assembly bias on the selection criteria, number density, and redshift of galaxy samples
• A machine-learning photometric classifier for massive stars in nearby galaxies II. The catalog
• A new look into the atmospheric composition of WASP-39 b
• A local, topology-independent parameterization of quasar IGM damping wings
• The Mass Budgets and Spatial Scales of Exoplanet Systems and Protoplanetary Disks
• An Almost-FLRW Universe as the Averaged Geometry in Macroscopic Gravity
• Insights into the dependence of galaxy properties on the environment with explainable machine learning models
• First Light And Reionization Epoch Simulations (FLARES) -- XIX: Supermassive black hole mergers in the early Universe and their environmental dependence
• Early Stellar Flybys are Unlikely: Improved Constraints from Sednoids and Large-$q$ TNOs
• Identifying Astrophysical Anomalies in 99.6 Million Cutouts from the Hubble Legacy Archive Using AnomalyMatch
• Prospects for Reconstructing the Free-floating Planet Mass Function at the Population Level with the Nancy Grace Roman Space Telescope
• The Stripped-Star Ultraviolet Magellanic Cloud Survey (SUMS): The UV Photometric Catalog and Stripped Star Candidate Selection
• Impact of anisotropic photon emission from sources during the epoch of reionisation
• The polarimetric response of the Nançay Radio Telescope and its impact on precision pulsar timing
• Accelerated Nonnegative Tensor Completion via Integer Programming
• Searching for stars ejected from the Galactic Centre in DESI
• Detectability of massive binary black holes with sub-mHz gravitational wave missions
• TCT investigation of the one-sided depletion of low-temperature covalently bonded silicon sensor P-N diodes
• Black Hole - Neutron Star and Binary Neutron Star Mergers from Population III and II stars
• Neutrino masses, matter-antimatter asymmetry, dark matter, and supermassive black hole formation explained with Majorons
• On the calculation of p-values for quadratic statistics in Pulsar Timing Arrays
• Kinetic theory of coupled binary-fluid-surfactant systems
• Modern approaches to building interpretable models of the property market using machine learning on the base of mass cadastral valuation
• Engineering Precise and Robust Effective Hamiltonians
• Binary black holes in the heat of merger
• Black hole ringdown spectroscopy of curvature-coupled scalar and pseudoscalar fields
• Stability of a cluster-disrupted mean-motion resonance (chain) in HR 8799 and PDS 70
• Multi-cloud crushing -- the collective survival of cold clouds in galactic outflows
• First joint absorption and T${}_e$-based metallicity measured in a GRB host galaxy at $z=4.28$ using JWST/NIRSpec
• Non-transiting exoplanets as a means of understanding star-planet interactions in close-in systems
• Apache Point Observatory follow-up of ACcelerating Candidate ExopLanet host Stars (APO ACCELS): Ages for 166 Accelerating Stars in the Northern Hemisphere
• Studying the multi-phase interstellar medium in the Large Magellanic Cloud with SRG/eROSITA -- I. Analysis of diffuse X-ray emission
• Hunting for the nature of the enigmatic narrow-line Seyfert 1 galaxy PKS 2004-447
• LevelSetPy: A GPU-Accelerated Package for Hyperbolic Hamilton-Jacobi Partial Differential Equations
• Study of noise in virtual distillation circuits for quantum error mitigation
• LiteBIRD science goals and forecasts: improved full-sky reconstruction of the gravitational lensing potential through the combination of Planck and LiteBIRD data
• Gravitational Wave Peep Contributions to Background Signal Confusion Noise for LISA
• INTEGRAL, eROSITA and Voyager Constraints on Light Bosonic Dark Matter: ALPs, Dark Photons, Scalars, $B-L$ and $L_i-L_j$ Vectors
• Optical Counterparts to X-ray sources in LSST DP1
• Deriving thin-film averaged equations using computer algebra
• Quantum Machine Learning for Identifying Transient Events in X-ray Light Curves
• The Software Landscape for the Density Matrix Renormalization Group
• Obscured and unobscured X-ray AGNs I: Host galaxy properties
• Gas-Poor Hosts and Gas-Rich Companions of $z\approx$3.5 Radio Active Galactic Nuclei: ALMA Insights into Jet Triggering and Feedback
• Validation & Testing of the CROBAR 3D Coronal Reconstruction Method with a MURaM simulation
• Linking Multi-Site Sex Ad Data at the Individual Level to Aid Counter-Trafficking Efforts
• JWST/NIRSpec Observations of Salacia-Actaea and Máni: Exploring Population-level Trends among Water-ice-rich Kuiper Belt Objects
• Can Big Black Holes Merge with the Smallest Black Holes?
• MrMARTIAN: A Multi-resolution Mass Reconstruction Algorithm Combining Free-form and Analytic Components
• Revisiting the Radial Metallicity Gradient-Age Relation in the Milky Way's Thin and Thick Disks
• The role of migration traps in the formation of binary black holes in AGN disks
• Generalized Perturbed Kepler Problem: Gravitational Wave Imprints from Eccentric Compact Binaries
• Towards Accurate Asteroseismic Masses for Luminous Giants
• Stars Born in the Wind: M82's Outflow and Halo Star Formation
• Hyperparameter Optimization in the Estimation of PDE and Delay-PDE models from data
• The intragroup light in KiDS+GAMA groups: A stacking analysis
• AMBER: Algorithm for Multiplexing spectrometer Background Estimation with Rotation-independence
• Cross-Domain Evaluation of a Deep Learning-Based Type Inference System
• 200,000+ Deep Learning-inferred Periods of Stellar Variability from the All-Sky Automated Survey for Supernovae
• Early Stages of Dusty Tori: The First Infrared Spectra from a Highly Multiscale Quasar Simulation
• One latent to fit them all: a unified representation of baryonic feedback on matter distribution
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• STRAWBERRY: Finding haloes in the gravitational potential
• The Evolution and Internal Structure of Neptunes and Sub-Neptunes: The importance of thermal conductivity in non-convective regions
• The Galaxy Activity, Torus, and Outflow Survey (GATOS): N. Unveiling physical processes in local active galaxies. Unsupervised hierarchical clustering of JWST MIRI/MRS observations
• The impact of cosmic filaments on the abundance of satellite galaxies
• Characterizing the host galaxies and delay times of Ca-rich gap transients vs 91bg-like SNe and normal Type Ia SNe
• Correlating Visual Characteristics and Cryogenic Performance of Superconducting Detectors
• First Overtone Mode in the Ringdown Signal of GW231028
• NEXUS: A Search for Nuclear Variability with the First Two JWST NIRCam Epochs
• Stellar-activity analysis of the nearby M dwarf GJ 526. Multi-dimensional Gaussian-process modelling of RV, FWHM and S-index
• Investigation of mass substructure in gravitational lens system SDP.81 with ALMA long-baseline observations
• On the contribution of cosmic-ray interactions in the circumgalactic gas to the observed high-energy neutrino flux
• On the connection between nitrogen-enhanced field stars and the Galactic globular clusters
• Subgrid modelling of MRI-driven turbulence in differentially rotating neutron stars
• Exploring the History of Stellar Mergers with Chemistry: Examining the Origins of Massive $\alpha$-Enriched Stars using Carbon Isotope Ratios
• The large-scale kinematics of young stars in the Milky Way disc: first results from SDSS-V
• Numerical Modeling of Relativistic Effects in Synchrotron-Emitting Shocks
• AVISM: Algorithm for Void Identification in coSMology
• Untangling the Complex Nature of AGN Variability with Fairall 9
• Uncertainty and bias of cosmology and astrophysical population model from statistical dark sirens
• Impact of near-degeneracy effects on linear rotational inversions for red-giant stars
• Planet-driven density waves in protoplanetary discs: numerical verification of nonlinear evolution theory
• MUSEQuBES: Physical conditions, origins, and multi-element abundances of the circumgalactic medium of an isolated, star-forming dwarf galaxy at z=0.57
• SIGNALS of Giant HII Regions: A Spatially Resolved Analysis of NGC 604
• Rise of the forsaken relics: connecting present-day stellar streams and phase-mixed galaxies to the Epoch of Reionization
• Impact of Charge Transfer Inefficiency on transit light-curves: A correction strategy for PLATO
• Toward First-Principles Multi-Messenger Predictions: Coupling Nuclear Networks with GR Radiation-MHD in {\tt Gmunu}
• Radiatively Cooled Binary Mass Transfer: Flow Structure, Luminosities, and L2 Outflows Across Mass Transfer Rates
• A comprehensive look into the accuracy of SpEC binary black hole waveforms
• ParaToric 1.0: Continuous-time quantum Monte Carlo for the toric code in a parallel field
• The Formation of Dwarf Galaxy Disks
• Quasinormal modes from numerical relativity with Bayesian inference
• Deep JWST spectroscopy of galaxies in a candidate ionized bubble at $z=8.7$: probing reionization at pMpc scales with Ly$\alpha$ emission
• Resurging from the ashes: A spectral study of seven candidate revived radio fossils in nearby low-mass galaxy clusters
• Survival of the accretion disk in LMC Recurrent Nova 1968-12a: UV--X-ray case study of the 2024 eruption
• The Nearby Evolved Stars Survey III: First data release of JCMT CO-line observations
• The metallicity dependence of long-duration gamma-ray bursts
• The dynamics of S-stars and G-sources orbiting a supermassive compact object made of fermionic dark matter
• The imprint of gas on gravitational waves from LISA intermediate-mass black hole binaries
• RIGEL: Feedback-regulated cloud-scale star formation efficiency in a simulated dwarf galaxy merger
• Near the Runaway: The Climate and Habitability of Teegarden's Star b
• The Solar Neighborhood. LV. M Dwarf Twin Binaries -- One in Five Twin Sibling Pairs Are Mismatched in Activity and/or Rotation
• QUEST (Quasar Unsupervised Encoder and Synthesis Tool): A machine learning framework to generate quasar spectra
• The Next Generation Virgo Cluster Survey (NGVS). XL. The Morphological Classification of Virgo Cluster Galaxies
• The nature of ASASSN-24fw's occultation: modelling the event as dimming by optically thick rings around a sub-stellar companion
• Numerically stable evaluation of closed-form expressions for eigenvalues of $3\times 3$ matrices
• Machine Learning-Driven Analysis of kSZ Maps to Predict CMB Optical Depth $\tau$
• Enumeration of Autocatalytic Subsystems in Large Chemical Reaction Networks
• Chasing the storm: Investigating the application of high-contrast imaging techniques in producing precise exoplanet light curves
• Efficient Implementation of the Spin-Free Renormalized Internally-Contracted Multireference Coupled Cluster Theory
• When action is not least for systems with action-dependent Lagrangians
• Pulse profile modelling of the accretion-powered millisecond pulsar SAX J1808.4-3658 using NICER data from its 2019 and 2022 outbursts
• Disk fraction among free-floating planetary-mass objects in Upper Scorpius
• Revisiting wideband pulsar timing measurements
• Active learning emulators for nuclear two-body scattering in momentum space
• Cosmological simulations with rare and frequent dark matter self-interactions
• Low Frequency Marsquakes and Where to Find Them: Back Azimuth Determination Using a Polarization Analysis Approach
• The impact of relativistic corrections on the detectability of dark-matter spikes with gravitational waves
• The effects of alloy disorder on strongly-driven flopping mode qubits in Si/SiGe
• Flexible Gravitational-Wave Parameter Estimation with Transformers
• The impact of lunar topography on the 21-cm power spectrum for grid-based arrays : Insights for the Dark-ages EXplorer (DEX)
• A sensitivity analysis of interstellar ice chemistry in astrochemical models
• The mysterious Globular Cluster population of MATLAS-2019
• The Competing Influence of Ram Pressure and Tidal Interaction in NGC 2276
• Detection of Small Holes by the Scale-Invariant Robust Density-Aware Distance (RDAD) Filtration
• An Adaptive Distributed Stencil Abstraction for GPUs
• Impact of baryons on the population of Galactic subhalos and implications for dark matter searches
• VLBI Observations of SN 2012au Reveal a Compact Radio Source a Decade Post Explosion
• Mapping the Distorted Dark Matter Distribution of the LMC-SMC System Prior to Milky Way Infall with Basis Function Expansions
• Classical Be Stars and Classical Be Star Binaries from LAMOST DR12
• Fading Echoes of Interaction: Probing Centuries of Preexplosion Mass-Loss in Four Type IIn Supernovae
• GLIMPSE-D: Metallicity Decline in Faint Galaxies: Implications for [O III]+Hb Luminosity Function and Reionisation Budget
• Revealing massive black hole astrophysics: The potential of hierarchical inference with extreme mass-ratio inspiral observations
• A comprehensive search for high-velocity X-ray sources: New compact object binary candidates in the Gaia era
• Combined LOFAR-uGMRT analysis of the diffuse radio emission in the massive clusters Abell 773 and Abell 1351
• Constraints on gravitational waves from the 2024 Vela pulsar glitch
• Jas4pp -- a Data-Analysis Framework for Physics and Detector Studies
• Revisiting the Perseus Cluster II: Metallicity-Dependence of Massive Stars and Chemical Enrichment History
• The asymmetric structure of the inner disc around HD 142527 A with VLTI/MATISSE
• A FUV-optical approach for studying hierarchical star formation in nearby galaxies with UVIT
• VENUS: Strong-lensing model of MACS J1931.8-2635 -- revealing the farthest multiply imaged supernova
• Validation of standardized data formats and tools for ground-level particle-based gamma-ray observatories
• Narrow absorption lines from intervening material in supernovae: III. Supernovae and their environments
• An Archival Optical Counterpart Search for Extragalactic Fast X-Ray Transients Discovered by Einstein Probe
• Redundant is Not Redundant: Automating Efficient Categorical Palette Design Unifying Color & Shape Encodings with CatPAW
• All the Massive Galaxy Overdensities during Reionization: JWST Rest-Frame Optical Selection Reveals Young, Chemically Evolved Galaxies Embedded in Dense, Neutral Gas at z > 5
• Towards an optimal extraction of cosmological parameters from galaxy cluster surveys using convolutional neural networks
• ARCHITECTS I: Impact of subgrid physics on the simulated properties of the circumgalactic medium
• Between Plateaus and Slopes: A Data-Driven Exploration of Spectral Diversity Across Type IIP/L Supernovae
• Illuminating the Mass Gap Through Deep Optical Constraint on a Neutron Star Merger Candidate S250206dm
• Linear filament and nested cluster evolution tomography (LANCET) I. Capture the evolution of dense gas in 14-parsec filament G316.8
• On the Frobenius number of certain numerical semigroups
• Probing Heavily Obscured AGN in Major Galaxy Mergers Using the mm-X-ray Correlation
• Halo Photometry and Asteroseismology for 98 of the Brightest Stars Observed by TESS
• The LOFAR sub-arcsecond view of the high-redshift radio relic in PSZ2G091.83+26.11
• Discovery of a runaway star likely ejected by a Type Iax Supernova
• The velocity dispersion function of red galaxies in four Hubble Frontier Fields galaxy clusters
• A Panchromatic JWST Spectrum of a Giant Starspot on the Fully Convective M-dwarf TOI-3884
• Neutrino mass limits and decaying dark matter: background evolution versus perturbations
• Quantifying the Milky Way, LMC and their interaction using all-sky kinematics of outer halo stars
• Quantifying yeast colony morphologies with feature engineering from time-lapse photography
• The ALPINE-CRISTAL-JWST Survey: Gas-phase abundance gradients of main sequence star-forming galaxies and their kinematics at $4<z<6$
• Vertical Structure of Protoplanetary Disks in Scattered Light: A large sample analysis
• Ashes of FIRE: Modeling Dust Grain Size Evolution in the Local Group with FIRE
• MUSE-DARK-II: 3D morpho-kinematic modelling of lensed galaxies. Tully-Fisher relation of $z\sim 1$ star-forming galaxies
• The CAVITY project. The spatially resolved SFR of galaxies in voids
• The Star Formation Factory revisited I. The impact of metallicity on collapsing star-forming clouds
• Hyperaccreting Neutron Stars inside Massive Envelopes: The Implausibility of Thorne-Żytkow Objects
• Improving INTEGRAL/SPI data analysis of GRBs
• The Hierarchical Structure of Galactic Haloes: Generalised N-Dimensional Clustering with CluSTAR-ND
• Identifying Changing-Look AGN Transitions in Light Curve Data with the Zwicky Transient Facility
• Icy Volatile Enhancements in Evolving Protoplanetary Disks
• Discovery of the First Octupole Pulsation Mode in a delta Scuti Star: A Stationary l = 3 Sectoral Mode
• Radio detection of supernova remnant G310.7-5.4 with $\gamma$-ray counterpart: Abeona SNR
• Analytic Inverse Design of Temporal Metamaterials via Space-Time Duality
• Characterizing the bolometric-photoevaporative transition in young sub-Neptunes with radiation-hydrodynamic simulations
• JWST Observations of Starbursts: Dust Processing in the M82 Superwind
• A fast tree algorithm for multi-component coagulation equation
• On The Nonthermal Power Laws In Magnetized Turbulent Plasmas
• A Validated Low-to-Intermediate Mass Planetary Interior Structure Model and New Mass-Radius Relations
• Lifetimes and Rotation within the Solar Mean Magnetic Field
• uGMRT and MeerKAT observation of RXCJ0232-4420: a quiet cluster with a giant radio halo
• On the Relationship between Solar Spicules and Propagating Coronal Disturbances: The Role of Shocks
• HETDEX Public Data Release 1: Source Catalog 2 and Data Cubes from ~90 sq deg of Integral-Field Optical Spectroscopy
• Direct detection of cool molecular gas in a star-forming galaxy at $z=7.31$
• Primordial Black Hole Triggered Type Ia Supernovae II: Comparison with Supernova Remnants and Galactic Chemical Evolution
• The Tale of a Hungry Subgiant and Its Brown Dwarf: Interior Radiative Damping Dominates the Tidal Evolution of TOI-5882
• Atmospheric asymmetries in WASP-121 b revealed by rotational transits detected with JWST
• Hadronic Processes, Plasma Evolution and Neutrino Emission in Magnetic Towers of Neutron-Star Merger Remnants
• KRONOS I: The $1-2.8\mu$m JWST Transmission Spectrum of the 23 Myr V1298 Tau c
• The NANOGrav 15 yr Data Set: Customized Chromatic Noise Models
• Euclid: Discovery of 31 new quasars at $6.6<z<7.8$
• Pre-flare and active region plasma flows and structure seen by the short wavelength camera on SOLAR-C/EUVST
• Direct Imaging Discovery of Giant Exoplanet $\beta$ Pictoris d: A Decade-Long Game of Hide-and-Seek
• Tracing black hole and galaxy growth across environments since cosmic noon
• Transverse Oscillations and Wave Propagation in the Magnetically Dominated M87 Jet
• Multicellular Tumour Spheroids Exposure to Pulsed Electric Field: A Combined Experimental and Mathematical Modelling Study Highlighting Temporal Dynamics of DAMP Release and Accelerated Regrowth at Intermediate Field Intensities
• Mid-infrared Variability-based AGN Selection using the Multi-epoch Photometric Data from WISE
• Measuring the evolution of stellar bars with the host galaxy's spin
• exoALMA XX: Tomographic Detection of Embedded Planets in Protoplanetary Disks
• The Environments of Star-Forming Galaxies Detected in the SFACT Survey: Do Mergers and Interactions Drive the Star Formation?
• Stellar age determination using deep neural networks: Isochrone ages for 1.3 million stars, based on BaSTI, MIST, PARSEC, Dartmouth and SYCLIST evolutionary grids
• Centaur 2013 VZ70: Debris from Saturn's irregular moon population?
• Mock Observations of Multiple Stellar Populations in Tidal Streams of Palomar 5 for the Chinese Space Station Survey Telescope
• Direct Images of CO2 Absorption in the Atmosphere of a Super-Jupiter: Enhanced Metallicity Suggestive of Formation in a Disk
• Learn&Drop: Fast Learning of CNNs based on Layer Dropping
• The dark and featureless surface of rocky exoplanet LHS 3844 b from JWST mid-infrared spectroscopy
• Spectral component imaging of solar X-ray flares
• Measuring Dust Masses of Protoplanetary Disks in Serpens and L1641/L1647 with ALMA
• The dark matter wake of a galactic bar revealed by multichannel Singular Spectral Analysis
• Shock-type inference of L1157 B2 using methanol desorption
• The X-ray/UV Connection in NGC 5548: A Rapidly Varying Corona
• The SNIa Runaway LP 398-9: Detection of Circumstellar Material and Surface Rotation
• Confirming the Magnetic Field Detection at the Surface of $\chi$ Cyg
• Classification of a New X-ray Catalog of Likely Counterparts to 4FGL-DR4 Unassociated Gamma-ray Sources Using a Neural Network
• A one-parameter two-zone leptonic model for the blazar sequence
• Meta-learners for few-shot weakly-supervised optic disc and cup segmentation on fundus images
• Evidence of Possible Spectral Variability in the Patroclus-Menoetius Binary System
• CoSeNet: A Novel Approach for Optimal Segmentation of Correlation Matrices
• Scalable Stellar Parameter Inference Using Python-based LASP: From CPU Optimization to GPU Acceleration
• Covertly Active Comet (139359) 2001 ME1
• The mass distribution in and around the Local Group
• Periodic 6.7 GHz $\mathrm{C}{\mathrm{H}}_3\mathrm{OH}$ maser emission in G353.273+0.641: First candidate for a pulsating high-mass protostar
• A framework for modeling the evolution of young stellar objects
• Photometric Mapping of Carbonaceous/Siliceous Dust and Water Ice in the ISM with JWST: Applications to the Dense Sightlines
• 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
• A Dormant Captured Oort Cloud Comet Awakens: (18916) 2000 OG44
• Radio Variability in Recently-Quenched Galaxies: The Impact of TDE or AGN Driven Outflows
• Galaxy And Mass Assembly (GAMA): From filaments to voids, how extreme environment affects gas metallicity and SFR in galaxies
• Rotation Curves in z~1-2 Star-Forming Disks: Comparison of Dark Matter Fractions and Disk Properties for Different Fitting Methods
• Silicate Sundogs: Probing the Effects of Grain Directionality in Exoplanet Observations
• New Metrics for Identifying Variables and Transients in Large Astronomical Surveys
• 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
• Optimizing Convolution Direction and Template Selection for Difference Image Analysis
• PyNoetic: A modular python framework for no-code development of EEG brain-computer interfaces
• Active region upflows in various coronal structures and their coupling to the lower atmosphere
• A Diagnostic Kit for Optical Emission Lines Shaped by Accretion Disc Winds
• Chemodynamics of BoötesI with $S^5$: Revised Velocity Gradient, Dark Matter Density, and Galactic Chemical Evolution Constraints
• NIHAO-LG: The uniqueness of Local Group dwarf galaxies
• Survey of Profile Parameters of the $6196\mathring{A}$ Diffuse Interstellar Band. From Uniform Profiles to Doppler Splitting and Blueshifts
• On the origin of super-global spin-up trends of X-ray pulsars in HMXB systems
• An Interpretable AI Framework to Disentangle Self-Interacting and Cold Dark Matter in Galaxy Clusters: The CKAN Approach
• Dusty Clump Survival in Supernova Ejecta: Dust-Mediated Growth vs. Crushing by the Reverse Shock
• Optimal message passing for molecular prediction is simple, attentive and spatial
• The periodicity of three-dimensional oscillatory reconnection
• Unequal-mass mergers of dark matter haloes with rare and frequent self-interactions
• The Influence of Central Body Tides on Catastrophic Disruptions of Close-in Planetary Satellites
• Selecting Clusters and Protoclusters via Stellar Mass Density: II. Application to HSC-SSP Observations
• Selecting Clusters and Protoclusters via Stellar Mass Density: I. Method and tests on Mock HSC-SSP catalogs
• NGTS-EB-8: A double-lined eclipsing M+M binary discovered by citizen scientists
• Milky Way Mass Through Escape Velocity Curve from LAMOST K Giants
• Enhanced Astrometry of the Rapid ASKAP Continuum Survey for Precise Localisation of Fast Radio Bursts
• A Search for Planetary Metastable Helium Absorption in the V1298 Tau System
• ASAS-SN search for optical counterparts of gravitational-wave events from the third observing run of Advanced LIGO/Virgo
• CY Aquarii: A Triple System with Twin Companions
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• First IFU observations of two GRB host galaxies at cosmic noon with JWST/NIRSpec
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• Numerical Simulations of the Random Angular Momentum in Convection: Implications for Supergiant Collapse to Form Black Holes
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• Estimating Stellar Atmospheric Parameters and [α/Fe] for LAMOST O-M type Stars Using a Spectral Emulator
• A study on late time UV-emission in core collapse supernovae and the implications for the peculiar transient AT2018cow
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• Phase-resolved Hubble Space Telescope WFC3 Spectroscopy of Weakly-Irradiated Brown Dwarf GD 1400 and Energy Redistribution-Irradiation Trends in Six WD$-$BD Binaries
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• Constraining the shape of dark matter haloes using only starlight. I. A new technique and its application to the galaxy Nube
• TelescopeML -- I. An End-to-End Python Package for Interpreting Telescope Datasets through Training Machine Learning Models, Generating Statistical Reports, and Visualizing Results
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• Accelerating key bioinformatics tasks 100-fold by improving memory access
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• The Gaia Ultracool Dwarf Sample -- IV. GTC/OSIRIS optical spectra of Gaia late-M and L dwarfs
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• A MultiWavelength Study of the Symbiotic Mira HM Sge with SOFIA and HST
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• Ground-Based Mid-IR Direct Imaging: The Origin of the Thermal Background on the Keck II Telescope and Correcting Instrumental Systematics
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• The Solar System Notification Alert Processing System (SNAPS): Asteroid Population Outlier Detection
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• Time Delay Cosmography: Analysis of Quadruply Lensed QSO SDSSJ1433 from Wendelstein Observatory
• Calibration of the ComPair Balloon Instrument
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• The effect of near-core mixing on rejuvenation and the asteroseismic properties of massive accretors
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• Resolving the fastest ejecta from binary Neutron Star mergers: implications for electromagnetic counterparts
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• A preliminary exploration of the effects of baseline length for the LIFE space mission
• Investigating the young stellar populations and hierarchies in nearby galaxies with the UVIT. II. Presenting the properties of ~25,000 UV-detected star-forming clumps
• Planetary Rhythms: Synchronous Circulation on Variably Irradiated Asynchronous Planets
• The GALAH Survey: Neutron-Capture Elemental Abundances for 350,000 Gaia-RVS spectra and the Chemodynamics of Accreted Structures
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• Initiation of Superradiance from Different Collective-Spin States
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• First Detection of HC5N in a Class II Disk around TW Hya
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• An Automated Photometric Pipeline for the 80cm Xizang University Telescope
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• Scattered light signatures of flyby-induced warps in protoplanetary discs
• X-class flare on Dec 31, 2023, observed by the Solar Ultraviolet Imaging Telescope on board Aditya-L1
• Parameter resolution of near-Earth asteroids using LISA
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• Light Deflection under the Gravitational Field of Jupiter -- Testing General Relativity
• The Ellis and Baldwin test of the Cosmic Dipole: Exploring the impact of multiple flux density cuts
• The FAST Hundred-Deg${}^2$ HI Deep (HD${}^2$) Survey: Early Results from the Pilot Survey
• Probing growth precursor diffusion lengths by inter-surface diffusion
• BrahMap: A scalable and modular map-making framework for the CMB experiments
• Resolved properties of a luminous "hinge clump" in the compact group of galaxies NGC\,6845
• Pushing the Limit of Asteroseismic Detection for Cool Dwarfs using TESS and Deep Learning
• Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa$\beta$ narrow-band imaging
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• Bulgeless Evolution And the Rise of Discs (BEARD) III. A numerical simulation view of satellites around Milky-Way analogues
• OrganicHAR: Towards Activity Discovery in Organic Settings for Privacy Preserving Sensors Using Efficient Video Analysis
• No Stream Left Unscathed: The imprint of a host galaxy
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• Study of the Inner Structure of the Molecular Torus in IRAS 08572+3915 NW with Velocity Decomposition of CO Rovibrational Absorption Lines
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• Detecting inhomogeneous chiral condensation from the bosonic two-point function in the $(1+1)$-dimensional Gross-Neveu model in the mean-field approximation
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• TESS Data for Asteroseismology: Photometry
• Distance estimation of the high-velocity cloud Anti-Center Shell
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• Decay of acoustic turbulence in two dimensions and implications for cosmological gravitational waves
• The ALMA survey to Resolve exoKuiper belt Substructures (ARKS) XI: Gas-dust interactions and radial offsets between micron and millimetre-sized grains
• Which molecule traces what: chemical diagnostics of protostellar sources
• JWST high-contrast spectroscopy with speckle modelling: Atmospheric retrievals of the T dwarf companion HD 19467 B
• The Treasury of Extremely Metal-Poor O Stars
• Redshifts of Objects near 3C 220.3
• A Homogeneous Catalog of Rossiter-McLaughlin Systems: Distinct $e$-$\lambda$ Trends in Three Gas-Giant Mass Regimes
• Time-resolved JWST Retrieval Analysis of the Coldest Brown Dwarf: Temperature and Chemical Variations in WISE 0855-07
• A Minute-Cadence Deep Bulge Survey: First Data Release of DREAMS
• Hadronic Scenario for Galactic PeVatron LHAASO J1912+1014u Supported by Fermi-LAT $\gamma$-ray Data and FUGIN CO Data
• Tilsotua: Reproducing Slitmask Sky Positions for use with the LRIS Multislit Archive
• Environmental Sculpting of Galaxy Structure at Fixed Stellar Mass: A Multi-Scale Analysis Across Cosmic Time using 3 Million HSC Galaxies
• Clustering redshifts with the 21cm-galaxy cross-bispectrum
• Subluminous Type IIP SN 2024abfl as a Result of a Significantly Low-energy Fe-core Collapse
• Exploring the gaseous halos of z>3 radio galaxies with UVES and JWST/NIRSpec
• Three-dimensional transport-induced chemistry on temperate sub-Neptune K2-18b, Part II: the combined effects of atmospheric dynamics and chemical reactions
• Testing OH Megamaser Identification Methods in HI Surveys: Updated Source-Flagging Algorithms and New Detections in ALFALFA
• Impact of Massive Binary Star and Cosmic Evolution on Gravitational Wave Observations II: Double Compact Object Rates and Properties
• Evidence for Environmental Stripping in the Coma Cluster
• SDSS-V LVM: Verifying what, and where, the 'Galactic Center' Lobe is
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• Acoustic instability at shock-wave precursors
• Physical Conditions in the LMC's Quiescent Molecular Ridge: Fitting Non-LTE Models to CO Emission
• Resolving circumgalactic gas flows around a z$\approx$3.6 quasar using MUSE and ALMA
• Inversion of Hydrogen-rich Atmosphere and Water Content for GJ 486b
• An XMM-Newton Analysis of the Supermassive Black Hole Binary Candidate MCG+11--11--032
• Phase spirals induced by the gas warp
• Ability-Based Methods for Personalized Keyboard Generation
• The Delay Time Distribution of Tidal Disruption Events
• Lecture notes on Machine Learning applications for global fits
• Correctness criteria for complex Langevin
• An Overview of CHIME, the Canadian Hydrogen Intensity Mapping Experiment
• Underlying mechanisms of phase transitions in scalar-tensor theories
• Response approach to the integrated shear 3-point correlation function: the impact of baryonic effects on small scales
• First Trigonometric Parallax Measurements with the KVN and VERA Array (KaVA)
• CORSIKA 8: A General Framework for Particle Cascade Simulations
• Could the high-mass black holes from gravitational-wave observations be explained by lensing?
• Information content of JWST transmission spectroscopy of the exoplanet HAT-P-12b from the optical to the mid-infrared
• Discovery and Detailed Study of the M31 Classical Nova AT 2023tkw: Evidence for Internal Shocks
• Observations of Uranus at High Phase Angle as Seen by New Horizons
• A multi-fluid approach for polydisperse pebble accretion: From particles to fluids, establishing the multifluid framework
• Imladris: a detailed and flexible model for galaxy simulations with individual stars
• Multi-tasking through quantum annealing
• A Robust Framework for Secure Cardiovascular Risk Prediction: An Architectural Case Study of Differentially Private Federated Learning
• The miniJPAS survey quasar selection I: Mock catalogues for classification
• A novel Cosmic Filament catalogue from SDSS data
• A ready-to-deploy MLOps software platform for satellite and NEO detection at meter-class ground-based observatories
• Imprints of tidal interactions on the stellar distribution of satellite galaxies: implications for dark matter deficient galaxies
• Serial MultiView: an efficient approach to mitigating atmospheric spatial-structure errors for VLBI astrometry
• Resizing the giants: How modelling adiabatic interiors impacts predicted planetary radii
• Spectroscopic Modeling of Luminous Transients Powered by H-Rich and He-Rich Circumstellar Interaction
• The Progenitor Systems of Classical Novae in M31
• Bias on Tensor-to-Scalar Ratio Inference With Estimated Covariance Matrices
• Irregular Repeating Tidal Disruption Events due to Diffusive Tides
• A machine learning approach to estimate mid-infrared fluxes from WISE data
• Constraining the synchrotron peak and estimating the VHE brightness of a sample of extreme high synchrotron peak blazars
• Test of the Statistical Isotropy of the Universe using Gravitational Waves
• Sulfur fractionation in coronal plumes as observed by Solar Orbiter/SPICE
• A Modernized View of Coherence Pathways Applied to Magnetic Resonance Experiments in Unstable, Inhomogeneous Fields
• Are Stellar Embryos in Perseus Radio-Synchrotron Emitters? Statistical data analysis with Herschel and LOFAR paving the way for the SKA
• Stellar associations powering HII regions $\unicode{x2013}$ II. Escape fraction of ionizing photons
• On the Importance of the Convective Urca Process in 3D Simulations of a Simmering White Dwarf
• Zandpack: A General Tool for Time-dependent Transport Simulation of Nanoelectronics
• On the detection of stellar wakes in the Milky Way: a deep learning approach
• Highly Efficient Selection of High-Redshift Emission-Line Galaxies for future DESI-like surveys with Deep Multi-band Imaging
• NIRPS tightens the mass estimate of GJ 3090 b and detects a planet near the stellar rotation period
• A "Hyperburst" in the MAXI J0556-332 Neutron Star: Evidence for a New Type of Thermonuclear Explosion
• Solar-like dynamos and rotational scaling of cycles from star-in-a-box simulations
• A Single Line-Emitter Identified in an Unbiased Search with JWST/NIRSpec: Multi-Object Coronagraphy for Slitless Spectroscopy
• First statistical constraints on galactic scale outflows properties traced by their extended Mg II emission with MUSE
• Fluctuation dynamos in supersonic turbulence at $\mathrm{Pm}\gtrsim 1$
• ABCMB: A Python+JAX Package for the Cosmic Microwave Background Power Spectrum
• Probabilistic modeling of Cherenkov emission from particle showers
• A Young Supernova Selection Pipeline For The LSST Era
• Ion-Scale Solitary Structures in the Solar Wind Observed by Solar Orbiter and Parker Solar Probe
• 3D elemental abundances of stars at formation across the histories of Milky Way-mass galaxies in the FIRE simulations
• The Atacama Cosmology Telescope: Extragalactic Point Sources in the Southern Surveys at 150, 220 and 280 GHz observed between 2008-2010
• Kinematic Evidence for Open Cluster Origins of Galactic Binary Neutron Stars
• Identifying Host Galaxies of Binary Black Hole Mergers with Next-Generation Gravitational Wave Detector Networks
• Heavy interstellar scattering toward the near end of the Galactic bar
• Quantum Machine Learning with SQUID
• Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
• Uncovering subdominant multipole asymmetries in binary black-hole mergers
• Deep Learning Pose Estimation for Multi-Label Recognition of Combined Hyperkinetic Movement Disorders
• An infrared echo from a circumstellar disk in the hydrogen- and helium-poor SN 2024aecx
• Atmospheric characterization of HIP 67522 b with VLT/CRIRES+. VLT/CRIRES+ suggests a heavier planet and hints at deuterium fractionation
• Assessing membership projection errors in star forming regions
• Revisiting the Perseus Cluster III: Role of Aspherical Explosions on its Chemical Composition and Extension to Metal-Poor Stars and Galaxies
• Unveiling BLR Structure in AGN with High Resolution X-Ray Spectra: An Analytic Approach to Wind Emission Line Profiles
• PlotChain: Deterministic Checkpointed Evaluation of Multimodal LLMs on Engineering Plot Reading
• Metallicity Structure in Galactic Longitude-Velocity Diagrams of the Milky Way Disk and FIRE-2 Simulations
• Local environmental dependence on weak-lensing shear statistics
• Constraining Nuclear Molecular Gas Content with High-resolution CO Imaging of GOALS Galaxies
• Optical lattice with spin-dependent sub-wavelength barriers
• Constraining the selection corrected luminosity function and total pulse count for radio transients
• Primordial helium-3 redux: The helium isotope ratio of the Orion nebula
• Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations
• Causal inference in time series in terms of Rényi transfer entropy
• Dynamical mass determination and partial eclipses of the heartbeat star HD 181793
• EstrellaNueva: an open-source software to study the interactions and detection of neutrinos emitted by supernovae
• The SOL $\text{(Solar Origin and Life)}$ Project: Detailed characterization of candidates for the ZAMS and Subgiant stages
• Radio continuum emission from a tidal dwarf galaxy
• Modelling the Utility of Group Testing for Public Health Surveillance
• The Sequential Monte Carlo goes NUTS: Boosting Gravitational-Wave Inference
• Diffusion in quantum state preparation: From passive cooling to system-bath engineering
• Limitations for adaptive quantum state tomography in the presence of detector noise
• A joint voxel flow-phase field framework for ultra-long microstructure evolution prediction with physical regularization
• Constraining Lorentz and parity violations in gravity with multiband gravitational wave observations
• Data-driven quasiconformal morphodynamic flows
• Reconsidering the consistent use of precessing, higher order multipole models for gravitational wave analyses
• Ultraviolet Spectroscopy and TARDIS Models of the Broad-lined Type-Ic Supernova 2014ad
• BE Lyncis: A Pulsating Star in the Most Eccentric Binary with a Massive Unseen Companion
• A NuSTAR Census of the X-ray Binary Population of the M31 Disk
• PISCOLA: a data-driven transient light-curve fitter
• Quantifying Symmetry: Transformation Information for Planetary Nebulae and Supernova Remnants
• EWOCS-V: Is Wd1-72 a recent post-interaction WR+O binary?
• A closer look at the young stellar group around Sh 2-295
• The impact of selection criteria on the properties of green valley galaxies
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• Structural parameters and possible association of the Ultra-Faint Dwarfs Pegasus III and Pisces II from deep Hubble Space Telescope photometry
• SemanticBridge - A Dataset for 3D Semantic Segmentation of Bridges and Domain Gap Analysis
• The Multiband Imaging Survey for High-Alpha PlanetS (MISHAPS) I: Preliminary Constraints on the Occurrence Rate of Hot Jupiters in 47 Tucanae
• Maximum likelihood estimation of log-affine models using detailed-balanced reaction networks
• MOA-2020-BLG-135Lb: A New Neptune-class Planet for the Extended MOA-II Exoplanet Microlens Statistical Analysis
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• Classification of Radio Backgrounds at Cosmic Dawn and 21 cm Signal Confirmation Using Neural Networks
• LibppRPA: An Open-Source Library for Particle-Particle Random Phase Approximation
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• Across the Universe: GW231123 as a magnified and diffracted black hole merger
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• Hubble Expansion Signature on Simulated Halo Density Profiles: A Path to Observing the Turnaround Radius
• Measurements of quasar proximity zones with the Ly$\alpha$ forest of DESI Y1 quasars
• MUSE Analysis of Gas around Galaxies (MAGG) -- VII. Emission line galaxies near strong blended Ly$\alpha$ absorption systems at $z\gtrsim 3$
• Three topologies of deep neural networks for pulse height extraction
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• libyt: an In Situ Interface Connecting Simulations with yt, Python, and Jupyter Workflows
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• The frame-dragging vector potential on galaxy scales from Dark-Matter-only Newtonian $N$-body simulations
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• DRAGNs in the Forest: Identifying Artifacts with Random Forest Models in the VLASS DRAGNs Catalog
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• The Directly-Imaged Exoplanet Host Star 51 Eridani is a Gamma Doradus Pulsator
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• Improving Photometric Galaxy Clustering Constraints With Cross-Bin Correlations
• Deprojection of external barred galaxies from photometry
• Stellar Cores Live Long and Prosper in Cuspy Dark Matter Halos
• Skykatana: a scalable framework to construct sky masks for the Vera Rubin Observatory and large astronomical surveys
• φ-FD : A well-conditioned finite difference method inspired by φ-FEM for general geometries on elliptic PDEs
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• Resolving the large exoKuiper belt of the HD 126062 debris disc and extended gas emission in its vicinity
• Particle loads for cosmological simulations with equal-mass dark matter and baryonic particles
• Estimation of the lifetime of slow-decaying unipolar active regions in the framework of the turbulent erosion model
• Lees-Edwards boundary conditions for translation invariant shear flow: implementation and transport properties
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• eminus -- Pythonic electronic structure theory
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• Revealing the Connection Between the Filamentary Hierarchy and Star Cluster Formation in a Simulated NGC 628 Galaxy
• Learning Post-Newtonian Corrections from Numerical Relativity
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• The $N_H$ Distribution of Hard X-ray Selected AGN in the NEP Field
• DeepZipper II: Searching for Lensed Supernovae in Dark Energy Survey Data with Deep Learning
• Modelling the secular evolution of proto-planetary disc dust sizes -- A comparison between the viscous and magnetic wind case
• Equivariant Machine Learning Decoder for 3D Toric Codes
• The AMBRE Project: Line-broadening and stellar rotation of ESO/FEROS archived spectra
• Advancing multivariate time series similarity assessment: an integrated computational approach
• The Covariance of Photometric and Spectroscopic Two-Point Statistics: Implications for Cosmological Parameter Inference
• On the dwarf irregular galaxy NGC 6822. I. Young, intermediate and old stellar populations
• RydIQule Version 2: Enhancing graph-based modeling of Rydberg atoms
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• VERCEL: Verification and Rectification of Configuration Errors with Least Squares
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• Mitigating gain calibration errors from EoR observations with SKA1-Low AA*
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• Searching for Exotrojans in Pulsar Systems
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• The Simons Observatory: Studies of Phase Drift in RF Transmission Lines from the First Large-Scale Deployment of Microwave Frequency Multiplexing for Cosmology
• The Role of High-mass Stellar Binaries in the Formation of High-mass Black Holes in Dense Star Clusters
• Non-linear infusion of intrinsic alignment and source clustering: impact on non-Gaussian cosmic shear statistics
• Characterizing Timing Parameters in Commercial SERF-OPM Multichannel Systems for Biomagnetic Field Sensing
• SDSS-IV MaNGA: Data-Model Discrepancy in Temperature-sensitive Line Ratios for Star-forming Galaxies
• Optimal observational scheduling framework for binary and multiple stellar systems
• Global sampling of Feynman's diagrams through Normalizing Flow
• Testing the effect of progenitor's metallicity on ${}^{56}$Ni mass and constraining the progenitor scenarios in Type Ia supernovae
• Classification of abrupt changes along viewing profiles of scientific articles
• A User-Friendly Python Interface for the Numerical Relativity Code AMSS-NCKU
• Filter Function Formalism and Software Package to Compute Quantum Processes of Gate Sequences for Classical Non-Markovian Noise
• CONCERTO: forward modeling of interferograms for calibration
• Detection of HI filament: Pair Stacking vs. Filament Stacking
• Topological Components in a Community Currency Network
• Free-Free Gaunt factors for atmospheres of accreting pulsars observable with X-ray space missions
• Overcoming Separation Between Counterparts Due to Unknown Proper Motions in Catalogue Cross-Matching
• Lensed stars in galaxy-galaxy strong lensing -- a JWST prediction for the Cosmic Horseshoe
• Stochastic modelling of cosmic-ray sources for Galactic diffuse emissions
• The Nature of High-Redshift Massive Quiescent Galaxies -- Searching for RUBIES-UDS-QG-z7 in FLARES
• Exciting Stellar Eccentricity in Gaia BH3 via a Hidden Black Hole Binary
• The orbital dynamics of the LMC and SMC about the Milky Way
• Bar Evolution in Edge-on Galaxies: A Demographic Study of Boxy/Peanut Bulges
• Efficient tau-pair invariant mass reconstruction with simplified matrix element techniques
• Generation of Lognormal Synthetic Lyman-$\alpha$ Forest Spectra for $P_{1D}$ Analysis
• Probing the Cosmological Principle with CMB lensing and cosmic shear
• Spatio-Temporal Look-Ahead Trajectory Prediction using Memory Neural Network
• AwkwardForth: accelerating Uproot with an internal DSL
• XClass: An Automated Multiwavelength Machine-Learning Pipeline for Classification of Extragalactic X-ray Sources. I. Pipeline Description
• Precise Constraints on the Energy Budget of WASP-121 b from its JWST NIRISS/SOSS Phase Curve
• A Log-Linear Analytics Approach to Cost Model Regularization for Inpatient Stays through Diagnostic Code Merging
• Coupled-channel meson-meson scattering in the diabatic framework
• Thermal Sunyaev-Zel'dovich effect at the core of CL J1226.9+3332 revealed by NOEMA
• Sarc-Graph: Automated segmentation, tracking, and analysis of sarcomeres in hiPSC-derived cardiomyocytes
• Astrophotometric search for massive stars in the Milky way. Confronting Random Forest predictions with available spectroscopy
• Quantum Monte Carlo and Stabilizer States
• First constraints on the local ionization topology in front of two quasars at z ~ 7.5
• One, Two, Three: One empirical evaluation of a two-copy shadow tomography scheme with triple efficiency
• The DeepFMKit Python package: A toolbox for simulating and analyzing deep frequency modulation interferometers
• PHIP Sequences and Dipolar Fields
• The Calar Alto CAFOS Direct Imaging First Data Release
• Dynamical orbital evolution scenarios of the wide-orbit eccentric planet HR 5183b
• Deciphering the explosion mechanism of Type-Ia SNe using their remnants I: general properties and a case study on Tycho's SNR
• Forming Double Neutron Stars using Detailed Binary Evolution Models with POSYDON: Comparison to the Galactic Systems
• When Stars Mimic Monsters: Spectral Evidence for an $\eta$ Carinae-like Giant Eruption in SBS 0335$-$052 E
• Tracking the Source of Solar Type II Bursts through Comparisons of Simulations and Radio Data
• Constrained free energy minimization for the design of thermal states and stabilizer thermodynamic systems
• The Impact of Powerful Jets on the Far-infrared Emission of an Extreme Radio Quasar at z~6
• SPAN: A cross-platform Python GUI software for optical and near-infrared spectral analysis
• Magnetic Hysteresis Experiments Performed on Quantum Annealers
• HIP 67506 C: MagAO-X Confirmation of a New Low-Mass Stellar Companion to HIP 67506 A
• Redshift ~2.7 is not special
• Random Variate Generation with Formal Guarantees
• Turbulent transport regimes in the presence of an X-point magnetic configuration
• Sample Variance Denoising in Cylindrical 21-cm Power Spectra
• Efficient neutral-IGM inference from noisy 21-cm forest spectra with latent-space U-Net encoding and XGBoost
• Shared-optical-path VLBI frequency phase transfer from 86 to 258 GHz on an 8600 km baseline: Demonstrated with the APEX and IRAM 30 m telescopes
• YALTAPy and YALTAPy_Online: Python toolboxes for the $H_{\infty }$-stability analysis of classical and fractional systems with commensurate delays
• AdeptHEQ-FL: Adaptive Homomorphic Encryption for Federated Learning of Hybrid Classical-Quantum Models with Dynamic Layer Sparing
• Broad-band Spectral Modeling of Prompt Emission from Gamma-Ray Bursts Observed by the Transiting Exoplanet Survey Satellite
• Evolution of the ZTF SLRN-2020 star-planet merger
• SLEPLET: Slepian Scale-Discretised Wavelets in Python
• Estimating Free Parameters in Stochastic Oscillatory Models Using a Weighted Cost Function
• An Algorithm for Automated Extraction of Resonance Parameters from the Stabilization Method
• A New Framework to Detect Multi-Messenger Signals from Bright Sporadic Stochastic Gravitational Wave Background
• Exciton Energy Transfer in Conjugated Polymers via a Three-Level Donor-Acceptor Model
• Probing missing physics from inspiralling compact binaries via time-frequency tracks
• Existence-Uniqueness Theory and Small-Data Decay for a Reaction-Diffusion Model of Wildfire Spread
• Incremental Collision Laws Based on the Bouc-Wen Model: Improved Collision Models and Further Results
• Functional Renormalization for Signal Detection: Dimensional Analysis and Dimensional Phase Transition for Nearly Continuous Spectra Effective Field Theory
• Assessment of a Physics-based Retrieval of Exoplanet Atmospheric Temperatures from Infrared Emission Spectra
• A MaNGA about the Legacy I: Connecting the Assembly of Stellar Halo with the Average Star Formation History in Low-Redshift Massive Galaxies
• A Bayesian approach to high fidelity interferometric calibration I: mathematical formalism
• Beyond the Local Void: A data-driven search for the origins of the Amaterasu particle
• A Search for Radio Technosignatures at the Solar Gravitational Lens Targeting Alpha Centauri
• Constraints on the Spindown of Fully-Convective M Dwarfs Using Wide Field Binaries
• Solving the multi-messenger puzzle of the AGN-starburst composite galaxy NGC 1068
• A new method to correct for host star variability in multi-epoch observations of exoplanet transmission spectra
• Environmental Effects on the Dynamical Evolution of Star Clusters in Turbulent Molecular Clouds
• Testing the Limits of AGN Feedback and the Onset of Thermal Instability in the Most Rapidly Star Forming Brightest Cluster Galaxies
• walter: A Tool for Predicting Resolved Stellar Population Observations with Applications to the Roman Space Telescope
• Event2Audio: Event-Based Optical Vibration Sensing
• Characterization of the Cherenkov Photon Background for Low-Noise Silicon Detectors in Space
• The primary proton spectrum of the hadronic PeVatron candidate HAWC J1825-134
• Neutral Stellar Winds Toward the High-Mass Star-Forming Region G176.51+00.20
• Gravitational lensing of fast radio bursts: prospects for probing microlens populations in lensing galaxies
• A Simulation Framework for the LiteBIRD Instruments
• More sophisticated is not always better: comparison of similarity measures for unsupervised learning of pathways in biomolecular simulations
• A novel algorithm for high fidelity spectro-polarimetric snapshot imaging of the low-frequency radio Sun using SKA-low precursor
• The black hole X-ray binary MAXI J1348$-$630 in quiescence
• A hyperboloidal method for numerical simulations of multidimensional nonlinear wave equations: nonlinear tails
• Alternative LISA-TAIJI networks: detectability of the isotropic stochastic gravitational wave background
• An Open-Source Framework for Efficient Numerically-Tailored Computations
• Alouette: Yet another encapsulated TAUOLA, but revertible
• Microscopic approach to the quantized light-matter interaction in semiconductor nanostructures: Complex coupled dynamics of excitons, biexcitons, and photons
• Prospects for radio weak lensing: studies using LOFAR observations in the ELAIS-N1 field
• Remote sensing of tectonic induced stress across faults using high energy muon beams
• Stochastic elastohydrodynamics of contact and coarsening during membrane adhesion
• Initial Characterization of Stellar Photometry of Roman images from the OpenUniverse Simulations
• The DORCHA suite: nature, nurture, and the phase space distribution of the Milky Way's high redshift progenitors today
• Optimal alignment of Lorentz orientation and generalization to matrix Lie groups
• Unified reconstruction of the Lyman-alpha power spectrum with Hamiltonian Monte Carlo
• CMB line-of-sight integrators for nearly-isotropic cosmological models
• Spectral indices in active galactic nuclei as seen by Apertif and LOFAR
• Tensor Data Scattering and the Impossibility of Slicing Theorem
• A hospital demand and capacity intervention approach for COVID-19 in the UK
• Incommensurate magnetic ordering in CrB${}_2$
• Fornax 3D project: assessing the diversity of IMF and stellar population maps within the Fornax Cluster
• A planetary-mass candidate imaged in the Young Suns Exoplanet Survey
• Distance and extinction to the Milky Way spiral arms along the Galactic centre line of sight
• The Relativistic Schrödinger Equation through FFTW3: An Extension of quantumfdtd
• AnomalyMatch: Discovering Rare Objects of Interest with Semi-supervised and Active Learning
• Fast recovery of parametric eigenvalues depending on several parameters and location of high order exceptional points
• Accurate and efficient likelihood modeling for large-scale CMB data
• Iterative construction of the optimal sunspot number series
• Measuring spin precession from massive black hole binaries with gravitational waves: insights from time-domain signal morphology
• PERISTOLE: PackagE that geneRates tIme delay plotS caused by graviTatiOnaL lEnsing
• A magnetic field detection in the massive O-type bright giant 63 Oph
• Contactless pulse rate assessment: Results and insights for application in driving simulator
• Performance of a SiPM-based, plastic scintillator muon veto prototype for CUPID
• A dynamics-based density profile for dark haloes. I. Algorithm and basic results
• A large sub-Neptune transiting the thick-disk M4V TOI-2406
• The Number of Transits Per Epoch for Transiting Misaligned Circumbinary Planets
• The impact of the presence of water ice on the analysis of debris disk observations
• The impact of ultraviolet suppression on the rates and properties of strongly lensed Type IIn supernovae detected by LSST
• Model Independent Periodogram for Scanning Astrometry
• Detecting low-mass haloes with strong gravitational lensing I: the effect of data quality and lensing configuration
• Mapping the cosmic mass distribution with stacked weak gravitational lensing and Doppler lensing
• Search for Dark Matter in 2HDMS at LHC and future Lepton Colliders
• Grouped star formation: converting sink particles to stars in hydrodynamical simulations
• KAgoshima Galactic Object survey with Nobeyama 45-metre telescope by Mapping in Ammonia lines (KAGONMA): Star formation feedback on dense molecular gas in the W33 complex
• Semi-Supervised Learning for Lensed Quasar Detection
• The Contribution of AGN Accretion Disks to Hydrogen Reionization
• Formulation and evaluation of ocean dynamics problems as optimization problems for quantum annealing machines
• Pruning vineyards: updating barcodes and representative cycles by removing simplices
• Supernovae in colliding-wind binaries: observational signatures in the first year
• Standardization of Multi-Objective QUBOs
• Star-Galaxy Classification in Deep LSST Data with Random Forest: A Pilot study on the Data Preview 1 Release
• Advancing weak lensing mass mapping with a mask-aware HEALPix transformer
• Where within the 3C 84 jet are $\gamma$-rays produced?
• The WEAVE acquisition and guiding software: pattern recognition-based acquisition and multi-fibre guiding
• Advanced measurement techniques in quantum Monte Carlo: The permutation matrix representation approach
• Uncovering the Dominant Spatial Scales of the Sun's Magnetic Field in Solar Cycle 24
• The Journey to Dominance: How BCGs Evolve Differently from Other Massive Galaxies
• PISP: Projected-Space Inference of Stellar Parameters
• The steady-state population of Earth's co-orbitals of lunar provenance
• Enhancing gravitational-wave detection: a machine learning pipeline combination approach with robust uncertainty quantification
• Black Hole Survival Guide: Searching for Stars in the Galactic Center That Endure Partial Tidal Disruption
• Most Strong Lensing Deflectors in the AGEL Survey Are in Group and Cluster Environments
• Confirmation of Fe I on MASCARA-5 b's Dayside Observed With EXPRES
• CoronaGraph Instrument Reference stars for Exoplanets (CorGI-REx) I. Preliminary Vetting and Implications for the Roman Coronagraph and Habitable Worlds Observatory
• Quiescent Galaxy Size, Velocity Dispersion, and Dynamical Mass Evolution
• A 5kHz modulator for pyramid wavefront sensors
• The Bochum Survey of the Southern Galactic Disk: III. Complete Data Release
• The Perkins INfrared Exosatellite Survey (PINES) I. Survey Overview, Reduction Pipeline, and Early Results
• Hubble Space Telescope proper motions of Large Magellanic Cloud star clusters -- II. Kinematic structure of young and intermediate-age clusters
• Cosmology of the companion-axion model: dark matter, gravitational waves, and primordial black holes
• Time-dependent Turbulent Electron Acceleration and Transport in Solar Flares
• Forming off-center massive black hole binaries in dwarf galaxies through Jacobi capture
• AQP: An Open Modular Python Platform for Objective Speech and Audio Quality Metrics
• Improving Interoperability in Scientific Computing via MaRDI Open Interfaces
• The LMT 2 Millimeter Receiver System (B4R). I. Overview and Results of Science Demonstration
• The Gaia Astrometric Catalogue and Secular Aberration Drift in Proper Motions
• Confirmation of SRGt 062340.2-265751 as a nova-like cataclysmic variable with a possible magnetic nature
• Interferometric Detection and Orbit Modeling of the Subcomponent in the Hot-dust System $\kappa$ Tuc A: A Low-mass Star on an Eccentric Orbit in a Hierarchical-quintuple System
• Commissioning an Inexpensive Off-the-shelf Spectrograph for Radial-Velocity Studies
• Ram-pressure stripping caught in action in a young cluster at $z=2.51$
• 50-250 MHz Pulsar Census with an SKA-Low prototype station: Spectra and Polarization
• Ordinal Synchronization and Typical States in High-Frequency Digital Markets
• Structure Formation under Inelastic Two-Component Dark Matter: Halo Statistics and Matter Power Spectra in the High-$z$ Universe
• Quantifying the impact of relativistic precession on tidal disruption event light curves
• Near-IR CO and CN in classical Cepheids
• The eventful life journey of galaxy clusters. II. Impact of mass accretion on the thermodynamical structure of the ICM
• Learning Atomic Multipoles: Prediction of the Electrostatic Potential with Equivariant Graph Neural Networks
• Power spectrum multipoles and clustering wedges during the Epoch of Reionization
• A machine learning algorithm for minute-long Burst searches
• unxt: A Python package for unit-aware computing with JAX
• The Creation of Puffin, the Automatic Uncertainty Compiler
• Morphologies for DECaLS Galaxies through a combination of non-parametric indices and machine learning methods: A comprehensive catalog using the Galaxy Morphology Extractor (galmex) code
• A z$\sim$1 galactic-scale outflow transversally mapped to $\sim$50 kpc through gravitational-arc tomography
• Exploring Young Stellar Variability with Gaia DR3 light curves
• Time Evolution of Optical Darkness in GRB Afterglow: The Case of GRB 240825A
• Evaluating Quantumness, Efficiency and Cost of Quantum Random Number Generators via Photon Statistics
• The Atacama Cosmology Telescope: Machine Learning Driven Tools for Detecting Millimeter Sources in Timestream Pre-processing
• Comprehensive analysis of a symbiotic candidate V503 Her
• Where's Swimmy?: Mining unique color features buried in galaxies by deep anomaly detection using Subaru Hyper Suprime-Cam data
• Seafloor Weathering and Stochastic Outgassing Unlikely to Significantly Shorten the Future Lifespan of Earth's Terrestrial Biosphere
• A New Method for the Reconstruction of Strongly Lensed Galaxies with Resolved Kinematics
• Kinematics and Feedback in H II regions in the Dwarf Starburst Galaxy IC 10
• Observational insights into Sr I 4607 Å scattering polarization with DKIST/ViSP
• How to use Machine Learning to improve the discrimination between signal and background at particle colliders
• Estimating JUNO's Sensitivity to Solar Neutrino-to-antineutrino Conversion and Neutrino Magnetic Moments
• pythonradex: a fast Python re-implementation of RADEX with extended functionality
• A Study Revealing Physical Attributes of Supernova Remnant in G321.3-3.9
• Discovery and Characterization of Three New High-amplitude delta Scuti Stars from TESS Observations
• PyIRD: A Python-Based Data Reduction Pipeline for Subaru/IRD and REACH
• The eccentricity distribution of wide binaries and their individual measurements
• Fate of Bosonic Topological Edge Modes in the Presence of Many-Body Interactions
• Fuzzy expert system for the process of collecting and purifying acidic water: a digital twin approach
• Alfred: A Flexible, User-Friendly Python Package for Exoplanet Confirmation
• Depth Calibration of Double-sided Strip Germanium Detectors for the Compton Spectrometer and Imager Satellite
• ExoDNN: Boosting exoplanet detection with artificial intelligence. Application to Gaia Data Release 3
• The Population Synthesis Toolkit (PST) Python library
• LieDetect: Detection of representation orbits of compact Lie groups from point clouds
• Nature vs. Nurture: Investigating the Effects of Measurement Uncertainties in the Assessment of Potential Trends Between Planetary and Stellar Properties
• X-ray Polarization of Inverse Compton Scattering by Thermal and Nonthermal Electrons
• Impact of tides on non-coplanar orbits of progenitors of high-mass X-ray binaries
• When Structure is Silent: Opportunities for Algorithmic Dispatch in Linear Algebra
• Tidal adaptive softening and artificial fragmentation in cosmological simulations
• Gravitational Microlensing Rates in Milky Way Globular Clusters
• An Enumerative Embedding of the Python Type System in ACL2s
• Rotation of young solar-type stars as seen by Gaia and K2
• Size-Mass Relation Shows Its Colours: Contrasting Physical Imprints of Galaxy Evolution in Rest-Frame UV and Optical
• Towards a systematic treatment of observational uncertainties in forward asteroseismic modelling of gravity-mode pulsators
• Detectability of a spatial correlation between stellar-mass black hole mergers and Active Galactic Nuclei in the Local Universe
• High-spectral-resolution Observations of the [S II] Emission-line Doublet in the Filamentary Nebula Surrounding NGC 1275
• On the Turbulent Reduction of Drifts for Solar Energetic Particles
• A Detailed Analysis of Intermediate-scale Structure in Optical Extinction Curves: Expanded Census and Two-family Classification
• Passive spiral galaxies deeply captured by Subaru Hyper Suprime-Cam
• A catalog of near-IR absolute magnitudes of Solar System small bodies
• The symphony of pulsations and binarity among massive stars using HERMES spectroscopy and TESS photometry
• GJ 3929 b as the First Complete Rocky Worlds DDT Data Set
• Photon Ring Symmetries in Simulated Linear Polarization Images of Messier 87*
• Atmospheric Signatures of Common Envelope Evolution in White Dwarf Planets
• Syntriod: A Robust Initial Parameter Estimator for Radial Velocity Curve Solutions Beyond Conventional Sampling Limits
• Revisiting the Gas Dynamics of Henize 2-10: Possible Drivers of the Starburst
• Locate a stellar flare from the M dwarf LAMOST J1332+5057
• Low-frequency spectra of neutron star + OB supergiant binaries: Does wind density drive persistent and flaring modes of accretion?
• Role of non-thermal processes in the quiescent and active millimeter spectrum of a young M dwarf
• Constraining the shape of Milky Way satellites with distance gradients
• Ergodicity of FIRE: star formation variations within and between simulated galaxies
• Dynamic Photometric Variability in Three Young Brown Dwarfs in Taurus: Detection of Optical Flares with TESS data
• Searching for Type Ia Supernovae in the Dark Energy Spectroscopic Instrument
• An Approximate Bayesian Deep Learning Approach for Uncertainty-aware Differential Emission Measure Estimates in the Solar Corona from the SDO
• High performance Stingray
• Radar-Chart Analysis of Star-Formation Quenching Stages Across Circular Velocity Curve Classes in Nearby CALIFA Galaxies
• COSMOS2025: A Machine Learning Census of Massive Quiescent Galaxies at $2.5<\text{z}<5$
• GRB 160410A: the first Chemical Study of the Interstellar Medium of a Short GRB
• Cosmic Shear in Harmonic Space from the Dark Energy Survey Year 1 Data: Compatibility with Configuration Space Results
• Generating Stellar Obliquity in Systems with Broken Protoplanetary Disks
• A Fully Three-Dimensional Kinetic Particle-In-Cell Framework for Modeling Laser-Dielectric Interactions: Few-Cycle Pulse Damage
• Mapping feedback signatures in 3C 297: A quasar-host merger at Cosmic Noon
• GalPort: Investigation of the bar in action-angle space
• A Reversible Unwrapping Algorithm for Constant Pressure Molecular Dynamics Simulations
• Refined rotational state and shape model of (98943) Torifune ahead of the Hayabusa2# flyby
• Constraints on the Atmospheric Composition of 2002 XV${}_{93}$ from JWST Spectroscopy
• Bayesian inference in single-line spectroscopic binaries with a visual orbit
• The Longest-period Young Transiting Exoplanets. A Duo of Puffy Giants inside a Debris Disk
• Spin-Orbit Geometry of AU Mic b and c from Back-to-Back Transits Observed Contemporaneously with Magellan PFS, LCOGT, and CHEOPS
• Fast Sampling of Cosmological Initial Conditions with Gaussian Neural Posterior Estimation
• Revisiting BD-06 1339b: A Likely False Positive Caused by Stellar Activity
• The black hole occupation fraction as a fossil record of seeding, dynamics, and galaxy assembly
• Constraining the geometry of the gas surrounding a typical galaxy at $z=3.4$ with Ly$\alpha$ polarization
• The VMC survey -- XLVI. Stellar proper motions in the centre of the Large Magellanic Cloud
• Zwicky Transient Facility and Globular Clusters: The RR Lyrae gri-Band Period-Luminosity-Metallicity and Period-Wesenheit-Metallicity Relations
• Optimising reference library selection for reference-star differential imaging of discs with SPHERE/IRDIS