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: Stars over the dome
Stars over the dome
S Webcam

S Webcam

Webcam

N Webcam

Allsky

S Sky

Temperature
-4.9 °C

Humidity
 67%

Wind
12.9 km/h

Pressure
1016.3 hPa

Moon

Moon

 News from astronomynow.com
› Thank you from the editor
› 24 days of cosmic wonder
› Meteor shower calendar
› How to observe meteor showers
› 13 spooky images for Halloween
› How to see Comet Lemmon
› Hubble revisits a cosmic yardstick
› Europe’s planet hunting spacecraft complete and ready for final testing
› See Titan’s shadow transit Saturn – next chance 2038!
› Nova outburst in Centaurus
RSS  Latest preprints on astro-ph:
› Habitability of exoplanets orbiting flaring stars
› ESO Expanding Horizons White Paper: Electromagnetic counterparts of massive BH mergers with LISA
› Detection of Lensed Gravitational Waves in the Millihertz Band Using Frequency-Domain Lensing Feature Extraction Network
› A Velocity Coupled Radial Acceleration Ansatz for Disk-Galaxy Rotation Curves: Fits to SPARC, Bayesian Inference, and Parameter Identifiability
› Sensitivity of Weak Lensing Surveys to Gravitational Waves from Inspiraling Supermassive Black Hole Binaries
› On the Cooling of Compact Stars in Light of the HESS J1731-347 Remnant
› Neural Network for Simulating Radio Emission from Extensive Air Showers
› Impact of the EPOS.LHC-R hadronic interaction model on the Centaurus A ultrahigh-energy cosmic-ray scenario
› A Modal Approach to Constrain Inflation through Numerical Bispectra
› Early Planet Formation in Embedded Disks (eDisk). XIX. Structures of molecular outflows
› Elemental abundance pattern and temperature inversion on the dayside of HAT-P-70b observed with CARMENES and PEPSI
› Episodic planetesimal disruptions triggered by dissipation of gas disk
› Numerical Simulations of the Circularized Accretion Flow in Population III Star Tidal Disruption Events. I. The Accretion Flow and the Wind
› Multiband Gravitational Wave Detection Prospects for M31 UCXB-1 System in Low and Middle Frequency Band
› Can A Kinematically Hot and Thick Disk Form A Bar? : Role of Highly Spinning Dark Matter Halos
› Particle production and Higgs reheating
› Numerical simulation of lunar response to gravitational waves and its 3D topographic effect using the spectral-element method
› VLBI Diagnostics of Off-axis Jets in Radio Flares of Tidal Disruption Events
› A systematic study on the aromatic and aliphatic hydrocarbon emission features of nearby galaxies using AKARI near-IR spectra
› Investigating the signs of evolutionary characteristics in the energy spectrum of shock wave acceleration
› The Effect of Magnetic Field Dissipation in the Inner Heliosheath: Reconciling Global Heliosphere Model and Voyager Data
› A self-consistent 3D MHD model producing a solar blowout jet
› Golden and Silver Dark Sirens for precise H0 measurement with HETDEX
› The rotation curve of the Milky Way measured by Classical Cepheids from Gaia DR3
› Comprehensive study of solar type II radio bursts and the properties of the associated shock waves
› Compact Ca II K Brightenings Precede Solar Flares: A Dunn Solar Telescope Pilot Study
› Spectral State Switching in Mrk 421: Results from the AstroSat LAXPC/SXT Observations
› Implications of Cosmic Birefringence for Multi-Field ALP Dark Matter
› Long-term monitoring of repeating FRB 20220912A with the uGMRT at low radio frequencies
› A Rare Millisecond Pulsar with Cross-Pole Emission: Single-Pulse Insights from PSR J1857+0943
› The First X-ray Polarimetry of GRS 1739--278 Reveals Its Rapidly Spinning Black Hole
› TITAN DR1: An Improved, Validated, and Systematically-Controlled Recalibration of ATLAS Photometry toward Type Ia Supernova Cosmology
› A large, long-lived, slowly-expanding superbubble across the Perseus Arm
› WST spectroscopic variability alerts: discovery space, data flow system requirements
› Superradiant and dynamical spin-down of neutron stars with gravitational wave implications
› From emission to absorption: the FAST observation of the OH 18-cm lines from the Comet C2025/A6
› Cosmic-Ray-Constrained LSTM Model for Geomagnetic Storm Prediction
› Multiband optical variability on diverse timescales of the blazar Ton 599 from 2011 to 2023
› Inferring Eccentricity of Binary Black Holes from Spin-Orbit Misalignment
› Primordial black holes and smooth coarse-graining in excursion set theory
› Searching for Cosmological Collider in the Planck CMB Data II: collider templates and Modal analysis
› Radio Supernovae
› An Enhanced "Flux-Corrected Transport"-Based Plasmasphere Refilling Model
› GraviBERT: Transformer-based inference for gravitational-wave time series
› $Sp(4,\mathbb{Z})$ modular inflation
› Pre-Supernova (Anti)Neutrino Emission Due to Weak-Interaction Reactions with Hot Nuclei
› Methods for Detecting Gravitational Waves from mini-Extreme-Mass-Ratio Inspirals I: Statistics Based on Time-Frequency Signal Tracks
› Methods for Detecting Gravitational Waves from mini-Extreme-Mass-Ratio Inspirals II: A Spectral-Leakage-Aware Framework
› Impact of neglecting center-of-mass acceleration in parameter estimation of stellar-mass black holes
› Small-scale turbulent dynamo for low-Prandtl number fluid: comparison of the theory with results of numerical simulations
› Mass-to-Horizon Entropic Cosmology: A Unified Thermodynamic Pathway to Cosmic Acceleration
› Detection of very high-energy gamma-ray emission from the radio galaxy M87 with LHAASO
› Redshift-space distortion constraints on the neutrino mass and models to alleviate the Hubble tension
› Sombrero Galaxy as an Accelerator of Ultrahigh Energy Cosmic Ray Nuclei
› One-loop correction to primordial tensor modes during radiation era
› Precise measurements of the cosmic ray proton energy spectrum in the "knee'' region
› Search for Lorentz Invariance Violation with spectral lags of GRB 190114C using profile likelihood
› Self-Interacting Dark Matter with Mass Segregation: A Unified Explanation of Dwarf Cores and Small-Scale Lenses
› Towards sub-milliarcsecond astrometric precision using seeing-limited imaging
› Probabilistic Link Budget Analysis for Low Earth Orbit Satellites in the Optical Regime
› Snowball Bistability Vanishes at Moderate Orbital Eccentricity
› Feedback-Controlled Beam Pattern Measurement Method Using a Power-Variable Calibration Source for Cosmic Microwave Background Telescopes
› Cosmological Prediction from the joint observation of MeerKAT and CSST at $z$ = 0.4 $\sim$ 1.2
› Probing the large-scale magnetic field inside the Sun from three decades of observed surface magnetograms
› HI Content of Group Galaxies from the FAST All Sky HI Survey
› High-energy astrochemistry in the molecular interstellar medium
› NICER Magnetar Burst Catalog
› Vertically resolved minimal-set k-distribution for thermal infrared absorption: an application to the atmosphere of Venus
› The Extended Baryonic Tully-Fisher Relation for SDSS MaNGA Galaxies
› Minijets and Broken Stationarity in a Blazar : Novel Insights into the Origin of $\gamma$-ray Variability in CTA 102
› Optimizing Bayesian model selection for equation of state of cold neutron stars
› Impact of Non-Thermal Leptogenesis with Early Matter Domination on Gravitational Waves from First-order Phase Transition
› A New Definition of Horndeski Theory and the Possibility of Multiple Scalar Field Extensions

  ↓↑    

Return to main page of Mt. Suhora Observatory
Copyright © 2002-2025 Astronomy Department, University of National Education Commission. All Rights Reserved.