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: Before observations ...
Before observations ...
S Webcam

S Webcam

Webcam

N Webcam

Allsky

S Sky

Temperature
13.8 °C

Humidity
 68%

Wind
3.2 km/h

Pressure
1015.5 hPa

Moon

Moon

 News from astronomynow.com

› 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
› XRISM solves gamma-Cas’s 50-year X-ray mystery
› 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
RSS  Latest preprints on astro-ph:

› Gas Motions in Hydra-A: XRISM Constraints on ICM Kinematics Across Jet-Inflated Cavities
› Search for Planetary-mass Black Holes with an Improved Viterbi Algorithm
› Dissecting the Scalar Cosmological Collider with the Cosmic Microwave Background
› Late-infall-induced formation of giant planets, multi-generational planetesimals, and disk substructures
› Dark Energy Bubble as Dynamical Dark Energy: Properties and CMB Constraints
› Probing large mass-splitting inelastic Dark Matter with RES-NOVA
› Bispectrum BAO and the baryon-dark matter relative velocity
› Star formation powers optical line emission from the CGM
› GUEST: Gravitational Universe Exploration with Satellite Tracking. A passive satellite laser-ranging mission for the dark gravitational Universe
› Characterizing Microlensing Planetary System OGLE-2014-BLG-0676L with High-Resolution Image Constrained Light Curve Modeling
› Precise Determination of the Metallicity and C/O of WASP-39~b From a Single JWST Instrument Mode with Phase-Resolved Cross-Correlation Retrievals
› The Next Generation Virgo Cluster Survey (NGVS). II. A Catalog of Galaxies in the Virgo Cluster
› Nancy Grace Roman Space Telescope Wide Field Instrument: Bright Point Source Saturation Response and Persistence Properties from Thermal-Vacuum Testing
› First results for second generation SiSeRO CCD devices
› Can We Find the Emission Mechanism Behind the Extremely Bright GRB 230812B?
› Vz-GAL Dusty Star-Forming Galaxies: Revisiting the CO-H2 Conversion Factor Tension
› Detection of cosmic strings by gravitational wave lensing. Predictions for Einstein Telescope
› Chondrite Parent Bodies as Escaped Satellites of Proto-Planetary Embryos
› The impact of Hawking radiation from primordial black holes on recombination and the Hubble tension
› Capture of interstellar objects during stellar encounters
› Stream-Driven Ignition of a Realistic Undisturbed Helium Shell on a White Dwarf
› A multiwavelength light curve analysis of the very fast nova V1723 Sco
› Time-Domain Axion Searches with Magnetic White Dwarfs
› Morphology-spin connection in the SAMI Galaxy Survey
› Examining the stellar-merger origin of the blue main sequence in the open cluster NGC\,3532 with N-body simulations
› Azimuthal molecular variations in the AB Aur planet-forming disk
› Universal scaling between magnetar field and initial spin period for short gamma ray bursts
› Estimating stellar metallicities from Gaia DR3 XP data using LAMOST DR10
› The XMM-Newton Line Emission Analysis Program (X-LEAP) III: Earth's Magnetospheric X-ray Emission Revealed by 22-Year XMM-Newton Observations
› Semi-Analytical Model for the Evolution of Stellar Binaries in the Empty Loss Cone of Massive Black Holes
› Enhanced Astrometry of the Rapid ASKAP Continuum Survey: Mid and High Frequency Epochs
› Searching for $\gamma$-ray emission from a bona fide Compact Symmetric Object sample: a $\gamma$-ray signal near GB6 J0906+4124
› KIC 6464285: A Solar-type Eclipsing Binary in a Hierarchical Triple System with Quasi-periodic Out-of-eclipse Modulations
› Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity
› Forward Modeling of the $\delta$ Sct Star V1790 Ori: $\Delta \nu$, $\Omega$, Resolution and Non-adiabatic Effects
› Influence of local and global solar magnetic fields on medium-term forecasting of the number and parameters of coronal mass ejections
› A Type Ia Supernova Candidate at $z\sim4.3$: A Transient Interloper in the Search for $z\sim14$ Galaxies
› Molecular gas hidden in plain sight in the early Universe
› Be/X-Ray Binaries: Phenomenology, Variability, and Accretion~Dynamics
› Consistent Multi-Wavelength Spectral Modeling of Cool White Dwarfs with Carbon-Polluted Atmospheres
› An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars
› Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer
› Dynamical formation of long-period exoplanets systems in evolving binary stars
› Optical Spectroscopy and Temporal Evolution of the Nova V1405 Cas
› Physical Properties of 6.7 Million Galaxies from the DESI Bright Galaxy Survey: Spectral Fitting and Systematic Tests with Mock Spectra
› Determination of the horizontal velocity field in the solar atmosphere: Method validation using 3D MHD model
› Identifying and Determining Atmospheric Parameters of BHB Stars Based on LAMOST DR11
› Will a Supernova explode in CD-30{\deg}11223?
› Testing Theories of Solar Coronal Heating with Three-Dimensional Forward Modeling
› NAPTIME: A Neural-Process Framework for Rubin Alert Classification
› Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model
› The Large Magellanic Cloud through the lens of the James Webb Space Telescope: Binaries and the mass function in the galaxy's outskirts
› Astrophysics on GPUs: introducing AGILE 1.0
› Euclid: Inferring star-formation history via cross-correlations of photometric clustering and shear with the cosmic infrared background
› Three-Dimensional Dust Distribution in the Jovian System from Juno/Waves Observations: Insights into the Halo Ring and Magnetospheric Dust
› Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653
› Gravitational-Wave Sky Mapping with Pulsar Timing Arrays: The Full Earth-Pulsar Response and Fundamental Resolution Limits
› Beyond the $\alpha$ model: scaling the wind-driven accretion rate in protoplanetary disks using systematic non-ideal magnetohydrodynamical simulations
› Search for continuous gravitational waves from the pulsar J0435+3233
› Electron Temperature Gradients Regulate the Duration of Two-Stage Plasmasphere Refilling
› Gravitational waves from self-resonance during reheating with a quantum-corrected inflaton potential
› Hawking emission of massive vector fields by Kerr black holes
› Detecting Cosmological Stasis with Future Gravitational Wave Observatories
› Modified Cosmology from Mass-to-Horizon Relation: Observational Bounds
› Stochastic template banks for GW searches using low-discrepancy sequences
› Domain Walls From Confining Bubbles: $SU(N_{c})$ Yang Mills at Finite $\theta$
› Accretion of multipolar massive complex scalar field packets by a Schwarzschild black hole
› Quarkyonic Stars with Strangeness
› Astrophysical Neutrino Sources as Colliders
› GWTC-5.0: Tests of General Relativity
› Gravitational wave echoes as probes of the maximum mass of strange stars in quadratic curvature-matter coupled gravity
› Optomechanical transfer factors for scattered light noise estimations in the beamtubes of ground-based gravitational wave detectors
› Dark matter searches with a 13 meV threshold superconducting sensor array
› X-ray and Radio campaign of the Z-source GX 340+0: discovery of X-ray polarization and its implications
› Evidence for a $\sim 43$ GeV $\gamma$-ray line signal in a stacking analysis of the Virgo, Fornax, and Ophiuchus Galaxy clusters
› Polarization Measurement of Gamma-ray Bursts with Fermi-GBM: The Case of GRB 180720B
› Revealing the $\chi_{\rm eff}$-$q$ Correlation among Coalescing Binary Black Holes and Tentative Evidence for AGN-driven Hierarchical Mergers
› Seeing the Outer Edge of the Infant Type Ia Supernova 2024epr in the Optical and Near Infrared
› Simulating the Solar Corona with Multiple Solar Photospheric Magnetic Maps during the 8 April 2024 Total Solar Eclipse
› GA-NIFS: Powerful and frequent outflows in moderate-luminosity active galactic nuclei at $z\sim3-6$
› VLBI Diagnostics of Off-axis Jets in Radio Flares of Tidal Disruption Events
› Hypersoft X-ray Sources as a Low-Energy Class of Luminous Cosmic Emitters
› Monitoring the upper atmospheric temperature and interplanetary magnetic field with the GRAPES-3 muon telescope
› Cosmic voids evolution in modified gravity via hydrodynamics
› A Realistic Pulsar -- Supermassive Black Hole Timing Model
› ALMA High-J CO Spectroscopy of High-Redshift Galaxies. II. 0.03" Resolution CO Kinematics Reveal Super-Eddington Accretion in a Dust-Obscured Galaxy at z=3.111
› Interpreting Swift and NuSTAR Observations of the Low-Luminosity Active Galactic Nucleus NGC 4278 with Radiatively Inefficient Accretion Flows and Implications for Neutrino Emission
› Very long-term relaxation of harmonic 1D self-gravitating systems
› Enhanced foreground mitigation in thermal SZ Compton-$y$ maps via polarization and deprojection
› The tidal evolution of satellite galaxies in cosmological simulations: insights from COLIBRE
› Deriving volume density profiles of filaments from observed surface densities
› Breaking Free from the Swampland of Impossible Universes through the DESI Portal
› HWO Target Stars and Systems: Activity and Rotation Catalog (ARC) of Potential Target Stars for the Habitable Worlds Observatory
› On the Faint Early-time Radio and X-ray Emissions in TDE2025aarm
› The Role of Stellar Spin in Repeating Partial Tidal Disruption Events
› Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution
› Amortized Simulation-Based Inference of Colliding-Wind Binaries from Short, Noisy Image Time Series
› The Hubble Missing Globular Clusters Survey IV. Ultra-faint compact satellites of the Milky Way. The case of Koposov 2
› Nebular_AGN: A CIGALE module for fitting AGN emission lines
› Pushing the Primordial Frontier: Exact Linear Solutions in Multifield Inflation
› The Effects of Energy Conservation in Simulating Solar Eruptions
› Thermal Sunyaev-Zel'dovich cross-correlations with unWISE galaxies: disentangling radio contamination, dust properties, and electron pressure
› Numerical polology: towards next-generation model-building for cosmology
› Deep Learning for Astrophysics: An Open Textbook from the NASA Cosmic Origins AI/ML Science and Technology Interest Group
› Assembly bias from nuisance to probe I: the relation between galactic conformity and the linear matter clustering
› The Three Hundred Project: Validating $H_0$ inference from mock X-ray and millimetre analyses of galaxy clusters
› Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing
› Enabling Cosmic Web Analysis at Gigaparsec Scales: A Multi Block Approach for DisPerSE
› Eccentricity as a Magnifying Glass: Precision Population Inference Enabled by Eccentric Neutron Star-Black Hole Mergers
› Unveiling dark energy properties with high-sensitivity cross-correlations of neutral hydrogen intensity mapping and galaxy surveys
› Constraints on Primordial Black Hole Dressed by Dark Matter Halo from Microlensing Effect of Fast Radio Bursts
› CW Cas: A solar-type contact binary system with an unseen third companion in a hierarchical quadruple system
› Solar, Heliospheric and Ionospheric Physics: Pathfinders, Precursors and SKAO Perspective
› An Unsupervised Search for Novel Instrumental Glitches in LIGO O4a: Multi-Scale Sensitization, Empirical Physical Vetoes, and Rate Upper Limits
› Regression to the Mean can Explain Saturation of Geomagnetic Storms
› Galaxy dynamics, gravitational Vlasov-Poisson system, Landau damping, and scattering theory
› Static horizons in cosmology
› Cryogenic sub-Hz cROss torsion bar detector with quantum NOn-demolition Speed meter (CHRONOS) for gravitational wave detection
› Renormalization-Group Invariant Parity-Doublet Model for Nuclear and Neutron-Star Matter
› Measuring Primitive Accumulation: An Information-Theoretic Approach to Capitalist Enclosure in PIK2, Indonesia
› GWTC-4.0: Tests of General Relativity. II. Parameterized Tests
› Seidr update: photonic 'black magic' for high-contrast interferometry using kernel-nulling and photonic lanterns

  ↓↑    

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