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RSS  Latest preprints on astro-ph:

› The General Antiparticle Spectrometer (GAPS) Antarctic Balloon Payload
› Can radio occultations constrain Uranus or Neptune's internal rotation periods?
› A population-based approach to understanding radio AGN feedback with LOFAR: The LoTSS Deep Fields
› Hamilton's Object Revisited: A challenging source redshift of a strong lensing configuration
› The fragmentation properties of massive star-forming regions in 30Dor-10 at 2000 au resolution
› Quasi-Periodic Microstructures in Pulsar Emission: Automated Detection and Archival Survey
› HI 21-cm absorption in low- and high-excitation radio-loud AGNs at $z
› Radio detection of supernova remnant G310.7-5.4 with $\gamma$-ray counterpart: Abeona SNR
› Search for Anisotropic Pair Halos Associated with Blazar Jets
› A giant solution to the disk mass budget problem of planet formation
› Stability of Multiplanet Systems Through Hot Jupiter Destruction
› Neural Simulation-based Inference with Hierarchical Priors for Detached Eclipsing Binaries
› Measuring neutrino mass and asymmetry through galaxy pairwise peculiar velocity
› Resolving the Dust Budget Crisis at $z \sim 8$ with Optically Thick, High-Density Molecular Clumps: MACS0416_Y1
› Prevailing thermally-pulsing-asymptotic-giant branch stars in the near-infrared rest-frame spectra of distant quiescent galaxies: towards robust galaxy ages and masses
› The curved jet in the young star FN Tau
› The FUor Mass Distribution Matches the Solar Neighborhood IMF: Evidence for a Universal Eruptive Phase
› Pulsational mass loss from supermassive stars creates the compact shells of Little Red Dots
› The apparent Large Magellanic Cloud star cluster age gap
› The First Infrared Portrait of A Solar-Like Host Star with Debris Disk: Pioneering High-Resolution H- and K-Band Spectroscopy of HD115617 with Comparative Optical Spectrum Analysis
› Circumbinary Discs as the Origin of Cirumstellar Material around Interacting H-poor Supernovae and Fast Blue Optical Transients
› MAUVE-MUSE: Ionization and Kinematic Signatures of Environmental Effects on Virgo Cluster Disks
› Feeling the Pressure: Effects of Formation Pressure on the Physical Properties of Titan Haze Analogs
› Unraveling Chemical Enrichment in Extreme Emission-Line Galaxies: A Multi-Element Bayesian View of Bursty Star Formation and Galaxy Evolution in DESI
› Purely Quadratic Non-Gaussianity from Tachyonic Instability: Primordial Black Holes and Scalar-Induced Gravitational Waves
› SN 2007it on the RISE -- a radio detection of an interacting supernova 18 years post-explosion
› Cold molecular gas distribution and kinematics in the low-metallicity dusty starburst of Mrk 996 resolved with ALMA
› Detections of nearly bias-free core shifts with 5-30 $\mu$as precisions at 8-43 GHz in BL Lacertae
› Fast-Cooling Synchrotron in Decaying Magnetic Fields: Implications for the GRB Spectral Distribution
› Science from the In Situ Exploration of the Proxima Centauri System
› Photometric Super-Resolution for Improving Galaxy Morphological Measurements using Conditional Generative Adversarial Networks
› Sub-Neptunes Show a Stronger Correlation with Cold Jupiters than Super-Earths Especially in Metal-rich Systems
› Solar Energetic Particle Events and Associated Type II Radio Bursts from Different Source Regions
› Measuring Tianlai's primary beam using sky model
› Ancient 'ghost' planetary nebulae discovered with amateur telescopes
› Shortest period for outer orbit in compact hierarchical triple? Discovery of SB1 around V0885 Per
› Europa's Lyman-$\alpha$ emissions from HST/STIS observations
› Stellar flare-driven evolution of primordial early exo-Earth atmospheres: Insights from a Young M Dwarf Flare model
› The core of the problem: Physical limits of the core-S\'ersic model
› XRF 241001A/SN 2024aiiq: A Faint Soft X-ray Transient Detected by SVOM with a Broad-Line Type Ic Supernova Revealed by JWST
› Formation of classical Be-stars of the early spectral subclass in the case of nonconservative mass transfer in close binary systems
› The Evolution of the SFR-M_* relation at 0.1
› Mid-infrared JWST spectra of carbon stars in the Large Magellanic Cloud
› The January 2010 flare of Mrk421: Insights from a stochastic acceleration model
› Polytropic stellar wind models with strongly localized heating
› Approximating General Relativity in Core-Collapse Supernova Simulations
› Deep VLBI constraints on compact radio cores in four ultraluminous X-ray sources
› Review: A new method for estimation and use of systematic errors in Poisson regression
› A Python/CuPy Software Correlator for QUEST: Real-Time Performance and Initial Imaging
› Forecasts of CMB $E$-mode anomalies for AliCPT-1
› Photometric Identification of Unresolved Binary Stars in Nearby Open Star Clusters
› The Be star omicron Cas is indeed the primary of a triple system
› Machine Learning-Based Characterization of Solar p-Mode Frequency Shifts during Solar Cycle 25
› A Search for Rotation Measure Flare Candidates in Repeating Fast Radio Bursts
› Self-regulated galaxy evolution within a self-consistently varying galaxy-wide IMF
› Stellar separation shapes spin-orbit alignment in visual binaries
› Neural posterior estimation of the neutrino direction in IceCube using transformer-encoded normalizing flows on the sphere
› Greybody Factor, Resonant Frequencies, and Entropy Quantization of Charged Scalar Fields in the Kerr-EMDA Black Hole
› Self-Interaction and Galactic Magnetic Field Bounds on Millicharged Magnetic Monopole Dark Matter
› Ultra-High-Energy Tau Neutrinos as Probes of Lorentz Invariance
› Photon and neutrino fluxes from spheroidal dwarf galaxies in a decaying DM model
› Reshaping the inner shadow of a Kerr black hole by a torn accretion disk
› Time evolution of a Nambu-Goto string coiling around a Kerr black hole
› Interaction between nuclear clusters and superfluid phonons in the neutron-star inner crust
› Spontaneous Baryogenesis from Axions on Induced Electroweak Walls
› Primordial Magnetogenesis and Gravitational Waves from ALP-assisted Phase Transition
› Irreducible Gravitational Wave Background as a Particle Detector
› Geodesic Completeness in General Cosmological Scenarios
› Novel geometrical test of cosmological expansion from photometric data
› The Optical and Infrared Are Connected
› A Systematic Search for Trace Molecules in the Atmosphere of Exoplanet K2-18 b
› MasconCube: Fast and Accurate Gravity Modeling with an Explicit Representation
› Galaxy Metallicity Gradients in the Reionization Epoch from the FIRE-2 Simulations
› Simulation budgeting for hybrid effective field theories
› Explodability matters: how realistic neutrino-driven explosions change explosive nucleosynthesis yields
› The Atacama Cosmology Telescope: stellar mass growth in massive galaxy clusters from DR5 over the past 7 billion years
› Weak-Lensing Analysis of the Galaxy Cluster Abell 85: Constraints on the Merger Scenarios of Its Southern Subcluster
› The first AKRA mass map reconstruction from HSC Y1 data
› Role of prompt cusps in driving the core collapse of SIDM halos
› Back-End System of BURSTT
› SLICE -- Combining Strong Lensing and X-ray in AC 114. Further Insights into the Merger Scenario
› High-Resolution Measurements with the CTAO Southern Array: The Case for Pulsar Wind Nebulae
› Nonlinear Weak Lensing reconstruction for Galaxy Clusters
› AT2024wpp: An Extremely Luminous Fast Ultraviolet Transient Powered by Accretion onto a Black Hole
› AstroSat UV Deep Field IV. An Extended UV disk around a massive spiral galaxy at z=0.67
› Using Astrometry to Break Degeneracies in Stellar Surface Mapping
› Atmospheric characterization of HIP 67522 b with VLT/CRIRES+. VLT/CRIRES+ suggests a heavier planet and hints at deuterium fractionation
› Observational Properties of Near-Maximally Spinning Supermassive Black Holes
› The diagnostic temperature discrepancy as evidence for non-Maxwellian coronal electrons
› Extended Radio Galaxies in EMU: A Comparative Look at Source-Finding Techniques
› Optical transients from non-explosive double white-dwarf mergers: the case of a central neutron star remnant
› A New Method to Simulate Dark Matter-Baryon Interactions and Application to an Isolated Disk Galaxy
› Global asteroseismology of 19,000 red giants in the TESS Continuous Viewing Zones
› Chromospheric turbulence as a regulator of stellar wind mass flux
› POLARIS: A Sparse Radial Neutrino Telescope Design for the Pacific Ocean
› The steady-state population of Earth's co-orbitals of lunar provenance
› Photometry and physical characterization of near-Earth asteroid 2025 FA22 from one apparition
› ExoNet: Calibrated Multimodal Deep Learning for TESS Exoplanet Candidate Vetting using Phase-Folded Light Curves, Stellar Parameters, and Multi-Head Attention
› Kardashev's Conundrum: Statistical Falsification of the Standard Kardashev Model and the Kardashev--Sagan--Nakamoto Resolution
› NOEMA3D: Spatially resolved dust, CO, and [C I] in massive star-forming main sequence galaxies at cosmic noon
› Machine Learning Supports Existence of Previously Unrecognized Transient Astronomical Phenomena in Historical Observatory Images
› Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
› Earth's Infrared Background
› Generalized neutrino isocurvature
› Angular momentum of vacuum bubbles in a first-order phase transition
› Disentangling spinning and nonspinning binary black hole populations with spin sorting
› Attenuation of the ultra-high-energy neutrino flux by dark matter scatterings
› Hunting for new glitches in LIGO data using community science
› Sensitivity forecasts for gravitational-wave detectors to dark matter decaying into gravitons
› Thermodynamics vs Teleodynamics: A Cosmological Divide?
› General gravitational properties of neutron stars: curvature invariants, binding energy, and trace anomaly
› Bayesian Constraints on the Neutron Star Equation of State with a Smooth Hadron-Quark Crossover
› Gravitational waves from warm inflation in the weak dissipative regime
› Morphological Evolution of Higher Order Nonlinear Kinetic Alfv\'en Waves in Structured Galactic Environments

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