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Astronomia w Krakowie
Photo: Międzynarodowa Stacja Kosmiczna i Księżyc z halo
Międzynarodowa Stacja Kosmiczna i Księżyc z halo
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RSS  Latest preprints on astro-ph:

› The Real-Time Data Processor Framework for Data Handling and Analysis of High-Energy Instruments
› Dynamical Friction Constraints on the Dark Matter Hypothesis Across Astronomical Scales
› Igniting galaxy formation in the post-reionization universe
› Probing the dawn of galaxies: star formation and feedback in the JWST era through the GAEA model
› Hot accretion onto spiral galaxies: the origin of extended and warped HI discs
› Dark Matter in White Dwarfs: Implications for Their Structure
› Making the most of pure parallels: Machine learning augmented photometric redshifts for sparse JWST filter sets
› Effects of density stratification on Rossby waves in deep atmospheres
› Photon Orbit Signatures in Spectra of Black Hole Accretion Disks
› Do Planets Affect the Behavior of the Long-term Solar Activity?
› Stellar Evolution with Radiative Feedback in AGN Disks
› Energy-dependent SEP Fe/O abundances during the May 2024 superstorm
› Event Reconstruction for Radio-Based In-Ice Neutrino Detectors with Neural Posterior Estimation
› Revealing Hidden Cosmic Flows through the Zone of Avoidance with Deep Learning
› Spectral Diversity in Type Ibn Supernovae and the Large Host Offset of SN2024acyl
› Origin and Evolution of the $\Omega$ Structure in the Head-Tail Radio Galaxy of Abell 3322
› Non ideal Transport Processes in the Solar Atmosphere
› SOFIA FEEDBACK Survey: The Eagle Nebula in [C II] and Molecular Lines
› Cosmic voids and the kinetic analysis. V. Hubble tension, the cosmological constant and aperiodic filaments
› Ultra-Diffuse, Ultra-Different: Observed vs. Simulated Ultra-Diffuse Galaxies Live in Fundamentally Different Halos
› Low redshift observational constraints on dark energy models using ANN - CosmicANNEstimator
› Super amplification of lunar response to gravitational waves driven by thick crust
› Early evidence for isotropic planetary obliquities in young super-Jupiter systems
› Exploring Cosmological Constraints of the Void-Lensing Cross-Correlation in the CSST Photometric Survey
› Machine-Learning Estimation of Energy Fractions in MHD Turbulence Modes
› Neural Network identification of Dark Star Candidates. I. Photometry
› Neural Network identification of Dark Star Candidates. II. Spectroscopy
› Limiting Eccentricity in Restricted Hierarchical Three-Body Systems with Short-Range Forces
› TESS and ground-based observations of WZ Sge-type dwarf novae in outburst
› Hadronic Processes in Advection-Dominated Accretion Flow as the Origin of TeV Excesses in BL Lac Objects
› NANOGrav 15-year gravitational-wave signals from binary supermassive black-holes seeded by primordial black holes
› Partial Null Point Reconnection of an Eruptive Filament
› 3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae
› Revealing an Oscillating and Contracting Compact Corona near the Event Horizon of the Supermassive Black Hole in 1ES 1927+654
› Cepheid Metallicity in the Leavitt Law (C- MetaLL) survey: IX: Spectroscopic detection of rare earth Dysprosium, Erbium, Lutetium and Thorium in Classical Cepheids
› Constraining gravity with the decay rate of cosmological gravitational potential
› The Initial mass function of field stars with mass $\leq$ 1 $M_{\odot}$ varies with metallicity
› Discovery of a 9.67-s pulsar in an ultraluminous X-ray source in NGC 4631 with XMM-Newton
› Massive stars exploding in a He-rich circumstellar medium XII. SN 2024acyl: A fast, linearly declining Type Ibn supernova with early flash-ionisation features
› An alternative theory of magnetic flux tubes in strong fields via axion origin photons
› The Apache Point Observatory extra-Galactic Evolution Experiment (APOeGEE): Chemical Abundance Trends for Seven Dwarf Spheroidal Galaxies in the APOGEE Survey
› Magnetohydrodynamic simulation assessment of a potential near-ultraviolet early ingress in WASP-189b
› Spectroscopic analysis of hydrogen and silicon in bright fireballs: New insights into meteoroid composition
› Transiting Exoplanets from Sharjah Astronomical Observatory (SAO-M47): The Exoplanet HAT-P-25b Using L and V Filters
› Artificial Precision Polarization Array: Sensitivity for the axion-like dark matter with clock satellites
› How the gradient of $M_{\rm d}$ versus UV field strength yields insights into the ages of protoplanetary disc populations
› Dust Collisions in Protoplanetary Disks: Atomic Simulations of the Surface Free Energy
› Cutana: A High-Performance Tool for Astronomical Image Cutout Generation at Petabyte Scale
› The TeV emission of 3C273: inverse Compton radiation from shear-accelerated high-energy electrons in the large-scale jet?
› The AGORA High-resolution Galaxy Simulations Comparison Project. X: Formation and Evolution of Galaxies at the High-redshift Frontier
› Study the nature of dynamical dark energy by measuring the CMB polarization rotation angle
› The ALMA-ATOMS-QUARKS survey: Resolving a chemically rich massive protostellar outflow
› Environmental effects in stellar mass gravitational wave sources II: Joint detections of eccentricity and phase shifts in binary sub-populations
› 2D unified atmosphere and wind simulations for a grid of O-type stars
› Parameterizing Noise Covariance in Maximum-Likelihood Component Separation
› Automatic detection of CMEs using synthetically-trained Mask R-CNN
› The Pre-Outburst Properties of the FU Ori Object HBC 722
› Peculiarities in the infrared emission of PAH-C$_{60}$ adducts
› Addressing the DESI DR2 Phantom-Crossing Anomaly and Enhanced $H_0$ Tension with Reconstructed Scalar-Tensor Gravity
› Dynamical Masses of Young Stellar Multiple Systems with the VLBA (DYNAMO-VLBA)
› $\texttt{unimpeded}$: A Public Grid of Nested Sampling Chains for Cosmological Model Comparison and Tension Analysis
› Intermittency in Collisionless Large-Amplitude Turbulence
› On the Exoplanet Yield of Gaia Astrometry
› KGB-evolution: a relativistic $N$-body code for kinetic gravity braiding models
› Dark Energy Survey Year 3 results: Simulation-based $w$CDM inference from weak lensing and galaxy clustering maps with deep learning. I. Analysis design
› Magnetic Field-Line Curvature and Its Role in Particle Acceleration by Magnetically Dominated Turbulence
› Boson Stars Hosting Black Holes
› Quadrature-witness readout for backscatter mitigation in gravitational-wave detectors limited by back-action
› Astrophysical Constraints on Charged Black Holes in Scalar--Tensor--Vector Gravity
› Upgrade of Super-Kamiokande with Gadolinium
› Probing Gravitational Wave Speed and Dispersion with LISA Observations of Supermassive Black Hole Binary Populations
› Observational Constrains on the Sgr A$^*$ Black Hole Immersed in a Dark Matter Halo: Shadow and S2 Star Orbit
› Accelerated Sequential Posterior Inference via Reuse for Gravitational-Wave Analyses
› Novel Numerical Methods for Accurate Space Thermal Analysis: Enforcing View Factors and Modeling Diffuse Reflectivity
› Mitigating effects of nonlinearities in homodyne quadrature interferometers
› Equivalence of scalar-tensor theories and scale-dependent gravity
› Effective matter sectors from modified entropies
› On the Bondi accretion of a self-interacting complex scalar field
› Demonstrating Agreement between Radio and Fluorescence Measurements of the Depth of Maximum of Extensive Air Showers at the Pierre Auger Observatory
› Radio Measurements of the Depth of Air-Shower Maximum at the Pierre Auger Observatory
› The Most Energetic Transients: Tidal Disruptions of High-Mass Stars
› Astrophysical assumptions and equation of state framework have larger impact on equation of state inference than individual neutron star observations
› Coronal hole picoflare jets are progenitors of both fast and Alfv\'enic slow solar wind
› JWST PRIMER: A deep JWST study of all ALMA-detected galaxies in PRIMER COSMOS -- dust-obscured star-formation history back to z $\simeq$ 7
› Cosmology with supernova Encore in the strong lensing cluster MACS J0138$-$2155: photometry, cluster members, and lens mass model
› Comprehensive JWST+ALMA Study on the Extended Ly$\alpha$ Emitters, Himiko and CR7 at $z\sim 7$: Blue Major Merger Systems in Stark Contrast to Submillimeter Galaxies
› Higher-Order Mean-Motion Resonances Can Form in Type-I Disk Migration
› Black Hole Survival Guide: Searching for Stars in the Galactic Center That Endure Partial Tidal Disruption
› Starlight from JWST: Implications for star formation and dark matter models
› Introducing the Descriptive Parametric Model: Gaseous Profiles for Galaxies, Groups, and Clusters
› Non-minimal light-curvature couplings and black-hole imaging
› Probing the accretion geometry of black hole X-ray binaries: A multi-mission spectro-polarimetric and timing study
› Testing scalar dark matter clumps with Pulsar Timing Arrays
› Testing Coasting Cosmologies with Large-Scale Structure Growth
› Broadband Low-Resolution Spectrograph - SpectrumMate LR
› An investigation into correlations between FRB and host galaxy properties
› The validity of separate-universe approach in transient ultra-slow-roll inflation
› Quantitative Morphology of Galactic Cirrus in Deep Optical Imaging
› Cosmic Cartography II: completing galaxy catalogs for gravitational-wave cosmology
› A Systematic Search for AGN Flares in ZTF Data Release 23
› Measuring the splashback feature: Dependence on halo properties and history
› Hubble constant constraint using 117 FRBs with a more accurate probability density function for ${\rm DM}_{\rm diff}$
› MrMARTIAN: A Multi-resolution Mass Reconstruction Algorithm Combining Free-form and Analytic Components
› Glitch analysis and asteroseismic modelling of subgiant $\mu$ Herculis: confirming and interpreting the $\Gamma_1$ peak as the helium glitch
› A Dark Matter Model with Quadratic Equation of State: Background Evolution and Structure Formation
› The SPAr burning: proton captures powering carbon-oxygen shell mergers in massive stars
› Optical/infrared observations of the extraordinary GRB 250702B: a highly obscured afterglow in a massive galaxy consistent with multiple possible progenitors
› The Tidal Torque Theory Revisited: II. Rotational Halo Properties
› The Sunburst Arc with JWST. IV. The importance of interaction, turbulence, and feedback for Lyman-continuum escape
› Dependency of the Bar Formation Timescale On The Halo Spin
› Neural Posterior Estimation for Cataloging Astronomical Images from the Legacy Survey of Space and Time
› Order-by-order Modeling of Exoplanet Radial Velocity Data
› Pre-perihelion Development of Interstellar Comet 3I/ATLAS
› Mass-radius relationship and gravitational wave emission from magnetized spheroidal quark stars
› The cosmological analysis of DES 3$\times$2pt data from the Effective Field Theory of Large-Scale Structure
› Stellar Spectroscopy Using Diffraction Grating, CMOS Monochrome Sensor, and Reflecting Telescopes
› Properties of Carbon-rich AGB Stars in the LMC and the Milky Way
› Determining the impact of post-main-sequence stellar evolution on the transiting giant planet population
› Euclid Quick Data Release (Q1). The average far-infrared properties of Euclid-selected star-forming galaxies
› Study of Four nulling pulsars with FAST
› First Associated Neutrino Search for a Failed Supernova Candidate with Super-Kamiokande
› The first year of LISA Galactic foreground
› Prospects for Probing Sub-GeV Leptophilic Dark Matter with the Future VLAST
› Graviton-photon conversion in stochastic magnetic fields
› Inflation models selected by the swampland distance conjecture with the Lyth bound
› Nuclear chiral density wave in neutron stars?
› Equation of state for hyperonic neutron-star matter in SU(3) flavor symmetry
› Ionospheric responses over the Antarctic region to Intense Space Weather events: Plasma Convection vs. Auroral Precipitation

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