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
11.9 °C

Wilgotność
 65%

Wiatr
0.0 km/h

Ciśnienie
1017.9 hPa

Moon

Księżyc

 Wiadomości z astronet.pl

› 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?
› Fotografujemy zorzę polarną…
RSS  Najnowsze prace na astro-ph:

› Mosaic: Area-Closed Spherical Surface Mosaics Induced by Cartesian Grids
› Polarization Birefringence and Waveform Systematics in GW231123
› Expected redshift drift for tilted observers
› The limits of feedback from active galactic nuclei
› Halo-driven Origin and Suppression of Over-massive Black Holes and Little Red Dots
› The pair-instability origin of supernova 2023vbw
› Thermostats, Not Engines: A New Picture of Halo Gas Regulation
› The interaction phase of engine-driven explosions and high-energy winds
› Spinning out of focus: The challenge of rotational line broadening in exoplanet reflection spectroscopy
› Hot DQs, magnetic and metal-polluted white dwarfs: spectroscopic insights from a Gaia machine-learning-selected 500 pc sample
› A 14-year-old Mystery: The Peculiar Case of the Engine-driven SN 2012ap
› Stellar encounters in the solar neighbourhood and the special case of GJ~710
› Searching for the Third Wheel: High-Contrast Imaging Constraints on Tertiaries to Black Hole and Neutron Star Binaries
› A Revised Mass and Period for the Habitable Zone super-Earth GJ 3378b: A Planet Straddling the Cosmic Shoreline
› Co-evolution of Supermassive Black Holes and their Host L* galaxies: implications for Milky Way and M31
› Neutrino Flavor Conversion Shapes the Rate of Failed Core-collapse Supernovae
› Feedback driven interactions between dark and luminous matter to explain tight galaxy scaling relations
› Is the Binary Black Hole Population Inference from Gravitational-Wave Data Robust?
› Modeling the probability distribution for cosmological analysis with photometrically classified samples
› SN 2023fyq: direct detection of a Type Ibn supernova progenitor and its multi-wavelength environmental constraints
› Probing the Mass-loss Histories of Type IIn and II-L Supernovae with Late-time Radio Observations
› The EDGES Analysis Pipeline: Description and Validation
› The bound origin of low-mass stellar binaries
› The Torques Acting on Accreting Millisecond X-Ray Pulsars in the Outburst and Quiescent States, and During the Long-Term Evolution
› The First Remotely Detected Biosignature May Not Be the Most Common: Implications for JWST and HWO
› Multiwavelength Probes of Cosmic Ray Transport in Molecular Cloud Structures
› A Rare Population of Intermediate-mass Helium Stars Between Hot Subdwarfs and Wolf-Rayet Stars
› Extracting redshifts from 2D slitless spectroscopic images using deep learning for the CSST galaxy survey
› XRISM detection of the 6.4 keV Fe K$\alpha$ line in the radio galaxy Cygnus A
› Simulation study of the cosmic ray Sun shadow with a time-dependent solar magnetic field model
› SN 2023dbc in M108: Optical and Near-Infrared Observations of a Highly-Obscured, Moderately Energetic Stripped-Envelope Supernova
› The Rapid ASKAP Continuum Survey VII: Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) Second Data Release -- Unveiling the Magnetised Sky
› Magnetised CGM Gas at z~1 revealed by SPICE-RACS
› Circular polarization of the cosmic microwave background induced by the optical Magnus effect on gravitational lensing
› Determination of the best dark matter profile for the Milky Way with Gaia DR3 using Bayesian Model Comparison
› Red novae, their progenitors, and remnants
› The ${}^{13}\mathrm{CO}(2{-}1)/^{12}\mathrm{CO}(2{-}1)$ Line Ratio from 100 Molecular Clouds in the Large Magellanic Cloud
› PEARLS: JWST Counterparts of Micro-Jy Radio Sources in the NEP Time Domain Field. II. All Four Spokes
› Nonlinear electrodynamics in magnetars: systematic effects on radius constraints and timing analysis
› Systematic KMTNet Planetary Anomaly Search. XIII. Complete Sample of 2021 Prime Field Planets
› Jet-Structure Imprint on the Curvature Tail of Gamma-Ray Burst Prompt Emission
› A Framework for Applying the Loeb-Turner $\alpha$-Slope Test to Archival Photometry of Trans-Neptunian Objects
› On the Nature of Candle-Flame-Shaped Solar Flares and Sub-Alfv\'enic Supra-Arcade Plasma Downflows
› Constraints on Self-Interacting Fuzzy Dark Matter from the Stellar Kinematics of the Dwarf Galaxy Leo II
› Identifying observable MeV lines from the decays of weak and main $r$-process isotopes in mergers
› HI Observations of Baryon-Dominated Dwarf Galaxy Candidates
› A growth of early superhump: Multi color observation of the WZ Sge star TCP J23580961+5502508
› Radio Emission from Fast Blue Optical Transients Powered by Trans-relativistic Shocks in Confined Circumstellar Material
› Understanding corona and disk evolution in black hole X-ray binaries through a comprehensive study of their broadband variability and QPO characteristics
› The Deep Learning-Based Dual-Branch Multimodal Fusion Model for Solar Flare Prediction
› From inter-filamentary gas to filaments and hubs: gas flows in the Mon R2 hub-filament system
› Precise and Rapid Parameter Inference of Kilonova with Conditional Variational Autoencoder
› Exploring the Transitional Parameter Space of Blazars using Gamma-ray and X-ray Population Diagnostics
› Bidirectional Plasma Jets Driven by Magnetic Reconnection: Observations by GST and SDO
› Stellar Density Classification and Regression for CSST Multi-color Imaging Using Deep Learning
› Accretion geometry and spectral evolution in 1A 1118-61: a comparison of the 2009 and 2026 outbursts
› GRMHD Simulations of Magnetized Accretion Disk/Jet: Variabilities of Black Holes and Spectral Energy Distributions in Magnetic States
› Accelerating Redshift-Conditioned Galaxy Image Synthesis with One-step Generative Modeling
› Population synthesis of active galactic nuclei based on the radiation-regulated unification model
› Charged-current neutrino opacity within the relativistic Hartree-Fock framework for astrophysical simulations of core-collapse supernovae and binary neutron star mergers
› Diffuse gamma-ray emission in the vicinity of open cluster Berkeley 87
› Four-Body Gravitational Microlensing Events Involving Both a Binary Lens and a Binary Source
› 'Unacceptable to our people': Diverse cultural beliefs, Indigenous rights, and the future of human activities on the Moon
› BISTRO Survey: Gravity-Dominated and Magnetically Regulated Star Formation in M17 SW
› Classification of IGR J20084+3221 as an Intermediate Polar using X-ray and Optical Observations
› Coupled quintessence with a potential from supergravity exhibits sign-changing interaction
› The First Insights into an Ultraluminous X-ray Pulsar with XRISM: Phase-Resolved High-Resolution Spectroscopy of the Fe K-shell Band of M82 X-2
› A Hycean Interpretation of K2-18b Supported by Photochemical Atmospheric Compositional
› Assessing the Impact of Source Confusion for GREX-PLUS based on Deep JWST NIRCam Imaging
› Impact of Satellite Constellations on Observations with the 80-cm Telescope and the Mini-SiTian at the Xinglong Observatory, NAOC
› Higher-order statistics of the stochastic gravitational wave background from supermassive black hole binaries
› Nuclear Activity and Host Galaxy Properties of Low-Luminosity AGN Identified from VLA Observations
› Search for the Highest-energy Quasiperiodic Oscillation in the Black Hole X-Ray Binary Candidate Swift J1727.8-1613
› Chemistry and IR emission of acetylene in planet-forming regions of T Tauri disks. Impact of elemental abundances and dust properties
› Spectral energy-loss bump and $\gamma$-ray pulsar halos
› Anisotropic Ejecta from Binary Neutron Star Mergers: Self-Consistent Main Thermal and Late-Time Radio Emission of NS-Powered Kilonovae
› Inferring stellar metallicity and elemental abundances from kinematic and spectroscopic data using machine learning -- Implications for exoplanet host stars
› Testing the reliability of magnetic field strength measurements for M dwarfs
› SDSS-V: Revealing a weak accretion state in X-ray selected red quasars
› Gravitational lensing time delay beyond the Shapiro/geometry split
› Photometric classification of quasars from DES and photo-$z$ estimation with Machine Learning
› Wolf-Rayet stellar evolution models with improved treatment of the atmosphere
› Quadratic Dark Energy Phase-Space Dynamics and Analysis
› Sub-stellar Strange Quark Matter Objects: Predicting a New Class of Highly-Compact Candidates
› FastChem 4: New chemical elements and improved convergence behaviour
› Two kinds of Galactic source populations could explain the cosmic-ray observation up to the "knee" region
› Polarization Observations of a Sample of 6.7 GHz Methanol Masers
› Sungrazer comets as analogs of star-planet magnetic interactions
› Constraining the magnetic field strength of a flaring radio core in the compact steep spectrum source 3C 138
› Primary gravitational waves at high frequencies II: Emergence of the exponential cut-off in the power spectrum
› Discovery of variable polarization in H$\alpha$ profile of symbiotic star Y Gem: A case for orbital-phase dependent variation of Raman-scattered Ly$\beta$ emission
› Probing Reionization up to the Mark: The Marked Power Spectrum to unveil the HI 21-cm signal from the EoR
› A Three-Dimensional Exploration of Magnetic Fields, Rotation, and Shock Revival in a $39 M_\odot$ Core-Collapse Supernova Progenitor
› A fast tree algorithm for multi-component coagulation equation
› 7DT Insight: Variability in Young Stellar Objects
› Iron line diagnostics of the stellar wind in X1908+075
› Velocity-resolved [O I] 63,145 um, [C II] 158 um, and OH line mapping along the Orion BN/KL explosive outflow and irradiated shocks
› (An)Isotropy in Pantheon+ and Type Ia supernova samples: intrinsic limits of directional tests
› Datacubes of H$\alpha$, CaII K, CaII H and H$\epsilon$ line profiles of the full solar disk recorded daily at Meudon observatory since 2017 and some typical profiles of solar features
› A 4200-hour HyperFlash and \'ECLAT campaign on the hyperactive FRB 20240114A: constraining energetics with the most brilliant bursts
› Towards the Deployment of the First NectarCAM, a Medium-Sized-Telescope Camera for the Cherenkov Telescope Array Observatory
› Primordial power spectrum reconstructions from BOSS + eBOSS
› Faster CMB lensing with control variates
› CCD () photometry of the open cluster NGC 6793 and its dynamical evolution
› The Wide Field Imager (WFI) Instruments for the Polarimeter to Unify the Corona and Helliosphere (PUNCH)
› Recoupled Dark Radiation reconciling CMB and DESI BAO measurements
› WaveDriver: a Laser Guide Star AO System for HWO
› Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2-604207
› A universal framework to identify eccentric binary mergers: GW200105 case study
› Modifications of CMB Temperature and Polarization Quadrupole Signals in Thurston Spacetimes
› Wide parameter-space O3 search for continuous gravitational waves from unknown neutron stars in binary systems
› Particle Dynamics, Shadow and Hawking Sparsity of a Kalb-Ramond Black Hole Coupled to Nonlinear Electrodynamics
› Freeze-in Warm Dark Matter via Dimension-6 Operators in 3-3-1 Models
› StAD: Stein Amortized Divergence for Fast Likelihoods with Diffusion and Flow
› Rapidly Rotating Neutron Star Collapse in Massive Scalar-Tensor Theories
› Bidirectional Internal Squeezing for Gravitational-Wave Detectors
› Constraints on non-canonical chaotic inflation from ACT DR6 and BICEP/Keck data
› Gauge-invariant cosmological perturbations in Type 3 New General Relativity and background-hierarchy bounds
› Warm inflation in Weyl geometric gravity
› Direct On-Wafer Measurements of Noise Parameters in C- and X-bands at $T=4$ K
› A reversed solar illumination dependence of unintended emission from Starlink Direct-to-Cell satellites at 72-234 MHz with the EDA2
› An EFT Map of Axion Dark Radiation from Reheating
› Impact of the axion-like self-interactions in gravitational atoms for LISA
› Positive Running of the Spectral Index for Scalar Theory and Modified Gravity
› Pole Skipping, Avoided Crossing, and Resonant Excitation in Kerr Quasinormal Modes near Algebraically Special Frequencies
› Proton-to-Alpha Branching Ratio in the $^{12}$C+$^{12}$C fusion reaction at Astrophysical Energies
› The impact of seasonality over the sensitivity of Einstein Telescope and the SNR of CBC signals at the Sardinia candidate site
› Cosmological perturbations of TDiff fields
› Probing (sub-)solar-mass black holes and superspinars with current and next-generation gravitational-wave observatories
› Astrophysics equation of state inference with Bayesian chiral effective field theory uncertainties
› Self-Supervised Conformal Prediction with Equivariant Bootstrapping for Image Uncertainty Quantification
› Traditional statistical representations outperform generative AI in identifying expert peer reviewers
› Modelling DSA, FAST and CRAFT surveys in a z-DM analysis and constraining a minimum FRB energy
› Globular cluster distributions as a dynamical probe of dark matter
› Constraints on primordial non-Gaussianity from Quaia
› Method for testing diffusive shock acceleration and diffusion propagation of 1-100 TeV cosmic electrons with multiwavelength observations of the Geminga halo and pulsar wind nebula
› SPT-3G D1: Axion Early Dark Energy with CMB experiments and DESI
› Characterizing the host galaxies and delay times of Ca-rich gap transients vs 91bg-like SNe and normal Type Ia SNe
› Extracting latent representations from X-ray spectra. Classification, regression, and accretion signatures of Chandra sources
› Multi-species Dark Matter with Warmth and Randomness
› FLAMINGO: Tracing the co-evolution of hot gas and black holes in galaxy groups and clusters
› A Census of Double-Peaked Lyman-alpha Emitters in MAGPI: Classification, Global Characteristics, and Spatially Resolved Properties
› Radiatively Cooled Binary Mass Transfer: Flow Structure, Luminosities, and L2 Outflows Across Mass Transfer Rates
› Observing Orbital Decay in the Ultracompact Hot Subdwarf Binary System ZTFJ213056.71+442046.5
› SE3D: Testing the recovery of stellar population, dust and structural properties on mock-observed toy model and simulated galaxies
› SE3D: Building a radiative transfer emulator to fit panchromatic resolved galaxy observations with 3D models of dust and stars
› Non-Gaussianity in SMICA
› The Shear-to-Cosmology Paradigm I. Hybrid Field-Level and Simulation-Based Framework for Weak Lensing Surveys
› Stellar feedback drives the baryon deficiency in low-mass galaxies
› Measurements of quasar proximity zones with the Ly$\alpha$ forest of DESI Y1 quasars
› The GRB Intrinsic Duration Distribution: Progenitor Insights Across Cosmic Time
› The Contribution of Stars, Dust, Neutral Gas and SMBHs in Galaxies to the Cosmic Baryon Inventory
› proto-Lightspeed: a high-speed, ultra-low read noise imager on the Magellan Clay Telescope
› The Nulling Interferometry Cryogenic Experiment (NICE): Architecture, requirements, and preliminary warm precursor results
› Polarization Signatures of Inspiraling Hotspots around Kerr Black Holes
› Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework
› Is the overconcentration of pristine populations in Galactic globular clusters real? An N-body approach to the problem
› Pure Natural Inflation Passes the ACT
› Kinematics of Wolf-Rayet Stars in the LMC: Clues to Subtype Origins
› The SMUGGLE-Ring project: Bar and bulge effects on nuclear disk and ring formation
› Variable ADAF disk as the origin of Changing-Look AGN
› Solar Extreme Ultraviolet Spectrograph and High-energy Imager (SEUSHI): Design, Development, and Pre-Flight Calibration
› Hot blue progenitors of stellar-mass black holes
› Stellar Coronal Mass Ejections with HWO: A Science Case Concept
› JWST Exoplanetary Worlds and Elemental Survey (JEWELS) II: Condensation Temperature Trends and Galactic Chemical Evolution in JWST Planet-Hosting Stars
› Status of the COSmological Microwave Observations CALibrator
› Ellipsoidal modulation and multi-wavelength activity in the pre-cataclysmic binary RX J1553.0+4457
› Chromosphere of the quiet sun: II. Atmospheric response to small-scale magnetic flux emergence
› Multiwavelength Analysis of PSR J0437-4715 with Pulse Profile Modeling
› Gravitational Lensing of Gravitational Waves from Astrophysical Sources: Theory, Detection, and Applications
› Exploring Enceladus's Interior Structure Using Electromagnetic Induction
› On the residual missing mass of the Bullet Cluster
› Unveiling $f(R)$ Gravity with Void-Galaxy Cross-Correlation Multipoles
› Photometric determination of the mass accretion rates of pre-main sequence stars. IX. Recent star formation in the periphery of NGC 346
› Gravitational-wave Tomography of the Moon: Constraining Lunar Structure with Calibrated Gravitational Waves
› Dynamical Evolution of V-Shaped Collision Debris
› Improving Slow-Roll Estimates in Starobinsky Inflation Using Analytic Hubble Parameter
› Testing the consistency of gravitational waves and large scale structure constraints on dark energy
› False Vacuum Decay across the Quantum-to-Thermal Crossover: A Comparison of Real-Time Observables
› U-spin symmetry energy and hyperon puzzle
› Low-frequency radio telescopes sensitivity to light dark matter
› The effects of dark energy on the matter-gravity coupling
› Cosmographic Connection Between Cosmological And Planck Scales: The Barrow-Tsallis Entropy
› Quarkyonic matter and hadron-quark crossover from an ultracold atom perspective
› Time-of-Flight Constraints on Neutrino Millicharge from Supernova Neutrinos in Galactic Magnetic Fields
› A study on Dusty Plasma Physics and the examination of Jeans Criteria for the Milky Way

  ↓↑    

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