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RSS  Latest preprints on astro-ph:

› Astrophysics Wrapped 2025: Year-in-Review of Every Astrophysics arXiv Paper from 2025
› GAMERA-OP: A three-dimensional finite-volume MHD solver for orthogonal curvilinear geometries
› What Suppresses Star Formation in Bulge-Dominated Early-Type Galaxies?
› Direct pathway to the Early Supermassive Black Holes: A Red Super-Eddington Quasar in a Massive Starburst Host at $z=7.2$
› Unraveling the Origin of Unequal Mass Gravitational Wave Events: Insights from a Galactic High Mass X-ray Binary
› A boost in the precision of cluster-mass models: Exploiting the extended surface brightness of the lensed supernova Refsdal host galaxy
› Searching for the Shortest-wavelength Aromatic Infrared Bands: No Evidence for the Predicted 1.05 $\mu$m Polycyclic Aromatic Hydrocarbon Feature
› A tight relation between the distribution of globular clusters and dark matter in AS1063
› An analytic approximation to the covariance between pre- and post-reconstruction galaxy two-point statistics
› Sign-Switching Dark Energy: Smooth Transitions with Recent \textit{DESI DR2} Observations
› Excitation and Damping of Oscillation Modes in Gaseous Planets
› Bayesian Analysis for Remote Biosignature Identification on exoEarths (BARBIE) IV: Analyzing CO2 Detections in the Near-IR to Determine the Long-Wavelength Cut-off for the Habitable Worlds Observatory Coronagraph
› Precursors in tidal disruption events: repeating, fast, and AGN-hosted TDEs
› Assembly bias and local Primordial non-Gaussianity from DESI DR1 Quasars
› Eye of the beholder: Observer reference frame bias in Hickson-like compact groups of galaxies
› TSSC comet-centered data products from TESS 3I/ATLAS observations
› New Time-Dependent WFC3/IR Inverse Sensitivities
› First-Principles Polar-Cap Currents in Multipolar Pulsar Magnetospheres
› The Role of Faraday Rotation in the Polarization of the X-rays from Magnetically Powered Black Hole Coronas
› Abundances in 78 metal-rich bulge spheroid stars from APOGEE
› Broadband Timing and Spectral Study of Accreting Millisecond X-ray Pulsar SAX J1808.4$-$3658 during Its 2022 Outburst
› Correlated and uncorrelated Monte Carlo neutron capture rate variations in weak $\textit{r}$-process simulations
› Cosmological Simulation with Population III Stellar Feedback and Metal Enrichment I: Model Description And Convergence Test
› Parker Solar Probe observations of solar energetic particle (SEP) events with inverse velocity arrival (IVA) features
› Odd Radio Circles Modeled by Shock-Bubble Interactions
› Unusual Circumstances of the 2024 June 8 GLE
› A Protoplanet Candidate in the PDS 66 Disk Indicated by Silicon Sulfide Isotopologues
› Full-Spectrum Machine Learning Diagnostics for Interstellar PAHs
› Guangqi: A two-dimensional radiation hydrodynamic code with realistic equation of states
› The Structure and Evolution of LRDs: Insights from JWST NIRSpec Medium and High Resolution Spectroscopy at $z\sim4$
› Bundle adjustment of Hayabusa2's ONC images and controlled color mosaic map of Ryugu
› Graph Neural Network Prediction of Infrared Spectra of Interstellar Polycyclic Aromatic Hydrocarbons
› KMT-2016-BLG-1337L: A Saturn-mass planet orbiting within a binary system of low-mass stars
› Ballistic Surfing Acceleration as a Coherent Mechanism for Electron Acceleration in Galaxy Cluster Shocks
› ALMA Band 9 CO(6--5) Reveals a Warm Ring Structure Associated with the Embedded Protostar in the Cold Dense Core MC 27/L1521F
› Murriyang cryogenic phased array feed: spectral-line results and noise-reduction methods
› ESO White Paper on Intensity Interferometry: Cosmology, Fundamental Physics, Quantum Optics
› A rotational line CO cooling rate prescription for AGB outflows
› Tracking the dynamical, chemical and spectral evolution of molecular cores with PrestaLine: Gorynych
› CHIME/Slow overview and pilot survey: A new backend to search for second-duration radio transients with the CHIME telescope
› X-ray line diagnostics of the multi-phase gas in the Centaurus cluster core with XRISM/Resolve
› On The Stability Of $H_0$ And The Inverse Distance Ladder
› Constraints on GRB Jet Properties from IceCube Upper Limits: Insights from GRB 221009A and GRB 240825A
› The optical-infrared relation for active galactic nuclei: The role of contaminations
› Constraining Axion-like Particles through Multi-epoch Monitoring of Strong Gravitational Lenses
› BSN-VI: Multiband Light Curve Modeling of Four W UMa-Type Contact Binaries I. Revisiting Energy Transfer Mechanisms and Luminosity Behavior
› GAME: Genetic Algorithms with Marginalised Ensembles for model-independent reconstruction of cosmological quantities
› Upper limit on HF(1-0) absorption in a dusty star-forming galaxy at $z = 6$: Constraints on early fluorine enrichment
› The Effect of Gravitational Stratification on Kink Oscillations in Curved Coronal Loops
› Gaps and Rings: A Near-Universal Trait of Extended Protoplanetary Discs
› Observations of Binary Stars with the 1.3-m Devasthal Fast Optical Telescope Using Speckle Interferometry: An Attempt
› STEP survey: III. STEPping stones between the clouds: the star formation history of the Magellanic Bridge
› Pre-perihelion Emergence of the CN Gas Coma in 3I/ATLAS Temporally and Spatially Resolved by the 7-Dimensional Telescope
› A nearby He-rich superluminous supernova at photospheric phases
› Anomaly Hunter for Alerts (AHA): Anomaly Detection in the ZTF Transient Alert Stream
› Demographics of Wandering Black Holes Powering Off-Nuclear Tidal Disruption Events
› TIC-65910228 b / NGTS-38 b, a 180 day transiting warm super-Jupiter
› Statements of Current States of the Art for Key non-Coronagraphic Technologies for HWO
› Self-Consistent Direct Method for Chemical Abundances in High-z Galaxies with JWST
› Photometric classification of supernovae detected by the Zwicky Transient Facility using noise augmentation
› How hard is dust in debris disks?
› Spatially resolved star-formation histories of local post-starburst galaxies: Starburst and quenching spatial patterns consistent with recent mergers
› H$_2$ Ortho-Para Spin Conversion on Inhomogeneous Grain Surfaces. II. impact of the rotational energy difference between adsorbed ortho-H$_2$ and para-H$_2$ and implication to deuterium fractionation chemistry
› TIC65910228b: A single-transit discovery of a massive long-period warm Jupiter with TESS
› Presaging Doppler beaming discoveries of double white dwarfs during the Rubin LSST era
› An updated constraint for the Gravitational Wave Background from the Gamma-ray Pulsar Timing Array
› V515 And: An Intermediate Polar in the Period Gap Exhibiting Outbursts
› $\texttt{GPUmonty}$: A GPU-accelerated relativistic Monte Carlo radiative transfer code
› A non-perturbative framework for N-point functions of locally non-Gaussian fields
› Towards a complete scheme of cosmological neutrino self-interactions: Collision term for a wide range of mediator masses
› Dark matter effects on the properties of hybrid neutron stars
› Chiral symmetry restoration and hyperon suppression in neutron stars
› Big Bang Nucleosynthesis and the Neutrino-Extended Standard Model Effective Field Theory
› Statistics of time and frequency-averaged spectra in gravitational-wave background searches
› Negative thermal expansion in ice I polytypes
› Addressing the Hubble tension with Sterile Neutrino Dark Matter
› NuRadioMC: Simulating the radio emission of neutrinos from interaction to detector
› No evidence for p- or d-wave dark matter annihilation from local large-scale structure
› Asteroseismically Inferred Ages of 132,000 Red Giants with TESS
› Testing the cosmological principle on gigaparsec scales
› CMB line-of-sight integrators for nearly-isotropic cosmological models
› SKA-Low simulations for a cosmic dawn/epoch of reionisation deep field
› Gravitational Waves from First-Order Phase Transitions Assisted by Temperature-Enhanced Scatterings
› Simulating a Gaussian stochastic gravitational wave background signal in pulsar timing arrays
› 3D hydrodynamic simulations of massive main-sequence stars -- IV. Internal gravity waves matter for SLF variability
› Multi-resolution kinematic modelling of nearby galaxies: a demonstration using MHONGOOSE observations
› A $\tau-$DM relation for FRB hosts?
› Cepheid Metallicity in the Leavitt Law (C-MetaLL) survey: IX. Metallicity dependence of Period-Wesenheit relations based on a homogeneous spectroscopic sample
› The JWST EXCELS survey: Insights into the nature of quenching at cosmic noon
› V717 Andromedae: An Active Low Mass Ratio Contact Binary
› The Case for Space: Estimating Precise Time Delays from Ground- and Space-Based Observations of Lensed Supernovae with Glimpse
› Geometry of the Milky Way's dark matter from dynamical models of the tilted stellar halo
› The luminosity function and clustering of bright quasars in the FLAMINGO cosmological simulations
› Localized Deviations from the CO-PAH Relation in PHANGS-JWST Galaxies: Faint PAH Emission or Elevated CO Emissivity?
› Dynamics in the Cores of Self-Interacting Dark Matter Halos: Reduced Stalling and Accelerated Core Collapse
› Velocity dispersion functions of pressure-supported galaxies in EAGLE simulations with varying active galactic nucleus feedback
› A redshift-independent theoretical halo mass function validated with Uchuu simulations
› The disk precession in a Be star-magnetar binary and its application to the rotation measure of FRB 20201124A
› Towards ALMA2040: An update from the European community and invitation to contribute
› Astrophysical Implications of Eccentricity in Gravitational Waves from Neutron Star-Black Hole Binaries
› IK Pegasi and the Double-merger Path to Type Ia Supernovae
› Star formation outside galaxies undergoing gravitational and hydrodynamic interactions: Dust attenuation and the star formation rate
› Physical and Chemical Characterization of GY 91's Multi-ringed Protostellar Disk with ALMA
› Spatial distribution of organics in the Horsehead nebula: Signposts of chemistry driven by atomic carbon
› Nucleus and Postperihelion Activity of Interstellar Object 3I/ATLAS Observed by Hubble Space Telescope
› LISA Non-Linear Dynamics and Tilt-To-Length Coupling
› Constraints on cyclotron features and accretion regime in the high-mass X-ray binary 4U 1700-37 from NuSTAR
› A Two-Dimensional Analytic Solution for the Generation of Hyperbolic Trajectories Via A Single Close Encounter with Applications To Interstellar Objects
› Sensipy: simulate gamma-ray observations of transient astrophysical sources
› Scalar-induced gravitational waves and primordial black holes from a localized bump or dip feature in a single-field inflationary potential
› Keck Observations in the INfrared of Taurus and $\rho$ Oph Exoplanets And Ultracool dwarfs (KOINTREAU) II: Two Young Bound Companions to Ophiuchus Stars
› Discrete Chi-Square Method can model and forecast complex time series
› Trace anomaly contributions to semi-classical wormhole geometries
› Fast and Flexible Neutrino Decoupling Part I: The Standard Model
› Towards an anomaly detection pipeline for gravitational waves at the Einstein Telescope
› The meaning of "Big Bang"
› Assessing astrophysical foreground subtraction in DECIGO using compact binary populations inferred from the first part of the LIGO-Virgo-KAGRA's fourth observation run
› Primordial black holes and Scalar-Induced Gravitational Waves formed by inflation potential with non-trivial characteristics
› Direct power spectral density estimation from structure functions without Fourier transforms
› Suppression of Gravitational-Wave Echoes in Diffeomorphism-Invariant Nonlocal Quantum Gravity

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