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
16.9 °C

Humidity
 69%

Wind
9.7 km/h

Pressure
1013.0 hPa

Moon

Moon

 News from astronomynow.com

› 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
› Dark matter may come in multiple forms, new model suggests
RSS  Latest preprints on astro-ph:

› Bayesian Inferences on Analytical Equations of State Approximations of Neutron Stars
› $\Lambda$CDM in a courtroom
› Inhomogeneous Cloud Coverage and Altitude-Dependent Heat Transport on the Hot-Jupiter NGTS-10 Ab from its Optical-to-Infrared Phase Curve
› A Dark-matter Origin of Little Red Dots: Early Seeding and Super-Bondi Accretion
› On the dynamical accessibility of twin stars
› CMB-HD Foregrounds: Simulations, Source Detection, and Foreground Removal
› Population III Host Candidates at $z\sim2$: Strong He II $\lambda1640$ and Absent UV Metal Lines in HETDEX Ly$\alpha$ Emitters
› A pair of unequal jets imparted the kick velocity to the neutron star of Cassiopeia A
› Dynamic Accretion Disk-Corona Connection and Broad Fe K$\alpha$ Variability in Mrk 766 Revealed by Time-Resolved High Resolution X-Ray Spectroscopic Analysis
› Jet Feedback and the Self-Regulated Growth of Black Holes Embedded in AGN Disks
› Optical Spectroscopy of a Candidate O-Star X-ray Binary in M33
› The Missing Black Hole in the Large Magellanic Cloud: A Dynamical Prediction for Its Present-Day Location
› Forged in Quenching: Morphological Transformation across Star-forming and Quiescent Galaxies in EAGLE
› JWST Observations of Starbursts: A Young Bubble in NGC 253's Central Starburst
› Peering Beyond the Veil of Last Scattering: A View of the Universe with CMB Spectral Distortions
› Rescuing Kepler's False Positives: A Possible Habitable Zone Exoplanet in the Triple Star System KOI-1623
› Filament Formation via Collision-induced Magnetic Reconnection -- Kinematic Features
› Gravitational Wave Bias in IllustrisTNG300 from Machine-Learned Population-Synthesis Calibrated Merger Rates
› What the Solar System Can Teach Us About Rocky Exoplanets
› Cosmic Noon Galaxies in the Hubble Ultra Deep Field with MIRI Wide-Field Slitless Spectroscopy
› Formation of Merging Black Hole Binaries Inside Massive AGN Stars
› The Post-Outburst Spectrum of L1415-IRS
› Neutron Star Merger Universality Relations for a Quark--Hadron Crossover Equation of State
› Disentangling Stellar Mass and Environmental Effects on eROSITA AGN Activity using multi-wavelength data from GAMA, WISE, GALEX, and DESI Legacy Survey
› Determination of the Angular Distributions of Dynamical and Emission Parameters of GRB Relativistic Outflows
› Using Gravity as an Age Indicator for Young Stars
› NOCTURNE. II. Extreme radio variability in the heart of early-stage active galactic nuclei
› Properties of the circumstellar matter around the pair-instability supernova candidate SN 2018ibb revealed by its light curve
› Optomechanical design of an ADC and image rotator for the HJST Coud\'e Spectrograph at McDonald Observatory
› Commissioning the AIP's ultrafast laser Inscription facility: defining the parameter space for type-I waveguide fabrication
› SAMI and TNG-Cluster: tracing galaxy spin and environmental transformation across cluster phase-space and cosmic time
› CNN-Based Inference of Gaseous Halo Properties from Synthetic X-ray and 21-cm HI Observations
› RAMA: A new agile AO bench for the telescope FEELINGS
› Right Energy, Wrong Profile: Why the 43 GeV Cluster Line Is Unlikely to Be Dark Matter
› Characterizing bright $\delta$ Scuti pulsators using TESS light curves:II. Pulsation amplitude and energy distributions
› The Variation of Circumstellar Parameters through Early Stellar Evolution
› The Study of Detailed Morphology of Milky Way Dwarf Galaxies: Draco and Bo\"otes I
› Design of an atmospheric dispersion corrector and double scrambler for improved fiber coupling and illumination uniformity for the HET HRS
› Probing multi-state dark matter via optical absorption lines in DESI spectra
› Multi-wavelength Constraints on Dust Dynamics and Size Evolution in Protoplanetary Disk Rings. II. Observational Implications
› Supernova nucleosynthesis: a review
› Radiation Pressure Instability-Driven Variability of Line-Driven Disk Winds in AGNs: Connection to Periodic Luminosity Variations and UFO Appearance
› Probing the All-sky Distribution of Soft X-ray Emission Associated with the Milky Way
› Cosmological information from field-level analysis in redshift space
› Discovery of radio emission from the exoplanet $\beta$ Pictoris b
› Lower central dark matter densities in nearby galaxies than predicted by simulations
› Population synthesis of low-mass binaries with wind-accreting neutron stars
› The study of AF And. I. Hydrogen abundance constraints and dynamically-consistent wind model of the hot state
› H$_2$O emission as tracer of pebble drift: insights from coupling transport and thermochemical models
› Testing a Pre-Supernova Contribution to $^{44}$Ti in Cassiopeia A
› The asymmetric limbs of HD 209458 b observed with JWST NIRCam F322W2/F444W
› Triple coronal hard X-ray source observed by STIX during a failed filament eruption
› Impact of Equation of State on Black Hole Accretion Flows and Radiative Properties
› Supernova Kinetic Yield oN galactic Emission Tracers (SKYNET) I. Contribution of radiative supernova remnants to Galactic N + emission
› Gravitational lensing of gravitational waves by galaxy clusters
› Promise and pitfalls of plasma emission as an exo-space-weather tool
› An ALMA Band 7 survey of SDSS/Herschel quasars in Stripe 82: II. The nature of FIR-bright quasars
› The UV-to-FIR environments of nearby Type Ia supernovae with the DustPedia Galaxy Catalogue -- I. Local versus global host properties
› Hardware-efficient neural networks for FPGA-based radio triggering of extensive air showers
› Pushing HST to the limit: Detection completeness and morphology robustness of faint galaxies in the EGS field
› Lyman-$\alpha$ forest 1D flux power spectrum constraints on QSO-assisted reionization models
› Around the water snowline: I. Effects of dynamical and chemical interplay on mid-infrared water spectra of protoplanetary discs
› Optimal exposure time for satellite imaging? A trade-off between residual tip-tilt and registration accuracy
› The evolution of discs and the epoch of formation\newline of giant planets around solar type stars
› Saturns Are Not Large Neptunes: The effect of removing inflated giants from empirical mass-radius relations
› How Small is Large Enough? Determining Minimal Cluster Sizes for Molecule Adsorption on Interstellar Amorphous Ice
› Stellar age is not disk age
› Determining elemental composition in laboratory meteorite ablation spectra through radiative transfer modeling
› Investigating past high-energy fluxes with paleo-detectors
› No statistically significant evidence for a correlation between stellar and planetary composition
› Count-based spectral component imaging (CCI) of solar flares in X-rays
› The WEFT project: I. The emergence of turbulence in a cosmic filament
› Glycine in the interstellar medium revisited: Resolving conformational complexity kinetically
› PyExoCross 2.0: A Python Framework for LTE and non-LTE Spectra, Cross Sections, and Spectroscopic Post-processing of Atomic and Molecular Line Lists
› A fast radio burst from a non-targeted low-frequency survey
› Caught by its own light: Wimpzillas, the LHAASO knee and the diffuse $\gamma$-ray sky
› A self-consistent orbital architecture for GG Tau A. I. Simultaneous orbital fitting of the hierarchical triple
› Large ${\rm Pm}$ small-scale kinematic dynamo in protoneutron stars
› Characterization of IBEX LmAPD detectors at CEA for future low-noise NIR astronomy instruments
› DewTwin-Coin: an onboard autonomous framework for lunar water-ice prospecting using Chandrayaan-3 LIBS and ChaSTE data
› Assessing ionospheric effects on image quality in the LOFAR Decametre Sky Survey
› X-ray to Mid-IR Spectral Energy Distributions: A Catalog of X-ray Selected AGNs in the XMM-COSMOS Survey
› Running Hubble Constant with the Redshift as a Marker of Evolutionary Dark Energy
› The Equivalence Principle in the Dark Sector in light of DESI
› Spontaneous wandering of the magnetic axis in pulsars: 3D magneto-thermal simulations and the imprint on braking indices
› Stellar Ages of M Dwarf Hosts of Temperate Sub-Neptunes
› Constraints on the central engine of merger-driven long gamma-ray bursts
› Secular evolution of viscous and self-gravitating protoplanetary discs with magnetic winds
› $B$-sure. Part II. Scattering transforms as robustness test for tensor-to-scalar ratio detection from CMB observations
› Dark Radiation Sticks Together: Dark QCD and the Hubble Tension
› Multiple-Mediator-Affected Ultra-High-Energy Neutrino Attenuation: Hints for 5D ${U(1)}_{L_\mu - L_\tau}$ in IceCube
› Bridging the chirp-mass gap: searching for gravitational waves from inspiraling ultra-compact binaries using LIGO O4ab data
› Charging of rotating black holes: kinetic simulations of black hole magnetospheres
› Bridging Between Statistical Mechanics and Black Hole Evolution: Theoretical Formalism
› Limits on the Inferred Hubble Constant Bias from a Local McVittie Gravitational Field
› Impact of the Host Galaxy on the Search for Gravitational-Wave Microlensing by Compact Objects
› Adding slow magnetoacoustic mode to the HLL-type multi-state approximate Riemann solution
› Cosmological Constrained Axion-Portal Inelastic Dark Matter for the LZ Event
› Vanilla Scotogenic Model at the future Muon Collider
› Strong magnetic field inside degenerate relativistic plasma and the impacts on the neutrino transport in Core-Collapse Supernovae
› The Cocytos Stream: A Disrupted Globular Cluster from our Last Major Merger?
› Combined tracer analysis for DESI 2024 BAO
› Cosmic Shear constraints from HSC Year 3 with clustering calibration of the tomographic redshift distributions from DESI
› XID+PRIMA, II: Stepping Through Hyperspectral Imaging to Deblend PRIMAger Beyond the Extragalactic Confusion Limit
› Induced Scattering of Fast Radio Bursts in Magnetar Magnetospheres
› Mixing-induced thermal instabilities and coronal condensations
› The FLAMINGO Project: Exploring the X-ray--cosmic-shear cross-correlation as a probe of large-scale structure
› The Curious Case of Centaurus A: On the Subject of the Quenched satellites
› Ly{\alpha} forest bounds on sterile neutrino production via neutrino self-interactions
› On gravitational baryogenesis in inflationary $f(R)$ Cosmologies
› Pad\'e semi-cosmographic reconstruction of residual dark energy in decaying dark matter cosmology: DESI DR2 BAO constraints and mock 21 cm forecasts
› Metal Mayhem at z~7-10: Diversity and Evolution of Gas-Phase Metallicity Gradients
› FastQSL 2: A Comprehensive Toolkit for Magnetic Connectivity Analysis
› DeepDive: Simultaneous Formation of Massive Quiescent Galaxies in High-Redshift Galaxy Overdensities
› A Physics Informed Bayesian Neural Network for the Neutron Star Equation of State
› Discovery of a Compact Hub-Filament System in G286.21+0.17 with JWST and ALMA: Insights into Protocluster Formation and Competitive Accretion
› Scalable Dark Siren Cosmology with gwcosmo: GPU Acceleration, Validation and Systematics
› Temperature-resolved sensitivities of $^{56}{\rm Ni}$ production to helium-burning reactions in pair-instability supernovae
› Temporal Invariance Is an Illusion: Time-Dependent Influences of the Galactic Magnetic Field on UHECR Observations
› A Unified Halo Mass Function Across Dark Matter Models from High-Resolution Multi-Scale Simulations
› Time-dependent cosmic-ray escape from wind bubbles: hard spectra formation
› Effects of Super-rotating Jets on Phase-Resolved Transmission Spectra at High Spectral Resolution
› Traversing the Galactic Centre in space and time
› Galaxy Power Spectrum at Two-Loop Order: Implications for Weak Lensing Surveys and New Physics
› Optically Selected Superthin Galaxies Remain Thin in the Near-infrared
› Robust Heteroskedastic Matrix Factorization: A Generalization of PCA that Flags Outliers and Handles Missing Data
› Using Ringed Disks to Determine Fundamental Parameters of Planet Formation
› Implementation of frequency-correlated noise in CMB component separation: Method, Validation, and Early Applications
› Conformally Interacting Dark Energy with Early and Late-Time Measurements
› Why Azimuthal Averaging Works in Halo Lensing: Symmetry and Power Counting for Nonlinear Shear and Magnification
› Active galactic nucleus activity in brightest cluster galaxies at intermediate redshifts in Sunyaev-Zel'dovich--selected clusters
› Host Galaxy UV Emission and Dust Reddening in Little Red Dots
› Exploring the dynamics of the Coma galaxy cluster by mapping its X-ray emission line profiles with XRISM
› Evolution of the High-Energy Excess in Swift J1727.8-1613 during Its 2023 Flare State
› Forecasting Coupled Dark Energy Parameters with the One-Loop Galaxy Power Spectrum
› Spectator Composes a Gravitational Canon: Spectator-field-triggered Phase Transition During Inflation and its Anisotropic Gravitational Wave Signals
› Probing the Kinematic Dipole with LISA: an analytical treatment
› Structure of the $^8$B and $^8$Li nuclei and the astrophysical $S_{17}(0)$-factor of the $^7$Be($p,\gamma$)$^8$B direct capture process within a three-body model
› Neutrino helicity oscillations in astrophysical environments: A many-body approach
› Parametrized beyond-Teukolsky framework in the time domain
› DANSur_HM: Modularly incorporating higher modes in a deep learning based gravitational-wave surrogate
› A distance-independent constraint on the axion-electron coupling from RGB stars

  ↓↑    

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