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: Dome at sunrise
Dome at sunrise
S Webcam

S Webcam

Webcam

N Webcam

Allsky

S Sky

Temperature
11.1 °C

Humidity
 80%

Wind
0.0 km/h

Pressure
1018.7 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:

› The Local Star Formation Environment Predicts Young Star Cluster Radii: Evidence from PHANGS-MUSE H-alpha Maps
› Environmental dependence in the halo model informed by the FLAMINGO simulations
› Missing Light, Misleading Confidence: Optical-Module Readout Loss and Signal Reliability in Neutrino Telescopes
› Analysis of Binary O-type Star Systems Using Recurrent Neural Networks
› Multiline Spectropolarimetric Evidence for Photospheric Reconnection in Ellerman Bombs from DKIST
› A Two-Population von Mises--Fisher Distribution of the Magnetic Field Direction in the Young Solar Wind
› Consistently Reproducing Early Galaxy Observations and 21-cm Signal during the Epoch of Reionization
› Extending SOMPZ beyond Spectroscopic Coverage for Roman Weak Lensing
› Multimessenger Probes of Primordial Black Holes with Gravitational Wave and 21 cm Observations
› Beyond the dust: JWST reveals extinction and ice content in local (U)LIRGs
› Beyond the Disc--Spheroid Dichotomy at $0.6 < z < 8.0$: Evidence for a Morphological Indeterminacy Regime from JWST
› Microbial Methanogenesis on Mars: A Life Detection Target for an MLE-Type Mission and Future Human Exploration
› Can Blue UV-Bright Galaxies Drive Reionization at Cosmic Dawn? An $M_{\rm UV}=-19.6$ Galaxy with $f_{\rm esc}\approx0.85$ at $z=9.244$
› The evolution of 3C 306 in the galaxy cluster RXCJ1454.4+1622: linking spectral ageing, ICM conditions, and jet dynamics through MHD simulations
› A DECADE of Giants: A catalog of 42,000 optically identified galaxy clusters from 13,000 $\mathrm{deg}^2$ of the sky
› Modeling Multi-band Active Galactic Nuclei Lightcurves Using an Self-supervised Attentive Neural Process Network
› Mass-loss Rates of 74 Bow Shock OB Stars: No Evidence for Bi-stability Behavior
› rapidsim: A Python interface and cross-platform distribution framework for the RAPID protoplanetary disc simulation code
› Intermittent turbulence as the driver of stochastic heating in the near-Sun solar wind
› Magnetic-field constraints for four magnetic cataclysmic variables from simultaneous continuum and cyclotron modeling
› PRIMA prototype spaceflight KID readout electronics laboratory characterization
› Spiraling into the `snail' cluster MCXC J0157.4-0550
› Numerical estimation of the capture ability of Neptunian mean motion resonances II. Influence of eccentricity and inclination
› Critical magnetic Reynolds number of the weakly-collisional turbulent dynamo in supersonic plasmas
› Prospects for submillimeter VLBI of black hole photon rings with a stratospheric balloon-borne telescope
› Models of spectral bumps of primary cosmic rays and multi-messenger tests
› Statistical Strong Lensing V. Inference with Microlensed Quasars
› Granulation in Color: The Chromatic Stellar Flicker of LTT-9779 and WASP-121
› Newly Identified Planetary Nebula Candidates in M31 using Deep-Learning Search of Hubble Space Telescope Images
› Forecasting the Resolvability of Stellar Velocity Dispersions in Ultra-faint Dwarf Galaxies
› Radar and Infrasound Observations of the 2026 May 30 Cape Cod Bay Superbolide
› Robustness of C/O and mean molecular weight under disequilibrium chemistry
› Attitude Estimation of Falcon 9 Rocket Body Based on Photometric Characteristics
› Galactic warps constrain equivalence-principle violation in the dark sector
› Clumpy Outflows from Super-Eddington Accreting Black Holes. II. Conditions for Clump Formation
› Gravitational filtering, magnetic-field inhomogeneity and Coulomb collisions in a kinetic model of a plasma atmosphere with stochastic heating at its base
› Inverse-designed tapers to improve throughput of on-chip astrophotonic spectrographs
› V347 Aurigae: from Peak to Quiescence
› Mid-infrared Imaging of SR 12 c with JWST/MIRI: Grain Growth in an Evolved Circumplanetary Disk
› The Impact of an AGN on PAH Spectral Features in Galaxy Evolution Simulations: Continuum Dilution and Excitation of PAHs
› Long-term ultraviolet variability of Taurus T Tauri stars from the IUE archive
› An Enhanced Intersecting-Lines Method for Optical Loss Characterization in SIS Heterodyne Receivers
› Impact of Residual Gain Errors on the Detectability of Ionized Bubbles during Reionization with SKA 21-cm observations
› Tidal Disruption Events in Active Galactic Nuclei: Thermal Radiation and Jets
› A 4-20 GHz Superconducting 90deg Hybrid Using Capacitively Loaded Coupled Lines for 2SB Heterodyne Receivers
› Single-Transit Parameter Estimation with Calibrated Uncertainties
› The Star Formation Histories of Different Components of M31's Halo from Photometric Estimates of Fe and $\alpha$ Abundances
› Simulations of Particle Acceleration by an Interplanetary Shock Observed at 0.07 au and 0.7 au
› Spectroscopic Studies of Meteors within the Skytinel Network
› MACE: Multigroup-Multiangle Integrated Thermal Compton Scattering Kernel
› Beyond dust in local cosmography: perturbative Vlasov predictions
› Companions of Hot Jupiters: two decades of radial velocity monitoring with CORALIE
› Mode power and stability in radial post-AGB pulsations
› IMF-aware N-body forward modelling of membership selection functions for young open clusters
› Activity Cycles in Solar-Type Stars
› Ultraviolet accretion continua reveal a transition in T Tauri magnetic topology
› Statistical Analysis of Neutron Star Cooling: Implications for the Nuclear Equation of State and Nucleon Pairing
› Dynamical response of a protoplanetary disk to an FU Ori-type outburst
› Connecting galaxy structure, quenching, and halo environments during cosmic noon
› Hyperonic Direct-Urca Neutrino Emission with Lattice-QCD-Informed Form Factors
› The Next Generation Virgo Cluster Survey (NGVS). XXIX. Demography of Nuclear Star Clusters
› Characterization of integrating-sphere systematic effects for photon calibration of the KAGRA gravitational wave detector
› Reading Between the Lines: How Much Information Remains After Fitting a Stellar Spectrum?
› Constraints on the Progenitor of SN 2023bee from its Nebular-Phase Spectra
› Plate-YOLO: An End-to-End Object Detection Framework for Robust Astrometric Registration of Historical Plates
› Velocity-resolved Ionization Mapping of the Broad-line Region. II. Signatures of Eccentric Broad-line Regions from a Quantitative Photoionization-Based Model
› The DARWIN Project: Cosmological Simulations of Galaxy Formation down to Dwarf Scales in Diverse Environments
› A Morphology-Based Cross-Tracer Ratio for Robust BAO Tests
› Hostbusters: constraining $H_0$ and binary formation channels through gravitational-wave host galaxy associations
› A high-Galactic-altitude scattering screen: scintillation from Globular Cluster pulsar M53A
› Constraints on the Cosmic Expansion Rate Using the DECam Local Volume Exploration Survey and the Fifth Gravitational Wave Transient Catalog
› Gravity-mode main-sequence asteroseismology of 16 open clusters and associations
› Gravitational Instability of Cold Axion Dark Matter Beyond Minimal Coupling
› Kinematic structure and age of a Scorpius--Centaurus subcomponent: implications for PDS 70 planetary system
› A 36.34-day Sub-Neptune Candidate Transiting the Nearby K Dwarf TIC 402710280
› The Solar System through dust maps. Encounter statistics with interstellar gas
› Late-time distance consistency and model-independent curvature inference with strong lensing, quasars, and galaxy clusters
› Pulse Morphology and Spectral Study of LPT J1634+44 Using GMRT
› Probing the Interstellar Medium towards the Double Pulsar and the Gum Nebula using Low-Frequency Pulse Broadening Measurements
› Effect of galaxy mergers on dust masses
› Competitive roles of turbulence and magnetic field on the formation of unipolar outflows in isolated molecular cloud cores
› Disc breaking and parametric instability in warped accretion discs driven by differential precession
› Kinematics and Thermodynamics of Coronal Mass Ejections
› Linear Polarimetry of the Solar Corona during the Total Solar Eclipse of 8 April 2024: Multi-Band Observations and HDR Imaging
› Linear gas mass density: a unifying descriptor of Cosmic Filaments
› The Central Molecular Zone of our Galaxy, a chemical complexity factory: first interstellar detections of molecules towards G+0.693
› The Milky Way's Early Disk Was Built in Bursts. I. Evidence from Low-angular-momentum, High-$\alpha$ Stars Scattered Out of the Protodisk by Merger Events
› Star formation history of Draco revealed by DESI DR1: suppressed early star formation efficiency for Milky Way dwarf galaxies
› The accretion flow and jet of M87: broadband modelling across spatial scales
› Joint Fit of Galaxy Cluster Scaling Relations from Individual Weak Lensing Data: Comparison with Stacked Analysis and a Real Data Test
› Exploring the Evidence for Evolving Dark Energy with the Jeffreys prior
› PRISMS/U13151. A Glimpse into the Earliest Phases of Galaxy Formation through an Ultra-Faint System $\approx$ 500 Myr after the Big Bang
› Probing the Assembly of Triangulum: Precision Metallicities and $\alpha$ Abundances of M33's Star Clusters from APOGEE Integrated-Light Spectroscopy
› Extending the M33 Extinction Map with Radio and Far-Infrared Gas Observations
› The EMA Justitia Probe: Terminator Frame-Based Deployment Orbit Selection and Surface Coverage Analysis
› ERGO-ML and how to directly infer the multi-temperature nature of intra-cluster gas: simulation-based inference with TNG-Cluster
› Evolving only the observed spacetime region: perfectly parallel lightcone simulations with sCOLA
› Neutrino self-interactions in light of DESI and CMB-SPA
› Detection Forecasting for Blazars at MeV Energies with Fermi-LAT Swift-BAT Cross Match
› Mean-Field Backreaction in Single-Field Inflation
› Deep X-ray Observations of the Gamma-ray Bright Pulsar Wind Nebula HESS J1303-631
› Cosmological implications of two mock TianQin standard siren catalogs generated under different background cosmological models
› X-ray Comptonization in an Accreting Kerr Black Hole System with a Tilted Disc and Thermal Corona; A General-Relativistic Monte Carlo Simulation: I. Model, Radiative Transfer and Spectral-Timing Properties
› Low-mass and High-sSFR H$\alpha$ Emitters at $z \sim 2$ in the ZFOURGE-COSMOS Field
› Energy extraction from a rotating black hole via magnetic reconnection: Bumblebee gravity
› Cislunar navigation is an observability problem: arc-length thresholds, Gramian conditioning, and the Doppler lever
› How do late-time photons "record" primordial curvature perturbations?
› Breaking the axion abundance-isocurvature relation: Scale invariance and high-scale inflation
› Static tidal Love numbers of Schwarzschild and non-Schwarzschild black holes in quadratic gravity
› Moser Regularization of the CR3BP for Symmetric Orbits: Bifurcation Networks of Lunar Orbits
› Destinies of Plasmoids Formed from the Magnetic Reconnection Occurring within the Ergo Region of a Rotating Black Hole
› Multigroup Implicit Monte Carlo Radiation Hydrodynamics on Moving Voronoi Meshes with STORM and RICH
› Moving Beyond Quasinormal Modes and Reinterpreting Direct Waves in Binary Black Hole Merger-Ringdowns
› Lorentz-Invariance Violation with neutrinos from gamma-ray bursts using IceCube High-Energy Starting Events 12-year dataset
› Upper bounds on the number of images produced by point-mass lenses at different distances
› Hubble Susceptibility: Beyond Effective-Mass Spectroscopy in the Cosmological Collider
› HyQ-LC: Improving Light-Curve Classification with Hybrid Quantum--Classical Learning
› Searching for lensed gravitational waves with unlensed templates
› Primordial black holes in braneworld gravity: A gateway to hidden dimensions and the dark Universe
› Dark Matter Interpretations of the Galactic Center Gamma-Ray Excess with 18 Years of Fermi-LAT Data and the FL16Y Source Catalog
› The FENIKS Survey: Stellar-Halo Mass Relationship of Central and Satellite Galaxies in UDS and COSMOS at 0.2 < z < 4.5
› Novel geometrical test of cosmological expansion from photometric data
› Antenna Technology Readiness for the Black Hole Explorer (BHEX) Mission
› Supernova dust synthesis --- Carbonaceous dust in the very early universe
› Redshift Assessment Infrastructure Layers (RAIL): Rubin-era photometric redshift stress-testing and at-scale production
› Revisiting the CMB homogeneity scale: low multipoles removal effect and extragalactic foreground masking
› Towards the Habitable Worlds Observatory: Retrieval of Reflection Spectra from Evolving Earth Analogues using 1D CNNs
› A High Incidence of Mid-infrared Variability in Local Ultraluminous Infrared Galaxies
› Structure of Turbulent Radiative Mixing Layers
› A New Bayesian Framework with Mass-Radius-Space Priors to Constrain the Neutron Star Equation of State
› The MAGPI Survey: co-evolution of baryons and dark matter in star-forming disk-like galaxies at $0.1 \lesssim z \lesssim 0.85$
› Primordial Black Hole Abundance from Reionization
› Effects of Viscosity on Sloshing Cold Fronts in Galaxy Clusters
› A targeted machine learning approach for detecting diffuse radio emission with Astronomaly: Protege
› oMEGACat. IX. Chemical Tagging of Omega Centauri Populations with Machine-Learning-Inferred Abundances from the MUSE Spectrograph
› Testing the isothermal Jeans model for self-interacting dark matter halos in the collapse phase
› Robustness of Neural Networks for CMB Polarization Foreground Removal
› Stars with Plumbing Issues: The Multi-component Ejecta of Common Envelopes
› From photometric surveys to HI intensity mapping: Improving constraints on magnification biases while testing gravity
› Tidal Heating of Stellar Clusters in Fuzzy Dark Matter Halos
› Unveiling Hidden Lyman Alpha Emitters in the DESI DR1 Data
› The Metallicity Distribution of the Ultra-Faint Dwarf Galaxy Segue 1
› A 4200-hour HyperFlash and \'ECLAT campaign on the hyperactive FRB 20240114A: constraining energetics with the most brilliant bursts
› Impact of the equation of state on core collapse supernovae I: the low-$T/|W|$ instability
› Ultraviolet diversity of Little Red Dots as a probe for direct-collapse black hole ages
› Prospects for Astrobiology and Technosignature Searches with the Vera C. Rubin Observatory Legacy Survey of Space and Time
› Intermediate States in Chaotic Triple Evolution and Applications to Black Hole Merger Statistics
› Something green beneath the surface: The dynamical nature of Fossil Structures in IllustrisTNG-100
› A cross-calibration approach for polarisation-sensitive detectors in CMB experiments: application to LiteBIRD's polarisation angle calibration
› JWST Characterization of Earth Quasi-Satellite (469219) Kamo`oalewa
› A comprehensive Gaia DR3 study of the open cluster NGC 6134: Bayesian distances, present-day mass function, mass segregation, and structural decomposition
› Debris Disc Substructures Induced by Secular Planetary Perturbations
› When X-ray Features Fail to Identify Intrinsic Emitters: Label Noise and Luminosity Overlap in Machine Learning Classification of AGN and Star-forming Galaxies
› Morphological Bias: How Ellipticals and Spirals Trace the Cosmic Web Differently
› The stability of radially anisotropic rotating stellar systems with a central density cusp
› Influence of local and global solar magnetic fields on medium-term forecasting of the number and parameters of coronal mass ejections
› NAPTIME: A Neural-Process Framework for Rubin Alert Classification
› STORM: RDMA-based Monte Carlo Transport Scheme for Distributed-Memory Particle Simulations
› Probing an Intermediate-Mass Black Hole Companion of Sagittarius A* with Pulsar Timing
› Magnetic pressure anisotropy in ultra-dense white dwarfs: Landau quantization and neutronization effects
› The impact of recombination during tidal disruption events
› A deep learning algorithm for black hole spin estimation using hot-spot secondary images
› A giant magnetic eruption from the asymptotic giant branch star Mira A
› Molecular and Atomic Gas Associated with the Gamma Ray Supernova Remnant RCW 103
› The Impact of Errors in the Shape Function of Rotating Neutron Stars in the Oblate Schwarzschild Approximation
› The onset of the strong backreaction regime in axion inflation, an analytical study
› Accretion Rates and Thermohaline Convection in Polluted White Dwarfs
› Calibration of the Next Generation Palomar Spectrograph as a Stellar Speedometer
› Consistency and precision of very long baseline interferometry source coordinate time series
› Error Propagation from Integral Moments and Spectral Derivatives of Stokes Profiles to Magnetic Observables
› Re-interpreting the GRS 1915+105 observations within the variable TADAF scenario
› Chondrule size averaging in two and three dimensions
› Towards breaking the degeneracy between stellar ages and unresolved multiplicity
› The Structure in the Structure Function of Black Hole Light Curves
› 3D Global Climate Simulations of Synthetic Mars Warming
› Galactic Outflows and Star-Formation Quenching: A JWST Perspective
› The dawn of the first galaxies
› Neutrino production at the extreme vicinity of supermassive black hole in NGC 1068
› Dark Matter Particle Explorer: Ten-Year On-Orbit Performance and Scientific Outcomes
› Improving Slow-Roll Estimates in Starobinsky Inflation Using an Analytic Hubble Parameter
› Gravitational waves from cosmic superstrings and gauge strings
› Relative Jump Distance: a diagnostic for Nested Sampling
› A mass invariant in a compressible turbulent medium
› Probing Compact Binary Coalescences in the Decihertz GW Band with IndIGO-D
› Gravitational Wave Propagation in K-essence Cosmology: Theory and Observational Constraints
› Stochastic scalar-tensor inflation and beyond
› SPLIT: Loosely-coherent inference of long-inspiral gravitational-wave sources for robustness against modeling and data outliers
› Massive Graviton Dark Matter from a Gapped Continuum
› Decoupling Limit of Quiver Theories and the Angular Spectra of Extreme C-metrics
› Gravitational-wave parameter estimation with machine-learning generated surrogate waveforms
› MADGRAV: a multilevel anomaly-detection pipeline for gravitational-wave searches applied to LIGO data
› Multi-Band Constraints on Cosmic Strings: Unifying Harmonic and Burst Spectra

  ↓↑    

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