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: widok na Babią Górę
widok na Babią Górę
S Webcam

Kamerka S

Webcam

Kamerka N

Allsky

Niebo

Temperatura
14.4 °C

Wilgotność
 86%

Wiatr
0.0 km/h

Ciśnienie
1009.1 hPa

Moon

Księżyc

 Wiadomości z astronet.pl

› Relacja ze Spaceshield Hack 2026 – kosmiczny hackathon prosto ze Stalowej Woli
› Astronomowie znaleźli najsilniejsze dowody na istnienie pól magnetycznych egzoplanet
› Kosmiczny przegląd miesiąca AstroNETu – maj 2026 roku
› Niebo w czerwcu 2026 roku
› Wybuch New Glenna podczas testu – Blue Origin apeluje o zbieranie szczątek
› Dalekie ekspozycje w astrokrajobrazie
› NASA przedstawiła szczegóły planów bazy księżycowej – w tym 3 nowe misje
› 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
RSS  Najnowsze prace na astro-ph:

› GREX-PLUS Science Book v2
› UK White Paper on Space-based total solar eclipse observations: structure and dynamics of the solar atmosphere
› The free-streaming length of dark matter from JWST observations of 28 strong gravitational lenses
› Little red dots as a cosmological probe: constraining $H_0$ with quasi-periodic pulsations
› Strong environmental AGN enhancement among DSFGs in z > 2 protoclusters
› Metal-Poor Gas Accretion Drives Giant Clump Formation at 0.6 < z < 2.6
› Toward decision-aware AI for LSST-scale time-domain astronomy
› Nonthermal Particle Acceleration by Magnetic Pumping in Pulsating Plasmas
› Eppur binaria non \'e esclusa: Gaia astrometry does not disfavor a binary origin for Long Secondary Periods
› TOI-3664 b, TOI-4034 b & TOI-6564 b: Three new hot Jupiters around stars approaching the terminal age main sequence
› Dynamical models of cluster members to probe the total mass properties of cluster subhalos. I. A comparison with parametric strong lensing models
› AGN Line-Intensity Mapping: A Probe of Faint Black Holes at Cosmic Noon
› Constraining the jet base emission of M87* with past and future Event Horizon Telescope observations
› A Decade to Map the Diffuse Universe: FRB-QSO Pairs with HST/COS Spectroscopy
› The WISSHFUL program: the highest redshift UFO discovered in a non-lensed QSO
› The Influence of Opacity on Inferred MHD Wave Signatures in the Lower Solar Atmosphere
› Hot Degenerate Components in Blue Stragglers: A Multi-Wavelength SED Analysis of Nine Open Clusters with Swift/UVOT
› How Common Are Common Envelopes? Quantifying Their Role in Forming Gravitational-Wave Sources
› Strong [OIII]$+$H$\beta$ emitters dominated the ionizing budget at $z\sim7$
› Constraining Orbital Eccentricity of a Supermassive Black Hole Binary Candidate PKS 2131-0211
› Sky-Plane Velocity Distributions of Interstellar Objects and Implications for Their Detection
› Bulk vs. turbulent motions at the centres of galaxy clusters: AGN-driven turbulence according to TNG-Cluster
› The DESI results impact the local determination of $H_0$
› Entropy-mode imprints in the solar corona: non-exponential damping and phase shifts of compressive oscillations
› A Critical UV Legacy: A Hubble Roadmap for HWO Science Readiness
› Building a Roadmap for Hubble science into the 2030s: Crucial UV spectroscopy of Oe stars in nearby galaxies
› Ultraviolet-Driven Atmospheric Degeneracies Challenge Conventional Biosignature Frameworks for Terrestrial Planets with Ultracool M Dwarf Hosts: An Archean-Analog TRAPPIST-1 e Case Study
› On the potential for inhomogeneities to mimic an evolving dark energy
› Complex Analysis of Askaryan Radiation: UHECR Reconstruction with Askaryan Radio Array
› A Kinematic Study of Wolf-Rayet Stars at the Galactic Center I: Binary Candidates and Constraints on the Binary Fraction
› The Double-lined Eclipsing $\gamma$ Doradus System AX Draconis in a 0.568-day Orbit
› Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations
› A linear residual structure across galaxy rotation curves
› Station-Keeping Approach for Extremely Low Lunar Orbits with Solar Sailing
› Dark asteroids exhibiting intermediate characteristics between C and X types
› Mapping Active Star-Formation in Serpens and the Aquila Rift
› Metastability in Emergent Dark Energy: A New Framework Confronting Cosmological Observations
› Joint Multi-Period Fermi-LAT and LHAASO Constraints on Axion-Like Particles from Mrk 421 Using Profile Likelihood with Gaussian Copula Correlation
› Evolution of the stellar mass function in open clusters from a universal and unsegregated initial state
› WISE Photometry of Galaxies within 10 Mpc
› Two Fabry-Perots and two calibration units for CARMENES
› Simulation of proton-induced activation for low-Earth orbit high energy astrophysics missions
› Galaxy morphology dependent (black hole mass)-(velocity dispersion) relations: implications for gravitational wave forecasts and cosmological simulations
› Fiber-coupling of Fourier Transform Spectrographs
› Observing the integrated and spatially resolved Sun with ultra-high spectral resolution
› The X-ray emission of the long-period transient and accreting cataclysmic variable ASKAP J174508.9-505149
› Reconstructing dark energy with fewer assumptions
› Early Results from GLASS-JWST. XXVI. Spatially Resolved Star Formation and Balmer Decrements at $1.1
› The Analysis of the Influence of Coordinate Error of Observation Station On the Construction Accuracy of Pulsar Time
› Near- to Far-Infrared Spectral Energy Distribution Analysis of Interacting Galaxies in Hickson Compact Groups 56 and Stephan's Quintet (HCG 92)
› Modeling Gamma-Ray Burst Spectra with Convolutional Neural Networks: Fast-Cooling Synchrotron Emission in a Decaying Magnetic Field
› Planet engulfment in the chemically anomalous HD 129171/HD 129209 pair
› Simulations of interaction between outflow and surrounding broken power-law circumnuclear medium: implications for different radio light curves of TDEs
› Narrow spectral artifact investigation and mitigation in LIGO data from the fourth LIGO-Virgo-KAGRA observing run
› The quenching time and timescale distribution of z~2 quiescent galaxies from precise colour distribution analysis
› The Multi-phase Biconical Outflow in the local IR-Luminous Merger IRASF01364-1042
› Morphological and mineralogical characterization of the Freundlich-Sharonov Basin: Implications for the lunar farside magmatism
› Interaction of Fast Magnetoacoustic Wave with the Localized Coronal Null and Generation of the Energetic Alfv\'en Wave Packet
› Grain-size evolution and rapid dust growth in high-redshift galaxies
› Detectability of secondary images from flares near Sgr A* with mock GRAVITY data
› Mass-Orbital Period Distribution of Massive White Dwarfs Formed Through Stable Mass Transfer
› AKRA 3.0: A matrix-free Inversion Framework for Weak Lensing Mass Mapping and Its Application to DES Y3 Data
› Probing a new subclass of llGRB-SN transients: Insights from EP250304a and its associated supernova
› A New Member of the Fast and Furious Family: A Relativistic and Time-Variable UV Outflow in a Luminous Quasar
› Peas and USPs: Can Stellar Spindown and Peas in a Pod Replicate Ultra-Short-Period Planet Characteristics?
› gr8stars II : judgement day for spectroscopic parameter model systematics
› Sensitivity Limits and Operational Threshold Calibration for DINOv2-based Gravitational-Wave Glitch Characterization: A Strain-Domain Mock Data Challenge on LIGO O4a
› Bar-induced deflection of open cluster tidal tails
› Research Note: Ghostly DLAs in SDSS DR16
› A micronova burst in the intermediate polar IGR J17014-4306
› Minor Ions as a Diagnostic of Solar Wind Heating: Inverted Mass-to-Charge Scaling in Imbalanced Turbulence
› A high-energy neutrino flare associated with nearby bright interacting supernova SN 2021foa
› The Atacama Cosmology Telescope: Probing new signatures of ultralight axions with gravitational lensing
› Depolarization and Polarization-Transfer Rates for Solar He I Lines due to Collisions with Neutral Hydrogen
› Dynamical evolution and dissolution timescale of young stellar clusters in the Orion star-forming complex
› Analytic insight into the physics of SASI II. Spiral instability of the prograde mode in a rotating stellar core
› Phenomenology of Inflaton-Driven Early QCD Confinement and Solution to Axion Isocurvature Problem
› What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2
› Heavy-element paleodetectors for Higgsino dark matter
› Gravitational Wave Imprints of a High-Quality Axion and the Origin of Flavor Hierarchies
› Behavior of kinetic instabilities in a dynamically forming resonant distribution
› Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy
› Black Bounce Solutions from a Self-Interacting 3-Form Field in General Relativity
› Hub-Aware Hybrid Search: Accelerating the Locally Aligned Ant Technique
› $\tt BlackHawk$ $\tt v3.0$: Hawking Radiation from Regular Black Holes
› Detecting Tidal Resonances in Binary Neutron Stars
› On the Possibility of a Strong First-Order Phase Transition in Neutron Stars
› Short Gravitational-Wave Transients as Probes of Cosmic Domain Walls
› Probing the Hubble Tension with an Infinite-Future Condition on the Hubble Parameter
› Reducing Model Error Using Optimised Galaxy Selection: Weak Lensing Cluster Mass Estimation
› Evidence that Planets in the Radius Gap Do Not Resemble Their Neighbors
› The three phases of self-gravitating scalar field ground states
› Prospects for optical detections from binary neutron star mergers with the next-generation multi-messenger observatories
› The DESI Y1 RR Lyrae catalog I: Empirical modeling of the cyclic variation of spectroscopic properties and a chemodynamical analysis of the outer halo
› The DESI Y1 RR Lyrae catalog II: The metallicity dependency of pulsational properties, the shape of the RR Lyrae instability strip, and metal rich RR Lyrae
› The VLA Frontier Fields Survey: A 6GHz High-resolution Radio Survey of Abell2744
› Pristine Massive Star Formation Caught at the Break of Cosmic Dawn
› A New Boundary Condition on Reionization
› MESAlab: A Python pipeline for MESA grid processing with integrated GYRE/MESA-RSP execution
› The Discovery of an Active Wind from the Milky Way's Black Hole
› Measurement of Substructure from the Kinematics of the GD-1 Stellar Stream
› The Synthetic Absorption Line Spectral Almanac (SALSA)
› A cosmographic analysis using DESI-DR2 and strong lensing: II. Distance Ratio measurements
› Measurement of angular cross-correlation between the cosmological dispersion measure and the thermal Sunyaev--Zeldovich effect
› JWST lensed quasar dark matter survey IV: Stringent warm dark matter constraints from the joint reconstruction of extended lensed arcs and quasar flux ratios
› A new Gaia census of OB associations within 1 kpc
› A New Torus Generator for AGAMA
› Actions of highly eccentric orbits
› Searching potential astronomical sites in Ethiopia
› CLiENT: A new tool for emulating cosmological likelihoods using deep neural networks
› Probing millisecond magnetar formation in binary neutron star mergers through X-ray follow-up of gravitational wave alerts
› TIC-65910228 b / NGTS-38 b, a 180 day transiting warm super-Jupiter
› Bounds on Lorentz invariance violation from muon fluctuations at the Pierre Auger Observatory
› Varstrometry for Off-nucleus and Dual Subkiloparsec AGN (VODKA): Three Quadruply Lensed Quasars at Cosmic Noon in HST and JWST
› Probing the Dispersion and Rotation Measure Contributions from Supernova Remnants in Fast Radio Burst Source Environments with 1D SNR Simulation
› The rotational and magnetic properties of Polaris from long-term spectropolarimetric monitoring
› SPHEREx mapping of diffuse PAH and H II emission in the Galactic plane
› Resolving Oblique Star-Disk Collisions in Quasi-Periodic Eruptions: Numerical Requirements and the Importance of Geometry
› Euclid preparation. CII. Non-Gaussianity of 2-pt statistics likelihood: Parameter inference with a non-Gaussian likelihood in Fourier and configuration space
› Deep Adaptive Optics Imaging Rules Out a Helium Star Companion to PSR J1928+1815
› The Evolution of Star-Forming Gas in STARFORGE: From Clouds, to Cores, to Stars
› Hyperaccreting Neutron Stars inside Massive Envelopes: The Implausibility of Thorne-\.Zytkow Objects
› Mean tropical year length at arbitrary ecliptic longitude
› The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover
› On the Nature of Candle-Flame-Shaped Solar Flares and Sub-Alfv\'enic Supra-Arcade Plasma Downflows
› A Systematic NLTE Study of Very Metal-Poor Stars with Metallicity Down to $-4.3$ dex. II. Lithium Abundance and New Insight to the Lithium Plateau
› Discovery of a Featureless Tidal Disruption Event at z~1 with the Wide Field Survey Telescope
› Constraining Early Dark Energy cosmological models with Big Bang Nucleosynthesis
› Long-term investigation of gamma Cas analogs
› New Supernova Constraints on Neutrinophilic Dark Sector - Vector Mediators
› Gamma-Rays and Gravitational Waves from Inelastic Higgs Portal Dark Matter
› Inference with finite time series II: the window strikes back
› Self-regularized entropy: What does black hole entropy predict for tests of Kerr no-hair theorem?
› Generalized Lema\^itre time for rotating and charged black holes and its near-horizon properties
› Comprehensive Ab Initio Quantum Computations of CO$_{\rm 2}$-H$_{\rm 2}$ and CO$_{\rm 2}$-He Collisional Properties
› A Unified Dark-Matter--Driven Relativistic Bondi Route to Black-Hole Growth from Stellar to Supermassive Scales
› Exceptional line and pseudospectrum in black hole spectroscopy
› On Cosmological Correlators at One Loop
› Primordial Black Hole Formation in $f(R)=R+\alpha R^2$ Gravity: Perturbative and Non-Perturbative Analysis
› Rotation-dependent $I$-Love-$Q$-$\delta M$ relations in perturbation theory
› Constant-roll $\beta$-exponential inflation: Palatini formalism
› Realization of quintom dark energy after DESI DR2 in Nieh-Yan modified teleparallel gravity
› Noise budget of Cryogenic sub-Hz cROss torsion bar detector with quantum NOn-demolition Speed meter (CHRONOS)
› Impact of the axion-like self-interactions in gravitational atoms for LISA
› Charging Across the Phantom Divide with Modified Gravity
› Radiation-induced electron spin polarization in ultrarelativistic kinetic turbulence

  ↓↑    

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