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: Teleskop 60cm na Suhorze
Teleskop 60cm na Suhorze
S Webcam

Kamerka S

Webcam

Kamerka N

Allsky

Niebo

Temperatura
1.7 °C

Wilgotność
 94%

Wiatr
9.7 km/h

Ciśnienie
1008.1 hPa

Moon

Księżyc

 Wiadomości z astronet.pl

› Japońska technologia powraca na ISS. Pierwsza misja nowej kapsuły zaopatrzeniowej HTV-X
› Medale dla Polski na IV Międzynarodowej Olimpiadzie z Astronomii i Astrofizyki Juniorów
› Katalog Caldwella: C50
› Misje kosmiczne XX wieku: Columbia
› Jak pogoda wpływa na misje kosmiczne?
› Początek 4. Międzynarodowej Olimpiady z Astronomii i Astrofizyki Juniorów
› Jak wygląda praca geologa planetarnego? – wywiad z Dr Jakubem Ciążelą
› Katalog Caldwella: C8
› Największy polski (toruński) radioteleskop w tarapatach
› W Układzie Słonecznym: Pas Planetoid
RSS  Najnowsze prace na astro-ph:

› Generating background-corrected VPHAS+ HiPS with Montage
› Metallicity regulates planet formation across all masses
› Definition of Exoplanets and Brown Dwarfs
› Analytic Marginalization over Binary Variables in Physics Data
› How to Build an Empirical Speed Distribution for Dark Matter in the Solar Neighborhood
› Shadows of the Colossus: Hierarchical Black Hole Mergers in a 10-million-body Globular Cluster Simulation
› XRISM constraints on the velocity power spectrum in the Coma cluster
› Suppressed "lump" EM signature in radiation pressure dominated accreting massive black hole binaries
› The velocity dispersion profile of nine open clusters in the solar neighborhood
› Likelihood Reconstruction for Radio Detectors of Neutrinos and Cosmic Rays
› Illuminating the Diffuse Radio Emission in Low-Mass Cluster: Abell 13
› Characterizing Low-Latency Sky Localization in Multi-Detector Gravitational-Wave Networks
› Dynamical Dark Energy Meets Varying Electron Mass: Implications for Phantom Crossing and the Hubble Constant
› SPYGLASS. VII-A. The Demographics and Ages of Small Nearby Young Associations
› Under Pressure: Decoding the Effect of High Densities on Derived Nebular Properties
› Earth Analogs in Reflected Light: Insights from Early Spectral Characterization in Unconstrained Orbits
› Evidence for Dynamical Dark Energy using DESI DR2 Ly$\alpha$ Forest
› On the acceleration of cosmic rays at the post-adiabatic shocks of supernova remnants
› Tracing The Start and End of Cosmic Reionization - Exploring The Role of Ionizing Sources as drivers
› Quasi-Biennial Oscillations and Rieger-type Periodicities in a Babcock-Leighton Solar Dynamo
› The variability angular diameter distance and the intrinsic brightness temperature of active galactic nuclei
› Impact of Charge Transfer Inefficiency on transit light-curves: A correction strategy for PLATO
› The Solar Neighborhood. LV. M Dwarf Twin Binaries -- One in Five Twin Sibling Pairs Are Mismatched in Activity and/or Rotation
› Discovery of multi-temperature coronal mass ejection signatures from a young solar analogue
› Do Young Suns Produce Frequent, Massive CMEs? Results from Five-year Dedicated Optical Observations of EK Draconis and V889 Hercules
› Coronal Mass Ejections from Young Suns: Insights from Solar and Stellar Observations and Models
› The oscillation properties of the Blue Large Amplitude Pulsators (BLAPs): relative change rate of periods, excitations, and period relations
› A great diversity of spectral shapes in the ionising spectra of z ~ 0.6 - 1 galaxies revealed by HST/COS and possible detection of nebular LyC emission
› Living with Neighbors. V. Better-aligned Spiral+Spiral Galaxy Pairs Show Stronger Star Formation
› Constraining the Hubble Constant using Cross-Correlation of Gravitational Wave Events with Flux-Limited Galaxy Catalog
› RGC: a radio AGN classifier based on deep learning. I. A semi-supervised model for the VLA images of bent radio AGNs
› Ultraviolet Spectral Evidence for Ansky as a Slowly Evolving Featureless Tidal Disruption Event with Quasi-periodic Eruptions
› Avoiding PBH overproduction in inflation model with modified dispersion relation
› K-DRIFT: Unveiling New Imagery of the Hidden Universe
› Photometric and Spectroscopic Studies of Four Low Mass-ratio Contact Binaries with Period Longer than 0.7 days
› Analyzing GW231109_235456 and understanding its potential implications for population studies, nuclear physics, and multi-messenger astronomy
› SWIFTGalaxy: a Python package to work with particle groups from SWIFT simulations
› Instability and vertical eccentricity variation in global hydrodynamic disk simulations
› SHELLQs-JWST: Revealing the Spectra of Extended Emission in 12 z > 6 Quasar Host Galaxies using the JWST NIRSpec Fixed Slit
› Multivariate Time Series Classification of Fermi - Detected Gamma-Ray Transients Using Convolutional-Recurrent Neural Networks
› Introducing the Seyfert-LINER Index (SLI): High Resolution (
› Probing AGN-ISM Feedback through Extended X-ray Emission in ESO 137-G034
› Magnesium Isotopic Detection in Cool Stars: Tracing Nucleosynthetic Signatures from MgH Features
› Multi-Modal Masked Autoencoders for Learning Image-Spectrum Associations for Galaxy Evolution and Cosmology
› Detecting ultralight dark matter in the Galactic Center with pulsars around Sgr A*
› Probing Axion-Photon conversion via circular polarization imprints in the CMB $V$-mode observations
› Beyond the Local Group - I: Cosmic Filaments Govern the Spatial Alignments of Galaxy Pairs
› Cosmic magnification on high-redshift submillimeter galaxies
› A new group of low-spin $50-70M_\odot$ Black Holes and the high pair-instability mass cutoff
› Discriminating Between Models of the Nanohertz Gravitational-Wave Background with Pulsar Timing Arrays
› Prospects for Observing the Microquasar SS 433 with the LACT Array
› Radio Follow-Up Observations of a Weak-Line Quasar Exhibiting Remarkable X-ray Variability
› FOXES: A Framework For Operational X-ray Emission Synthesis
› The Missing Mechanism: Picoflare Heating in the Solar Corona
› Stellar Wind-Blown Bubbles as Environments for Late-Time Rebrightening of Gamma-Ray Burst Afterglows
› The MDW H{\alpha} Sky Survey: Data Release 1
› HI Content of Group Galaxies from the FAST All Sky HI Survey
› Discovery and Timing Follow-Up of Two FAST-Discovered Pulsars from the FAST CRAFTS Survey
› Constraint on the physical origin of GRB prompt emission via its non-detected diffuse neutrino emission
› The cosmochemistry of planetary systems
› Morphological and Kinematical Diagnostic of FU Orionis-type Outburst Mechanisms
› Impact of Subsurface Temperature Gradients on Emission Spectra of Airless Exoplanets: the Solid-state Greenhouse and Anti-Greenhouse
› Revisiting the 150 MHz Radio Luminosity Function of Star-Forming Galaxies with LOFAR Deep Fields through a Refined Statistical Framework
› Coronal Mass Ejections Deflected by Newly Emerging Flux: A Combined Analytic and Numerical Study
› Detecting Intermediate-Mass Black Holes out to 20 Mpc with ELT/HARMONI: The Case of FCC 119
› A test of Amati relation using HII galaxy distances
› The Velocity Map Asymmetry of Ionized Gas in MaNGA II. Correlation between Velocity Map Morphology, Star Formation, and Metallicity in Regular Disk Galaxies
› SN2017ckj: A linearly declining Type IIb supernova with a relatively massive hydrogen envelope
› SN 2024iss: A Double-peaked Type IIb Supernova with Evidence of Circumstellar Interaction
› Spatially Resolved, Multiphase Mass Outflows of the Seyfert 1 Galaxy NGC 3227
› Exploring the accelerating black holes from the observations of quasi-periodic oscillations in X-ray binaries
› Testing the cosmic distance duality relation using model-independent approach
› A Statistical Study of delta-Sunspots from Solar Cycle 23 to 25
› Evaluating the chromospheric structure model of AD Leo using RH1.5D and magnetic field data
› A Search for Supermassive Black Hole Binary Candidates in 46-Year Radio Light Curves of 83 Blazars
› Constraining and Comparing the Dynamical Dark Energy and f(R) Modified Gravity Models with Cosmological Distance Measurements
› Revisiting Very High Energy Gamma-Ray Absorption in Cosmic Propagation under the Combined Effects of Axion-Like Particles and Lorentz Violation
› Luminosity Functions and Detectability of Binary Neutron Star Merger-nova Signals with Various Merger Remnants
› A volcanic chronosequence as a time-resolved paleo-detector array to study the cosmic-ray flux in the Late Pleistocene and Holocene
› The Detectability of Lunar-Origin Asteroids in the LSST Era
› The Sun as an X-ray star V.: A new method to retrieve coronal filling factors
› Recasting and Forecasting Dark Matter Limits Without Raw Data: A Generalized Algorithm for Gamma-Ray Telescopes
› Open-Source High-Fidelity Orbit Estimation for Planetary Science and Space Situational Awareness Using the Tudat Software
› Spinning-down RU Lup. Constraints on the physics of the outflow from high-resolution spectroscopy
› QUEST (Quasar Unsupervised Encoder and Synthesis Tool): A machine learning framework to generate quasar spectra
› Fundamental effective temperature measurements for eclipsing binary stars - VI. Improved methodology and application to the circumbinary planet host star BEBOP-3
› Development of the Reconstruction Procedure of the Fluorescence detector Array of Single-pixel Telescopes for measuring Ultra-High Energy Cosmic Rays
› Using Type-II Cepheids as Extragalactic Standard Candles: Distances to M31
› Automated Exploration of Radical-Molecule Chemistry: The Case of Oxirane + CH in the ISM
› Fine details in solar flare ribbons: Statistical insights from observations with the Swedish 1-m Solar Telescope
› The spatial distribution of dwarf and giant galaxies in and around Virgo cluster
› Energetics of star-planet magnetic interactions: Novel insights from 3D modelling
› The effects of stellar activity cycles on planetary atmospheric escape and the HeI 1083nm transit signature
› Can KM3-230213A be compatible with a cosmogenic origin?
› The AMBRE Project: Line-broadening and stellar rotation of ESO/FEROS archived spectra
› The role of supercluster filaments in shaping galaxy clusters
› The First Star-by-star $N$-body/Hydrodynamics Simulation of Our Galaxy Coupling with a Surrogate Model
› Alma Luminous Star catalogue IV: A Massive star census in the Magellanic Clouds
› The Programmable Liquid-crystal Active Coronagraphic Imager for the 4-m DAG telescope (PLACID) instrument: installation and commissioning update
› The Cosmic Baryon Cycle in IllustrisTNG: flows of mass, energy, and metals
› First detection of ultra-high energy emission from gamma-ray binary LS I +61 303
› The influence of a stably stratified layer on the hydromagnetic waves in the Earth's core and their electromagnetic torques
› From Rare Events to a Population: Discovering Overlooked Extragalactic Magnetar Giant Flare Candidates in Archival Fermi Gamma-ray Burst Monitor Data
› The MiMO Catalog: Physical Parameters and Stellar Mass Functions of 1,232 Open Clusters from Gaia DR3
› Validating Open Cluster Candidates with Photometric Bayesian Evidence
› The Near-Ultraviolet Spectra of FU Orionis Accretion Disks
› Solar flare forecasting with foundational transformer models across image, video, and time-series modalities
› MIGHTEE-HI: The HI mass-stellar mass relation of massive galaxies and the HI mass function at 0.25
› Improved UVIS Aperture Corrections derived from Focus Diverse PSF Maps
› A targeted radio survey of infrared-selected bow shock candidates
› Dynamical friction shear and rotation in Chaplygin cosmology
› Separation of gain fluctuations and continuum signals in total power spectrometers with application to COMAP
› Unveiling stellar (and planetary) internal dynamics with the fully compressible MUSIC code
› Galactic bars and active galactic nucleus fuelling in the second half of cosmic history
› Unveiling the collision between molecular outflows: observational evidence and hydrodynamic simulations
› Discovery of SN 2025wny: a Strongly Gravitationally Lensed Superluminous Supernova at z = 2.01
› The MandelZoom project II: the impact of stellar feedback on black hole accretion through an $\alpha$-disc in dwarf galaxies with a resolved interstellar medium
› Cosmic Vine: High abundance of massive galaxies and dark matter halos in a forming cluster at z=3.44
› Dark Energy Survey Year 6 Results: Clustering-redshifts and importance sampling of Self-Organised-Maps $n(z)$ realizations for $3\times2$pt samples
› Dark Energy Survey Year 6 Results: Redshift Calibration of the Weak Lensing Source Galaxies
› COMAP Pathfinder -- Season 2 results IV. A stack on eBOSS/DESI quasars
› Cosmic magnification on multi-catalogue Herschel submillimetre galaxies
› The Compressed 3D Lyman-Alpha Forest Bispectrum
› HST-COS Transit Spectroscopy of KELT-20b: First Detection of Excess Far-ultraviolet Absorption From an Ultra-hot Jupiter
› Learning and Interpreting Gravitational-Wave Features from CNNs with a Random Forest Approach
› Propellantless space exploration
› A Search for Ultra-Light Vector Dark Matter with a Rotating Torsion Balance
› Beyond Point Matching: Evaluating Multiscale Dubuc Distance for Time Series Similarity
› Electroweak Baryogenesis with \texttt{BARYONET}: a self-contained review of the WKB approach
› Superhorizon Isocurvature as a Window into Dark Matter Production
› Seafloor Topography Enhances KM3NeT Sensitivity to ANITA-like Events
› Bubble wall velocity with out-of-equilibrium corrections
› Zernike Mode Sorting with Vortex Phase Filters: Perfect Coronagraphs and Ideal Wavefront Sensors
› Inferring neutron-star Love-Q relations from gravitational waves in the hierarchical Bayesian framework
› The Ultra Slow-Roll Phase Of Warm Inflation In Braneworld Cosmology
› Symmetry principles of gravitational perturbations in thermal environments
› Thermodynamic Geodesics in Bardeen Regular Black Hole: Conventional vs. Modified Geometrothermodynamics Metrics
› Refined Low-Energy Supernova Constraints on Lepton Flavor Violating Axions
› Some Properties of Multi-Component Axion Dark Matter
› Primordial black hole formation from collapsing domain walls with full general relativity
› Exploring the Landscape of Spontaneous CP Violation in Supersymmetric Theories
› Tensor network methods for quantum-inspired image processing and classical optics
› Validation of field cage and cathode for low radioactivity operation with the CYGNO experiment
› Lensing, not luck! Detection prospects of strongly lensed gravitational waves
› Charge Trap Analysis in a SENSEI Skipper-CCD: Understanding Low-Energy Backgrounds in Rare-Event Searches
› Observable Signatures of Quarkyonic Phase in Neutron Stars
› Scheduling multiple agile Earth observation satellites with multiple observations
› Galactic Positrons from Thermonuclear Supernovae
› Evolutionary optimization of cosmological parameters using metropolis acceptance criterion
› Ultra-high-energy Cosmic Ray Sources can be Gamma-ray Dim
› GaiaUnlimited: The old stellar disc of the Milky Way as traced by the Red Clump
› Breaking boundaries: extending the orbit-averaged Fokker-Planck equation inside the loss cone
› A Quadratic Equation of State to Cosmic Acceleration: Entropy Evolution and Phantom Crossing
› galsbi: A Python package for the GalSBI galaxy population model
› The impact of the redshift-dependent selection effect of halos on the redshift-space power spectrum
› Structure and Dynamics of the Young Massive Star Cluster Westerlund 1
› Interpreting the HI 21-cm cosmology maps through Largest Cluster Statistics. Part II. Impact of the realistic foreground and instrumental noise on synthetic SKA1-Low observations
› Forecasts for interacting dark energy with time-dependent momentum exchange
› The Route to Unveil the Cosmic Genealogy of Supermassive Black Hole Binaries Using Nano-Hertz Gravitational Waves and Galaxy Surveys
› Magnetorotational instability in a solar near-surface mean-field dynamo
› Modeling the Light Curve and Spectra of SN 2023aew
› The mantle-inner core gravitational mode of oscillation in a strong magnetic field regime
› Radiation-magnetohydrodynamic Simulations of Accretion Flow Formation After a Tidal Disruption Event
› Tracing cosmic voids with fast simulations
› Hybrid Quark Stars with Quark-Quark Phase Transitions
› SAMPLE -- Stratospheric Altitude Microbiology Probe for Life Existence -- A Method of Collection of Stratospheric Samples Using Balloon-Borne Payload System
› Harnessing the potential of PyStoch: detecting continuous gravitational waves from interesting supernova remnant targets
› Radio signatures of AGN-wind-driven shocks in elliptical galaxies: From simulations to observations
› Radio Emission from a Nearby M dwarf Binary
› The 300 TeV photon from GRB 221009A: a Hint at Non-linear Lorentz Invariance Violation?
› Carpet-3 300 TeV Photon Event as an Evidence for Lorentz Violation
› DIPLODOCUS I: Framework for the evaluation of relativistic transport equations with continuous forcing and discrete particle interactions
› Fractality of open clusters in singles, pairs, and groups
› Search for Past Stellar Encounters and the Origin of 3I/ATLAS
› Fast X-ray Transient Detection with AXIS: application to Magnetar Giant Flares
› Assessing the feasibility range of Solar-powered Planetesimals Redirection operations for Terraforming
› Neural Enhancement of the Traditional Wang-Sheeley-Arge Solar Wind Relation
› Stellar halo subtraction alternative for accreting companions' characterization with integral field spectroscopy: Analytical and on-sky demonstration on the PDS70, HTLup, and YSES1 systems
› Dynamic or Systematic? Bayesian model selection between dark energy and supernova biases
› The GECKOS Survey: Resolved, multiphase observations of mass-loading and gas density in the galactic wind of NGC 4666
› von Karman - Howarth Similarity of Spatial Correlations and the Distribution of Correlation Lengths in Solar Photospheric Turbulence
› CHRONOS: Cryogenic sub-Hz cROss torsion bar detector with quantum NOn-demolition Speed meter
› MEGATRON: the impact of non-equilibrium effects and local radiation fields on the circumgalactic medium at cosmic noon
› A Giant Peanut-shaped Ultra-High-Energy Gamma-Ray Emitter Off the Galactic Plane
› JWST Observations of SN 2024ggi II: NIRSpec Spectroscopy and CO Modeling at 285 and 385 Days Past the Explosion
› Spatio-Temporal Evolution of the March 2022 ICME Revealed by Multi-Point Observations of Forbush Decreases
› DIPLODOCUS II: Implementation of transport equations and test cases relevant to micro-scale physics of jetted astrophysical sources
› Non-linear structure formation with elastic interactions in the dark sector
› A family of binaries with an extreme mass ratio
› Optimizing Kilonova Searches: A Case Study of the Type IIb SN 2025ulz in the Localization Volume of the Low-Significance Gravitational Wave Event S250818k
› Close-in faint companions mimicking interferometric hot exozodiacal dust observations
› Pre-perihelion Development of Interstellar Comet 3I/ATLAS
› Debiasing cosmological parameters from large-scale foreground contamination in Cosmic Microwave Background data
› Doubling the Number of Blue Large-Amplitude Pulsators: Final Results of Searches for BLAPs in the OGLE Inner Galactic Bulge Fields
› Covariant diagonalization of the perfect fluid stress-energy tensor
› Superradiant scattering of electromagnetic fields from ringing black holes
› Primordial Non-Gaussianity from Light Compact Scalars
› Phase transitions in the inner crust of neutron stars within the superfluid band theory: Competition between $^1\text{S}_0$ pairing and spin polarization under finite temperature and magnetic field
› Entanglement between pair-created twin universes with opposite time arrows should leave a birthmark on CMB spectrum
› Constraining the Coexistence of Freeze-in Dark Matter and Primordial Black Holes
› Can local White Dwarfs constrain Dark Matter interactions?
› On the Present Status of Inflationary Cosmology
› Avoidance of Big Crunch Singularity in the Q-SC-CDM model via nonminimal coupling: Theory and Data Analyses
› Smooth hybrid inflation in light of ACT DR6 data
› Muffled Murmurs: Environmental effects in the LISA stochastic signal from stellar-mass black hole binaries
› A comprehensive dynamical and phenomenological analysis of structure growth in curvature-modulated coupled quintessence scenario
› Imprints of screened dark energy on nonlocal quantum correlations
› GWKokab: An Implementation to Identify the Properties of Multiple Population of Gravitational Wave Sources
› Ghost-free, gauge invariant SVT generalizations of Horndeski theory
› Gravitomagnetic-Hydrodynamics and Turbulence in Early Universe
› Axion Perturbations: A General Analytical Treatment

  ↓↑    

Powrót do strony głównej Obserwatorium
Deklaracja dostępności cyfrowej
Biuletyn Informacji Publicznej UP
Copyright © 2002-2025 Katedra Astronomii Uniwersytetu Komisji Edukacji Narodowej w Krakowie. Wszelkie prawa zastrzeżone