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RSS  Latest preprints on astro-ph:

› Geomagnetic storm suppression of photographic plate transient detections in the POSS-I archive: an independent physical variable strengthening the nuclear test correlation
› FluxMC: Rapid and High-Fidelity Inference for Space-Based Gravitational-Wave Observations
› The neighboring stars of N6946-BH1 and the observational characteristics of failed supernovae
› Electromagnetic Flares from Compact-Object Mergers in AGN Disks: Signatures and Predictions
› PANORAMIC: The Dawn of Massive Quiescent Galaxies I. Number Density and Cosmic Variance from 1000 arcmin$^2$ NIRCam Imaging
› Winding Back the Clock: Recent Star Formation Histories of Massive Quiescent Galaxies Are Consistent With Their Rapid Number Density Evolution Since $\mathbf{z\sim7}$
› Characterizing the Gamma-ray Emission from Low-Luminosity AGN
› Toward Early-type Eclipsing Binaries as Extragalactic Milestones: First Calibration of the SBCR from O- and B-type Stars in Detached Eclipsing Binaries
› Universal Dark-matter Density Profiles of Cosmic Filaments
› Two-stage disruption of resonant chains
› Lithium and the evolution of intermediate-mass T Tauri and Herbig stars. Rotation, accretion, and planets
› Wide Jets or Low Rates: Reconciling Short GRB and Gravitational-Wave Neutron Star Merger Rates
› Super-Solar Metallicity and Tentative Evidence for Photochemistry on WASP-96b from JWST and Ground-Based VLT Transmission Spectroscopy
› Photon-Count Statistics of Crab X-ray Pulses: Skellam Behavior and Excess Variance in the Main Pulse
› Kinetic magnetohydrodynamics and Landau fluid closure in relativity
› Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars
› A New Method for Testing Einstein's Theory of Gravity Close to Rapidly Spinning Black Holes
› Great Walls of Cosmic Baryons in the Northern Sky
› A generic $\omega_b$ tension in early-time solutions to the Hubble tension
› A Comprehensive Atmospheric Retrieval Analysis of 22 James Webb Space Telescope Spectral Energy Distributions of Cool Brown Dwarfs
› Azimuthal Dust Polarization from Aerodynamically Aligned Grains as Evidence for the Streaming Instability in Protoplanetary Disks
› Identification of a Radio Counterpart to SN 2025ulz in the S250818k Localization Area
› Identifying signatures of inflow onto face-on galaxies using the Balmer decrement
› SN2023ixf: Radiative-transfer modeling of the photospheric phase evolution from the ultraviolet to the infrared
› Gas Giants Formed by Gravitational Instability May Accrete Atmospheres with Super-Stellar Carbon to Oxygen Ratios
› Approximating the Fourier Transform of Ring-Like Images: the Focal Expansion
› Local primordial non-Gaussianity using cross-correlations of DESI tracers
› A Chemical Mismatch Between Young Stars and Their Inner Disks
› The JWST Search for Earth-Luna Analogs: Upper Limits on Exomoons and Refined Ephemerides for TOI 700 d and e
› JWST Lensed Quasar Dark Matter Survey V: Measuring the minimum halo mass with strong gravitational lensing
› Constraints on the Injection of Radiation in the Early Universe
› High-contrast imaging of Galactic Cepheids with VLT/SPHERE
› Explaining Neural Networks on the Sky: Machine Learning Interpretability for Cosmic Microwave Background Maps
› The Cluster Completeness Correction Calculator (C-4): A Neural-Network framework and pilot application to the LEGUS Survey of NGC 628
› Statistics of blob properties in two types of coronal streamers
› Scientific Validation of the SPARC4 Pipeline: Multi-band Imaging, Polarimetry, and Photometric Time Series for Improved Characterization of Transiting Exoplanets
› A Catalog of Mid-infrared Variable Sources in the Ecliptic Poles
› Accurate polarization calibration of FAST spectral data for measurements of Zeeman splittings of OH megamasers in IRAS 02524+2046
› Adiabatic Mass Loss In Binary Stars. VI. Massive Helium Binary Stars
› Detectability of continuous gravitational waves from planetary-mass companions orbiting compact stars
› Reconstruction of fast-rotating neutron star observables with the neural network
› The NANOGrav 15 yr and 20 yr Datasets: Timing Events and Pulse Shape Changes
› Reconstructing a large-scale matter-density contrast profile to reconcile Pantheon+ supernovae with DESI DR2 BAO in an inhomogeneous universe
› Galactic-scale evolution of classical and complex radio galaxies. Impact of ambient morphology and jet geometry
› Multi-Quark Clustering in Neutron-Star Matter from Color-Spin Molecular Dynamics
› One sightline, many systems: a FLASH discovery of HI towards scintillating quasar PKS 0405-385
› Searching for Contact Binaries with LAMOST and TESS
› Remnant recoil and host environments of GWTC-4.0 binary black-hole mergers
› WALLABY pilot survey: HI depletion times within the stellar discs of nearby galaxies
› What can galaxy clustering really tell us about the galaxy-halo connections?
› Investigation of Transit Timing and an Optical Transmission Spectrum of the Hot Jupiter WASP-11 b
› Extreme Blazars Observed with MAGIC: Second Catalog Release
› The Broken Similarity: Sinking and Merging of Dark Matter Subhalos Across Hierarchical Levels
› Higher resolution optical spectra of $M_*
› Stellar Population Characterisations in nearby, dusty Early-Type Galaxies
› Non-LTE Ionization Modeling for Helium and Strontium in Neutron Star Merger Ejecta
› Instrumental development for Cryogenic sub-Hz cROss torsion bar detector with quantum NOn-demolition Speed meter (CHRONOS)
› Strontium and helium in the kilonova AT2017gfo: Origin of the 1{\mu}m feature constrained via NLTE calculations
› Unveiling axion signals in galactic supernovae with future MeV telescopes
› Model-independent constraints on generalized FLRW consistency relations with bootstrap-based symbolic regression
› Forward analytical model for the optical selection bias on galaxy cluster lensing profiles
› Diagnostic Consistency Tests of the Concordance Cosmology
› Probing the Evolution of Dark Energy: A Joint Analysis of DESI DR2, Pantheon+, and Cosmic Chronometers
› Comments on "The impact of Solar magnetic field configurations on the production of gamma rays at the Solar disk'' (arXiv:2512.01403)
› Developing Pre-Supernova Neutrino Support for sntools
› Study of the migration of Earth-like planets in planetesimal disks and the formation of debris disks
› Testing X-ray Periodicity and Long-Term Trend in PG 1553+113 via Targeted Swift-XRT Monitoring
› The Transit Timing and Transmission Spectrum of Hot Jupiter WASP-43 b from a decade of Multi-band Transit Follow-up Observations
› An 18 - 25 GHz spectroscopic survey of southern hemisphere dense cores
› Orbital inclination estimates for overcontact binaries using the derivatives of light curves
› Testing parity with composite-field spectra of BOSS and DESI luminous red galaxies
› The Cohesive Object Sequence: The Mass-Density Distribution of Astronomical Objects from Asteroids to Stars
› cuRAMSES: Scalable AMR Optimizations for Large-Scale Cosmological Simulations
› Lyman-$\alpha$ Forest Signatures of Mixed Fuzzy and Cold Dark Matter
› Spectroscopic confirmation of dual and offset quasars from the Subaru HSC-SSP program
› Star-planet magnetic interactions in photoevaporating exoplanets
› Hunting Dark Matter with the Einstein Telescope
› Investigating ACS/WFC Amp-to-Amp Sensitivities
› On the observational distinguishability of the Kerr and Kerr-Hayward metrics to EHT
› Deep Spectroscopy with DESI for Photometric Redshift Training and Calibration
› Testing the 3-equation Kuhfuss Convection Model using the Sun
› Focal plane wavefront control with model-based reinforcement learning
› Effective stability estimates close to resonances with applications to rotational dynamics
› Revisiting The Gravitational Mirroring In Presence of Compact Objects
› Electroweak Doublet Dark Matter for a Galactic Halo Gamma-Ray Excess
› Ion Weibel Instability in the hybrid framework: the optimal resolution
› Gravitational Waves from Matter Perturbations of Spectator Scalar Fields
› Cosmological collider signals of modular spontaneous CP breaking
› Twisted doughnuts: Thick disk torus around equatorial asymmetric black hole
› Modeling complex plasma instabilities in space plasmas - Three-component electron formalism of heat-flux instabilities
› Valence and Rydberg excited state bond dissociation curves of CO2 from orbital-optimized density functional calculations
› Noise budget of Cryogenic sub-Hz cROss torsion bar detector with quantum NOn-demolition Speed meter (CHRONOS)
› JZ-Tree: GPU friendly neighbour search and friends-of-friends with dual tree walks in JAX plus CUDA
› $\xi R\phi^2$ non-minimal coupling, and the long range gravitational potential for different spin fields from 2-2 scattering amplitudes
› Posterior Predictive Checks for Gravitational-wave Populations: Limitations and Improvements
› Massive Exchange and the Sign of the Equilateral Bispectrum
› Effects of pair freeze-out on photon distributions in BBN epoch
› Cosmological Simulations of Stellar Halos with Gaia Sausage-Enceladus Analogues: Two Sausages, One Bun?
› Spectral Imaging with QUBIC: building frequency maps from Time-Ordered-Data using Bolometric Interferometry
› Temporary EHBL-like behavior of Markarian 501 during July 2014 VHE flaring
› Strong LensIng and Cluster Evolution (SLICE) with JWST: Early Results, Lens Models, and High-Redshift Detections
› ACT-ing on inflation: Implications of non Bunch-Davies initial condition and reheating on single-field slow roll models
› Eccentric millisecond pulsar + subdwarf B star from rotationally delayed accretion-induced-collapse scenario
› Impact of initial mass function on the chemical evolution of high-redshift galaxies
› Frabjous: Deep Learning Fast Radio Burst Morphologies
› Testing Dark Matter with Generative Models for Extragalactic Stellar Streams
› Impact of black hole spin on low-mass black hole-neutron star mergers
› The Fraction of Clumpy Galaxies in JADES over $2
› Hillas meets Eddington: The case for blazars as ultra-high-energy neutrino sources
› Fuzzy dark matter dynamical friction: stalling of globular clusters induced by dynamical heatings
› Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift
› XSNAP: An X-ray Supernova Analysis Pipeline with Application to the Type II Supernova 2024ggi
› Constraining interacting dark energy models with black hole superradiance
› Absorption effects in the expanding Universe: spectral transmittance functions of intergalactic medium for distant sources
› The DREAMS Project: Disentangling the Impact of Halo-to-Halo Variance and Baryonic Feedback on Milky Way Dark Matter Density Profiles
› Optical polarimetry of the accreting black hole X-ray binary Swift J1727.8$-$1613 over the state transition and radio ejections
› Tracking Protostellar Variability in Massive Protoclusters with ALMA: I. Insights from QUARKS and MaMMOtH
› Cygnus X-3: A variable petaelectronvolt gamma-ray source
› A Shocked Wind Interpretation of an Odd Radio Circle
› Early Planet Formation in Embedded Disks (eDisk). XIX. Structures of molecular outflows
› The Double-Peaked Calcium-Strong SN 2025coe: Progenitor Constraints from Early Interaction and Ejecta Asymmetries
› HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them
› Accretion disc winds in X-ray binaries
› VLBI Observations of SN 2012au Reveal a Compact Radio Source a Decade Post Explosion
› Spectroscopic confirmation of a large and luminous galaxy with weak emission lines at $\mathbf{z = 13.53}$
› The long quest for vacuum birefringence in magnetars: 1E 1547.0-5408 and the elusive smoking gun
› Statistical Predictions of the Accreted Stellar Halos around Milky Way-Like Galaxies
› The Bondi universe: Can negative mass drive the cosmological expansion?
› An Open-Source High-Level Graphical Signal Processing Language with Simulation and HDL Generation
› NE2025: An Updated Electron Density Model for the Galactic Interstellar Medium
› Revisiting the Perseus Cluster II: Metallicity-Dependence of Massive Stars and Chemical Enrichment History
› Revisiting the Perseus Cluster III: Role of Aspherical Explosions on its Chemical Composition and Extension to Metal-Poor Stars and Galaxies
› FRB scattering statistics through the CGM are sensitive to morphology and intermittency
› Active Galactic Nuclei-driven Metallicity Enrichment in the Interstellar Medium of Mrk 573
› Temporal Variation of the Coronal Radius Parameter in a Jetted Tidal Disruption Event: Swift J1644+57
› The diagnostic temperature discrepancy as evidence for non-Maxwellian coronal electrons
› VHE gamma-ray intranight variability from BL Lacertae during the extreme flaring state of 2022
› ALMAGAL VIII. Early phases of triggered star formation in source AG286.0716$-$1.8229
› Exploring the interplay of late-time dynamical dark energy and new physics before recombination
› STRADAViT: Towards a Foundational Model for Radio Astronomy through Self-Supervised Transfer
› Spectroscopic Redshifts for 461 Euclid Q1 Strong Gravitational Lenses from NISP Slitless Spectroscopy
› Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data?
› Beyond $f(\phi)\mathcal{G}$: Gauss--Bonnet inflation with $\mu(\phi,X)$
› Random gas motions inside sub-parsec scale supercritical filaments
› Resummation of Universal Tails in Gravitational Waveforms
› Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear
› 5-Dimensional Gravitational Raman Scattering: Scalar Wave Perturbations in Schwarzschild-Tangherlini Spacetime
› Teaching Astronomy with Large Language Models
› Quantum corrections to symmetron fifth-force profiles
› Detectability of axion-like dark matter for different time-delay interferometry combinations in space-based gravitational wave detectors
› Evaporation of Primordial Black Holes in a Thermal Universe: A Thermofield Dynamics Approach

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