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RSS  Latest preprints on astro-ph:

› Searching for Life-As-We-Don't-Know-It: Mission-relevant Application of Assembly Theory for Exoplanet Life Detection
› SpectralUnmix: A Torch-Based Regularized Non-negative Matrix Factorization
› The ocean worlds science case for the Pollux spectropolarimeter
› Martian concretion sizes predicted from two independently constrained inputs: atmospheric dust grain size and obliquity-forced wetting duration
› Masses of Potentially Habitable Planets Characterized by the Habitable Worlds Observatory
› AREPAS: A Resource for Exploring Protostellar Accretion Systems - Data Release I
› Kinematic cosmic dipole from a large sample of strong lenses
› Solar twins in Gaia DR3 GSP-Spec II. Age distribution and its implications for the Sun's migration
› GSE vs. LMC: reshaping of radially biased stellar haloes by satellites
› The TRGB-SBF Project. IV. A Color Calibration of the TRGB in the JWST F090W+F150W Filters
› FlowSN: Normalising Flows for Simulation-Based Inference under Realistic Selection Effects applied to Supernova Cosmology
› Isophote shape analysis and the unfortunate subtlety of dwarf galaxy structure
› Gravitational Wave Measurement of the Mbh-Mbulge Intrinsic Scatter at High Redshift
› Large-scale environments of star-forming active galactic nuclei: How black hole mass, accretion rate, and luminosity connect to dark matter halos
› Long GRB 250916A: an Off-axis Powerlaw Jet with Thermal Cocoon
› The Kinematically Hot, Extremely Metal-Poor C-19 Stellar Stream in DESI DR2
› Spontaneous Baryogenesis and Primordial Black Hole Dark Matter from Ultra-Slow-Roll Inflation
› A systematic study of AGN feedback in a disk galaxy I: global overview
› AGN obscuration in optical and X-rays: Host properties and the interplay of nuclear and galactic gas and dust in a combined SDSS-XMM sample
› Imprints of Reheating Dynamics on Gravitational Waves from Phase Transitions
› Not Where You Left Them: Displaced $\gamma$-Rays and X-Rays Reveal the Cosmic Ray Scattering Rate
› Thermal Evolution of the Central Star in Pa 30
› Upgrading Alpha Crucis to a seven star system. Discovery of Bb and orbital misalignment
› Cold giant discoveries from a joint radial-velocity and astrometry framework
› Unveiling Massive Main-Sequence Stars in Sextans A through Panchromatic Photometry
› Very long-term relaxation of harmonic 1D self-gravitating systems
› Neutrino Spectral Pinching in 3D Core-Collapse Supernovae: Late-Time Convergence, Failed-Explosion Signatures, and Viewing-Angle Dispersion
› Two Point Correlation Function Estimation with Contaminated Data
› Post-processing Probabilistic Forecasts of the Solar Wind by Data Mining Similar Scenarios
› PACHA: Probing AGN Coronae with High-redshift AGN
› New Observations of the Strongly Magnetic O-star NGC 1624-2 Reveal Its Magnetic South Pole
› Strong Prevalence of Hammerhead Velocity Distributions Close to the Heliospheric Current Sheet
› Proto-NUX: A prototype telescope for ground-based near-ultraviolet observations
› Balmer Decrements and Nebular-Stellar Reddening in JADES Galaxies at $2.7
› Galactic Stellar Halo Luminosity Function
› An Orbit for a Massive Wolf-Rayet Binary in the LMC: An Example of Binary Evolution
› Imploding Remnants: detection bias against AGNs in massive clusters
› Gravitational Lensing Effects by Galaxy Clusters on Ionised Bubble Size Distribution during the Epoch of Reionisation
› BLUEPRINT: Blue-dominant Lyman-alpha (Ly$\alpha$) emission as an evidence of gas inflow in ultra-low-mass galaxies at z = 3
› Marginally stable nuclear burning triggered at different depths of the neutron star surface in Low-mass X-ray binary 4U 1608-52
› Numerical Simulations of the Circularized Accretion Flow in Population III Star Tidal Disruption Events. II. Radiative Properties
› Three-dimensional Global Relativistic Radiation Magnetohydrodynamics of Magnetically Arrested Disk Accretion Flows in AGNs
› 50-250 MHz Pulsar Census with an SKA-Low prototype station: Spectra and Polarization
› Atmospheric Escape Rates from Mars - If it Orbited an Old M-Dwarf Star
› JWST's PEARLS: A clumpy ring galaxy at $z = 4.0148$
› Warm Inflation Beyond the Markovian Limit
› SN 2023axu: A Type IIP Supernova Interacted with a Low-Density Stellar Wind1
› Exploring the Viability of Fisher Discriminants in Galaxy Morphology Classification
› Constraints on Axion-Photon Mixing from Fast Radio Burst Dispersion Measures
› pyKurucz: A Pure Python Reimplementation of Kurucz SYNTHE for Stellar Spectrum Synthesis
› A unified scalar-field resolution of the $H_0$, $S_8$ and evolving Dark Energy tensions
› Revisiting early afterglows of gamma-ray bursts with finite-thickness ejecta: Implications from XRF 080330 and GRB 080710
› The Inner and Outer Shock Layers of Bow Shocks in Cataclysmic Variables
› Merger-driven buildup of the $M_{\rm BH}$ - $M_*$ relation bridging high-$z$ overmassive black holes with the local relation
› Reconstruction of Cepheid Radial Velocity Curves from the shape of the V-band Light Curves
› Self-consistent-field method for triaxial differentiated bodies in hydrostatic equilibrium
› Photometric and Spectral Evolution of the Symbiotic Nova HM Sagittae since 2003
› Origin of open clusters revealed by the evolution of the m_max$-$M_ecl relation
› Equilibrium figure of Haumea and possible detection by stellar occultation
› Continuum Reverberation in Bright Quasars Using NASA/ATLAS
› Binary disruption during the early phase of open clusters
› Chemo-dynamical reconstruction of Milky Way globular cluster progenitors: age--metallicity relations and the universality of multiple stellar populations
› The impact of baryons on weak lensing statistics as a function of halo mass and radius
› Energy dependence of the X-ray power spectrum in NGC4051 and NGC4395
› Cosmological gravity on all scales V: MCMC forecasts combining large scale structure and CMB lensing for binned phenomenological modified gravity
› \HI 21-cm Line Properties of the Nearby LIRG IRAS 04296+2923
› Unveiling the biconical geometry of the outflow in the ultraluminous X-ray source NGC 5204 X-1
› AS-Bridge: A Bidirectional Generative Framework Bridging Next-Generation Astronomical Surveys
› Identifying highly magnetized white dwarfs: A dimensionality reduction framework for estimating magnetic fields
› The Cold Debris Disk Surveys I. Host Star Properties
› The twin-jet system in the FRII radio galaxy 3C 452: A sub-parsec scale VLBI study
› Sensitivity to Axion-like Particle dark matter with very-high-energy gamma-ray observations of Active Galactic Nuclei located behind Galaxy Clusters
› A Cloudy Fit to the Atmosphere of WASP-107 b
› Detection of a weak magnetic field in the Balmer emission line white dwarf WDJ1653-1001
› Chemical radial gradients for the bulge-bar stellar populations from the APOGEE survey
› The shocking features in the closest rich galaxy cluster Norma
› Comparison of Bar Formation Mechanisms. IIIA. The role of classical bulges in spontaneous bar formation
› Rediscussion of eclipsing binaries. Paper XXIX. The F-type twin system BS Draconis
› The Targeted Standard Siren Cosmology with Pulsar Timing Arrays
› AstroSat-UVIT observations of a possibly interacting pair of galaxies in HCG 77
› Small-Scale and Transient EUV Kernels in Solar Flare Ribbons
› GATOS N: The first direct kinematic evidence of dusty outflows from AGN via PAH kinematics of local Seyfert galaxies with JWST
› X-ray evidence from NuSTAR for a Mach 3 shock in Merging Galaxy Cluster ZWCL 1856.8
› Comparing the $M_{gas}-N_{yso}$ Relation inside a Giant Molecular Cloud
› Magnetoacoustic Shocks and Spectropolarimetric Signals in He I 10830 {\AA}
› Scale-Dependent Loop Corrections to the Inflationary Power Spectrum
› An Updated \synthpop Model for Microlensing Simulations I: Model Description, Evaluation, and Microlensing Event Rates Near the Galactic Center
› Intrinsic Nonlocality of Spin- and Polarization-Resolved Probabilities in Strong-Field Quantum Electrodynamics
› Rayleigh-Taylor Unstable Flames: Thin and Thick
› Plasma effects on gravitational lensing and shadow observables of a Kerr-like black hole in a dark matter halo
› Analytic Singular Slow-roll Inflation
› Phase Retrieval using Nonlinear Curvature Sensing within Convergent Beams
› Overdamping of Neutron-Mirror-Neutron Transitions in Neutron Stars
› Assessing the robustness of amortized simulation-based inference to transient noise in gravitational-wave ringdowns
› Shifted-geodesic approximation for spinning-body gravitational wave fluxes
› Hawking Radiation from Tunneling in Black Hole Quantum Mechanics
› Strong Evidence Against a Statistically Isotropic Universe
› A search for super-imposed oscillations to the primordial power spectrum in Planck and SPT-3G 2018 data
› Tidal deformability of black holes surrounded by thin accretion disks
› Novel density profile for isothermal cores of dark matter halos
› Quintessential Implications of the presence of AdS in the Dark Energy sector
› Redshift Assessment Infrastructure Layers (RAIL): Rubin-era photometric redshift stress-testing and at-scale production
› Curvaton in light of the ACT results
› Stellar initial mass function in the 100-pc solar neighbourhood
› Constraining the contribution of Seyfert galaxies to the diffuse neutrino flux in light of point source observations
› Cosmic baryon census with fast radio bursts and gravitational waves
› Finding strangelets in cosmic rays from HESS J1731-347, a possible strange quark star using the Cherenkov Telescope Array Observatory
› Atmospheric Characterisation with the Twinkle Space Telescope Following Advances from JWST Observations
› Constraints on Dark Matter Models from Supermassive Black Hole Evolution
› Islands of Electromagnetic Tranquility in Our Galactic core and Little Red Dots that Shelter Molecules and Prebiotic Chemistry
› Introducing SESHAT: A Tool for Object Classification from JWST Catalogs
› Ultra-Faint Milky Way Satellites Discovered in Carina, Phoenix, and Telescopium with DELVE Data Release 3
› A constant upper luminosity limit of cool supergiant stars down to the extremely low metallicity of I Zw 18
› SN 2019vxm: A Shocking Coincidence between Fermi and TESS
› A Smooth Transition from Giant Planets to Brown Dwarfs from the Radial Occurrence Distribution
› Stellar Cores Live Long and Prosper in Cuspy Dark Matter Halos
› The polar IL Leo in a low accretion state
› High-energy Emission from Turbulent Electron-ion Coronae of Accreting Black Holes
› Scalar-induced gravitational waves and primordial black holes from a localized bump or dip feature in a single-field inflationary potential
› Time-variable Scattered Light in Herbig Disks Observed with Subaru/SCExAO
› The Dawes Review 14: A Decade of Ultra-Diffuse Galaxies
› The rotational and magnetic properties of Polaris from long-term spectropolarimetric monitoring
› A candidate proton cyclotron feature in the ultraluminous X-ray source NGC 4656 ULX-1
› Spectral Decomposition Reveals Surface Processes on Europa
› Translating current ALP photon coupling strength bounds to the Randall-Sundrum model
› Freeze-In Dark Matter and Leptogenesis: a $\psi'$SM route
› Dark Matter Clumps as Sources of Gravitational-Wave Glitches in LIGO/Virgo/KAGRA data
› Multi-field TDiff theories: the mixed regime case
› Testing Seesaw and Leptogenesis via Gravitational Waves: Majorana versus Dirac
› Natural inflation in Palatini $F(R)$
› Superluminal constraints from ultra-high-energy neutrino events
› Resonances in binary extreme mass ratio inspirals
› The reason peculiar velocities grow faster in general relativity than in Newtonian gravity
› Schwarzian Theory and Cosmological Constant Problem
› Scaling Laws for Template-Free Detection of Environmental Phase Modulation in Gravitational-Wave Signals
› Orbital Dynamics and Gravitational Wave Signatures of Extreme Mass Ratio Inspirals in Galactic Dark Matter Halos
› On the Value of Tokeniser Pretraining in Physics Foundation Models

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