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RSS  Latest preprints on astro-ph:

› Calibration-independent consistency test of BAO and SNIa data: update
› Evolutions of mean distance ratios in the planetary and satellite systems under primary tides and nebular gas drag effects
› Comprehensive Gaia DR3-Based Astrometric, Photometric, and Kinematic Studies of the Binary Open Cluster $h$ and $\chi$ Persei
› Accretion Rate Changes Detected in a Polluted White Dwarf
› Assessing the Vera Rubin Observatory's Ability to Discover Asteroid Impactors Before They Collide with Earth
› A shot in the dark: searching for dark substructures in the RX J0437+00 galaxy cluster
› TORRCH: Tomographic reconstruction of the reionization of cosmic hydrogen with Ly${\alpha}$ emitters and non-Ly${\alpha}$-selected galaxies
› A Binary-Based Reassessment of the Age and Stellar Properties of NGC 7789 Using Twelve Binary Components
› Measuring the Black Hole and Accretion Parameters of Sagittarius A* from EHT Observations using a Semi-Analytic Model
› proto-Lightspeed: a high-speed, ultra-low read noise imager on the Magellan Clay Telescope
› Relaxing DESI DR2 BAO Constraints on $\sum m_\nu$ with Planck and SPT-3G 2018 in the Context of SPT D1
› A first GLIMPSE into star clusters populations across cosmic time
› UNCOVER/MegaScience Finds Uniform and Highly Bursty Star Formation at 3 < z < 9, consistent with the High-Redshift UV Luminosity Function
› MeerKAT observations of Abell 1775 and Abell 1795: the discovery of a hadronic radio halo?
› A differential-geometry approach to black hole characterization of megamaser systems in static spherically symmetric spacetimes
› The detectability of bars at high redshift: a case study using Euclid-like mock observations of TNG50 simulated galaxies
› Unifying cluster and galaxy cosmology analyses using the galaxy-halo connection
› TOI-6692b: An eccentric 130 day period giant planet with a single transit from TESS
› Hot, Retrograde Tilted MADs: Misaligned, Precessing, and Shaped by Electromagnetic Torques
› Characterization of the commercial spectrograph system for astronomical observations: PIXIS 1300BX Camera and IsoPlane 320A Spectrograph
› XMM-Newton observations of ten high-redshift CAMIRA clusters of galaxies
› Bondi-Hoyle-Lyttleton accretion flow in a stratified layer
› Unveiling a Thin Filament of the Cosmic Web in the Ursa Major Supergroup
› Star formation outside galaxies undergoing gravitational and hydrodynamic interactions: dust attenuation and the star formation rate
› Constraints on the Hot Circumgalactic Medium around Nearby L* Galaxies from SRG/eROSITA All Sky Survey
› On the Use of Field RR Lyrae as Galactic Probes -- VIII. Early Formation of the Galactic Spheroid
› Multi-wavelength Study of A Superflare on RS CVn-type Star HD22468 Triggered at Hard X-ray by SVOM
› Simulations of multi-phase gas in and around galaxies
› GRBAlpha, VZLUSAT-2 and GRBBeta -- GRB observations with CubeSats
› Cosmological analysis of a viable $f(R)$ gravity model
› Investigating Twin Star Equation of States in Light of Recent Astrophysical Observations
› ALMA publication statistics
› One H2 molecule per ten million H-atoms reveals sub-pc scale cold overdensities at z~4
› Pushchino Multibeam Pulsar Search. X. Observations of pulsars at declinations above $+53^o$
› When Primordial Black Holes Absorb During the Early Universe
› Illuminating the Physics of Cosmic Origin and Evolution: A UK Space Frontiers 2035 White Paper
› Improved measurements of the age of JWST galaxies at z=6-10
› [HP99] 159 -- Properties of the first Supersoft X-ray Source with a Helium star donor
› Mercury-Ar$\chi$es: a high-performance n-body code for planet formation studies
› Superhumps in active dwarf novae. Part I: ER Ursae Majoris
› Magnetic threads and gravity: ALMA Observations of IRDC G14.225-0.506
› Flux-ratio anomalies in cusp quasars reveal dark matter beyond CDM
› Gaia20dsk: A new MNor discovered by the GLORIOUS collaboration
› Six New Circumbinary Disk Occultation (CBO) Candidates from the Zwicky Transient Facility
› Kinematics of young star clusters in the outer north-eastern region of the Small Magellanic Cloud
› The Astrosky Ecosystem: An independent online platform for science communication and social networking
› The Origins of Planets for ArieL (OPAL) Key Science Project: the end-to-end planet formation campaign for the ESA space mission Ariel
› Cosmography with $\Lambda$-Szekeres Models
› Extragalactic Planetary Nebulae (xPNe). Determining Distances out to 100 Mpc and the Renaissance of the PN Luminosity Function Method
› A more inclusive effective dark fluid equation of state parameter: constraints from SKA and Euclid like surveys
› Dynamics of AGN feedback in the X-ray bright East and Southwest arms of M87, mapped by XRISM
› Drawing the line between explosion and collapse in electron-capture supernovae -- I. Impact of conductive flame speeds and ignition conditions on the explosion mechanism
› CosmoSlider: An educational tool for cosmology
› Fast Magnetoacoustic Wave Behavior with Gravitationally Stratified, Magnetically Inhomogeneous Media
› The shape function of the observed growth index
› The scaling relations of galaxies with different morphology: comparison among WINGS, MANGA and Illustris data samples
› Forecast on the generalised dark matter properties from a Euclid-like survey
› Improving constraints on primordial non-Gaussianity from Quaia with a new cosmological observable: angular redshift fluctuations
› Probabilistic Graphical Models in Astronomy
› Calibrating redshift distributions at $z>2$ with Lyman-$\alpha$ forest cross-correlations
› ReveaLLAGN 1: JWST Emission-Line Spectra Reveal Low-Luminosity AGN with UV-Deficient SEDs and Warm Molecular Gas
› Post-Perihelion Integral Field Spectroscopy of the Interstellar Comet 3I/ATLAS
› A compact object with a K type star companion in the solar neighborhood: a wide post common envelope binary with a white dwarf candidate
› Probing dark matter interactions with a RES-NOVA prototype cryogenic detector
› Searching for Ultralight Scalar Dark Matter with Clocks in Low Earth Orbit
› Analysis of $M1$ capture in the $\alpha(d,\gamma)^6$Li reaction
› Thick Lunar Crust Amplifies Gravitational-Wave Signal
› Universal relation between dipole polarizability of finite nuclei and neutron-star compactness
› Cosmic ray electron boosted light dark matter: Implications of LZ 2025 data
› Anisotropy Strikes Back: Modified Gravity and Dark Matter Halos
› Science Opportunities of Wet Extreme Mass-Ratio Inspirals
› The 2.5-meter Wide Field Survey Telescope Real-time Data Processing Pipeline I: From raw data to alert distribution
› Precision Determination of Scintillation Screen Parameters from Annual Modulation Measurement of Pulsar Scintillation Arc Curvature with the FAST Telescope
› Inflationary attractors and radiative corrections in light of ACT data
› Multiplicity of young isolated planetary mass objects in Taurus and Upper Scorpius
› Eternal inflation near inflection points: a challenge to primordial black hole models
› The role of migration traps in the formation of binary black holes in AGN disks
› Cosmological Constraints on Neutrino Masses in a Second-Order CPL Dark Energy Model
› 21 cm forest one-dimensional power spectrum as an indirect probe of dark matter particles and primordial black holes
› Orbit-based structural decomposition and stellar population recovery for edge-on barred galaxies
› Probing Stellar Kinematics with the Time-Asymmetric Hanbury Brown and Twiss Effect
› StarEmbed: Benchmarking Time Series Foundation Models on Astronomical Observations of Variable Stars
› SCATTER Common Envelope Formalism for Triples
› Euclid preparation: LXXXVII. Non-Gaussianity of 2-point statistics likelihood: Precise analysis of the matter power spectrum distribution
› Photon rest mass from localized fast radio bursts with improved distribution of dispersion measure from extragalactic gas
› JWST Confirmation of a Runaway Supermassive Black Hole via its Supersonic Bow Shock
› Machine Learning vs. Spectral Energy Distribution Fitting: A Comparative Analysis of Accuracy in Stellar Mass Estimation
› Sustainable, Local Socio-Economic Development Through Astronomy
› Captured are circularized: A relativistic treatment of extreme mass ratio inspirals crossing accretion disks
› The Characteristic Mass and Energy Conversion Efficiency in the Cusp-Core Transition of Dark Matter Haloes: Implications for Scaling Relations and Supernova feedbacks
› One Attempt at Building an Inclusive & Accessible Hybrid Astronomy Conference: FRB 2025
› The FarView Low Frequency Radio Array on the Moon's Far Side: Science and Array Architecture
› Slow and fast collective neutrino oscillations: Invariants and reciprocity
› A Model of Dark Matter and Energy
› GALILEO: Galactic Axion Laser Interferometer Leveraging Electro-Optics
› LISA double white dwarf binaries as Galactic accelerometers
› Estimating Soil Electrical Parameters in the Canadian High Arctic from Impedance Measurements of the MIST Antenna Above the Surface
› Density perturbations in nonminimally coupled gravity: symptoms of Lagrangian density ambiguity
› K-nonizing
› Effects of dynamical capture on two equal-mass nonspinning black holes
› Potential divergence in tracing $\mu$ and $\tau$ flavors of astrophysical neutrinos
› Taxonomy of periodic orbits and gravitational waves in a deformed Schwarzschild black hole spacetime
› GlueNN: gluing patchwise analytic solutions with neural networks
› Exact general solutions for cosmological scalar field evolution in a vacuum-energy dominated expansion

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