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

Big Dipper over the dome

S Webcam

N Webcam

S Sky
Temperature
6.6 °C
Humidity
58%
Wind
0.0 km/h
Pressure
1013.4 hPa

Moon
Latest preprints on astro-ph:
›
Spatially Resolved AGN Ionization and Star Formation at Cosmic Noon with JWST/JEMS ›
Geomagnetic Storm Impacts On The Ionosphere Over T\"urkiye During Solar Cycle 25: Focusing On The May 2024 Storm ›
Probabilistic neural network approach to determining parameters of eclipsing binaries ›
Constraints on the Galactic Chemical Evolution of $^3\rm{He}$ ›
Tree-ring structure of Galactic bar resonance in N-body simulations ›
Low-mass Active Galaxies in the SAMI Galaxy Survey with Spatially-resolved Spectroscopy ›
Euclid preparation. Non-Gaussianity of 2-pt statistics likelihood: Parameter inference with a non-Gaussian likelihood in Fourier and configuration space ›
Three Thousand Motion-Confirmed L and T Dwarf Candidates from the Backyard Worlds:~Planet 9 Citizen Science Project ›
Calibrating Photometric Mid-Infrared Star Formation Rates for JWST ›
Analysing Turbulent Energy Cascade in a Coronal Mass Ejection using Empirical Mode Decomposition ›
The unusually red delay spectrum of the low-mass black hole AGN NGC\,4051 as revealed by intensive continuum reverberation mapping with the Las Cumbres Observatory ›
Low-mass failed supernovae and the $10\,M_{\odot}$ peak in the merging black hole mass distribution ›
Galaxy formation in the first billion years ›
The Cosmic Web in the DESI Early Data Release: A Probabilistic Environment Catalog ›
Insights from GRBs for optical follow-up of gravitational wave counterparts ›
Impacts of Voids, Line of Sight Interactions, and Local Emission Environment on Detectability of Gamma-Ray AGN ›
The velocity field of our Milky Way outer stellar halo based on DESI DR2 ›
The Galactic Halo Rotation by Weyl Incorporated Gravity ›
Unusually Hot Interiors Could Reconcile the Missing Methane Problem for Warm-to-Hot Exoplanets with Hydrogen Atmospheres ›
Smoluchowski Coagulation Equation and the Evolution of Primordial Black Hole Clusters ›
Cosmological Constraints on the Generalized Uncertainty Principle from Redshift-Space Distortions ›
Estimates of the Dynamic Characteristics of Binary Systems for Traversable Wormholes Search ›
Diverse lifestyles of bar-like galaxies and their coevolution with the brightest galaxy in the most massive cluster of TNG50 ›
Spectroscopic Case Studies of Four Long-duration Transition-region Explosive Events ›
Heating of a plasma sheet in nonequilibrium ionization with nonthermal electrons ›
SN2024abfl: A Low-Luminosity Type IIP Supernova at the Low-Mass End of Core Collapse ›
The impact of the eROSITA bubbles on Galactic cosmic-ray transport ›
The Real and Pseudo Dispersion Measures of FRB~20220912A ›
Milky-Way-like stars in a galaxy core 8 billion years ago revealed by gravitational lensing ›
Asteroseismic Diagnostics for Red Giants with Kepler: Measuring epsilon and Small Frequency Separations in 16,000 Stars ›
CORSIKA 8: A General Framework for Particle Cascade Simulations ›
Spectropolarimetry of the changing-look active galactic nucleus NGC 1566 and its potential link to supermassive black hole binaries ›
Gaussian Process Inference of Stochastic Magneto-Active Dynamics and Viscosity in Swift J1727.8-1613 ›
Geant4-IcyMoons: Simulating Electron Interaction Physics in Irradiated Astrophysical Ices ›
No evidence for dynamical dark energy from the Combo correlation of GRBs ›
Multiplicity of Massive stars in the Milky Way (M3W). I. Project description, UNWIND, application to GLS 11 448, and DIB catalog ›
SDSS J153231.80+420342.7: a triple black hole candidate with a close binary black hole ›
Non-minimally coupled quintessence with sign-switching interaction ›
Consistency relations of amplitude and phase fluctuations of gravitational waves magnified by strong gravitational lensing ›
A research roadmap for assessing the feasibility of warming Mars ›
GECAM discovery of a peculiar magnetar X-ray burst (MXB 221120) from SGR J1935+2154 associated with a fast radio burst ›
Revealing the neutrino mass through persistent homology of the cosmic web ›
Magneto-Active Environments in Pulsar Binaries with the MeerKAT Telescope: I. Pulsar sample and their basic properties ›
Hot Rocks Survey V: Secondary Eclipse Photometry of GJ 3473 b with JWST/MIRI ›
Possible Reforms of the Tibetan Lunisolar Calendar ›
Plummer Dark Matter Black Hole with Topological Defects: Shadow, Greybody Factors, Quasinormal Modes, and Thermodynamics ›
A framework for creating galaxy models in the geometry of the conservation group with dark matter halos and flat rotation curves ›
Lights, Camera, Axion: Tracing Axions from Supernovae in the Diffuse $\gamma$-ray Sky ›
Influence of tides and self-gravity on Ultra-Light Dark Matter Bounds from Dwarf Galaxies ›
Is Gravity Always Enough to Yield a Classical Universe? ›
High-Frequency Gravitational Wave Constraints from Graviton-Photon Conversion in the M87 Galaxy ›
Supermassive Primordial Black Holes from a Catalyzed Dark Phase Transition for Little Red Dots ›
Bipartite Solution to the Lithium Problem ›
Vacuum bubbles from cosmic ripples ›
Nonperturbative suppression of beyond-General-Relativity effects in quadratic gravity ›
High-power Test and System Integration of Direct RF Sampling Based LLRF Control and Monitoring System for S-Band Accelerating Structures ›
Small-Scale Dynamo for Full Spectrum of Hydrodynamic Turbulence in Kazantsev Model ›
Interior geometry of black holes as a probe of first-order phase transition ›
The Axion Helical Misalignment Mechanism ›
Triggering physical plasmoids in forming current sheets: conditions and diagnostics ›
Localized Steps toward ACT-Favored Inflation ›
AstroConcepts: A Large-Scale Multi-Label Classification Corpus for Astrophysics ›
X-ray Response of the Fully-Depleted, p-Channel SiSeRO-CCD ›
Detection of Gamma-ray Halos around Nearby Late-type Galaxies ›
Halo Spin Depends on The Distance to Cosmic Filament ›
Conservative limits on primordial black holes from the LIGO-Virgo-KAGRA observations ›
Interstellar dust production, destruction and effects of dust depletion in galaxies ›
Alleviating the Hubble tension with Torsion Condensation (TorC) ›
Rotating Neutron Stars with Dark Matter Halos ›
Revealing Unresolved White Dwarf-Main Sequence Binaries using Gaia DR3 and GALEX I. A Volume limited study of 100 pc ›
A nearly pristine star from the Large Magellanic Cloud ›
Semianalytical Accretion-Tracer Emission: Forming Planets Are Intrinsically Faint ›
A GLIMPSE into the very faint-end of the H$\beta$+[OIII]$\lambda\lambda$4960,5008 luminosity function at z=7-9 behind Abell S1063 ›
Galaxy Underdensities Host the Clearest IGM Ly$\alpha$ Transmission and Indicate Anisotropic Reionization ›
Thermal Deformations in Super-Eddington Magnetized Neutron Stars: Implications for Continuous Gravitational-Wave Detectability ›
BlazEr1: The eROSITA Blazar Catalog. Blazars and Blazar Candidates in the First eROSITA Survey ›
Fast End-to-End Framework for Cosmological Parameter Inference from CMB Data Using Machine Learning ›
Data-driven Radiative Magnetohydrodynamics Simulations with the MURaM Code: Coronal Heating and Dynamics in an Emerging Active Region ›
unimpeded: A Public Grid of Nested Sampling Chains for Cosmological Model Comparison and Tension Analysis ›
Rotational Light-Curve Recovery & Predictions of the LSST Yield of Hildas ›
SRG/eROSITA-SDSS view on the relation between X-ray and UV emission for quasars ›
The GLASS-JWST Early Release Science Program. V. H$\alpha$ luminosity functions at $z\sim1.3$ and $z\sim2.0$ ›
Ring Asymmetry and Spin in M87* ›
Exploring Composition Mixing in Kilonova Ejecta with Ray-by-ray Simulations ›
A Closer Look at the Dynamical State of the High-redshift Galaxy Cluster SPT-CL J2215-3537 ›
Sunspot simulations with MURaM -- I. Parameter study using potential field initial conditions ›
The approximate gravitational lensing multiple plane mass sheet degeneracy ›
Measurement of the Full Shape of the Thermal Sunyaev-Zeldovich Power Spectrum from South Pole Telescope and {\it Herschel}-SPIRE Observations ›
Estimation of neutron star mass and radius of FRB 20240114A by identification of crustal oscillations ›
Inhomogeneous magnetic coupling in exoplanets: the stop & go of WASP-18 b's atmospheric flows ›
A Bayesian Method for Air-Shower Reconstruction using Information Field Theory ›
Small-Scale and Transient EUV Kernels in Solar Flare Ribbons ›
Primordial black holes and the velocity acoustic oscillations features in 21 cm signals from the cosmic Dark Ages ›
A bending in the size-mass relation of star-forming galaxies across $0.5 < z < 6.0$ at a critical stellar mass of $10^{10}M_\odot$ revealed by JWST ›
Primordial Non-Gaussianity and the Field-Level Cramer-Rao Bound ›
Dynamics and stability of magnetized AGN-blown bubbles in clusters of galaxies ›
Universality of Halo Shape and its Morphological Evolution across Cosmic Time ›
A Black Hole Star at Cosmic Noon: Extreme Balmer break, photospheric continuum, and broad absorption by thick winds in a Little Red Dot at z=1.7 ›
Formation and disruption of wide binaries in star clusters revealed by N-body simulations ›
The radial component of the local Galactic magnetic field in 3D ›
Impostor Among $\nu$s: Dark Radiation Masquerading as Self-Interacting Neutrinos ›
Exploration of vertical self-resonant bifurcations from Distant Retrograde Orbits (DROs) in the Earth-Moon Circular Restricted Three-Body Problem (CR3BP) ›
String Corrected Scalar Field Inflation Compatible with the ACT Data ›
Demagnifying gravitational lenses as probes of dark matter structures and nonminimal couplings to gravity ›
Plotting correlated data ›
Sculpting of Martian brain terrain reveals the drying of ancient Mars ›
What does it take to have $N_{\rm eff} < 3$ at CMB times? ›
Searches for Continuous Gravitational Waves from Supernova Remnants in the first part of the LIGO-Virgo-KAGRA Fourth Observing run ↓↑