Podchorazych 2, 30-084 Krakow, Poland.
tel.: (+48 12) 662 6301;
fax: (+48 12) 637 2243;
Obs. tel.: (+48) 502 113714
Mount Suhora Astronomical Observatory

view from south-east

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Latest preprints on astro-ph:
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Gender equality activities in Astronomical Society of Japan ›
Verifying the STIS Time Dependent Sensitivity Trends with the Primary CALSPEC Standards ›
The Effects of Complex Accretion Disk Geometry on Broadened Iron K$\alpha$ Lines ›
The Simons Observatory: Improved Cryogenic Struts for use in the Large Aperture Telescope Receiver ›
Euclid Quick Data Release (Q1). AstroVink: A vision transformer approach to find strong gravitational lens systems ›
Fast, Stable, and Physical: Hyperbolic, Magnetic Field-Aligned Diffusion in SPH ›
A SPHEREx Pipeline and Spectral Library for Ultracool Dwarfs ›
An Extended Parametric Model for Self-interacting Dark Matter Halos ›
Understanding HWO's Field of Regard and Characterization Requirement Trade Space with a Dynamic Observation Scheduling Algorithm ›
Differentiable Forward Modeling for Efficient and Accurate Shear Inference ›
Electromagnetic Precursors to Binary Neutron Star Mergers: Kinetic Simulations of Magnetospheric Flaring ›
Large language models are not the problem ›
CCAT: Silicon-Platelet Feedhorns for Submillimeter Wavelengths ›
Downward ultra-high-energy neutrino detection in the air with radio antennas at ground-based observatories ›
Backlighting the Cosmic Web with Fast Radio Bursts: An Anthology of Dispersion Measure Cross-Correlations with Large-Scale Structure and Baryon Tracers ›
FPGA-based Matched Filter Group Optimisation for SKA Pulsar Search Engine ›
Short timescale variation in the submillimeter flux of Sagittarius A* ›
Repeated Sunspot Light Bridge Jets Associated with Slipping Base Brightenings ›
The science from asteroid sample return missions ›
Formalizing Galaxy Population Evolution: Drift and Mergers as Transport Processes on Manifolds ›
Caustic Skeleton and the Local Cosmic Web: the Coma Cluster node and the Pisces-Perseus ridge ›
The circumstellar environment of the young, low-mass dipper star JH 223. Accretion and large-scale magnetic field topology ›
Asteroseismic rotation rates of hot subfwarf B stars hint at transient accretion from leftover common envelope matter ›
Non-LTE corrections for determinations of europium abundances in F-G-K stars in a broad metallicity range ›
Quiescent and flaring states of three active stars: V834 Tau, LQ Hya, and BY Dra ›
Signature of iron line profile from a Kerr-like wormhole ›
The Leiden/ESA Astrophysics Program for Summer Students (LEAPS) ›
A Morphological Identification and Study of Radio Galaxies from LoTSS DR2. I. The "Winged'' Radio Galaxies ›
Thermal background reduction for mid-infrared imaging by low-rank background and sparse point-source modelling ›
A study of the spatial evolution of the Radcliffe wave in a sample of young open star clusters ›
Testing $\Lambda$CDM with ANN-Reconstructed Expansion History from Cosmic Chronometers ›
Quiescent fractions in high-redshift galaxy groups reflect their hot-or-cold state of gas accretion ›
How lonely are the Binary Compact Objects Detected by the LIGO-Virgo-KAGRA Collaboration? ›
Spatially resolved metallicity and ionization in the merging system Gz9p3 at z=9.3 ›
Radial evolution of Alfv\'en wave Parametric Decay Instability in the near-Sun solar wind: Effects of Temperature Anisotropy ›
A Quasar--Companion System Without AGN Outflow at $z \sim 6$: The Case of PSO J083+11 ›
A homogeneous three-dimensional view of Molecular Cloud kinematics out to 2.5 kpc. Using Young Stellar Objects and Open Clusters as complementary tracers ›
Synchrotron polarization of anisotropic electron distribution in GRB prompt emission ›
The Effect of Mass Loss and Convective Overshooting on the Pre-Collapse Structure, Composition, and Neutrino Emission of Red Supergiants ›
MUSE-DARK III: The evolution of the radial acceleration relation at intermediate redshifts ›
Ultra-high-energy $\gamma$-ray imprints from PeV particles accelerated by supernova remnants ›
Constraints on the Primordial Black Hole Abundance using Pulsar Parameter Drifts ›
Variability of Sagittarius A* at 3 GHz on minute-scale with MeerKAT ›
Radiative feedbacks as drivers for quasi-periodic-oscillation activity in black-hole X-ray binaries ›
From core to envelope: revealing the deep dynamics of stars with two convective zones ›
The Sound of the Universe: A Resonant Gravitational Instability Driven by Baryon-Dark Matter Relative Drift ›
Exploring the diversity of kilonovae with 3D radiative transfer I. The polar direction ›
Dense Matter and Compact Stars in Strong Magnetic Fields ›
CosmicDancePro -- Measuring LEO satellite's orbital decay and network connectivity implications during solar storms ›
WAsp: The Wideband (W) Adaptive-Scale Pixel (Asp) Deconvolution Algorithm for Interferometric Imaging ›
Forecasting the occupancy of satellite megaconstellations in SKA observations ›
First Statistical Study of Over 100 Magnified Stellar Events at Redshift $z \approx 0.725$ with JWST ›
Reionization, UV Luminosity and 21$\,$cm Sensitivity to Primordial Magnetic Fields: Impact of Energy Losses ›
Simulation of a protoplanetary disk accretion activity due to a collision with a gas stream ›
Precision Analysis for $\boldsymbol{H_0}$ Using Upcoming Multi-band Gravitational Wave Observations ›
On the redshift evolution of the spin parameter in cosmological simulations ›
Describing the swdatatoolkit: A Space Weather Data Analysis Library ›
From Anomaly to Candidate Technosignature: The Threshold Problem of the Loeb Scale ›
Determination of the sensitivity of the DEAP-3600 experiment to supermassive charged gravitinos ›
Gradient-Produced Neutrinos ›
Cosmic-Ray Signatures of Annihilating and Semi-Annihilating Dark Matter via One-Step Cascades ›
Solar Reflection of Inelastic Dark Matter ›
Data-Driven Acceleration of Eccentricity Reduction for Binary Black Hole Simulations ›
Simulation-based Inference for Gravitational Waves from Binary Neutron Stars: Application of Summary Data from Heterodyning ›
Machine Learning for Multi-messenger Probes of New Physics and Cosmology: A Review and Perspective ›
Gauge-independent approach to inflation in quadratic gravity ›
The Decoupling of Binaries from Their Circumbinary Disks ›
On the Relationship of Dichotomy of Mars and Occurrence of Dust Devils with Crustal Magnetic Fields ›
The Large Smooth Patch on Comet 9P/Tempel 1: Remnant of a Recent Past Event ›
A Mysteriously Tight H$\alpha$-[O III] Correlation and Non-Case B Balmer Decrements Revealed by the Spectra from the James Webb Space Telescope NIRSpec Instrument ›
The Missing Hard Photons of Little Red Dots: Their Incident Ionizing Spectra Resemble Massive Stars ›
Probing dense environments around Sgr A* with S-stars dynamics ›
Cross-correlations between the CLAMATO Lyman-alpha forest and galaxies within the COSMOS field ›
Crosschecking Cosmic Distances from DESI BAO and DES SNe ›
Generalized Distributions of Host Dispersion Measures in the Fast Radio Burst Cosmology ›
$O_k$ null test with multi-task Gaussian processes: cosmic curvature and data compatibility ›
Most Rocky Sub-Neptunes are Molten: Mapping the Solidification Shoreline for Gas Dwarf Exoplanets ›
Anisotropic diffusion modeling of cosmic-ray lepton propagation ›
Comprehensive study of solar type II radio bursts and the properties of the associated shock waves ›
Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter ›
Magma Ocean Waves and Thermal Variability on Lava Worlds ›
Expanding the High-z Supernova Frontier: "Wide-Area" JWST Discoveries from the First Two Years of COSMOS-Web ›
Subsolar mass black holes from stellar collapse induced by primordial black holes ›
Probing Compact Objects in Wide-Orbit Binaries with Joint LAMOST LRS and MRS ›
Oxygen left behind: Atmospheric Enrichment due to Fractionation in Sub-Neptunes using BOREAS ›
Effects of the symmetry energy slope on magnetized neutron stars ›
The no-hair theorems at work in the tidal disruption event AT2020afhd ›
Probing Physics Beyond the Standard Model through Combined Analyses of Next-Generation Type Ia Supernova, CMB, and BAO Surveys ›
The Pristine HeII Emitter near GN-z11: Constraining the Mass Distribution of the First Stars ›
Automatic search for transiting planets in TESS-SPOC FFIs with RAVEN: over 100 newly validated planets and over 2000 vetted candidates ›
Big Bang Nucleosynthesis Constraints on the CCC+TL Cosmology ›
Multi-scale Gas Structure and Dynamics in an Extragalactic Central Molecular Zone ›
The GMRT archive atomic gas survey -- IV. Consistency of the dark matter halo perturbation parameter from morphological and kinematic lopsidedness of galaxies ›
JOYS: Launching and destruction of dust in protostellar jets. The case of BHR71-IRS1 with JWST/MIRI ›
VLTI-GRAVITY observations of blazars ›
X-Shooting ULLYSES: Massive stars at low metallicity XV. On the metallicity dependence of B-supergiant mass-loss rates ›
Sensing Gravity with Polarized Electromagnetic Radiation ›
Gravitational Wave Birefringence from Fuzzy Dark Matter ›
Consistent $N_{\rm eff}$ fitting in big bang nucleosynthesis analysis ›
A Compact Story of Positivity in de Sitter ›
Electron Heat Flux and Whistler Instability in the Earth's Magnetosheath ›
Dynamical response of twin stars to perturbations ›
Design of low-energy transfers in cislunar space using sequences of lobe dynamics ↓↑