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RSS  Latest preprints on astro-ph:

› Oort Cloud Bombardment by Dark Matter
› Tidal disruption event rates across cosmic time: forecasts for LSST, Roman, and JWST and their constraints on the supermassive black hole mass function
› How Do Disk Galaxies Form?
› The GMRT archive atomic gas survey -- III. Comparative Study of Dark Matter Halos in Nearby Galaxies
› Wiggling Through the ICM: Multi-Resolution Radio Imaging of a Tailed Radio Galaxy in MACS J1354.6+7715
› Classifying white dwarfs from multi-object spectroscopy surveys with machine learning
› Establishing a relationship between the cosmological 21 cm power spectrum and interferometric closure phases
› Abundant hydrocarbons in a buried galactic nucleus with signs of carbonaceous grain and polycyclic aromatic hydrocarbon processing
› Multi-spin stellar velocity maps of the most massive galaxies
› Clustering of z~6.6 Quasars and [O III] Emitters Constrains Host Halo Masses and Duty Cycles in 25 ASPIRE Fields
› Differentiable Stochastic Halo Occupation Distribution with Galaxy Intrinsic Alignments
› ASPIRE: The Environments and Dark Matter Halos of Luminous Quasars in the Epoch of Reionization
› Testing black hole space-times with the S2 star orbit: a Bayesian comparison
› The Impact of Galaxy Formation on Galaxy Biasing, and Implications for Primordial non-Gaussianity Constraints
› Complex hydrogen chemical equilibrium and Gaia low mass problem in cool white dwarfs
› The CON-quasar stage of IRAS 07251-0248 E
› Wide sdB binaries. I. Orbital and atmospheric parameters
› Modeling the recent interactions between the Magellanic Clouds and Milky Way
› Dynamics of the coronal magnetic field in the 2022-10-02 X-class flare
› Detailed TESS-Based Light Curve Modeling and Fundamental Parameter Estimation of 27 W UMa-Type Contact Binaries
› On the forced orbital plane of the Hilda asteroids
› ICM-SHOX III. The case of MACS J0018.5+1626, a radio relic that looks like a radio halo?
› Wising up to CatWISE: using simulation-based inference to interpret the ecliptic bias and confirm the cosmic dipole excess
› Shocks, Winds, and a Torus: The Large Binocular Telescope Interferometer (LBTI) Resolves the Active Nucleus of NGC 4151
› The Galaxy Bias Profile of Cosmic Voids:A Comparison of Void Finders
› Growth of High-Redshift Quasars from Fermion Dark Matter Seeds
› Thermal Eclipse Observation of the Young Hot Neptune AU Mic b with Spitzer
› Searching for gravitational waves from compact binary mergers powering long gamma-ray bursts during LIGO-Virgo-KAGRA's O3 run
› Rotating strange dwarfs and their indistinguishability from white dwarfs
› A gamma-ray-emitting blazar B3 1239+376 at z = 3.82 identified in a multi-wavelength context
› ALMA 873 $\mu$m Polarization Observations of the PDS~70 Disk
› Evolution of cataclysmic variables under different magnetic braking prescriptions
› IFU Spectroscopic Study of the Planetary Nebula Abell 30: Mapping the Ionisation and Kinematic Structure of the Inner Complex
› An Accretion-Modulated Internal Shock Model for Long GRBs
› First Detailed MeerKAT Imaging Spectroscopy of a Solar Flare
› Galactic seismology: can a disc-crossing impulse explain the large-scale perturbations in the Milky Way's disc?
› Sulfur Enrichment in Close-in Exoplanet Atmospheres Induced by Pebble Drift across the Salt Line
› Fractal dimension of the cosmic web with different galaxy types
› B-field Orion Protostellar Survey (BOPS). IV: The Relative Orientation Between Magnetic Fields and Density Structures in Young Protostellar Envelopes
› The sub-arcsecond ILT view of the Bo\"{o}tes Deep Field: A link between low-frequency kiloparsec radio morphology and AGN driven ionised outflows
› Dark Energy After DESI DR2: Observational Status, Reconstructions, and Physical Models
› Habitability of Tidally Heated H$_2$-Dominated Exomoons around Free-Floating Planets
› A Chemistry-First Centered Icy Chemical Inventory of Protostellar Sources with JWST
› ELFO: A Python package for emission line fitting optimization in integral field spectroscopy data
› The Double-Burst Nature and Early Afterglow Evolution of Long GRB 110801A
› Mergers Drive Structural Complexity but Not Starbursts in Lyman-$\alpha$ Emitters at $3 < z < 4$: A JWST Spatially Resolved View
› Probing Compact Objects in Wide-Orbit Binaries with Joint LAMOST LRS and MRS
› The Correlation Length of Turbulence in Magnetic Clouds
› Nano-particle Transition Matrix code implementation
› Effects of Dynamo-Generated Large-Scale Magnetic Fields on the Surface Gravity ($f$) Mode
› Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys
› Exploring the central engines of gamma-ray bursts from prompt light curves
› Particle acceleration signatures in the time-dependent one-zone synchrotron self-Compton model of blazar flares
› XGAP with uGMRT I: Old AGN plasma in merging galaxy groups
› MESS: Multi-Epoch Spectroscopic Solver for Detecting Double-Lined Systems
› Coalescence Forensics: Weighing the Hosts of Hierarchical Binary Black Hole Mergers
› The kinematic cosmic dipole beyond Ellis and Baldwin
› Relativistic Dynamics and Bondi-Hoyle-Lyttleton Accretion onto Rotating Embedded Black Hole Models
› Momentum-conserving self-gravity in the phantom smoothed particle hydrodynamics code. Parallel dual tree traversal for the symmetric fast multipole method
› MIGHTEE/COSMOS-3D: The discovery of three spectroscopically confirmed radio-selected star-forming galaxies at z=4.9-5.6
› Bayesian imaging inverse problem with scattering transform
› Photometric variability of nitrogen-rich Wolf-Rayet stars in Magellanic Clouds with OGLE
› Microlensing constraint on Primordial Black Hole abundance with Subaru Hyper Suprime-Cam observations of Andromeda
› Predicting galaxy bias using machine learning
› The Effects of Non-ideal Mixing in Planetary Magma Oceans and Atmospheres
› Early growth of massive black holes in dynamical dark energy models with negative cosmological constant
› The JWST EXCELS survey: The ages and abundances of $3
› Long-term timing of the relativistic binary PSR J1906+0746
› Tracing AGN Feedback Power with Cool/Warm Outflow Densities: Predictions and Observational Implications
› Improved Heavy Dark Matter Annihilation Search from Dwarf Galaxies with HAWC
› Cosmographic parameters from current and next-generation gravitational wave detectors
› Does Cosmology require Hermiticity in Quantum Mechanics?
› Time lags and their association with the Boundary Layer structure in a Z source GX 349+2
› Direction-dependent calibration with image-domain gridding
› Testing cosmic anisotropy with cluster scaling relations
› Water absorption confirms cool atmospheres in two little red dots
› ACT DR6+Planck impact on inflation with non-zero vacuum expectation value and the post-inflationary behavior
› Relic of quadrupole deformation produced in a hot neutron star era
› Impact on Inferred Neutron Star Equation of State due to Nonlinear Hydrodynamics, Background Spin, and Relativity
› Suppression of Gravitational-Wave Echoes in Diffeomorphism-Invariant Nonlocal Gravity
› Intereses convergentes: los a\~nos previos a la visita de Einstein a la Argentina en 1925
› Simulating first-order phase transition during inflation
› An approximate Kappa generator for particle simulations
› Induced-Gravity Higgs Inflation in Palatini Supergravity Confronts ACT DR6
› On the stability of viscous Riemann ellipsoids
› Detecting gravitational wave background with equivalent configurations in the network of space based optical lattice clocks
› Early-universe constraints on the electron mass
› Mesoscopic chemical potentials across the (hyper)nuclear landscape
› deci-Hz Gravitational Wave Observations on the Moon and Beyond
› Foreground removal and 21 cm signal estimates: comparing different blind methods for the BINGO Telescope
› Impact of Interacting Dark Energy on the Growth of Matter Density Perturbations: Observational Constraints from DESI and Multi-Probe Data
› Orbital eccentricity in a neutron star - black hole binary merger
› Spins of Black Holes in X-ray Binaries and the Tension with the Gravitational Wave Measurements
› Orbital Eccentricity and Spin-Orbit Misalignment Are Evidence that Neutron Star-Black Hole Mergers Form through Triple Star Evolution
› Stabilizing simulation-based cosmological Fisher forecasts: a case study using the Voronoi volume function
› Characterizing Density and Gravitational Potential Fluctuations of the Interstellar Medium
› Resolving Black Hole Family Issues Among the Massive Ancestors of Very High-Spin Gravitational-Wave Events Like GW231123
› Phantom crossing or dark interaction?
› Magnetic Flux Emergence in Binary Neutron Star Remnants
› On the synergetic use of Ariel and JWST for exoplanet atmospheric science
› Resonant W and Z Boson Production in FSRQ Jets: Implications for Diffuse Neutrino Fluxes
› Search for neutrino emission from blazar $\gamma$-ray flares accounting for possible neutrino time delays
› Gravitational Wave Spectral Shapes as a probe of Long Lived Right-handed Neutrinos, Leptogenesis and Dark Matter: Global versus Local B-L Cosmic Strings
› A Modified 3D Biconical Outflow Model: Spatial Constraints on AGN-driven Outflows
› Interacting binaries on the Main Sequence as in-situ tracers of mass transfer efficiency and stability
› Large-Scale Galaxy Correlations from the DESI First Data Release
› Connecting Star Formation in the Milky Way and Nearby Galaxies -II. An Observationally Driven Analytical Model for Predicting Cloud-Scale Star Formation Rates
› The spectrum of $n_s$ constraints from DESI and CMB data
› An Active Galaxy Cluster Merger at Cosmic Noon Revealed by JWST Weak Lensing and Multiwavelength Probes
› Fast rotations in galaxies at cosmic noon indicate central concentration of stars, dark matter or massive black holes
› Distinct Rotational Evolution of Giant Planets and Brown Dwarf Companions
› A first GLIMPSE into star clusters populations across cosmic time
› Fast Magnetoacoustic Wave Behavior within Gravitationally Stratified, Magnetically Inhomogeneous Media
› Prompt cusps in hierarchical dark matter halos: Implications for annihilation boost
› The FLAMINGO Project: Exploring the X-ray--cosmic-shear cross-correlation as a probe of large-scale structure
› An emulator for the ionizing photon mean free path in ultra-high resolution simulations: the implications of mean free path measurements for the reionization history
› Gravitational Waves from Feebly Interacting Particles in a First Order Phase Transition
› Twisted magnetar magnetospheres: a class of semi-analytical force-free non-rotating solutions
› Dark-Matter-Enhanced Probe of Relic Neutrino Clustering
› Importance of Shot Noise in the Search for an Isotropic Stochastic Gravitational-Wave Background with Next Generation Detectors
› Gauge Dependence of Scalar-Induced Gravitational Waves from Isocurvature Perturbations: Analytical Results
› WIMP Freeze-out dynamics under Tsallis statistics
› Misalignment dynamics of Scalar Condensates with Yukawa coupling: Particle and Entropy Production
› Coordinate Systems and Transforms in Space Physics: Terms, Definitions, Implementations, and Recommendations for Reproducibility

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