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: zanim się zacznie pracę ....
zanim się zacznie pracę ....
S Webcam

Kamerka S

Webcam

Kamerka N

Allsky

Niebo

Temperatura
3.3 °C

Wilgotność
 92%

Wiatr
12.9 km/h

Ciśnienie
1016.4 hPa

Moon

Księżyc

 Wiadomości z astronet.pl

› Film poklatkowy (timelapse) w astrofotografii
› Start misji Artemis II – od podstaw
› Kosmiczny przegląd miesiąca AstroNETu – marzec 2026 roku
› Katalog Caldwella: C49
› Podwójny debiut dla Chin – pierwszy lot rakiety Kinetica-2 i kapsuły Qingzhou-1
› Niebo w kwietniu 2026 roku
› Scanway debiutuje na Głównym Rynku GPW
› Znamy wyniki II Olimpiady Astronomicznej Juniorów
› Nowe plany NASA ujawnione we wtorek
› Powrót Starshipa już za 2 tygodnie?
RSS  Najnowsze prace na astro-ph:

› Out-of-Domain Stress Test for Temporal Braid Group Privilege Escalation Detection
› Site selection constraints and options for LILA-Pioneer and LILA-Horizon
› A high-resolution study of the double radio relic system in MACS J1752.0+4440
› An analytical approach to binary populations in globular clusters
› Supernova 2025wny: High-angular resolution Keck/NIRC2 observations and preliminary lens modeling
› Cosmology-Independent Constraints on the Etherington Relation and SNeIa Absolute Magnitude Evolution from DESI-DR2
› PLATO input catalogs for technical calibration and fine guidance
› Cosmic-web quenching with DESI DR1: T-Web environments and mass-dependent red/blue classification
› Return to the Great Attractor: Strong Evidence for a Steradian-sized Flow Converging at $\sim$70 Mpc within the GA Supercluster and Aligned with the CMB Dipole
› Speed-Error Cross-Correlation Dating of Ancient Star Catalogues, with Application to the Almagest
› The South Pole Telescope AGN Monitoring Campaign: First Release of SPTpol Bright AGN Light Curves
› The Inner Dark-Matter Structure of Galaxies
› Extreme Values of Black Hole to Stellar Mass Ratio for High-Redshift Galaxies
› Monitoring Volatile Evolution in Disrupting Comet D/2021 A1 (Leonard) with NOEMA and APEX
› Pulsar scintillation studies with LOFAR III. Annual variations in PSR~J0814$+$7429
› The dwarf nova EX Draconis: a short review
› The accretion-driven eruption of the recurrent nova T Corona Borealis
› The Stellar "Snake"-III: Co-evolution of Stars and Molecular Clouds Unveiled by Gaia, MWISP, and LAMOST
› What Are Pulsar Companions Made of? Using Gravitational Tides to Probe Their Compositions
› Spectroscopic Redshifts for 461 Euclid Q1 Strong Gravitational Lenses from NISP Slitless Spectroscopy
› PhDLspec: physical-prior embedded deep learning method for spectroscopic determination of stellar labels in high-dimensional parameter space
› Spin effects in superfluidity, neutron matter and neutron stars
› Inferring population III star properties from the 21-cm global signal
› Single field slow-roll inflation with step uplift to $n_s=1$
› Holmberg IX: A Unique, Infant but Inactive Galaxy as Revealed via a Multiwavelength Approach
› Tearing Driven Reconnection: Energy Conversion Involving Firehose Kinetic Instabilities (2D Hybrid M\"obius Simulations)
› Optical observations and atomic environment of supernova remnant G25.1-2.3
› PENELLOPE: IX. Lithium, iron and barium elemental abundances in eight nearby young clusters
› Tracing the relic nature of compact galaxies through their globular cluster systems
› Machine Learning Assisted NEO Discovery and Polarimetric Characterisation with Astronomical Surveys
› Evidence of Enhanced Ionization in Protostellar Envelopes
› A statistical study of the environmental age of core-collapse supernovae based on VLT/MUSE integral-field-unit spectroscopy
› A 1151-Year Quasi-Commensurability Among the Pre-Uranian Planets: Empirical Detection and Statistical Characterization
› Quantitative spectroscopy of single and multiple OB-type stars. Non-LTE spectrum analysis with machine learning
› Which filaments matter: the relative scalings of anisotropic infall
› The tidal evolution of satellite galaxies in cosmological simulations: insights from COLIBRE
› Isochrone-cloud fitting and asteroseismology of the Kepler open cluster NGC6866
› Cosmological Constraints from GW-FRB Associations without Redshift Measurements for LIGO-Virgo and Cosmic Explorer
› Mapping the redshift drift at various redshifts through cosmography
› DeepDISC-Euclid: Source Classification and Photometric Redshifts in Euclid Deep Field North With a Pixel-Level Deep Learning Approach
› CO and N2 Produced from H2O, CO2, and NH3 Cometary Ice Analogs
› Parametric SED Modelling of Protoplanetary Discs: Validation and Application to an Unstudied YSO
› UNIONS-3500 Weak Lensing: II. B-mode validation for cosmic shear
› Stars Born in the Wind II: Widespread Extra-planar Star Formation in M82's Halo
› The Black Hole Mass Gap as a New Probe of Millicharged Particles
› Millicharged Particle Production During Late-Stage Stellar Evolution
› Imprint of matter-antimatter asymmetry on collapsing domain walls
› Exact general relativistic solutions for a cylindrically symmetric stiff fluid matter source
› Proton Temperature Anisotropy Across Interplanetary Shocks: A Statistical Analysis with WIND observations
› A comparison of methods for Poisson regression in the presence of background
› Spacetime backreaction on particle trajectory could source flat rotation curve
› Revisiting the Rhoades-Ruffini bound
› Near-infrared emission line diagnostics for AGN from the local Universe to redshift 3
› Chaos in Inhomogeneous Neutrino Fast Flavor Instability
› Wideband Monitoring of FRB 20180916B Across a Half-Decade Bandwidth Using the Upgraded GMRT
› Influence of photometric galaxies redshift distribution in BAO estimation
› Category-based Galaxy Image Generation via Diffusion Models
› EMPRESS. XV. A New Determination of the Primordial Helium Abundance Suggesting a Moderately Low $Y_\mathrm{P}$ Value
› Interacting bosonic dark energy and fermionic dark matter in Einstein scalar Gauss-Bonnet gravity
› Tracing the high-z cosmic web with Quaia: catalogues of voids and clusters in the quasar distribution
› Moderate Nesting and Cross-Equatorial Asymmetry of Active Regions in Solar Cycle 24
› NGC 3521 as the Milky Way near twin: spectral energy distribution from UV to radio decameter ranges
› Exploring the Limits of Machine Learning Classification of Neutron Star Matter Models
› Mapping the Distorted Dark Matter Distribution of the LMC-SMC System Prior to Milky Way Infall with Basis Function Expansions
› Investigating the Center-to-Limb Effects in Helioseismic Data Using 3D Radiative Hydrodynamic Simulations
› Time delay measurements with Broken Power Law model
› Little Red Dots as Hidden Neutrino Sources
› Inferring hemispheric asymmetries of stellar active regions through the information content of astrometric signals
› Radio-Interferometric Image Reconstruction with Denoising Diffusion Restoration Models
› Coupled Thermal-Chemical Evolution Models of Sub-Neptunes Reveal Atmospheric Signatures of Their Formation Location
› Stone Skipping Black Holes in Ultralight Dark Matter Solitons
› Formation of first star clusters under the supersonic gas flow -- III. Environmental trends and halo-to-halo scatter in the Pop III IMF
› Mechanism for reduction of the afterpulsing rate of PMTs
› Discovery of a $z\simeq 4.9$ Lyman-$\alpha$ Emitter Protocluster: Wavelength-Dependent Environmental Effects on Galaxy Structure
› The Age of the R127 & R128 Clusters: Implications for the LBV
› Discovery of Bimodal Drift Rate Structure in FRB 20240114A: Evidence for Dual Emission Regions
› Identifying AGNs from X-ray detections-I: Metallicity calibrations in AGNs with X-ray luminosity as the primary input parameter
› An Intertwined Short and Long GRB with 4-minute Separation
› Traces of Helium Detected in Type Ic Supernova 2014L
› Muonic Boson Limits: Supernova Redux
› The UV Sensitivity of Axion Monodromy Inflation
› Detecting Parity-Violating Gravitational Wave Backgrounds with Pulsar Polarization Arrays
› Accelerating parameter estimation for parameterized tests of general relativity with gravitational-wave observations
› QCD-driven dark matter: AQNs formation and observational tests

  ↓↑    

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