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: Zachód widziany z Obserwatorium
Zachód widziany z Obserwatorium
S Webcam

Kamerka S

Webcam

Kamerka N

Allsky

Niebo

Temperatura
0.5 °C

Wilgotność
 49%

Wiatr
0.0 km/h

Ciśnienie
1000.7 hPa

Moon

Księżyc

 Wiadomości z astronet.pl

› Kosmos w 2026 roku: czego wyczekiwać?
› Pixinsight cz.VI – Łączenie zdjęć monochromatycznych w kolorowy obraz
› Co marsjańskie trzęsienia ziemi mówią o jego historii
› Katalog Caldwella: C75
› Silne dowody na atmosferę na skalistej egzoplanecie
› Przełomowe odkrycie! Pierwsza planeta swobodna odkryta i ,,zważona” przez polskich naukowców
› Rozsiewanie nasion za pomocą satelity – projekt Greenstar
› Katalog Caldwella: C98
› Niebo w styczniu 2026 roku
› Podsumowanie roku 2025 w astronomii i astronautyce
RSS  Najnowsze prace na astro-ph:

› DeepInflation: an AI agent for research and model discovery of inflation
› The Ep-Liso correlation: A new diagnostic tool for kilonova transients
› Sample-efficient non-Gaussian noise reduction in gravitational wave data via learnable wavelets
› One Attempt at Building an Inclusive & Accessible Hybrid Astronomy Conference: FRB 2025
› Semi-analytical approach to Ly$\alpha$ multiple-scattering in 21-cm signal simulations
› The era of precision cosmology with voids
› Chemical evolution of close massive binaries -- tidally-enhanced or tidally-suppressed mixing?
› Most Hot Jupiters Were Cool Giant Planets for More Than 1 Gyr
› The Little Red Dots Are Direct Collapse Black Holes
› Mach $>3$ shocks at the tips of both eROSITA bubbles
› Hunting the first Cosmic Giants: formation and detectability of Direct Collapse Black Holes around high-redshift quasars
› Decameter-sized Earth Impactors -- II: A Bayesian Inference Approach to Meteoroid Ablation Modeling
› The Distance to NGC 4258 from Individual Maser Component Tracking
› Fast X-ray transients in NuSTAR data
› Cosmo-FOLD: Fast generation and upscaling of field-level cosmological maps with overlap latent diffusion
› A Not-So-Compact Companion: Massive, Oversize White Dwarf in a Post-Common Envelope Eclipsing Binary
› The Self-Limiting Nature of Jet-Modulated Thermal Conduction in Cool Core Clusters
› Mirror images of lensed star clusters with mismatched spectral energy distributions: A possible signature of top-heavy stellar initial mass functions and extreme stars in high-redshift star clusters
› Neutron star cooling implications and magnetic field of the Vela Junior central compact object from all XMM-Newton and Chandra spectra
› Cold gas formation triggered by active galactic nuclei jet feedback in galaxy cluster cores
› An azimuthally resolved study of sloshing cold fronts in three nearby galaxy clusters
› MeV absorption in gamma-ray bursts as a probe of their progenitor winds
› Growth of Light Seed Black Holes in the Early Universe
› Ultraviolet spectroscopy reveals a hot and luminous companion to the Be star + black hole candidate MWC 656
› Erythrohenosis -- The crimson chronicles of two giants
› Stirring Things Up: Bar-induced substructures in the stellar halo of a cosmological Milky Way analogue
› The Role of Inner Halo Angular Momentum (Spin) in Shaping Dark Matter Bars in Milky Way Analogs
› The Carousel Lens I: A Spectroscopic Survey of the Carousel Lens Field
› Deep Chandra Observations of the z = 1.16 Relaxed, Cool-core Galaxy Cluster SPT-CL J2215-3537
› Inferring Meteoroid Properties with Dynamic Nested Sampling: A Case Study of Orionid and Capricornid Shower Meteors
› PyISH: Python Integral Field Spectroscopy Simulation for HWO
› Astrometric Radial Velocities from the Hipparcos-Gaia Catalog of Accelerations and Implications for Astrometric Acceleration Measurements
› Prospects of Prompt Gamma-Ray Burst Polarimetry with POLAR-2
› Supermassive black hole mass inference with the optical flares of tidal disruption events
› Dark Energy Survey Year 6 Results: MagLim++ Lens Sample Selection and Measurements of Galaxy Clustering
› The failed failed-supernova scenario of M31-2014-DS1
› Searching for Isolated Black Hole Candidates within 15 pc of the Solar System in Gaia DR3
› Extra modes in helium-core-burning stars probing an infra core cavity
› Control algorithms for dual-wavefront sensor single-conjugate adaptive optics
› Spectral Variability of the Star HD 141569A
› Exotic optical variability in the black hole X-ray binary IGR J17091-3624
› New techniques to investigate the AGN-SF connection with integral field spectroscopy
› IRMaGiC: Extending Luminous Red Galaxy Selection into the infrared with joint LSST and Roman HLIS Data
› Dark Energy Survey Year 6 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing
› Signatures of a Tidally Induced Spiral Arm at the Anticenter of the Milky Way and a Kinematically Extended Anticenter Stream Using DESI DR2
› The Effects of Radially Varying Diffusivities on Stellar Convection Zone Dynamics
› A JWST Paschen-alpha Calibration of the Radio Luminosity-Star Formation Rate Relation at z~1.3
› SETI Observations of k-Hz Periodic Radio Signals from Five Nearby Stars with FAST at L Band
› A New Framework for Multi-Line Analysis Combined Kernel PCA and Kernel SHAP: A Case of NGC 1068 ALMA Band 3 Data
› Constraints on Axion-Like Particles from Ultra-High-Energy Observations of 3HWC J1908+063 with HAWC
› Decomposing the growth mechanisms of galaxies over the last 10 billion years
› CSST Strong Lensing Preparation: Cosmological constraints from double-source-plane strong lensing systems in era of CSST
› Detailed lens modeling and kinematics of the submillimeter galaxy G09v1.97. An analysis of CO, H2O, H2O+, and dust continuum emission
› Closed-Form Statistical Relations Between Projected Separation, Semimajor Axis, Companion Mass, and Host Acceleration
› Cosmological Constraints on f(T,B) Gravity from Observations of Early and Late Universe
› The puzzle of composition of cosmic rays with energies (2-12.5) EeV according to muon detectors data of the Yakutsk EAS array
› Evidence of mutually exclusive outflow forms from a black hole X-ray binary
› Polarization properties of changing-look active galactic nuclei: NGC 1365 and NGC 2992
› The Intermediate-Mass Black Hole Reverberation Mapping Project: Stable Optical Continuum Lags of an IMBH in the Dwarf Galaxy NGC 4395 Over Years
› The Supernova Remnant G284.3$-$1.8 and Its Relation to the Gamma-ray Binary 1FGL J1018.6$-$5856
› SN 2023zcu: A Type IIP SN with Early Flash Features
› Dark Energy Survey Year 6 Results: Magnification modeling and its impact on galaxy clustering and galaxy-galaxy lensing cosmology
› Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework
› Modeling X-ray reflection spectra from returning radiation: application to 4U 1630$-$47
› The First Upper Bound on the Nano-Hertz Gravitational Waves and Galaxy Cross-Correlation signal using 15-year NANOGrav Data and DESI Galaxy Survey
› Dark Energy Survey: DESI-Independent Angular BAO Measurement
› ExoMiner++ 2.0: Vetting TESS Full-Frame Image Transit Signals
› Small scale turbulence alongside with large scale turbulence in a z~sim 2 star Forming Galaxy with outflowing wind, revealed by Multi-point structure functions
› The eJWST active galactic nucleus observation catalogue
› MIGHTEE: The evolving radio luminosity functions of star-forming galaxies to $z\sim 4.5$ and the cosmic history of star formation
› Towards gravitational wave parameter inference for binaries with an eccentric companion
› Modelling the Time-variable Broadband Emission and Correlation Study of FSRQ S5 1044+71
› AGN in Gaia Alerts: from flares to Changing Look Quasars
› Numerical study of multiple solar flare induced modulation of Very Low Frequency (VLF) diurnal profile
› Kinematics of the HII region NGC 7538 from study of the Ha line
› MSA-3D: Connecting the Chemical and Kinematic Structures of Galaxies at $z \sim 1$
› How a Close-in Planet Protects its White Dwarf Host from Pollution
› A study of the high-inclination population in the Kuiper belt -- V. Mean motion resonances beyond 50 AU
› Three-dimensional GRMHD simulations of jet formation and propagation in self-gravitating collapsing stars
› CO Diffusion on Interstellar Amorphous Solid Water: A Computational Study
› Comment on "Application of the three-dimensional telegraph equation to cosmic-ray transport" (arXiv:1606.08272)
› Properties and Possible Physical Origins of $\gamma$-ray Emission in Extreme Synchrotron Blazars
› A Theory of transmission spectroscopy of planetary winds: Spectral-line saturation and limits on mass-loss inference
› Dark Energy Survey Year 6 Results: Galaxy-galaxy lensing
› A nomenclature for individual exocomets
› Probing Heavily Obscured AGN in Major Galaxy Mergers Using the mm-X-ray Correlation
› The early r-process nucleosynthesis scenarios
› Implications of the continuous radio-loudness distribution among AGNs in the local Universe
› Alkali recondensation into chondrules
› Revealing massive black hole astrophysics: The potential of hierarchical inference with extreme mass-ratio inspiral observations
› Magneto-Archeology of White Dwarfs. Revisiting the fossil field scenario with observational constraints during the red giant branch
› The importance of super-Eddington black hole accretion for the emergence of massive quiescent galaxies at high redshift
› Transit distances and composition of low-velocity exocomets in the $\beta$ Pic system
› Cosmic strings, domain walls and environment-dependent clustering
› The Circumbinary Disk of HD 34700A: I. CO gas kinematics indicate spirals, infall, and vortex motions
› The baryonic mass-size relation of galaxies. II. Implications for the evolutionary paths between star-forming and passive galaxies
› A radially broad collisional cascade in the debris disk of $\gamma$ Ophiuchi observed by JWST
› Tracing the Galactic Disk with Gaia DR3: A Deep Study of Berkeley 17, 18, and 39 Open Star Clusters
› A spectroscopically confirmed, strongly lensed, metal-poor Type II supernova at z = 5.13
› RV$\times$TESS I: Modeling Asteroseismic Signals with Simultaneous Photometry and RVs
› CO$_2$ collision-induced line parameters for the $\nu_3$ band of $^{12}$CH$_4$ measured using a hard-collision speed-dependent line shape and the relaxation matrix formalism
› Scalar Quasi-Normal Modes in Black Hole Gravitational Lensing
› Emergent Large Lepton Mixing from Neutrino Refraction in Dark Matter
› Neutrino production mechanisms in strongly magnetized quark matter: Current status and open questions
› Higher Harmonics of Double White Dwarfs in the Centihertz Band: Linking LISA and DECIGO
› The role of angular momentum in general relativity: heuristic and covariant interpretations
› A SiPM-Based RICH Detector with Timing Capabilities for Isotope Identification
› Testing the three massive neutrino paradigm: Constraints on Neutrino Properties and Interactions from Recent Experimental Data
› The relativistic restricted three-body problem: geometry and motion around tidally perturbed black holes
› Combined constraints on dark photons from high-energy collisions, cosmology, and astrophysics
› Efficient prior sensitivity analysis for Bayesian model comparison
› Chemical evolution of antimatter domains in early Universe
› Exact general solutions for cosmological scalar field evolution in a vacuum-energy dominated expansion
› A magnetic avalanche as the central engine powering a solar flare
› GRMHD simulations of black hole accretion variabilities: Implications to hard state X-ray binary transients
› Comparative biosignatures with systemic retrievals
› Exploring selection biases in FRB dispersion-galaxy cross-correlations with magnetohydrodynamical simulations
› Repeating flares, X-ray outbursts and delayed infrared emission: A comprehensive compilation of optical tidal disruption events
› A binary-related origin mediated by environmental conditions for blue straggler stars
› CHEX-MATE: New detections and properties of the radio diffuse emission in massive clusters with MeerKAT
› Coupled Time-Dependent Proton Acceleration and Leptonic-Hadronic Radiation in Turbulent Supermassive Black Hole Coronae
› Silane-Methane Competition in Sub-Neptune Atmospheres as a Diagnostic of Metallicity and Magma Oceans
› Dynamical tide modified Roche limit in eccentric, asynchronous binaries
› Radio Emission from Broad Absorption Line Quasars
› Generation of Lognormal Synthetic Lyman-$\alpha$ Forest Spectra for $P_{1D}$ Analysis
› Observation of an Accreting Planetary-Mass Companion with Signs of Disk-Disk Interaction in Orion
› Black-hole mass estimation through accretion disk spectral fitting for high-redshift blazars
› Islands of Electromagnetic Tranquility in Our Galactic core and Little Red Dots that Shelter Molecules and Prebiotic Chemistry
› A Practical Framework for Estimating the Repetition Likelihood of Fast Radio Bursts from Spectral Morphology
› Intermediate-Mass Stripped Stars in the Magellanic Clouds: Forward Modeling the Observed Population Discovered Via UV Excess
› Physical properties of long-rising type II Supernovae -- Bayesian Analytic Modeling and Spectrophotometric Correlations
› Potential Thermal Profiles of The Third Interstellar Object 3I/ATLAS
› Estimating accretion times of halo substructures in the Milky Way
› Radiation magnetohydrodynamics simulations of Population III star formation during the Epoch of Reionization
› Made-to-Measure Outperforms Schwarzschild's Method
› The FAST-SETI Milky Way Globular Cluster Survey I: A Pilot Multibeam On-the-Fly Search of Five Globular Clusters at L-Band
› Enhanced detection limits in the SHINE F150 survey through the Regime Switching Model. Optimizing thresholds and investigating environmental noise
› Multi-bandpass Photometry for Exoplanet Atmosphere Reconnaissance (MPEAR) with the Habitable Worlds Observatory (HWO) -- I. Differentiating Earth from Neptunes During Discovery
› Magnetic field generation in mergers of massive main sequence stars
› Understanding the chemistry of temperate exoplanets atmospheres through experimental and numerical simulations
› Diffusive or Ballistic? Distributions and Spectra of PeV Cosmic Rays around Microquasars
› Measurement of the extragalactic background light at 8600\r{A} using dark cloud shadow and the CaII-triplet lines
› The effects of star-gas interactions on binary evolution in open clusters
› Disc Winds From Accreting Systems in the 2040s
› Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter
› Catching 3I/ATLAS Using a Solar Oberth
› Origins of the UV continuum and Balmer emission lines in Little Red Dots: observational validation of dense gas envelope models enshrouding the AGN
› Cluster number counts in dark energy model with energy and momentum coupling to dark matter
› Habitable Worlds Observatory's Concept and Technology Maturation: Initial Feasibility and Trade Space Exploration
› Updated Metallicity Diagnostics for Precision Oxygen Abundance Measurements in High-$z$ Galaxies with JWST
› Observational Signatures of Planetary Tidal Disruption Events Around Solar-Mass Stars
› Possible time-variable iron-K$\alpha$ emission in the circumnuclear region of the Circinus galaxy
› A multi-wavelength study of the 2025 low state of the intermediate polar BG CMi
› Scalar and vector dark matter admixed neutron stars with linear and quadratic couplings
› Task-parallelism in SWIFT for heterogeneous compute architectures
› Studying Ionospheric Phase Structure Functions Using Wide-Band uGMRT (Band-4) Interferometric Data
› Speed of sound peak in isospin QCD: a natural prediction of the Medium Separation Scheme
› $\textit{Ab initio}$ Exact Calculation of Strongly-Correlated Nucleonic Matter
› Suppression of scalar perturbations due to a heavy axion
› Evolution of an Alfv\'en Wave-Driven Proton Beam in the Expanding Solar Wind
› Constraints on gravitational waves from the 2024 Vela pulsar glitch

  ↓↑    

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