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

gwiazdy nad kopułą

Kamerka S

Kamerka N

Niebo
Temperatura
18.1 °C
Wilgotność
53%
Wiatr
1.6 km/h
Ciśnienie
1025.9 hPa

Księżyc
Najnowsze prace na astro-ph:
›
A No-Go Theorem for the Mass-Radius Relation of Solitons ›
Mergers via failed common envelope as a route towards intermediate-mass stripped stars ›
A Precise Measurement of the Fermi-LAT Galactic Center Excess Morphology and Spectrum ›
No Blue without Red: Evolutionary Properties of Super-Early Galaxies ›
Mg II h&k spectral line properties computed using 3D radiative transfer in an enhanced network region simulated with the MURaM-ChE code ›
Strong X-ray Variability of I Zwicky 1: Obscuration from Clumpy Accretion-Disk Winds ›
Magnetic field dynamics in isolated neutron stars with an external dipole field ›
Star-planet interaction in the Proxima system ›
JWST-DECO: The Impact of Accretion on Mid-Infrared Observable Water in Planet-forming Disks ›
The first 3D MHD core-collapse progenitors I: General properties, convection and nuclear burning ›
Towards Doppler eclipse mapping of hot Jupiters. An observational perspective on WASP-33 b with SPIRou ›
The $\tau$ of Neutral Hydrogen: Increased CMB Optical Depth at Long Wavelengths ›
The first 3D MHD core-collapse progenitors II: Rotation, magnetic-field amplification, and magnetic topology ›
Gravitational waves from cosmic strings with friction: analytical approximations and parameter space ›
The unique capabilities of HST for stellar physics Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars ›
The Solar Dynamics Observatory in the Living With a Star Era: From Solar Observations to Predictive Heliophysics ›
\texttt{calypso}: a Parameter-Conditioned Stochastic Surrogate Model for Circumbinary Accretion Time-Series ›
Gaia Exoplanet Orbits, Demographics, and Evolution Survey (GEODES): Characteristics of Three Long-Period Companions Accelerating their Host Stars ›
JWST reveals anomalously enhanced methane outgassing from below Chiron's water ice and carbon dioxide bearing surface ›
SDSS+JWST Census of Stellar and Nebular Dust Attenuation at $z \sim 0$-7: Mass Dependence and Redshift Evolution ›
A Strongly Parametrized Mass Ratio Model for the Stable Mass Transfer Channel: a Case Study of the $10 \, \rm{M}_{\odot}$ Peak ›
Constraining the Photon Intensity of Extragalactic Background Light with the HAWC Observatory for the Blazar Mrk 421 ›
Increasing the Precision of Surrogate Models for Weak Lensing Mass Maps with Flow Matching ›
Evidence of radial-migration driven Galactic disc expansion with the U-shape stellar age profile ›
A Gaia-linked High-purity QSO Candidate Catalog in Selected Fields with Extinction-binned Calibration and Spectrum-informed Training ›
An Improved HDBSCAN-based Detection and Tracking Method for Solar Active Regions in Magnetograms ›
TESS Observations of Stochastic Low-frequency Variability in Extreme Helium Stars ›
Suppression of star formation at the centre of barred AGN galaxies ›
Rotation-curve residuals reveal a suppressed acceleration branch in dwarf galaxies ›
Superrotation and Jet Migration in Simulations of Jupiter's Convective Zone and Weather Layer ›
The dual effect of group-scale environments on galaxy quenching during cluster infall: pre-processing and protection ›
Dissecting the Perseus-Pisces supercluster observed with CFHT-MegaCam: Exploring late-type galaxy shape alignments within the local cosmic web ›
Size-Dependent Fresh Surface Signatures in Asteroid Families: Observational Evidence from Dual-Band Albedo Analysis ›
Cosmological constraints from neighbor-density-weighted marked correlation functions ›
Performance analysis of extragalactic classifications in Gaia Data Release 4 ›
ALMA CO-CAVITY I. Resolved Molecular Gas in Void Galaxies ›
Nature of HD 251108: an RS CVn binary with a long-term evolving spot ›
Insights from Analytical Theory of Eccentric Circumbinary Disks II. Forced Modes and Resonance for Precessing Binaries ›
Cosmic web stripping and starvation of low-mass filament galaxies in TNG50 ›
TOI-7154b: A Close-in Massive Brown Dwarf in an Eccentric Orbit ›
Disruption of a Giant: Spectroscopic Identification of Members in the Periphery and Tidal Tails of $\omega$ Centauri ›
Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona ›
A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz ›
Examining extinction distributions for type Ia supernovae in simulated 3D galaxies ›
Ensemble asteroseismology: An ensemble approach to detecting signatures of solar-like oscillations in K-dwarfs ›
Design and Development of Cassegrain Module for PARAS-2 Spectrograph (CAMPAS) ›
Scalable Dark Siren Cosmology with gwcosmo: GPU Acceleration, Validation and Systematics ›
Inferring the role of binary neutron star mergers in r-process nucleosynthesis with multi-messenger observations using Cosmic Explorer and Einstein Telescope ›
Atomic gas properties at the positions of supernovae Type Ia, II, and Ib/c ›
51 Peg b revisited with VLT/CRIRES+. Constraints on atmospheric thermal structure, chemical composition, and an alternative orbital solution ›
A Markov-Chain-Monte-Carlo-based Hybrid Noise Inference for Continuous Wavelet Power Spectra: with Applications to Solar and Stellar Oscillatory Signals ›
Multi-layered model-based characterisation of the local-Universe galaxy data from the GAMA survey ›
Investigation of the Two-Dimensional Velocity Field of the Large-Scale Coronal Wave from September 6, 2011 using the SOLERwave Tool ›
Long-term optical and near-infrared photometric evolution of SN 2019vxm, an interacting Type IIn supernova ›
Gas Fraction and Depletion Time Drive the Main-Sequence Scatter in Massive Galaxies at $z\sim1.5$ ›
Modeling (Sub-)millimeter Scattering Properties of Fractal and Consolidated Porous Particles: Applications to Protoplanetary Disks ›
HiFAST: An HI data calibration and imaging pipeline for the FAST IV: The stray-radiation correction ›
The FAST Hundred-Deg$^2$ HI Deep (HD$^2$) Survey: Early Results from the Pilot Survey ›
The s- and r- components of the proto-solar composition ›
New substellar candidates identified through deep learning in the F150 sample of the large-scale SHINE direct imaging survey ›
A Wavelet-Integrated Search Pipeline for Narrowband Technosignatures in FAST Observations of 33 Exoplanet Systems ›
Hydrodynamic model of nonthermal emission from the Fermi bubbles ›
Gaia-Sausage-Enceladus: Lithium evolution from early red-giant-branch and main-sequence stars ›
Probing the environments of FRI and FRII radio galaxies in LoTSS DR2 with galaxy clusters ›
Probing Solar Wind Structures with Solar Energetic Particle Observations from Solar Orbiter ›
GMRT Survey of Radio Emission from Magnetic Massive Stars -- I: Emission from Single Stars at sub-GHz Frequencies ›
Gaia FGK benchmark stars: abundances of \textit{n}-capture elements of the third version ›
Sharper Than Ever: Do Modern Observations Pin Down the Solar Radius to Converge on New Standards? ›
Unsupervised Chemo-Dynamical Dissection of the Inner Galactic Halo: Discovery of Five Accreted Substructures with SDSS-V and Gaia ›
Astrophysical Parameters of 5056 Open Star Clusters from Bayesian Nested Sampling with PARSEC Isochrones ›
Integral field spectroscopy with no IFUs: combining wide-field rotational slitless spectroscopy with tomographic reconstruction ›
An extremely bright slow-rising afterglow from an off-axis jet in GRB 260310A ›
cloelib: A Flexible Python Library for Computing Cosmological Observables in the Euclid Era ›
cloelike: A Python Library for Cosmological Likelihood Inference in the Euclid Era ›
Minor Merger, Major Growth: An Overmassive, Highly Accreting Black Hole Powering a Secondary AGN In a Cosmic Noon Minor Merger ›
Evaluation and Modeling of Pneumatic Percussive Drill for Martian Subsurface Access ›
Gravitational Field of a Rotating Mass on an Expanding Universe ›
Cuspidal Singularities in Collapsing Domain Walls ›
Enhanced Stellar Production of Weakly Interacting Slim Particles from Non-Thermal Nuclear Cascades ›
Quasiradial oscillations of rotating hybrid neutron stars ›
Reachability for Low-Thrust Trajectories via Maximum Initial Mass ›
Natural Metric-Affine Inflation: Reloaded ›
Rapid cooling of the Cassiopeia A neutron star due to superfluid quantum criticality ›
Catalog-based detection of unrecognized blends in deep optical ground based imaging ›
Cloudy mornings and clear evenings on a gas giant exoplanet ›
Probing spectral variability in NGC 4490 ULX-8 over 24 years of XMM-Newton, Chandra and Swift-XRT observations ›
Cosmic shear with one component and its application to future radio surveys ›
Source REconstruction of Arcs behind Cluster Halos (SourceREACH): A New Source Reconstruction Algorithm Optimized for Giant Arcs and Galaxy Cluster Lenses ›
Consequences of radially correlated rotation curves for galaxy mass models ›
Rotational Light-curve Recovery and Predictions of the LSST Yield of Hildas ›
Maximum Energy of Particles Accelerated in Gamma-Ray Burst Afterglow Shocks ›
Little Red Dot $-$ Host Galaxy $=$ Black Hole Star: A Gas-Enshrouded Heart at the Center of Every Little Red Dot ›
Simulation-based cosmological inference from optically-selected galaxy clusters with $\texttt{Capish}$ ›
POSEIDON I: The Dynamical Origins of Transiting Neptunes ›
Anisotropic Diffusion in Pulsar Halos: Interpreting the asymmetric morphology of Geminga and Monogem halos measured by HAWC ›
pyKurucz: A Pure Python Reimplementation of Kurucz ATLAS12 and SYNTHE for Stellar Spectrum Synthesis ›
Implications of a Cosmogenic Origin of KM3-230213A for Ultra-High-Energy Protons ›
The dominance of turbulence over magnetism in the formation of massive star cluster seeds ›
Reliability of uGMRT Band-4 Polarimetry: Results from a Quadrature Hybrid Polarizer Bypass Experiment ›
Correlation between Ultrahigh-Energy Neutrino KM3-230213A and Gamma-Ray Bursts ›
TDCOSMO XXV: A "soup-to-nuts" 6.5% $H_0$ measurement $-$ strong lensing and dynamics with a maximally flexible mass sheet ›
Superfluid $^3$He aerogel experiments as a laboratory neutron star analogue ›
Investigating the formation channel of GW231123: Population III stars or hierarchical mergers? ›
Detectability of Polarized Gamma-ray Emission from Blazar Flares with COSI ›
The NUV transit of XO-3 b ›
Stellar Age Compression Reshapes Interpretations of the Milky Way Thick-Disk Formation History ›
SN 2023fyq: direct detection of a Type Ibn supernova progenitor and its multi-wavelength environmental constraints ›
29SiO and 30SiO J=1--0 maser signatures in Galactic AGB stars: the impact of third dredge up and turbulence velocity ›
Spectra as Language: Large Language Models for Scalable Stellar Parameter and Abundance Inference ›
Pulsar timing solutions for 17 pulsars at 150 MHz from the Irish LOFAR station ›
Follow the wobble: Statistical methods to detect astrometric binary asteroids in Gaia FPR ›
Thermodynamical uncertainties for primordial black holes from cosmological phase transitions ›
Shedding light on dark matter spikes through refractive neutrino masses ›
Global time-frequency search for stellar-mass binary black holes in LISA ›
Superfluid fraction in the crystal phase of the inner crust of neutron stars ›
Cosmological coupled black holes immersed in dark sector ›
Greybody Factor, Resonant Frequencies, and Entropy Quantization of Charged Scalar Fields in the Kerr-EMDA Black Hole ↓↑