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
Cloud conditions

Cloud

Rain conditions

Rainfall

Allsky

S Sky

Temperature
8.3 °C

Humidity
 78%

Wind
9.7 km/h

Pressure
1018.5 hPa

Moon

Moon

 News from astronomynow.com

› 13 spooky images for Halloween
› How to see Comet Lemmon
› Hubble revisits a cosmic yardstick
› Europe’s planet hunting spacecraft complete and ready for final testing
› See Titan’s shadow transit Saturn – next chance 2038!
› Nova outburst in Centaurus
› Astronomy Now relaunches digital platform
› Potentially habitable planet TRAPPIST-1e displays tentative evidence for an atmosphere
› Ten-Year Lease Extension Confirmed at Herstmonceux Observatory
› Venus and Jupiter’s bright morning conjunction
RSS  Latest preprints on astro-ph:

› Pulsar Detection with Deep Learning
› Tidally driven inertial waves enhance eccentricity damping and spin evolution in planets and stars
› The kSZ optical depth degeneracy and future constraints on local primordial non-Gaussianity
› The Ray Tracing Sampler: Bayesian Sampling of Neural Networks for Everyone
› Updated dark pixel fraction constraints on reionization's end from the Lyman-series forests of XQR-30
› Unveiling Extended Components of 'Little Red Dots' in Rest-Frame Optical
› Model-Independent Inference of Galaxy Star Formation Histories in the Local Volume
› Exploring the quasar disc-wind-jet connection with LoTSS and SDSS
› Demystifying flux eruptions: Magnetic flux transport in magnetically arrested disks
› Figuring Out Gas & Galaxies In Enzo (FOGGIE) XI: Circumgalactic O VI Emission Traces Clumpy Inflowing Recycled Gas
› Cosmological Simulations of Weakly Collisional Plasmas with Braginskii Viscosity in Galaxy Clusters
› Spiral Structure Diversity in Milky Way Analogs from TNG50: The Role of Gas and Disk Dynamics
› WOCS XCIII: NGC 7789: the Evolution of Li, Stellar Rotation, and Extended Main Sequence Turnoffs
› New Pipeline for Efficient Analysis of Large Spectroscopic Samples of OB Stars
› Resolved HII regions in NGC 253: Ionized gas structure and suggestions of a universal density-surface brightness relation
› 25 Years of Groundbreaking Discoveries with Chandra
› Chemical separation of stellar populations: analytic solutions for chemical evolution models with metallicity-dependent yields
› A three-dimensional reconstruction of the interstellar magnetic field toward a star-forming region
› Mitigating gain calibration errors from EoR observations with SKA1-Low AA*
› Atmospheric collapse and re-inflation through impacts for terrestrial planets around M dwarfs
› On the Universality of the Relation Between Magnetic Fields and Star Formation in Galaxies
› TRIShUL: Technique for Reconstructing magnetic Interstellar Structure Using starLight polarization
› NEOForCE: Near-Earth Objects' Forecast of Collisional Events
› Potential Thermal Profiles of The Third Interstellar Object 3I/ATLAS
› Lyman-$\alpha$ radiation pressure regulates star formation efficiency
› A Natural Language Interface for Efficient Data Retrieval in SDSS
› HS-ANET: Star Spectral Type Enhanced Astrometric Calibration for Hyper Spectral Space Imaging
› How does ice shell geometry shape ocean dynamics on icy moons?
› Gravitational-Wave Constraints on Neutron-Star Pressure Anisotropy via Universal Relations
› Ram pressure shaping HVC droplets -- FAST HI observations of HVC AC-III and theoretical interpretation
› Hot Jupiter Origin and Tidal Evolution Constrained by a Broken Age-Frequency Relation
› Accretion rates of stellar-mass compact objects embedded in AGN discs
› Evidence of cosmic-ray acceleration up to sub-PeV energies in the supernova remnant IC 443
› Direct Numerical Simulations of Oxygen-Flame-Driven Deflagration-to-Detonation Transition in Type Ia Supernovae
› Multi-Faceted Emission Properties of PSR J2129+4119 Observed with FAST
› Rotation Measure Analysis of Shocks and Sloshing Fronts in a Galaxy Cluster Merger Simulation
› A new particle-based code for Lagrangian stochastic models applied to stellar turbulent convection
› Stellar Parameters and Evolutionary Pathways of the Subgiant system HIP 72217
› A Triple-GEM Time Projection Chamber for Wide Field-of-View Hard X-ray Polarimetry: First Results
› Theoretical models for the Late Thermal Pulse in post-AGB stars: the case of DY Cen
› The SOMA MM Survey. I. An Astrochemical Census of Massive Protostars
› The role of black hole feedback on galaxy star formation and the degeneracy with halo quenching
› Apsidal Motion in O-Star Binaries: GENEC rotating binary models put to the k2-test
› Interstellar Comet 3I/ATLAS: Evidence for Galactic Cosmic Ray Processing
› Weak-Lensing Detection of Intercluster Filaments in Three Nearby Cluster Systems
› Shock-driven heating in the circumnuclear star-forming regions of NGC 7582: Insights from JWST NIRSpec and MIRI/MRS spectroscopy
› Tracing the evolution of brightest galaxies and diffuse light in galaxy groups
› {\sc ampere}: A tool to fit heterogeneous observations consistently
› oMEGACat. VIII. A Subpopulation Census of {\omega} Centauri
› Model-independent late-universe measurements of $H_0$ and $\Omega_\mathrm{K}$ with the PAge-improved inverse distance ladder
› $\Lambda$vCF: Extending $\Lambda$CDM into a Unified Model with Particle Creation
› The light curve model fitting of LMC Cepheids: MESA-RSP versus Stellingwerf's code predictions
› XRISM Observations of The Prototypical Cold Front in Abell 3667
› Joint Analysis of Optical, Near-Infrared And Mid-Infrared Variability of 4 Quasars at Redshift < 1
› Optimizing Long-term Variability of AGN Light Curves. I. A Case Study with ZTF Observations in the EGS Field
› Neon is an inhibitor of CO hydrogenation in pre-stellar core conditions
› The dance of dust: Investigating young stellar object dipper variability
› The rotation speed of the spiral pattern in the Milky Way galaxy
› In space there will be no need to scream - Limits to the presence of giant planets in the $\zeta^2$ Ret system
› A summary of instruments proposed for observing pulsating variables from the Mt. Abu Observatory
› CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
› A test of invariance of halo surface density for FIRE-2 simulations with cold dark matter and self-interacting dark matter
› Combined Orbital and Thermal Evolution of Oort Cloud Comets
› The $N_H$ Distribution of Hard X-ray Selected AGN in the NEP Field
› A Star's Death by a Thousand Cuts: The Runaway Periodic Eruptions of AT2023uqm
› The magnetic fields of the dusty nuclei and molecular outflows of Arp 220
› Hybrid Physical-Neural Simulator for Fast Cosmological Hydrodynamics
› The second data release of the Indian Pulsar Timing Array: Investigating the Effect of Coronal Mass Ejection on PSR J1022+1001 and a Possible Mode Change of PSR J2145-0750
› The chemical DNA of the Magellanic Clouds IV. Unveiling extreme element production: the Eu abundance in the Small Magellanic Cloud
› Tidal disruption events with SPH-EXA: resolving the return of the stream
› The 2024 July 16 Solar Event: A Challenge To The Coronal Mass Ejection Origin Of Long-Duration Gamma-Ray Flares
› Investigating episodic mass loss in evolved massive stars IV. Comprehensive analysis of dusty red supergiants in NGC 6822, IC 10, and WLM
› An extremely fast fading population II dwarf nova candidate: caught spectroscopically on the rise
› The ODYSSEUS Survey. Spatial correlation of magnetospheric inclinations points to parsec-scale star-cloud connection
› Stellar Spectroscopy Using Diffraction Grating, CMOS Monochrome Sensor, and Reflecting Telescopes
› Flinch: A Differentiable Framework for Field-Level Inference of Cosmological parameters from curved sky data
› Active Dwarf Galaxy Database II: Connections between Host Galaxy Properties and Black Hole Accretion Signatures
› The Weighing Halos Accurately, Locally, and Efficiently with Supernovae (WHALES) Survey Overview and Initial Data Release
› Unbiased Primordial Gravitational Wave Inference from the CMB with SMICA
› Compact Accretion Disks in the Aftermath of Tidal Disruption Events: Parameter Inference from Joint X-ray Spectra and UV/Optical Photometry Fitting
› The Library of Exoplanet Atmospheric Composition Measurements: Population Level Trends in Exoplanet Composition with ExoComp
› Boosting the cosmic 21-cm signal with exotic Lyman-$\alpha$ from dark matter
› Beyond general relativity: gravitational waves in non-minimally coupled theories
› Ensuring Outcome-Based Curriculum Coherence through Systematic CLO-PLO Alignment and Feedback Loops
› Beyond GRMHD: A Robust Numerical Scheme for Extended, Non-Ideal General Relativistic Multifluid Simulations
› KM3-230213A and IceCube Neutrino Events from Metastable Dark Matter of Primordial Black Hole Origin
› Testing the type-II seesaw mechanism with gravitational waves
› Generative Artificial Intelligence for Air Shower Simulation
› Mapping Anisotropies in the Stochastic Gravitational-Wave Background with space detector networks
› Study of neutrino spin oscillations in a gravitational field with a differential equations method
› Wavefront Curvature and Transverse Atomic Motion in Time-Resolved Atom Interferometry: Impact and Mitigation
› Charged Rotating Black Hole and the First Law
› Supermassive black holes from inflation constrained by dark matter substructure
› Constraining binary mergers in AGN disks using the non-observation of lensed gravitational waves
› Resurrecting Gravitational Vector Modes and their Magnetogenesis
› Timescales of Quasar Accretion Discs from Low to High Black Hole Masses and a Turnover at the High Mass End
› EELG1002: A Record-Breaking [OIII]+H$\beta$ EW $\sim 3700$\AA~Galaxy at $z \sim 0.8$ -- Analog of Early Galaxies?
› Radiation-driven dusty outflows from early galaxies
› The role of equation of state on the spin-up of millisecond pulsars
› Detecting stochastic gravitational wave background from cosmic strings with next-generation detector networks: Component separation based on a multi-source astrophysical foreground noise model
› COSMOS Spectroscopic Redshift Compilation (First Data Release): 488k Redshifts Encompassing Two Decades of Spectroscopy
› Probing the cosmic baryon distribution and the impact of AGN feedback with FRBs in CROCODILE simulation
› Capturing Small-Scale Reionization Physics: A Sub-Grid Model for Photon Sinks with SCRIPT
› What Determines the Brightness of the Magnetically Open Solar Corona?: Insights from Three-dimensional Radiative Magnetohydrodynamic Simulations and Observations
› Identifying Astrophysical Anomalies in 99.6 Million Cutouts from the Hubble Legacy Archive Using AnomalyMatch
› A Hyperactive FRB Pinpointed in an SMC-Like Satellite Host Galaxy
› Hubble constant measurement from QPEs as electromagnetic counterparts to extreme mass ratio inspirals
› Planetary Obliquity Excitation Through Pre-Main Sequence Stellar Evolution
› A Late-time Radio Survey of Type Ia-CSM Supernovae with the Very Large Array
› Application of interpretable data-driven methods for the reconstruction of supernova neutrino energy spectra following fast neutrino flavor conversions
› Beyond monoculture: Polydisperse moment methods for sub-stellar atmosphere cloud microphysics II. A three-moment gamma distribution formulation for GCM applications
› Cosmological Preference for a Positive Neutrino Mass at 2.7$\sigma$: A Joint Analysis of DESI DR2, DESY5, and DESY1 Data
› SN 2024gy: Multi-epoch Spectroscopic Features Suggestive of Delayed Detonation in a Type Ia Supernova
› The role of migration traps in the formation of binary black holes in AGN disks
› In-Situ Formation of the Cold Classical Kuiper Belt
› Numerical simulations of oscillations for axisymmetric solar backgrounds with differential rotation and gravity
› SDSS-V LVM: Detectability of Wolf-Rayet stars and their He II ionizing flux in low-metallicity environments I. The weak-lined, early-type WN3 stars in the SMC
› AGN-heated dust revealed in "Little Red Dots"
› Acceleration of Heavy Ions at Non-Relativistic Collisionless Shocks
› Binary-lens Microlensing Degeneracy: Impact on Planetary Sensitivity and Mass-ratio Function
› Exploring the Early Universe with Deep Learning
› Understanding the Origins of Super-Puff Planets: A New Mass-Loss Regime Coupled to Planetary Evolution
› SPYGLASS. VII-A. The Demographics and Ages of Small Nearby Young Associations
› Magrathea v2: A planetary interior modeling platform in C++
› Probing the Physical and Chemical Characteristics of an Extremely Early Class 0 Protostar in G204.4-11.3A2-NE
› Evolution of accretion disc-corona in the TDE Candidate AT 2019avd
› Filamentary accretion flows in high-mass star-forming clouds
› Population of Binary Black Holes Inferred from One Hundred and Fifty Gravitational Wave Signals
› AnomalyMatch: Discovering Rare Objects of Interest with Semi-supervised and Active Learning
› Constraints to Lorentz violation and ultrahigh-energy electrons in D-foamy space-times
› Constraining the Deviation of Kerr Metric via Bumpy Parameterization and Particle Swarm Optimization in Extreme Mass-Ratio Inspirals
› Spinning black holes in astrophysical environments
› Multi-scale optimal control for Einstein Telescope active seismic isolation
› Numerical computation of electromagnetically sourced nonlinear tails
› Precision gravity constraints on large dark sectors
› Observable spins in gravitational waves from compact binary mergers
› Illuminating the lantern: coherent, spectro-polarimetric characterisation of a multimode converter

  ↓↑    

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