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RSS  Latest preprints on astro-ph:

› A New Plotly-Dash-based Query Infrastructure for the Keck Observatory Archive
› Resonant Axion-Photon Conversion in the Early Inspiral of Neutron Star Binaries
› GW-FALCON: A Novel Feature-Driven Deep Learning Approach for Early Warning Alerts of BNS and NSBH Inspirals in Next-Generation GW Observatories
› Coupled Map Lattice for Astronomical Object Formation: A Scenario for Evolution from Star to Disk, Arms, and Companions
› Well-being and career instability across genders in the Spanish Astronomical Society
› PSR J0024$-$7204ai: a massive, eccentric binary system in the globular cluster 47 Tucanae
› Intracluster globular clusters as tracers of the mass assembly of the Hydra I galaxy cluster
› UV and Optical Signatures of Late-time Disk Instabilities in Tidal Disruption Events
› ABCMB: A Python+JAX Package for the Cosmic Microwave Background Power Spectrum
› Searching for Extragalactic Exoplanets: A Survey of the Sagittarius Dwarf Galaxy Stream with TESS
› Barium Stars Across the Milky Way: Probing Their Origins via the GALAH Survey
› The diverse nature of spiral arms in the Auriga Superstars cosmological hydrodynamic simulations
› The dependence of triggering mechanisms on radio AGN sub-types: the role of galaxy mergers
› Measuring Pulsar Distances from Chirping Orbital Periods
› Orbital eccentricity can make neutron star g-mode resonances observable with current gravitational-wave detectors
› Detection horizon for the neutrino burst from the stellar helium flash
› Magnetohydrodynamic Precipitation
› AGN in massive galaxies identified via optical broadband variability: lessons from VST-COSMOS for future LSST science
› Mimicking the large-scale structure of the Local Universe. Synthetic pre-labelled galaxies in large-scale structures
› Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET)
› The eruptive young star IRAS 21204+4913
› Three-Dimensional Kinematics of the Oxygen-rich Supernova Remnant G292.0+1.8
› A Response to paper Critical Evaluation of Studies Alleging Evidence for Technosignatures in the POSS1-E Photographic Plates by Watters et al. (2026)
› Helium superluminous SN 2021bnw : an explosion of a massive star with a pre-outburst
› Vertical Temperature Structure in Io's Atmosphere from ALMA SO$_2$ Observations
› Multi-Arrival Infrasound from Meteoroids: Fragmentation Signatures versus Propagation Effects in a Fine-Scale Layered Atmosphere
› GPS constellation search for exotic physics messengers coincident with the binary neutron star merger GW170817
› New Insights from Revisiting the Rotation Period of the Strongly Magnetic O Star, NGC 1624-2
› On the dynamics, thermodynamics and fine structure of virtual erupting filaments
› Calibrating the Tip of the Red Giant Branch and measuring Magellanic Cloud distances to 2% exclusively with Gaia
› The First Instrumentally Documented Fall of an Iron Meteorite: atmospheric trajectory and ground impact
› Cosmological Averaging in Nonminimally Coupled Gravity
› A Quantum Genetic Algorithm with application to Cosmological Parameters Estimation
› Coronal Non-Thermal and Doppler Plasma Flows Driven by Photospheric Flux in 28 Active Regions
› Scaling solutions in three-form cosmology
› Precise measurement of WASP-31 b's Rossiter-McLaughlin effect and characterization of the planet transmission spectra
› Upper atmosphere dynamics and drivers of volatiles loss from terrestrial-type (exo)planets
› Cosmic topology. Part IIc. Detectability with non-standard primordial power spectrum
› A homogeneous view of asymptotic giant branch carbon stars as seen by Gaia
› An observational test of the plasma lensing effect using QSOs with and without MgII absorption
› Bridging Scales in Black Hole Accretion and Feedback: Subgrid Prescription from First Principles
› Inference of horizontal velocity fields from the induction equation in the solar atmosphere. I. Analytical and numerical solutions in 2D
› Dust measurements with the Mars Dust Counter on board Nozomi (PLANET-B)
› Morphological variations of solar granules in the presence of magnetic fields
› Aligned and misaligned metallicity gradients in young stars and star-forming regions in the EAGLE discs
› Fast computation of temperature and polarization coupling matrices
› Searching for Axion-like particle Dark Matter with Time-domain Polarization: Constraints from a protoplanetary disk
› Bayesian parameter study of the Seyfert-starburst composite galaxies NGC 1068 and NGC 7469
› Spectroscopic analysis and RHD modeling of the first Ca II H and H-epsilon flare spectra from DKIST/ViSP
› Detecting the neutrino mass via the cross-correlation between matter tracers and the ISWRS effect?
› Hot subdwarf stars from the Hamburg Quasar Survey
› The Montreal Open Clusters and Associations (MOCA) Database: A Census of Nearby Associations, Open Clusters, and Young Substellar Objects within 500 pc of the Sun
› Impact of rotation on the amplitude of acoustic modes in solar-like stars: Insights from hydrodynamical simulations
› Slow focus sensor for the Keck I laser guide star adaptive optics system using focal plane wavefront sensing
› Deep Learning for Point Spread Function Modeling in Cosmology
› Between Plateaus and Slopes: A Data-Driven Exploration of Spectral Diversity Across Type IIP/L Supernovae
› WISDOM Project - XXVII. Giant molecular clouds of the lenticular galaxy NGC 1387: similarities with spiral galaxy clouds
› Nearest Neighbour-Based Statistics for 21cm-Galaxy Cross-Correlations in the Epoch of Reionization
› Exploring Chaotic Motion of a Particle in the Centre of a Galaxy with a Prolate Halo
› Venting and Outgassing Simulations of Pressurized Lunar Modules: Contamination of the Lunar Environment
› Model selection with the Pantheon+ Type Ia SN sample
› Blackening Cryosphere: Revealing Hotspot Shifts and HGB-Based Forecasting of Absorbing Aerosol Threats over the Himalayan Frozen Frontiers
› May Negative Mass Objects exist in the sky?
› IT-DPC-SRI: A Cloud-Optimized Archive of Italian Radar Precipitation (2010-2025)
› The Sun Can Strongly Constrain Spin-Dependent Dark Matter Nucleon Scattering Below the Evaporation Limit
› Enhanced Cosmic-Ray Antinuclei Fluxes with Dark Matter Annihilation into SUEPs
› Primordial black hole evaporation in a thermal bath and gravitational waves
› Some phenomenological aspects of a quantum-corrected Reissner-Nordstr\"{o}m black hole: quasi-periodic oscillations, scalar perturbations and thermal fluctuations
› Radial oscillations of pulsating neutron stars: The UCIa equation-of-state case
› Hubble-Scale Tachyonic Shocks from Low-Scale Inflation -- A New Gravitational-Wave Window on Inflation
› Probing neutrino emission at GeV energies from compact binary mergers with the IceCube Neutrino Observatory
› Revisiting bright delta Scuti stars and their period-luminosity relation with TESS and Gaia DR3
› WISDOM project -- XVIII. Molecular gas distributions and kinematics of three megamaser galaxies
› Identifying 850 delta Scuti pulsators in a narrow Gaia colour range with TESS 10-minute full-frame images
› Astrometric constraints on stochastic gravitational wave background with neural networks
› Gravitational waves from cosmic strings for pedestrians
› The HST-Hyperion Survey: Companion Fraction and Overdensity in a z ~ 2.5 Proto-supercluster
› Influence of finite-temperature effects on CMB power spectrum
› Stochastic analysis of finite-temperature effects on cosmological parameters by artificial neural networks
› Late-blooming magnetars: awakening as long period transients after a dormant cooling epoch
› The Single-Degenerate Channel Leads to Type Iax and Not Type Ia Supernovae due to Premature Ignition
› Characterizing bright $\delta$ Scuti pulsators using TESS lightcurves
› The Diversity and Evolution of Dust Attenuation Curves from Redshift z ~ 1 to 9
› Investigating the Gamma-Ray Emission from Explosive Dispersal Outflows with Fermi-LAT
› A hybrid active galactic nucleus feedback model with spinning black holes, winds and jets
› Carnegie Supernova Project: Fast-Declining Type Ia Supernovae as Cosmological Distance Indicators
› Dark-to-black super accretion as a mechanism for early supermassive black hole growth
› Beyond CPL: Evidence for dynamical dark energy in three-parameter models
› Crosschecking Cosmic Distances from DESI BAO and DES SNe Points to Systematics
› JWST/MIRI-MRS view of the metal-poor galaxy CGCG 007-025: the spatial location of PAHs and very highly ionized gas
› Ephemeris and Almanac Design for Lunar Navigation Satellites
› Formation Channels of Magnetars
› Synchrotron radiation from NGC 470 HLX1 - a hidden hyperluminous accreting neutron star?
› Non-Gaussianity in SMICA
› JWST observations of three long-period AM CVn binaries: detection of the donors and hints of magnetically truncated disks
› Fluctuation dynamos in supersonic turbulence at ${\rm Pm} \gtrsim 1$
› Multigroup Radiation Diffusion on a Moving Mesh: Implementation in RICH and Application to Tidal Disruption Events
› Digging into the Interior of Hot Cores with ALMA (DIHCA). VI. The Formation of Low-mass Multiple Systems in High-mass Cluster-forming Regions
› Prediction of Multi-Wavelength Afterglows Associated with FRB 20200120E and FRB 20201124A
› WLM: Dynamics of an isolated Dwarf Irregular Galaxy Under Ram Pressure in the Local Group
› Dynamics of the coronal magnetic field in the 2022-10-02 X-class flare
› Seasonal Variation of Polar Ice: Implications for Ultrahigh Energy Neutrino Detectors
› First statistical constraints on galactic scale outflows properties traced by their extended Mg II emission with MUSE
› Is cosmic birefringence due to dark energy or dark matter? Simulation-based inference
› Self-Consistent Direct Method for Chemical Abundances in High-z Galaxies with JWST
› Microphysical Model of Jupiter's Great Red Spot Upper Chromophore Haze
› The Numerics of VMEC++
› Deflection angle in the strong deflection limit: A perspective from local geometrical invariants and matter distributions
› Explaining the PeV Neutrino Fluxes at KM3NeT and IceCube with Quasi-Extremal Primordial Black Holes
› Secluded Dark Composites and Remnant Binding Fields
› Gravothermal Pile-Up of Collisional Dark Matter Around Compact Objects
› Testing Real WIMPs with CTAO
› Nonstrange and strange quark matter at finite temperature within modified NJL model and protoquark stars
› Coordinate Systems and Transforms in Space Physics: Terms, Definitions, Implementations, and Recommendations for Reproducibility
› Multibanded Reduced Order Quadrature Techniques for Gravitational Wave Inference

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