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RSS  Latest preprints on astro-ph:

› Stellar Detection Counts Are Invariant Across Geomagnetic Storm Intensity in POSS-I Plates: Ruling Out the Plate Sensitivity Artifact and Confirming Source-Specific Transient Suppression
› AI--Assisted Exploration: DHOST Theories without Quantum Ghosts
› Classifying Supermassive Black Hole Growth Regimes to Observables Across Cosmological Simulations with Forecasts for LSST
› A First Investigation of Repeated-Signal Localization of Strongly Lensed Gravitational Waves for Multimessenger Astronomy
› On the Gamma-ray Efficiency of Superluminous Supernovae: Potential Detections and Population-Level Constraints
› Old Universe, Young SNe Ia: A Statistical Analysis of Type Ia Supernova Progenitor Age from 6,983 TITAN Host Galaxies, and Implications for Cosmology
› A data-driven prediction for the primordial deuterium abundance
› SDSS-V LVM: Verifying what, and where, the 'Galactic Center' Lobe is
› Carbonaceous Chondrites provide evidence for late-stage planetesimal formation in a pressure bump
› Possible fractal nature of accretion flows in MAD and SANE simulations: Implications to GRS 1915+105
› Evidence for Environmental Stripping in the Coma Cluster
› Dynamical dark energy from Kretschmann scalar at low redshifts
› Neutron star atmospheres composed of fusion ashes
› A search for the first galaxies across $>0.6$ deg$^2$ of JWST imaging: new evidence for a rapid decline in star-formation activity at $z>12$
› Persistence of the Millihertz X-ray Quasi-Periodic Oscillation in the Active Galactic Nucleus 1ES 1927+654
› The Metallicity Gradient of Sagittarius Dwarf Spheroidal Galaxy Prior to Infall Constrained by S-PLUS Observations of its Tidal Stream
› heliostack: A Novel Approach to Minor Planet Discovery
› Stellar Coronal Mass Ejections with HWO: A Science Case Concept
› The Qz5 Survey (II): Metallicity Evolution of Damped Ly{\alpha} Systems Out to z$\sim$5
› GeV emission in the region of Vela: a new view of the supernova remnant
› The Role of Cluster Environments in Quiescent Galaxy Stellar Halo Assembly
› AstroSURE: Learning to Remove Noise from Astronomical Images Without Ground Truth Data
› W UMa-Type Contact Binaries in the Tidal Tails of Young Open Cluster COIN-Gaia 25 and Mamajek 4
› Dense Ionized Outflow with Five Narrow Components in a Dust-obscured Galaxy
› Carbon Cycle Imbalances on Arid Terrestrial Planets with Implications for Venus
› Signatures of Massive Neutrinos in the Cosmic Web via Persistent Homology
› A newly born spider system at the core of a radio shell: Evidence for a low-energy supernova
› Cosmoglobe: Mapping the Universe from the Milky Way to the Big Bang
› Testing Weak Equivalence Principle with IceCube Event and Blazar
› Search for galactic structures and study of their kinematics in the Gaia era
› Long-Term Dynamical Evolution and Ejection of Near-Earth Asteroids
› Potential of Gaia XP Spectra in Red Giant Star Asteroseismology: A Deep-Learning Approach
› A Radio Changing-state Jet in the Narrow-line Seyfert 1 Galaxy J1105+1452
› Dark ages bounds on non-accreting massive compact halo objects
› Simple approximations of some statistical functions
› Strong MHD Turbulence and Coherent Structures as Drivers of Cosmic Particle Acceleration
› Signatures of Suppressed Matter Clustering revealed by Fast Radio Bursts
› The Changing-look Phenomenon Accompanied by an Accretion Mode Transition in NGC 3786
› Suppressed Magnetogenesis from Ultralight Dark Matter due to Finite Conductivity
› Quasi-periodic pulsations and three-dimensional magnetic reconnection during 2022 March 31 flare observed by IRIS & STIX
› Probing Red Giant Interiors with G-Dominated Mixed Modes I: The Cases of KIC 9145955, KIC 9970396, KIC 9882316 and KIC 11968334
› VASCO: A fully automated CASA pipeline for large volume VLBI data calibration
› Comparison of Effective Dissipation Channels in Warm Higgs Inflation from Warm Background Evolution
› Kardashev's Conundrum: Statistical Falsification of the Standard Kardashev Model and the Kardashev--Sagan--Nakamoto Resolution
› A Giant Ring on the sky
› Ice as a Photochemical Shield: Adsorption Energetics and Spectroscopic Modulation of Interstellar Thiocyanates HCSCN and HCSCCH in TMC-1
› Characterizing Earth analogs may require a moderate or high-resolution spectrograph
› Dust-driven streaming instability and magnetic field amplification downstream of supernova remnant shocks
› Turning Galaxy Rotation Curves into Radial Cosmic Chronometers: A Nexus Paradigm Approach
› The Recurrent Nova Population in M31
› Constraining Cosmological and Astrophysical Parameters with the Cosmic Star Formation History
› Spatio-temporal Characteristics of Very Long-periodic Pulsations in Solar Metrewave Bursts: Implications for their Origins
› Testing cosmological isotropy with gravitational waves and gamma-ray bursts
› The Quenching Mechanisms of Field Dwarf Galaxies
› Clock Noise Cancellation in Heterodyne Links between Optical Cavities for Space-Borne Gravitational-Wave Telescopes
› Exploring Polarized Millimeter Emission from Protoplanetary Disks with Irregular Dust Grains
› A scaling relation for core heating by giant impacts and implications for dynamo onset
› The effect of interstellar scattering on coherent radio emission from stars: the case of CU Vir
› Three Subclasses of the Intensity-tracking Pattern in Gamma-Ray Burst Spectral Evolution
› Rotation-induced Relaxation of Supernova Constraints on Axionlike Particles
› Producing High-Resolution Martian Surface Temperature Maps Using VIR-TIR Relationships
› Study on the detector energy response of SVOM/GRM
› Vaulting the barrier: An intrinsic mechanism to fuel the gas beyond the nuclear ring into the central region of barred galaxies
› BEACON: JWST NIRCam Pure-parallel Imaging Survey. III. Constraints on the UV LF and the Clustering of z~7-14 Galaxies
› Efficiently emulating distribution functions in gigaparsec volumes for varying cosmological parameters
› Mapping the CMB with QUBIC spectral imaging
› In-depth analysis of the clustering of dark matter particles around primordial black holes. Part III: CMB constraints
› Superfluid $^3$He aerogel experiments as a laboratory neutron star analogue
› The trigger and localization system of SVOM-GRM
› X-Ray Polarization from the Atoll 4U 1735-44 Suggests a Low Inclination
› A barotropic alternative to Early Dark Energy for alleviating the $H_0$ tension
› Smokescreen: A Python package for data vector blinding and encryption in cosmological analyses
› JWST Exoplanetary Worlds and Elemental Survey (JEWELS) II: Condensation Temperature Trends and Galactic Chemical Evolution in JWST Planet-Hosting Stars
› Do time delay effects explain galactic velocity profiles?
› Equation of State for warm Neutron Star outer crusts
› On the relative CNO underabundance in quasar absorption systems at $z \sim 3$ arising from Population III enrichment and attenuation by intermediate-mass black holes and primordial baryon accretion
› Gravitational Waves from the Cosmic Dawn: Tracing Cosmic Black Hole Binaries with ET, LGWA and LISA
› Latest results from the IceCube Neutrino Observatory
› The Metal Content of Resolved Galaxies
› Understanding the complex morphology of a CME II: how pre-eruptive conditions shape CME evolution
› Galaxy Populations in the IllustrisTNG Caustic Skeleton
› Impact of Cold Jupiter Scattering on the Mean-Motion Resonance of Inner Small Planets
› From Gaia to GaiaNIR: I. Probing dark matter halos in globular clusters
› Rapid and Predictive Planet Population Synthesis Model (RAPPS) I. Upgraded model and resulting synthetic populations
› Characterizing the velocity anisotropy of the Milky Way's stellar halo
› Two Potential Exoplanets around A-type Stars Selected from 18 Planetary Candidates
› Sensitivity of Dry Lava Planet Atmospheric Emission Spectra to Changes in Lava Compositions
› From Gaia to GaiaNIR: II. A new view of the Milky Way bar
› Dust characterization of halos -- The extended emission in protoplanetary disks
› The MeerKAT Fornax Survey VII. Characterisation of the Fornax cluster's magnetic field and new insights on magnetisation in large scale systems
› Probing the 3D Structures of Supernovae through IR Signatures of CO and SiO
› Spectroscopic survey of faint planetary-nebula nuclei. VII. Thirty new hydrogen-deficient central stars
› Fourth-order galaxy-galaxy-lensing: Theoretical framework and direct estimation
› Molecular Clouds at the Edge of the Galaxy II. Physical properties and scaling relations
› Correcting radar meteor fluxes for observing biases
› Active-region Modulation of Subsurface Meridional Flows and Magnetic Flux Transport on the Sun
› NOEMA3D: Resolving radial gas flows in disk galaxies at z~1.1-1.6 with high-resolution CO observations
› NOEMA3D: Spatially resolved dust, CO, and [C I] in massive star-forming main sequence galaxies at cosmic noon
› A Census of Na D-traced neutral ISM and outflows at $0.6
› The T16 Planet Hunt: 10,000 New Planet Candidates from TESS Cycle 1 and the Confirmation of a Hot Jupiter Around TIC 183374187
› If at First You Don't Succeed, Trispectrum: I. Estimating the Matter Power Spectrum Covariance with Higher-Order Statistics
› Effect of gap width on turbulent transition in Taylor-Couette flow
› On-Orbit Space AI: Federated, Multi-Agent, and Collaborative Algorithms for Satellite Constellations
› Baryon Asymmetry from Electroweak-Symmetric Domain Walls
› Investigating the Neutrino Mass Ordering Problem via Ternary Plots
› Morphological Evolution of Higher Order Nonlinear Kinetic Alfv\'en Waves in Structured Galactic Environments
› Automated Classification of Plasma Regions at Mars Using Machine Learning
› Hydrodynamics of Filtered Dark Matter: A Two-Component Approach
› Testing $\alpha$-attractor P-model of inflation by Cosmic Microwave Background radiation
› A short course in general relativity
› A Unified Bogoliubov Approach to Primordial Gravitational Waves: From Inflation to Reheating
› Deterministic Trust Regions for Finite-Window Black-Hole Spectroscopy in GW250114
› Thermodynamic behavior of cosmological models with fractional entropy
› Inferring lunar wake potentials from electron phase space densities
› Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions
› Probing Cosmic-Ray-Boosted and Supernova-Sourced Sub-GeV Dark Matter with Paleo-Detectors
› Looking for Lights from the Darkness: Signals from MeV-scale Solar Axion-like Particles
› Classical and quantum evolution of inflationary fluctuations
› On the curlometer measurement of field-aligned and perpendicular currents in low Earth orbit: Swarm observations and whole geospace simulations
› Assessing observational constraints on dark energy
› Simulations of Interacting Binary Systems -- Pathways to Radio Bright GRB Progenitors
› LavAtmos 2.0: Incorporating Volatiles Species in Vaporization Models
› Non-linear Cosmological Perturbations for Coupled Dark Energy
› Reconstructing the Thermal Sunyaev Zeldovich Power Spectrum from Planck using the ABS Method
› Helium Accumulation and Thermonuclear Instabilities on Accreting White Dwarfs: From Recurring Helium Novae to Type Ia Supernovae
› Ram-Pressure Stripping Caught in Action in a Forming Cluster at z $\sim$ 2.5
› An Alternative Hubble parameter: Explaining DESI data and High redshift Supermassive Black Hole
› Thermochemical models of outer core convection with heterogeneous core-mantle boundary heat flux
› The role of three-dimensional effects on ion injection and acceleration in perpendicular shocks
› GW231123 Formation from Population III Stars: Isolated Binary Evolution
› DESI Strong Lens Foundry III: Keck Spectroscopy for Strong Lenses Discovered Using Residual Neural Networks
› Detection of HI filament: Pair Stacking vs. Filament Stacking
› Technique-agnostic exoplanet demography for the Roman era -- I. Testing a demography retrieval framework using simulated Kepler-like transit datasets
› Expectations for the first supermassive black-hole binary resolved by PTAs II: Milestones for binary characterization
› Expectations for the first supermassive black-hole binary resolved by PTAs I: Model efficacy
› Probing departures from $\Lambda$CDM by late-time datasets
› Cavendish experiment with fast radio bursts on cosmological scales
› Singular Value-based Atmospheric Tomography with Fourier Domain Regularization (SAFR)
› Observation of In-ice Askaryan Radiation from High-Energy Cosmic Rays
› Evidence of dynamical dark energy found via the DESI DR2 Lyman$\alpha$ forest
› Towards Reconciling Reionization with JWST: The Role of Bright Galaxies and Strong Feedback
› Probing the origin of the kilonova candidate GRB 230307A: analysis of host galaxy and offset
› A Comprehensive Sulfur Chemistry Network Including Excited S(1D) and SO(1{\Delta}) for the XODIAC Photochemical Model: Accounting for Missing Sulfur Processes in Venus and Exo-Venus Analogs
› MUSE Analysis of Gas around Galaxies (MAGG) -- VII. Emission line galaxies near strong blended Ly$\alpha$ absorption systems at $z\gtrsim3$
› Probing the sensitivity of dark energy dynamics to equation of state parametrization flexibility
› Thawing Quintessence: Priors, evidence, and likely trajectories
› Isotropic stochastic gravitational wave background reconstruction for Taiji constellation
› The Emission and Suppression of Line Features in Luminous Transients
› Predictability of bursts of a recurrent nova using topological data analysis and machine learning
› Classical Be Stars and Classical Be Star Binaries from LAMOST DR12
› TeV Gamma-Rays from the Low-Luminosity Active Galactic Nucleus NGC 4278: Implications for the Diffuse Neutrino Background
› SED and Galactic kinematic diagnostics for dormant BH/NS binary candidates
› The Bondi universe: Can negative mass drive the cosmological expansion?
› Nested Fermi and eROSITA bubbles require very similar $\sim10^{56}$ erg collimated Galactic-center outbursts; their asymmetry indicates an eastern density gradient
› An Exploration of the Equation of State Dependence of Core-Collapse Supernova Explosion Outcomes and Signatures
› New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method
› Exploring the magnetic field of the ultraluminous X-ray pulsar NGC 4631 X-8
› Planet formation at the inner edge of the dead zone -- I. the interplay between accretion outbursts and dust growth
› Direct VLBI Detection of Interstellar Turbulence Imprint on a Quasar: TXS 2005+403
› Terraforming Mars: Mass, Forcing, and Industrial Throughput Constraints
› The Intrinsic Multiplicity Distribution of Exoplanets Revealed from the Radial Velocity Method. II. Constraints on Giant Planet Multiplicity from Different Surveys
› Low-energy atmospheric neutrino flux calculation with accelerator-data-driven tuning
› Interstellar Object 3I/ATLAS Observed from Mars by China's Tianwen-1 Spacecraft
› Detection of a weak magnetic field in the Balmer emission line white dwarf WDJ1653-1001
› Blackbody Quasar and Radio Source (BBQSORS): A Candidate of Transitional Little Red Dots with a $T\sim10^4\ K$ Blackbody Spectrum
› FAST Polarization Catalog of FRB 20240114A
› Resizing the giants: How modelling adiabatic interiors impacts predicted planetary radii
› Constraining Lyman-Werner Feedback from Velocity Acoustic Oscillations in the Cosmic Dawn 21 cm Signal
› Secular Light Curve of Exocomet 3I/ATLAS, and its Location on a Comet Evolutionary Diagram
› A consistent MOND modelling of the Bullet Cluster
› No country for old stars -Spectroscopic confirmation of the first intermediate-age RR Lyrae in the open cluster Trumpler 5
› Requiem for a belt: A spatial and kinematical reinterpretation of Gould's Belt in light of Gaia
› BROOM: a python package for model-independent analysis of microwave astronomical data
› Age bimodality in pseudo-bulges of barred spiral galaxies: Bar-driven evolution across cosmic time
› The Neptunian ridge as a natural outcome of high-eccentricity tidal migration
› Statistical properties of the gravitational force through ordering statistics
› Theoretical and observational constraints on early dark energy in $F(R)$ gravity
› Axion Star Bosenova in Axion Miniclusters
› Extending the Dynamical Systems Toolkit: Coupled Fields in Multiscalar Dark Energy
› Scalaron dark matter dynamics: effects of Higgs non-minimal coupling to gravity
› A Unified Dark-Matter--Driven Relativistic Bondi Route to Black-Hole Growth from Stellar to Supermassive Scales
› Auto-encoder model for faster generation of effective one-body gravitational waveform approximations
› Sub-threshold post-merger gravitational waves can constrain the hot nuclear equation of state
› Creation of spin-3/2 dark matter via cosmological gravitational particle production
› The First Model-Independent Upper Bound on Micro-lensing Signature of the Highest Mass Binary Black Hole Event GW231123
› Spec-o3: A Tool-Augmented Vision-Language Agent for Rare Celestial Object Candidate Vetting via Automated Spectral Inspection
› Photon Propagation through Magnetar-Hosted Axion Clouds: Time Delays and Polarimetric Constraint

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