ul. Podchorążych 2, 30-084 Kraków.
tel.: (+48 12) 662 6301;
fax: (+48 12) 637 2243;
Obs. tel.: (+48) 502 113714
Obserwatorium Astronomiczne na Suhorze

Zachód Słońca

Kamerka S

Kamerka N

Niebo
Temperatura
3.1 °C
Wilgotność
84%
Wiatr
1.6 km/h
Ciśnienie
1025.1 hPa

Księżyc
Najnowsze prace na astro-ph:
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Constraining the Lifespan of Intelligent Technological Civilization in the Galaxy ›
Gaia DR3 Analysis of Four Open Clusters Toward the Galactic Anticenter ›
You can't see me: super-Eddington growth hindering X-ray detection in high-z broad-line AGNs ›
A Morphology Catalog of Galaxies in CEERS: Evolution in the Size and Color Gradients of Galaxies Since Cosmic Dawn ›
A steadily declining dispersion measure for the repeating fast radio burst FRB 20220529A: Evidence for an FRB engine embedded in an expanding supernova remnant ›
XRISM Observation of the Supernova Remnant N103B: Velocity Structure and Thermal Properties ›
Filamentary Hierarchies and Superbubbles II: Impact of superbubbles and galactic dynamics on filament formation and fragmentation ›
JWST COMPASS: NIRSpec/G395H Transmission Observations of the Sub-Neptune HD 15337 c ›
JWST COMPASS: A NIRSpec G395H Transmission Spectrum of Radius Valley-Dweller TOI-260 b ›
It's a matter of time: Empirical Constraints on Supernova Yields and Delay Times from Dwarf Spheroidal Galaxies ›
Unveiling the X-ray properties of the eclipsing Cataclysmic Variable UU Aqr: spatially and spectrally-resolved two-component emission ›
STILTS-NLI: A Natural Language Interface for STILTS ›
Detection of CO$_2$ ice in the planetary nebula NGC 6302 ›
Identifying Evolutionary Stages of Molecular Clumps through Unsupervised and Supervised Machine Learning ›
3D-Herschel: Constraining Dust Emission with Panchromatic Modeling of 3D-HST Galaxies ›
Little Red Dots as Obscured Little Blue Dots: A Super-Eddington Unification Model ›
First Determination of the Cosmic Microwave Background Radiation Temperature at $z\!=\!0.68$ Using Molecular Absorption Lines ›
Cepheid-based Distances to NGC 4303 and NGC 1068 ›
ZTF Monitoring of $\gamma-$ray emitting Narrow Line Seyfert 1 Galaxies ›
AGN Feedback and the Development of Dusty Multiphase Gas in X-ray Emitting Elliptical Galaxies ›
PICASO 4.0: Clouds and Photochemistry in Climate Models of Brown Dwarfs and Exoplanets ›
Halo Photometry and Asteroseismology for 98 of the Brightest Stars Observed by TESS ›
High Spectral Resolution X-ray Observations of the Evolved Supermassive Stellar Binary System $\eta$ Carinae - Iron K$\alpha$ Band Profile Revealed with XRISM ›
Accretion-modified Stars in Accretion Disks of Active Galactic Nuclei: Contribution to AGN disk viscosity ›
Cosmic Environment as the Primary Driver of Dwarf Satellite Statistics ›
Using Lithium and Beryllium to Study Structure and Evolution of Rotating Stars: Spite Plateau of Halo Stars ›
WFST Astrometric Calibration -- I. Modeling Global Geometric Distortion with Zernike Polynomials ›
Identify ~20,000 Li-rich Giants in the LAMOST Low-Resolution Survey ›
Shadows of Giants: Constraints on Stupendously Large Black Holes from Negative Sources against the Cosmic Microwave Background ›
A Multi-Diagnostic Observational Framework for Magnetosonic Solitary Waves During Geomagnetic Storms in Solar Cycles 24 and 25 using Cluster II Mission ›
JWST-DECO: Temporal Variations in the Mid-IR Silicate Features of Two T Tauri Discs Based on Spitzer and JWST observations ›
Universality in Space Time $\omega$ modes of Quarkyonic Stars ›
VLBI Detections of Compact Nuclei in Spiral-hosted Double-lobed Radio-loud Active Galactic Nuclei (DRAGNs): Evidence for Weak Parsec-Scale Jet Activity ›
Automated Identification of the Tip of the Red Giant Branch in Globular Clusters with Gaia Data ›
Relativistic Tidal Dissipation and the Gravitational-wave Signal of a White Dwarf Orbiting an Intermediate-Mass Black Hole ›
KMT-2024-BLG-3237: Another Free-Floating Planet Candidate with Angular Einstein Radius Measurement ›
Beyond Colors: Probing Redshifts from Galaxy Morphology in Single-band Images with ViT-MDNz ›
The ASKAP Variables and Slow Transients (VAST) Extragalactic Survey - Data Release 1 ›
Trial dispersion measure spacing in fast radio burst searches with HEIMDALL ›
(1+1)-Dimensional Schr\"odinger-Poisson equation with contact interaction ›
Statistical Study of Rapid Blue Excursions as Mass Conduits in Solar Atmosphere ›
Gaia DR3 supervised classification of asteroid reflectance spectra ›
Black hole Limits Redefined: Extreme Efficiency in Black Hole Jets ›
Probing the Atmospheres of Young Long-Period Sub-Neptune Progenitors with ELT/ANDES ›
Detection of circumstellar disks around nearby young brown dwarf candidates ›
Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model ›
A FUV - optical approach for studying hierarchical star formation in nearby galaxies with UVIT ›
The Environmental Switch in Black Hole Feeding: Bar-Driven vs. Merger-Driven Growth in IllustrisTNG50 ›
The MARTINI Platform (I): Se I-X atomic calculation and expansion opacity for early-stage kilonova spectral analysis ›
Group Pre-processing in J1611+4026: Minor Rejuvenation of a Massive ETG fueled by Interaction-driven Gas Transfer ›
Pulse-resolved Classification and Characteristics of Long-duration GRBs with \emph{Swift}-BAT Data.II. Main Burst versus Extended Emission ›
The Evolution of Nulling in Pulsars ›
Demonstrating Single Photon Counting with Kinetic Inductance Detectors from 3.8 to 25 $\mu$m ›
Eating planets makes you younger: The magnetic dynamo rejuvenation of GJ 504 by planetary engulfment ›
Energy Deposition by Galactic Cosmic Rays and Implications for Ozone Chemistry ›
Cosmic voids as a probe of the nature of dark matter: simulations and galaxy survey forecasts ›
Tight bounds on the Mawell-Carroll-Field-Jackiw parameters using Fast Radio Bursts ›
Warm Debris Disk Candidates around Nearby FGK Stars from LAMOST DR12 ›
Characterising the magnetospheric accretion process of DF Tauri's primary ›
Phase-Induced Amplitude Apodization Complex Mask Coronagraph (PIAACMC) on-sky demonstration with MagAO-X ›
Correlated residuals in Tully-Fisher and Fundamental Plane relations and their impact on peculiar velocity measurements ›
The LOFAR sub-arcsecond view of the high-redshift radio relic in PSZ2G091.83+26.11 ›
Measurements of the HI intensity mapping power spectrum at low redshifts with MIGHTEE data: comparison with detected HI galaxies ›
A High-Throughput AES-GCM Implementation on GPUs for Secure, Policy-Based Access to Massive Astronomical Catalogs ›
Stochastic Evolution of Galactic Star Formation with Halo Coupling, AGN Quenching and Hopf Bifurcation Dynamics ›
TEPCat: The Transiting Extrasolar Planet Catalogue ›
Distribution functions for spheroids ›
Searching for low-mass stars with magnetically-induced hyper-inflated radii ›
Sulfur fractionation in coronal plumes as observed by Solar Orbiter/SPICE ›
The extremely low-luminosity Type Iax SNe 2022ywf and 2023zgx ›
A Lorentz-Covariant Spectral Universality of Stochastic Fields ›
The Axion-Photon Mixing and the Extragalactic Magnetic Background: Plateau Regimes, Resonances, and Non-Gaussian Boosts ›
Elevated Eccentricities in the Radius Valley Hint at Water-Rich Mini-Neptunes ›
Tidal Synchronization of Binaries in Pleiades ›
Variability of the X-ray obscuring wind in Mrk 335 with XMM-Newton/RGS ›
Imprints of primordial magnetic fields on the late-time Universe ›
Dyson spheres on H-R diagram ›
A White Dwarf Tidal Disruption by an Intermediate-Mass Black Hole as the Progenitor of Ultra-long GRB 250702B ›
A precessing jet from a supermassive black hole: multi-wavelength observations of S5 1044+71 ›
Extreme Emission Line Galaxies in CEERS Are Powered by Star Formation, not AGN ›
Deep ensemble graph neural networks for probabilistic cosmic-ray direction and energy reconstruction in autonomous radio arrays ›
Revisiting the Perseus Cluster II: Metallicity-Dependence of Massive Stars and Chemical Enrichment History ›
Revisiting the Perseus Cluster III: Role of Aspherical Explosions on its Chemical Composition and Extension to Metal-Poor Stars and Galaxies ›
TESS Planet Occurrence Rates Reveal the Disappearance of the Radius Valley Around Mid-to-Late M Dwarfs ›
Lepton asymmetry leading to baryogenesis by primordial black holes ›
Conformal symmetry in force-free electrodynamics ›
Fluctuating polytropic processes, turbulence, and heating ›
The global structure of the time delay likelihood ›
Current-carrying string network evolution in an external magnetic field ›
Anomalous cosmic rays within the inner heliosphere: Observations of helium by the High Energy Telescope onboard Solar Orbiter ›
The 2027-2034 Vision for Nuclear Physics in Canada, with an outlook to 2041 ›
ACT-Consistent B-L Higgs Inflation in Supergravity ›
The Delta-isobar masquerade: intrahadronic phase transitions and their quark-mimicking signatures in neutron stars ›
Investigating potential benefits of future sub-L1 missions with STEREO-A ›
Confinement transition to gravitational waves in the one-flavor $SU(4)$ Hyper Stealth Dark Matter theory ›
Ruling Out Spiky WIMP Dark Matter using Indirect Searches ›
Exploring Ambient Radio Frequency Emissions ›
The dramatic transition of the extreme Red Supergiant WOH G64 to a Yellow Hypergiant ›
Black holes and gravitational waves from phase transitions in realistic models ›
Decoding FRB energetics and frequency features hidden by observational incompleteness ›
Polynomial Potential Inflation in the ACT Era: From CMB to Primordial Black Holes ›
Delensing CMB B-modes using galaxy surveys: the effect of galaxy bias and matter clustering non-linearities ›
A Semi-Supervised Learning Method for the Identification of Bad Exposures in Large Imaging Surveys ›
Mergers Fall Short: Non-merger Channels Required for Galactic Heavy Element Production ›
Galaxy Zoo: Cosmic Dawn -- morphological classifications for over 41,000 galaxies in the Euclid Deep Field North from the Hawaii Two-0 Cosmic Dawn survey ›
Overview of the ESCAPE Dark Matter Test Science Project for Astronomers ›
4MOST Cosmology Redshift Survey (CRS): Clustering properties of CRS BG and LRG target catalogues ›
ALMAGAL VII. Cataloging Hierarchical Mass Structure from Cores to Clumps across the Galactic Disk ›
Constraining Power of Wavelet vs. Power Spectrum Statistics for CMB Lensing and Weak Lensing with Learned Binning ›
Where Giants Dwell: Probing the Environments of Early Massive Quiescent Galaxies ›
Superluminal Wave Activation at Relativistic Magnetized Shocks ›
The Polarization and Magnetic Field of the Radio Arc as Observed by ALMA at 100 GHz ›
The winds of OBA hypergiants and luminous blue variables: Dynamically-consistent atmosphere models reveal multiple wind regimes ›
Denoising the Deep Sky: Physics-Based CCD Noise Formation for Astronomical Imaging ›
Kolmogorov analysis of pulsar TOA ›
Long Photometric Cycles in Double Periodic Variables from Nodal Precession of a Tilted Accretion Disk ›
Time-variable Scattered Light in Herbig Disks Observed with Subaru/SCExAO ›
Fermi-LAT 16-year Source List ›
Exocometary physics: material release and tails ›
Fundamental quantum limits for detecting ultrahigh frequency gravitational waves ›
Nonlinear causality of Israel-Stewart theory with diffusion ›
Accretion of a Vlasov gas by a Kerr black hole ›
Bondi-type accretion onto a Kerr black hole in the kinetic regime ›
Resonance in black hole ringdown: Benchmarking quasinormal mode excitation and extraction ›
Black Hole Superradiance of Interacting Multi-Field ›
High Mass Dark Matter Searches With the High Speed Flux From the Large Magellanic Cloud ›
Thermoelectric coefficients of two-flavor quark matter from the Kubo formalism ↓↑