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RSS  Latest preprints on astro-ph:
› A Minimal Four-Thruster System for Comet-Based Interstellar Navigation
› Trajectory Stability and Signature Diagnostics for Comet-Based Interstellar Navigation
› The birth of the intracluster medium: the evolution of multiphase gas and Lyman-$\alpha$ haloes in a simulated $z\sim3$ protocluster
› MIGHTEE-HI: Mass Models and Dark Matter properties
› Ram-pressure-induced star formation in low-mass galaxies infalling on-to the Coma cluster: insights from DESI
› Anti-Solar Differential Rotation May Have Revived Magnetic Braking in the Subgiant 31 Aquilae
› What Shape is the Inflationary Bispectrum?
› Search For a Counterpart to the Subsolar Mass Gravitational Wave Candidate S251112cm
› Confirming Nunki as the closest core collapse progenitor candidate to the Sun
› Ultrahigh-Energy Gamma-Ray Sources Need Not Be Hadronic PeVatrons
› Optical outburst evolution of the transient black hole X-ray binary Swift J1727.8-1613: Disc response to jet ejections and late-outburst emergence of powerful disc winds
› A Mass Transferring Brown Dwarf Binary on a 57 Minute Orbit
› Stars stably accreting from substellar objects
› The Physics of Mass Transfer in Substellar and Low-Mass Binaries
› The SPHINX public data release. II. Using low-ionisation absorption lines and dust attenuation to predict Lyman continuum escape
› Ultraviolet variability in Radio-Loud Active Galactic Nuclei observed by UVIT onboard AstroSat
› Quantifying the Scientific Potential of Intermediate and Extreme Mass Ratio Inspirals with the Laser Interferometer Space Antenna
› Compton-thick AGN in the NuSTAR Era. XI. Analyzing 11 CT-AGN Candidates Selected with Machine Learning
› Stellar characterization with photometric colors from J-PLUS and 2MASS surveys
› Long-term outburst activity of comet 17P/Holmes and constraints on ejecta size distributions
› SLSim: a strong lensing population simulation package
› Fast partial-sky spherical harmonic transforms
› Reconstructing the Type Ia Supernova Absolute Magnitude with Two-Probe Physics-Informed Neural Networks
› Planetesimal formation via the streaming instability persists under turbulence driven by magnetorotational instability
› Diffuse X-ray Emission in the Sagittarius C Complex
› Stereoscopic Observation of Recurrent Streamer Waves Driven by Successive Slow Coronal Mass Ejections
› When turbulence beats magnetism: origin of massive star cluster seeds
› State-dependent broadband X-ray timing reconfiguration in the changing-look AGN NGC 1566
› Optical variability and optical--mid-infrared dust lags in Type~1 changing-look AGNs
› On the shape of the ascending branch of the light curves of Long Period Variables
› Bar-Informed Kinematic-Distance Mapping of Molecular Gas in the Inner Milky Way
› An Analysis of Large Astronomical Detector Controller Systems and Implications for Future ESO Detector Systems
› Modeling supernova feedback in galaxy formation simulations with energy-conserving momentum injection
› EMU/GAMA: Refining Dust Extinction Corrections for H{\alpha} Luminosity Functions Using Radio-Based Calibration
› KMTNet Synoptic Survey of Southern Sky II: Data Reduction and Real-Time Transient Detection Pipeline
› Revealing the Spectral Properties of Galactic Interstellar Medium by Survey Observations
› Natura Non Facit Saltum: An Analytical Model of Smooth Slow-Roll to Ultra-Slow-Roll Transition
› Magnetic field measurements in a sample of Class I and Flat-Spectrum protostars observed with SPIRou
› Tightening Cosmological Constraints Within and Beyond $\Lambda$CDM Using Gamma-Ray Bursts Calibrated with Type Ia Supernovae
› Optical transients from non-explosive double white-dwarf mergers: the case of a central neutron star remnant
› VERITAS Observations Contemporaneous with the LHAASO Detection of NGC 4278
› Why Are Some Optically Red Spirals NUV-r Blue?
› The Potential for Hadronic Particle Acceleration in Galactic Pulsar Wind Nebulae
› Mass Inventory of the Solar System Beyond the Sun: A Systematic Compilation with Uncertainty Budget
› Forecasting Sensitivity to Modified Dispersion Effects in Pulsar Timing Arrays
› Photometric masses for long period CVs: the case study of CSS131106
› Searching for Molecular Signatures in 14 Transiting Exoplanets with SPIRou
› RABBITS - III. Modelling relativistic accretion discs around spinning black holes in galaxy formation simulations
› A high-resolution X-ray view of the ultra-fast outflow in MAXI J1810-222
› Scatter in the Relation between Persistent Radio Source Luminosity and Fast Radio Burst Rotation Measure: A Window into Circum-burst Environments
› The Engine and its Flows: Little Red Dot spectra are shaped by the column densities of their gas envelopes
› A 3D physico-chemical model of a pre-stellar core. II. Dynamic chemical evolution in a pre-stellar core model using tracer particles
› Long-algorithm based quantum search for gravitational wave
› Interstellar Dust Transport Through the Heliosphere Including the Sector Region
› Inflation with the Gauss-Bonnet term in the Palatini formulation
› Gravity anomaly from laboratory experiments to astrophysics
› The effects of bar strength and kinematics on galaxy evolution II: The global and local impacts of slow-strong bars
› Enhanced foreground mitigation in thermal SZ Compton-$y$ maps via polarization and deprojection
› The Revised Evolutionary Volume Tolman Test: Cosmological Constraints from Galaxy Evolution
› Kinetic-based macro-modeling of the solar wind at large heliocentric distances: Kappa electrons at the exobase
› Test of a 34 GHz EOM laser frequency comb at ESPRESSO
› PRODIGE -- envelope to disk with NOEMA VIII. Sulfur oxides trace a shock caused by a streamer in the inner envelope of a protostar
› Radiative GRMHD simulations of puffy accretion discs: Numerical versus analytical models of sub-Eddington accretion
› The Sunrise Chromospheric Infrared Spectro-Polarimeter SCIP: an instrument for SUNRISE III
› Simulations of a 2 x 1.5D coded aperture camera for X-ray astronomy
› The efficient delivery of highly-siderophile elements to the core creates a mass accretion catastrophe for the Earth
› The chemical DNA of the Magellanic Clouds VI. Origin and evolution of neutron-capture elements in the SMC
› JWST Reveals Two Overmassive Black Hole Candidates in Dwarf Galaxies at z $\approx$ 0.7: Pushing Black Hole Searches into the Dwarf-Galaxy Regime
› Characterization of molecular outflows at core-scale in the massive clump AGAL G345.0029-0.224
› On the Astrophysical Origin of Binary Black Hole Subpopulations: A Tale of Three Channels?
› Self-Limited Accretion onto Embedded Binaries in a Uniform Medium
› In situ U Pb chronology and chemistry of zirconolite in the andesitic meteorite Erg Chech 002
› Comprehensive VLBI observations of Galileo satellites with the AuScope array
› Extended Theories of Electrodynamics in $f(R)$ Gravity
› The imitation game (r)evolutions: $Q$-star effective shadow from GRMHD analysis
› Is the Turner Window Open? Seeking Closure with Resonant Absorption of Galactic Axions in NaI Dark Matter Detectors
› Multi-Component Dark Matter as a Solution to the Galactic Center GeV Excess
› Spin crossover in FeO under shock compression
› Scale-Aware Navigation of Astronomical Survey Imagery Data on High Resolution Immersive Displays
› Modified Friedmann equations and non-singular cosmologies in $d=4$ non-polynomial quasi-topological gravities
› Compressive Structures in the Foreshock of Collisionless Shocks
› Origin of radio polarization in pulsar polar caps
› Encyclopedia Magneticum: Scaling Relations from Cosmic Dawn to Present Day
› Hint towards inconsistency between BAO and Supernovae Dataset: The Evidence of Redshift Evolving Dark Energy from DESI DR2 is Absent
› The DORCHA suite: nature, nurture, and the phase space distribution of the Milky Way's high redshift progenitors today
› Characterizing Compact-object Binaries in the Lower Mass Gap with Gravitational Waves
› Numerical simulations of jet launching and breakout from collapsars
› Renzo's rule revisited: A statistical study of galaxies' baryon - dark matter coupling
› Stringent constraint on the CCC+TL cosmology with $H(z)$ Measurements
› Primordial Gravitational Waves in Parity-violating Symmetric Teleparallel Gravity
› The origin of extreme N-emitters in star-forming galaxies at z$
› Alpha effect and dynamo in density-stratified turbulence with large-scale shear: applications to protoplanetary discs and astrophysical clouds
› A novel algorithm for GPU-accelerated particle-mesh interactions implemented in the QUOKKA code
› Inferring Stellar Densities with Flexible Models I: The Distribution of RR Lyrae in the Milky Way with $\textit{Gaia}$ DR3
› First galaxy ultraviolet luminosity function limits on dark matter-proton scattering
› Islands in Simulated Cosmos: Probing the Hubble Flow around Groups and Clusters
› Toward First-Principles Multi-Messenger Predictions: Coupling Nuclear Networks with GR Radiation-MHD in {\tt Gmunu}
› Properties of current sheets in two-dimensional tearing-mediated incompressible magnetohydrodynamic turbulence
› Revisiting the Radio Lateral Distribution Function: An amplitude dependence on $X_{\rm max}$ and primary composition
› Reproducing Abell 2744 with the HyperMillennium Simulation
› The SEEDZ Simulations: Methodology and First Results on Massive Black Hole Seeding and Early Galaxy Growth
› New multiprobe analysis of modified gravity and evolving dark energy
› Baryonic Feedback across Halo Mass: Impact on the Matter Power Spectrum
› A study of transients from ground-based surveys reveals new ultra-compact accreting white dwarf binaries
› The impact of Solar magnetic field configurations on the production of gamma rays at the Solar disk
› Ripples in the baryon to dark matter ratio in $\Lambda$CDM: implications for galaxy formation
› Machine learning for the early classification of broad-lined Ic supernovae
› Radio Morphing: Fast computation of inclined air shower radio emission
› Fates of the sub-stellar objects (FOSSO) I. Fates of the known brown dwarfs in main-sequence--BD binaries
› The Cosmological Simulation Code OpenGadget3 - Implementation of Self-Interacting Dark Matter
› Mock Observations of Multiple Stellar Populations in Tidal Streams of Palomar 5 for the Chinese Space Station Survey Telescope
› py5vec: a modular Python package for the 5-vector method to search for continuous gravitational waves
› Out of oxygen: Extremely metal-poor galaxy candidates identified at $2.5 < z < 6.5$ with deep JADES medium-band imaging
› EGS-z11-R0: a red, dust-rich galaxy at Cosmic Dawn
› Resonant scattering at the center of the galaxy cluster PKS 0745-191 with XRISM
› Cosmic Dipole as a Symmetry Response: From the Ellis--Baldwin Formula to Correlation Function Dipoles
› Constraints to the inert doublet model of dark matter with very high-energy gamma-rays observatories
› Astrophysical Black holes: An Explanation for the Galaxy Quenching
› (H)ALPing the 511 keV line: A thermal DM interpretation of the 511 keV emission
› Neutrino Telescope Event Classification on Quantum Computers
› Do plasmoids induce fast magnetic reconnection in well-resolved current sheets in 2D MHD simulations?
› Global Non-Axisymmetric Hall Instabilities in a Rotating Plasma
› Constraints on Genesis Cosmology from the Smeared Null Energy Condition
› Dynamic Black-hole Emission Tomography with Physics-informed Neural Fields
› Gauge-independent gravitational waves from a minimal dark $U(1)$ sector with viable dark matter candidates

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