Podchorazych 2, 30-084 Krakow, Poland.
tel.: (+48 12) 662 6301;
fax: (+48 12) 637 2243;
Obs. tel.: (+48) 502 113714
Mount Suhora Astronomical Observatory

Dome at sunrise

S Webcam

N Webcam

S Sky
Temperature
1.4 °C
Humidity
87%
Wind
0.0 km/h
Pressure
1007.1 hPa

Moon
Latest preprints on astro-ph:
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GenASiS: General Astrophysical Simulation System. II. Self-gravitating Baryonic Matter ›
Formation and Evolution of Antimatter Objects ›
Non-Singular Bouncing cosmology from Phantom Scalar-Gauss-Bonnet Coupling: Reconstruction with Observational Insights ›
Saturn's Evolutionary History and Seismology: Survival of Deep Stably Stratified Regions in Evolutionary Models of Saturn Consistent with Ring Seismology ›
Gravitational-Wave Signals for Supernova Explosions of Three-Dimensional Progenitors ›
WLM: Dynamics of an isolated Dwarf Irregular Galaxy Under Ram Pressure in the Local Group ›
Radiation-hydrodynamics of star-disc collisions for quasi-periodic eruptions ›
The Rhythm of the ISM: Tracing the Timescales of Gas Evolution and Star Formation across Galactic Environments ›
Cosmic CO and [CII] backgrounds and the fueling of star formation over 12 Gyr ›
The Electromagnetically Isolated Global Signal Estimation Platform (EIGSEP) ›
IRS 9: The Case for a Dynamically-Ejected Star from the Galactic Center ›
Probabilistic inference in very large universes ›
Structure and Evolution of Multi-Cluster within Galactic Disc: Gaia DR3 Insights into Eight Open Clusters ›
White Dwarf Merger Remnants with Cooling Delays on the Q Branch Lack Strong Magnetism ›
Lightcurve Modelling of 2,205 ZTF DR2 Type~Ia Supernovae: Implications for SN Ia Physics and Cosmology ›
An infrared echo from a circumstellar disk in the hydrogen- and helium-poor SN 2024aecx ›
Overview of The SDSS-V Magellanic Genesis Survey ›
Degeneracies and modelling choices in double-plane time-delay cosmography ›
Visual inspection of potential exocomet transits identified through machine learning and statistical methods ›
Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation ›
Search for Faint Lone Double-Peaked H$\alpha$ Lines as IMBH Signatures in the MUSE Deep Field ›
Imaging Venus-like Worlds: Spectral, Polarimetric, and UV Diagnostics for the Habitable Worlds Observatory ›
Cyclotron lines in subcritical X-ray pulsars: Monte Carlo simulations reveal the origin of the observed variability ›
Time Lag between Accretion and Wind Events in the T Tauri Star RY Tau ›
Probing The Dark Matter Halo of High-redshift Quasar from Wide-Field Clustering Analysis ›
Molecular Gas Morphological Analogues for the Milky Way ›
The approximate gravitational lensing multiple plane mass sheet degeneracy ›
Unraveling the Brown Dwarf Desert: Four New Discoveries and a Unifying, Period-Coded Picture ›
Serial Charge Transfer Efficiency in ACS/WFC ›
Ultra-hot Jupiter atmospheres at high spectral resolution ›
Ca ii 854.2 nm in an enhanced network region simulated with MURaM-ChE ›
Probing beyond the Standard Model with gravitational waves from phase transitions ›
Validating the Angular Sizes of Red Clump Stars with Intensity Interferometry ›
Resolving the Tachocline using Inversion of Rotational Splitting Derived from Fitting Very Long and Long Time Series ›
ExoDNN: Boosting exoplanet detection with artificial intelligence. Application to Gaia Data Release 3 ›
Investigating particle acceleration in the Wolf-Rayet bubble NGC 2359 ›
Inferring Interstellar Medium Density, Temperature, and Metallicity from Turbulent H II Regions ›
FORGE'd in the Early Universe: The Effect of Protostellar Outflows on Pop III Accretion ›
Line-Intensity Mapping ›
Subaru/HSC NB395 view of NGC 5466: metallicity, mass function, and the nature of its tidal stream ›
From Grism to IFU: Revising the Redshift and Nature of the Massive Dusty Galaxy S1 with JWST and ALMA ›
How Distance Affects GRB Prompt Emission Measurements ›
Long-term timing evolution of four Anomalous X-Ray Pulsars ›
The orbital parameters of gamma-ray binary PSR~J2032+4127 ›
The SAMI Galaxy Survey: Quenching of Star Formation in Clusters III. Ram-Pressure-Affected Galaxy Populations ›
Evidence for a 3.0$\sigma$ Deviation in Gravitational Light Deflection from General Relativity at Cosmological Scales with KiDS-Legacy and CMB Lensing ›
Digging into the chemical complexity in the outer Galaxy: A hot molecular core in Sharpless 2-283 ›
Periodic 6.7 GHz $\mathrm{CH_3OH}$ maser emission in G353.273+0.641: First candidate for a pulsating high-mass protostar ›
A surprisingly large asymmetric ejection from Mira A ›
SQUIDPOL: Seoul National University QUadruple Imaging Device for POLarimetry ›
Convolutional Neural Networks for classifying galaxy mergers: Can faint tidal features aid in classifying mergers? ›
Seeing Wiggles without Seeing Wiggles: BAO Recovery in 21 cm Intensity Mapping with Deep Learning ›
Emulating galaxy and peculiar velocity clustering on non-linear scales ›
The asymmetric structure of the inner disc around HD 142527 A with VLTI/MATISSE ›
Unlocking the dynamics of Young Stellar Objects: Time-Domain Interferometry with six 4-m class telescopes ›
The ESO SupJup Survey IX: Isotopic evidence of a recent formation for Luhman 16AB ›
SN 2024igg: A Super-Chandrasekhar/03fg-like SN exhibiting C II-dominated spectra after explosion ›
Surface Density of Disk Galaxies in MOND ›
Atmospheric characterization of HIP 67522 b with VLT/CRIRES+. VLT/CRIRES+ suggests a heavier planet and hints at deuterium fractionation ›
Similarities and differences between solar and stellar flare pulsation processes ›
Shells and bubbles around compact clusters of massive stars: 3D MHD simulations ›
Kinematic Signatures in the Stellar Halo from Cosmological Encounters between the Milky Way and its Clouds ›
Post-impulsive millimeter emission of the 2022-05-04 solar flare ›
Euclid. Properties and performance of the NISP signal estimator ›
Narrow absorption lines from intervening material in supernovae: III. Supernovae and their environments ›
On the Influence of Pluto on Twotino Dynamics Through Their Mutual 4:3 Mean Motion Resonance ›
A Method for Thermal Radiation Transport Using Backward Characteristic Tracing ›
A case for Case A: detailed look at binary black hole formation through stable mass transfer ›
Light-Curve and Spectral Properties of Type II Supernovae from the ATLAS survey ›
The Tarantula Massive Binary Monitoring VII. On the nature of the eccentric O+BH binary candidate VFTS 812 ›
Broadband infrared spectroscopy of methanol isotopologues in pure, H2O-rich, and CO-rich ice analogues ›
Architectures of Planetary Systems II: Trends with Host Star Mass and Metallicity ›
Probing Atmospheric Escape Through the Near-Infrared Helium Triplet ›
JWST imaging of the Pleiades: anisotropy of turbulence in the cold neutral medium ›
Constraining cosmological simulations with peculiar velocities: a forward-modeling approach ›
Observational imprints of tidal internal gravity wave dissipation in star-planet systems ›
Temporal variations of solar inertial mode parameters from GONG (2002--2024) and HMI (2010--2024): Rossby modes ($3 \leq m \leq 16 $) and $m=1$ high-latitude mode ›
Star Grazing with Alumina Grass: Antireflection coatings in the visible and near-infrared on IPX-Clear Microlenses assisted by Grass-like Alumina ›
An Open Database of Lunar Regolith and Simulants Properties ›
JWST Discovery of High-Velocity Mid-Infrared Ionized Outflows in Ultraluminous Infrared Galaxies F11119+3257 and F05189-2524 ›
Modified Teleparallel $f(T)$ Gravity, DESI BAO and the $H_0$ Tension ›
Unifying the dynamical classification of early-type galaxies: kinematic deficits in IllustrisTNG versus observations ›
The FLAMINGO Project: Exploring the X-ray--cosmic-shear cross-correlation as a probe of large-scale structure ›
Scale-Invariant Bounce Cosmology in Weyl f(Q) Gravity with Quintom Signature ›
Observational signatures of charged Bardeen black holes in perfect fluid dark matter with a cloud of strings ›
Probing the Charged Hayward Black Hole in Dark Matter and String Cloud Environments through Shadow, Geodesics, and Quasinormal Spectrum ›
The emergent Big Bang scenario ›
The favoured twin: on the dynamical response of twin stars to perturbations ›
The ubiquitous flavor pendulum ›
Consistent Evaluation of the No-Boundary Proposal ›
Cosmological phase transitions: from particle physics to gravitational waves, semi-analytically ›
Direct power spectral density estimation from structure functions without Fourier transforms ›
Exploring Hyperon Skyrme Forces in Multi-$\Lambda$ Hypernuclei and Neutron Star Matter ›
Generation and Expansion-Driven Growth of Switchbacks in the Outer Solar Corona and Solar Wind ›
Deep-Learning Denoising of Radio Observations for Ultra-High-Energy Cosmic-Ray Detection ›
Cosmological Correlator Discontinuities from Scattering Amplitudes ›
Exploring the Origin and Dynamics of Solar Magnetic Fields ›
Compact object of HESS J1731-347 and its implication on neutron star matter ›
Large scale structure prior knowledge in the dark siren method ›
Mapping the Orbital Landscape of Perturbing Planet Solutions for Single-Planet Systems with TTVs ›
Dark Energy Survey: implications for cosmological expansion models from the final DES Baryon Acoustic Oscillation and Supernova data ›
Little red dots as young supermassive black holes in dense ionized cocoons ›
Die Hard: The On-Off-Cycle of Galaxies on the Star Formation Main Sequence ›
New Constraints on Dark Photon Dark Matter with a Millimeter-Wave Dielectric Haloscope ›
Photometry and Spectroscopy of SN 2024pxl: A Luminosity Link Among Type Iax Supernovae ›
Power law $\alpha$-Starobinsky inflation ›
A Systematic Search for Big Dippers in ASAS-SN ›
Cosmological Zoom-In Simulation of Odd Radio Circles as Merger-Driven Shocks in Galaxy Groups ›
$\nu p$-process in Core-Collapse Supernovae: Imprints of General Relativistic Effects ›
Inside-Out Planet Formation. VIII. Onset of Planet Formation and the Transition Disk Phase ›
Prospects for Deep-Learning-Based Mass Reconstruction of Ultra-High-Energy Cosmic Rays using Simulated Air-Shower Profiles ›
The Connection between Dusty Star-Forming Galaxies and the First Massive Quenched Galaxies ›
Gravitational-Wave Signatures of Highly Eccentric Stellar-Mass Binary Black Holes in Galactic Nuclei ›
Anomalous scattering of pulsars towards the Gum Nebula ›
The impact of superradiance on the spin evolution of variably accreting massive black holes ›
Illuminating gravitational wave sources with Sgr A* flares ›
Blazar PKS 0446+11 -- Neutrino connection study using a lepto-hadronic model ›
Extending the Frontier of Spatially-Resolved Supermassive Black Hole Mass Measurements to at $1\lesssim z\lesssim2$: Simulations with ELT/MICADO High-Resolution Mass Models and HARMONI Integral-Field Stellar Kinematics ›
Planet Migration in Protoplanetary Disks with Rims ›
Solitary Alfv\'en Waves ›
A Persistently Active Fast Radio Burst source Embedded in an Expanding Supernova Remnant ›
The GLEAM 4-Jy (G4Jy) Sample: III. Further host-galaxy identification, and redshift assessment ›
A Spatially Resolved Evolutionary Sequence of Multi-wavelength AGN Host Galaxies ›
DAO: A New and Public Non-Relativistic Reflection Model ›
Projected sensitivity of CTAO to axion-like particles from blazars with a machine learning approach ›
New and updated timing models for seven young energetic X-ray pulsars, including the Big Glitcher PSR J0537-6910 ›
Jet-torus interaction revealed by sub-parsec SO absorption in NGC 1052 ›
Accretion flow around Kerr metric in the infra-red limit of asymptotically safe gravity ›
Dynamical mass of a solar-like oscillator at the main-sequence turnoff from Gaia astrometry & ground-based spectroscopy ›
Neutron star cooling implications and magnetic field of the Vela Junior central compact object from all XMM-Newton and Chandra spectra ›
Hubble Tension as an Effect of Horizon Entanglement Nonequilibrium ›
How well is the local Large Scale Structure of the Universe known? CosmicFlows vs. Biteau's Galaxy Catalog with Cloning ›
Critical Evaluation of Studies Alleging Evidence for Technosignatures in the POSS1-E Photographic Plates ›
Isotropic Equivalence of STVG--MOG and $\Lambda$CDM and Its Breakdown in Large--Scale Anisotropic Cosmological Observables ›
MARVELously Dark: the gravothermal evolution of dwarf halos in velocity-dependent SIDM ›
Challenges and Opportunities of Gravitational Wave Searches above 10 kHz ›
Probing displaced (dark)photons from low reheating freeze-in at the LHC ›
Fuzzy dark matter soliton as gravitational lens ›
Emergent Turbulence in Nonlinear Gravity ›
Noninflationary solution to the monopole problem ›
Nonmodal growth and optimal perturbations in magnetohydrodynamic shear flows ›
A quantum information method for early universe with non-trivial sound speed ›
Emission of Nambu-Goldstone bosons from the semilocal string network ›
The Gravitational Wave Memory from Binary Neutron Star Mergers ›
Phase space analysis of an exponential model in $f(Q)$ gravity including linear dark-sector interactions ›
Enhancing online estimation of CBC parameters with the low-latency MBTA analysis ↓↑