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
13.3 °C

Wilgotność
 70%

Wiatr
0.0 km/h

Ciśnienie
1026.2 hPa

Moon

Księżyc

 Wiadomości z astronet.pl

› 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
› Spotkaj eksperta. Efekty misji IGNIS: mózg w kosmosie – komunikacja bez użycia mięśni
› Nowe dowody dotyczące atmosfer w układzie TRAPPIST-1
› Start Sojuza-5 Irtysz: czy Rosja wraca w kosmos?
RSS  Najnowsze prace na astro-ph:

› Fisher Information Velocity: A New Geometric Channel for Precision Glitch Identification in Gravitational-Wave Detectors
› Information Content of the Cosmic Web
› (LRDs)$^2$: The Low-ReDshift Little Red Dots Survey. II. DESI DR1 Sample
› First-Principles Turbulence-Driven Deflagration-to-Detonation Transition Mechanism for Near-Chandrasekhar Mass White Dwarf Progenitors
› Investigating central star formation in local AGN host galaxies: is there tension between coeval growth and AGN feedback?
› Gravitational wave detectability range informed by external messengers
› Interstellar Medium-Driven Orbital Transport -- I. Radial Heating and Migration
› Massquerade: Impacts of Mass Ratio Reversals on Binary Black Hole Merger Rates and Mass Distributions
› Still non-accelerating: age-bias correction in supernova cosmology is robust to host-progenitor age mapping
› Decomposing cool stellar populations with H-band spectral fluctuations: Long-period variable stars in NGC 5128 and carbon stars in NGC 5102
› A Magnetized Black Hole Envelope Model for Little Red Dots
› Molecular gas properties of star-forming brightest group galaxies at $z \sim 0.3$
› Predicting intermediate-mass black hole formation in star clusters with machine learning
› Advancing the detection of low surface brightness galaxies. I. ATTILA: multi-tAsking deTecTIon tool for Lsb gAlaxies
› JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: stellar population catalogue for galaxies in GOODS-N and GOODS-S
› 29SiO and 30SiO J=1--0 maser signatures in Galactic AGB stars: the impact of third dredge up and turbulence velocity
› The Absolute Age of the Open Cluster NGC 6791 and Its Implications for Galactic Archaeology and Asteroseismic Calibration
› Bayesian Modeling of NICER Cometary X-ray Spectra: A Legacy Survey of Solar-Wind Charge Exchange
› High-Latitude Zonal Jets in the Martian Upper Atmosphere Driven by Non-Orographic Gravity Waves
› Milky Way Mapper decoded abundances -- II: From patterns to paths
› A Generalized Template Matching Algorithm for Correcting Jitter Noise in Pulsar Timing
› Evidence for neutron capture in heavy-metal hot subdwarfs: Far-UV spectroscopy of EC22536-5304 and LSIV-14 116
› The powerful shocks in RS Oph: NuSTAR X-ray data and a complete review
› Powerful Radio Sources in the Southern Sky. IV. Observations of the G4Jy-3CRE Catalog with the Australian Square Kilometre Array Pathfinder
› An AGN in the Antennae galaxies ?
› Photospheric abundances of the rapidly-rotating A-type star Altair
› Discovery of a Featureless Tidal Disruption Event at z~1 with the Wide Field Survey Telescope
› Machine Learning applications to Galaxy Clusters
› Self-Supervised ConvLSTM for Fermi Large Area Telescope Transient Detection
› There and back again: Mysterious optical pulse profile behavior of the transitional millisecond pulsar PSR J1023+0038
› Blue-tilted Runnings and the JWST Early Galaxy Tension
› Spectra as Language: Large Language Models for Scalable Stellar Parameter and Abundance Inference
› A Unified H i Rotation Curve Database for 129 Local Volume Dwarf and Irregular Galaxies
› Dark photon -- Assisted Primordial Magnetogenesis
› Quasi-Simultaneous Broadband Spectral Energy Distributions of a Sample of Fermi Blazars -- I. Correlation Results
› Silicate cosmic dust grain collisions in the interstellar medium: A molecular dynamics study
› A Robust Deep Learning Framework for Prominence Detection through Composite Feature Representations
› Nature of 4FGL J2249.4+6229: Evidence for a redback system with a cool companion and low X-ray and $\gamma$-ray luminosities
› Probing close-in satellites of Trans-Neptunian Objects through thermal and direct size measurements
› Signatures of Modified Gravity Below $\mathcal{O}(10)$ Mpc in a Dynamical Dark Energy Background
› Magnetar Fireballs and Short Bursts: Curved Spacetime Lensing, QED Effects, High-Energy Spectra and Polarization, and Energy-Time Impulse Responses
› Seyfert galaxy targets for KM3NeT neutrino telescope
› Prospects for detecting surface color heterogeneity on asteroid surfaces from sparse multiband photometric survey data
› Constraining Spatial Curvature with Priors from Swampland Conjectures
› A Weak Fe K$\beta$ Emission Line in the Broad-Line Radio Galaxy 3C 111 Observed with XRISM: An Ionized Wind Absorption Feature?
› Reconstruction of annual solar irradiance over the last three millennia
› STARFIRE-2: Can we detect the global redshifted 21-cm signal from the cosmic dawn in Earth orbit?
› Maximum Lifetime of the Vegetative Biosphere
› Hostless extragalactic transients in Fink: Results from the ELEPHANT pipeline
› Machine Learning Techniques for Astrophysics and Cosmology: Lyman-$\alpha$ forest
› MICONIC: The multiphase circumnuclear region of Centaurus A as seen with JWST/MIRI MRS observations. I. Spectral inventory and properties of the warm molecular disk
› The habitability trade-off: Chemical decoupling and quenching in massive galaxies
› Pulsar timing solutions for 17 pulsars at 150~MHz from the Irish LOFAR station
› Seismic signature of a magnetic field in the $\gamma$ Doradus star KIC 2309579
› Probing the ion-neutral drift velocity towards the L1544 prestellar core: Detection of ambipolar diffusion using N$_2$D$^+$ and para-NH$_2$D
› Configuration of the $\xi$ Tau system constrained by multi-technique observations
› Iron Fluorescence in X-class Solar Flares: Aditya-L1/SoLEXS Observations
› JWST observations of a planetary nebula support jet-driven explosion of core-collapse supernova remnant RCW 103
› Scattered light signatures of flyby-induced warps in protoplanetary discs
› The impact of evolving dark energy on the Weyl potential measured from the Dark Energy Survey Year 3 data
› Decoding the Radial Velocity Signatures of Solar Faculae with 3D MHD Simulations
› Search for radio polarization in the particle-accelerating colliding-wind binaries WR 147 and HD 167971
› HWO Target Stars and Systems: Activity and Rotation Catalog (ARC) of Potential Target Stars for the Habitable Worlds Observatory
› Towards precision cosmology with Void x CMB correlations (II): Impact of mock catalogs on the Void x CMB lensing signal
› Evidence of Radius Inflation Based on 50 Transiting Brown Dwarfs and Low-mass Stellar Companions
› Energetic Feasibility of Redirecting Trans-Neptunian Objects onto Mars-Impacting Orbits: Continuous Thrust and Gravity Assist Trajectories
› Dwarf Galaxy Constraints on Interacting Fermionic Dark Matter
› Follow the wobble: Statistical methods to detect astrometric binary asteroids in Gaia FPR
› Polarized 3D Synthetic Turbulence I: Magnetic Field Line Random Walk
› A Three-Dimensional Tomographic Reconstruction of the Galactic Cosmic-Ray Proton Density
› Mass Segregation in the CMZoom Survey
› Generation of Quantum Turbulence by Neutrino Cooling in Neutron Stars
› Primordial black holes in excursion set theory: Formation probabilities, mass functions, and window functions
› Variation of Venusian Gravity Wave Absolute Momentum Fluxes and Drag as Retrieved from the Akatsuki Mission
› A very rapidly rotating white dwarf in nova YZ Reticuli
› From protogalaxy through thick and thin: Why did the Milky Way evolve in three kinematic phases?
› Wave-optics gravitational wave lensing in modified gravity
› Numerical simulations of shock-driven, supersonic turbulence in colliding three-temperature laboratory plasmas
› Three-Dimensional Velocity Analysis and Particle Size Dynamics from Multi-Site RGB-Photometry of Noctilucent Clouds
› On the Presence of a Tertiary Compact Object in GW190814
› PIC simulations of nonrelativistic high-Mach-number oblique shocks propagating in a turbulent medium
› Probing freeze-in dark matter using Bose-Einstein condensate in neutron star
› Dark Energy in Ghost-free non-local Gravity
› Dynamics of Binary System around a Supermassive Black Hole :Binary Scattering and Eccentric vZLK Oscillations
› X-ray and extreme-ultraviolet spectra from collisions of Ar$^{18+}$ and O$^{8+}$ ions with neutrals
› Dimming of Photon Ring due to Photon-Axion Conversion around Kerr Black Holes
› Galaxy and halo angular clustering in LCDM and Modified Gravity cosmologies
› Precision Inflationary Predictions: Impact of Accurate End-of-Inflation Dynamics
› Redshift Evolution of the HII Galaxy $L$-$\sigma$ Relation: Gaussian Process Analysis and Cosmological Implications
› Large, fast and accurate HI intensity maps with latent overlap diffusion
› COSMOS-Web galaxy groups: Evolution of red sequence and quiescent galaxy fraction
› Testing Lens Models of PLCK G165.7+67.0 Using Lensed SN H0pe
› A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff
› FOGGIE: Figuring Out Gas & Galaxies In Enzo XII. The Formation and Evolution of Extended HI Galactic Disks and Warps with a Dynamic Circumgalactic medium
› The impact of our peculiar motion on primordial non-Gaussianity measurements using the LIGER4GAL framework
› Isocurvature-induced features in multi-field Higgs-$R^2$ inflation
› A Search for Radio Technosignatures from Interstellar Object 3I/ATLAS with the Allen Telescope Array
› Golden and Silver Dark Sirens for precise H0 measurement with HETDEX
› Towards precision cosmology with Voids x CMB correlations (I): Roman-Agora mock catalogs and pipeline validation
› Satellite-borne $\gamma$-ray astrophysics from coherent interactions in oriented crystals
› Uncovering the Next Galactic Supernova with the Vera C. Rubin Observatory
› There and back again? Neutral outflows in z~3.5 quiescent galaxies
› At the stellar noise frontier: A transit survey of 121 TESS M3--M6 dwarfs
› Single-source-class interpretation of the diffuse astrophysical neutrino flux
› Turning the knobs on dust evolution: Comparing codes, parameters and their effects on planet formation and disc observables
› Evolution of Quasi-Periodic Eruptions in the post-TDE Accretion Disk Perturbed by an Orbiting Star
› A Post-starburst Galaxy Undergoing Ram-pressure Stripping at Redshift 3.06
› Large-scale Morphology of the Optical F-corona from a Total Solar Eclipse Observation During the Artemis II Lunar Flyby
› A Salpeter-like filament linear density function across nearby molecular clouds
› Rapid-response 1.3 mm Observations of GRB 260127A with the Submillimeter Array
› SFUMATO#: A GPU-accelerated code for self-gravitational radiation hydrodynamics simulation with adaptive mesh refinement
› Probabilistic Spectral Reconstruction of Trans-Neptunian Objects from Sparse Photometry: A Framework for Taxonomy, Survey Optimization, and Outlier Detection
› Spectral Evidence of Heavy Nuclei from the Neutron Star Crust in Magnetar Bursts
› A short-period binary OGLE-BLG-ELL-006503 showing slow variations in brightness
› The one and the only: the pulsar - white dwarf system in NGC 6749
› A single power law for the TRAPPIST-1 flare distribution across four orders of magnitude in energy
› Dependence on the Equation of State in SPH Simulations of Proto-Uranian Disk Formation from a Giant Impact
› Effective Field Theory for a Baryon-Correlated Dark Matter Profile
› The Beauty of k2: Probing Stellar Interiors Using Apsidal Motion. I. The Benchmark Massive Binary HD 152248
› Probing radiative electroweak symmetry breaking with colliders and gravitational waves
› Warm Inflation with Pseudo-scalar Couplings
› Thermal and Magnetic effects on Bulk Viscosity in Binary Neutron Star Mergers
› GW231123: Overlapping Gravitational Wave Signals?
› Thick Lunar Crust Amplifies Deci-Hertz Gravitational-Wave Signal
› Testing the Spacetime Geometry of Sgr A* with the Relativistic Orbit of S2 star
› High Sensitivity Methodologies to Detect Radio Band Gravitational Waves
› Squashed Pyramid Interferometer Network (SPIN): Direct Access to Chirality of Cosmological Gravitational Waves
› Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries
› Structure of the $^8$B and $^8$Li nuclei and the astrophysical $S_{17}(0)$-factor of the $^7$Be($p,\gamma$)$^8$B direct capture process within a three-body model
› New Exponential and Polynomial $\xi$-attractors
› Reviving primordial black hole formation in slow first-order phase transitions
› The Era of Extremely Large Optical Telescopes: The ELT

  ↓↑    

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