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: The Orion Nebula (M42) imaged from Mt. Suhora
The Orion Nebula (M42) imaged from Mt. Suhora
Cloud conditions

Cloud

Rain conditions

Rainfall

Allsky

S Sky

Temperature
10.8 °C

Humidity
 72%

Wind
4.8 km/h

Pressure
1016.5 hPa

Moon

Moon

 News from astronomynow.com
› JWST’s ‘impossible’ early galaxies may be even more massive than we thought
› How to observe the 12 August 2026 solar eclipse
› Falcon 9 lunar impact: More than a new crater
› Euclid opens a new window on the first billion years of cosmic history
› Caught in the act: the wind that could kill a galaxy
› Europe’s Mars rover may land in the remains of a vast ancient water system
› Moon dust preserves record of life’s building blocks
› Dark matter may come in multiple forms, new model suggests
› Witness to history: Artemis II, lunar exploration and hope
› Artificial Intelligence uncovers more than 100 new worlds in NASA data
RSS  Latest preprints on astro-ph:
› A comparative study of emergent dark energy models
› A Multi-instrument Generalized Lomb-Scargle Periodogram Implementation
› Leveraging Impact Parameter to Mitigate the Transit Light Source Effect: Early Insights from TRAPPIST-1
› On what scales does strong lensing robustly constrain the mass profile of low-mass perturbers?
› High-contrast aperture masking interferometry: detecting companions within the diffraction limit
› One-point matter PDFs beyond TopHat filters
› Investigating the Multiwavelength Emission of Binary SMBH Candidate SDSS J095036.75+512838.1
› AT 2016blu: Accretion-Powered Outbursts in a Luminous Blue Variable and Compact Object Binary
› Effects of Outer Giant Planets on In Situ Formation of Inner Super-Earths
› JWST Spatial-Spectral Mapping of Green Comet C/2022 E3 (ZTF)
› Mapping the z>=5 SiIV Column Density Distribution onto the Galaxy Stellar Mass Function Using the Cumulative Absorption Cross Section
› Statistical Analysis of Minifilament Eruptions Using Full-disk H$\alpha$ Blue-wing Observations at Big Bear Solar Observatory
› Accounting for Transit Timing Detectability: Biases in Planetary Radius and Orbital Period
› Physics-Informed Bayesian Optimization Warm-Starts for Sequential Convex Programming in Asteroid Surface Hopping
› Amplifying the imaging power of digital sky surveys with space telescopes data and generative AI
› Microwave Remote Sensing of Giant Planet Atmospheres: Considerations for Saturn and Uranus Orbiter Missions
› Effects of Ambient Medium Profiles on the Evolution of Relativistic Magnetized Jets
› A Dark Matter Masquerade: Degeneracies in Black Hole and Accretion Inference from X-ray Reflection Measurements and Prospects for Compact Dark Matter Halo Constraints
› BSN: Light Curve Modeling and Orbital Period Analysis of the Contact Binaries OV Leo and V339 Leo
› Pandora cluster Lensing, AGN, and Transient Exploration (PLATE) from JWST Multi-Epoch Imaging. I. Discovery of a type II supernova candidate in a spiral galaxy at $z=0.7$
› Chang'e 7 Lunar Lander Optical Camera-Telescope: Optical Astronomy from the Moon
› GRB 220101A: a most energetic $10^{54}$ erg long GRB triggered by two supernovae 3.5 seconds apart
› Pulse profiles of accreting neutron stars - A review of analysis methods, observations, and theoretical models
› Excitation and Recombination Data for Nd I-V with Applications to Kilonovae
› Probing cosmological phase transitions with SKAO through nano-Hz gravitational-wave portal
› EXPO: a quantum leap in fast, wide-band X-ray polarimetry for astrophysics
› The DIRECD coronal mass ejection direction catalog: three-dimensional propagation inferred from coronal dimmings
› Ultra-Deep imaging of the starless galaxy candidate Cloud-9
› Hyperonic compact stars with vector portal dark matter
› The impact of tidal locking on Earth-like planetary dynamos
› Nucleosynthesis in the Accretion-induced Collapse of magnetised, Rotating White Dwarfs
› NAIR-APREXIS: Enabling photonics-based instruments for long-baseline interferometry and integral-field spectroscopy
› Gas-phase and Surface Chemistry in the Massive Star-Forming Region RCW\,120
› The superclumps of the local Milky Way. Supercloud fragmentation and the sites of star formation
› NestyNet. III. Symbolic Regression from Analytic Neural Surrogates
› DOLPHIN (Device of Line Photometry in Nasmyth): A Switchable Multiband Photometer for the ISAS 1.3-m Telescope
› EWOCS VII : Unveiling the faint diffuse X-ray emission in Westerlund 1
› The GASKAP-HI Survey towards the Magellanic Clouds: Cold Atomic Gas Survival and Evolution in the Large Magellanic Cloud
› Transit Searches for Habitable-Zone Exoplanets with Artificial Intelligence
› The curious case of HCO$^+$: Extreme abundances under extreme conditions
› Angular momentum in isolated disc galaxies: Insights from TNG100
› CtaAgnVar : a Pipeline for Variability Studies with the Cherenkov Telescope Array Observatory
› alpha_theta waves in the tachoclines of Sun-like stars
› Constraining neutron-star properties with ensembles of thermonuclear bursts: application to SRGA J144459.2-604207
› Physical Calibration of a Minimal Effective Field Theory of the Three-Dimensional Lyman-$\alpha$ Forest
› Model independent lensing sub-structure detection with multiply-imaged star clusters constellations
› Generation of TeV Photons by PeV Neutrinos in Dense Astrophysical Environments
› The [Ne V] AGN Diagnostic in SDSS-IV/eBOSS: An Anticorrelation Between Ionization State and AGN Luminosity in Low-Redshift Coronal-Line Galaxies
› Does Cumulative XUV Unify the Neptunian Desert?
› The Random Magnetic Field of the Milky Way
› VLASS Discovery of a Luminous Galactic Radio Transient Evolving on Decade Timescales
› Diversity of Galaxy Centers from Small-Scale Isocurvature
› High-Energy Neutrino Constraints on memory burdened Bardeen and Kerr Primordial Black Holes
› Circularly polarized gravitational waves from parity-violating scalar-tensor theory
› TeV-scale leptogenesis in a parity symmetric neutrino mass model
› Characterizing the temporal evolution of Biermann-battery-driven magnetic reconnection in laser-ablated plasmas
› Effective Field Theory for Freezing Gravity with Minimally Coupled Matter
› Tunneling from a Slowly Rolling Multifield Background Using Tadpole Subtraction
› Trace Anomaly and Effective Topological Sources in Neutron Stars
› Portability of Fortran's 'do concurrent' on GPUs II
› Causal Gravitational-Wave Production Does Not Generate Infrared Adiabatic Curvature
› Bayesian P-spline recovery of stochastic gravitational-wave backgrounds in LISA
› Qubits for Dark Matter Hunting
› Ion Irradiation of GridPix Detector at Bonn Isochronous Cyclotron
› Neutron star matter with hyperons: Bayesian comparison of nucleonic and SU(6)/SU(3) hyperonic models
› From Timbuktu to SKA: Who owns the Astronomy knowledge Africa produces?
› Resonance crossings as entire functions of the Koopman operator
› DESIVAST: A Catalog of Low-Redshift Voids using Data from the DESI DR1 Bright Galaxy Survey
› Detecting Secular Perturbations in Kepler Planetary Systems Using Simultaneous Impact Parameter Variation Analysis (SIPVA)
› Energy-Space Analysis of Tidal Stripping in Stellar-Dark Matter Systems
› GWTC-4.0: Constraints on the Cosmic Expansion Rate and Modified Gravitational-wave Propagation
› Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4
› The DESI DR1 Peculiar Velocity Survey: Fundamental Plane Catalogue
› Method on Using Shadow Altitude to Remove Geocoronal H$\alpha$
› ICM-SHOX III. The case of MACS J0018.5+1626, a radio relic that looks like a radio halo?
› Radiation GRMHD Models of Accretion onto Stellar-Mass Black Holes: III. Near-Eddington Accretion
› Second Order Closures for the Radiative Transfer Equation: Some Are Unstable
› Universal Non-Gaussian Signatures from Transient Instabilities
› Wings of little dots: Exponential broad lines from a stratified BLR
› SN 2022riv in RX J2129: Discovery, Spectroscopic Classification, and Microlensing of a Strongly Lensed Type Ia Supernova from JWST and HST Observations
› Neutrino self-interactions in post-reionization era: Lyman-$\alpha$, 21-cm and cross-spectra
› Differentiable Forward Modeling for Efficient and Accurate Shear Inference
› The major cluster merger in Abell 2034 as seen by XRISM: Strong turbulence and spectral anomalies?
› Earliest simultaneous multi-color optical observations of GRB 230328B: from 41 seconds to the host-galaxy identification
› The Quasar Main Sequence of Super-Eddington NLSy1 Galaxies
› CCAT: Optical Design of the 410 GHz Prime-Cam Module
› Diffractive Sail H-Reversal Trajectory: Theoretical Feasibility, Design Strategies, and Applications
› Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics
› Simulating Zernike-based CWFSing with HCIPy
› Tracing Lyman alpha escape in the CRISTAL-02 galaxy at z~5.3
› Multi-scale Memory and Regime Shift in the Hyperactive Repeating FRB 20240114A
› Gravitational Waves and Primordial Black Holes produced by Dark Meta Stable Vacuum Decay
› Automatic classification pipeline for glitches in the Virgo detector
› Higgs boson mass and thermal wino dark matter from Starobinsky supergravity with the MSSM
› An Introduction to Bayesian and Frequentist Simulation-Based Inference with Machine Learning

  ↓↑    

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