Obserwatorium Astronomiczne na Suhorze Strona główna
in English
ul. Podchorążych 2, 30-084 Kraków. tel.: (+48 12) 662 6301; fax: (+48 12) 637 2243; Obs. tel.: (+48) 502 113714
  • Strona główna
  • Dla studentów
  • Wydarzenia

Obserwatorium Astronomiczne na Suhorze

Informacje
  • Harmonogram
  • O Obserwatorium
  • Pracownicy
  • Publikacje
  • Zdjęcia
  • Instrukcje · Programy
  • Pogoda
Gwiazdy Zaćmieniowe
  • TIDAK (baza danych O-C)
Linki
  • Astronomia
  • Astronomia w Polsce
  • Inne
Popularnonaukowe
  • Kalendarz astronomiczny
  • Fazy Księżyca
  • Materiały edukacyjne do pobrania
  • Astronomia w Krakowie
Astronomia w Krakowie
Zdjecie: Suhora w nocy
Suhora w nocy
S Webcam

Kamerka S

Webcam

Kamerka N

Allsky

Niebo

Temperatura
8.7 °C

Wilgotność
 67%

Wiatr
0.0 km/h

Ciśnienie
1023.1 hPa

Moon

Księżyc

 Wiadomości z astronet.pl

› Kosmiczny przegląd miesiąca AstroNETu – luty 2026 roku
› Niebo w marcu 2026 roku
› Artemis III nie wyląduje na Księżycu. NASA ogłasza duże zmiany
› Startrails, czyli najprostszy astrokrajobraz
› W Układzie Słonecznym: Granice Układu Słonecznego
› Tam, gdzie SPACE spotyka DEFENCE. SpaceShield Summit 2026 – ostatnie wolne miejsca!
› Misje kosmiczne XX wieku: program Sojuz
› Pixinsight cz. VII – XTerminatory
› Stany Zjednoczone odtajniły informacje o programie satelitów szpiegowskich JUMPSEAT
› Wstęp do astrofotografii krajobrazowej
RSS  Najnowsze prace na astro-ph:

› Two-body relaxation in the EMRI-TDE disk model for Quasi Periodic Eruptions
› Bridging the Prandtl number gap: 3D simulations of thermohaline convection in astrophysical regimes
› High Velocity Circumstellar Gas Orbiting a White Dwarf Star
› Constraints on White Dwarf Hydrogen Layer Masses Using Gravitational Redshifts
› The Role of the Heliosphere in Shaping the Observed Cosmic Ray Spectral Anisotropy
› Synthetic Spectral Library of Optically Thick Atmospheres for Little Red Dots
› The ESPRESSO Redshift Drift Experiment III -- The Third Epoch of QSO J052915.80-435152.0
› Negative superhumps in cataclysmic variables driven by retrograde apsidal disk precession
› Latitude-Dependent Time Variations of the Solar Tachocline
› Isocurvature Constraints on Dark Matter from Evaporated Primordial Black Holes
› Polarisation angle variability in tidal disruption events
› Rapid jet ejection from PKS 0215+015 coincident with a high-energy neutrino event
› Not all nitrogen-rich field stars originate from globular clusters
› The Gravitational-wave Optical Transient Observer (GOTO) data pipeline and workflow for transient discovery
› Crunching, Bouncing, and Cyclical Cosmologies from Dark Sector Interactions
› Particle acceleration and pitch-angle evolution in relativistic turbulence
› Observations of a Twin Pair of Atypical Solar Flares and a Magnetic-reconnection Scenario
› Disc Fragmentation. III. The need for a new paradigm for formation of planets within close binary systems
› Mantle Convection and Nightside Volcanism on Lava World K2-141 b
› The Effect of Atmospheric Chemistry on the Optical Geometric Albedos of Hot Jupiters
› Alpha Cygni Variables as Seen from the Transiting Exoplanet Survey Satellite
› Water enrichment of forming sub-Neptune envelopes limited by oxygen exhaustion
› Quantifying Element Importance for Mass Recovery from Population III Supernova Yield Fits
› The primordial nature of the C-19 stellar stream
› Effects of Resolution and Local Stability on Galactic Disks: 2. Halo Resolution and Softening on Bar Formation
› Evidence for a Delayed UV Counterpart to X-ray Quasi-periodic Eruptions in Ansky
› Observational Properties of Near-Maximally Spinning Supermassive Black Holes
› The solar-like latitudinal distribution of flaring activities revealed by TESS, APOGEE and GALAH
› Mechanism for reduction of the afterpulsing rate of PMTs
› An Adolescent and Near-Resonant Planetary System Near the End of Photoevaporation
› A Tale of Two Origins: In-Situ versus Accreted Nitrogen-Rich Field Stars in the MW
› Dynamics of planetary rings under thermal forces
› Polarity-Resolved Far-Side Magnetograms Based on Helioseismic Measurements
› The MUSE-Faint survey V. The binary fraction of Leo T
› Transverse Oscillations and Wave Propagation in the Magnetically Dominated M87 Jet
› FEASTS and MHONGOOSE: HI Column Density Distribution at $z=0$ for $N_\mathrm{HI}>10^{17.8}\, \mathrm{cm}^{-2}$
› Simulation and Data Processing of Beamforming Experiments with Four 21CMA Stations
› Compact Absorbers surrounding the M87 AGN Revealed by ALMA Band 3 Observations1
› Ionic Liquid Biospheres
› Discovery of energy-dependent phase variations in the polarization angle of Cen X-3
› Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils
› Single-star optical turbulence profiling techniques for the SHIMM and other Shack-Hartmann instruments
› Diffusive dark fluids with Planck-2018 and DESI BAO DR2 Measurements
› Molecular absorption of Cherenkov light at CTAO
› Gaia DR3 high radial velocity stars: Genuine fast-moving objects or outliers?
› The many boundaries of the stratified dark matter halo
› Luminosity-Dependent Variations in the Secondary Maximum of Type Ia Supernovae and Their Connection to Host Galaxy Morphology
› Spatial Property of Multiple Metallic Populations in the Tidal Stream of {\omega} Centauri
› Wind Accretion in Massive Binaries Experiencing High Mass Loss Rates: II. Eccentricity
› A signal dedispersion algorithm for imaging-based transient searches
› New morpho-kinematic classification: The two-dimensional spatial distribution of stellar specific angular momentum in late-type galaxies
› Tilted, warped, and eccentric disks
› Reproducing the stellar-mass dependence of the giant planet occurrence rate with pebble accretion models
› The Evolution of X-ray Spectra in Tidal Disruption Events
› Component masses in stellar and substellar binaries from Gaia astrometry and photometry
› Search for quasar pairs with Gaia astrometric data III. Confirmation of 16 dual quasars and 36 projected quasars
› Dynamics of the TWA 7 planetary system and possibility of an additional planet
› An Origin of Radially Aligned Filaments in Hub-Filament Systems
› ATLAS100 -- I. A volume-limited sample of supernovae and related transients within 100 Mpc
› Nemesis: A Multi-Scale, Multi-Physics Algorithm for Astrophysics
› MOSS II: Mid frequency radio catalog of Saraswati core region
› Estimating the dynamical masses of dwarf galaxies in the presence of binary-star contamination
› Multi-wavelength insights into the pulsar wind nebula candidate near 1LHAASO J0343+5254u: an obscured merging galaxy cluster?
› Testing gravitational wave polarizations with LISA
› The Periastron Passage of T Tauri South B as Viewed by ALMA: Millimeter Flux Variations and Dust Heating Triggered by Orbital Motion
› A broadband search for coherent emission in radio-cataclysmic variables
› Probing Axions with Relativistic Jet Polarimetry
› A fast method to derive relative small-scale magnetic field variations from high resolution spectroscopy
› Neutrino mass limits and decaying dark matter: background evolution versus perturbations
› $\mathcal{H}$-EFTCAMB: A Cobaya-Integrated, Python-Wrapped Extension of EFTCAMB for Covariant Horndeski Gravity
› Radiative Corrections in Supergravity Models of Inflation
› Orbital Dynamics and Gravitational Wave Signatures of Extreme Mass Ratio Inspirals in Galactic Dark Matter Halos
› The Cost of Circularity: Quantifying Eccentricity-Induced Biases in Binary Black Hole Inference
› Probing Planck-Scale Physics with High-Frequency Gravitational Waves
› Nonlinear physics of axion inflation
› Sommerfeld enhancement from unstable final-state particles in dark matter annihilation
› Weinberg Angle, Neutron Abundance in BBN, and Lifetime
› Emerging trends in Cislunar Space for Lunar Science Exploration and Space Robotics aiding Human Spaceflight Safety
› Data-Driven Prediction of Chaotic Transition in Periapsis Poincar\'e Maps
› Magnetic monopoles and high frequency gravitational waves from quasi-stable strings
› Effects of isovector spin-orbit interaction on the charge-weak form factor difference in $^{48}$Ca, $^{208}$Pb, $^{90}$Zr and $^{62}$Ni
› Data Unfolding: From Problem Formulation to Result Assessment
› Ultra slow-turn inflation
› A More Rigorous Test Problem For Viscous Hydrodynamics Codes
› LISA and $\gamma$-ray telescopes as multi-messenger probes of a first-order cosmological phase transition
› Absence of antisymmetric tensor fields : Clue from f(R) model of gravity
› UVIT/AstroSat observation of TW Hya
› Understanding the UV/Optical Variability of AGNs through Quasi-Periodic Large-scale Magnetic Dynamos
› A Quasar Pair Sample Compiled from DESI DR1
› Magnetically arrested transmutation of a compact star
› AGNBoost: A Machine Learning Approach to AGN Identification with JWST/NIRCam+MIRI Colors and Photometry
› Little Red Dots as self-gravitating discs accreting on supermassive stars: Spectral appearance and formation pathway of the progenitors to direct collapse black holes
› Prior-free cosmological parameter estimation of Cosmicflows-4
› A MaNGA about the Legacy I: Connecting the Assembly of Stellar Halo with the Average Star Formation History in Low-Redshift Massive Galaxies
› Hillas meets Eddington: The case for blazars as ultra-high-energy neutrino sources
› Impact of stochastic star-formation histories and dust on selecting quiescent galaxies with JWST photometry
› Euclid: Discovery of bright $z\simeq7$ Lyman-break galaxies in UltraVISTA and Euclid COSMOS
› On the origin of counterrotating stellar disks in TNG50. I
› Revisiting the Orbital Dynamics of the Hot Jupiter WASP-12 b with New Transit Times
› Multi-messenger constraints on LIGO/Virgo/KAGRA gravitational wave binary black holes merging in AGN disks
› Mitigating gain calibration errors from EoR observations with SKA1-Low AA*
› StarDICE IV: correcting visible photometry from atmospheric gray extinction using thermal infrared observations
› High CO/H2 ratios supports an exocometary origin for a CO-rich debris disk
› Euclid Quick Data Release (Q1). Searching for giant gravitational arcs in galaxy clusters with mask region-based convolutional neural networks
› The Evolution in Coma Molecular Composition of Comet C/2017 K2 (PanSTARRS) Across the H$_2$O Sublimation Zone: ALMA Imaging of an H$_2$O-Dominated Coma
› In-Orbit GRB Identification Using LLM-based model for the CXPD CubeSat
› Adsorption of volatiles on dust grains in protoplanetary disks
› The impact of supermassive black holes on exoplanet habitability: I. Spanning the natural mass range
› Accelerating reionization constraints: An ANN-emulator framework for the SCRIPT Semi-numerical Model
› The Northern High Time Resolution Universe pulsar survey: II. Single-pulse search set-up and simulations
› CH$_3$OH and HCN in Interstellar Comet 3I/ATLAS Mapped with the ALMA Atacama Compact Array: Distinct Outgassing Behaviors and a Remarkably High CH$_3$OH/HCN Production Rate Ratio
› Forecasting Constraint on Primordial Black Hole Properties with the CSST $3\times2$pt Analysis
› On the magnetic field evolution of interplanetary coronal mass ejections from 0.07 to 5.4 au
› Comments on "Little ado about everything" by A. Lapi et al. and on cosmological back-reaction
› Resolving dust and Ly{\alpha} emission in a lensed galaxy at the epoch of reionization with JWST/CANUCS
› Magnetic field spreading from stellar and galactic dynamos into the exterior
› Nanohertz Gravitational Waves
› The long quest for vacuum birefringence in magnetars: 1E 1547.0-5408 and the elusive smoking gun
› The kinematic cosmic dipole beyond Ellis and Baldwin
› MIGHTEE/COSMOS-3D: The discovery of three spectroscopically confirmed radio-selected star-forming galaxies at z=4.9-5.6
› Analysis of Galactic cirrus filaments in HSC-SSP high-resolution deep images using artificial neural networks
› Search for Sub-Solar Mass Binaries in the First Part of LIGO's Fourth Observing Run
› Cosmological Simulation with Population III Stellar Feedback and Metal Enrichment I: Model Description And Convergence Test
› ALMA Band 9 CO(6--5) Reveals a Warm Ring Structure Associated with the Embedded Protostar in the Cold Dense Core MC 27/L1521F
› Simultaneous Double Transits of Phobos and Deimos as Seen from the Martian Surface: A Millennium Catalogue
› Primordial Black Hole Formation in Rastall Gravity: Shifted Collapse Threshold and Exponential Abundance Sensitivity
› Constraining the mass of the M31 ionized baryon Halo using CHIME/FRB Catalog 2
› The First Four Ground-Level Enhancements in the 1940s: Investigation, Digitisation, and Analysis of Forgotten Data
› Long-term Spectroscopic Survey of the Hyades Cluster: The Binary Population
› Parameterizations of the Hubble Constant: Logarithmic vs Power-Law Expansion from the Binned Master Sample of SNe Ia
› LCEz4-M1: A Lyman Continuum Emitter Candidate at z = 4.444 in the MUSE Hubble Ultra Deep Field
› Triaxial Schwarzschild Models of Brightest Cluster Galaxies with Long-Slit LBT Data
› A New Identification Method and Sample of Counter-Rotating Disk Galaxies in SDSS-IV MaNGA DR17
› Predicting Gaia astrometry's ability to constrain the populations of circumbinary planets
› Modeling transport in weakly collisional plasmas using thermodynamic forcing
› Towards Realistic Detection Pipelines of Taiji: New Challenges in Data Analysis and High-Fidelity Simulations of Space-Based Gravitational Wave Antenna
› Cosmology of Cubic Poincar\'e Gauge gravity
› Improved Binary Black Hole Search Discriminator from the Singular Value Decomposition of Non-Gaussian Noise Transients
› Impact of cavities on the detection of quadratically coupled ultra-light dark matter
› Dancing in the dark: probing Dark Matter through the dynamics of eccentric binary pulsars
› Hints of Dark Matter Spikes in Low-mass X-ray Binaries: a critical assessment
› Breaking Eternal Inflation: Empirical Viability of a Spontaneous Collapse Scenario
› Stochastic Limit of Growing Gravitational Wave Memory from Sources in the Early Universe and Astrophysical Sources
› High Power RF Pulse Shaping Tests with NG-LLRF and Cool Copper Collider Prototype Structure

  ↓↑    

Powrót do strony głównej Obserwatorium
Deklaracja dostępności cyfrowej
Biuletyn Informacji Publicznej UP
Copyright © 2002-2026 Katedra Astronomii Uniwersytetu Komisji Edukacji Narodowej w Krakowie. Wszelkie prawa zastrzeżone