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RSS  Latest preprints on astro-ph:

› A Correlation Between Black Hole Mass and Dark Matter Halo Concentration in Cosmological Simulations
› CoBiTS: Single-detector discrimination of binary black hole signals from glitches using deep learning
› Bridging stellar evolution and planet formation: from birth, to survivors of the fittest, to the second generation of planets
› Diffusive or Ballistic? Distributions and Spectra of PeV Cosmic Rays around Microquasars
› Pulsational Instability of Quasi-Stars: Interpreting the Variability of Little Red Dots
› First-Principles Formalism for Simulating Self-Interacting Dark Matter
› The Clustering of Little Red Dots from Ultra-Strongly Self-Interacting Dark Matter
› Time-resolved X-ray spectra of Proxima Centauri as seen by XMM-Newton
› Widespread Shocks in an Odd Radio Circle Host Galaxy
› Monitoring and Evaluating Astronomy-for-Development Initiatives
› Characterization of telecentric dual-etalon Fabry-P\'erot systems from observational data. Properties of the CRISP2 instrument at the Swedish 1-m Solar Telescope
› Constrained Brownian-bridge prior for neutron-star equation-of-state inference
› Designing the Community Infrastructure for ESO's Next Transformational Facility. Equitable Governance and Sustainable Teams for 2040s Astronomy
› Precision Spectroscopy for 1.9 Million Galaxies from SDSS-IV: Improved Spectral Measurements and Catalogs for eBOSS
› A recurrent 70-100 minute quasi-periodic pulsation in the intermediate-aged mid-M dwarf GJ 3512
› The rotation-magnetism relationship in solar-type stars. Constraining magnetic flux emergence rates
› The Impact of the MAST Data Archive
› Double Hot Jupiter Formation through Mirrored ZLK Migration in Binary Star Systems: The Case of WASP-94
› A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array
› Continuous Wide-Field Optical Monitoring for Very Early-Phase Transient Discovery
› Red noise-based false alarm thresholds for astrophysical periodograms via Whittle's approximation to the likelihood
› Unlocking the physics of dwarf galaxies in the 2040s: The case for a next-generation wide-field spectroscopic facility with fibres and IFUs
› Discovery of a Luminosity-dependent Continuum Lag in NGC 4151 from Photometric and Spectroscopic Continuum Reverberation Mapping
› Measurements of quasar proximity zones with the Lyman-$\alpha$ forest of DESI Y1 quasars
› Robust and scalable simulation-based inference for gravitational wave signals with gaps
› On Lorentz Variability of Magnetically Dominated Relativistic Outflows
› The size of 3I/ATLAS from non-gravitational acceleration
› Standard Sirens in 2040s: Probing the Cosmic Expansion History with Gravitational Waves and Spectroscopic Galaxy Surveys
› Energy-Dependent Shifts of Medium-Scale Anisotropies in Very-High-Energy Cosmic Rays Observed by LHAASO-KM2A
› The evolution of obscured AGN across cosmic time -- A large quasar survey for the 2040s
› Unveiling Long-Period Variables in M33's Central Region: Insights into Stellar Evolution and Star Formation via Near-Infrared Photometry
› Imaging the LkCa 15 system in polarimetry and total intensity without self-subtraction artefacts
› Observed Low-Plasma-$\beta$ Temperature Anisotropy Constraint Driven by $\alpha$-Particle Drift
› Searches for Prompt Low-Frequency Radio Counterparts to Gravitational Wave Event S250206dm with the OVRO-LWA Time Machine
› Harmony of the Spheres: Extension to All Points of an Algorithm for Producing a Density Field with Given Two-, Three-, and Four-Point Correlation Functions
› Detecting stellar flares in the presence of a deterministic trend and stochastic volatility
› Formation of Be stars via wind accretion: Case study on Black hole + Be star binaries
› The Extended Baryonic Tully-Fisher Relation for MaNGA Galaxies
› Linear Analyses of Thermal Instability in Stratified Medium
› Solar jet-induced perturbation propagating through coronal loops and in-loop electron beam transport indicated by type II and type N radio bursts
› Photospheric horizontal magnetic field decrease preceding a major solar eruption
› Towards Understanding the Milky Way's Matter Field and Dynamical Accretion History based on AI-GS3 Hunter
› Towards Unveiling the Origins of the Milky Way Bulge through Multi-band-Messenger Sky Surveys
› Addendum to "Cygnus~X-3 as a semi-hidden PeVatron'' discussing the LHAASO 2025 data
› Recurrence plot analysis of blazar gamma-ray light curves: Exploiting the time-domain capabilities of Fermi-LAT
› Spider-Webb: Spatially-Resolved Evidence of Inside-Out Quenching in the Spiderweb Protocluster at $z \sim 2$
› Nanohertz Gravitational Waves
› Accretion geometry in neutron star low-mass X-ray binaries during the hard spectral state
› Detecting false positives with PLATO using double-aperture photometry and centroid shifts
› Orbital classification in rotating bar potentials using an empirical proxy of the second integral of motion
› Solar Vortex Detection With Velocity Field Normalisation: Eliminating False Positives
› Constraints on the polarization angle oscillations of the Crab Nebula with the Simons Array and its applications to the search for axion-like particles
› EuroHPC SPACE CoE: Redesigning Scalable Parallel Astrophysical Codes for Exascale
› Optical SETI at ESO in the 2040s
› Weak Lensing Mass Calibration of the ACT DR5 Galaxy Clusters with the DES Year 3 Weak Lensing Data
› Validating the CROCODILE model within the AGORA galaxy simulation framework
› Fragmenting Filaments and Evolving Cores -- Insights from Dust Polarisation Study of a filament in Northern Orion B
› $\Omega_1\Omega_2$-$\Lambda$CDM: A promising natural extension of the standard model of cosmology
› On the Diversity of Pulsar's Frequency-Dependent Circular Polarization
› The Milky Way Bulge Extra-Tidal Star Survey: NGC 6569
› Physical Conditions for Synthesis of Sc, Ti, and V in Neutrino-driven Supernovae
› The Simons Observatory: Detector Polarization Angle Calibration using Sparse Wire Grid with Initial Data Sets of the Small Aperture Telescope
› GW231123: A Case for Binary Microlensing in a Strong Lensing Field
› Height and Energy Evolution of X-ray Double Sources in a Solar Flare
› DESI DR2 Constraints on the $R_h=ct$ Universe: Model Viability and Comparison with $\Lambda$CDM
› Raman Spectroscopy of Salt Deposits from the Simulated Subsurface Ocean of Enceladus
› ALMA Observations of Cold Methanol Gas in the Large Magellanic Cloud (LMC): N79 South GMC
› Illuminating the Dark Sector: Understanding Modified Gravity Signatures with Cross-Correlations of Gravitational Waves and Large-Scale Structure
› The IXPE and multifrequency polarimetric view of the extreme blazars 1ES 1101-232 and RGB J0710+591
› Enhanced Non-Thermal Line Broadening inside Coronal Cavities above Solar Prominences revealed by Spectral Imaging CoronaGraph
› Outburst Characteristics of Transient Low Mass X-ray Binary 4U 1608-52
› Multi-wavelength study of the pre-eruption dip in the recurrent nova T Coronae Borealis preceding imminent nova eruption
› Orbital Stability of Moons Around the TRAPPIST-1 Planets
› Disentangling the hemispheres of Teegarden's Star b with LIFE
› Identifying Quasi-Periodic Micropulses in Pulsars with FAST Using Convolutional Neural Networks
› Dynamically close galaxy pairs from the unWISE survey: Testing the merger-AGN-star formation connection
› Towards DM-free search for Fast Radio Bursts with Machine Learning -- I. An implementation on multibeam data
› Sensitivity of CTAO to axion-like particles from blazars: a machine learning approach
› Observations of the 21 cm HI Line from the Milky Way galaxy using Pyramidal Horn Radio Telescope
› Search for Axion-Like Particles from Nearby Pre-Supernova Stars
› Optical Follow-Up Strategies for the Next Neutrino-Detected Galactic Core-Collapse Supernova
› Galaxy And Mass Assembly (GAMA): Deconstructing the galaxy stellar mass function by star formation and environment
› Machine learning for the early classification of broad-lined Ic supernovae
› Diagnosing the AGN population origin of TeV neutrinos with their spatial correlation
› Dynamics of clusters of galaxies in the presence of dark energy: Virgo cluster
› GALATEA: The 15-m Galactic Archaeology Spectroscopic Surveyor
› Confining nonlinear electrodynamics black holes: from thermodynamic phases to high-frequency phenomena with accretion process
› Revealing the intricacies of radio galaxies and filaments in the merging galaxy cluster Abell 2255. II. Properties of filaments using multi-frequency radio data
› Low-redshift 3D Lyman-{\alpha} Forest Correlations with China Space Station Telescope
› Strong model-agnostic constraints for twin-star solutions
› Predicting coronal mass ejection travel times using enhanced model-guided machine learning
› Shock-induced magnetic reconnection driving Ellerman bomb emission and a spicule
› Do low-redshift observations open the doors to an open universe?
› Deep Learning for Primordial $B$-mode Extraction
› Non-local-in-time structure formation and sixth-order galaxy bias
› Impact of Galaxy Cluster Environment on the Stellar Mass Function of Galaxies
› Period Change of the Binary System WR+O V444 Cyg: Updated Ephemeris Formula
› Deep H{\alpha} survey of the Coma cluster: The Catalog
› InterACTing dark radiation models after ACT
› High-Precision Differential Radial Velocities of C3PO Wide Binaries: A Test of Modified Newtonian Dynamics (MOND)
› A High-Resolution NUV Transmission Spectrum of KELT-9b: Mg II and Fe II Escaping from the Hottest Known Giant Planet
› A cosmologist's take on Little Red Dots
› Are Primordial Black Holes Truly Fine-Tuned?
› Ionizing Photon Production Efficiencies and Chemical Abundances at Cosmic Dawn Revealed by Ultra-Deep Rest-Frame Optical Spectroscopy of JADES-GS-z14-0
› Magnetically supramassive and hypermassive compact stars
› Effects of helium sedimentation on late star formation in galaxy clusters
› Constraints on gravitational waves from the 2024 Vela pulsar glitch
› New Multi-messenger Probe of Dark Matter-Nucleon Interactions from Ultra-high Energy Cosmic Ray Acceleration
› Superfluid fraction in the crystal phase of the inner crust of neutron stars
› Revisiting Mars' Induced Magnetic Field and Clock Angle Departures under Real-Time Upstream Solar Wind Conditions
› A Framework for Lorentz-Dirac Dynamics and Post-Newtonian Interaction of Radiating Point Charges
› Traversable wormholes inside anisotropic magnetized neutron stars: physical properties and potential observational imprints
› Energetically-dominant Sunward-Propagating Alfv\'en Waves Near 1 au and Their Relation to Large-scale Magnetic Switchbacks
› Optical appearance, Hawking radiation, and Barrow thermodynamics of Letelier black hole in electromagnetic universe
› Scalar-Mediated Inelastic Dark Matter as a Solution to Small-Scale Structure Anomalies
› Gravitational Production of Massive Spin-2 Particles During Reheating
› Bose-Einstein Condensate dark matter with logarithmic nonlinearity
› The First Model-Independent Upper Bound on Micro-lensing Signature of the Highest Mass Binary Black Hole Event GW231123
› Ultra-high precision high voltage system for PTOLEMY
› Parameter estimation for the GWTC-4.0 catalog with phenomenological waveform models that include orbital eccentricity and an updated description of spin precession
› The tidal gap: causality bound on exotic compact objects with applications in the solar and sub-solar mass range
› Neutron star crust and outer core equation of state from chiral effective field theory with quantified uncertainties
› Probing Dark Sectors with Exploding Black Holes: Gamma Rays
› The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and its Implications for Structure Growth
› Hint of dark matter-dark energy interaction in DESI DR2 and current cosmological dataset?
› ContEvol formalism: numerical methods based on Hermite spline optimization
› Time Non-locality in Dark Matter and LSS
› Modeling and measuring the anisotropic halo 3-point correlation function: a coordinated study
› Constraining primordial black hole abundance with Insight-HXMT
› On the Role of Chapman's Hydrostatic Solar Wind Mechanism in Parker's Hydrodynamic Solar Wind Model
› Stellar Stripping and Disruption in Disks around Supermassive Black Hole Binaries: Repeating nuclear transients prior to LISA events
› Cosmological search for sterile neutrinos after DESI 2024
› The Ultraviolet Type Ia Supernova CubeSat (UVIa): Science Motivation & Mission Concept
› Multi-copy Axion Transfer Function and Observational Implications of Effective de Broglie Scales
› Periodicities in radio emissions from the Jupiter's magnetosphere and consequences for radio emissions from star-exoplanet systems
› Interacting dark energy after DESI DR2: a challenge for $\Lambda$CDM paradigm?
› Challenges in the detection of gases in exoplanet atmospheres
› A Detailed Investigation of HD 209458 b HST & JWST Transmission Spectra with SANSAR
› The ambiguous AT2022rze: Changing-look AGN mimicking a supernova in a merging galaxy system
› Accurate and efficient likelihood modeling for large-scale CMB data
› TDCOSMO 2025: Cosmological constraints from strong lensing time delays
› Indicator Functions: Distilling the Information from Gaussian Random Fields
› The link between galaxy merger, radio jet expansion and molecular outflow in the ULIRG IRAS 00183-7111
› An Enhanced Thermodynamic Framework for Third-Order Galaxy Correlation Functions: A Physically Motivated Closure and Observational Test
› Measuring black hole spins with x-ray reflection spectroscopy: A GRMHD outlook
› On the statistical convergence of N-body simulations of the Solar System
› Effects of Lorentz invariance violation on charged particles and photon production in astrophysical sources
› Reconnection-driven Flares in M87*: Proton-Synchrotron-powered GeV Emission
› Equation vs. AI: Predict Density and Measure Width of molecular clouds by Multiscale Decomposition
› SPAN: A cross-platform Python GUI software for optical and near-infrared spectral analysis
› Mitigating incoherent excess variance in high-redshift 21 cm observations with multi-output cross-Gaussian process regression
› A comprehensive spectroscopic reference of the solar system and its application to exoplanet direct imaging
› Blade Antenna-SDR System Prototype for the CANTAR Global 21-cm Experiment: Simulations, Measurements, and In-Situ Results
› Modeling spectral filtering effects on color-matching functions: Implications for observer variability
› Mysteries of Capotauro: investigating the puzzling nature of an extreme F356W-dropout
› Active galactic nuclei-heated dust revealed in "little red dots"
› Hurst Index of Gamma-Ray Burst Light Curves and Its Statistical Study
› Predicting stellar collision outcomes of main sequence stars
› MCI: Multi-Channel Imager on the Chinese Space Station Survey Telescope
› Exponential quintessence with momentum coupling to dark matter
› Echoes from the dark: Galaxy catalog incompleteness in standard siren cosmology
› Ultra-long Gamma-ray Bursts from Micro-Tidal Disruption Events: The Case of GRB 250702B
› The Colors of Ices: Measuring ice column density through photometry
› The very faint X-ray transient Swift J174610-290018 at the Galactic center
› On the statistical characterization of the synchrotron multi-zone polarization of blazars
› Transverse Velocities in Real-Time Cosmology: Position Drift in Relativistic N-Body Simulations
› Is Dark Energy Changing? Probing the Universe's Expansion with present and future astronomical probes
› TOI-3288 b and TOI-4666 b: two gas giants transiting low-mass stars characterised by NIRPS
› Formation of protostars and the launching of stellar core outflows with moving-mesh radiation non-ideal magnetohydrodynamics
› Polarization based direction of arrival estimation using a radio interferometric array
› The Lensing Counter Narrative: An Effective Description of Small-Scale Clustering in Weak Lensing Power Spectra
› Mitigating Nonlinear Systematics in Weak Lensing Surveys II: Stability and Diagnostics with Intrinsic Alignment
› Unified Kraft Break at ~6500 K: A Newly Identified Single-Star Obliquity Transition Matches the Classical Rotation Break
› Validation of optical pathlength stability in a LISA test-bench demonstrator
› JWST Exoplanetary Worlds and Elemental Survey (JEWELS) I: High-Precision Chemical Abundances of 20 FGK Planet-Hosting Stars from JWST Cycle 2
› Spectroscopic characterization of a remarkable temporally varying, triple-lensed quasar at z=2.67
› GLIMPSE-D: An Exotic Balmer-Jump Object at z=6.20? Revisiting Photometric Selection and the Cosmic Abundance of Pop III Galaxies
› DESI-DR1 $3 \times 2$-pt analysis: consistent cosmology across weak lensing surveys
› The Power of DESI for Photometric Redshift Calibration: A Case Study with KiDS-1000
› Understanding the Neutron Star Population with the SKAO telescopes
› Hydrodynamic Evolution and Detectability of Nova Remnants in the Galactic Center
› The contribution from small scales on two-point shear analysis: comparison between power spectrum and correlation function
› Observations of AGN-driven feedback: dynamics and ionization of the filaments in M87
› Boosted dark matter from primordial black holes produced in a first-order phase transition
› The effect of split endcaps on the flow dynamics in a tall Taylor-Couette setup
› Sound waves from primordial black hole formations
› The Possibility of Formation of Compact Boson Stars via Cosmological Evolution of a Background Scalar Field
› Revisiting Isocurvature Bounds on the Minimal QCD Axion
› Boosted dark matter versus dark matter-induced neutrinos from single and stacked blazars
› Dark wounds on icy moons: Ganymede's subsurface ocean as a dark matter detector
› Eccentricity signatures in LIGO-Virgo-KAGRA's BNS and NSBH binaries
› Observing Double White Dwarfs with the Lunar GW Antenna
› Electron Inertia and Magnetic Reconnection
› Streamlined Supergravity
› The meaning of "Big Bang"
› Can the 3 neutrino masses really be found using SN 1987A data?
› Quantum Walks and Exact RG in de Sitter Space
› Delayed Scaling of Multi-Type Cosmic F- and D-strings in VOS Models

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