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: Sunset from the kitchen window
Sunset from the kitchen window
S Webcam

S Webcam

Webcam

N Webcam

Allsky

S Sky

Temperature
22.9 °C

Humidity
 49%

Wind
0.0 km/h

Pressure
1017.7 hPa

Moon

Moon

 News from astronomynow.com
› Binoculars to boost your night-sky viewing
› Lyra’s stunning smoke ring – M57
› Is the Hubble Tension Resolved?
› Universe’s end – sooner rather than later
› Caught in the current of the wonderful Whirlpool
› A faint star will reveal itself as it throws a hissy-fit
› Saturn’s Rings to “Disappear”
› The Lithium Problem
› Discover the many fascinating moons of our Solar System
› A bigger and better helicopter to Mars
RSS  Latest preprints on astro-ph:
› Time Invariant Sensor Tasking for Catalog Maintenance of LEO Space objects using Stochastic Geometry
› Symmetry-protected conservation of superhorizon inflationary perturbations to all loops
› Challenge-Based Funding to Spark Origins Breakthroughs
› Satellite Constellations Exceed the Limits of Acceptable Brightness Established by the IAU
› Constraining the magnetic field in the galaxy cluster Abell 2142 using MeerKAT L-band polarisation data
› Quantum stress-energy at timelike boundaries: testing a new beyond-$\Lambda$CDM parameter with cosmological data
› Orbit and atmosphere of HIP 99770 b through the eyes of VLTI/GRAVITY
› Constraining Dynamical Dark Energy from Galaxy Clustering with Simulation-Based Priors
› Energy-Dependent Transport of Cosmic Rays in the Multiphase, Dynamic Interstellar Medium
› SMA and NOEMA reveal asymmetric sub-structure in the protoplanetary disk of IRAS23077+6707
› PyMGal: A Python Package for Generating Optical Mock Observations from Hydrodynamical Simulations
› Mid-Infrared Dust Evolution and Late-time Circumstellar Medium Interaction in SN 2017eaw
› XRISM Observation of the Ophiuchus Galaxy Cluster: Quiescent Velocity Structure in the Dynamically Disturbed Core
› Lya2pcf: an efficient pipeline to estimate two- and three-point correlation functions of the Lyman-$\alpha$ forest
› Fewer Companions in the Crowd: The Low Close Binary Fraction in Globular Clusters from Gaia RVS
› On the cosmic-ray distribution in the Galactic Center region: New insights from H.E.S.S
› CHEX-MATE: New detections and properties of the radio diffuse emission in massive clusters with MeerKAT
› Causal Discovery of Latent Variables in Galactic Archaeology
› DeepCHART: Mapping the 3D dark matter density field from Ly$\alpha$ forest surveys using deep learning
› $\textit{Eppur Si Muove}$: Self-Sustained Streaming Motions in Multi-Phase MHD
› Metal-poor single Wolf-Rayet stars: the interplay of optically thick winds and rotation
› The formation and evolution of Supermassive disks in IllustrisTNG
› Modeling Cosmic Ray Electron Spectra and Synchrotron Emission in the Multiphase ISM
› Study of the peculiar variable star Khavchenko 1
› Searching for new Hypervelocity Stars with Gaia DR3 and VLT/FORS2 Spectroscopy
› Forecast for growth-rate measurement using peculiar velocities from LSST supernovae
› Testing Origin-of-Life Theories with the Habitable Worlds Observatory (HWO)
› Prebiosignatures with the Habitable Worlds Observatory (HWO)
› An outer-disk SX Phe variable star in Rubin Data Preview 1
› Probing the variations of interstellar dust abundance and properties within and between galaxies with HWO UV spectroscopy in the Local Volume
› Characterization of the Cherenkov Photon Background for Low-Noise Silicon Detectors in Space
› Magnetic field monitoring of four massive A-F supergiants
› Modeling the Cosmological Lyman-$\alpha$ Forest at the Field Level
› Fuzzy dark matter halos with repulsive self-interactions: coherent soliton and halo vortex network with moderate self-coupling
› X-ray polarization of Z-type neutron star low-mass X-ray binaries -- I. Model-independent, time-resolved X-ray polarimetry
› Exploring the probing power of gamma-Dor's inertial dip for core magnetism: case of a toroidal field
› Formation of Complex Organic Molecules in Prestellar Cores: The Role of Non-Diffusive Grain Chemistry
› Radio Continuum Studies of Ultra-Compact and Short Orbital Period X-Ray Binaries
› Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
› LIGO/Virgo/KAGRA neutron star merger candidate S250206dm: Zwicky Transient Facility observations
› The Density Profile of Dynamical Halos
› FAST search for circumstellar atomic hydrogen. III. Planetary nebulae at Galactic latitudes |b|>10degree
› A 3mm molecular line survey toward IRC+10216
› Hints of noncold dark matter? Observational constraints on barotropic dark matter with a constant equation of state parameter
› Diversity of rocky planet atmospheres in the C-H-O-N-S-Cl system with interior dissolution, non-ideality, and condensation: Application to TRAPPIST-1e and sub-Neptunes
› The Instrumental Background of EP/FXT
› Simulation-Efficient Cosmological Inference with Multi-Fidelity SBI
› Evidence for enhanced mass transfer in the disc preceding the transition to the soft state in MAXI J1820+070
› A Comprehensive study of time delay between optical/near-infrared and X-ray emissions in black hole X-ray binaries
› Neural translation for Stokes inversion and synthesis
› Head-on collisions of fuzzy/cold dark matter subhalos
› The radiative subpulse modulation and spectral features of PSR B1929$+$10 with the whole pulse phase emission
› Energy-dependent temporal study of GX 13+1 with AstroSat observation
› Misaligned external gas acquisition boosts central black hole activities
› Connecting mean-field theory with dynamo simulations
› The effect of local magnetic fields in quiet regions of stellar atmospheres simulated with MANCHA
› Testing Nambu-Goto approximation of cosmic string by lattice field simulations
› Ultralight fuzzy dark matter review
› Asteroids fail to retain cometary impact signatures
› Attributing the point symmetric structure of core-collapse supernova remnant N132D to the jittering jets explosion mechanism
› Sub-Neptunes Are Drier Than They Seem: Rethinking the Origins of Water-Rich Worlds
› Light Curve Analysis Of W-uma Type Binary Systems Rz Umi, Oq Uma, Lp Uma
› Microlensing of dark matter models in the Milky Way
› Hybrid Quark Stars with Quark-Quark Phase Transitions
› Is $\omega_0 \omega_a$CDM a good model for the clumpy Universe?
› Close-in planet induces flares on its host star
› Timing and spectral studies of SRGA J144459.2$-$604207 with NICER, Einstein Probe, IXPE, NuSTAR, Insight-HXMT and INTEGRAL during its 2024 outburst
› Searching for planet-induced radio signal from the young close-in planet host star HIP 67522
› The Gaia-ESO Survey: Projected Rotational Velocities of B stars in the Carina Nebula
› Photospheric Helium Abundance in Cool Giants -- A Comprehensive Study
› The Evolution of Substructure during Star Cluster Assembly
› Probing Generalized Emergent Dark Energy with DESI DR2
› CO2 infrared spectra on silicate dust grain analogs: Implications for JWST observations
› Chemical constraints on the dynamical evolution of the cold core L694
› Template-Fitting Meets Deep Learning: Redshift Estimation Using Physics-Guided Neural Networks
› The Evolution of Pop III.1 Protostars Powered by Dark Matter Annihilation. I. Fiducial model and first results
› A period-increasing oscillation signal in a long gamma-ray burst
› New Agegraphic Dark Energy Driven Reconstruction of \boldmath{$f(Q)$} Gravity and its Cosmological Implications
› The impact of differential rotation on the stochastic excitation of acoustic modes in solar-like pulsators
› Extreme Forward Scattering Observed in Disk-Averaged Near-Infrared Phase Curves of Titan
› A first look at rocky exoplanets with JWST
› A binary origin of ultra-long period radio pulsars
› Differentiation, the exception not the rule -- Evidence for full miscibility in sub-Neptune interiors
› Inverse Velocity Dispersion of Solar Energetic Protons Observed by Solar Orbiter and Its Shock Acceleration Explanation
› Atmospheric model-trained machine learning selection and classification of ultracool TY dwarfs
› Discovery and study of the eclipsing variable star Grigoriev 1
› The BoRG-$JWST$ Survey: Analogs at $z\sim8$ to the UV-luminous Galaxy Population at $z\gtrsim10$
› Evidence of the Earth's inner radiation belts during the low Solar and geomagnetic activity obtained with the STEP-F instrument
› Physics. Tasks With Solutions
› Test mass charge management in the detection of gravitational waves in space based on UV micro-LED
› Black-hole - neutron-star mergers: new numerical-relativity simulations and multipolar effective-one-body model with spin precession and eccentricity
› Modeling Gravitational Wave Modes from Binaries with Arbitrary Eccentricity
› Preliminary analysis of the annual component of the polar motion over 180-year data interval
› Power-Law Bounces in $f(R)$ Gravity: Analysis of the Ekpyrosis and Accelerating Regimes
› Black Holes Immersed in Galactic Dark Matter Halo
› Stability of Thin Shell and Wormhole Configurations: Schwarzschild, Schwarzschild -- (Anti-) de Sitter, and FLRW Spacetimes
› Earth-Scattering Induced Modulation in Low-Threshold Dark Matter Experiments
› Uniform rate inflation in $f(T, \mathcal{T})$-gravity
› A waveform and time digitization mainboard prototype for TRIDENT neutrino experiment
› Detection probability of light compact binary mergers in future observing runs of the current ground-based gravitational wave detector network
› Muffled Murmurs: Environmental effects in the LISA stochastic signal from stellar-mass black hole binaries
› A Non-Inflationary Axion and ALP Misalignment Mechanism
› Perturbative unitarity bounds on field-space curvature in de Sitter spacetime: purity vs scattering amplitude
› Gravitational Wave Signatures of Periodic Motion near Higher-Derivative Einstein-\AE ther Black Holes
› Khronon-Tensor theory reproducing MOND and the cosmological model
› New Constraints on Neutrino-Dark Matter Interactions: A Comprehensive Analysis
› Improved First Estimates to the Solution of Kepler's Equation
› Multi-messenger signatures of delayed choked jets in tidal disruption events
› Probing Chemical Enrichment in Extremely Metal-Poor Galaxies
› Distinguish dark matter theories with the cosmic web and next-generation surveys I: an alternative theory of gravity
› Limits on Early Matter Domination from the Isotropic Gamma-Ray Background
› The Mass of the Vela Pulsar Progenitor and the Age of the Vela-Puppis Complex
› Ultrahigh-energy neutrino searches using next-generation gravitational wave detectors at radio neutrino detectors: GRAND, IceCube-Gen2 Radio, and RNO-G
› Fast radio bursts as a probe of gravity on cosmological scales
› Where is the Super-Virial Gas? The Supply from hot inflows
› Fe I 6173 {\AA} Emission During White-Light Solar Flares
› Machine Learning Approach for Estimating Magnetic Field Strength in Galaxy Clusters from Synchrotron Emission
› On the universality of the halo mass function beyond ${\Lambda}$CDM cosmology
› SECRET: Stochasticity Emulator for Cosmic Ray Electrons
› Central Cluster Galaxies: A Hotspot for Detectable Gravitational Waves from Black Hole Mergers
› Fast Generation of Weak Lensing Maps in Modified Gravity with COLA
› Gas outflows in two recently quenched galaxies at z = 4 and 7
› Sleeping Giants Arise: Monitoring the Return of Three Changing-Look Quasars to Their High States
› Extended source fringe flats for the JWST MIRI Medium Resolution Spectrometer
› Spatially resolved [CII]-gas conversion factor in early galaxies
› Stellar ejection velocities from the binary supernova scenario: A comparison across population synthesis codes
› An accreting dwarf star orbiting the S-type giant star pi1 Gru
› Analytic Model for Covariance Matrices of the 2-, 3-, and 4-Point Correlation Functions in the Gaussian Random Field Approximation
› Rapid Spectral Evolution of SGR 1935+2154 During its 2022 Outburst
› Physical Conditions of the Ionized Superwind in NGC 253 with VLT/MUSE
› The curvaton ACTs again
› High-Velocity Molecular Clouds in M83
› Evolution of star clusters with initial bulk rotation via N-body simulations
› Quantum cosmological perturbations in bouncing models with mimetic dark matter
› Planetesimal Scattering Efficiency of Cold Giant Planet Architectures
› Constraints on Dark Energy Models Using Late Universe Probes
› Self-Interacting Dark-Matter Spikes and the Final-Parsec Problem: Bayesian constraints from the NANOGrav 15-Year Gravitational-Wave Background
› Detectability of dark matter density distribution via gravitational waves from binary black holes in the Galactic center
› Low-metallicity massive single stars with rotation. III. Source of ionization and C-IV emission in I Zw 18
› Probing the detectability of electromagnetic signatures from Galactic isolated black holes
› Dynamical analysis of logarithmic energy-momentum squared gravity
› On probing turbulence in core-collapse supernovae in upcoming neutrino detectors
› Cosmological scaling of precursor domain walls
› Cosmic-Ray Cooling in Active Galactic Nuclei as a New Probe of Inelastic Dark Matter
› Role of internal space correlations in the dynamics of a higher-dimensional Bianchi type-I universe: shear scalar and Hubble parameter perspectives
› Filtered cogenesis of PBH dark matter and baryons
› Classical and quantum cosmology of $f(R)$ gravity's rainbow in Schutz's formalism
› Evolution of a kink-antikink ensemble in a quantum vacuum
› Fast detection and reconstruction of merging Massive Black Hole Binary signals
› On the Probability of the Initial Conditions for Inflation and Slow Contraction
› Micro Black Hole Dark Matter

  ↓↑    

Return to main page of Mt. Suhora Observatory
Copyright © 2002-2025 Astronomy Department, Cracow Pedagogical University. All Rights Reserved.