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
Cloud conditions

Cloud

Rain conditions

Rainfall

Allsky

S Sky

Temperature
12.2 °C

Humidity
 77%

Wind
0.0 km/h

Pressure
1016.2 hPa

Moon

Moon

 News from astronomynow.com
› 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
› Witness to history: Artemis II, lunar exploration and hope
› Artificial Intelligence uncovers more than 100 new worlds in NASA data
RSS  Latest preprints on astro-ph:
› Radio Galaxies detection and characterization using deep learning techniques
› NestyNet. IV. Laws Chosen by Nothing in Advance
› On the importance of the IGM/CGM enrichment in determining chemical abundances during the first 600 Myr
› EROSE: An algorithm searching for resolved Local Group satellites. The impact of combining different photometric bands on the detectability of Milky Way satellites in the LSST
› A Highly Reflective Atmosphere on the Lava World TOI-561b Revealed by JWST/NIRSpec Phase Curve
› On the performance of pre-trained vision transformers for supernova spectral classification using different spectral representations
› Beyond orientation: Evidence for distinct physical regimes among Little Red Dots and Little Blue Dots
› The Milky Way Joins the Extragalactic World: I. PHANGS
› Assessing the Impact of High-Resolution Imaging on Statistical Validation of TESS Planet Candidates
› Relativistic blob signatures in the M87 jet at sub-parsec scales
› Supernovae Ia ejecta velocities and host galaxy environments: the role of survey-selection effects
› When the stars don't align: Investigating inconsistencies in binary black hole formation across population synthesis codes
› Image persistence flagging for SPHEREx
› Galactic Electron-Positron Annihilation Emission from X-Ray Binaries with Transient and Persistent Jets
› Simulation Tests of PSF Modeling for Cosmic Shear with the Vera C. Rubin Observatory
› A surviving pink spinel records an early aluminous melt on the ureilite parent body
› Hydrodynamical simulations of the merging cluster El Gordo in a two-state self-interacting dark matter scenario
› Indirect evidence of the $2175\,\mathring{\mathrm{A}}$ extinction bump within the dusty torus of SDSS J141945.50+524648.0
› CPD-82 291: Multi-sector TESS Photometry and SED Analysis of an Active Eclipsing Binary
› Pair Discharges and Radio Emission from Pulsar Magnetospheres
› WISE J005128.08+645651.7: An enigmatic R Coronae Borealis star
› Beyond dynamical dark energy: the role of dark sector interactions after DESI DR2
› Discovery of an Extremely Luminous Sporadic Radio Pulsar
› Searching for signatures of self-interacting dark matter in halos from full-physics simulations: From 3D structure to projected observables
› MIAO-ALMA: Shocks and Protostellar Outflows in 70 $\mu$m-dark clumps with $L/M$ $
› Finite-Solid-Angle Boltzmann Radiation Transport on Dynamical Spacetimes in AthenaK
› Pair Discharges and Radio Emission from Millisecond-Pulsar and White-Dwarf Magnetospheres
› Correlation of gamma-ray and optical variability of BL~Lacertae during the period of high blazar activity
› Particle acceleration and non-thermal broadband spectrum of extended shocked outflows in black hole binary V4641 Sgr - a galactic pevatron
› The imprint of individual neutron star spins on ejecta, $r$-process nucleosynthesis, and kilonovae in binary neutron star mergers
› Discovering Dual-Origin Slow Wind from Solar Orbiter with Self-Supervised Contrastive Learning
› AstroBind: Machine learning prediction of binding energy distributions on interstellar water ice from geometric surface descriptors
› [CII] as a global cold gas tracer in novel hydrodynamical simulations
› Particle Dark Matter in the 1980s and 1990s
› Anisotropies in the PTA gravitational wave background: what can they teach us about supermassive black hole binaries?
› Modeling the technical specifications for future multi-object spectroscopy instrumentation
› The Cosmic Ultraviolet Background at the Galactic Poles
› Primordial Asymmetries, Primordial Equation of State & Primordial Black Holes
› Variational Bayesian Inference for the Spectral Structure of LISA Noise
› Constraining Gravitational Waves from Superconducting Cosmic Strings with the Dark Ages $21$-cm Signal
› Assessment of the 5 August 2026 Falcon 9 Upper-Stage Lunar Impact: Energetics, Crater Scaling, and Comparison with LRO Observations
› Automated Shape-Model-Based Astrometry of Phobos from Mars Express SRC Images
› Galactic Microquasar and Supernova Remnants Imprinting on Diffuse Neutrino and Gamma-Ray Sky
› The Mass-Size Plane Does Not Resolve the Identifiability Limit of the Radial Acceleration Relation
› Instrumental artifacts in photonic lantern spectroastrometry and their mitigation with PLred
› A superflare of BP Tau simultaneously caught by EP X-ray and TESS optical observations
› On the formation of subdwarf B stars via engulfment of substellar companions
› Spin-Orbit Alignment of Two Neptune-size Planets Younger than 500 Myr: TOI-560 b and TOI-5082 b
› Exoplanet System Architecture: Sculpting the Inner Regions
› Where Do Periodic Density Structures Acquire Coherence? A Low-Coronal Resonator Candidate and a 12-Event STEREO/SECCHI Transfer Test
› On the formation of retrograde S-type planets in binaries with a polar circumbinary disk
› Observational Evidence for the Kinematic Memory of Cosmic Filaments from Satellite Orbital Orientations
› Probing AU-Scale Magnetic-Field Reversals in the Interstellar Medium with Pulsar Scintillation
› Tidal disruption of stellar binaries as a pathway to exotic transients
› Timing, Polarization, and Single-Pulse Properties of Long-Period FAST Pulsars
› A Two-month, Galaxy-targeted NIR Follow-up of the Sub-solar-mass Gravitational Wave Candidate S251112cm: Probing Electromagnetic Counterpart Scenarios
› Thermochemical constraints on a primordial-origin of gas-rich debris disks
› ASKAP discovery of a pair of large radio bubbles: on the origin of odd radio circles
› Korean Space Collision Environment Assessment Framework Based on 3D-Cell Model
› Six new doubly eclipsing quadruples in a 2+2 architecture
› Extensive Air Showers Parameters Estimation Using Machine Learning Techniques with Simulations of the FAST Telescope
› The star formation history of NGC 2276: Comparison between SED modeling and hydrodynamical simulations
› When a neural surrogate cannot accelerate a solver: runtime share, closed-loop drift, and the economics of uncertainty gating in a stiff coupled simulation
› Effects of near-surface sedimentary structure on Newtonian noise for the Einstein Telescope: a 2-D numerical study
› Reconstructing the Auger UHECR Dipole: A Hybrid Analysis of 4LAC AGNs and Nearby Starburst Galaxies
› Neutron star masses from electron-capture supernovae under equation-of-state uncertainties
› Development of an adaptive optics testbed at MPIA for the ELT/Planetary Camera and Spectrograph (PCS)
› Solar chemical composition
› Dynamics of Wave Structures in Multifield Fuzzy Dark Matter Halos
› An improved view of cosmic-ray transport and the galactic outflow in NGC 253
› Potential sublimating exocomets around the young star PDS 70
› AI-Assisted Extraction of Follow-up Observations from GCN Circulars in Astro-COLIBRI
› Intra-system Uniformity through Planetary Embryo Accumulation
› Binary Neutron Star Merger Simulations with Microphysical Equation of State using Spritz
› Preparing for the Early eVolution Explorer: Photometric Diagnostics of Magnetospheric Accretion Geometry in Young Stellar Objects
› Breakout/Interchange Reconnection as a driver of Jets, Fast CME, and Solar Energetic Particles
› Black holes from a Higgs-like field in the radiation era
› FASHI DR2: A Catalog of 132 Low-Redshift HI 21 cm Absorption Systems
› Exploring Long-period Architectures: Four New Planet Candidates from Kepler with Periods >342 days
› Inverting and Up-channelizing Critically-Sampled Polyphase Filter Banks
› Inflationary Kicks and Coulomb Filtering of Spectator Dark Matter
› BLG723.31.34651 as an eclipsing Roche lobe-filling sdOB+WD binary
› Fragmentation and tidal locking in young quadruple systems
› The Road to Normalcy: Environment-Driven Evolutionary Pathways for Primordial Black Holes
› Disentangling propagation effects from Fast Radio Burst spectra: An analysis on simulated data
› The ALMA EGO-10 Survey of Massive Protoclusters: Correlation of 1.3 mm Continuum Source Clustering with Evolutionary State
› Strong Lensing Cosmology with Population-level Calibrated Neural Ratio Estimation
› Dust trapping, collisional velocity and velocity dispersion in gravito-turbulent discs
› Preparing for the Early eVolution Explorer: The Impact of Flare Temperature on Ozone Column Depth in Earth-Like Atmospheres
› The descendants of $z \gtrsim 10$ JWST galaxies in the COLIBRE simulations
› Development of Neutron Transmutation Doped Germanium (NTD-Ge) for Cryogenic Applications
› Cryogenic Mechanical Loss of GaAs/AlGaAs Crystalline Coatings
› Testing f(R) gravity using gravitational-wave signals from binary mergers
› Kerr-Newman and genuine Kerr black holes in the Bertotti-Robinson magnetic field
› The Schwarzschild Black Hole in an External Gravitational Tidal Field: the Quasinormal Spectrum
› Plasmon-polaritons in a rarefied nonrelativistic neutron gas
› Extreme mass-ratio inspirals around rotating accelerating black holes
› Correlated and coincident noise in Einstein Telescope's triangular configuration
› What AstroPT knows about galaxies, and what that can teach us about LLMs
› Neural Operator based Multi-Field Reconstruction of Inner Solar Boundary State
› Impact of Bubble Nucleation History and Friction on Primordial Black Hole Formation
› Signed Sound-Speed Deformations of BSk24-Anchored Barotropes: Neutron-Star Response
› Complex frequency evolution of direct waves from binary black hole mergers
› Analytical Cosmological Collider at Strong Mixing in Laplace Space
› Action-selected currents and a singular conservation closure in two-fluid energy--momentum-squared cosmology
› Traceable Spectral Inference via Influence Functions: Efficient Data Attribution and Error Proxies for the Ariel Mission
› Updated Upper Limits on the Isotropic Gravitational-Wave Background from LIGO, Virgo, and KAGRA Data through April 2025
› Gravitational waves from the early universe
› Episodic super-Eddington accretion as a clue to Overmassive Black Holes in the early Universe
› Role of Matter Inhomogeneity on Fast Flavor Conversion of Supernova Neutrinos
› Constraining the Baryon Fraction in Extragalactic Diffuse Ionized Gas with 124 Localized Fast Radio Bursts
› Differentiable Halo Mass Prediction and the Cosmology-Dependence of Halo Mass Functions
› Higher-order methods of radiative transfer in simulations of the epoch of reionisation: Pn versus M1
› Can a gamma-ray dim radio blazar produce a 200-PeV neutrino? The case of PMN J0606$-$0724 and KM3-230213A
› Binary-lens Microlensing Degeneracy: Impact on Planetary Sensitivity and Mass-ratio Function
› Giant Planets and Eccentric Orbits Are Common Around Galactic Thick Disc Stars
› Precision Spectroscopy for 1.7 Million Galaxies from SDSS-IV: Improved Spectral Measurements and Catalogs for eBOSS
› Axion misalignment as a synchronization phenomenon
› Minutes-long soft X-ray prompt emission from a compact object merger
› Lensing without mixing: Probing Baryonic Acoustic Oscillations and other scale-dependent features in cosmic shear surveys
› Hidden mass in early galaxies revealed by bottom-heavy initial mass functions
› A New Strategy for Using Spectroscopic Phase Curves to Characterize Non-Transiting Planets
› Dynamical Mass Constraints on Transition Disk Perturbers with the G23H Catalog
› Two-body relaxation in the EMRI-TDE disk model for Quasi Periodic Eruptions
› XMM-Newton Observation and Optical Monitoring of the Candidate Redback Millisecond Pulsar 1FGL J0523.5$-$2529
› Spectral Map Making with SPHEREx
› Hydrogen-helium immiscibility boundary in gas-giant planetary interiors from machine-learning molecular dynamics
› An astrometric search for planets in debris disk systems
› A detailed MOND modelling of the Bullet Cluster
› Classifying Supermassive Black Hole Growth Regimes to Observables Across Cosmological Simulations with Forecasts for LSST
› First measurement of wind line formation regions in an early O-type star
› Bayesian component separation and power spectrum estimation for 21 cm intensity mapping data cubes
› A PINK update: Improvements to the CELEBI fast radio burst data reduction and analysis pipeline
› Hidden worlds: A non-transiting candidate planet in the Neptunian desert around the solar-type pulsator KIC 9139163
› Exploring the High-Redshift 21-cm Signal via Self-Consistent Simulations using Artificial Neural Network Emulation
› Radio Continuum Emission from Evolving Star-Forming Galaxies -- I. Correlations Involving the Total Synchrotron Luminosity
› Individual Star Sampling in Star Formation Simulations: A Semi-Deterministic Model
› UV-to-optical insights into the BH$^*$ model in little red dots
› Magnetic fields at the dawn of structure formation I. The CARLA J1510+5958 proto-cluster
› Licence to Bin: Accurate and Scalable Inference for Binary Neutron Stars in Next-Generation Gravitational-Wave Detectors
› Joint Modeling of GD-1 and C-19 as Old Streams
› Angular Momentum Transport in Protoplanetary Disks
› Validation of the Hybrid Bias Expansion model for the galaxy bispectrum
› A nonrelativistic radiative transfer module for Idefix
› The performance of the TA$\times$4 surface detector array: 4.3 years of the first-half expansion
› A Scalable Path to Astrometric Exomoon Discoveries with the Nautilus Space Observatory
› A Calibration Audit of a Gaia XP White-Dwarf Main-Sequence Binary Catalog: How Much the BP-Band Residual Contaminates at Its Bound and Above
› Observations of X-ray quasi-periodic eruptions
› Mid-Infrared Colors Vary with Galactic Environment: Contrasting Star-Forming Disks, Young Centers, and Quiescent Star-Formation Deserts
› Shock cooling emission from late-time mass loss in low-mass He star binaries
› Gravitational Lensing Predictions from Wave Simulations of Fuzzy Dark Matter
› Web-Halo Model Peak-Background Split (WHM-PBS): halo bias as a distribution, not a number
› A closer look at the WISPIT 2 host star. Evidence for a spectroscopic binary
› Upgrading LBTI/NOMIC with a quadruple annular groove phase mask and GeoSnap detector for imaging nearby, habitable-zone exoplanets
› Day-timescale Quasi-periodic Oscillations of the Gev BL Lac RX J0805.4+7534 with TESS
› Pixel-Level Calibration for Space-Based High Precision Astrometry Using Young's Fringes
› Atmospheric Light Pollution by Proposed Reflect Orbital Space Mirrors
› Parametric Study of the Torus Instability Threshold
› $R_{\rm e}$, or not $R_{\rm e}$: Developing $R_5\equiv R_{-2}$ as a scale radius for galaxy sizes, masses, and mass-to-light ratios
› PowerFull: fast and accurate computation of the relativistic angular galaxy power spectrum including local primordial non-Gaussianity
› The Atacama Cosmology Telescope: Passband Measurements with an Analysis of Systematic Errors
› The GASKAP-HI Survey towards the Magellanic Clouds: Cold Atomic Gas Survival and Evolution in the Large Magellanic Cloud
› Transit Searches for Habitable-Zone Exoplanets with Artificial Intelligence
› Gravitational Radiation from hyperbolic encounters in the presence of dark matter
› Exploring Ultralight Dark Matter Self-Coupling via the Gravitational Wave Background
› Gravitational memory meets astrophysical environments: exploring a new frontier through osculations
› Large Neutrino "Collider"
› Ultra-Strongly Self-Interacting Dark Matter: From Phenomenology to Astrophysical Observables
› Abiogenesis on Different Star Types; a Dissipative Photochemical Perspective
› From the Wavefunction of the Universe to In-In-Correlators: A Perturbative Map to All Orders
› Observing Micro Black Hole Dark Matter
› Dispersion Relations of Collective Flavor Excitations in Dense Neutrino Media
› Stable black hole solutions with cosmological hair
› Misalignment from kicks: the impact of particle interactions on ultra-light dark matter
› Echoes of Global Cosmic Strings
› A High-Precision Statistical Analysis of the SN1987A Neutrino Temporal Distribution
› Limits of the Rastall--Einstein Equivalence: Matter-Action Compatibility, FLRW Dynamics, and Exceptional Sectors
› Hidden quantum-informatic symmetries of quasi-de Sitter backgrounds
› Modality Analysis via Spacing with the Dimodal Software Libraries
› Resonance crossings as entire functions of the Koopman operator

  ↓↑    

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