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Astronomia w Krakowie
Photo: Halo, moon dogs and parhelic circle around the Moon
Halo, moon dogs and parhelic circle around the Moon
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 News from astronomynow.com
› 3I/ATLAS was born in the deep freeze
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RSS  Latest preprints on astro-ph:
› The Role of the Core in Setting Massive Neutron-Star Radii
› A Framework for Evaluating Forward Contamination Risk for Bio-ISRU Microorganisms
› Continuous Learning of Gravity Field Irregularities Around Small Bodies via Neural Hamiltonian ODEs
› An unresolved extreme warm infrared excess toward a nearby low-mass star
› Impact of galaxy intrinsic alignments on non-Gaussian weak lensing statistics for modified gravity
› Clustering-based halo mass assignment for high-redshift galaxies: method, validation, and application to JWST
› Constraining dark matter using 20-year INTEGRAL/IBIS observations I: Primordial black holes
› Little Red Dots are Direct-Collapse Black Hole-Forming Galaxies
› Reconsidering the role of bright and dark gravitational-wave standard sirens for cosmology
› Time-Integrated Searches for Sub-TeV Neutrino Sources with IceCube-DeepCore
› Resolved SED Modeling with JWST and ALMA: The Role of Stellar Mass Surface Density in Regulating Star Formation in Cosmic Noon Galaxies
› Galaxies in the first two billion years: Earlier formation and quenching with surface-density modulated star formation and feedback
› BAQARO: Tracing Stochastic Black Hole Growth Histories and Quasar Lightcurves in a Cosmological Context
› Unified modelling of broad and narrow optical-UV emission lines from massive black holes: interpreting high-redshift JWST observations
› The Role of Big Bang Nucleosynthesis in Joint Cosmological Analyses
› Long-term X-ray spectral analysis of Cygnus X-1 using AstroSat
› Which Type Ia supernova observables best indicate the ages of their progenitor stars?
› Probing Lorentz Invariance Violation in Cosmogenic Neutrino Propagation with KM3-230213A
› A Proliferated Space Architecture for Time-Domain Astrophysics
› Probabilistic characterization of blending with LSST and application to cluster lensing cosmology
› Hidden structures in the UHE sky: unveiling potential sources via spectral signatures
› NOEMA probes the [CII] and dust content in a 2175{\AA} UV Bump Galaxy at $z=7.1$
› Plasma Heating and Energization in Hot-Onset Flare Precursor Events
› Steepening Optical Slopes in Exoplanet Transmission Spectra with Charged Hazes
› OSIRIS-REx Returned a Pristine Sample of Asteroid Bennu: Takeaways from the Mission's Contamination Control and Knowledge Program
› Electromagnetic Probes of the Supernova Engine
› Mapping the Quasar Main Sequence in the UV range: A Connection with the UV Fe III Emission
› Stellar bar occurrence in TNG50 and TNG100: disentangling environmental effects and assembly history at z = 0
› High water D/H ratio of the interstellar object 3I/ATLAS is consistent with a low-metallicity origin
› A Localized Current-Sheet Magnetic-Diffusion and Heating Prescription for Ideal-GRMHD Simulations of M87*-like Accretion Flows
› Evolution of first-interaction second-harmonic anisotropy in cosmic-ray air showers
› A systematic study of the long-term mid-infrared color variations of Seyfert 1 galaxies
› KMT-2026-BLG-0083L: A Two-Jovian-Planet System Orbiting an M Dwarf Discovered by Microlensing
› Superoutbursts and Superhumps of Cataclysmic Variables observed with TESS
› The constrainability of galaxy positions in the $M_*$ -- SFR plane from SED fitting
› Magnetic Fields and Asymmetric Accretion in the Class 0 Protostellar System L1527 IRS
› Terminal instability of the Solar System triggered by stochastic solar mass loss
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› E-INSPIRE - II. Finding relics from wide-sky multi-band surveys: A proof-of-concept machine learning regression algorithm
› Optical Follow-Up of Two Spider Pulsar Candidates: An Irradiated Redback and a Possible Double Giant Impostor
› Heavy Seed Black Hole Growth in Metal-Enriched Halos through Disk-Induced Stellar Disruptions: A Semi-Analytical Modelling
› Large-Scale Latitude-time Relationships Between the Green-Line Corona and Sunspot Activity During Solar Cycles 18-24
› Plasmoid-Trapped Condensation Associated with a Transient Thermal-Instability-Like Process in Chromospheric Magnetic Reconnection
› Identification of Cosmic Chronometers in the GAMA Survey
› Limits on a Host Star around a Saturn-mass Free-floating Planet Candidate KMT-2024-BLG-0792/OGLE-2024-BLG-0516
› Probing Inflationary Origins of Primordial Black Holes with LIGO--Virgo--KAGRA O1--O4a data
› The influence of free-free absorption on the radio spectrum of Particle-Accelerating Colliding-Wind Binaries
› The Infrared Glow of Galactic Outskirts: A New Window with NASIM
› XMST: An Extended Minimum Spanning Tree Framework with Objective Fracture-Scale Selection
› Late-Time Evolution of the Massive Stellar Merger M101 OT2015-1
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› An efficient approach to resistive GRMHD simulations of binary neutron star mergers
› High-redshift supermassive black hole population from core-collapse in self-interacting dark matter halos
› The atomic C/O ratio of KELT-9b
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› The Nature of Small-Scale Perturbation Modes in a Nonstationary Self-Gravitating Disk
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› Big Bang For Your Helium Buck
› Implications of the LISA stochastic signal from eccentric stellar mass black hole binaries in vacuum
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› Accretion onto a moving black hole for stiff equations of state
› Path-Degenerate Quantum Interferometry for Decoherence Mitigation in Gravitational-Wave Detectors
› A semicoherent resampling method for long-transient gravitational wave searches with applications to subsolar-mass primordial black-hole binaries
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› Intrinsic pressure anisotropy in spherical Proca stars
› Constraints on Galactic Dark Photons from a DALI Prototype
› The DALI Haloscope: A Magnetized Phased Array Coupled to a Semi-Open Fabry--P\'erot Resonator
› The Wavelet Detection Filter: a real time unmodeled pipeline for gravitational wave transients, ranking coincidences with a graph neural network
› Reconstructing the Dark Matter Equation of State with Compact Object Inspirals
› \texttt{cWB-space}: A time-frequency transient-search pipeline for LISA
› Probing Two-dimensional Asymmetries of an Exoplanet Atmosphere from Chromatic Transit Variation
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› Gas distributions inside and around haloes in the alternative dark matter simulations AIDA-TNG
› ABCMB: A Python+JAX Package for the Cosmic Microwave Background Power Spectrum
› A Wide and Deep Exploration of Radio-detected Active Galactic Nuclei with Subaru HSC (WERGS). XIII. High-z Radio Quasar Selection from HSC--VLASS over $\sim1200$ deg$^2$
› The Heavy Tailed Non-Gaussianity of the Supermassive Black Hole Gravitational Wave Background
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› Hessian-based photometric substructure as an evolutionary tracer of OB cluster candidates in M31
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› Mass-Orbital Period Distribution of Massive White Dwarfs Formed Through Stable Mass Transfer
› The quasi-star model for Little Red Dots: potential and challenges
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› Identifying Kilonovae in the Presence of Optical Afterglow for the Wide Field Survey Telescope
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› The Non-Principal-Axis Rotation and Convex Shape Model of Earth Quasi-Satellite and the Target of China's Tianwen-2 Mission (469219) Kamo`oalewa
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› Milky Way Structure from Double White Dwarf Gravitational-Wave Sources
› Magnetising the quokka code with fast, second-order accurate, error-correcting schemes for magnetohydrodynamics on GPUs
› Testing Chemical Tagging with LAMOST: Intrinsic Abundance Dispersion of Subgiant Stars in the Galactic Disk
› From Stars to Waves: Non-deterministic Inference of Microlensed Gravitational Waves
› On the Theory of Bulk Viscosity of Cold Plasmas and Thermodynamics of Alkali-Noble Gas Cocktails
› Spectral sirens cosmology from binary black holes populations with sharper mass features
› Branching Universes
› Extreme, transient bursts of energy in the auroral ionosphere. I. Predictive radar tracking
› Orbital evolution of asymmetric binaries within accreting environments
› Enhanced electron-beam lithography to reduce the frequency scatter of 200-400 GHz superconducting microstrip resonators for on-chip filterbank spectrometers
› Oscillations of Dissipative Neutron Stars: The Impact of Hyperonic Reaction Rates
› Theoretical Aspects of Direct Waves in Kerr Black Holes: Pole-Splitting Method for Ringdown Analysis

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