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Dome at sunrise
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RSS  Latest preprints on astro-ph:

› The indiscriminate adoption of AI threatens the foundations of academia
› Observing solar vortices with existing and future instrumentation. Solar Physics International Network for Swirls (SPINS) white paper (Helio)
› Cosmo3DFlow: Wavelet Flow Matching for Spatial-to-Spectral Compression in Reconstructing the Early Universe
› Statistical isotropy of the universe and the look-elsewhere effect
› TDE 2025abcr: A Tidal Disruption Event in the Outskirts of a Massive Galaxy
› Why do we do astrophysics?
› A method for constructing the joint mass function of binary stars
› Modern tidal interaction models for rapid binary population synthesis: I. Methods
› Machine Learning Methods for Stellar Collisions. I. Predicting Outcomes of SPH Simulations
› Forged by Feedback: Stellar Properties of Brightest Group Galaxies in Cosmological Simulations
› The stellar-to-halo mass relation of central galaxies across three orders of halo mass
› Keck Observations in the INfrared of Taurus and $\rho$ Oph Exoplanets And Ultracool dwarfs (KOINTREAU) II: Two Young Bound Companions to Ophiuchus Stars
› New Deep Radio Continuum Imaging Still Indicates a Large Reservoir of Undiscovered Millisecond Pulsars in Terzan 5
› The Keck/DEIMOS Stellar Archive: I. Uniform Velocities and Metallicities for 78 Milky Way Dwarf Galaxies and Globular Clusters
› The Keck/DEIMOS Stellar Archive: II. Dynamical Masses and Metallicities for a Uniform Sample of Milky Way Satellites
› Optimizing Deep Learning Photometric Redshifts for the Roman Space Telescope with HST/CANDELS
› Evidence for neutrino emission from X-ray Bright Seyfert Galaxies in the Southern Hemisphere using Enhanced Starting Track Events with IceCube
› The Landscape of Unstable Mass Transfer in Interacting Binaries and Its Imprint on the Population of Luminous Red Novae
› On the Expected Orbitally-modulated TeV Signatures of Spider Binaries: The Effect of Intrabinary Shock Geometry
› Linking Solar Magnetism, Extreme Solar Particle Events and Stellar Superflares
› The S-PLUS Fornax Project (S+FP): An extragalactic catalog covering $\sim$ 5 virial radii around NGC 1399 with galaxy properties
› Long-Term Evolution of Close-in Sub-Neptunes and Outer Planetary Embryos: Atmospheric Mass Loss and Origin of Planets Inside and Outside the Radius Gap
› Cold and eccentric: a high-spectral resolution view of 51 Eri b with VLT/HiRISE
› Solar Wind Heating Near the Sun: A Radial Evolution Approach
› Evidence that SOL2012-06-03 Late Phase $\gamma$ Rays are Produced by $>$300 MeV Protons from CME-Shock Acceleration of Suprathermals from the Flare
› Carbon from Interstellar Clouds to Habitable Worlds
› Re-visiting the Canis Major star-forming region with Gaia data release 3 data
› Carbon-Enhanced Metal-Poor Star Candidates in the Milky Way from J-PLUS and S-PLUS
› Constraining the Evolution of the HI Spin Temperature with Fast Radio Bursts
› Efficient reduction of stellar contamination and noise in planetary transmission spectra using neural networks
› Searching for radio emission from stellar wind-magnetosphere interaction or co-rotation breakdown in brown dwarfs
› MAGNUS III: Mild evolution of the total density slope in massive early-type galaxies since z$\sim$1 from dynamical modeling of MUSE integral-field stellar kinematics
› Not Earth-like Yet Temperate? More Generic Climate Feedback Configurations Still Allow Temperate Climates in Habitable Zone Exo-Earth Candidates
› Data-driven Magnetohydrodynamic Simulation of the Initiation of a Coronal Mass Ejection with Multiple Stages
› A 682-second X-ray Periodicity in CH Cygni: Evidence for a Magnetic White Dwarf
› First Detection of $\gamma$-Ray Emission from the Compact Symmetric Object JVAS J1311+1658
› Cosmic-ray electron propagation in NGC 3044 from radio continuum observations
› Linking {\it Fermi} blazars and radio galaxies through accretion and jet radiation mechanisms
› Distance Estimation and Sky Localization of Eccentric Double White Dwarf Binaries from Gravitational Wave Observations inside Globular Clusters
› The role of detailed gas and dust opacities in shaping the evolution of the inner disc edge subject to episodic accretion
› JWST spectra are consistent with the edge-on star-forming galaxy scenario for the "runaway supermassive black hole"
› Chemistry in the High expansion-velocity C-rich evolved star AFGL2233. Isotopic ratios, peculiarities and evolutionary status
› The metal-poor tail of the APOGEE survey I. Uncovering [Fe/H] < -2.5 stars from the inner Galaxy to the Magellanic Clouds
› The metal-poor tail of the APOGEE survey II. Spectral analysis of Mg and Si in very metal-poor APOGEE spectra
› Deep and Sparse Denoising Benchmarks for Spectral Data Cubes of High-z Galaxies: From Simulations to ALMA observations
› GECAM discovery of the second FRB-associated Magnetar X-ray Burst from SGR J1935+2154
› Pollux test bench: from NUV to FUV polarimetric measurements
› Reevaluating thermal instability in a uniform plasma: an extended analysis of instability domains
› Massive stars as gravitationally lensed transients -- Insights on the high-mass initial mass function
› HD 164604 c: a second giant planet on a 15-yr orbit and the constraint of the planet-planet mutual inclination
› An Enhanced Formation Channel for Galactic Dual-Line Gravitational-Wave Sources: von Zeipel-Lidov-Kozai effect in Triples Involving Sgr A*
› A search for new symbiotic stars in the Milky Way: Using machine learning techniques applied to photometric databases
› X-ray stellar feedback in low-metallicity starbursts: Insights from the template starburst galaxy ESO 338-IG04 and its halo
› Beyond $\Lambda$CDM: fundamental constants as cosmological observables
› TESS planets in known radial velocity cold Jupiter systems: Hot super Earth occurrence is enhanced by cold Jupiters
› Population Properties of Binary Black Holes with Eccentricity
› Early Architecture Concepts for the Habitable Worlds Observatory -- System Design, Modeling, and Analysis
› Most Strong Lensing Deflectors in the AGEL Survey are in Group and Cluster Environments
› New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method
› Future Perspectives on Black Hole Jet Mechanisms: Insights from Next-Generation Observatories and Theoretical Developments
› Beyond thermal approximations: Precise cosmological bounds on Axion-Like Particles
› Non-thermal X-ray Emission from Merging Massive Black Hole Binaries
› Unmasking LHAASO J2108+5157: Near Infrared Insights into a Mysterious TeV Source
› Pushing the Limits of Atomic Dark Matter: First-Principles Recombination Rates and Cosmological Constraints
› Gravitational scalar production with a generic reheating scenario
› Accelerated expansion of the universe purely driven by scalar field fluctuations
› The measurable impact of the 2pN spin-dependent accelerations on the jet precession of M87$^\ast$
› Shocks, compressible perturbations, and intermittency in the very local interstellar medium: Voyager 1 and 2 observations and numerical modeling
› Bridging the Kinetic-Fluid Gap: Ion-Driven Magnetogenesis to Prime Cosmic Dynamos
› Unidentified falling objects in the LHC as dark matter signals
› Photons x Force: Differentiable Radiation Pressure Modeling
› Machine learning exploration of binding energy distributions of H2O at astrochemically relevant dust grain surfaces
› Collisionless relaxation as the origin of the anisotropic, non-thermal, and multi-temperature momentum distributions observed in space plasmas
› Light to Heavy, Brief to Eternal: An Axion for Every Occasion (in the Early Universe)
› First measurement of the correlation between cosmic voids and the Lyman-$\alpha$ forest
› Crustal lattice pressure as a source of neutron star mountains
› A second-scale periodicity in an active repeating fast radio burst source
› Sagittarius A* near-infrared flares polarization as a probe of space-time I: Non-rotating exotic compact objects
› Ten-dimensional neural network emulator for the nonlinear matter power spectrum
› Design and optimization of neural networks for multifidelity cosmological emulation
› The pulsar wind nebula around B1853+01 in X-rays
› A semi-coherent search for optical pulsations from Scorpius X-1
› The Interpolation Constraint in the RV Analysis of M-Dwarfs Using Empirical Templates
› Supermassive black hole growth from stellar binary encounters
› H-alpha as a Tracer of Star Formation in the SPHINX Cosmological Simulations
› The stability of propagating plane inertial waves in rotating fluids
› Cosmological Prediction from the joint observation of MeerKAT and CSST at $z$ = 0.4 $\sim$ 1.2
› JWST Observations of Starbursts: PAHs Closely Trace the Cool Phase of M82's Galactic Wind
› In-situ globular clusters in alternative dark matter Milky Way galaxies: a first approach to fuzzy and core-like dark matter theories
› The rise and fall of Little Red Dots could be driven by the environment
› From Common Envelope Evolution to Luminous Red Novae I: A One-dimensional Radiation Hydrodynamic Model
› HyperAIRI: a plug-and-play algorithm for precise hyperspectral image reconstruction in radio interferometry
› A volcanic chronosequence as a time-resolved paleo-detector array to study the cosmic-ray flux in the Late Pleistocene and Holocene
› Figuring Out Gas & Galaxies In Enzo (FOGGIE) XI: Circumgalactic O VI Emission Traces Clumpy Inflowing Recycled Gas
› REBELS-IFU: Spatially Resolved Ionizing Photon Production Efficiencies of 12 Bright Galaxies in the Epoch of Reionization
› The Spontaneous Genesis of Solar Prominence Structures Driven by Supergranulation in Three-Dimensional Simulations
› Accurate cosmological emulator for the probability distribution function of gravitational lensing of point sources
› MIRI spectrophotometry of GN-z11: Detection and nature of an optical red continuum component
› Asymptotic constraints for 1D planar grey photon diffusion from linear transport with special-relativistic effects
› A Galactic Transformation -- Understanding the SMC's Structural and Kinematic Disequilibrium
› Simulation-based inference with neural posterior estimation applied to X-ray spectral fitting -- III Deriving exact posteriors with dimension reduction and importance sampling
› Diagnosing the AGN population origin of TeV neutrinos with their spatial correlation
› The Cosmic-ray Knee as a Local Signature of Nearby PeVatrons
› Stellar masses of optically dark galaxies: uncertainty introduced by the attenuation law and star-formation histories
› Canceling Effects of Conjunctions Render Higher Order Mean Motion Resonances Weak
› Accretion Rate Changes Detected in a Polluted White Dwarf
› Primordial Black Hole signatures from femtolensing and spectral fringe of Gamma Ray Bursts
› A Faint Progenitor System for the Faint Supernova 2024vjm
› Continuous Gravitational Waves from Supersoft X-ray Sources: Promising Targets for deci-Hz Detectors
› Characterisation of starspot structure and differential rotation of Kepler-411
› EMU Radio Observations of Barred Spiral Galaxy NGC 5938 (Araish)
› Investigating the Nested Structure of the Outflow from the Low Luminosity Protostar IRAS 16253-2429 using JWST and ALMA
› Kilohertz Gravitational Waves from Binary Neutron Star Mergers: Full Spectrum Analyses and High-density Constraints on Neutron Star Matter
› Probing Non-Minimal Dark Sectors via the 21 cm Line at Cosmic Dawn
› Geodesics and Shadows in the Kerr-Bertotti-Robinson Black Hole Spacetime
› Lepton number crossings are insufficient for flavor instabilities
› An Implementation to Identify the Properties of Multiple Population of Gravitational Wave Sources
› Quasinormal Ringing and Unruh-Verlinde Temperature of the Frolov Black Hole
› First Multi-Constellation Observations of Navigation Satellite Signals in the Lunar Domain by Post-Processing L1/L5 IQ Snapshots
› Effect of noise characterization on the detection of mHz stochastic gravitational waves
› Realization of quintom dark energy after DESI DR2 in Nieh-Yan modified teleparallel gravity

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