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 from south-west
view from south-west
S Webcam

S Webcam

Webcam

N Webcam

Allsky

S Sky

Temperature
4.1 °C

Humidity
 94%

Wind
0.0 km/h

Pressure
1025.4 hPa

Moon

Moon

 News from astronomynow.com

› Happy New Year, Mars! The Red Planet is turning 39
› 3I/ATLAS was born in the deep freeze
› Roman Space Telescope launches on mission to survey the Universe
› 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
RSS  Latest preprints on astro-ph:

› Unveiling photometric transients with the ILMT and their follow-up using DOT
› TNGC-SIDM I: Evolution of massive cluster mergers under the self-interacting dark matter paradigm
› How JWST is Revolutionizing Our View of Early Galaxy Formation
› Identity Crisis: Untangling Mass-Ordering Artifacts from Compact-Object Pairing in Gravitational-Wave Populations
› EMRIs in Kerr Spacetime: The Role of Inclination Diffusion
› Any colour you like: The diverse chromaticities of white dwarfs
› The Dance of the Little Red Dots: Spectroscopy of Two Blue Companions at z = 3.9 and 5.5 Reveals Young, Metal-Poor Starbursts Merging with Their LRDs within a Few Hundred Myr
› Wave Cold Dark Matter Can Reproduce the Radial Acceleration Relation in X-ray Elliptical Galaxies
› The Second Catalog of Low-Energy Fermi-LAT Sources
› Audible curvaton: modulated phase transition as the origin of large-scale curvature perturbations and gravitational wave anisotropies
› GroArnold: A Framework for Constructing Action-based Models for Triaxial Galaxies and Dark Matter Halos
› A Nonlinear General Implicit Runge-Kutta Integrator for Multifluid Charged Dust and Gas
› Forecasting a Cosmological 21 cm Stacking Detection with Early HIRAX Data
› Thermodynamically consistent equation of state tables for use in giant planet and brown dwarf interior modeling
› Substructure-enhanced Collisional Relaxation in Stellar Systems
› Scalar-Assisted Growth of Supermassive Black Holes: Boson-Mass Windows and Observational Constraints
› JWST observations of 47 Tucanae: I. The low-mass main sequence down to the hydrogen-burning limit
› The mass functions of multiple stellar populations in 47 Tucanae
› The convective-transition gap in 47 Tucanae with JWST
› jax-SNANA: A GPU-accelerated Supernova Framework for the SBI Era
› Kinetic Theory of the EFTofLSS : A Halo-Based Approach
› First L-type substellar object discovered in the vicinity of the embedded cluster NGC 2023
› SPICY 30021: an embedded bona fide FUor with a mid-infrared precursor
› The connection between massive galaxies and their dark matter haloes from $z=0.25$ to $z \sim 4$ from the combined COSMOS, XMM-LSS and ECDF-S fields
› Velocity-field estimation techniques for on-disk solar coronal bright fronts (CBFs) and shock-wave propagation
› The Atacama Cosmology Telescope: DR6 Constraints on Isotropic Time-Dependent Cosmic Birefringence from Axion-like Particles
› Neural networks applied to forecasting the astroclimatic and meteorological parameters in an operational context
› MOSS III: MeerKATs view on the galaxy populations in two massive galaxy clusters
› Science-Driven Performance Requirements for UV Coronagraph Design: Implications for O$_3$ Detection in Earth-like Atmospheres
› Understanding the Complex Morphology of a Coronal Mass Ejection. III: How to Create a Severe Geomagnetic Storm
› A Distinct Type of Standstill in Ultra-Compact White Dwarf Binaries
› Are Broad Mg II Galaxies Fading AGN?
› SQuIGGLE: Radio AGN Found Predominantly in Young, Gas-rich Post-starburst Galaxies at z ~ 0.7
› Emergence of high-mass stars in complex fiber networks (EMERGE) VII. Multi-Tracer Column Density Synthesis
› Galactic Outflows and Star-Formation Quenching: A JWST Perspective
› Studying the Near-horizon Jet of M87 using Millimeter Balloon-borne VLBI stations
› Chandra-JWST Probing the Effects of Moderate X-Ray Superflares on Protoplanetary Disks
› Paleo-heat flux estimates across Enceladus derived from flexural response of the ice shell
› Tracing Accretion and Inner-Disk Gas Evolution in the Orion Nebula via Br-alpha and CO
› The Limits of Tidal Circularization and Atmospheric Escape for Mini-Neptunes and Super-Earths: The Case of TOI-2257 b
› Twisted Pseudodisk and Asymmetric Mass Accretion on the Circumstellar Disk II: Parameter Survey
› The Contribution of Mergers and Accretion to Dark Matter Halo Assembly: An Excursion Set Theory Approach
› Transients and Stellar Activity as Revealed by Ultraviolet Diagnostic Tracers
› Deep X-ray View of a Distant Protocluster Anchored by a Quasar at $z=6.63$: No Evidence for Enhanced X-ray AGN Activity
› A JWST View of Cosmic Star Formation from $z\sim0$ to 9 with Hydrogen Recombination Lines in the COSMOS and GOODS-N fields
› Hot Molecular Hydrogen in Galaxies at Redshift ~ 0.2-1.5 Revealed by JWST
› Large-scale Environmental Dependence of AGN Activity Revealed by JWST Pa$\alpha$ Emitters
› ExoEcho: Exoplanet Ephemerides Change Observations. III. A JWST Survey for Transit Timing Variations of 37 Exoplanets
› Search for Sub-Solar Mass Binaries in the First and Second Part of LIGO's Fourth Observing Run O4a-O4b
› Magnetic Reconnection Governs the Entire Lifecycle of Solar Eruptive Magnetic Flux Rope
› Emission spectroscopy of KELT-2A b with Gemini-North/IGRINS-2: hints of a stellar C/O ratio and sub-stellar metallicity
› Simulations of Dust Content and Attenuation in $z=5-15$ Galaxies
› Optimal Design of Shaped Pupil Lyot Coronagraph for China's Large Segmented Telescope
› Barflow: Modeling Gas Kinematics of Bar-Driven Flows
› A possible evolutionary connection between high-mass X-ray binary pulsars and isolated rotation-powered pulsars
› Cosmology with strong gravitational lenses
› Development and characterization of a millimeter-wave circular polarization observation method using a quarter-wave plate with Simons Array
› Correlation of galactic very-high-energy gamma-ray sources detected by LHAASO with high-energy neutrinos
› Post-merger rotational evolution of magnetised single hot subdwarfs results in slow rotation due to magnetic braking
› Constraint on particle mass of dark matter based on XTE J1814-338 observation and DANS model
› Microcaustics: Fast GPU-Accelerated Dynamical Microlensing of Time-Dependent Extended Sources
› Evidence for Suppressed Non-thermal Broadening in a Flare Ribbon from Stereoscopic Observations
› High-Frequency Transverse Waves in Chromospheric Fibrils Revealed by DKIST
› Identifying Planetary Nebulae Candidates from IPHAS and VPHAS+ Surveys via YOLO Deep Learning Models
› Large dust grains escaping from a supernova remnant
› Strong gravitational lensing with Euclid
› A heterogeneous set of unusual quasars selected from astrometry and broad-band photometry
› specwizard: A Public Python Framework for Creating Synthetic Absorption Spectra from Hydrodynamical Simulations
› LiDO: The Large inclination Distant Objects Survey
› Linear Polarization of Synchrotron Radiation from Very-small-pitch-angle Electrons
› Black Hole Binary Mergers in Galactic Nuclei: Combined Effects of Secular Dynamics and Stellar Flybys
› PDRs4All XXIII. JWST-MIRI template spectra of PAHs in the Orion Bar obtained with blind signal separation
› Low-cost neural summaries for cosmological inference: an ensemble of convolutional neural networks trained on approximate simulations
› On-sky performance and prospects of near-infrared CMOS detectors in exoplanet detection: first year of SPIRIT
› RPCA: a Resolved PSF reconstruction method for undersampled images
› Sleeping or Dead? Probing the Quenching Mechanism of JWST Dormant Galaxies at z > 3 with ALMA
› The Role of Environment in Shaping the Assembly Timelines of Massive Quiescent Galaxies at Cosmic Noon
› The physical and chemical structure of TMC-1. The spatial distribution and excitation conditions of carbon, oxygen, and sulfur bearing species: Depletion of CO and CS
› Galactic Morpholography: Linking present-day galaxy compactness to assembly history and relic formation in the COLIBRE simulations
› Nova shells in 3D: I. A catalog of integral field spectroscopic observations
› Testing Departures from the $\Lambda$CDM model in f(T) Gravity with DESI DR2
› Stationary Resistive MHD Solutions Near an Isolated Three-Dimensional Magnetic Null
› Tracking a solar energetic eruption and associated energetic particles from Sun to spacecraft
› Flares and flux ropes: an entangled story
› HD 152384: A 5 Myr old debris disk system showing a gaseous ring of refractory elements at the dust sublimation radius
› Optical constraints on intranight variability in TeV HBLs from a two-year Asiago Schmidt monitoring campaign
› Uncovering the origin of complex velocity distributions in edge-on disc galaxies
› R&D activity in INAF on light instrumentation for continuous optical turbulence monitoring
› Search for High-Energy Neutrinos from Infrared Flares
› Galaxy-to-galaxy stochasticity has a limited impact on reionization and the 21-cm signal at fixed mean emissivity
› Revisiting the Optical F-corona from the Artemis II Total Solar Eclipse with RAW Data: How Far Can Consumer JPEG Images Be Trusted for Astronomical Photometry?
› Exact map-space beam convolution via spin-mapmaking
› Constrain the Size of Broad Line Region in NGC 1068 Using Sub-millimeter Excess
› HD 120678: a classical Be star with a tilting heartbeat disk
› The ringing Large Magellanic Cloud: evidence for a recent dwarf-dwarf collision
› Geometrical and Optical Design of the GUEST Laser-Ranged Test Masses for the Detection of Gravitational Waves in the $\mu$Hz range
› Thermalization of the Primordial Stochastic Gravitational-Wave Background
› IRAC-Excess Galaxies in the NIRSpec Wide Survey: physical properties of bright EELGs at $z\sim7$ and implications for Reionization
› Bouncing Bianchi Type I Universes with Interacting Vacuum
› Origin of the red spectral tilt in Inflation without an Inflaton
› Probing Planet Formation within 10 au: Dust Substructures in Extremely Compact Protoplanetary Disks
› Rotochemical heating of neutron stars in 2D
› Updates to STIS NUV Dark Calibration
› Joint Line Intensity Recovery from Multi-Tracer Cross-Correlations
› The contact frontier in Galactic civilization networks: radial structure and the Galactic habitable zone
› LHAASO Constraints on New-Source Cosmic Rays:Abundance Scenarios and Injection Spectral Indices
› A Parsec-Scale Transient High-Frequency-Peaked Radio Source in the Very Large Array Sky Survey Brightening and Fading over a Decadal Timescale
› A Step-Like Transition Underlying the Life and Death of Galaxies
› Modelling the 6.7 GHz Methanol Flaring in G358.93-0.03 Using the Maxwell-Bloch Framework
› Can bosenovae deplete the galactic dark matter?
› Revealing the Spatial Distribution of Dust and Plasma Solitary Waves in Jupiter's Innermost Magnetosphere Using Juno Waves Observations
› Dynamics of a switchback-like magnetic deflection induced by a propagating coronal jet
› Refurbishment and Cryocooler Upgrade of the CPAPIR Wide-Field Near-Infrared Camera: Design, Integration, and Lessons Learned
› Binary-lens amplification of starlight: from magnification flares to quasi-periodic tracking of orbital evolution
› GRB 181201A: Spectropolarimetric Constraints on Prompt Emission and Magnetic Field Structure
› International Astrophysical Consortium for High-energy Calibration: Summary of the 18th IACHEC Workshop
› Nonlinear Perturbations of Relativistic Stars
› Spinformation: do gravitational-wave events carry information beyond effective spins?
› Strong-Field Gravitational-Wave Lensing from Ray-Traced Arrival-Time Surfaces
› Black Hole Fine Structure
› The WDM time-frequency transform in gravitational-wave data analysis II: Evolutionary spectrum and noise covariance
› Magnetically Charged Black Holes from Grand Unified Theory
› Radion/Dilaton portal freeze-in dark matter in extra-dimensional theories
› Quantum noise and torque correlations in a torsion-bar Sagnac speed meter
› Testing Charged Black Holes Embedded in Anisotropic Matter and Surrounded by Plasma through Gravitational Lensing: Bounds from the Sloan Lens ACS Survey
› All Quiet on the Vector Front: Scalar Growth and Perturbative Control in Horndeski--Weyl-squared Gravity
› Correlation between gravitational wave frequencies as a signature of new black hole physics
› Biases in Ringdown Tests of General Relativity from Gravitational-Wave Microlensing
› $^{16}$O(p,$\gamma$)$^{17}$F Reaction and the C and O Isotopic Ratios in Red Giant Branch Stars
› Transient PULSE: Code for the Transient Propagation of UltraLight (pseudo)Scalars to Earth
› Dark Energy Survey Year 6 Results: improved mitigation of spatially varying observational systematics with masking for the MagLim++ lens sample
› Evidence of galaxy cluster rotation and intrahalo gas motions in the cosmic microwave background
› A Very Rich Bimodal Galaxy Cluster Merger: RXC J0032.1+1808
› Validation of Satellite Lifetime Predictions at Leonid Space
› The stellar-to-halo mass relation of central galaxies across three orders of halo mass
› CHRONOS Science Program
› Probing the magnetic field of a coronal mass ejection with PSR J1022+1001
› Identifying heating processes in simulations with an entropy-based scheme: A single jet episode in a galaxy cluster
› Delayed Radio Flares in Neutrino-associated Blazars: The Case of TXS 0506+056
› Probing scalar-tensor-induced gravitational waves in the nHz band: NANOGrav and SKA
› The DESIRED strong-line calibrations: I. New empirical metallicity relations for the local and high-redshift universe
› Probing the 3D Structures of Supernovae through IR Signatures of CO and SiO
› Astrophysical Parameters of 5056 Open Star Clusters from Bayesian Nested Sampling with PARSEC Isochrones
› Cosmo-PINN: A Physics-Informed Neural Network for Cosmological Reconstruction
› Time-reversed stochastic inflation in the quantum well
› Diocotron Modes in Pulsar Magnetospheres: Charge Diffusion and Implications for Radio Emission Variability
› WaveDM.jl: An Adaptable Simulation Framework for Dynamics of Baryonic and Wave Dark Matter on Galaxy Scales
› Testing the prevalence of hydrogen-silicate miscibility in young sub-Neptunes
› Investigation and Mitigation of a Prominent Off-Axis Stray Light Path in Rubin Observatory Commissioning
› Enhanced Astrometry of the Rapid ASKAP Continuum Survey: Mid and High Frequency Epochs
› Volcanic Satellites and Ion Escape in the Magnetospheres of Ultra-Cool and Brown Dwarf Stars
› Physical Characterization of Moon Impactor 2025-010D
› Hyperaccreting Magnetised Neutron Stars inside Rotating Massive Envelopes: Low-Power Jets and Precursor Flares
› Diameters and Temperatures VII: High-angular resolution measurements of Solar-type stars with the CHARA Array
› pynucastro 3: A community library for nuclear astrophysics
› Continuum Variability in AGN: Evidence for Systematically Suppressed Fluctuations in the BAL Population
› Modelling Fourier filtering wavefront sensors for PSD-based methods: the AOPERA tool
› Field-Level Baryon Acoustic Oscillation Reconstruction of the DESI DR1 Luminous Red Galaxies with Linear Field Transformer (LiFT)
› The Study of Detailed Morphology of Milky Way Dwarf Galaxies: Draco and Bo\"otes I
› Evolving dark energy and a younger Universe from cosmic inhomogeneity
› A forest of emission lines observed by Sunrise III/SUSI above the solar limb
› Vector field dark matter search with Sagnac interferometer
› Rotational excitation of SiC$_6$ by collisions with helium: cross sections, rate coefficients and non-LTE modeling
› Axial-Dipole and Equatorial-Dipole Coronal Holes: Congruent Magnetic Geometry, Divergent Evolution
› How much can shape degeneracies affect the Hubble constant measurement?
› Scaling Up: A Global Optical/X-ray Correlation For Reprocessing Across Black Hole Masses
› 3D Global Climate Simulations of Synthetic Mars Warming
› Searching for Ultra-Light Axions with Twisted Cavity Resonators of Anyon Rotational Symmetry with Bulk Modes of Non-Zero Helicity
› Cosmic Rays as an Interdisciplinary Earth Observation Tool: From Particle Physics and Atmospheric Processes to Geosciences and Urban Science
› Correlative Microstructural Analysis of a Weathered Nantan Meteorite Fragment
› Collider Probes of Dark Energy Microphysics
› Axion Misalignment Across First-Order Phase Transitions
› Quantum Field Theory Of Cosmological Perturbations Induced By Ultralight Dark Matter

  ↓↑    

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