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 from north-east

S Webcam

N Webcam

S Sky
Temperature
8.3 °C
Humidity
54%
Wind
0.0 km/h
Pressure
1015.0 hPa

Moon
Latest preprints on astro-ph:
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Cosmological constraints from the DESI DR1 joint power spectrum and bispectrum analysis ›
Survival of the most compact: the life and death of satellite halos in self-interacting dark matter ›
Revisiting the Milky Way stellar long bar and the 3 kpc arm ›
Impact of subhalo dynamical friction heating on the formation of the first structures in the universe ›
A Planetary Illusion's Funeral: Non-detection of a Gaia DR3 Exoplanet Candidate, and the Role of Intermediate-precision Radial Velocities in Gaia Exoplanet Follow-up ›
Flux-Averaged Force Multipliers ›
Archaeology of Galactic Nuclei Activity ›
The Journey to Dominance: How BCGs Evolve Differently from Other Massive Galaxies ›
The Vera C. Rubin Observatory Prompt Processing System ›
COSMOS-3D: Black Hole Mass Estimators and Luminosity Functions of Paschen-line AGNs ›
SpecZoo: An AI-Powered Platform for Spectral Analysis and Visualization in Science and Education ›
Expected evolution of the binary system ATLAS J1138-5139 ›
Furax: A Modular JAX Framework for Linear Operators in Astrophysical and Cosmological Data Analysis ›
A Concept of Next-Generation Atmospheric Cherenkov Telescope Array (NG-ACTA) ›
Precise parameter determination of the open cluster NGC 1647 via asteroseismology of p-mode pulsators ›
HAWC Study on the Ultra-High-Energy Gamma-Ray Emissions from the Pulsar Wind Nebula G32.64+0.53 ›
Morphological Signatures of Gravitational Evolution, Redshift-Space Distortions, and Massive Neutrinos in Large-Scale Structure ›
The radial velocity stability for reference sources in the MWISP CO survey ›
The FAST Galactic Plane Pulsar Snapshot Survey. IX. Timing Three Binary Pulsars with Wide Orbits and Low Orbital Eccentricities ›
Smoothed Particle Hydrodynamics in pkdgrav3 for Shock Physics Simulations. II. Shear Strength ›
FATHOMER survey: III. Preliminary HI galaxy identification results ›
Three outstanding physical questions for K2-18 b and other temperate sub-Neptunes ›
The dusty envelopes of asymptotic giant branch stars with ultraviolet excesses ›
Recovery of 21 cm BAO: a configuration-space correlation function analysis ›
The characteristics of variability of AGNs based on the structure function ›
Modeling Quasar Photo-$z$ Distribution and Uncertainty. A Study Based on the Kilo-Degree Survey ›
Constraints on the $^{12}$C$(\alpha, \gamma)^{16}$O and $^{16}$O+$^{16}$O Reaction Rates from Binary Black Holes Detected via Gravitational Wave Signals ›
A Complete X-ray View of Supernova Remnant W28 with Einstein Probe: Spatial Distribution of Parameters and Origin of the Thermal-Composite Morphology ›
VHE gamma-ray intranight variability from BL Lacertae during the extreme flaring state of 2022 ›
On the cosmology dependence of the cluster weak-lensing mass bias ›
High-energy neutrino flux from SN2024ggi: constraints from semi-analytic modeling of its post-explosive emission ›
Connection-angle dependence of proton anisotropy in ground-level enhancement events ›
Observations of Exocomets ›
The Arc in the DX Cha Circumbinary System: Evidence For a Retrograde Circumbinary Disk ›
High-resolution mid-IR spectroscopy of SVS 13-A with EXES/SOFIA: The surprisingly high CH$_3$OH/H$_2$O ratio in the planet-forming zone of a solar mass protostar ›
Monte Carlo conformal prediction for quantifying uncertainty in radio galaxy classification under ambiguous ground truth ›
Three-body Mean Motion Resonance Chains as a Delivery Mechanism for White Dwarf Pollution ›
Unveiling large-scale rotational motions in the intragroup medium at z~1 through gravitational-arc tomography ›
Retrieving the Red Edge on Earth-like Planets with Heterogeneous Clouds and Surfaces ›
A Century of Radial Velocity and Astrometric Monitoring of 70 Oph AB: New PFS Data and Constraints on Planetary Companions ›
Evidence of Long-Lived Powerful Gyrosynchrotron Radio Emission in the Close Binary FF UMa ›
Early emission characterization of TDE2025aarm ›
Numerically stable equations for the orbital evolution of compact object binaries ›
Theory of optical long-baseline interferometry on polarized sources ›
A New Multi-Constraint Potential Field Source Surface (PFSS) Extrapolation Model ›
Cosmological forecast from the full-sky angular power spectrum and bispectrum of 21cm intensity mapping ›
SPT-3G D1: Maps of the millimeter-wave sky from 2019 and 2020 observations of the SPT-3G Main field ›
VINTERGATAN-GM: long-lived satellite planes induced by a massive GSE-like merger ›
Improved constraint on the Hubble constant from dark sirens with LIGO/Virgo/KAGRA O4a ›
Galaxy sizes as complementary (zero-)bias tracers of local primordial non-Gaussianity ›
New Constraints on the Jovian Narrowband Radio Components from Juno/Waves Observations and 3D Geometrical Simulations ›
Toward universal coalescence models for antideuteron production ›
Recursive Penrose processes in electrically charged black hole spacetimes: Backreaction and energy extraction ›
Cosmology and modified GW propagation from the BNS mass function at third-generation detector networks ›
Observational imprints and quasi-Periodic oscillations of magnetically charged anti-de Sitter black holes ›
Vector-channel scattering of dark particles in a Sp(4) gauge theory ›
On the Universal Cuspy Behavior in Black Hole Shadows ›
Casimir-Induced Quintessence in Dark Dimension ›
A dual description of quarks and baryons: Quarkyonic matter within a relativistic quark model ›
Can QCD Axions Survive the Cosmological Constant Problem? ›
Cislunar State and Uncertainty Propagation via the Modified Generalized Equinoctial Orbital Elements ›
Reheating in runaway inflation models via the evaporation of mini primordial black holes ›
Reconstructing the whole 6D properties of the Sagittarius stream with N-body simulations ›
LISA and $\gamma$-ray telescopes as multi-messenger probes of a first-order cosmological phase transition ›
Physics of 1 keV line in X-ray binaries ›
An ancient system hidden in the Galactic plane? ›
Modeling the Spectral Energy Distribution of Active Galactic Nuclei: Implications for Cosmological Simulations of Galaxy Formation ›
Hard X-ray/Soft gamma-ray Laue Lenses for High Energy Astrophysics ›
The impact of new ($\alpha$, n) reaction rates on the weak s-process in metal-poor massive stars ›
Accurately simulating core-collapse self-interacting dark matter halos ›
Comparing LambdaCDM, wCDM, and w0waCDM models with DESI DR2 BAO: Redshift-Resolved Diagnostics and the Role of rd ›
Application of interpretable data-driven methods for the reconstruction of supernova neutrino energy spectra following fast neutrino flavor conversions ›
SPARCS -- combining radiation hydrodynamics with non-equilibrium metal chemistry in the SWIFT astrophysical code ›
The Yasone catalogue: three new Milky Way satellites and 17 further hypercompact candidates ›
The Hidden Life of Stars: Embedded Beginnings to AGB Endings in the PHANGS-JWST Sample. I. Catalog of Mid-IR Sources ›
A first look at quasar-galaxy clustering at $z\simeq7.3$ ›
Eternal inflation bubble collision signature on CMB remote dipole and quadrupole fields ›
J-PAS: forecast on the primordial power spectrum reconstruction ›
Galactic foreground residue biases in cosmic-microwave-background lensing-convergence reconstruction and delensing of B-mode maps ›
Caustic crossings in giant arcs with extended dark matter objects ›
The Intermediate Mass Black Hole in Omega Centauri: Constraints on Accretion from JWST ›
Detection of the Pairwise Kinematic Sunyaev-Zel'dovich Effect and Pairwise Velocity with DESI DR1 Galaxies and ACT DR6 and Planck CMB Data ›
COSMOS-3D: Dense Circumnuclear Gas across Black Hole Growth Phases at z ~ 3 ›
Extended Wess-Zumino Dark Radiation Model with Interacting Scalar Field Dark Matter and Stepped Dark Radiation ›
OutLines: Modeling Spectral Lines from Winds, Bubbles, and Outflows ›
From emission to absorption: the FAST observation of the OH 18-cm lines from the Comet C2025/A6 ›
CMB anisotropies from cosmic (super)strings in light of ACT DR6 ›
A 2% determination of $N_{\rm eff}$ from primordial element abundance, cosmic microwave background, and baryon acoustic oscillation measurements ›
Cosmological peculiar velocities in general relativity ›
Emulation of SPHEREx Galaxy Power Spectra I: Neural Network Details and Optimization ›
A Minimal Four-Thruster System for Comet-Based Interstellar Navigation ›
Trajectory Stability and Signature Diagnostics for Comet-Based Interstellar Navigation ›
ID-MAGE II: The Star Forming Satellites of Low-Mass Hosts ›
G objects as Primordial Black Hole-Neutron Star Remnants: Population Modeling and Multi-Wavelength Observables ›
Quantum Damping of Cosmological Shear: A New Prediction from Loop Quantum Cosmologies ›
Scalar-Mediated Inelastic Dark Matter as a Solution to Small-Scale Structure Anomalies ›
Cosmic Rays as an Interdisciplinary Earth Observation Tool: From Particle Physics and Atmospheric Processes to Geosciences and Urban Science ›
Axions on a Hyperbolic Ride: Geometric Suppression of CMB Isocurvature and a Blue-Tilted Spectrum ›
Modified Teleparallel $f(T)$ Gravity, DESI BAO and the $H_0$ Tension ›
Cosmological Spacetimes with Sign-Changing Spatial Curvature and Topological Transitions ›
Multi-Field Dilaton Screening Beyond the Thin-Shell Mechanism ↓↑