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: Dome at sunrise
Dome at sunrise
S Webcam

S Webcam

Webcam

N Webcam

Allsky

S Sky

Temperature
-2.9 °C

Humidity
 93%

Wind
0.0 km/h

Pressure
997.8 hPa

Moon

Moon

 News from astronomynow.com

› 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
› 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
RSS  Latest preprints on astro-ph:

› MAJORS II: HCO+& HCN Abundances in W40
› A constrained linear model for continuum normalization of stellar spectra
› An X-ray-Emitting Proto-Cluster at $z\approx5.7$ Reveals Rapid Structure Growth
› The Role of Long Period Variable Stars in Observational Astrophysics
› The CO snow line favours strong clumping by the streaming instability in protoplanetary discs with porous grains
› GLIMPSE-D: Metallicity Decline in Faint Galaxies: Implications for [O III]+Hb Luminosity Function and Reionisation Budget
› A GLIMPSE into the UV Continuum Slopes of the Faintest Galaxies in the Epoch of Reionization
› Stellar and orbital characterization of three low mass M dwarf binary stars with dynamical spectroscopy from the Habitable Zone Planet Finder
› POEMMA-Balloon with Radio: A multi-messenger, multi-detector balloon payload
› Exomoons and Exorings with the Habitable Worlds Observatory II: Finding Endor with Lunar Eclipses
› Revisiting Stellar equatorial rotational velocities with Gaia DR3 line broadening -- the dependence on temperature, mass and age
› The Sound of Noise: Leveraging the Inductive Bias of Pre-trained Audio Transformers for Glitch Identification in LIGO
› GLIMPSE-DDT spectroscopic properties of faint-end galaxies at $z\sim6$: Towards first metal enrichment, dust production, and ionizing photon production
› The 2025 Evaluation of Experimental Thermonuclear Reaction Rates (ETR25)
› Origin of Coronal Extreme Ultraviolet Shockwaves without a Coronal Mass Ejection Event
› RM-Tools: Software for Analyzing Polarized Radio Spectra
› H$_2^{18}$O in the terrestrial planet-forming regions of protoplanetary disks
› Accretion Properties of the Young Brown Dwarf 2MASS J08440915-7833457
› The TDE Population from First-Principles Models of Stellar Disruption and Debris Dynamics
› Asymmetrical thermonuclear supernovae triggered by the tidal disruption of white dwarfs
› Twenty-four thousand hours of GREENBURST observations with the GBT
› Spatial distribution of organics in the Horsehead nebula: signposts of chemistry driven by atomic carbon
› A dynamical systems approach to studying the equivalence principle in dilaton gravity
› From cosmological simulations to binary black hole mergers: The impact of using analytical star formation history models on gravitational-wave source populations
› Gamma-ray Emission from the S147 Region: Indication of Escaping Cosmic Rays Interacting with Molecular Clouds
› Orbital stability of compact three-planet systems III. The role of three-body resonances
› Metallicity Structure in Galactic Longitude-Velocity Diagrams of the Milky Way Disk and FIRE-2 Simulations
› Model independent test of the FLRW metric and the curvature in light of DESI DR2
› Mathematical Anatomy of Neutrino Decoherence in Red Turbulence: Fractional Calculus and Convergence of the Perturbative Series
› Self-consistent $N$-body simulation of Planetesimal-Driven Migration. II. The effect of PDM on planet formation from a planetesimal disk
› Observations of the temporal evolution of Saturn's stratosphere following the Great Storm of 2010-2011. II. Latitudinal distribution of CO and stratospheric winds
› Fast variability and circular polarization of the 6.7 GHz methanol maser in G33.641$-$0.228
› Probing the Diversity of Type Ia Supernova Remnants in 3-D Hydrodynamic Simulations with X-ray Spectral Synthesis
› A multi-technique search for year-scale $\gamma$-ray quasi-periodic modulation in the high-redshift FSRQ PKS~2052$-$47
› Interaction of Black Hole Magnetospheres with Inclined Ambient Fields
› A Quiescent Galaxy in a Gas-Rich Cosmic Web Node at z~3
› Massive dusty multiphase outflow in local merger shows no sign of slowing on kiloparsec scales
› Ultraviolet Signatures of Jet-Ejecta Interaction in Early Kilonovae: Prediction from Realistic Atomic Opacities
› An unexpected population of quenched galaxies harbouring under-massive SMBHs revealed by tidal disruption events
› Analyzing PAHs as a Tracer of Anomalous Microwave Emission Near the Galactic Plane Using the COSMOGLOBE DIRBE Reduction
› SPT-3G D1: A Measurement of Secondary Cosmic Microwave Background Anisotropy Power
› The RoPES project with HARPS and HARPS-N II. A third planet in the multi-planet system HD 176986
› Revealing the link between halo mass and radio jet activities in quasars
› Climates of Terrestrial Exoplanets and Biosignatures
› Apparent Dark-Energy Evolution from Cosmic Inhomogeneities
› On the rotational properties of M-type asteroids: recent evidence for higher rotation rates
› On the contradictory case of the binary system HD 81809 hosting two pulsating solar-like stars observed by TESS
› Replicating weak-lensing summary-statistic covariances with normalizing flows
› The IACOB project: XVI. Surface helium abundances in Galactic O-type stars: indications for identifying binary interaction products
› How well is the local Large Scale Structure of the Universe known? CosmicFlows vs. Biteau's Galaxy Catalog with Cloning
› The Need for Ultra High Resolution X-ray Imaging
› Euclid preparation. Galaxy power spectrum modelling in redshift space
› Encounters Between M33 and Present-Day M31 Satellites Hint at a Previous Group Accretion
› Extreme winds on the emerging dayside of an ultrahot Jupiter
› Molecular Gas Detections in Eight Faint DSFGs with Red NIR Colors at z = 1.2-2.5
› Probabilistic Interpolation of Sagittarius A*'s Multi-Wavelength Light Curves Using Diffusion Models
› Bottom-heavy initial mass functions reveal hidden mass in early galaxies
› Fading Echoes of Interaction: Probing Centuries of Mass-Loss in Four Old Type IIn Supernovae
› General Scalar Field Inflation ACT Attractors: Utilizing the $n_s(r)$ relation
› A Remedy of the Trans-Planckian Censorship Problem with Smooth Slow-roll to Power-law Inflation Transitions in Scalar Field Theory
› An Analytic Scale-dependent Dark Matter Profile and the Baryonic Tully-Fisher Relation
› Quantum Cosmology as a Hydrogen atom: Discrete $\Lambda$ and cyclic Universes from Wheeler-DeWitt quantization
› Enhancing online estimation of CBC parameters with the low-latency MBTA analysis
› Pathology of the Unified Dark Sectors in Modified General Relativity
› Sunward Streaming 3He-rich SEP Events Observed by Solar Orbiter and Parker Solar Probe during Perihelion Passage
› Graviton energy spectra arising from the KSVZ axion model
› An Introduction to Single-Antenna Radio Astronomical Polarimetry
› Formation of trapped vacuum bubbles during inflation, and consequences for PBH scenarios
› User Guide to UVIT Data Reduction
› When relics were made: vigorous stellar rotation and low dark matter content in the massive ultra-compact galaxy GS-9209 at z=4.66
› Unified reconstruction of the Lyman-alpha power spectrum with Hamiltonian Monte Carlo
› Spectral Properties of Irradiated Circumbinary Disks around Binary Black Holes Governed by Hydrogen Opacities Dependent on Temperature and Density
› The NIKA2 cosmological legacy survey at 2 mm: catalogs, colors, redshift distributions, and implications for deep surveys
› Pulsations change the structures of massive stars before explosion: interpreting SN 2023ixf and SN 2024ggi
› Semi-analytic studies of accretion disk and magnetic field geometry in M87*
› Noisy Timing Behavior is a Feature of Central Compact Object Pulsars
› SIGNALS of Giant HII Regions: A Spatially Resolved Analysis of NGC 604
› Next-Generation Improvements in Giant Exoplanet Evolutionary and Structural Models
› Proton-rich production of lanthanides: the $\nu i$ process
› Rapidly rotating hot nuclear and hypernuclear compact stars: integral parameters and universal relations
› Clustering properties of the CatWISE2020 quasar catalogue and their impact on the cosmic dipole anomaly
› A Case for an Inhomogeneous Einstein-de Sitter Universe
› Growth of Metal-Enriched Supermassive Stars by Accretion and Collisions
› Solar carbon abundance from 3D non-LTE modelling of the diagnostic lines of the CH molecule
› The Origins of the Bulk flow
› Inflationary relics from an Ultra-Slow-Roll plateau
› Multi-wavelength Signatures of Supernova Shock Breakout from Red Supergiants in Two Dimensions
› Through Thick and Thin: The Cosmic Evolution of Disk Scale Height
› An eclipsing 8.56 minute orbital period mass-transferring binary
› Suppression of Fast Flavor Conversion by Red Turbulence in Supernovae
› Updated Metallicity Diagnostics for Precision Oxygen Abundance Measurements in High-redshift Galaxies with JWST
› Nuclear astrophysics
› The Carousel Lens I: A Spectroscopic Survey of the Carousel Lens Field
› Beyond solar metallicity: How enhanced solid content in disks re-shape low-mass planet torques
› Confronting Inflation and Reheating with Observations: Improved Predictions
› Inflationary dynamics of non-minimally coupled $f(R)$ matter-curvature theories
› Consistent Four-derivative Heterotic Truncations and the Kerr-Sen Solution
› Virtual states and exponential decay in small-scale dynamo
› Spectral instability of horizonless compact objects within astrophysical environments
› Axion condensates in neutron stars and radial oscillation modes
› Constraining a de Broglie--Bohm quantum bounce cosmology with Planck data
› Probing dark matter interactions with a RES-NOVA prototype cryogenic detector
› Gravitational wave detectors from an experimental perspective
› Development of Low-Noise Two-stage dc-SQUID for TES Detector Readout

  ↓↑    

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