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Moon and Jupiter over the small dome
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RSS  Latest preprints on astro-ph:

› Isotropic Equivalence of STVG--MOG and $\Lambda$CDM and Its Breakdown in Large--Scale Anisotropic Cosmological Observables
› Little Red Dots on FIRE: The Ability of Bursty Galaxies to Host an Abundant Population of High-Redshift AGN
› The Little Blue and Red Dots Rosetta Stones: Non-Gaussian broad lines, hot dust, and X-ray weakness
› Physically-motivated priors in the local distance ladder significantly reduce the Hubble tension
› Drifters on the edge of town: $\lambda$ Bo\"otis stars in clusters
› The Perpendicularity of Dust Lanes and Radio Jets in Early-Type Galaxies: Implications for AGN Feedback
› Subsolar mass black holes from stellar collapse induced by primordial black holes
› Insights into the Physical Nature of Polar Ring Galaxies from H I Observations
› Warps survive beyond fly-by encounters in protoplanetary disks. RW Aur A as a case study
› Obscured AGN at z < 1.5: X-ray to Far-Infrared SEDs and Host Galaxy Morphologies in the GOODS Fields
› Observational Implications of Cosmic Ray-Inverse Compton 'Boosted' Cool Cores in Clusters
› The LBT $Y_{\rm p}$ Project I: An Improved Determination of the Primordial Helium Abundance -- Project Description, Sample Selection, Observations, and Methodology
› The LBT $Y_{\rm p}$ Project II: MODS Spectra, Physical Conditions, and Oxygen Abundances in Local Metal-Poor Nebulae
› The LBT $Y_{\rm p}$ Project III: LUCI Spectra of Metal-Poor Nebulae
› The LBT Y$_\mathrm{p}$ Project IV: A New Value of the Primordial Helium Abundance
› The LBT $Y_{\rm p}$ Project V: Cosmological Implications of a New Determination of Primordial $^4$He
› Mapping dark matter in the Bullet Cluster using JWST imaging and spectroscopy
› X-Ray Analysis of an Off-Axis Merger Stage Binary Galaxy Cluster: PSZ2 G279.79+39.09
› Fast, dust-poor outflows in the local candidate dual AGN MCG-03-34-64 observed with VLT/ERIS
› High energy neutrinos from pulsar-powered optical transients: LFBOTs as potential origin of the KM3NeT event KM3-230213A
› Tensions in Cosmology: Interpreting Them Through Inhomogeneous Models
› Editorial: Mass and Angular Momentum Transport of Rapidly Rotating Hot Stars
› Testing the Association of Supermassive Black Hole Infrared Flares and High-energy Neutrinos
› Conversion Layer Controls the Evolution of Magnetic Deflections Near the Alfven Surface
› How isotropic is dark energy?
› Unveiling BLR Structure in AGN with High Resolution X-Ray Spectra: An Analytic Approach to Wind Emission Line Profiles
› Older Ages for 23 Pre-Main Sequence Stars in Upper Scorpius Using Dynamical Mass-Constrained Stellar Evolutionary Models
› Constructing a gravitational wave analysis pipeline for extremely large mass ratio inspirals
› A Formation Crisis of Repeating Partial Tidal Disruption Events
› SED and Galactic kinematic diagnostics for dormant BH/NS binary candidates
› The GECKOS Survey: Extraplanar ionised gas in star-forming galaxies from eDIG to galaxy-scale winds
› Probing Star-Forming Properties via ALMA Observations of Massive Protocluster IRAS 15596-5301
› The size-velocity dispersion relationship of Galactic HII regions
› The accretion-ejection connection in the asymmetric Th 28 jet revealed by MUSE-NFM
› Distinguishing the nature of dark matter by mapping cosmic filaments from Lyman-alpha emission
› On the dynamics of magnetoviscous warped discs around compact objects
› Apsidal motion and TESS light curves of two southern eclipsing binaries with high eccentricity: V1647 Sgr and V2283 Sgr
› A unified framework for hot accretion flows with finite angular momentum: from Bondi-like to disc-like regimes
› Detection of an Extremely Luminous Radio Counterpart to the Be/X-ray Binary A0538-66
› Ultra-High Energy Cosmic Rays from the Galactic Center
› Prediction of multi-wavelength emissions associated with X-ray flare and extended emission of GRBs
› Statistical study for binary star evolution in dense embedded clusters
› Ground Level Enhancement (GLE#77) in the gamma-ray component: First observation from Arctic and Antarctic stations
› Approximation of the reception coefficients of cosmic rays neutron component for latitude measurement
› Operational Solar Flare Forecasting System Using an Explainable Large Language Model
› The SPIRou Legacy Survey: Detection of a nearby world orbiting in the habitable zone of Gl725B achieved by correcting strong telluric contamination in near-infrared radial velocities with WAPITI
› Rotational Spectroscopy as a Tool to Study Vibration-Rotation Interaction: Investigations of $^{13}$CH$_3$CN and CH$_3$$^{13}$CN up to $v_8 = 2$ and a Search for $v_8 = 2$ Transitions toward Sagittarius B2(N)
› X-ray Spectroscopy of Disk Winds in Black Hole X-ray Binaries
› MAGAZ3NE: Dust Deficiency in Ultramassive Quiescent Galaxies at $3
› Millimeter and submillimeter spectroscopy of methylallene, CH$_3$CHCCH$_2$
› Equatorially Asymmetric Magnetic Fields and Their Impact on Black Hole Accretion Dynamics
› QSOFEED: Investigating warm molecular, low- and high-ionization atomic gas in six type-2 quasars with GTC/EMIR
› The Bondi universe: How negative mass drives the cosmological expansion
› Linear perturbation theory and structure formation in a Brans-Dicke theory of gravity without dark matter
› G183: An outer galaxy filament feeding a massive protostar
› Seeds of supermassive black holes in general relativistic and alternative cosmologies: Implications of massive seeds
› Contrastive Learning of Extragalactic Stellar Streams: Sculpting a Latent Space of Representations with DES DR2 Photometry
› Stereoscopic Observations of Solar X-ray Sources Explained by a Data-Constrained Magnetohydrodynamic Simulation
› Quantifying the C/O ratio in the planet-forming environments around very-low-mass stars
› Rediscussion of eclipsing binaries. Paper XXVIII. The metallic-lined system DV Bootes
› Inhibiting Conduction by He Mixing in Interiors of Jupiter and Saturn
› The Simons Observatory: On-sky performance of radio-transparent multi-layer insulation (RT-MLI) using Styroace-II Styrofoam
› HEP digital micromirror devices for precision solar spectroscopy
› Sunspot simulations with MURaM -- I. Parameter study using potential field initial conditions
› Human versus Artificial Inteligence; a significant example in astrophysics, alas
› The Effect of Tidal Heating and Volatile Budgets on the Outgassed Atmosphere of 55 Cancri e
› Physical origin of very-high-energy gamma rays from the low-luminosity active galactic nucleus NGC 4278 and implications for neutrino observations
› Too many or too massive? Investigating the high-$z$ demography of active SMBHs from JWST
› Evolution of Supermassive Black Hole Pairs on Inclined Orbits in Post-Merger Galaxies
› MARVELously Dark: the gravothermal evolution of dwarf halos in velocity-dependent SIDM
› Denoising the Deep Sky: Physics-Based CCD Noise Formation for Astronomical Imaging
› PDRs4All: XVIII. The evolution of the PAH ionisation and PAH size distribution across the Orion Bar
› Comparison of MOND and Verlinde's emergent gravity in dwarf spheroidals
› When inflationary perturbations refuse to classicalise: the role of non-Gaussianity in Wigner negativity
› Axions on a Hyperbolic Ride: Geometric Suppression of CMB Isocurvature and a Blue-Tilted Spectrum
› A Maximum Entropy Conjecture for Black Hole Mergers
› Sculpting of Martian brain terrain reveals the drying of ancient Mars
› Nonlocal Corrections to Scalar Field Effective Action in de Sitter spacetime
› Exact black holes and black branes with bumpy horizons supported by superfluid pions
› High-bandwidth frequency domain multiplexed readout of transition-edge sensors for neutrinoless double beta decay searches
› The Impact of Star Formation and Feedback Recipes on the Stellar Mass and Interstellar Medium of High-Redshift Galaxies
› Zooming-in on cluster radio relics -- I. How density fluctuations explain the Mach number discrepancy, microgauss magnetic fields, and spectral index variations
› Possible evidence for extended X-ray emission surrounding PSR B0656+14 with eROSITA
› J-PAS and PFS surveys in the era of dark energy and neutrino mass measurements
› Fast Low Energy Reconstruction using Convolutional Neural Networks
› Non-Separable Halo Bias from High-Redshift Galaxy Clustering
› The Effective Field Theory of Large Scale Structure for Mixed Dark Matter Scenarios
› Phantom crossing or dark interaction?
› Jitter Sensing and Control for Multi-Plane Phase Retrieval
› PHECT: A lightweight computation tool for pulsar halo emission
› Lense-Thirring precession of neutron-star accretion flows: Relativistic versus classical precession
› Dark Degeneracy in DESI DR2: Interacting or Evolving Dark Energy?
› An improved model for the effect of correlated Si-III absorption on the one-dimensional Lyman-$\alpha$ forest power spectrum
› Resistive Scaling in the Magnetic Helicity-Driven Inverse Cascade
› BICEP/Keck XX: Component-separated maps of polarized CMB and thermal dust emission using Planck and BICEP/Keck Observations through the 2018 Observing Season
› Exotic PeVatrons as sources of ultra-high-energy gamma rays
› EIGER VIII: First stars signatures in the connection between OI absorption and Galaxies in the Epoch of Reionization
› Probing Primordial black holes with the distortion of Stochastic Gravitational Wave Background
› Gravitational-wave and electromagnetic detections in the context of the CosmoDC2 LSST synthetic catalog
› Hydrodynamic Simulations of Tidal Disruption Encores
› Photometric Redshifts in JWST Deep Fields: A Pixel-Based Alternative with DeepDISC
› Close-in compact super-Earth systems emerging from resonant chains: slow destabilization by unseen remnants of formation
› Sequential Fragmentation of C/2025 K1 (ATLAS) After Its Near-Sun Passage
› A Galactic Transformation -- Understanding the SMC's Structural and Kinematic Disequilibrium
› Defects and Inconsistencies in Solar Flare Data Sources: Implications for Machine Learning Forecasting
› Tales of stellar and binary co-evolution, told by stellar oscillations -- Binary demographics and their impact on stellar mass, orbits, and age estimates in main-sequence and red-giant stars
› How is Cold Gas Loaded into Galactic Nuclear Outflows?
› A Comprehensive Interpretation of Fermi-LAT Pulsars: Fundamental-Plane Death Border, Visibility Thresholds, and GeV-TeV Unification
› A Dynamo Confinement Scenario for the Solar Tachocline and its Implications for Spin-down in the Radiative Spreading Regime
› Discovery of 1H-cyclopent[cd]indene (c-C11H8) in TMC-1 with the QUIJOTE line survey: A new three-ringed polycyclic aromatic hydrocarbon
› ExoMiner++ 2.0: Vetting TESS Full-Frame Image Transit Signals
› Lensing without mixing: Probing Baryonic Acoustic Oscillations and other scale-dependent features in cosmic shear surveys
› Fast variability and circular polarization of the 6.7 GHz methanol maser in G33.641$-$0.228
› How well is the local Large Scale Structure of the Universe known? CosmicFlows vs. Biteau's Galaxy Catalog with Cloning
› Radio-Near Infrared Imaging of Dual Active Galactic Nuclei Candidates
› A redshift survey of the nearby galaxy cluster Abell 2199 : No upturn of the faint-end slope of galaxy luminosity function
› Projective Transformations for Regularized Central-Force Dynamics: Hamiltonian Formulation
› Comparing Simulated and Observed Particle Energy Distributions through Magnetic Reconnection in Earth's Magnetotail
› Asymptotics of spherical dynamos exhibiting a small-scale MAC balance
› Fitting NANOGrav 15-year data and ACT data with modified inflation in entropic cosmology
› Multi-probe analysis of strong-field effects in $f(Q)$ gravity
› Searching for axion dark matter with magnetic resonance force microscopy
› Towards First Detection of the Solar MSW Transition With JUNO
› Exponential plateaus and inflation in metric-affine gravity
› A framework for LISA population inference
› Spectrum of radiation from global strings and the relic axion density

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