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

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Latest preprints on astro-ph:
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Oort Cloud Bombardment by Dark Matter ›
Tidal disruption event rates across cosmic time: forecasts for LSST, Roman, and JWST and their constraints on the supermassive black hole mass function ›
How Do Disk Galaxies Form? ›
The GMRT archive atomic gas survey -- III. Comparative Study of Dark Matter Halos in Nearby Galaxies ›
Wiggling Through the ICM: Multi-Resolution Radio Imaging of a Tailed Radio Galaxy in MACS J1354.6+7715 ›
Classifying white dwarfs from multi-object spectroscopy surveys with machine learning ›
Establishing a relationship between the cosmological 21 cm power spectrum and interferometric closure phases ›
Abundant hydrocarbons in a buried galactic nucleus with signs of carbonaceous grain and polycyclic aromatic hydrocarbon processing ›
Multi-spin stellar velocity maps of the most massive galaxies ›
Clustering of z~6.6 Quasars and [O III] Emitters Constrains Host Halo Masses and Duty Cycles in 25 ASPIRE Fields ›
Differentiable Stochastic Halo Occupation Distribution with Galaxy Intrinsic Alignments ›
ASPIRE: The Environments and Dark Matter Halos of Luminous Quasars in the Epoch of Reionization ›
Testing black hole space-times with the S2 star orbit: a Bayesian comparison ›
The Impact of Galaxy Formation on Galaxy Biasing, and Implications for Primordial non-Gaussianity Constraints ›
Complex hydrogen chemical equilibrium and Gaia low mass problem in cool white dwarfs ›
The CON-quasar stage of IRAS 07251-0248 E ›
Wide sdB binaries. I. Orbital and atmospheric parameters ›
Modeling the recent interactions between the Magellanic Clouds and Milky Way ›
Dynamics of the coronal magnetic field in the 2022-10-02 X-class flare ›
Detailed TESS-Based Light Curve Modeling and Fundamental Parameter Estimation of 27 W UMa-Type Contact Binaries ›
On the forced orbital plane of the Hilda asteroids ›
ICM-SHOX III. The case of MACS J0018.5+1626, a radio relic that looks like a radio halo? ›
Wising up to CatWISE: using simulation-based inference to interpret the ecliptic bias and confirm the cosmic dipole excess ›
Shocks, Winds, and a Torus: The Large Binocular Telescope Interferometer (LBTI) Resolves the Active Nucleus of NGC 4151 ›
The Galaxy Bias Profile of Cosmic Voids:A Comparison of Void Finders ›
Growth of High-Redshift Quasars from Fermion Dark Matter Seeds ›
Thermal Eclipse Observation of the Young Hot Neptune AU Mic b with Spitzer ›
Searching for gravitational waves from compact binary mergers powering long gamma-ray bursts during LIGO-Virgo-KAGRA's O3 run ›
Rotating strange dwarfs and their indistinguishability from white dwarfs ›
A gamma-ray-emitting blazar B3 1239+376 at z = 3.82 identified in a multi-wavelength context ›
ALMA 873 $\mu$m Polarization Observations of the PDS~70 Disk ›
Evolution of cataclysmic variables under different magnetic braking prescriptions ›
IFU Spectroscopic Study of the Planetary Nebula Abell 30: Mapping the Ionisation and Kinematic Structure of the Inner Complex ›
An Accretion-Modulated Internal Shock Model for Long GRBs ›
First Detailed MeerKAT Imaging Spectroscopy of a Solar Flare ›
Galactic seismology: can a disc-crossing impulse explain the large-scale perturbations in the Milky Way's disc? ›
Sulfur Enrichment in Close-in Exoplanet Atmospheres Induced by Pebble Drift across the Salt Line ›
Fractal dimension of the cosmic web with different galaxy types ›
B-field Orion Protostellar Survey (BOPS). IV: The Relative Orientation Between Magnetic Fields and Density Structures in Young Protostellar Envelopes ›
The sub-arcsecond ILT view of the Bo\"{o}tes Deep Field: A link between low-frequency kiloparsec radio morphology and AGN driven ionised outflows ›
Dark Energy After DESI DR2: Observational Status, Reconstructions, and Physical Models ›
Habitability of Tidally Heated H$_2$-Dominated Exomoons around Free-Floating Planets ›
A Chemistry-First Centered Icy Chemical Inventory of Protostellar Sources with JWST ›
ELFO: A Python package for emission line fitting optimization in integral field spectroscopy data ›
The Double-Burst Nature and Early Afterglow Evolution of Long GRB 110801A ›
Mergers Drive Structural Complexity but Not Starbursts in Lyman-$\alpha$ Emitters at $3 < z < 4$: A JWST Spatially Resolved View ›
Probing Compact Objects in Wide-Orbit Binaries with Joint LAMOST LRS and MRS ›
The Correlation Length of Turbulence in Magnetic Clouds ›
Nano-particle Transition Matrix code implementation ›
Effects of Dynamo-Generated Large-Scale Magnetic Fields on the Surface Gravity ($f$) Mode ›
Forecast on $f(R)$ Gravity with HI 21cm Intensity Mapping Surveys ›
Exploring the central engines of gamma-ray bursts from prompt light curves ›
Particle acceleration signatures in the time-dependent one-zone synchrotron self-Compton model of blazar flares ›
XGAP with uGMRT I: Old AGN plasma in merging galaxy groups ›
MESS: Multi-Epoch Spectroscopic Solver for Detecting Double-Lined Systems ›
Coalescence Forensics: Weighing the Hosts of Hierarchical Binary Black Hole Mergers ›
The kinematic cosmic dipole beyond Ellis and Baldwin ›
Relativistic Dynamics and Bondi-Hoyle-Lyttleton Accretion onto Rotating Embedded Black Hole Models ›
Momentum-conserving self-gravity in the phantom smoothed particle hydrodynamics code. Parallel dual tree traversal for the symmetric fast multipole method ›
MIGHTEE/COSMOS-3D: The discovery of three spectroscopically confirmed radio-selected star-forming galaxies at z=4.9-5.6 ›
Bayesian imaging inverse problem with scattering transform ›
Photometric variability of nitrogen-rich Wolf-Rayet stars in Magellanic Clouds with OGLE ›
Microlensing constraint on Primordial Black Hole abundance with Subaru Hyper Suprime-Cam observations of Andromeda ›
Predicting galaxy bias using machine learning ›
The Effects of Non-ideal Mixing in Planetary Magma Oceans and Atmospheres ›
Early growth of massive black holes in dynamical dark energy models with negative cosmological constant ›
The JWST EXCELS survey: The ages and abundances of $3 ›
Long-term timing of the relativistic binary PSR J1906+0746 ›
Tracing AGN Feedback Power with Cool/Warm Outflow Densities: Predictions and Observational Implications ›
Improved Heavy Dark Matter Annihilation Search from Dwarf Galaxies with HAWC ›
Cosmographic parameters from current and next-generation gravitational wave detectors ›
Does Cosmology require Hermiticity in Quantum Mechanics? ›
Time lags and their association with the Boundary Layer structure in a Z source GX 349+2 ›
Direction-dependent calibration with image-domain gridding ›
Testing cosmic anisotropy with cluster scaling relations ›
Water absorption confirms cool atmospheres in two little red dots ›
ACT DR6+Planck impact on inflation with non-zero vacuum expectation value and the post-inflationary behavior ›
Relic of quadrupole deformation produced in a hot neutron star era ›
Impact on Inferred Neutron Star Equation of State due to Nonlinear Hydrodynamics, Background Spin, and Relativity ›
Suppression of Gravitational-Wave Echoes in Diffeomorphism-Invariant Nonlocal Gravity ›
Intereses convergentes: los a\~nos previos a la visita de Einstein a la Argentina en 1925 ›
Simulating first-order phase transition during inflation ›
An approximate Kappa generator for particle simulations ›
Induced-Gravity Higgs Inflation in Palatini Supergravity Confronts ACT DR6 ›
On the stability of viscous Riemann ellipsoids ›
Detecting gravitational wave background with equivalent configurations in the network of space based optical lattice clocks ›
Early-universe constraints on the electron mass ›
Mesoscopic chemical potentials across the (hyper)nuclear landscape ›
deci-Hz Gravitational Wave Observations on the Moon and Beyond ›
Foreground removal and 21 cm signal estimates: comparing different blind methods for the BINGO Telescope ›
Impact of Interacting Dark Energy on the Growth of Matter Density Perturbations: Observational Constraints from DESI and Multi-Probe Data ›
Orbital eccentricity in a neutron star - black hole binary merger ›
Spins of Black Holes in X-ray Binaries and the Tension with the Gravitational Wave Measurements ›
Orbital Eccentricity and Spin-Orbit Misalignment Are Evidence that Neutron Star-Black Hole Mergers Form through Triple Star Evolution ›
Stabilizing simulation-based cosmological Fisher forecasts: a case study using the Voronoi volume function ›
Characterizing Density and Gravitational Potential Fluctuations of the Interstellar Medium ›
Resolving Black Hole Family Issues Among the Massive Ancestors of Very High-Spin Gravitational-Wave Events Like GW231123 ›
Phantom crossing or dark interaction? ›
Magnetic Flux Emergence in Binary Neutron Star Remnants ›
On the synergetic use of Ariel and JWST for exoplanet atmospheric science ›
Resonant W and Z Boson Production in FSRQ Jets: Implications for Diffuse Neutrino Fluxes ›
Search for neutrino emission from blazar $\gamma$-ray flares accounting for possible neutrino time delays ›
Gravitational Wave Spectral Shapes as a probe of Long Lived Right-handed Neutrinos, Leptogenesis and Dark Matter: Global versus Local B-L Cosmic Strings ›
A Modified 3D Biconical Outflow Model: Spatial Constraints on AGN-driven Outflows ›
Interacting binaries on the Main Sequence as in-situ tracers of mass transfer efficiency and stability ›
Large-Scale Galaxy Correlations from the DESI First Data Release ›
Connecting Star Formation in the Milky Way and Nearby Galaxies -II. An Observationally Driven Analytical Model for Predicting Cloud-Scale Star Formation Rates ›
The spectrum of $n_s$ constraints from DESI and CMB data ›
An Active Galaxy Cluster Merger at Cosmic Noon Revealed by JWST Weak Lensing and Multiwavelength Probes ›
Fast rotations in galaxies at cosmic noon indicate central concentration of stars, dark matter or massive black holes ›
Distinct Rotational Evolution of Giant Planets and Brown Dwarf Companions ›
A first GLIMPSE into star clusters populations across cosmic time ›
Fast Magnetoacoustic Wave Behavior within Gravitationally Stratified, Magnetically Inhomogeneous Media ›
Prompt cusps in hierarchical dark matter halos: Implications for annihilation boost ›
The FLAMINGO Project: Exploring the X-ray--cosmic-shear cross-correlation as a probe of large-scale structure ›
An emulator for the ionizing photon mean free path in ultra-high resolution simulations: the implications of mean free path measurements for the reionization history ›
Gravitational Waves from Feebly Interacting Particles in a First Order Phase Transition ›
Twisted magnetar magnetospheres: a class of semi-analytical force-free non-rotating solutions ›
Dark-Matter-Enhanced Probe of Relic Neutrino Clustering ›
Importance of Shot Noise in the Search for an Isotropic Stochastic Gravitational-Wave Background with Next Generation Detectors ›
Gauge Dependence of Scalar-Induced Gravitational Waves from Isocurvature Perturbations: Analytical Results ›
WIMP Freeze-out dynamics under Tsallis statistics ›
Misalignment dynamics of Scalar Condensates with Yukawa coupling: Particle and Entropy Production ›
Coordinate Systems and Transforms in Space Physics: Terms, Definitions, Implementations, and Recommendations for Reproducibility ↓↑