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
-2.4 °C
Humidity
93%
Wind
4.8 km/h
Pressure
1020.3 hPa

Moon
Latest preprints on astro-ph:
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Geomagnetic storm suppression of photographic plate transient detections in the POSS-I archive: an independent physical variable strengthening the nuclear test correlation ›
FluxMC: Rapid and High-Fidelity Inference for Space-Based Gravitational-Wave Observations ›
The neighboring stars of N6946-BH1 and the observational characteristics of failed supernovae ›
Electromagnetic Flares from Compact-Object Mergers in AGN Disks: Signatures and Predictions ›
PANORAMIC: The Dawn of Massive Quiescent Galaxies I. Number Density and Cosmic Variance from 1000 arcmin$^2$ NIRCam Imaging ›
Winding Back the Clock: Recent Star Formation Histories of Massive Quiescent Galaxies Are Consistent With Their Rapid Number Density Evolution Since $\mathbf{z\sim7}$ ›
Characterizing the Gamma-ray Emission from Low-Luminosity AGN ›
Toward Early-type Eclipsing Binaries as Extragalactic Milestones: First Calibration of the SBCR from O- and B-type Stars in Detached Eclipsing Binaries ›
Universal Dark-matter Density Profiles of Cosmic Filaments ›
Two-stage disruption of resonant chains ›
Lithium and the evolution of intermediate-mass T Tauri and Herbig stars. Rotation, accretion, and planets ›
Wide Jets or Low Rates: Reconciling Short GRB and Gravitational-Wave Neutron Star Merger Rates ›
Super-Solar Metallicity and Tentative Evidence for Photochemistry on WASP-96b from JWST and Ground-Based VLT Transmission Spectroscopy ›
Photon-Count Statistics of Crab X-ray Pulses: Skellam Behavior and Excess Variance in the Main Pulse ›
Kinetic magnetohydrodynamics and Landau fluid closure in relativity ›
Implications of low neutron star merger rates for gamma-ray bursts, r-process production and Galactic double neutron stars ›
A New Method for Testing Einstein's Theory of Gravity Close to Rapidly Spinning Black Holes ›
Great Walls of Cosmic Baryons in the Northern Sky ›
A generic $\omega_b$ tension in early-time solutions to the Hubble tension ›
A Comprehensive Atmospheric Retrieval Analysis of 22 James Webb Space Telescope Spectral Energy Distributions of Cool Brown Dwarfs ›
Azimuthal Dust Polarization from Aerodynamically Aligned Grains as Evidence for the Streaming Instability in Protoplanetary Disks ›
Identification of a Radio Counterpart to SN 2025ulz in the S250818k Localization Area ›
Identifying signatures of inflow onto face-on galaxies using the Balmer decrement ›
SN2023ixf: Radiative-transfer modeling of the photospheric phase evolution from the ultraviolet to the infrared ›
Gas Giants Formed by Gravitational Instability May Accrete Atmospheres with Super-Stellar Carbon to Oxygen Ratios ›
Approximating the Fourier Transform of Ring-Like Images: the Focal Expansion ›
Local primordial non-Gaussianity using cross-correlations of DESI tracers ›
A Chemical Mismatch Between Young Stars and Their Inner Disks ›
The JWST Search for Earth-Luna Analogs: Upper Limits on Exomoons and Refined Ephemerides for TOI 700 d and e ›
JWST Lensed Quasar Dark Matter Survey V: Measuring the minimum halo mass with strong gravitational lensing ›
Constraints on the Injection of Radiation in the Early Universe ›
High-contrast imaging of Galactic Cepheids with VLT/SPHERE ›
Explaining Neural Networks on the Sky: Machine Learning Interpretability for Cosmic Microwave Background Maps ›
The Cluster Completeness Correction Calculator (C-4): A Neural-Network framework and pilot application to the LEGUS Survey of NGC 628 ›
Statistics of blob properties in two types of coronal streamers ›
Scientific Validation of the SPARC4 Pipeline: Multi-band Imaging, Polarimetry, and Photometric Time Series for Improved Characterization of Transiting Exoplanets ›
A Catalog of Mid-infrared Variable Sources in the Ecliptic Poles ›
Accurate polarization calibration of FAST spectral data for measurements of Zeeman splittings of OH megamasers in IRAS 02524+2046 ›
Adiabatic Mass Loss In Binary Stars. VI. Massive Helium Binary Stars ›
Detectability of continuous gravitational waves from planetary-mass companions orbiting compact stars ›
Reconstruction of fast-rotating neutron star observables with the neural network ›
The NANOGrav 15 yr and 20 yr Datasets: Timing Events and Pulse Shape Changes ›
Reconstructing a large-scale matter-density contrast profile to reconcile Pantheon+ supernovae with DESI DR2 BAO in an inhomogeneous universe ›
Galactic-scale evolution of classical and complex radio galaxies. Impact of ambient morphology and jet geometry ›
Multi-Quark Clustering in Neutron-Star Matter from Color-Spin Molecular Dynamics ›
One sightline, many systems: a FLASH discovery of HI towards scintillating quasar PKS 0405-385 ›
Searching for Contact Binaries with LAMOST and TESS ›
Remnant recoil and host environments of GWTC-4.0 binary black-hole mergers ›
WALLABY pilot survey: HI depletion times within the stellar discs of nearby galaxies ›
What can galaxy clustering really tell us about the galaxy-halo connections? ›
Investigation of Transit Timing and an Optical Transmission Spectrum of the Hot Jupiter WASP-11 b ›
Extreme Blazars Observed with MAGIC: Second Catalog Release ›
The Broken Similarity: Sinking and Merging of Dark Matter Subhalos Across Hierarchical Levels ›
Higher resolution optical spectra of $M_* ›
Stellar Population Characterisations in nearby, dusty Early-Type Galaxies ›
Non-LTE Ionization Modeling for Helium and Strontium in Neutron Star Merger Ejecta ›
Instrumental development for Cryogenic sub-Hz cROss torsion bar detector with quantum NOn-demolition Speed meter (CHRONOS) ›
Strontium and helium in the kilonova AT2017gfo: Origin of the 1{\mu}m feature constrained via NLTE calculations ›
Unveiling axion signals in galactic supernovae with future MeV telescopes ›
Model-independent constraints on generalized FLRW consistency relations with bootstrap-based symbolic regression ›
Forward analytical model for the optical selection bias on galaxy cluster lensing profiles ›
Diagnostic Consistency Tests of the Concordance Cosmology ›
Probing the Evolution of Dark Energy: A Joint Analysis of DESI DR2, Pantheon+, and Cosmic Chronometers ›
Comments on "The impact of Solar magnetic field configurations on the production of gamma rays at the Solar disk'' (arXiv:2512.01403) ›
Developing Pre-Supernova Neutrino Support for sntools ›
Study of the migration of Earth-like planets in planetesimal disks and the formation of debris disks ›
Testing X-ray Periodicity and Long-Term Trend in PG 1553+113 via Targeted Swift-XRT Monitoring ›
The Transit Timing and Transmission Spectrum of Hot Jupiter WASP-43 b from a decade of Multi-band Transit Follow-up Observations ›
An 18 - 25 GHz spectroscopic survey of southern hemisphere dense cores ›
Orbital inclination estimates for overcontact binaries using the derivatives of light curves ›
Testing parity with composite-field spectra of BOSS and DESI luminous red galaxies ›
The Cohesive Object Sequence: The Mass-Density Distribution of Astronomical Objects from Asteroids to Stars ›
cuRAMSES: Scalable AMR Optimizations for Large-Scale Cosmological Simulations ›
Lyman-$\alpha$ Forest Signatures of Mixed Fuzzy and Cold Dark Matter ›
Spectroscopic confirmation of dual and offset quasars from the Subaru HSC-SSP program ›
Star-planet magnetic interactions in photoevaporating exoplanets ›
Hunting Dark Matter with the Einstein Telescope ›
Investigating ACS/WFC Amp-to-Amp Sensitivities ›
On the observational distinguishability of the Kerr and Kerr-Hayward metrics to EHT ›
Deep Spectroscopy with DESI for Photometric Redshift Training and Calibration ›
Testing the 3-equation Kuhfuss Convection Model using the Sun ›
Focal plane wavefront control with model-based reinforcement learning ›
Effective stability estimates close to resonances with applications to rotational dynamics ›
Revisiting The Gravitational Mirroring In Presence of Compact Objects ›
Electroweak Doublet Dark Matter for a Galactic Halo Gamma-Ray Excess ›
Ion Weibel Instability in the hybrid framework: the optimal resolution ›
Gravitational Waves from Matter Perturbations of Spectator Scalar Fields ›
Cosmological collider signals of modular spontaneous CP breaking ›
Twisted doughnuts: Thick disk torus around equatorial asymmetric black hole ›
Modeling complex plasma instabilities in space plasmas - Three-component electron formalism of heat-flux instabilities ›
Valence and Rydberg excited state bond dissociation curves of CO2 from orbital-optimized density functional calculations ›
Noise budget of Cryogenic sub-Hz cROss torsion bar detector with quantum NOn-demolition Speed meter (CHRONOS) ›
JZ-Tree: GPU friendly neighbour search and friends-of-friends with dual tree walks in JAX plus CUDA ›
$\xi R\phi^2$ non-minimal coupling, and the long range gravitational potential for different spin fields from 2-2 scattering amplitudes ›
Posterior Predictive Checks for Gravitational-wave Populations: Limitations and Improvements ›
Massive Exchange and the Sign of the Equilateral Bispectrum ›
Effects of pair freeze-out on photon distributions in BBN epoch ›
Cosmological Simulations of Stellar Halos with Gaia Sausage-Enceladus Analogues: Two Sausages, One Bun? ›
Spectral Imaging with QUBIC: building frequency maps from Time-Ordered-Data using Bolometric Interferometry ›
Temporary EHBL-like behavior of Markarian 501 during July 2014 VHE flaring ›
Strong LensIng and Cluster Evolution (SLICE) with JWST: Early Results, Lens Models, and High-Redshift Detections ›
ACT-ing on inflation: Implications of non Bunch-Davies initial condition and reheating on single-field slow roll models ›
Eccentric millisecond pulsar + subdwarf B star from rotationally delayed accretion-induced-collapse scenario ›
Impact of initial mass function on the chemical evolution of high-redshift galaxies ›
Frabjous: Deep Learning Fast Radio Burst Morphologies ›
Testing Dark Matter with Generative Models for Extragalactic Stellar Streams ›
Impact of black hole spin on low-mass black hole-neutron star mergers ›
The Fraction of Clumpy Galaxies in JADES over $2 ›
Hillas meets Eddington: The case for blazars as ultra-high-energy neutrino sources ›
Fuzzy dark matter dynamical friction: stalling of globular clusters induced by dynamical heatings ›
Metallicity Gradients in Modern Cosmological Simulations II: The Role of Bursty Versus Smooth Feedback at High-Redshift ›
XSNAP: An X-ray Supernova Analysis Pipeline with Application to the Type II Supernova 2024ggi ›
Constraining interacting dark energy models with black hole superradiance ›
Absorption effects in the expanding Universe: spectral transmittance functions of intergalactic medium for distant sources ›
The DREAMS Project: Disentangling the Impact of Halo-to-Halo Variance and Baryonic Feedback on Milky Way Dark Matter Density Profiles ›
Optical polarimetry of the accreting black hole X-ray binary Swift J1727.8$-$1613 over the state transition and radio ejections ›
Tracking Protostellar Variability in Massive Protoclusters with ALMA: I. Insights from QUARKS and MaMMOtH ›
Cygnus X-3: A variable petaelectronvolt gamma-ray source ›
A Shocked Wind Interpretation of an Odd Radio Circle ›
Early Planet Formation in Embedded Disks (eDisk). XIX. Structures of molecular outflows ›
The Double-Peaked Calcium-Strong SN 2025coe: Progenitor Constraints from Early Interaction and Ejecta Asymmetries ›
HI-bearing dark galaxies predictions from constrained Local Group simulations: how many and where to find them ›
Accretion disc winds in X-ray binaries ›
VLBI Observations of SN 2012au Reveal a Compact Radio Source a Decade Post Explosion ›
Spectroscopic confirmation of a large and luminous galaxy with weak emission lines at $\mathbf{z = 13.53}$ ›
The long quest for vacuum birefringence in magnetars: 1E 1547.0-5408 and the elusive smoking gun ›
Statistical Predictions of the Accreted Stellar Halos around Milky Way-Like Galaxies ›
The Bondi universe: Can negative mass drive the cosmological expansion? ›
An Open-Source High-Level Graphical Signal Processing Language with Simulation and HDL Generation ›
NE2025: An Updated Electron Density Model for the Galactic Interstellar Medium ›
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 ›
FRB scattering statistics through the CGM are sensitive to morphology and intermittency ›
Active Galactic Nuclei-driven Metallicity Enrichment in the Interstellar Medium of Mrk 573 ›
Temporal Variation of the Coronal Radius Parameter in a Jetted Tidal Disruption Event: Swift J1644+57 ›
The diagnostic temperature discrepancy as evidence for non-Maxwellian coronal electrons ›
VHE gamma-ray intranight variability from BL Lacertae during the extreme flaring state of 2022 ›
ALMAGAL VIII. Early phases of triggered star formation in source AG286.0716$-$1.8229 ›
Exploring the interplay of late-time dynamical dark energy and new physics before recombination ›
STRADAViT: Towards a Foundational Model for Radio Astronomy through Self-Supervised Transfer ›
Spectroscopic Redshifts for 461 Euclid Q1 Strong Gravitational Lenses from NISP Slitless Spectroscopy ›
Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data? ›
Beyond $f(\phi)\mathcal{G}$: Gauss--Bonnet inflation with $\mu(\phi,X)$ ›
Random gas motions inside sub-parsec scale supercritical filaments ›
Resummation of Universal Tails in Gravitational Waveforms ›
Dark Matter Velocity Distributions for Direct Detection: Astrophysical Uncertainties are Smaller Than They Appear ›
5-Dimensional Gravitational Raman Scattering: Scalar Wave Perturbations in Schwarzschild-Tangherlini Spacetime ›
Teaching Astronomy with Large Language Models ›
Quantum corrections to symmetron fifth-force profiles ›
Detectability of axion-like dark matter for different time-delay interferometry combinations in space-based gravitational wave detectors ›
Evaporation of Primordial Black Holes in a Thermal Universe: A Thermofield Dynamics Approach ↓↑