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

View to the south-west

S Webcam

N Webcam

S Sky
Temperature
9.6 °C
Humidity
61%
Wind
0.0 km/h
Pressure
1025.5 hPa

Moon
Latest preprints on astro-ph:
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Beyond Cloud-9: The case for discovering more HI-rich failed halos ›
The First Empirical Calibration of the MIR Abundance Diagnostic Ne$_{23}$ with JWST ›
Coupling between stellar and HI lopsidedness in Milky Way-type galaxies from the Auriga Superstars cosmological simulations ›
Unveiling the dynamics of the ultra-fast outflow in IRAS 13224-3809 with X-ray spectroscopy ›
Searching for GEMS: Three warm Saturns and a super-Jupiter orbiting four early M-dwarfs ›
Dwarf Galaxies Hosting Extreme Star-Forming Regions and (Variable) AGNs at Radio Wavelengths ›
SPYGLASS. VII-B. Tracing the Fragments of Massive Star Formation Using Low-Mass Associations ›
Chaotic Molecular Gas in Five Dusty Star-forming Galaxies in the Spiderweb Protocluster at $z = 2.16$ ›
A high-resolution K-band spectral atlas of massive stars ›
Characterizing six seismic solar analogs observed by Kepler, K2, and HERMES ›
Galaxy Zoo Bar Lengths: A Catalogue of Measurements from Hubble Space Telescope Images and the Evolution of Galactic Bar Structure at z < 1 ›
Geodesically Complete Curvature-Bounce Inflation ›
The A Supergiant Eclipsing Binary BM Cas: An Evolved, Intermediate Mass System ›
Dust cloud lifetimes of Scallop-shell stars ›
uGMRT and MeerKAT observation of RXCJ0232-4420: a quiet cluster with a giant radio halo ›
CORINOS V: Radiative transfer effects in protostellar ice observations ›
Molecular Outflows in the Nucleus of the Nearby Compton-thick AGN NGC 3079 ›
The major cluster merger in Abell 2034 as seen by XRISM: Strong turbulence and spectral anomalies? ›
Six New Variable Stars Discovered from Ground-Based Photometry and Characterized with TESS Data ›
Formation and Trapping of CO2 from Cryogenic Irradiation of Carbonate ›
Iron He-triplet signatures of shocks in the hottest galaxy clusters. Z/W line ratio, line broadening, and electron-ion temperature equilibration ›
Multi-messenger emission from choked jets in collapsar ›
Turbulence and Star Formation Suppression in Elliptical Galaxies: The Role of Active Galactic Nucleus Jet Wind Interaction ›
Extended Universal Rotational Curve of Spiral Galaxies ›
Active Galactic Nucleus Feedback in an Elliptical Galaxy. IV. The Importance of the Jet Wind Coupling ›
Star cluster formation from turbulent clumps. V. Stellar clustering around massive stars ›
The Solar System Notification Alert Processing System (SNAPS): Public access to SNAPS data and products ›
A benchmark for binary star interaction with a supermassive black hole in general relativity ›
Indication of gamma-Ray Quasi-periodicity in GB6 J1037+5711 from Multi-technique Timing Analysis ›
Foreground Mitigation and Power Spectrum Analysis for Tianlai Full-Sky 21 cm Survey Observation ›
The Critical Mass in Galaxy Evolution ›
First Detection of Faraday Rotation in a Gamma-Ray Burst Afterglow: Low Polarization and High Rotation Measure in GRB 260310A Reveal Jet Magnetic Structure and Environment ›
Primordial black hole dark matter from axion inflation ›
X-Ray Spectral Variability of the TeV HBL Blazar PG 1553+113 with XMM-Newton ›
Detection of optical quasi-periodic oscillation in the blazar 3C 454.3 ›
Finding Strongly Lensed Supernovae from Blended Light Curves ›
Thermal instability and rocky planetesimal formation in the inner regions of protoplanetary disks ›
Dense cores and filaments in M16: Enhanced formation efficiency in the stellar feedback-driven shell ›
An Extended Evaluation Split for DeepSpaceYoloDataset ›
Diffuse Gamma-ray Emission Around 4FGL J1626.0-4917 ›
Eclipsing time variations in close binaries produced by azimuthal dynamo waves ›
On the Difference Between Pulsar Radio Emission Beams from the Two Poles ›
Blazar flares from plasma blobs crossing the broad-line region ›
Probing dust properties through polarized scattered-light images of a sample of ring-shaped protoplanetary disks ›
Long-term study of the gamma-ray emission of Cygnus X-3 with MAGIC and Fermi-LAT ›
Radio signal generation in milliseconds: enabling multi-parameter reconstruction of ultra-high-energy cosmic rays ›
A Cosmological Uncertainty Relation and Late-Universe Acceleration ›
Robust AGN and host-galaxy decomposition in optical spectral fitting ›
TESS Asteroseismology of Red Giants in the Old Metal-Rich Open Clusters NGC 188 & NGC 6791 ›
Asteroseismic modelling of main-sequence solar-like stars and Kepler exoplanet host stars with the FICO procedure I. Catalogue of fundamental stellar properties ›
Anisotropy of Satellite Galaxies-I: Contrasting Correlations with Central Galaxy, Host Halo, and Large-Scale Filament Structures ›
Cosmological Observational Tests in the JWST Era. II: The Tolman Test ›
Probing the $\gamma$-ray Emission Origin of Two Star-forming Galaxies NGC 2403 and NGC 3424 with the Fermi-LAT ›
A New Perspective on Galactic Evolution: Studying the Outskirts of the Abell S1063 Galaxy Cluster ›
The Complex Structure of the Abell 548 - Abell 3367 Region ›
The Large Array Survey Telescope-Pipeline. II. Image Subtraction and Transient Detection ›
Pulsation-driven helium transport as a potential source of the Blazhko effect ›
Axion dark matter from extended misalignment with a constant-$\omega_\phi$ pre-oscillatory phase and dark radiation ›
Applications of 1.4 GHz diagnostics to Type Ia Supernova host galaxies ›
A common four-beam geometry reveals altitude-stratified GeV pulses in canonical young pulsars ›
On the polarization position angle jumps in FRB 20240114A ›
Cosmological intercept tension ›
The faint voice of a radio-weak BL Lacertae: modeling the broadband emission of WISE~J141046.00+740511.2 ›
Finding the one: identifying the host of compact binary mergers ›
The Influences of Hydrogen-Silicate-Iron Miscibility on the Demographics of Sub-Neptunes and Super-Earths ›
Chemical Taxonomy of $\omega$~Centauri: Ten Populations Reveal a Multi-Phase Enrichment History ›
The intrinsic dispersion of elemental abundance ratios in nearby metal-poor halo stars ›
Chiral-Transport-Induced Collective Modes in Strong Magnetic Fields and Their Implications for Neutron Star Phenomenology ›
Compressible Navier--Stokes Flow in Schr\"odinger-Type Variables ›
Agnostically decoding gravitational wave model deficiencies in GWTC-3 ›
Stable but Wrong: An Inference Limit in Galactic Archaeology ›
Gravitational wave constraints on the Paneitz operator ›
Theoretical and Experimental Constraints in the $\mu$--$\tau$ Four-Lepton Sector of the SMEFT: implications to neutrino self interactions ›
Stochastic Axion Mixing: A General Mechanism Beyond Decay Constant Constraints ›
Rotation-Induced Pressure Anisotropy in Newtonian White Dwarfs: Sequences and Applicability Criteria ›
Semi-analytic bounds on axion-like-particle supernovae emission ›
New gravitational-wave templates for metastable cosmic strings: Loop breaking versus network collapse ›
Beyond the Separatrix: Analytic Continuation of Darwin Variables for Plunging Geodesics in Schwarzschild Spacetime ›
Cosmology with Cosmic Voids ›
Reconciling Nonminimally Coupled Higgs Inflation with ACT DR6 Observations through Reheating ›
3C403: a candidate neutrino-emitting radio galaxy ›
The first radio view of a type Ibn supernova in SN 2023fyq: Understanding the mass-loss history in the last decade before the explosion ›
Supernovae drive large-scale, incompressible turbulence through small-scale instabilities ›
CosmoGen: A genetic algorithm framework for the exploration of dark energy dynamics ›
Adaptive Reconstruction of Cluster Halos (ARCH): Integrating Shear and Flexion for Substructure Detection ›
Is the Peculiar Galactic Center Transient Swift J174610.4-290018 A Nova Outburst? ›
QML-FAST -- A Fast Code for low-$\ell$ Tomographic Maximum Likelihood Power Spectrum Estimation ›
Archival Inference for Eccentric Stellar-Mass Binary Black Holes in Space-Based Gravitational Wave Observations ›
Acceleration of Ultrahigh Energy Particles from Fast Radio Bursts ›
Niebla: an open-source code for modeling the extragalactic background light ›
Hot accretion onto spiral galaxies: the origin of extended and warped HI discs ›
Charge-dependent spectral softenings of primary cosmic-rays below the knee ›
Cosmic Shear constraints from HSC Year 3 with clustering calibration of the tomographic redshift distributions from DESI ›
The stellar and dark matter distributions in early-type galaxies measured by stacked weak gravitational lensing ›
On the gravitational stratification of multi-fluid-multi-species plasma ›
Template-free search for gravitational wave events using coincident anomaly detection ›
A Response to paper Critical Evaluation of Studies Alleging Evidence for Technosignatures in the POSS1-E Photographic Plates by Watters et al. (2026) ›
NASA's Pandora SmallSat Mission: Simulating the Impact of Stellar Photospheric Heterogeneity and Its Correction ›
Broadband Searches for Extraterrestrial Technological Intelligence: a New Strategy To Find Nearby Alien Civilizations ›
Post-perihelion Coma Composition of the Interstellar Comet 3I/ATLAS from Optical Spectroscopy ›
Signatures of Reconnection and a Split Heliospheric Tail in High-Energy Energetic Neutral Atoms ›
G objects as Primordial Black Hole-Neutron Star Remnants: Population Modeling and Multi-Wavelength Observables ›
Observations of DNC and DCO$^+$ toward the $\int$-shaped Filament and Starless Cores in the Orion Molecular Clouds ›
Low-mass Active Galaxies in the SAMI Galaxy Survey with Spatially-resolved Spectroscopy ›
Second-Generation Mass Peak in the Gravitational-Wave Population as a Probe of Globular Clusters ›
Chemistry and ro-vibrational excitation of CH$^+$ in the planetary nebula NGC 7027 ›
Stellar feedback SPICEs up [C II] emission in the first galaxies ›
Formalizing Galaxy Population Evolution: Drift and Mergers as Transport Processes on Manifolds ›
SCAT Data Release 1: 1810 optical spectra of 1330 transients ›
Massive black holes and their galaxies ›
Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos ›
Blueberry and Green Pea galaxies live in low density environments ›
The IACOB project: XVII. Nitrogen abundances in Galactic O-type stars: further hints for separating binary-interaction products from effectively single stars ›
Enhancing Early Detection and Localization of Gravitational Waves via Eccentricity-Induced Higher Harmonic Modes with 2G Detector Networks ›
Inverting no-hair theorems: How requiring General Relativity solutions restricts scalar-tensor theories ›
Axions as Dark Matter, Dark Energy, and Dark Radiation ›
Chiral effects and Joule heating in hot and dense matter ›
Photon counting readout for detection and inference of gravitational waves from neutron star merger remnants ›
A Nonlocal Realization of MOND that Interpolates from Cosmology to Gravitationally Bound Systems ›
Massive boson stars: Stability and GW emission in head-on mergers ›
Fermion Thermal Field Theory for a Rotating Plasma (with Applications to Neutron Stars) ›
Anisotropic dispersion relation of ultralight Bose gases in modified Newtonian dynamics ›
Constraints on Primordial Black Holes from Galactic Diffuse Synchrotron Emissions ›
Warm dark matter from freeze-in at stronger coupling ›
Infrared Spectral Gap in a Gluonic Dark Sector as the Origin of the Galactic Acceleration Scale ›
Boson star-black hole binaries: initial data and head-on collisions ›
Investigating the Neutrino Mass Ordering Problem via Ternary Plots ↓↑