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 Mt. Suhora 60cm telescope
The Mt. Suhora 60cm telescope
Cloud conditions

Cloud

Rain conditions

Rainfall

Allsky

S Sky

Temperature
2.1 °C

Humidity
 90%

Wind
3.2 km/h

Pressure
1022.3 hPa

Moon

Moon

 News from astronomynow.com
› See Titan’s shadow transit Saturn – next chance 2038!
› Nova outburst in Centaurus
› Astronomy Now relaunches digital platform
› Potentially habitable planet TRAPPIST-1e displays tentative evidence for an atmosphere
› Ten-Year Lease Extension Confirmed at Herstmonceux Observatory
› Venus and Jupiter’s bright morning conjunction
› It’s time again for Perseid meteors!
› Lonely giant planets may form their own planetary systems
› Congratulations Professor Michele Dougherty – our new Astronomer Royal
› Astronomy Now under new ownership
RSS  Latest preprints on astro-ph:
› The optical photometric variability of Herbig Ae/Be stars from TESS
› Foundation Models for Astrobiology: Paper I -- Workshop and Overview
› The Astronomical Plate Digitization at SHAO
› Identification of Gamma Ray Pulsar Candidates in the \emph{Fermi}-LAT 4FGL-DR4 Unassociated Sources Using Supervised Machine Learning
› How precisely can we measure the ages of subgiant and giant stars?
› Tracing Planetary Accretion in a 3 Gyr-old Hydrogen-Rich White Dwarf: The Extremely Polluted Atmosphere of LSPM J0207+3331
› Next-Generation Improvements in Giant Exoplanet Evolutionary and Structural Models
› Multi-messenger Analysis of Supermassive Black Hole Binaries: The Joint-likelihood Approach
› A Vertically Orientated Dark Matter Halo Marks a Flip of the Galactic Disk
› That's so Retro: The Gaia-Sausage-Enceladus Merger Trajectory as the Origin of the Chemical Abundance Bimodality in the Milky Way Disk
› Metals versus Non-metals: Chemical Evolution of Hydrogen and Helium Isotopes in the Milky Way
› The ExoGRAVITY survey: a K-band spectral library of giant exoplanet and brown dwarf companions
› The Sonora Substellar Atmosphere Models VI. Red Diamondback: Extending Diamondback with SPHINX for Brown Dwarf Early Evolution
› The polar debris disc around 99 Herculis: A potential signpost for polar circumbinary planets
› Inferring cosmological parameters from galaxy and dark sirens cross-correlation
› Neutrino signal from the hadron-quark phase transition in the conversion of Neutron Stars into Quark Stars
› JWST imaging of omega Centauri: II. Evidence for a split white dwarf cooling sequence in the near-infrared
› Planetary Nebula Evolution for Single Stellar Models. The Formation of Neutral Spikes
› The CEERS Photometric and Physical Parameter Catalog
› Low-Frequency Gravitational Waves in Three-Dimensional Core-Collapse Supernova Models
› Understanding Exoplanet Habitability: A Bayesian ML Framework for Predicting Atmospheric Absorption Spectra
› The Distribution of Quenched Galaxies in the Massive z = 0.87 Galaxy Cluster El Gordo
› LATIS Data Release: $\sim4200$ Spectra of $z \sim 2-3$ Galaxies, Redshifts, and IGM Tomography Maps
› Measuring the Temperature of Extremely Hot Shock-Heated Gas in the Major Merger MACS~J0717.5+3745 With Relativistic Corrections to the Sunyaev-Zel'dovich Effect
› Constraining exoplanet interiors using observations of their atmospheres
› Event Horizon Telescope Pattern Speeds in the Visibility Domain
› Accretion-Regulated Type Transitions in Changing-Look AGNs: Evidence from Two-Epoch Spectral Analysis
› Constraints on the interacting holographic dark energy models: implications from background and perturbations data
› Tides from the cloud can induce the fast disruption of star clusters and offer an explanation for Gaia strings
› A Sharper View of the X-ray Spectrum of MCG--6-30-15 with XRISM, XMM-Newton and NuSTAR
› LAMOST Medium-resolution Spectroscopic Survey of the Rosette Nebula
› The Influence of Magnetic Complexity of Active Regions on Solar Wind Properties During Solar Cycles 23 and 24
› Galaxy Metallicity Gradients in the Reionization Epoch from the FIRE-2 Simulations
› A study of 80 known pulsars at 185 MHz using MWA incoherent drift-scan observations
› HST Confirms Sub-5 kpc Dual Quasar Pairs at Cosmic Noon
› 3D Moving-mesh Hydrodynamical Simulations of Wind/Jet Driven Ultraluminous X-ray Source Bubbles
› Investigating the $w$CDM Model with Latest DESI BAO Observations
› The Low-Frequency Spectra of Radio Pulsars
› Sub-Threshold Fermi-LAT Sources in the Vicinity of KM3-230312A
› Cosmology Likelihood for Observables in \Euclid (CLOE). 1. Theoretical recipe
› Identification of molecular line emission using Convolutional Neural Networks
› Magnetohydrodynamic shallow water equations with the alpha effect: Rossby-dynamo waves in solar--stellar tachoclines
› Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 4: Validation and Performance
› Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 5. Extensions beyond the standard modelling of theoretical probes and systematic effects
› Detecting dark matter substructure with lensed quasars in optical bands
› Euclid preparation. Cosmology Likelihood for Observables in Euclid (CLOE). 3. Inference and Forecasts
› A systematic search for orbital periods of polars with TESS. Methods, detection limits, and results
› The age and metallicity dependence of the near-infrared absolute magnitude and colour of red clump stars
› Hubble Constant and Mass Determination of Centaurus A and M83 from TGRB Distances
› Light Travel Time Effects in Kilonova Models
› Effect of stochastic kicks on primordial black hole abundance and mass via the compaction function
› Probing the geological setting of exoplanets through atmospheric analysis: using Mars as a test case
› deep-REMAP: Probabilistic Parameterization of Stellar Spectra Using Regularized Multi-Task Learning
› Safely simplifying redshift drift computations in inhomogeneous cosmologies: Insights from LTB Swiss-cheese models
› The choice of Planck CMB likelihood in cosmological analyses
› Generalized Distributions of Host Dispersion Measures in the Fast Radio Burst Cosmology
› What is the contribution of gravitational infall on the mass assembly of star-forming clouds? A case study in a numerical simulation of the interstellar medium
› Extending CSST Emulator to post-DESI era
› Hierarchical Progressive Survey (HiPS) format: moving from visualisation to scientific analysis
› Direct observation of the X-ray counterpart of the H{\alpha} filaments and of the sloshing spiral in the Perseus galaxy cluster
› Low-redshift constraints on structure growth from CMB lensing tomography
› Galaxy Underdensities Host the Clearest IGM Ly$\alpha$ Transmission and Indicate Anisotropic Reionization
› SN 2021lwz: Another Exotic Luminous and Fast Evolving Optical Type Ic Broad-Lined Supernova ?
› Deep uGMRT observations for enhanced calibration of 21 cm arrays -- I. First image and source catalogue
› JWST Observations of SN 2024ggi II: NIRSpec Spectroscopy and CO Modeling at 285 and 385 Days Past the Explosion
› Anchoring the Universe with Characteristic Redshifts using Raychaudhuri Equation Informed Reconstruction Algorithm (REIRA)
› Catalog of Mock Stellar Streams in Milky Way-Like Galaxies
› Targeted search for an individual SMBHB in NANOGrav 15-year and EPTA DR2 data sets
› Gauge Dependence of Scalar-Induced Gravitational Waves from Isocurvature Perturbations: Analytical Results
› Emission of Nambu-Goldstone bosons from the semilocal string network
› Dark matter Simplified models in the Resonance Region
› Hydrodynamic models of Reheating
› Emergence of advection-diffusion transport structure and nonlinear amplitude evolution of strongly driven instabilities
› Constraining the Cosmological Evolution of Post-Newtonian Parameters with Gravitational Wave Signals from Compact Binary Inspirals
› Effect of Finite-Temperature $\beta$-Decay Rates on the Rapid Neutron Capture Process
› Distinguishing between Black Holes and Neutron Stars within a Population of Weak Tidal Measurements
› When inverse seesaw meets inverse electroweak phase transition: a novel path to leptogenesis
› Thermal and magnetic effects on viscosity in Binary Neutron Star mergers
› Statistics of Current and Vorticity Structures in Relativistic Turbulence
› Interactions between syn-rift magmatism and tectonic extension at intermediate rifted margins
› Primordial Black Holes Place the Universe in Stasis
› Discovery of the Asymmetric Effect in the Response of Photoionization Gas
› Likelihood and appearance of life beyond the Earth: An astronomical perspective
› Synthetic Light Curves and Spectra for the Photospheric Phase of a 3D Stripped-Envelope Supernova Explosion Model
› Generative modelling for mass-mapping with fast uncertainty quantification
› Testing $f(R)$ Gravity from Cosmic Shear Measurements
› Constraining cosmological parameters using density split lensing and the conditional stellar mass function
› Current constraints on cosmological scenarios with very low reheating temperatures
› Cosmology from UNIONS weak lensing profiles of galaxy clusters
› OL\'E -- Online Learning Emulation in Cosmology
› Scale and redshift dependent limits on cosmic neutrino properties
› Conditional Autoencoder for Generating Binary Neutron Star Waveforms with Tidal and Precession Effects
› Forecasts and Simulations for Relativistic Corrections to the Sunyaev-Zeldovich Effect
› The systemic recoil velocity distribution and the scale height of field millisecond pulsar systems: Implications on neutron star retention fractions in star clusters
› Population demographics of white dwarf binaries with intermediate separations: Gaia constraints on post-AGB mass transfer
› Model-independent cosmological inference after the DESI DR2 data with improved inverse distance ladder
› Robust Evidence for Dynamical Dark Energy from DESI Galaxy-CMB Lensing Cross-Correlation and Geometric Probes
› Diversity of low-mass planet atmospheres in the C-H-O-N-S-Cl system with interior dissolution, non-ideality, and condensation: Application to TRAPPIST-1e and sub-Neptunes
› Simulation of Binary-Single Interactions in AGN Disks II: Merger Probability of Binary Black Holes during Chaotic Triple Process
› The Feasibility of a Spacecraft Flyby with the Third Interstellar Object 3I/ATLAS from Earth or Mars
› Luminous Late-time Radio Emission from Supernovae Interacting with Circumbinary Material
› GW-YOLO: Multi-transient segmentation in LIGO using computer vision
› Numerical simulations of oscillations for axisymmetric solar backgrounds with differential rotation and gravity
› Onset of CN Emission in 3I/ATLAS: Evidence for Strong Carbon-Chain Depletion
› HWO Target Stars and Systems: A Prioritized Community List of Potential Stellar Targets for the Habitable Worlds Observatory's ExoEarth Survey
› BGRem: A background noise remover for astronomical images based on a diffusion model
› Orbital decay candidates reconsidered: WASP-4 b is not decaying and Kepler-1658 b is not a planet
› Comparing XRISM cluster velocity dispersions with predictions from cosmological simulations: are feedback models too ejective?
› Benchmarking AI-evolved cosmological structure formation
› Hard X-ray view of two $\gamma$-ray detected low-luminosity active galactic nuclei: NGC 315 and NGC 4261
› Robust Measurement of Stellar Streams Around the Milky Way: Correcting Spatially Variable Observational Selection Effects in Optical Imaging Surveys
› A first look at quasar-galaxy clustering at $z\simeq7.3$
› Non-spherical effects on the mass function of Primordial Black Holes
› Simulations of Ellipsoidal Primordial Black Hole Formation
› Eastward Transients in the Dayside Ionosphere II: A Parallel-plate Capacitor-Like Effect
› A Characteristic Signature of Magnetospheric Wave-Particle Interactions Found in the Turbulent E-region
› Gravitational Waves from Resonant Transitions of Tidally Perturbed Gravitational Atoms
› Cosmological perturbations for smooth sign-switching dark energy models
› Dynamical scheme for computing the mass parameter of a system in a medium
› From geometry to cosmology: a pedagogical review of inflation in curvature, torsion, and extended gravity theories
› A Python Interface for Numerical Relativity Program AMSS-NCKU

  ↓↑    

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