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RSS  Latest preprints on astro-ph:

› Decisively Demonstrating Roman CGI's TTR5 Requirement by Reimaging a Newly-Discovered Brown Dwarf Orbiting a Bright Accelerating Star
› UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings
› Rhea-RT: Dynamical impact of Central Molecular Zone conditions on ISM properties and stellar feedback coupling
› KURVS: chemical properties from multiple strong line calibrations for star-forming galaxies at $z\sim1.5$
› Clues from $\mathcal{Q}$--A null test designed for line intensity mapping cross-correlation studies
› Orbital migration and heating history of the Galactic disc: a transition between the bimodal discs
› ClearPotential: Revealing Local Dark Matter in Three Dimensions
› The mysterious Globular Cluster population of MATLAS-2019
› Observational constraints on 3-forms dark energy
› Characterizing the Roman Grism Redshift Efficiency of Type Ia Supernova Host Galaxies for the High-Latitude Time-Domain Survey
› GA-NIFS: Powerful and frequent outflows in moderate-luminosity AGN at $z\sim3-6$
› Transient protostellar cores in high mass star forming regions revealed by time-resolved synthetic imaging of dust emission
› The Space-Based Time-Domain Revolution in Astrophysics
› Detailed Chemical Abundance Analysis of the Brightest Stars in the Turranburra and Willka Yaku Stellar Streams
› Validation of a Third Earth-sized Planet in the TOI-2267 Binary System
› The SPace-based InterFerometer Feasibility (SPIFF) Project: Enabling Future High-Resolution Astronomy Across the EM Spectrum
› Formation of circumstellar material during double-white-dwarf mergers and the early excess emissions in Type Ia supernovae
› Beyond prewhitening: detection of gravity modes and their period spacings in slowly pulsating B stars using the multitaper F-test
› Classification of a New X-ray Catalog of Likely Counterparts to 4FGL-DR4 Unassociated Gamma-ray Sources Using a Neural Network
› Stellar properties and chemical features of the Gaia Catalogue of Nearby Stars observed by GALAH DR4
› High-energy astrochemistry in the molecular interstellar medium
› Hipparcos, Gaia, and RVs reveal that the radio emitting F star HD 220242 has an M dwarf companion, a likely source of the radio emission
› The AURORA Survey: Constraining Chemical Enrichment Pathways at Cosmic Noon with Argon Abundances
› Deuterium fractionation and CO depletion in Barnard 5
› Discovery of Weak O VI Absorption in Underdense Regions of the Low-Redshift Intergalactic Medium
› Strong Bars, Strong Inflow: The Effect of Bar Strength on Gas Inflow
› Spectrally Resolved Gas Kinematics in Cygnus A: XRISM Detects AGN Jet-induced Velocity Dispersion in Multi-temperature Gas
› The Narrow Emission Lines of Seyfert 1 Galaxies: Comparisons with a Large SDSS Sample
› Galaxy Phase-Space and Field-Level Cosmology: The Strength of Semi-Analytic Models
› FEADME: Fast Elliptical Accretion Disk Modeling Engine
› EP250827b/SN 2025wkm: An X-ray Flash-Supernova Powered by a Central Engine and Circumstellar Interaction
› $^{12}$CO $J$=3--2 Observations of Tycho's supernova remnant: constraints on the environmental gas properties
› Irregularity in Active Fast Radio Burst Repeaters and Magnetar Periodic Radio Pulses: Time, Energy, and Frequency Analyses
› Relaxation of time-variable neutron-loaded relativistic jets across the photosphere and their GeV-TeV neutrino counterparts
› Hybrid corona and transient soft X-ray lags in Fairall 9
› Detectability of Atmospheric Biosignatures in Earth Analogs with Varying Surface Boundary Conditions: Prospects for Characterization in the UV, Visible, Near-Infrared, and Mid-Infrared Regions
› MorphZ: Enhancing evidence estimation through the Morph approximation
› Tracking Protostellar Variability in Massive Protoclusters with ALMA: I. Insights from QUARKS and MaMMOtH
› Refined M-type Star Catalog from LAMOST DR10: Measurements of Radial Velocities, $T_\text{eff}$, log $g$, [M/H] and [$\alpha$/M]
› Improved Identification of Strongly Lensed Gravitational Waves with Host Galaxy Locations
› Estimating stellar atmospheric parameters and elemental abundances using fully connected residual network
› The LEGA-C galaxy survey: multiple quenching channels for quiescent galaxies at $z\sim1$
› A Systematic Study of Magnetic Fields Impacts on Neutrino Transport in Core-Collapse Supernovae
› Detailed theoretical analysis of core Helium-burning stars: Mixed mode patterns I. Impact of the He-flash discontinuity and of induced semi-convection
› Multi-wavelength emission in resistive pulsar magnetospheres
› FAUST XXX: Dust enhancement in the young binary L1551 IRS 5
› Scintillating insights into PSR~J0737$-$3039A and the interstellar plasma of the Gum Nebula from MeerKAT
› Does the Babcock-Leighton dynamo operate in rapidly rotating solar-type stars? Exploration using a 3D dynamo model at different rotation rates
› Isotopomer-Specific Carbon Isotope Ratio of Complex Organic Molecules in Star-Forming Cores
› The SALT survey of helium-rich hot subdwarfs: final sample and classification
› Application of time-series analysis methods to a multiple-sector TESS observations: the case of the radio-loud blazar 3C 371
› Near Ultraviolet Transient Explorer (NUTEx): A CubeSat-Based NUV Imaging Payload for Transient Sky Surveys
› Stellar Evolution in Close Binaries: Processes and Outcomes
› Wind-mediated Eddington-limited emission in a 1e4 Black Hole Tidal Disruption Event
› MAUVE-MUSE: A Star Formation-driven Outflow Caught in the Act of Quenching the Stripped Virgo Galaxy NGC 4064
› An analytical framework for atmospheric tides on rocky planets. I. Formulation
› FAST-MEPSA: an optimised and faster version of peak detection algorithm MEPSA
› Is Dark Energy Dynamical in the DESI Era? A Critical Review
› Inflation at the End of 2025: Constraints on $r$ and $n_s$ Using the Latest CMB and BAO Data
› nDspec: a new Python library for modelling multi-dimensional datasets in X-ray astronomy
› Stellar masses and mass ratios for Gaia open cluster members
› OutLines: Modeling Spectral Lines from Winds, Bubbles, and Outflows
› Can accreting isolated neutron stars be detected?
› Constraints on the Population of Common Sources of Gravitational Waves and High-Energy Neutrinos with IceCube During the Third Observing Run of the LIGO and Virgo Detectors
› Model independent approach towards measuring expansion and growth factor from next generation galaxy clustering and lensing angular power spectrum
› A "New Hope" for Moon Formation: Presenting a Multiple Impact Pathway
› Applying the BF method on the DESI evidence for dynamical dark energy models
› Hidden No More: Spotlight on tidal disruption events in active galactic nuclei
› Chemical enrichment in LINERs from MaNGA. II. Characterizing the shape of their radial metallicity gradients
› Pressure and Star Formation in LITTLE THINGS Dwarf Irregular Galaxies
› Reaching diffraction-limited localization with coherent PTAs
› On the validity of the continuity equation in a modified gravity framework with CMB, DES 3x2pt and tomographic ISW data
› A remarkable Gaia-assisted discovery of a temporally varying, triple-lensed quasar at z=2.67
› Resolving the ionizing photon budget crisis with JWST/NIRCam HII clumping constraints at z=6
› Inflation in light of ACT/SPT: a new perspective from Weyl gravity
› Diversity in the haziness and chemistry of temperate sub-Neptunes
› Weighing the Milky Way's Satellite Galaxies Using Pulsar Accelerations
› Impact of geometry on 1D molecular-kinetics simulations of acoustic-gravity wave propagation into the exosphere
› The LISA Astrophysics "Disc-IMRI" Code Comparison Project: Intermediate-Mass-Ratio Binaries in AGN-Like Discs
› Updated and Projected Cosmic Microwave Background Bounds on WIMP Annihilation
› A vision for ground-based astronomy beyond the 2030s: How to build ESO's next big telescope sustainably
› A Stellar Magnesium to Silicon ratio in the atmosphere of an exoplanet
› Shedding Light on Large Space-Based Telescopes: Modeling Stray Light due to Primary Mirror Damage from Micrometeoroid Impacts
› Detection prospects for heavy WIMP dark matter near supermassive black holes, particularly in M31
› Signatures of star formation inside galactic outflows
› Evidence of galaxy cluster rotation in the cosmic microwave background
› CWTHF: Subhalo Identification with Continuous Wavelet Transform
› Lateral Deformation of Large-scale Coronal Mass Ejections during the Transition from Non-radial to Radial Propagation
› Two-dimensional PIC simulation of collective Thomson scattering in a beam-plasma system
› The meaning of "Big Bang"
› Blandford-Znajek Jets and the Total Angular Momentum Evolution of a Black Hole Connected to a Cosmic String
› The Eschatian Hypothesis
› Can the 3 neutrino masses really be found using SN 1987A data?
› Gravitational-wave parameter estimation to the Moon and back: massive binaries and the case of GW231123
› Dark matter mounds from the collapse of supermassive stars: a general-relativistic analysis
› Constraining Gravitational Dark Matter with LHAASO and Fermi-LAT
› Stationary Stars Are Axisymmetric in Higher Curvature Gravity
› Generation of proton beams at switchback boundary-like rotational discontinuities in the solar wind
› Identification and Characterization of the Topside Bulge of the Venusian Ionosphere
› A Nonlocal Realization of MOND that Interpolates from Cosmology to Gravitationally Bound Systems
› Nonlinear evolution of the ergoregion instability: Turbulence, bursts of radiation, and black hole formation
› Cosmological and lunar laser ranging constraints on evolving dark energy in a nonminimally coupled curvature-matter gravity model
› BinaryGFH-v2: Improved method to search for gravitational waves from sub-solar-mass, ultra-compact binaries using the Generalized Frequency-Hough Transform
› Subtracting compact binary foregrounds utilizing anisotropic statistic for third-generation gravitational-wave detectors
› Efficient pulsar distance measurement with multiple nanohertz gravitational-wave sources
› Exploring New Propagation Scales With Galactic Neutrinos
› Measuring the neutron star equation of state from EMRIs in dark matter environments with LISA
› Heterogeneous Cosmological Phase Transitions: Seeded by Domain Walls and Junctions
› Comprehensive survey of hybrid equations of state in neutron star mergers and constraints on the hadron-quark phase transition
› Bringing together African & European research communities with an inclusive astronomy conference
› Tidally Delayed Spin-Down of Very Low Mass Stars
› Probing Spin-Orbit Resonances with the Binary Black Hole Population
› Retrograde predominance of small saturnian moons reiterates a recent retrograde collisional disruption
› Euclid Quick Data Release (Q1): VIS processing and data products
› The dark side of the universe may be more harmonic than we thought
› On Validating Angular Power Spectral Models for the Stochastic Gravitational-Wave Background Without Distributional Assumptions
› SpiderCat: A Catalog of Compact Binary Millisecond Pulsars
› fftvis: A Non-Uniform Fast Fourier Transform Based Interferometric Visibility Simulator
› Caustic fringes for wave dark matter
› Pulsar Sparking: What if mountains on the surface?
› Cosmic sign-reversal: non-parametric reconstruction of interacting dark energy with DESI DR2
› Metal-poor single Wolf-Rayet stars: The interplay of optically thick winds and rotation
› Duration and properties of the embedded phase of star formation in 37 nearby galaxies from PHANGS-JWST
› Earliest Galaxy Evolution in the CANUCS+Technicolor fields: Galaxy Properties at $z\sim10-16$ seen with the Full NIRCam Medium and Broad Band Filters
› Collapsar Disk Outflows III: Detectable Neutrino and Gravitational Wave Signatures
› The z = 9.625 Cosmic Gems Galaxy was a "Compact Blue Monster" Propelled by Massive Star Clusters
› Eccentricity distribution of extreme mass ratio inspirals
› A milliarcsecond localization associates FRB 20190417A with a compact persistent radio source and an extreme magneto-ionic environment
› First Light for the GRAVITY+ Adaptive Optics: Extreme Adaptive Optics for the Very Large Telescope Interferometer
› The Most Probable Behaviour of the Dark Energy Equation of State Indicates a Thawing Quintessence Field: Tomographic Alcock-Paczy\'nski Test with Redshift-Space Correlation Function II
› Pre-flight Background Estimates for COSI
› Investigating episodic mass loss in evolved massive stars IV. Comprehensive analysis of dusty red supergiants in NGC 6822, IC 10, and WLM
› Direct multi-model dark-matter search with gravitational-wave interferometers using data from the first part of the fourth LIGO-Virgo-KAGRA observing run
› Dynamical Masses and Radiative Transfer Modeling of HD 698: a Be Binary in Evolutionary Transition
› On the Exoplanet Yield of Gaia Astrometry
› Finite Lifetime Fragment Model 4 for Striae Formation in the Dust Tails of Comets (FLM 4) Acceleration by Lorenz-force
› High-impact Scientific Software in Astronomy and its creators
› High-Precision Multi-Period Analysis of the Ellipsoidal Variable Candidate TIC~470127886 from TESS Photometry
› Advancing Identification method of Gamma-Ray Bursts with Data and Feature Enhancement
› The FAST-SETI Milky Way Globular Cluster Survey I: A Pilot Multibeam On-the-Fly Search of Five Globular Clusters at L-Band
› Resolving Interchange Reconnection Dynamics in a Fan-Spine-like Topology Observed by Solar Orbiter
› Interstellar Medium in Extremely High Star-Formation Regions: A Prospect of Observations on the Millimetron Space Observatory
› The Milky Way Imaging Scroll Painting Survey: Data Release 1
› Self-lensing of moving gravitational-wave sources can break the microlensing crossing timescale degeneracy
› The impact of AGN environmental effects on testing general relativity with space-borne gravitational wave detector
› Massive Star Clusters as sources of high-energy gamma radiation
› Clumpy, dense gas in the outflow of NGC 1266
› Testing models for angular power spectra: A distribution-free approach
› Angular momentum of vacuum bubbles in a first-order phase transition
› Modelling cosmic-ray transport: magnetised versus unmagnetised motion in astrophysical magnetic turbulence
› Black Hole Thermodynamics: Established Results, Unresolved Paradoxes, and Speculative Resolutions
› Trustworthy scientific inference with generative models
› A Markov Decision Process Framework for Early Maneuver Decisions in Satellite Collision Avoidance
› The complementary of CTAO, direct detection and collider searches for dark matter in Effective Field Theories and Simplified models
› High Energy Particle Production from Proton Synchrotron Radiation in Strong Magnetic Fields in Relativistic Quantum Field Theory
› Restrictions on Initial Conditions in Cosmological Scenarios and Implications for Simulations of Primordial Black Holes and Inflation
› Progress on the ALETHEIA project and a new approach to mitigate events overlap
› Questions related to the Deflection of Light by Gravity determined by Soldner, Einstein and Schwarzschild
› Bayesian Model Selection with an Application to Cosmology

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