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: gwiazdy nad kopułą
gwiazdy nad kopułą
Cloud conditions

Chmury

Rain conditions

Opady

Allsky

Niebo

Temperatura
14.7 °C

Wilgotność
 66%

Wiatr
1.6 km/h

Ciśnienie
1026.0 hPa

Moon

Księżyc

 Wiadomości z astronet.pl

› Creotech udostępnił strategię rozwoju na nadchodzące lata
› Starship IFT-12 poleciał: czy to krok SpaceX w stronę Księżyca?
› Masywne gromady gwiazd szybciej rozpraszają otaczające je obłoki gazowe
› Co w piszczy w Polskiej branży kosmicznej? Czyli XVIII Europejski Kongres Gospodarczy
› Łazik Curiosity odkrył na Marsie związki organiczne dotychczas tam niezidentyfikowane
› Lot testowy Starship V3 od SpaceX już niedługo. Co zmieniono?
› Dragonfly – testy idą pełną parą!
› Zapraszamy na wydarzenie SGH Aviation Days
› Misje kosmiczne XX wieku: misje słoneczne
› Kosmiczna inicjatywa państw Trójmorza
RSS  Najnowsze prace na astro-ph:

› A No-Go Theorem for the Mass-Radius Relation of Solitons
› Mergers via failed common envelope as a route towards intermediate-mass stripped stars
› A Precise Measurement of the Fermi-LAT Galactic Center Excess Morphology and Spectrum
› No Blue without Red: Evolutionary Properties of Super-Early Galaxies
› Mg II h&k spectral line properties computed using 3D radiative transfer in an enhanced network region simulated with the MURaM-ChE code
› Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds
› Magnetic field dynamics in isolated neutron stars with an external dipole field
› Star-planet interaction in the Proxima system
› JWST-DECO: The Impact of Accretion on Mid-Infrared Observable Water in Planet-forming Disks
› The first 3D MHD core-collapse progenitors I: General properties, convection and nuclear burning
› Towards Doppler eclipse mapping of hot Jupiters. An observational perspective on WASP-33 b with SPIRou
› The $\tau$ of Neutral Hydrogen: Increased CMB Optical Depth at Long Wavelengths
› The first 3D MHD core-collapse progenitors II: Rotation, magnetic-field amplification, and magnetic topology
› Gravitational waves from cosmic strings with friction: analytical approximations and parameter space
› The unique capabilities of HST for stellar physics Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars
› The Solar Dynamics Observatory in the Living With a Star Era: From Solar Observations to Predictive Heliophysics
› \texttt{calypso}: a Parameter-Conditioned Stochastic Surrogate Model for Circumbinary Accretion Time-Series
› Gaia Exoplanet Orbits, Demographics, and Evolution Survey (GEODES): Characteristics of Three Long-Period Companions Accelerating their Host Stars
› JWST reveals anomalously enhanced methane outgassing from below Chiron's water ice and carbon dioxide bearing surface
› SDSS+JWST Census of Stellar and Nebular Dust Attenuation at $z \sim 0$-7: Mass Dependence and Redshift Evolution
› A Strongly Parametrized Mass Ratio Model for the Stable Mass Transfer Channel: a Case Study of the $10 \, \rm{M}_{\odot}$ Peak
› Constraining the Photon Intensity of Extragalactic Background Light with the HAWC Observatory for the Blazar Mrk 421
› Increasing the Precision of Surrogate Models for Weak Lensing Mass Maps with Flow Matching
› Evidence of radial-migration driven Galactic disc expansion with the U-shape stellar age profile
› A Gaia-linked High-purity QSO Candidate Catalog in Selected Fields with Extinction-binned Calibration and Spectrum-informed Training
› An Improved HDBSCAN-based Detection and Tracking Method for Solar Active Regions in Magnetograms
› TESS Observations of Stochastic Low-frequency Variability in Extreme Helium Stars
› Suppression of star formation at the centre of barred AGN galaxies
› Rotation-curve residuals reveal a suppressed acceleration branch in dwarf galaxies
› Superrotation and Jet Migration in Simulations of Jupiter's Convective Zone and Weather Layer
› The dual effect of group-scale environments on galaxy quenching during cluster infall: pre-processing and protection
› Dissecting the Perseus-Pisces supercluster observed with CFHT-MegaCam: Exploring late-type galaxy shape alignments within the local cosmic web
› Size-Dependent Fresh Surface Signatures in Asteroid Families: Observational Evidence from Dual-Band Albedo Analysis
› Cosmological constraints from neighbor-density-weighted marked correlation functions
› Performance analysis of extragalactic classifications in Gaia Data Release 4
› ALMA CO-CAVITY I. Resolved Molecular Gas in Void Galaxies
› Nature of HD 251108: an RS CVn binary with a long-term evolving spot
› Insights from Analytical Theory of Eccentric Circumbinary Disks II. Forced Modes and Resonance for Precessing Binaries
› Cosmic web stripping and starvation of low-mass filament galaxies in TNG50
› TOI-7154b: A Close-in Massive Brown Dwarf in an Eccentric Orbit
› Disruption of a Giant: Spectroscopic Identification of Members in the Periphery and Tidal Tails of $\omega$ Centauri
› Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona
› A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz
› Examining extinction distributions for type Ia supernovae in simulated 3D galaxies
› Ensemble asteroseismology: An ensemble approach to detecting signatures of solar-like oscillations in K-dwarfs
› Design and Development of Cassegrain Module for PARAS-2 Spectrograph (CAMPAS)
› Scalable Dark Siren Cosmology with gwcosmo: GPU Acceleration, Validation and Systematics
› Inferring the role of binary neutron star mergers in r-process nucleosynthesis with multi-messenger observations using Cosmic Explorer and Einstein Telescope
› Atomic gas properties at the positions of supernovae Type Ia, II, and Ib/c
› 51 Peg b revisited with VLT/CRIRES+. Constraints on atmospheric thermal structure, chemical composition, and an alternative orbital solution
› A Markov-Chain-Monte-Carlo-based Hybrid Noise Inference for Continuous Wavelet Power Spectra: with Applications to Solar and Stellar Oscillatory Signals
› Multi-layered model-based characterisation of the local-Universe galaxy data from the GAMA survey
› Investigation of the Two-Dimensional Velocity Field of the Large-Scale Coronal Wave from September 6, 2011 using the SOLERwave Tool
› Long-term optical and near-infrared photometric evolution of SN 2019vxm, an interacting Type IIn supernova
› Gas Fraction and Depletion Time Drive the Main-Sequence Scatter in Massive Galaxies at $z\sim1.5$
› Modeling (Sub-)millimeter Scattering Properties of Fractal and Consolidated Porous Particles: Applications to Protoplanetary Disks
› HiFAST: An HI data calibration and imaging pipeline for the FAST IV: The stray-radiation correction
› The FAST Hundred-Deg$^2$ HI Deep (HD$^2$) Survey: Early Results from the Pilot Survey
› The s- and r- components of the proto-solar composition
› New substellar candidates identified through deep learning in the F150 sample of the large-scale SHINE direct imaging survey
› A Wavelet-Integrated Search Pipeline for Narrowband Technosignatures in FAST Observations of 33 Exoplanet Systems
› Hydrodynamic model of nonthermal emission from the Fermi bubbles
› Gaia-Sausage-Enceladus: Lithium evolution from early red-giant-branch and main-sequence stars
› Probing the environments of FRI and FRII radio galaxies in LoTSS DR2 with galaxy clusters
› Probing Solar Wind Structures with Solar Energetic Particle Observations from Solar Orbiter
› GMRT Survey of Radio Emission from Magnetic Massive Stars -- I: Emission from Single Stars at sub-GHz Frequencies
› Gaia FGK benchmark stars: abundances of \textit{n}-capture elements of the third version
› Sharper Than Ever: Do Modern Observations Pin Down the Solar Radius to Converge on New Standards?
› Unsupervised Chemo-Dynamical Dissection of the Inner Galactic Halo: Discovery of Five Accreted Substructures with SDSS-V and Gaia
› Astrophysical Parameters of 5056 Open Star Clusters from Bayesian Nested Sampling with PARSEC Isochrones
› Integral field spectroscopy with no IFUs: combining wide-field rotational slitless spectroscopy with tomographic reconstruction
› An extremely bright slow-rising afterglow from an off-axis jet in GRB 260310A
› cloelib: A Flexible Python Library for Computing Cosmological Observables in the Euclid Era
› cloelike: A Python Library for Cosmological Likelihood Inference in the Euclid Era
› Minor Merger, Major Growth: An Overmassive, Highly Accreting Black Hole Powering a Secondary AGN In a Cosmic Noon Minor Merger
› Evaluation and Modeling of Pneumatic Percussive Drill for Martian Subsurface Access
› Gravitational Field of a Rotating Mass on an Expanding Universe
› Cuspidal Singularities in Collapsing Domain Walls
› Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades
› Quasiradial oscillations of rotating hybrid neutron stars
› Reachability for Low-Thrust Trajectories via Maximum Initial Mass
› Natural Metric-Affine Inflation: Reloaded
› Rapid cooling of the Cassiopeia A neutron star due to superfluid quantum criticality
› Catalog-based detection of unrecognized blends in deep optical ground based imaging
› Cloudy mornings and clear evenings on a gas giant exoplanet
› Probing spectral variability in NGC 4490 ULX-8 over 24 years of XMM-Newton, Chandra and Swift-XRT observations
› Cosmic shear with one component and its application to future radio surveys
› Source REconstruction of Arcs behind Cluster Halos (SourceREACH): A New Source Reconstruction Algorithm Optimized for Giant Arcs and Galaxy Cluster Lenses
› Consequences of radially correlated rotation curves for galaxy mass models
› Rotational Light-curve Recovery and Predictions of the LSST Yield of Hildas
› Maximum Energy of Particles Accelerated in Gamma-Ray Burst Afterglow Shocks
› Little Red Dot $-$ Host Galaxy $=$ Black Hole Star: A Gas-Enshrouded Heart at the Center of Every Little Red Dot
› Simulation-based cosmological inference from optically-selected galaxy clusters with $\texttt{Capish}$
› POSEIDON I: The Dynamical Origins of Transiting Neptunes
› Anisotropic Diffusion in Pulsar Halos: Interpreting the asymmetric morphology of Geminga and Monogem halos measured by HAWC
› pyKurucz: A Pure Python Reimplementation of Kurucz ATLAS12 and SYNTHE for Stellar Spectrum Synthesis
› Implications of a Cosmogenic Origin of KM3-230213A for Ultra-High-Energy Protons
› The dominance of turbulence over magnetism in the formation of massive star cluster seeds
› Reliability of uGMRT Band-4 Polarimetry: Results from a Quadrature Hybrid Polarizer Bypass Experiment
› Correlation between Ultrahigh-Energy Neutrino KM3-230213A and Gamma-Ray Bursts
› TDCOSMO XXV: A "soup-to-nuts" 6.5% $H_0$ measurement $-$ strong lensing and dynamics with a maximally flexible mass sheet
› Superfluid $^3$He aerogel experiments as a laboratory neutron star analogue
› Investigating the formation channel of GW231123: Population III stars or hierarchical mergers?
› Detectability of Polarized Gamma-ray Emission from Blazar Flares with COSI
› The NUV transit of XO-3 b
› Stellar Age Compression Reshapes Interpretations of the Milky Way Thick-Disk Formation History
› SN 2023fyq: direct detection of a Type Ibn supernova progenitor and its multi-wavelength environmental constraints
› 29SiO and 30SiO J=1--0 maser signatures in Galactic AGB stars: the impact of third dredge up and turbulence velocity
› Spectra as Language: Large Language Models for Scalable Stellar Parameter and Abundance Inference
› Pulsar timing solutions for 17 pulsars at 150 MHz from the Irish LOFAR station
› Follow the wobble: Statistical methods to detect astrometric binary asteroids in Gaia FPR
› Thermodynamical uncertainties for primordial black holes from cosmological phase transitions
› Shedding light on dark matter spikes through refractive neutrino masses
› Global time-frequency search for stellar-mass binary black holes in LISA
› Superfluid fraction in the crystal phase of the inner crust of neutron stars
› Cosmological coupled black holes immersed in dark sector
› Greybody Factor, Resonant Frequencies, and Entropy Quantization of Charged Scalar Fields in the Kerr-EMDA Black Hole

  ↓↑    

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