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

In the dome

S Webcam

N Webcam

S Sky
Temperature
-- °C
Humidity
--%
Wind
-- km/h
Pressure
-- hPa

Moon
Latest preprints on astro-ph:
›
Effects of Pebble Accretion Isolation Mass on Observable Exoplanet Properties ›
Laser Metrology for Precision Alignment of Transmission Gratings in the REDSoX Soft X-ray Polarimeter ›
Orbital Migration of Interacting Stellar Mass Black Holes in Disks around Supermassive Black Holes. III. Mass Distribution of Hierarchical Mergers ›
Explosions from Rotating Very Massive Star Collapses to Black Holes: Effects of Nuclear Burning ›
Observational Constraints on Horizonless Compact Objects from Thermal Emission in AGNs ›
A binary black hole merger rate comparison within the same metallicity - star formation rate framework ›
Radio Properties of RS Canum Venaticorum Variables in VLASS and RACS ›
No Evidence for Nearby Circumstellar Material in the Type Ia Supernova 2025rbs ›
Abundant Heavy Black Hole Seeds from Moderate Lyman-Werner Radiation ›
High-Energy Neutrinos from Supernova Shock Breakouts in Circumstellar Media: Light Curves, Spectra, and Contribution to the Extragalactic Neutrino Background ›
The second Arcminute Microkelvin Imager -- Large Array Gamma-ray burst radio afterglow catalog ›
Old Disks Die Hard: How Does AGN Feedback Suppress Disk Formation in Milky Way Mass Galaxies? ›
MORFEO control strategy ›
The CMZ Asymmetries: Feeding or Feedback? ›
Performance Analysis of the Asgard/NOTT Nulling Interferometer: Optimizing Observing Modes for High-contrast Detection ›
H-$\alpha$ Integral Carrington Synoptic Maps Produced by NSO/NISP ›
Time-dependent multi-energy neutrino emission from symbiotic recurrent novae: the role of accretion disks ›
Energy Partitioning in Dust-catalyzed $\mathrm{H_2}$ and HD Formation Revealed by Molecular Simulations Considering Nuclear Quantum Effects ›
CCAT: a two-octave 1.024 GHz KID readout featuring an overlap-channel polyphase synthesis filter bank on RFSoC ›
Enhancing the performance and capabilities of the MIRI instrument on JWST ›
A chemo-dynamical search for planet-candidate hosts of possible extragalactic origin ›
Evidence for Dynamical Filtering: High Binary Fraction, Hard-binary Excess, and Unresolved Triples in the Surviving Core of NGC 6791 ›
On the Acceleration of Pulsar Timing computations using Normalising Flows and Parallelisation ›
How mergers shape galaxy morphology in the IllustrisTNG simulation ›
X-ray Activity of the RS CVn-type Star {\sigma} Gem with the First-Year Observations of Einstein Probe ›
Detection of possible burst oscillation in the neutron star low-mass X-ray binary 4U 1323-62 ›
The SAMI Galaxy Survey: Linking Tidal Features and Orbit Populations Using Schwarzschild Modelling ›
The galaxies' energy balance problem solved ›
High-order Paschen emission from the quiet-Sun off-limb chromosphere ›
Aether.jl : A High-Performance 3D MHD and Multifluid Dust Code Written in a Dynamic Language with an Interactive Human-AI Development Framework ›
The B-Index as a Diagnostic of Cool Stars: Assessing Metallicity Dependence of TiO Absorption in the Visible Spectrum ›
A Reproducible Two-Boundary Kinematic Correction for Baryonic Rotation-Curve Reconstruction in an 84-Galaxy SPARC Benchmark ›
Constraining Primordial Power Asymmetry from Galaxy Clustering and Peculiar Velocity Information ›
Cosmographic Reconstruction of the Quintessence Potential in Scalar-Tensor Gravity ›
Magnetoacoustic Portals in Quiet-Sun Fluxtubes Revealed by Chromospheric Spectropolarimetry with SUNRISE III/SCIP ›
Launching Jets in Tidal Disruption Events: Magnetic Flux Advection and Plasma Loading ›
Cosmicflows-4 and the Cosmological Consistency of Large-Scale Motions ›
The Evolution of the ACIS Contamination Layer on the Chandra X-ray Observatory from 2010 to 2026 ›
The Galactic Centre G+0.633-0.0604 Molecular Cloud: A New Gold Mine for Astrochemistry ›
Optical Spectroscopy of TeV-emitting BL Lac Candidates ›
XRISM reveals sloshing-driven gas motions in the core of Abell 2029 ›
How X-rays heat the IGM in different 21-cm simulation codes: a comparison between Licorice and Beorn ›
OH Line Detections in Southern Galaxies of the IRAS Revised Bright Galaxy Sample ›
The deepest color-magnitude diagrams for the benchmark open cluster NGC 2437 from Gaia and VVVX ›
Hydrogen Engulfment into Sub-Neptune Cores through Magma Ocean Convective Surface Renewal ›
ATLAS. IV. A JWST+MUSE Demographic Study of Ly$\alpha$ Profiles in Little Red Dots ›
Cosmic Ray Diffusion and the Origin of Very High Energy Gamma-Ray Emission in Young Massive Stellar Clusters ›
High-Frequency Thermal Noise in Michelson Interferometers ›
Unknown Unknowns: Model Misspecification in Machine Learning for Physics ›
From the Earth to the Sun ›
Quasinormal modes as exterior probes of black hole interiors in our Universe ›
Axion Isocurvature Perturbations Survive the Scaling Evolution of Axion Domain Walls ›
Gravitational Waves from Dimension-6 Assisted Peccei - Quinn Phase Transitions ›
Altitude-Dependent Near-Source Spectral Filtering of Meteor Infrasound Above 80 km and Consequences for Period-Based Energy Estimates ›
Physics of Circular Polarized Ion-Scale Waves in Hybrid Simulations of Alfv\'enic Fluctuations ›
Blazar Boosted Dark Matter in IceCube ›
Multivariate time series transformer embeddings for light curves of periodic variable stars ›
Identifying galactic binary systems of neutron stars and black holes with LISA ›
Creation of Viscous Dark Energy by the Hubble Flow: Comparison with SNe Ia Master Sample Binned Data ›
Stability Boundary of Neutron-Dark Matter Mixed Stars ›
Beyond Sgr A* and M87*: Sub-Microarcsecond Black Hole Shadow Detection via Lunar-based Extremely Long Baseline Interferometry ›
Distinguishing the nature of dark matter by mapping cosmic filaments from Lyman-alpha emission ›
Inferring population III star properties from the 21-cm global signal ›
Analysis of the Space Velocities of Several Samples of Open Star Clusters ›
Pulsar scintillation arcs formed from correlated volume scattering ›
Short-Range Forces Can Catalyze Extreme Orbital Evolution in Hierarchical Triples ›
3D Kinematic Reconstruction of the Crab Nebula That Includes the Northern Ejecta `Jet' ›
Prediction for IMAP: Revealing the Role of the Solar Magnetic Field in the Heliotail ›
The emergence of X-ray emission lines during relativistic radio-jet formation in the changing-look active galactic nucleus 1ES 1927+654 ›
The incidence of eROSITA X-ray AGN in the local Universe: from dwarf to massive galaxies ›
Environmental dependence of Type Ia supernova standardization on the local luminosity-weighted age ›
Three-Dimensional Dust Distribution in the Jovian System from Juno/Waves Observations: Insights into the Halo Ring and Magnetospheric Dust ›
Hubble tension: a short review of theoretical explanations ›
eRASSU J043115.8-711730 :the first pulsating symbiotic super-soft X-ray source in the Magellanic Bridge ›
GLOW II: A Census of Oxygen in Low-Mass Galaxies ›
A Helium-shell Burning Blue Horizontal Branch Star Produced from Common Envelope Evolution ›
Synchrotron and Inverse-Compton Signatures of Black to White Hole Explosions: Weibel-Mediated External Shocks in the Interstellar Medium ›
SPURS: Massive Stars, Dense Gas, and Ly$\alpha$ Escape in GN-z11 at $z = 10.6$ ›
Assessing Planetary Stability and Long-Term Habitability in Nearby Stellar Binaries: 70 Oph, 36 Oph, $\gamma$ Leo ›
NuOscProbExact: a fast, general-purpose code to compute exact two-, three-, and four-flavor neutrino oscillation probabilities ›
Achromatic, spin-odd Kerr EVPA as a null Frenet-Serret torsion integral on the photon ring ›
Revisiting $^7$Be Weak and Radiative Transition Rates in Big Bang Nucleosynthesis: Implications for the Primordial Lithium Problem ›
Phase Transitions and Gravitational Waves ›
Formation of bound composite vortices of a singly-quantized $^1$S$_0$ vortex and half-quantized $^3$P$_2$ vortices in the $^1$S$_0$-$^3$P$_2$ coexisting phase in neutron stars ›
Nonlinear hydrodynamics in spinning neutron stars: Theoretical universal relations and equilibrium solutions ↓↑