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
4.6 °C

Wilgotność
 93%

Wiatr
0.0 km/h

Ciśnienie
1022.8 hPa

Moon

Księżyc

 Wiadomości z astronet.pl

› Jak wygląda praca geologa planetarnego? – wywiad z Dr Jakubem Ciążelą
› Katalog Caldwella: C8
› Największy polski (toruński) radioteleskop w tarapatach
› W Układzie Słonecznym: Pas Planetoid
› Nagroda Nobla z fizyki 2025
› Misje Kosmiczne XX wieku: Enterprise
› Złożone cząsteczki organiczne na Enceladusie: odkrycie sondy Cassini
› Niebo w październiku 2025 roku
› III Olimpijska Liga Astronomiczna
› The outer limits of reason – recenzja książki
RSS  Najnowsze prace na astro-ph:

› Early massive galaxy formation in the core of a galaxy protocluster 650 million years after the Big Bang
› MESA-QUEST: Tracing the formation of direct collapse black hole seeds via quasi-stars
› The Blue Jay Survey: Deep JWST Spectroscopy for a Representative Sample of Galaxies at Cosmic Noon
› The PHANGS-MUSE/HST-Halpha Nebulae Catalogue
› Spatial Profiles of 3I/ATLAS CN and Ni Outgassing from Keck/KCWI Integral Field Spectroscopy
› Cross-correlation of Luminous Red Galaxies with ML-selected AGN in HSC-SSP III: HOD Parameters for Type I and Type II Quasars
› Violent mergers revisited: The origin of the fastest stars in the Galaxy
› Spin and Obliquity Distributions of Low-mass Planets Shaped by Dynamical Instability
› Connecting Cores and Black Hole Dynamics Across Scales: From Globular Clusters to Massive Ellipticals
› ELPIS: Accelerated metal and dust enrichment in a proto-cluster core at $z\approx8$
› Searching for GEMS: TOI-5916 b & TOI-6158 b are two Saturn-density planets orbiting M2 dwarfs
› Eruptive mass loss less than a year before the explosion of superluminous supernovae. II. A systematic search for pre-explosion eruptions with VLT/X-shooter
› Dwarf diversity in $\Lambda$CDM with baryons
› Delayed phase mixing in the self-gravitating Galactic disc
› Wind and nearby stellar environment of the quiescent luminous blue variable Var 2 in the Galaxy M33
› Preferential accretion of binary stars
› Hubble reveals complex multi-scale structure in the edge-on protoplanetary disk IRAS 23077+6707
› Evolutionary Links: From Gaia Neutron Star Binaries to Pulsar White Dwarf Endpoints
› The resilience of the sailboat stable region
› A (very) simple proof of the gravitational energy formula of polytropic spheres
› Magnetic Decay Index Profile and Coronal Mass Ejection Speed
› A Systematic North-South asymmetry in the Steady-state Climate of rapidly-rotating Oblique Water Worlds
› Ultraviolet radiation and neutrinos: two messengers from CCSNe in the CSM scenario
› Abundances of Rarely Detected s-process Elements Derived from the Ultraviolet Spectrum of the s-process-enhanced Metal-poor Star HD 196944
› Near the Runaway: The Climate and Habitability of Teegarden's Star b
› PLATOSpec: a precise spectrograph in support of space missions
› GALACTICNUCLEUS: A high angular resolution JHKs imaging survey of the Galactic centre
› Rotation of Polarization Angle in Gamma-Ray Burst Prompt Phase. III. The Influence of the Magnetic Field Orientation
› Impact of Cosmic Ray Acceleration on the Early Evolution of Bow Shocks around Massive Runaway Stars
› Deep JWST spectroscopy of galaxies in a candidate ionized bubble at $z = 8.7$: probing reionization at pMpc scales with Ly$\alpha$ emission
› The Two-Zone Temperature Distribution Model: Inferences on the Structure and Composition of Dusty Protoplanetary Disks
› Short-Lived Radioisotopic enrichment from AGB interlopers in low-mass star-forming regions
› Very-Long Baseline Interferometry Imaging with Closure Invariants using Conditional Image Diffusion
› Using gravitational lensing to probe for bright quintessential galaxies in the Epoch of Reionization
› A Possible Shutting-Down Event of Mass Accretion in An Active Galactic Nucleus at z~1.8
› Eternal inflation bubble collision signature on CMB remote dipole and quadrupole fields
› Polar Filaments Capture High Latitude Solar Poloidal Field Interactions and can Foretell the Future Sunspot Cycle Amplitude before Polar Field Precursors
› CCAT: Optical Responsivity, Noise, and Readout Optimization of KIDs for Prime-Cam
› Beyond the Brightest: A Deep Learning Approach to Identifying Major and Minor Galaxy Mergers in CANDELS at $z \sim 1$
› The AURORA Survey: Ionizing Photon Production Efficiency with Minimal Nebular Dust Attenuation Systematics
› Violent mergers can explain the inflated state of some of the fastest stars in the Galaxy
› Computational advances and challenges in simulations of turbulence and star formation
› YSO Variability in the W51 Star-Forming Region
› Encapsulating Textual Contents into a MOC data Structure for Advanced Applications
› A census of quiescent galaxies across $0.5 < z < 8$ with JWST/MIRI: Mass-dependent number density evolution of quiescent galaxies in the early Universe
› Is Milky Way stable all the way ? A TNG50 view from cosmic noon to the present day
› Experimental tests of the calibration of high precision differential astrometry for HWO
› Spatio-Temporal Evolution of the March 2022 ICME Revealed by Multi-Point Observations of Forbush Decreases
› Fe XVIII-XXIV K beta Inner-shell Absorption Lines in the X-ray Spectra of Neutron Star and Black Hole Binaries with XRISM
› Hidden Figures of Globular Clusters: Integrated Stellar Populations Impacted by Hot Subdwarfs
› Discovery of new magnetic {\delta} Scuti stars and impact of magnetism on pulsation excitation
› The rings of (2060) Chiron: Evidence of an evolving system
› Association of cold gas, massive galaxies, and AGNs in a filamentary protocluster traced by triple narrow-band imaging
› Infrared spectral signatures of light r-process elements in kilonovae
› Extremely UV-bright starbursts at the end of cosmic reionization
› Lanthanide Impact on the Infra-Red Spectra of Nebular Phase Kilonovae
› Catalog and Characterization of Science Orbit Configurations for an Enceladus Orbiter
› Optically thick winds of very massive stars suppress intermediate-mass black hole formation
› Enhanced Localization of Dark Lensed Gravitational Wave Events Enables Host Galaxy Identification and Precise Cosmological Inference
› Asteroseismic calibration of the Rossby number and its connection to the stellar dynamo and fundamental properties
› Jets in Low-Mass Protostars
› Faint galaxies in the Zone of Avoidance revealed by JWST/NIRCam
› A Catalog of Filaments in the Central Molecular Zone
› Limits of Standard Tidal Models at Quaoar: Matching Weywot's Orbit, Missing the Spin
› Polarization from Rapidly Rotating Massive Stars
› DIPLODOCUS II: Implementation of transport equations and test cases relevant to micro-scale physics of jetted astrophysical sources
› The double neutron star PSR J1946+2052 I. Masses and tests of general relativity
› Gamma-rays from Wolf-Rayet stellar winds
› Spectroscopic Reverberation Mapping for SARM: The Case of Mrk 1048 and Mrk 618
› Widespread Hot Molecular Gas Heated by Shear-induced Turbulence in the Galactic Center
› A 50-min coronal kink oscillation and its possible photospheric counterpart
› Using simultaneous mass accretion and external photoevaporation rates for d203-504 to constrain disc evolution processes
› Non-linear structure formation with elastic interactions in the dark sector
› Mass dependence of halo baryon fractions from the kinetic Sunyaev-Zeldovich effect
› Modeling gamma-ray signatures of particle acceleration in stellar clusters from GeV to PeV
› JWST and Keck Observations of the Off-Nuclear TDE AT 2024tvd: A Massive Nuclear Star Cluster and Minor-Merger Origin for its Black Hole
› A constant upper luminosity limit of cool supergiant stars down to the extremely low metallicity of I Zw 18
› The MIRI Excesses around Degenerates (MEAD) Survey I: A candidate cold brown dwarf in orbit around the nearby white dwarf 2MASS J09424023-4637176
› Formation of protostars and the launching of stellar core outflows with moving-mesh radiation non-ideal magnetohydrodynamics
› Cloudy with a chance of starshine: Possible photometric signatures of nebular-dominated emission in $1.5 < z < 8.5$ JADES galaxies
› Alleviating the $H_0$ tension through new interacting dark energy model in light of DESI DR2
› GEFF: The Gradient Expansion Formalism Factory - A tool for inflationary gauge-field production
› Searching for Stellar-Feedback-Driven Outflow Signatures: A Deep Dive into NGC 3741
› Energy calibration of LHAASO-KM2A using the cosmic ray Moon shadow
› The Influence of the Accretion Disc Structure on X-ray Spectral States in Symbiotic Binaries
› Enigmatic centi-SFU and mSFU nonthermal radio transients detected in the middle corona
› Tycho supernova exploded inside a planetary nebula (SNIP)
› The diverse shapes of binary asteroid satellites born from sub-escape-velocity moonlet mergers
› Hierarchical summaries for primordial non-Gaussianities
› Interacting galaxies in the IllustrisTNG simulations - IX: Mini mergers trigger AGN in cosmological simulations
› Mapping the Perseus Galaxy Cluster with XRISM: Gas Kinematic Features and their Implications for Turbulence
› An Ultra-Short Period Super-Earth and Sub-Neptune Spanning the Radius Valley Orbiting the Kinematic Thick Disk Star TOI-2345
› Visual morphological classification of the full MaNGA DR17 sample: a general characterization
› Born Dry or Born Wet? A Palette of Water Growth Histories in TRAPPIST-1 Analogs and Compact Planetary Systems
› The Gravitational Wave Memory from Binary Neutron Star Mergers
› Black Hole Ringdown Amplitudescopy
› Quasinormal modes from numerical relativity with Bayesian inference
› False Alarm Rates in Detecting Gravitational Wave Lensing from Astrophysical Coincidences: Insights with Model-Independent Technique GLANCE
› On the Speed-up of Wave-like Dark Matter Searches with Entangled Qubits
› Dynamically generated tilt of isocurvature fluctuations
› New Tests of Low-Scale Quantum Gravity with Cosmic-Ray Collisions
› Gravitational Wave Signatures from Lepton Number Breaking Phase Transitions with Flat Potentials
› Phase space analysis of an exponential model in $f(Q)$ gravity including linear dark-sector interactions
› Model of deep zonal flows in giant planets
› The importance of being non-minimally coupled: scalar Hawking radiation from regular black holes
› The probe limit in MHD and its implications for magnetic transport
› Observational Constraints on Chaplygin Gas Models in Non-Minimally Coupled Power Law $f(Q)$ Gravity with Quasars
› High-energy photons from Gamma-Ray Bursts, but no neutrinos
› Hunting Primordial Black Hole Dark Matter in Lyman-$\alpha$ Forest
› Reconstruction of the swampland conjectures with DESI DR1 BAO data
› Value Added Catalog of physical properties of more than 1.3 million galaxies from the DESI Survey
› Measuring Star Formation Histories from Asymptotic Giant Branch Stars I: A Demonstration in M31
› How Many Bursts Does it Take to Form a Core at the Center of a Galaxy?
› The $z \gtrsim 9$ galaxy UV luminosity function from the JWST Advanced Deep Extragalactic Survey: insights into early galaxy evolution and reionization
› Enhancing the reliability of machine learning for gravitational wave parameter estimation with attention-based models
› Unveiling the trends between dust attenuation and galaxy properties at z ~ 2 - 12 with the James Webb Space Telescope
› A Time-Dependent Solution for GSN 069 Disk Evolution and the Nature of Long-Lived Tidal Disruption Events
› The Giant Arc -- Filament or Figment?
› Clustering analysis of BOSS-CMASS galaxies with semi-analytical model for galaxy formation and halo occupation distribution
› HeII emitters at cosmic noon and beyond. Characterising the HeII {\lambda}1640 emission with MUSE and JWST/NIRSpec
› Prospects for probing dark matter particles and primordial black holes with the Square Kilometre Array using the 21 cm power spectrum at cosmic dawn
› Ultra-long MeV transient from a relativistic jet: a tidal disruption event candidate
› Tidal heating in detached double white dwarf binaries
› In-Situ Formation of the Cold Classical Kuiper Belt
› DIPLODOCUS I: Framework for the evaluation of relativistic transport equations with continuous forcing and discrete particle interactions
› The redshift distribution of Einstein Probe transients supports their relation to gamma-ray bursts
› Investigating aerosols as a way to reconcile K2-18 b JWST MIRI and NIRISS/NIRSpec observations
› Dwarf galaxy halo masses from spectroscopic and photometric lensing in DESI and DES
› Extended mass distribution of PBHs during QCD phase transition: SGWB and mini-EMRIs
› 1FLAT: a Firmamento-based catalog of AGN in Fermi-LAT high Galactic latitude {\gamma}-ray sources
› JWST Spectroscopy of SN Ia 2022aaiq and 2024gy: Evidence for Enhanced Central Stable Ni Abundance and a Deflagration-to-Detonation Transition
› Resolving stellar populations, star formation, and ISM conditions with JWST in a large spiral galaxy at z $\sim$ 2
› The Relation Between AGN and Host Galaxy Properties in the JWST Era: II. The merger-driven evolution of Seyferts at Cosmic Noon
› Resonant W and Z Boson Production in FSRQ Jets: Implications for Diffuse Neutrino Fluxes
› The Sunburst Arc with JWST. IV. The importance of interaction, turbulence, and feedback for Lyman-continuum escape
› Emergent Cosmological Expansion in Scalar-Tensor Theories of Gravity
› Anatomy of singlet-doublet dark matter relic: annihilation, co-annihilation, co-scattering, and freeze-in
› Verifiable type-III seesaw and dark matter in a gauged $\boldsymbol{U(1)_{\rm B-L}}$ symmetric model
› Characterized behaviors of black hole thermodynamics in the supercritical region
› Electroluminescence and charge multiplication in liquid xenon with a VCC-like Microstrip Plate
› Accelerated inference of binary black-hole populations from the stochastic gravitational-wave background
› Radio emission from airplanes as observed with RNO-G
› Projective Transformations for Regularized Central-Force Dynamics: Hamiltonian Formulation
› Space-based cm/kg-scale Laser Interferometer for Quantum Gravity
› Small Progenitors, Large Couplings: Type Ic Supernova Constraints on Radiatively Decaying Particles
› Splitting the Gravitational Atom: Instabilities of Black Holes with Synchronized/Resonant Hair
› GW250114 reveals black hole horizon signatures

  ↓↑    

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