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RSS  Latest preprints on astro-ph:

› How Dark is Dark Energy? A Lightcones Comparison Approach
› COSMOS-3D: Two obscured X-ray AGNs with hot dust and He I$\lambda$10830 absorption at z~3
› Photon (Non)Conservation in the Reduced Speed of Light Approximation and How to (Almost) Fix It
› The DREAMS Project: Disentangling the Impact of Halo-to-Halo Variance and Baryonic Feedback on Milky Way Satellite Galaxies
› Discovery of two little red dots transitioning into quasars
› Possible $\nu$ Source Class: 3-sigma Detection of High-Energy Neutrinos from Supermassive Black Hole Binary Candidates
› JCMT Constraints on the Early-Time HCN and CO Emission and HCN Temporal Evolution of 3I/ATLAS
› The Dependence of Earth Milankovitch Cycles on Martian Mass
› Cosmic chronometers with galaxy clusters: a new avenue for multi-probe cosmology
› Slow-Light Effect in the Jet-Launching Region of M87
› Image simulations of highly magnified clumpy galaxies
› Determining the Milky Way gravitational potential without selection functions
› Hidden in Plain Sight II: Characterizing the luminous companion to Kappa Velorum with VLTI/GRAVITY
› VENUS: When Red meets Blue -- A multiply imaged Little Red Dot with an apparent blue companion behind the galaxy cluster Abell 383
› SEAMLESS Survey: Four Faint Dwarf Galaxies Tracing Low-Mass Galaxy Evolution Across Environments
› Untangling the Sources of Abundance Dispersion in Low-metallicity Stars II: Neutron Capture Elements
› Kinematics of young stellar objects in NGC 2024 based on infrared proper motions
› A value-added catalogue of neural network-based europium abundances for GALAH DR4
› OASIS Survey Direct Imaging and Astrometric Discovery of HIP 71618 B: A Substellar Companion Suitable for the Roman Coronagraph Technology Demonstration
› Ripples in the baryon to dark matter ratio in $\Lambda$CDM: implications for galaxy formation
› Dynamo and Jet interconnections in GRMHD simulations of black hole accretion disks
› Constraining the Occurrence of ZLK-Induced White Dwarf Pollution with Dissipative Precession
› AT2022zod: An Unusual Tidal Disruption Event in an Elliptical Galaxy at Redshift 0.11
› Inefficient Circularization, Delayed Stream-Disk Interaction and Reprocessing: A Five-Stage Model for the Intermediate-Mass Black Hole Tidal Disruption Event EP240222a
› SCExAO/CHARIS and Gaia Direct Imaging and Astrometric Discovery of a Superjovian Planet 3--4 lambda/D from the Accelerating Star HIP 54515
› Impact of Nuclear Reaction Rate Uncertainties on Type I X-ray Burst Nucleosynthesis: A Monte Carlo Study
› High-Energy Extractions from Horizonless Compact Objects
› Dynamics of Streamers and Pseudostreamers and Implications for the Solar Wind
› $S^5$: Tidal Disruption in Crater 2 and Formation of Diffuse Dwarf Galaxies in the Local Group
› Convective Heat Transport Asymptotic Law in an $\alpha^2$ dynamo model
› Evolution of the Accretion Rate of Young Intermediate Mass Stars: Implications for Disk Evolution and Planet Formation
› Evaluating the Prospects of Cyclic Deconvolution across 312 Pulsars
› The SPHINX M dwarf Spectral Grid. II. New Model Atmospheres and Spectra to Derive Fundamental Properties of mid-to-late type M-dwarfs
› Solitary Alfv\'en Waves
› Driving mechanisms of solar active region geysers: The role of interacting magnetic flux
› Observing binary neutron star subpopulations with the Einstein Telescope
› How much gas and dust is in the $z=5.7$ Lyman Break Galaxy HZ10? An ALMA Band 10 to 4 and JWST/NIRSpec study of its interstellar medium
› Segmented-Polynomial-fitting Least Squares (SPLS): An optimized algorithm to find Earth twins
› Pad\'e Approximants for Fast Radio Bursts Diffuse Dispersion Measure
› The first extragalactic ultra-compact X-ray binary : a candidate black hole-white dwarf system
› "SNe Ia twins" in the Hubble flow, and the determination of H0
› High-Precision Amplitude-Modulated Continuous-Wave Lunar Laser Ranging
› The exotic black hole-neutron star binaries in our Galaxy
› Evolution and Mass Dependence of UV-to-near-IR Color Gradients up to z=2.5 from HST+JWST
› Updates on dipolar anisotropy in local measurements of the Hubble constant from Cosmicflows-4
› The near-Sun Heliospheric Current Sheet, fluid and kinetic properties
› Modeling Particle Acceleration and MWL Emission of a PeVatron Microquasar V4641 Sgr
› Quantification of abundance uncertainties in chemical models of exoplanet atmospheres
› A Statistical Analysis of Fluence and Energy Distributions of Non-repeating Fast Radio Bursts Detected by CHIME
› Radio, X-ray, and EUV signatures of internal and external reconnection of an erupting flux rope
› Stellar chemistry and planet size: insights from GALAH DR4
› Stranger Things: A Grid-based Survey of Strange Modes in Post-Main Sequence Models
› Silicate emission in a type-2 quasar: JWST/MIRI constraints on torus geometry and radiative feedback
› The role of the galaxy stellar mass function in determining the cosmological distribution of astrophysical transients with applications to fast radio bursts and merging binary black holes
› KM3NeT/ARCA stacking search for high-energy neutrinos from blazars
› Peculiar SN Ic 2022esa: An explosion of a massive Wolf-Rayet star in a binary as a precursor to a BH-BH binary?
› Search for persistent radio emission towards selected localised Fast Radio Burst positions using the MeerKAT Telescope
› Spectropolarimetric characterisation of exoplanet host stars in preparation of the $Ariel$ mission II. The magnetised wind environment of TOI-1860, DS Tuc A, and HD 63433
› SDSS-V LVM: Resolving Physical Conditions in the Trifid Nebula
› Direct observational evidence that higher-luminosity type 1 active galactic nuclei are most commonly triggered by galaxy mergers
› The Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey: Quasar Properties from Data Release 10 to 12
› VHE FSRQs with Fermi-LAT: VHE and even brighter states in high-z FSRQs due to an HBL-like component?
› On Constraining the Proposed Hierarchical Triple Scenario for an Eccentric Milli-Second Pulsar Binary PSR J1618-3921
› Insights into Extragalactic Background Light constraints with MAGIC archival data
› Distinguishing ram pressure from gravitational interactions: Applying the Size-Shape Difference method to real galaxies
› The suppression of the matter power spectrum: strong feedback from X-ray gas mass fractions, kSZ effect profiles, and galaxy-galaxy lensing
› The Composite Spectrum of QSO Absorption Line Systems in DESI DR2
› MIRI spectrophotometry of GN-z11: Detection and nature of an optical red continuum component
› A new constraint on the $y$-distortion with FIRAS: implications for feedback models in galaxy formation and cosmic shear measurements
› Effect of the avoided crossing on the rovibrational energy levels, resonances, and predissociation lifetimes within the ground and first excited electronic states of lithium fluoride
› Linearly Polarized Gravitational Waves from Bubble Collisions
› Properties of Stable Massive Quark Stars in Holography
› Thermoelectric coefficients of two-flavor quark matter from the Kubo formalism
› Exploring Leptogenesis, WIMP Dark Matter, and Gravitational Waves in an extended Scalar Framework
› Quasinormal modes of a static black hole in nonlinear electrodynamics
› Inflationary assessment of $F(\mathcal{R},\tilde{\mathcal{R}})$ Einstein-Cartan models
› Limiting Reduction and Modified Gravity
› Flexible Gravitational-Wave Parameter Estimation with Transformers
› Singular $\alpha$-attractors
› Modeling dark matter halos with self-interacting fermions
› Topological Shell Structures in Neutron Stars: Effects on Equilibrium, Oscillations, and Gravitational-Wave Signatures
› Neutron stars in $f(\mathbb{Q})$ gravity
› WASP-39b: exo-Saturn with patchy cloud composition, moderate metallicity, and underdepleted S/O
› The Case for Hot-Mode Accretion in Abell 2029
› Extremely luminous optical afterglow of an energetic gamma-ray burst GRB 230204B
› Concept integral field unit spectrometer instrument for the next-generation mm-wave cosmological surveys
› REBELS-IFU: Dust Build-up in Massive Galaxies at Redshift 7
› Feedback and dynamical masses in high-$z$ galaxies: the advent of high-resolution NIRSpec spectroscopy
› Scaling relations, dynamical heating and tidal disruption in spin $s$ ultralight dark matter models
› Probing the Distance Duality Relation with Machine Learning and Recent Data
› Time-resolved spectro-polarimetric analysis of extremely bright GRB 230307A: Possible Evidence of evolution from photospheric to synchrotron dominated emission
› Analyzing type Ia supernovae near-infrared light curves with Principal Component Analysis
› Polarization Angle Orthogonal Jumps in Fast Radio Bursts
› MINDS. Anatomy of a water-rich, inclined, brown dwarf disk: lack of abundant hydrocarbons
› The fate of the progenitors of luminous red novae: Infrared detection of LRNe years after the outburst
› Impact of magnetic field gradients on the development of the MRI: Applications to binary neutron star mergers and proto-planetary disks
› Structure and Magnetic Field of the Bright-rimmed Cloud IC 1396E/SFO 38
› Dark Classification Matters: Searching for Primordial Black Holes with LSST
› Planck Constraints on Axion-Like Particles through Isotropic Cosmic Birefringence
› Low-metallicity massive single stars with rotation. III. Source of ionization and C-IV emission in I Zw 18
› A systematic search for dormant galaxies at z~5-7 from the JWST NIRSpec archive
› A general polynomial emulator for cosmology via moment projection
› Testing Photometric Techniques for Measuring the Rest-Frame UV Spectral Slope Against JWST PRISM Spectroscopy
› Deep Learning Improves Photometric Redshifts in All Regions of Color Space
› Dark energy constraints in light of theoretical priors
› The Fate of Transonic Shocks around Black Holes and their Future Astrophysical Implications
› Spatially resolved gas-phase metallicity at z~2-3 with JWST/NIRISS
› XMAGNET : Kinetic, Thermal and Magnetic AGN Feedback in Massive Galaxies at Halo Masses $\sim 10^{13.5}$ M$_\odot$
› HD 44892: The youngest (or oldest?) gas-harbouring debris disc around an intermediate mass star
› Radiation damage to the Hubble Space Telescope during two Solar cycles, and correction of Charge Transfer Inefficiency using ArCTIc
› Macromodel-free flux-ratio prediction in quadruply imaged quasars with local constraints from lensed arcs
› LIMFAST. IV. Learning High-Redshift Galaxy Formation from Multiline Intensity Mapping with Implicit Likelihood Inference
› WIYN Open Cluster Study. XCVII. An Extended Radial-Velocity Survey and Spectroscopic Binary Orbits in the Open Cluster NGC 188
› Radiative hydrodynamic simulations of FIP fractionation in solar flares
› SN 2025coe: A Multiple-Peaked Calcium-Strong Transient from A White-Dwarf Progenitor
› No Observational Evidence for Dark Matter Nor a Large Metallicity Spread in the Extreme Milky Way Satellite Ursa Major III / UNIONS 1
› Multi-faceted light pollution modelling and its application to the decline of artificial illuminance in France
› Formation of protostars and the launching of stellar core outflows with moving-mesh radiation non-ideal magnetohydrodynamics
› On the Dusty Proximate Damped Lyman-{\alpha} System toward Q2310-3358 at z = 2.40
› Properties of Carbon-rich AGB Stars in the LMC and the Milky Way
› Kinematic scaling relations of disc galaxies from ionised gas at $z\sim1$ and their connection with dark matter haloes
› Low-energy Radio Bursts from Magnetar XTE J1810$-$197: Implications for Fast Radio Bursts
› Kinematic Mapping of Giant Arcs: A New Method to Locate Lensing Critical Curves
› On the planetary forcing of the Solar dynamo: Evidence from a Lagrangian framework
› Sequential Convex Programming for Multimode Spacecraft Trajectory Optimization
› Revisiting wideband pulsar timing measurements
› The Milky Way stellar halo is twisted and doubly broken: insights from DESI DR2 Milky Way Survey observation
› Holographic complexity and the Hubble tension: a quantum gravity portrayal for the large scale structure of the cosmos
› The Dynamics of Reheating in Loop Quantum Cosmology
› Superheavy dark matter from the natural inflation in light of the highest-energy astroparticle events
› Equation of state and Fermi liquid properties of dense matter based on chiral effective field theory interactions
› Precision predictions of Starobinsky inflation with self-consistent Weyl-squared corrections
› Gravitational scattering of two neutron stars
› MaxWave: Rapid maximum likelihood wavelet reconstruction of non-Gaussian features in gravitational wave data
› Eccentricity evolution consistency test to distinguish eccentric gravitational-wave signals from eccentricity mimickers
› The Great Impersonation: $\mathcal{W}$-Solitons as Prototypical Black Hole Microstates
› Chaotic Inflation RIDES Again

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