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 Orion Nebula (M42) imaged from Mt. Suhora
The Orion Nebula (M42) imaged from Mt. Suhora
S Webcam

S Webcam

Webcam

N Webcam

Allsky

S Sky

Temperature
-- °C

Humidity
 --%

Wind
-- km/h

Pressure
-- 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:
› A Parsec-scale Circumstellar Shell Around VX Sgr: Mass Loss and RSG/T\.ZO Nature
› JWST Observations of RR Lyrae in Leo P
› The impact of nonlinear Landau damping on cosmic ray streaming and the role of external turbulence
› A Vision for Little Red Dots in the Low-Redshift Universe with ALMA2040
› The Impact of High-Mass Clusters on the Binary Black Hole Merger Rate over Cosmic Time
› A Misaligned Debris Disk relative to the Host Star CPD-72 2713 from JWST/NIRCam Imaging
› Efficient numerical evolution of self-gravitating systems with dark-matter-baryon scattering
› CoRGI in MaNGA - II. NGC 5717: cold-gas accretion and disk growth in a BGG
› How Little Red Dots Turn Blue: Evolution of Kelvin-Helmholtz Contracting Black Hole Envelopes and Observational Diagnostics
› Tracing small-scale structure formation through cosmic time with strong gravitational lensing: A case for a next-generation sub-millimetre/millimetre interferometer
› Probing ordered magnetic fields in galaxies across cosmic time
› The Pristine survey XXIX. Data Release 2: Photometric metallicities for 15 millions stars down to $G\sim 20.5$
› Planet forming disk populations and their connection to the environment
› The unified Bound Dark Energy--Bound Dark Matter model: theory and constraints from DESI DR2
› HI rotation curves and mass-size relation for 568 galaxies from the Apertif Wide-area Extragalactic Survey
› Wandering intermediate-mass black holes and off-nuclear tidal disruption events from early star clusters
› Nonlocal Gravity, Restricted CPL Dynamics and DESI Constraints
› An Attenuation Bump at z=9.3: Probing Dust Diversity at Cosmic Dawn
› A model for the ongoing subcluster interaction in Centaurus
› Has JWST Seen Everything? Hunting for "NIRCam-dark" Dusty Star-Forming Galaxies at $z \simeq 6 - 9$ with ALMA2040
› ALMA2040: Understanding the Early Assembly of Galaxies - The Formation of Star-Forming Clumps and their Role in Shaping Galaxy Evolution
› Compact Dark Matter with Globular Cluster Pulsars
› The dawn of the first galaxies
› A Search for Dust in the Outflow of the HH212 Class 0 Protostellar System
› Beyond Mergers: the Role of Metallicity in Forming a Reservoir of Massive and Detached Binary Black Hole Systems
› The ALMA-QUARKS Survey. IV. Core Mass Function and Evolutionary Trends in Core Formation Efficiency and Chemistry
› Understanding cosmic explosions
› mm-jets in the multi-messenger era
› uGMRT Polarization Observations with Walsh Modulation
› Multi-Method Machine Learning Classification of Astronomical Sources with Rubin Data Previews: a Spectroscopy-Free Approach with DP1 and DP2
› What fuels the growth of stars and black holes in galaxies through cosmic time? The physics and chemistry of the interstellar medium in distant galaxies
› The optical colors of hidden spiral-like features in nine Virgo early--type dwarfs
› Modal estimation of high-order wavefront drifts on coronagraphic testbeds for high-contrast direct imaging of exoplanets
› Correlated Radio Frequency Interference Monitor for Radio Telescopes
› Study of pulse jitter characteristics of PSR J1744-1134: Towards high precision pulsar timing with InPTA
› FUGUE: A New GPU-accelerated General Relativistic Magnetohydrodynamics Code with Weak-Field Multipole Self-Gravity and Quasi-Stationary Kerr Black Hole Evolution
› Unveiling the Baryon Cycle Through Cosmic Time
› Self Calibrated Galaxy Groups from the DESI DR1 Bright Galaxy Survey
› Optimization of multi-resolution observation strategies for cosmic microwave background experiments
› The energetic atmosphere of the Sun
› JWST reveals a highly ionized nebula powered by an ultraluminous X-ray source with a massive black hole in the metal-poor galaxy Holmberg II
› A model for the image structure and spectral energy distribution of relativistic jets
› Disentangling geometry & growth in cosmic neutrino mass constraints: a more physical split and diagnostic
› EPRV Asteroseismology of the K dwarfs GJ 570 A and GJ 783 A with ESPRESSO. Empirical mode-amplitude scaling in tension with 3D convection simulations
› ACACIAS II: element abundances for 39 stars in the dwarf galaxy Sculptor
› Detecting and Identifying Supernovae in AGN Accretion Disks
› Finite-Element Asteroseismology I: Two-Dimensional Adiabatic Oscillations of Rapidly Rotating N=3 Polytropes
› Neutrino production at the extreme vicinity of supermassive black hole in NGC 1068
› Orbital Stability of Apsidally Aligned Planetary Systems
› ALMA observations towards M83 reveal N2H+ tracing dense gas
› CHARIZARD: A High-throughput Generic Pipeline for Present and Upcoming Interferometers
› Dark Matter Particle Explorer: Ten-Year On-Orbit Performance and Scientific Outcomes
› An Energetic Consistency Test for Feedback-Driven Gas Loss in Milky Way Dwarf Satellites
› A machine-learning-driven dataset of 144,111 polycyclic aromatic hydrocarbon infrared spectra for interpreting aromatic infrared bands
› Dust Activity Evolution and Constraints on Icy Grains in the Interstellar Comet 3I/ATLAS
› The Birth and Early Feedback of Massive Star Clusters Across the Local Universe
› Disk tilts in Milky Way-like galaxies and their link to mergers
› Post-perihelion dust activity and a candidate icy-grain halo in long-period comet C/2023 A3 (Tsuchinshan--ATLAS)
› Are High-EW LAEs good analogs for the earliest galaxies? A study on the ionizing conditions and gas properties of LAEs at $2\lesssim z\lesssim7
› Model-independent parameters from DESI DR1 LRG2 with an explicitly varying power-spectrum shape
› Optical observations of supernova candidates with the ILMT
› Thermodynamics of Viscously Heated Circumplanetary Disks
› Unveiling star formation at sub-solar metallicity with ALMA2040
› Resolving the Assembly of Disk Galaxies from the Epoch of Reionisation to Cosmic Noon
› Dust at cosmic dawn: unveiling the onset of dust and obscured star formation at $z\gtrsim8$
› Identification of ultra-high-energy neutrinos in vertical air showers with surface detectors
› Polarization Properties of Thomson-Scattering Triaxial Ellipsoids
› Probing cold gas and dust in quiescent galaxies across cosmic time
› Direct measures of black hole masses through cosmic time
› A ${}^{13}$CO Detection in a Massive Molecular Gas Flow in Abell 1795's Central Galaxy
› An HST survey of photometry and multiplicity of brown dwarfs and planetary-mass objects in the field of Taurus
› A Shell Collision Scenario for EP251222b/GRB 251222A: Connecting Prompt Emission and Double-Peaked Afterglow
› Probing fundamental physics with ALMA2040 mm-wavelength observations of neutron stars
› A clump population framework for star formation across galactic scales
› Thermal Sunyaev-Zel'dovich Effect in the circumgalactic medium - III: does richness matter?
› A first look at the protoplanet WISPIT 2 b with VLTI/GRAVITY+
› Beyond the Beacon: State and Corporate Competition after an Information-Rich Technosignature Detection
› Tracking the flow of interstellar gas across scales: from galaxies to star clusters
› AGN Feeding and Feedback: Resolving the Torus
› Molecular atlas of nearby galaxies through sensitive high-resolution multi-band molecular line surveys
› Mixed modified-gravity--modified-inertia MOND theories
› WALTzER: Wide-band Atmospheric Laboratory for Transiting Exoplanet Research
› Minkowski Functionals of CII Line Intensity Maps: Probing Astrophysics and Primordial Features
› Hydrostatic Equilibrium Constraints on the Fuzzy Dark Matter Mass from Dwarf Spheroidals: Method, Systematics, and Robustness
› From local chemistry to galactic evolution: unlocking the power of interstellar isotopes with ALMA2040
› ALMA2040: The High-Redshift Circumgalactic Medium. Imaging the fueling and feedback of galaxies in the early universe
› Extracting the Central Sound Speed of Neutron Stars through Intrinsic Stellar Structure Scaling with Reduced Equation-of-State Model Dependence
› Evolved stars, multiplicity and planets: Shaping and Being Shaped by Stellar Evolution
› Secular Evolution of Quasiperiodic Eruptions: eRO-QPE2
› Frontiers of chemical complexity in the interstellar medium: unveiling the cosmic origins of life
› Evolved stars: dust formation and mass loss
› Convective Oscillations of Cosmic Rays
› From Scaling Relations to Physical Laws: Constraining the Physics of Star Formation Across Local Galaxies
› Planet formation on solar system scales
› Star Formation across the Galaxy
› Stimulated capture of axion dark matter around primordial black holes
› Planetary system architectures in the final stages of planet formation
› Intermediate- and high-resolution optical spectroscopy on the nascent planetary nebula Vy 2-2: Evidence of binary-star evolution
› Disentangling Multi-epoch Single-lined Binary Star Spectra to Reveal Interstellar Medium Features via MCMC
› Time-reversible timestepping in many-body planetary systems
› Influence of numerical domain design in simulations of solar coronal heating with the MAGEC code
› Multi-wavelength Polarization as a Probe of Planet Formation
› Missed Detections and False Alarms in a CNN Technosignature Detector on Breakthrough Listen Data
› Chemistry on solar system scales
› The Radius-Luminosity Relationship for Active Galactic Nuclei with Hierarchical Bayesian Reverberation Mapping
› A Comprehensive AGN Inventory for the Dwarf-Dominated RESOLVE and ECO Surveys: Mass-Dependent AGN Types and Occupation Fractions
› Are $E>B$ regions essential for particle injection in relativistic magnetic reconnection?
› The gravitational constant and the cosmic microwave background
› The Mission Market: Flying NASA's Vetted, Unflown Science
› Investigation of an X-class Flare and Quasi-Periodic Pulsations in NOAA AR 13842 using SDO, Aditya-L1 and Solar Orbiter
› X-ray point sources towards the giant radio lobes of Centaurus A
› Stellar Mass Census of $S^4G$ Local Bars
› Properties and limitations of linear models for mutual coupling in 21 cm arrays
› Dark Matter in the Galaxy: Insights from the Dynamics of Stellar Streams
› ALMA2040: Mapping the Spatially Resolved Dust and Star Formation Physics Driving High-z Galaxy Assembly
› ALMA2040: Submillimeter-wave Limb Sounding of Venus and Mars
› High-frequency water megamasers as precision probes of black holes, galaxies and cosmology: A case for a next-generation sub-mm/mm interferometer
› Bridging the gap between stars and planets
› A Sample of Thick-Disk Stars Hosting Hot Jupiters
› Millimetre/Sub-Millimetre SETI: Expanding the Radio Technosignature Parameter Space with ALMA2040
› A New Method for Constraining 3D Exoplanet Atmospheres: Application to WASP-94A b's Panchromatic Spectrum
› Chemical Demographics of Star-forming Regions
› Identifying deformed exoplanets with JWST and Ariel: A target selection metric for phase curve observations
› Singles in Disguise: Kepler's Low-SNR Single-Transiting Systems as Incompletely Detected Multis
› LSST and Keck characterization of outer Main Belt comet P/2026 N2
› Breaking de Sitter Symmetry with Cosmic Topology: Cosmological Role of Infrared Vacuum Freedom
› The Forgetful Black Hole: Memory Burden and Hysteresis in Hawking Evaporation
› Coherent states of neutrinos in rotating matter
› Leptogenesis with a GeV-Scale Quasi-Dirac Neutrino
› Optimal Strategies for Gravitational-Wave Memory Detection with Noise Marginalization in Pulsar Timing Arrays
› Testing the inelastic dark matter interpretation of the LZ event with heavy-element experiments
› Displacement-noise-free gravitational-wave detector using quantum tomography of photon orbital angular momentum states
› Numerical simulations of low-mass black hole-neutron star mergers with moderate eccentricities
› From Cosmic Bounces to Primordial Black Holes: The Role of Primordial Magnetic Fields
› From Non-Thermal to Thermal: Cosmological Imprints of Self-Interacting Secluded Dark Matter
› Breakdown of hydrodynamic universality in causal first-order viscous neutron star oscillations
› Modified hydrogen recombination rate due to non-Hubble redshift effects
› From Axion Detection to Dark Matter Astronomy
› Axion String Source Modelling
› Multi-phase investigation of outflows in the circumgalactic and interstellar media of luminous quasars at z~5
› Barycenter kinematics in Local Group analogues
› Jittering jets in stripped-envelope core-collapse supernovae
› Constraining Dark Acoustic Oscillations with the High-Redshift UV Luminosity Function
› The formation of merging black holes via stable mass transfer in massive binary stars
› Using 23 Years of ACS/SBC Data to Understand Backgrounds: Significant Reductions in Expected Background Levels
› Using 23 Years of ACS/SBC Data to Understand Backgrounds: Explaining & Predicting Background Variations
› Dark matter dynamical friction on binary stars in the faintest dwarf galaxies: I. Analytical approach
› Confidently Wrong: Why Ignoring Binaries Biases IMF Inference at Large Sample Sizes
› The impact of gamma-ray propagation effects on indirect dark matter searches
› Mock Catalogs of Strongly Lensed Gravitational Waves via a Halo Model Approach with Space-borne Detectors
› A grid of fast-rotating, chemically-homogeneous, supernova and/or long-GRB progenitors
› Dissecting the 3D chemo-dynamical structures of NGC~1381: A galaxy hosting an ancient slow bar with an accretion-related bulge and thick disc
› Repulsive ultralight dark matter from Hosotani mechanism
› A Deep Look at the Ultra-Faint Milky Way Satellite Virgo III with Rubin Observatory Data Preview 2
› Co-design of ground-based gravitational wave detector networks
› ATLAS. III. Dust Around Little Red Dots: Hydrogen Line Ratios beyond Dust-free Non-Case B Models
› A binary black hole merger rate comparison within the same metallicity-star formation rate framework
› The Kick Velocities of Neutron Stars in Binary Systems
› TEMPUS: Relativistic coordinate time scales for any solar-system body from arbitrary ephemerides
› Beyond the BLUE I: the advantage ceiling - how much can any estimator beat the matched filter in mm/submm survey data?
› The optical high-resolution spectral archive of the HERMES spectrograph mounted on the 1.2m Mercator telescope
› JWST lensed quasar dark matter survey V: Hints of self-interacting dark matter from 29 quadruply imaged quasars
› Fast X-ray Transient EP260321a: Shock Breakout through an Extended Circumstellar Matter
› XuYi Interferometer Observation Simulator
› LazyTB: Extended LTB-solutions with Multiple Interacting Fluids
› Radio Continuum Study of One of the Brightest Large Magellanic Cloud Supernova Remnants N 132D
› Self-Interacting Dark Matter: From Particle Physics Theories to Structure Formation Simulations
› New Massless Spectra from Cosmic String Cusps
› Radial Oscillations of Viscous Stars
› Linear causality and stability constraints on relativistic second-order magnetohydrodynamics
› Classical conformal invariance and superhorizon dynamics in de Sitter
› ACT stands for Awkward Cosmology Theories
› Temperature effects on white dwarfs in modified gravity

  ↓↑    

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