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: View to Mt. Babia Gora
View to Mt. Babia Gora
S Webcam

S Webcam

Webcam

N Webcam

Allsky

S Sky

Temperature
-3.6 °C

Humidity
 93%

Wind
0.0 km/h

Pressure
1011.7 hPa

Moon

Moon

 News from astronomynow.com

› The Moon’s February world tour
› 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
RSS  Latest preprints on astro-ph:

› Revisiting the missing mass problem in MOND for nearby galaxy clusters
› Exploring Cosmological Tensions with Hubble Parameter Tomography via Linear Cosmography
› Correlation Calibration: A Hybrid Calibration Technique for Radio Interferometric Arrays
› Consistency of standard cosmologies using Bayesian model comparison and tension quantification
› The Host Galaxies of Active Galactic Nuclei with Direct Black Hole Mass Measurements
› Modelling the photometric and morphological evolution of disc galaxies in the cluster environment
› Searching for dark matter signals with high energy astrophysical neutrinos in IceCube
› Probing habitable regions with SRG/eROSITA
› Satellites and small bodies with ALMA: Insights into Solar System formation & evolution
› The imprint of AGN-driven outflows on the CGM: the case of Ly{\alpha} nebulae around high-z quasars
› Ne and Fe abundances in the ISM: Archival Study of Fe-L and Ne-K edges in Chandra and XMM-Newton
› Dynamic Zoom Simulations of structure formation beyond standard cosmology
› How Neutron Star Observations Point Towards Exotic Matter: Existing Explanations and a Prospective Proposal
› On the radial velocity wave in the Galactic disk
› Hypersoft X-ray Sources: A New Class of Luminous Cosmic Emitters
› Compact HII Regions as Clocks of Massive-Star Formation: Evidence for Long Formation Timescales
› Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50
› Disk-Regulated Mass Transfer Between Rotating Non-Degenerate Stars: Insights from Be and sdOB Binaries
› On the Difficulties with Late-Time Solutions for the Hubble Tension
› Treecode2: The Power of Pluralism. I. Static Tests
› Simulated LSST Observations of Real Metre-scale Impactors
› An Archival Optical Counterpart Search for Extragalactic Fast X-Ray Transients Discovered by Einstein Probe
› Characterization of the Polarization Beam Response of SPT-3G Using Point Sources
› Reversal of Spin: Comet 41P/Tuttle-Giacobini-Kresak
› Primordial Black Hole signatures from femtolensing and spectral fringe of Gamma Ray Bursts
› Super-knee cosmic rays from interacting supernovae
› The Massive and Distant Clusters of WISE Survey 2: Splashback Radii to z=1.65 from Galaxy Density Profiles
› The Massive and Distant Clusters of WISE Survey 2: Detection of splashback radii in galaxy cluster total light stacks
› ELUCID-DESI I: A Parallel MPI Implementation of the Initial Condition Solver for Large-Scale Reconstruction Simulations
› The Walkaway Star HP Tau/G2: Evidence for a Stellar Merger
› A Demonstration of a Neural Network as a Bridge Between Galaxy Simulations and Surveys
› The Non-Eruptive Reconfiguration of a Quiescent Filament After a Nearby Active Region Emergence
› Joint optical-digital design strategy for adaptive optics systems: application to wavelength selection for satellite imaging
› AB Aur, a Rosetta stone for studies of planet formation (IV): C/O estimates from CS and SO interferometric observations
› Universality of Primordial Anisotropies in Gravitational Wave Background
› SF2A Environmental Transition Commission: Summary of the 2025 workshop
› Mobile neutron monitor for latitude cosmic ray monitoring
› Studies on the spin and magnetic inclination evolution of magnetars Swift J1834.9-0846 under wind braking
› Rotational Behaviour of Exotic Compact Objects
› Introducing a new generation Adaptive Optics simulation framework: from PASSATA to SPECULA
› Galaxies caught in transition: the role of group environment in shaping the mass-size relation in the local Universe
› The effect of JWST/NIRSpec data reduction on the retrieval of WASP-39b atmospheric properties
› Dilution of accreted planetary matter in hot DA white dwarfs according to their mass
› Sensipy: simulate gamma-ray observations of transient astrophysical sources
› Heavy interstellar scattering toward the near end of the Galactic bar
› Forecasting Supermassive Black Hole Binary Gravitational Wave Probes: Prospects for Future Pulsar Timing Array and Space-Borne Detectors
› The X-ray properties of the most luminous quasars with strong emission-line outflows
› Primordial Black Hole Abundance from Reionization
› Merger Driven or Internal Evolution? A New Morphological Study of Tidal Disruption Event Host Galaxies
› Asteroseismic ages for 17,000 stars in Kepler, K2 and TESS
› Antenna for the detection of electromagnetic audio-band disturbances on-board LISA
› Magnetohydrodynamic instabilities in stellar radiative regions. I. Linear study of shear-driven instabilities
› Astrometric follow-up of near-Earth asteroid 2024 YR4 during a Torino scale level 3 alert
› Non-spherical BUFFALOs: a weak lensing view of the Frontier Field clusters and associated systematics
› Optical spectral characterization of OP 313. Constraining the contribution of thermal and non-thermal optical emission
› Towards a Fully Automated Pipeline for Short-Term Forecasting of In Situ Coronal Mass Ejection Magnetic Field Structure
› Mapping plasma properties of Cassiopeia A with XRISM/Resolve: a Bayesian analysis via UltraSPEX
› Spectral Appearance of Self-gravitating AGN Disks Powered by Stellar Objects: Universal Effective Temperature in the Optical Continuum and Application to Little Red Dots
› Dark Matter Heating of Compact Stars Beyond Capture: A Relativistic Framework for Energy Deposition by Particle Beams
› Scalar Tsunamis from Black Hole Formation
› Chiral phase transition with primordial black holes: Distinct phase structure and catalysis
› Gravastar on the brane with a timelike extra dimension
› Bayesian Constraints on the Neutron Star Equation of State with a Smooth Hadron-Quark Crossover
› Spin Light of neutrino in polarized matter
› Accelerating TTL noise post-processing via combined coefficients and alternative TDI configuration
› Real time, cross platform visualizations with zero dependencies for the N-body package REBOUND
› Many-body effects on dense matter with hyperons at finite temperature
› Parametric-Resonance Production of QCD Axions
› Gravitational Raman Scattering: a Systematic Toolkit for Tidal Effects in General Relativity
› The density-bounded twilight of starbursts in the early Universe
› Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies
› Investigating the role of nuclear parameters in Neutron Star oscillations: a model comparison
› The THESAN-ZOOM project: Burst, quench, repeat -- unveiling the evolution of high-redshift galaxies along the star-forming main sequence
› The THESAN-ZOOM project: central starbursts and inside-out quenching govern galaxy sizes in the early Universe
› The Shape of FIREbox Galaxies and a Potential Tension with Low-mass Disks
› ECHO21: a tool for modelling global 21-cm signal from dark ages to reionization
› Galaxy-scale lens search in the PEARLS NEP TDF and CEERS JWST fields
› Overmassive black holes in the early Universe can be explained by gas-rich, dark matter-dominated galaxies
› Tracing Missing Baryons in the Cosmic Filaments with tSZ and CMB-Lensing Stacking
› The THESAN-ZOOM project: Mystery N/O more -- uncovering the origin of peculiar chemical abundances and a not-so-fundamental metallicity relation at $3
› From Redshift to Real Space: Combining Linear Theory With Neural Networks
› The spin-orbit alignment hypothesis in millisecond pulsars
› Resolving the Planck-DESI tension by non-minimally coupled quintessence
› CLASH-VLT: The variance in the velocity anisotropy profiles of galaxy clusters
› The New Status Qvo? SN 2021qvo is Another 2003fg-like Type Ia Supernova with a Rising Light-Curve Bump
› Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations?
› Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
› The Simons Observatory: Characterization of the 220/280 GHz TES Detector Modules
› An Explicit M1 Radiation-hydrodynamics Scheme for Three-dimensional Protostellar Evolution
› Revisiting electron-capture decay for Galactic cosmic-ray data
› Probing AGN-ISM Feedback through Extended X-ray Emission in ESO 137-G034
› A Light-Cone Approach to Higher-Order Cosmological Observables
› VENUS: A Strongly Lensed Clumpy Galaxy at $z\sim11-12$ behind the Galaxy Cluster MACS J0257.1-2325
› Stellar streams around dwarf galaxies in the Local Universe
› Magnetic Field Amplification and Particle Acceleration in Weakly Magnetized Trans-relativistic Electron-ion Shocks
› ALMAGAL VI. The spatial distribution of dense cores during the evolution of cluster-forming massive clump
› Transformation of orientation and rotation angles of synchronous satellites: Application to the Galilean moons
› The Birth of Be Star Disks II. A High-Resolution Spectroscopic Campaign and TESS Observations of an Outburst of the Classical Be star {\lambda} Pavonis
› Ultimate large-$Rm$ regime of the solar dynamo
› The WINTER Observatory: A One-Degree InGaAs Survey Camera to study the Transient Infrared Sky
› Quantifying sunspot group nesting with density-based unsupervised clustering
› Lyman Continuum escaping from in-situ formed stars in a tidal bridge at z = 3
› A comprehensive study of the relations between the properties of planetary systems and the chemical compositions of their host stars
› Perihelion Asymmetry in the Water Production Rate of the Interstellar Object 3I/ATLAS
› A dynamical systems approach to studying the equivalence principle in dilaton gravity
› A quiescent galaxy in a gas-rich cosmic web node at z~3
› Investigating the origin of radio emission in candidate super-Eddington accreting black holes
› Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation
› Broadband infrared spectroscopy of methanol isotopologues in pure, H2O-rich, and CO-rich ice analogues
› Clustering of z~6.6 Quasars and [O III] Emitters Constrains Host Halo Masses and Duty Cycles in 25 ASPIRE Fields
› Sulfur Enrichment in Close-in Exoplanet Atmospheres Induced by Pebble Drift across the Salt Line
› The Double-Burst Nature and Early Afterglow Evolution of Long GRB 110801A
› Fundamental oscillations as a tool to distinguish boson stars from neutron stars and black holes
› Probing Boson Clouds with Supermassive Black Hole Binaries
› Reheating after the Supercooled Phase Transitions with Radiative Symmetry Breaking
› Time-Frequency Analysis of Non-Uniformly Sampled Signals via Sample Density Adaptation
› Metastable Strings and Gravitational Waves in One-Scale Models
› $Q$-balls, neural networks and galaxy rotation curves
› Numerical tiling-based simulations of decoherence in multifield models of inflation
› Strong lensing cosmography using binary-black-hole mergers: Prospects for the near future
› New Multi-messenger Probe of Dark Matter-Nucleon Interactions from Ultra-high Energy Cosmic Ray Acceleration
› Exact black holes and black branes with bumpy horizons supported by superfluid pions
› On the stability of viscous Riemann ellipsoids

  ↓↑    

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