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: Sunset from the kitchen window
Sunset from the kitchen window
S Webcam

S Webcam

Webcam

N Webcam

Allsky

S Sky

Temperature
18.4 °C

Humidity
 50%

Wind
0.0 km/h

Pressure
1016.0 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:
› Engineering of titanium transition edge sensor wafers for the BA4-90/150 receiver of BICEP Array
› Best practices for obtaining astrometric observations from JWST (274) NIRCam data
› Alfred: A Flexible, User-Friendly Python Package for Exoplanet Confirmation
› Radio Monitoring of the Changing-look AGN Mrk 590 I: VLA Observations Reveal A Bow-shock Driven Radio Brightening Event
› Primordial Black Holes as Cosmic Architects: Imprints of an extended mass function
› Scatter, bias, and chaos of satellite orbits in triaxial dark matter haloes
› SOAR TESS Survey III: Mapping the Stellar Companion Deficit around TESS Planet Candidates
› Barren but not Empty: The Impact of Void Environments on Galaxy and Halo Populations
› A Broken Clock Is Right Twice a Day: [Ce/Mg] Is Not a Universal Chemical Clock
› Assembly bias from nuisance to probe II: Salvaging linear clustering from DESI and SDSS data
› The origin of the stellar mass-size relation of satellite galaxies in the COLIBRE simulations
› $\texttt{SPINE}$: Symbolic Models to Predict the Evolution of the $\Lambda$CDM Nonlinear Power Spectrum
› Using CFHT's SITELLE to Probe the Long-Sought Supernova Remnant Shell in the Crab Nebula
› The host galaxies of 2003fg-like type Ia supernovae
› Paleo-Detectors as a Novel Probe of Dark Matter-Nucleus Effective Interactions
› Synchrotron self-Compton Reverse Shock in Energy-Injection and Radiative Scenarios
› Phase-Space Diagnostics for Dwarf Galaxies in Cluster Environments
› The Impact of Magnitude Uncertainties and K-corrections on Standard Siren Measurements of the Hubble Constant
› Active nests at solar maximum: How nested flux emergence dominated flaring activity and structured the heliosphere
› Non-equilibrium condensation of the first Solar System solids
› The MegaWave Radio Surveyor
› RadialPaths: Radial profiles in multi-centred astronomical structures
› HOLISMOKES -- XVIII. Cosmology with strongly lensed type II supernovae: Effects of instrumental setups on $H_0$
› COSMOS-Web: From early star-formation enhancement to late suppression in galaxy groups
› Cross-simulator transfer with foundation model summaries: Towards robust SKA-era reionization inference
› Microscopy assessment of two multiple-transient candidates
› Diversity of stripped-envelope supernova light curves from interaction with binary-driven circumstellar material
› Path to Black Hole Astrometric Microlensing from 10-Year KMTNet Database
› Numerical modelling of recombination-driven stellar winds
› Fine-scale flare structures and their energetic implications from short-exposure extreme-ultraviolet imaging
› Systematic uncertainties on DESI Tully-Fisher distances constrained with Integral Field Spectroscopy
› A radio continuum view of Stephan's Quintet: age, dynamics and origin of the shock
› Revisiting the Hubble tension with an inverse power-law early dark energy
› Visualizing Disequilibrium: Tracing Two-Point Correlations to Specific Spatial Structures in the Milky Way
› Background Intensity Estimation for Cassini-ISS Image Using Deep Learning-Based Diffusion Model
› Two Predicted, Concentric Nova Shells Surround the Prototype Dwarf Nova U Geminorum
› FRB 121102: No supernova-like ejecta or magnetar power, hinting at a binary WD merger
› Approximating the peculiar velocity distribution of dark matter halos with Tsallis statistics
› Investigating the disappearance of a type-C QPO in black hole X-ray binary Swift J151857-572147 with AstroSat
› Bifrost spectral inversions, Fast non-LTE solar chromospheric diagnostics from 3D simulations
› Spectro-Polarimetric Properties of CHIME FRB Sources
› Optical Discovery of New and Candidate Galactic Supernova Remnants Plus Optical Imaging of the Monogem Ring Supernova Remnant
› ELUCID-DESI II. Revealing dark matter mass, tidal, and velocity (MTV) fields using galaxy group phase information
› ANRe-M1: a GPU-accelerated numerical relativity code with multi-energy M1 neutrino transport
› SERENADE III: Insight into the Origin of the High Dust Temperature and High [O III]/[C II] Ratio at $z\gtrsim6$
› Carbon in J0815+4729: Casting A Shadow of Doubt on the Interpretation of CH Absorption in the Most Primitive Stars
› Classical Cepheids in the JWST and Roman Era: A New Theoretical Framework and its Metallicity Dependence
› Study on the Venusian Atmospheric Thermal Structure: A Comparative Analysis between VEX/Akatsuki and Venus-GRAM/VCD
› Derivative hierarchy as the origin of kernel-dependent trends in Gaussian process reconstructions of the hubble parameter
› Alkali lines at extreme densities and their impact on giant planet interior structure
› Energy-dependent slow collective flavor conversion of supernova neutrinos
› A Bayesian Framework for Constraining Magnetar Magnetic Fields from Repeating FRB Statistics
› The true masses of radial-velocity exoplanets constrained by stability
› Bumpy inflation from explosive particle production
› Not so typical doubly eclipsing systems
› Anisotropy-driven constraints on the transition from Galactic to extragalactic cosmic-ray sources
› Three-dimensional SPH simulations of the Caloris basin-forming impact: basin scaling, the gravity anomaly, and antipodal effects
› The solitary star cluster of the Andromeda XXV dwarf spheroidal
› HURACAN: A comparison of stellar and interstellar proper motions inside L1688
› Source models of ultrahigh-energy cosmic rays
› Catastrophic tidal disruption of heterogeneous rubble piles: a tale of two regimes
› Narrow-Shell Stochasticity in Source-Sink Models of the Low Earth Orbit Environment
› NGTS clusters survey - VI: Stellar rotation in seven young open clusters within the PLATO LOPS2 field
› Optimal transport regularized dynamic radio interferometric reconstruction
› Testing Narrow-jet Gamma-Ray Bursts as Sources of Ultrahigh-Energy Cosmic Rays
› Bright Metal-Poor Star Survey - I. Tomo-e Gozen narrow-band photometric survey and medium-resolution spectroscopic follow-up
› Towards the exploration of astrophysical datacubes through volumetric rendering within CARTA
› Revisiting the enigmatic sixth star cluster in the Fornax dwarf spheroidal galaxy
› Exploring the survivability of higher-order multiple protostellar systems -- The case of VLA1623
› Panchromatic Spectra of Nearby Low-mass and Sun-like Stars with Directly Imageable Habitable Zones
› Dust torques for realistic dust size distributions
› $N$-body simulations of the open cluster population in the Milky Way and the impact of GMC encounters
› Non-isothermal vertical distribution functions for the Milky Way
› Near universality of nonlinear transverse and radial velocity responses in spherical collapse with arbitrary radial profiles
› The MICADO first light imager for the ELT: first on-bench performance tests of the SCAO hybrid LQG+Integrator controller
› LightCube: A Parsec-Resolution 3D Model of the Local Far-Ultraviolet Interstellar Radiation Field
› Map of the Interstellar Continuum FUV Field within 800 Parsecs
› An Equation of State for Supercritical Silicate-Hydrogen Mixtures at Sub-Neptune Interior Conditions
› The JWST/NIRCam Scattered Light Disks GTO 2780 program: panchromatic coronagraphic imaging of the HD 10647, HD 32297, HD 61005, HD 107146, and HD 181327 debris disk systems
› The Atacama Cosmology Telescope: Constraints on the anisotropic screening and birefringence effects with DR6
› Deuterium Production in an Effective Field Theory Constructed from On-Shell Amplitudes
› Spatially Scanned STIS Spectra of the Exoplanet Host Star 55 Cnc
› Impact of Nuclear Level Density on $r$-Process Rare-Earth Peak Nucleosynthesis
› Getting Warmer: IceCube Nears Freeze Out
› Effects of the interaction of dark matter and neutron-star matter on extreme and intermediate mass-ratio inspirals
› Direct and Indirect searches for DM-electron interactions in sub-GeV DM models
› $\mu$DM: a new mechanism for the baryon-dark matter coincidence
› Scale Invariance and Compact Star Matter
› Quantum Selection of Classical Histories
› Mixed Dark Matter and Galaxy Clustering: The Importance of Relative Perturbations
› Lyman-alpha emission at the end of reionization: line strengths and profiles from MMT and JWST observations at z~5-6
› Assessing Self-Absorbed Molecular Lines as Tracers of Gravitational Collapse
› Updated constraints on interacting dark energy: A comprehensive analysis using multiple CMB probes, DESI DR2, and supernovae observations
› Quantifying Systematic Age Discrepancies in Very Young Star Clusters
› On Lorentz Variability of Magnetically Dominated Relativistic Outflows
› Fisher Forecasts for Cosmological Yields from $3\!\times\!2$pt Analysis of the Roman Space Telescope High Latitude Imaging Survey
› Cluster number counts in dark energy model with energy and momentum coupling to dark matter
› The origin of isolated millisecond pulsars in globular clusters
› Impact and interplay of $\Lambda$CDM analysis choices for LSST cosmic shear
› Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model
› Effects of resolution and local stability on galactic disks: Halo resolution and softening on bar formation
› The baryon content of magnetically arrested black hole disks and jets
› Weak-lensing Analysis of Intracluster Filaments in Abell 2744: Matched-filter Scans and Stepwise 2D Tracing
› The Neptunian ridge planet WASP-156 b does not have a polar orbit
› TRINITY: A coupled model of winds, radiation, and photoionised gas in molecular clouds. I. Methods and validation
› SMUGGLE-Ring: Evolutionary link between nuclear star cluster and nuclear disk
› Probing a new subclass of llGRB-SN transients: Insights from EP250304a and its associated supernova
› Angular momentum evolution in the CIELO simulations. I. Temporal evolution of gas-stellar misalignments and baryonic merger timing
› AutoClassMK: A public neural network for automatic 2D MK classification of normal stars in basic Python
› The limits of lattice inflation: a cautionary tale
› Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data
› Lower Your Rates: On Claims of a Binary Black Hole Merger-Rate Crisis
› The Impact of Non-Gaussian Line Spread Functions on Stellar Kinematic Recovery: Consequences for Dynamical Models
› Archival Diagnostics for Potential Background Contaminantsof Project Hephaistos Dyson Sphere Candidates
› Refined reduction and standardisation of 53 years of UBV photometry at Hvar
› Tracing black hole and galaxy growth across environments since cosmic noon
› Atmosphere mitigation in CMB observations using multi-frequency time-domain component separation
› Exploration of Exoplanet Atmospheres with the James Webb Space Telescope
› The Tidal Venus Phenomenon: Demographics and Case Studies
› Dipolar power asymmetry in wide-angle correlations of galaxy density, velocity and ellipticity
› The First X-Ray Polarimetry of the Typical Accretion Disk Corona Source 4U 1822-37
› Energy Partition in AGN-driven Bubbles of NGC 4438: From Nuclear Bubbles to a Galaxy-scale Outflow
› Indirect Searches for Dark Photon-Photon Tridents in Celestial Objects
› How light can ALP dark matter be?
› Generalized JMN Naked Singularity Models
› Gravitational wave signal and noise response of an optically levitated sensor in a Fabry-P\'erot cavity
› Primordial Magnetogenesis and Gravitational Waves from ALP-assisted Phase Transition
› Gravitational-wave astronomy with a space-based optical clock network
› When Do Autoregressive Sequence Models Forecast Physical Wavefields? A Controlled Study on Synthetic Seismograms
› Tunable responsivity and bandwidth in microwave kinetic inductance detectors via readout current nonlinearity

  ↓↑    

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