Mt. Suhora Astronomical Observatory Home page
po polsku
Podchorazych 2, 30-084 Krakow, Poland. tel.: (+48 12) 662 6301; fax: (+48 12) 637 2243; Obs. tel.: (+48) 502 113714
  • Home
  • Events & Conferences

Mount Suhora Astronomical Observatory

Information
  • About the Observatory
  • Equipment
  • Pictures
  • Staff
  • Publications
  • Telescope schedule
  • Weather
Eclipsing Binaries
  • TIDAK (O-C database)
Links
  • Astronomical links
  • Astronomy in Poland
  • Useful links
Amateurs & Education
  • Astronomical calendar
  • Lunar phases
  • Educational materials and links
  • Institute of Physics
Astronomia w Krakowie
Photo: view from north-east
view from north-east
S Webcam

S Webcam

Webcam

N Webcam

Allsky

S Sky

Temperature
8.3 °C

Humidity
 54%

Wind
0.0 km/h

Pressure
1015.0 hPa

Moon

Moon

 News from astronomynow.com

› Molten lava world points to new class of planet
› How to see the 3 March total lunar eclipse
› Diamond downpours in the outer Solar System
› The Moon’s February world tour
› Dr Allan Chapman (1946-2026)
› Potentially bright ‘sungrazing’ comet discovered
› Thank you from the editor
› 24 days of cosmic wonder
› Meteor shower calendar
› How to observe meteor showers
RSS  Latest preprints on astro-ph:

› Cosmological constraints from the DESI DR1 joint power spectrum and bispectrum analysis
› Survival of the most compact: the life and death of satellite halos in self-interacting dark matter
› Revisiting the Milky Way stellar long bar and the 3 kpc arm
› Impact of subhalo dynamical friction heating on the formation of the first structures in the universe
› A Planetary Illusion's Funeral: Non-detection of a Gaia DR3 Exoplanet Candidate, and the Role of Intermediate-precision Radial Velocities in Gaia Exoplanet Follow-up
› Flux-Averaged Force Multipliers
› Archaeology of Galactic Nuclei Activity
› The Journey to Dominance: How BCGs Evolve Differently from Other Massive Galaxies
› The Vera C. Rubin Observatory Prompt Processing System
› COSMOS-3D: Black Hole Mass Estimators and Luminosity Functions of Paschen-line AGNs
› SpecZoo: An AI-Powered Platform for Spectral Analysis and Visualization in Science and Education
› Expected evolution of the binary system ATLAS J1138-5139
› Furax: A Modular JAX Framework for Linear Operators in Astrophysical and Cosmological Data Analysis
› A Concept of Next-Generation Atmospheric Cherenkov Telescope Array (NG-ACTA)
› Precise parameter determination of the open cluster NGC 1647 via asteroseismology of p-mode pulsators
› HAWC Study on the Ultra-High-Energy Gamma-Ray Emissions from the Pulsar Wind Nebula G32.64+0.53
› Morphological Signatures of Gravitational Evolution, Redshift-Space Distortions, and Massive Neutrinos in Large-Scale Structure
› The radial velocity stability for reference sources in the MWISP CO survey
› The FAST Galactic Plane Pulsar Snapshot Survey. IX. Timing Three Binary Pulsars with Wide Orbits and Low Orbital Eccentricities
› Smoothed Particle Hydrodynamics in pkdgrav3 for Shock Physics Simulations. II. Shear Strength
› FATHOMER survey: III. Preliminary HI galaxy identification results
› Three outstanding physical questions for K2-18 b and other temperate sub-Neptunes
› The dusty envelopes of asymptotic giant branch stars with ultraviolet excesses
› Recovery of 21 cm BAO: a configuration-space correlation function analysis
› The characteristics of variability of AGNs based on the structure function
› Modeling Quasar Photo-$z$ Distribution and Uncertainty. A Study Based on the Kilo-Degree Survey
› Constraints on the $^{12}$C$(\alpha, \gamma)^{16}$O and $^{16}$O+$^{16}$O Reaction Rates from Binary Black Holes Detected via Gravitational Wave Signals
› A Complete X-ray View of Supernova Remnant W28 with Einstein Probe: Spatial Distribution of Parameters and Origin of the Thermal-Composite Morphology
› 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
› High-energy neutrino flux from SN2024ggi: constraints from semi-analytic modeling of its post-explosive emission
› Connection-angle dependence of proton anisotropy in ground-level enhancement events
› Observations of Exocomets
› The Arc in the DX Cha Circumbinary System: Evidence For a Retrograde Circumbinary Disk
› High-resolution mid-IR spectroscopy of SVS 13-A with EXES/SOFIA: The surprisingly high CH$_3$OH/H$_2$O ratio in the planet-forming zone of a solar mass protostar
› Monte Carlo conformal prediction for quantifying uncertainty in radio galaxy classification under ambiguous ground truth
› Three-body Mean Motion Resonance Chains as a Delivery Mechanism for White Dwarf Pollution
› Unveiling large-scale rotational motions in the intragroup medium at z~1 through gravitational-arc tomography
› Retrieving the Red Edge on Earth-like Planets with Heterogeneous Clouds and Surfaces
› A Century of Radial Velocity and Astrometric Monitoring of 70 Oph AB: New PFS Data and Constraints on Planetary Companions
› Evidence of Long-Lived Powerful Gyrosynchrotron Radio Emission in the Close Binary FF UMa
› Early emission characterization of TDE2025aarm
› Numerically stable equations for the orbital evolution of compact object binaries
› Theory of optical long-baseline interferometry on polarized sources
› A New Multi-Constraint Potential Field Source Surface (PFSS) Extrapolation Model
› Cosmological forecast from the full-sky angular power spectrum and bispectrum of 21cm intensity mapping
› SPT-3G D1: Maps of the millimeter-wave sky from 2019 and 2020 observations of the SPT-3G Main field
› VINTERGATAN-GM: long-lived satellite planes induced by a massive GSE-like merger
› Improved constraint on the Hubble constant from dark sirens with LIGO/Virgo/KAGRA O4a
› Galaxy sizes as complementary (zero-)bias tracers of local primordial non-Gaussianity
› New Constraints on the Jovian Narrowband Radio Components from Juno/Waves Observations and 3D Geometrical Simulations
› Toward universal coalescence models for antideuteron production
› Recursive Penrose processes in electrically charged black hole spacetimes: Backreaction and energy extraction
› Cosmology and modified GW propagation from the BNS mass function at third-generation detector networks
› Observational imprints and quasi-Periodic oscillations of magnetically charged anti-de Sitter black holes
› Vector-channel scattering of dark particles in a Sp(4) gauge theory
› On the Universal Cuspy Behavior in Black Hole Shadows
› Casimir-Induced Quintessence in Dark Dimension
› A dual description of quarks and baryons: Quarkyonic matter within a relativistic quark model
› Can QCD Axions Survive the Cosmological Constant Problem?
› Cislunar State and Uncertainty Propagation via the Modified Generalized Equinoctial Orbital Elements
› Reheating in runaway inflation models via the evaporation of mini primordial black holes
› Reconstructing the whole 6D properties of the Sagittarius stream with N-body simulations
› LISA and $\gamma$-ray telescopes as multi-messenger probes of a first-order cosmological phase transition
› Physics of 1 keV line in X-ray binaries
› An ancient system hidden in the Galactic plane?
› Modeling the Spectral Energy Distribution of Active Galactic Nuclei: Implications for Cosmological Simulations of Galaxy Formation
› Hard X-ray/Soft gamma-ray Laue Lenses for High Energy Astrophysics
› The impact of new ($\alpha$, n) reaction rates on the weak s-process in metal-poor massive stars
› Accurately simulating core-collapse self-interacting dark matter halos
› Comparing LambdaCDM, wCDM, and w0waCDM models with DESI DR2 BAO: Redshift-Resolved Diagnostics and the Role of rd
› Application of interpretable data-driven methods for the reconstruction of supernova neutrino energy spectra following fast neutrino flavor conversions
› SPARCS -- combining radiation hydrodynamics with non-equilibrium metal chemistry in the SWIFT astrophysical code
› The Yasone catalogue: three new Milky Way satellites and 17 further hypercompact candidates
› The Hidden Life of Stars: Embedded Beginnings to AGB Endings in the PHANGS-JWST Sample. I. Catalog of Mid-IR Sources
› A first look at quasar-galaxy clustering at $z\simeq7.3$
› Eternal inflation bubble collision signature on CMB remote dipole and quadrupole fields
› J-PAS: forecast on the primordial power spectrum reconstruction
› Galactic foreground residue biases in cosmic-microwave-background lensing-convergence reconstruction and delensing of B-mode maps
› Caustic crossings in giant arcs with extended dark matter objects
› The Intermediate Mass Black Hole in Omega Centauri: Constraints on Accretion from JWST
› Detection of the Pairwise Kinematic Sunyaev-Zel'dovich Effect and Pairwise Velocity with DESI DR1 Galaxies and ACT DR6 and Planck CMB Data
› COSMOS-3D: Dense Circumnuclear Gas across Black Hole Growth Phases at z ~ 3
› Extended Wess-Zumino Dark Radiation Model with Interacting Scalar Field Dark Matter and Stepped Dark Radiation
› OutLines: Modeling Spectral Lines from Winds, Bubbles, and Outflows
› From emission to absorption: the FAST observation of the OH 18-cm lines from the Comet C2025/A6
› CMB anisotropies from cosmic (super)strings in light of ACT DR6
› A 2% determination of $N_{\rm eff}$ from primordial element abundance, cosmic microwave background, and baryon acoustic oscillation measurements
› Cosmological peculiar velocities in general relativity
› Emulation of SPHEREx Galaxy Power Spectra I: Neural Network Details and Optimization
› A Minimal Four-Thruster System for Comet-Based Interstellar Navigation
› Trajectory Stability and Signature Diagnostics for Comet-Based Interstellar Navigation
› ID-MAGE II: The Star Forming Satellites of Low-Mass Hosts
› G objects as Primordial Black Hole-Neutron Star Remnants: Population Modeling and Multi-Wavelength Observables
› Quantum Damping of Cosmological Shear: A New Prediction from Loop Quantum Cosmologies
› Scalar-Mediated Inelastic Dark Matter as a Solution to Small-Scale Structure Anomalies
› Cosmic Rays as an Interdisciplinary Earth Observation Tool: From Particle Physics and Atmospheric Processes to Geosciences and Urban Science
› Axions on a Hyperbolic Ride: Geometric Suppression of CMB Isocurvature and a Blue-Tilted Spectrum
› Modified Teleparallel $f(T)$ Gravity, DESI BAO and the $H_0$ Tension
› Cosmological Spacetimes with Sign-Changing Spatial Curvature and Topological Transitions
› Multi-Field Dilaton Screening Beyond the Thin-Shell Mechanism

  ↓↑    

Return to main page of Mt. Suhora Observatory
Copyright © 2002-2026 Astronomy Department, University of National Education Commission. All Rights Reserved.