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RSS  Latest preprints on astro-ph:

› Foiling Black Hole Foils: Revealing Horizon Alternatives with Baryonic Atmospheres
› Supermassive black holes swallow stellar objects at high rates: from Little Red Dots to Black Hole Stars
› A targeted machine learning approach for detecting diffuse radio emission with Astronomaly: Protege
› What does it mean to take the mean? The effect of the averaging scale on the characterization of interstellar turbulence
› CLASH-VLT velocity anisotropy profiles in a stack of massive galaxy clusters
› Little Red Dots as Globular Clusters in Formation
› Exploring the Near Galactic Centre: A Comprehensive Study of Bulge OCs HSC 25, HSC 37, HSC 2878 Utilising Gaia DR3 Data
› Implications of the nanoHertz Gravitational-Wave Background for Galactic Feedback and Massive Black Hole Growth
› The large cores of dark matter and globular clusters in AS1063. Possible evidence of self-interacting dark matter. Or not
› The LOFAR Two-metre Sky Survey: VII. Third Data Release
› MadEvolve: Evolutionary Optimization of Cosmological Algorithms with Large Language Models
› Gas Accretion versus BH Merger driven Growth Modes of Supermassive Black Holes and Implications for the Little Red Dots
› Is the overconcentration of pristine populations in Galactic globular clusters real? An N-body approach to the problem
› Stellar microlensing as a probe of Primordial Black Holes: status and prospects
› Early Results from the Coma Legacy IFU Survey (CLIFS): Ram Pressure Induced Shocks and Ionization in Jellyfish Tails
› Planet-Disk Interactions and the Convective Overstability. I. Low Mass Planets
› Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. III. Comparison between Starspot Mapping, Zeeman Doppler Imaging, and Multiwavelength Variability
› CHARA Array Delay Lines: Upgrades, Performance and Future Directions
› Molecular diagnostics for the mid-infrared emission of planet-forming disks. Carbon and oxygen elemental abundances
› Diffusive Instabilities in Dusty Disks: Linear Growth and Nonlinear Breakdown
› Direct contact binary planetesimal formation from gravitational collapse
› The Carousel Lens II: Cosmological Constraints with GIGA-Lens
› Evolution of Low-Mass Population III Stars: Convection, Mass Loss, Nucleosynthesis, and Neutrinos
› Three Saturn-mass Microlensing Planets Identified through Signals from Peripheral-caustic Perturbations
› Effects of Symmetron on growth and RSD multipoles
› Graph--Based Event Fingerprints for Classifying Geomagnetic Storm--Driven Forbush Decreases
› First Detection of the Baryon Acoustic Oscillation (BAO) Feature in the 3-Point Correlation Function of DESI DR1 Luminous Red Galaxies
› Investigating Ionospheric TEC Variations in Solar and Geomagnetic Influences Across Solar Activity Phases
› Cosmic Ray Spectra and Metal Budget Regulated by the Galactic Wind
› Reinterpreting the sunward electron deficit: Implications for solar wind acceleration and core population formation
› The Enigmatic Type Icn Supernova 2024abvb Located ~22 kpc from Its Host Galaxy
› Propagation Characteristics of the April 21, 2023 CME
› A XRISM View of the Iron Line Complex in NGC 1068: Rethinking the Prototypical Compton-Thick AGN
› PDRs4All XXI. JWST-NIRCam Photometric properties of protoplanetary disks in the Orion Nebula Cluster
› SPT-CL J0417-4748: A Deep Chandra Study of a Relaxed Galaxy Cluster Without Central Star Formation
› Numerical analysis of Lyapunov Times for Trans-Neptunian Objects and Main-Belt Asteroids: stability, accuracy, and methodological comparisons
› High significance detection at 4.8 GHz of the radio halo in the Coma galaxy cluster with the Sardinia Radio Telescope
› Localized $^{18}$O production in white dwarf mergers
› Accretion Disk Magnetic Braking
› Deepest ever photographed Geminid with small but not negligible terminal mass
› A fast radio burst cyclone in technicolour: evidence of plasma lensing
› The Astronomical Telescope of the University of Stuttgart (ATUS): Development, Optimization, and Lessons Learned
› Euclid preparation. Impact of galaxy intrinsic alignment modelling choices on Euclid 3x2pt cosmology
› Benchmarking Photolysis Rates with Socrates (24.11): Species for Earth and Exoplanets
› Resolving the Multiple Component Outflows in PG 1211+143: II. The Soft X-ray View of the Ultra Fast Outflow
› The role of radiative torques in the molecular cloud core L43
› New self-consistent theoretical descriptions for mass-loss rates of O-type stars
› Searching for White Dwarf Candidates Formed Through Binary evolution in Star Clusters
› GOTO identification and broadband modelling of the counterpart to the SVOM GRB 250818B
› Chiral gravitational waves from multi-phase magnetogenesis
› Meteor statistics I: The distribution of instrumental magnitudes
› HOLISMOKES XX. Lens models of binary lens galaxies with five images of Supernova Winny
› Two warm sub-Saturn mass planets identified from the TESS Full Frame Images
› Interpreting the HI 21-cm cosmology maps through Largest Cluster Statistics III: Impact of the lightcone effect
› Investigating Nonlinear Quenching Effects on Polar Field Buildup in the Sun Using Physics-Informed Neural Networks
› Updated Constraints on Infrared Cutoff Models and Implications for Large-Scale CMB Anomalies
› Orbital Motions of Binaries in Orion South
› How Bursty is Star Formation at z>5?
› Particle-in-Cell Methods for Simulations of Sheared, Expanding, or Escaping Astrophysical Plasma
› New formula for Asymptotic behavior of the Synchrotron function
› Statistics of Daily Modulation in Dark Matter Direct Detection Experiments
› Solving BDNK diffusion using physics-informed neural networks
› Rotating Black Holes with Primary Scalar Hair: Shadow Signatures in Beyond Horndeski Gravity
› Prediction of Major Solar Flares Using Interpretable Class-dependent Reward Framework with Active Region Magnetograms and Domain Knowledge
› Gravitational Waves from Primordial Black Holes formed by Null Energy Condition Violation during Inflation
› Characterization of an MPPC-Based Scintillator Telescope and Measurement of Cosmic Muon Angular Distribution
› Comet-type periodic motions and their out-of-plane bifurcations in the Earth-Moon CR3BP: a computational symplectic analysis
› Prompt And Delayed Radio Bangs At Kilohertz By SN 1987A: A Test For Graviton-Photon Conversion
› Precessing Gamma Jets in extended and evaporating galactic halo as a source of GRB
› Inverse Compton Scattering onto BBR in High Energy Physics and Gamma (MeV-Tev) Astrophysics
› The role of \nu_{\tau} ultrahigh energy astrophysics in Km^3 detectors
› Adiabatic or Non-Adiabatic? Unraveling the Nature of Initial Conditions in the Cosmological Gravitational Wave Background
› Dark Energy Survey: Galaxy Sample for the Baryonic Acoustic Oscillation Measurement from the Final Dataset
› AbacusPNG: A modest set of simulations of local-type primordial non-Gaussianity in the DESI era
› Novel Physics of Escaping Secondary Atmospheres May Shape the Cosmic Shoreline
› The Effect of Foreground Galaxies on the Estimation of the Hubble Constant from Type Ia Supernovae
› X-ray emission in IllustrisTNG circum-cluster environments. II -- Possible origins of the soft X-ray excess emission
› Inflationary Fossils Beyond Perturbation Theory
› Can GW231123 have a stellar origin?
› Sound-Horizon-Agnostic Inference of the Hubble Constant and Neutrino Mass from BAO, CMB Lensing, and Galaxy Weak Lensing and Clustering
› A novel algorithm for GPU-accelerated particle-mesh interactions implemented in the QUOKKA code
› The warm outer layer of a Little Red Dot as the source of [Fe II] and collisional Balmer lines with scattering wings
› Millimeter-Wavelength Lens-Absorber-Coupled Ti/Al Kinetic Inductance Detectors
› StarEmbed: Benchmarking Time Series Foundation Models on Astronomical Observations of Variable Stars
› An Explicit M1 Radiation-hydrodynamics Scheme for 3D Protostellar Evolution
› Radiation-dominated polar emitting region of an accreting X-ray pulsar -- I. Polarization- and spectrum-dependent structure, and the emergent continuum
› Dark Energy Survey Year 3 results: Simulation-based $w$CDM inference from weak lensing and galaxy clustering maps with deep learning: Analysis design
› Data-driven Radiative Magnetohydrodynamics Simulations with the MURaM Code: the Emergence of Active Region 11158 and the X2.2 Flare
› Dust destruction by the supernova remnant forward shock in a turbulent interstellar medium
› JOYS: JWST MIRI/MRS spectra of the inner 500 au region of the L1527 IRS bipolar outflow
› A Universal CMB $B$-Mode Spectrum from Early Causal Tensor Sources
› JWST imaging of the Pleiades: anisotropy of turbulence in the cold neutral medium
› Exploring Cosmological Tensions with Hubble Parameter Tomography via Linear Cosmography
› TIC-65910228 b / NGTS-38 b, a 180 day transiting warm super-Jupiter
› The James Webb Space Telescope Absolute Flux Calibration. V. Near-Infrared Camera Wide Field Slitless Spectroscopy
› Production of Jets before Neutron Star Mergers
› Hipparcos period-luminosity relations for Miras and semiregular variables
› Relativistic magnetohydrodynamics in the early Universe
› Cosmic Axions Revealed via Amplified Modulation of Ellipticity of Laser (CARAMEL)
› High-Precision Measurement of D($\gamma$, $n$)$p$ Photodisintegration Reaction and Implications for Big-Bang Nucleosynthesis
› Shadow of rotating black holes with consistent thermodynamics
› Photon Accelerator in Magnetized Electron-Ion Plasma
› Post-Newtonian Dynamics of Radiating Charges: Canonical Formulation and Binary Inspiral Laws
› Dark Matter Heating of Compact Stars Beyond Capture: A Relativistic Framework for Energy Deposition by Particle Beams
› Some phenomenological aspects of a quantum-corrected Reissner-Nordstr\"{o}m black hole: quasi-periodic oscillations, scalar perturbations and thermal fluctuations

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