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Astronomia w Krakowie
Photo: Moon and Jupiter over the small dome
Moon and Jupiter over the small dome
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Pressure
1001.9 hPa

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RSS  Latest preprints on astro-ph:
› Orbital Debris in Earth Orbit: Operations, Stability, Control, and Market Formation
› A Physical Classification of Exoplanet Thermal Environments: Stellar Irradiation versus Tidal Heating
› Derivation of the Kompaneets equation using the boost operator approach
› Investigating the radio emission in the Perseus cluster with LOFAR sub-80 MHz LBA
› Phase spirals across galactic disks I: Exploring dynamical influences on winding
› oMEGACat. X. Shedding light on the disrupted dwarf galaxy of Omega Centauri
› Deviations from the radial acceleration relation in the central galaxies of clusters, subclusters, and groups
› Direct Evidence for Stellar Initial Mass Function Variation in the Milky Way
› The Environments of Luminous Fast Blue Optical Transients: Evidence for a Compact Object and Wolf-Rayet Star Merger Origin
› The impact of disc disruption on Milky Way satellite counts
› II- A hydrodynamical CLONE of the Virgo cluster to confront observed and synthetic galaxy population twins in a dense environment
› Revealing the nature of the starburst galaxies in the $z=2.4$ overdensity HATLAS J0849
› Reducing cosmological degeneracies by combining multiple classes of LISA gravitational-wave standard sirens
› A velocity-dependent two-scale model for cosmic string networks with small-scale structure
› SPHEREx mapping of diffuse PAH and H II emission in the Galactic plane
› Magnetic flux systems involved in the May 2024 solar energetic events from AR 13664 inferred through coronal dimmings
› Radiation-ionization hydrodynamic simulations of AGN line-driven winds lead to transient shielding and BAL/UFO signatures
› No strong associations between eccentricity and orbital architecture in Kepler compact multis
› Large Variations Seen in First Ultraviolet Spectroscopic M33 Dust Extinction Curves
› MICONIC: JWST/MIRI-MRS reveals heavily reprocessed PAH emission in the circum-nuclear disc of Centaurus A
› Brightest Cluster Galaxy ellipticity as proxy for halo shape: Orientation bias, assembly bias, and potential selection effects in SZ-selected clusters
› The KPF-SLOPE Survey - Small, Compact Multi-Planet Systems Appear Spin-Orbit Aligned
› Benchmarking Astrochemistry Paradigms: Relative Absence of $\rm{C_6H_5CN^+}$ in the Diffuse ISM
› Estimation of the magnetic field strength from ALMA dust polarization in the protocluster G327.29
› The shortest detected intra-day variability of active galactic nuclei in TESS survey
› Thermally inflated accretors in post-mass transfer binaries: Abell 35 and its class revisited
› The Vera C. Rubin Observatory Data Preview 1
› The Role of Reconnection at Magnetic Separators in Complex Solar Flare Ribbons
› IXPE view of the Crab pulsar following the 17 July and 6 August 2025 glitches
› A transdimensional sampling framework for pulsar timing noise modelling
› Rigorous Formulation of Finite-Sample and Finite-Window Effects in Galaxy Clustering
› Near-Infrared and Optical Observations of SN 2024rbc: The First Early Detection of CO and Dust in a Type Ib Supernova
› SM-Net: Learning a Continuous Spectral Manifold from Multiple Stellar Libraries
› A generalized method for estimating solar wind speeds and densities using spectral broadening for a Kolmogorov turbulence spectrum
› A Long Stellar Stream in M83: Possible Connection Between XUV Disks and Minor Mergers?
› GalSyn I: A Forward-Modeling Framework for Synthetic Galaxy Observations from Hydrodynamical Simulations and First Data Release from IllustrisTNG
› RRAT J1541+4703: A Rotating Radio Transient Exhibiting Normal Pulsar States
› Imprints of tidal interactions on the stellar distribution of satellite galaxies: implications for dark matter deficient galaxies
› A Catalog of 1,408 Carbon-Enhanced Metal-Poor Stars from LAMOST DR11
› The annular gap model under a rotating dipole field approximation: simulating gamma-ray light curve
› Unifying the X-ray coronae and ultra-fast outflows: a PBI-enhanced outflow-based corona model for the inner accretion disc
› Ising noise filter: physics-informed filtering for particle detectors
› Simultaneous Multi-band Optical Follow-up Observations of a Gamma-Ray Flare in BL Lacertae
› ZIMPOL detects scattering polarization in He I D$_3$ during a solar flare
› Refractive multi-conjugate adaptive optics for wide-field atmospheric turbulence correction
› Perturbative and numerical study of nonlinear relativistic effects in weak lensing
› SS Cygni: An analysis of quasi-periodic oscillations in the range of 0.25h to 8h
› Gas dynamics around dust asymmetries in turbulent disks
› Core-Collapse Supernovae and their Gravitational Wave Signals: The Status of Theory and Modeling
› Stellar Variability and Distance Indicators in the Near-infrared in Nearby Galaxies. II. Pulsating Stars in the Carina Dwarf Spheroidal
› Connecting Meteorite Spectra to Lunar Surface Composition Using Hyperspectral Imaging and Machine Learning
› New Insights into Erg Chech 002 Analogues in the Main Belt from Near-Infrared Spectroscopy
› Impact of Antenna Structure and Orientation on Forward-Modelled Global 21 cm Signal Recovery
› Derivation of the injection spectrum of positrons and electrons from Geminga and Monogem
› Simulation of laser travel-time on Mercury for BELA
› Machine Learning-Based Classification of Active Galaxies and Estimation of Supermassive Black Hole Masses
› Artificial precession and instability in solar system and planetary simulations: analytic and numerical results
› Short-Term Turbulence Prediction for Seeing Using Machine Learning
› The VLT/ERIS grating vector Apodizing Phase Plate coronagraph
› Exoplanet Search and Characterization with the Proposed POET Canadian Space Mission
› Massive star clusters detected by JWST as natural birth places to form intermediate-mass black holes
› Probing Interacting Dark Sectors with upcoming Post-Reionization and Galaxy Surveys
› Multi-mission Investigation of X-ray Superorbital Modulation in the Supergiant High Mass X-ray Binary 4U 1538-52
› Dynamical Systems in Cosmology: Reviewing An Alternative Approach
› From friction scaling to an efficient method for estimating bubble wall velocity
› Unlocking HST's Stellar Treasure Trove: Stellar Activity Minima for HAT-P-11 Offer Prime Windows for Transmission Spectroscopy
› Stable black hole solutions with cosmological hair
› Dichroic Dual-Angle Refractor: Multi-Cell Huygens' Metasurface-Based Circuit Approximation
› Cosmology with Logarithmic Corrected Horizon Entropy According to the Generalized Entropy and Variable-G Correspondence
› Mars in the Australian Press, 1875-1899. 1. Interpretation, Authority and Planetary Science
› Radial Oscillations of Viscous Stars
› A rotating GUP black hole: metric, shadow, and bounds on quantum parameters
› The read-out electronics for the FLASH experiment
› Impact of muons on the bulk viscosity of neutron star matter metamodels
› Lyman-$\alpha$ Forest Constraint on Dark Matter from Dark Sector Decay
› Probing small-scale anisotropic inflation with stochastic gravitational-wave background
› Quadratic energy-momentum squared gravity: constraints from big bang nucleosynthesis
› Refining Galactic primordial black hole evaporation constraints
› Advancing Stellar Streams as a Dark Matter Probe -- I: Evolution of the CDM subhalo population
› SZ Lyncis: A Non-Accreting Neutron Star-delta Scuti Binary Candidate Discovered via Dynamics and Asteroseismology
› Performance of the Gamma-ray Transient Monitor at the IHEP Electron-Beam Facility
› Search for spatial coincidence between magnetars and IceCube detected neutrinos
› Bayesian Component Separation for DESI LAE Automated Spectroscopic Redshifts and Photometric Targeting
› Jet-environment interaction after delayed collapse in binary neutron star mergers
› Investigating MAXI J1752-457 with NuSTAR in the aftermath of a superburst
› Modelling $\delta$ Scuti pulsations: A new grid of p, g, and f modes across pre-main-sequence to post-main-sequence evolution
› Bulk viscous cosmological models with a cosmological constant: Observational constraints
› HET/HPF observations of Helium in warm, hot, and ultra-hot Jupiters
› First direct detection of an RR Lyrae star conclusively associated with an intermediate-age cluster
› Semianalytical Accretion-Tracer Emission: Forming Planets Are Intrinsically Faint
› A Detailed Chemical Analysis of the Red Giant Orbiting the Black Hole $Gaia$ BH3: From Lithium to Thorium
› Equation-of-state-informed pulse profile modeling
› Redshift-Frame Systematics and Their Impact on the Hubble Constant from Pantheon+ Supernovae
› Simulated Rotation Measure Sky from Primordial Magnetic Fields
› Mass transfer stability for AM CVn binaries with white dwarf donors
› Voyager 1 Data Reveals Signatures of the Local Gas and Cosmic-Ray Source Distributions
› Portrait of a Galaxy on FIRE: Is the $\alpha$-bimodality a natural consequence of inside-out disc growth in a hierarchical formation scenario?
› Why Machine Learning Models Systematically Underestimate Extreme Values II: How to Fix It with LatentNN
› Gas rotation and turbulence in the galaxy cluster Abell 2029
› Clumps in High-Redshift Galaxies: Mass Scaling and Radial Trends from JADES
› BE Lyncis is not a Black Hole Binary: Lessons From Gaia and Hipparcos Astrometry
› Ridged Lagrangian Perturbation Theory (RLPT)
› Waveforms and Fluxes of Generic Extreme-Mass-Ratio Inspirals with a Spinning Secondary
› VHE gamma-ray intranight variability from BL Lacertae during the extreme flaring state of 2022
› On the cosmology dependence of the cluster weak-lensing mass bias
› Axionlike dark-matter winds driven by galactic baryon redistribution
› A large population of over-massive black hole quasars at z=0.3-0.8 revealed by eROSITA
› Low-Frequency Stochastic Gravitational-Wave Background in Gaia DR3 catalogue
› More accurate gravitational wave backgrounds from cosmic strings
› PT2GWFinder: A Package for Cosmological First-Order Phase Transitions and Gravitational Waves
› Primordial black hole formation in matter domination
› Bayesian power spectral density estimation for LISA noise based on penalized splines with a parametric boost
› Do plasmoids induce fast magnetic reconnection in well-resolved current sheets in 2D MHD simulations?
› Thermal Vacuum Cosmology Explains Hubble Tension

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