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 south-west

S Webcam

N Webcam

S Sky
Temperature
14.3 °C
Humidity
74%
Wind
0.0 km/h
Pressure
1015.4 hPa

Moon
Latest preprints on astro-ph:
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Tera-Hertz Counterparts to Fast Radio Bursts from Coherent Cherenkov Radiation by Tilted Bunches ›
The End of the Road for Far-infrared Reddening Maps? Evidence for Reddening Errors Driven by Changes in PAH Abundance ›
A Panchromatic View of Late-time Shock Power in the Type II Supernova 2023ixf ›
Hot, cold, and multi-component accretion flows around supermassive black hole binaries ›
The Wrath of KAN: Enabling Fast, Accurate, and Transparent Emulation of the Global 21 cm Cosmology Signal ›
Theory of Exozodi Sources and Dust Evolution ›
Late-time Hubble Space Telescope Ultraviolet Spectra of SN 2023ixf and SN 2024ggi Show Ongoing Interaction with Circumstellar Material ›
Semi-analytic studies of accretion disk and magnetic field geometry in M87* ›
MINDS. Strong oxygen depletion in the inner regions of a very low-mass star disk? ›
Characterizing, correcting, and repairing the effects of radiation damage in the COSI germanium cross-strip detectors ›
Comparative Analysis of Two Astrometric Measuring Methods on Five Known Binaries ›
Where does non-Universality in Assembly Bias come from? ›
Frequentist Cosmological Constraints from Full-Shape Clustering Measurements in DESI DR1 ›
Serendipitous discovery of a young cluster of galaxies at $z \sim 0.5$ projected next to the nearby tadpole galaxy KUG 1138 + 327 ›
Blue supergiants in the Pinwheel Galaxy M101: comparison with H II region chemical abundances, spectroscopic distance and an independent determination of the Hubble constant ›
The Design and Performance Characteristics of the NRL4 ASIC Developed for the COSI Small Explorer Gamma-ray Satellite ›
The BSN Application-I: Photometric Light Curve Solutions of Contact Binary Systems ›
Dark Matter and the Early Formation of Supermassive Black Holes ›
Limitations in constraining neutron star radii and nuclear properties from inspiral gravitational wave detections ›
BSN-II: The First Light Curve Study of Eight Total Eclipsing Contact Binary Stars with Shallow Fillout Factors ›
Evidence for ultra-water-rich ammonia hydrates stabilized in icy exoplanetary mantles ›
Mapping feedback signatures in 3C 297: A quasar-host merger at Cosmic Noon ›
Rings around giant planets and smaller bodies ›
Machine learning-based classification of variable stars using phase-folded light curves ›
Bayesian Inference of Gravity through Realistic 3D Modeling of Wide Binary Orbits: General Algorithm and a Pilot Study with HARPS Radial Velocities ›
The origin of extreme N-emitters in star-forming galaxies at z$ ›
Mitigating point-source contamination in CMB polarization: a Generalized Point Spread Function fitting approach ›
Cosmology-informed Neural Networks to infer dark energy equation-of-state ›
Long term variability of Cygnus X-1. IX. A spectral-timing comparison of Cygnus X-1 and MAXI J1820+070 in the hard state ›
Examining AGN UV/Optical Variability Beyond the Simple Damped Random Walk. II. Insights from 22 Years Observations of SDSS, PS1 and ZTF ›
Scalable and robust wide-field facet calibration with LOFAR's longest baselines ›
Magnetars in Binaries as the Engine of Actively Repeating Fast Radio Bursts ›
Origin of High Dark Remnant Fractions in Milky Way Globular Clusters: The Crucial Role of Initial Black Hole Retention ›
Investigating the Kinematics of Molecular Gas in Cometary Globule L1616 ›
How the cosmic voids contribute to stalling and quenching the giant galaxies on their surfaces ›
Detection of young massive white dwarfs in core-collapsed globular cluster NGC 362 ›
Linking Stochastic Self-Propagating Star Formation and Spatio-Temporal Point Processes ›
Destruction of "Peas in a Pod?" A Candidate Multi-planet System Around the Nearby, Bright Star, HD208487 ›
Activity-Cycle Variations of Convection Scales in Subsurface Layers of the Sun ›
Type IIb Supernova Progenitors in 3D: Variability and Episodic Mass Loss revealed by Radiation-Hydrodynamics Simulations ›
The JWST Rocky Worlds DDT Program reveals GJ 3929b to likely be a bare rock ›
Mass Loss and Subsequent Thermal Evolution of Surviving Helium White Dwarfs Shocked by Thermonuclear Supernovae ›
Group Therapy for Halos: Advancing Halo Mass Estimation for Galaxy Groups ›
Three-Dimensional Numerical Simulations of Magnetar Crust Quakes ›
The highest mass Kepler red giants -- II. Spectroscopic parameters, the amplitude-activity relation, and unexpected halo orbits ›
SMILES Data Release II: Probing Galaxy Evolution during Cosmic Noon and Beyond with NIRSpec Medium-Resolution Spectra ›
The Fraction of Distilled White Dwarfs with Long-Lived Habitable Zones ›
A Tale of Two Sightlines: Comparison of Hydrocarbon Dust Absorption Bands toward Cygnus OB2-12 and the Galactic Center ›
Spatially and Dynamically Extended Molecular Gas in Stephan's Quintet Revealed by ALMA CO(1-0) Total Power Mapping ›
Image Profile (IMPRO) Fitting of Massive Protostars. I. Method Development and Test Cases of Cepheus A and G35.20-0.74N ›
The Demographics of Binary Companions to Stripped-Envelope Supernovae: Confronting Observations with Population Synthesis ›
On constraining initial orbital eccentricity of purely inspiral events ›
Runaway stars and the Galactic supernova remnant landscape: non-thermal emission and observational evidence ›
Observational Analysis of Multi-thermal Counter-streaming Flows in a Forming Filament and Their Relationship with Local Heating at Filament Footpoints ›
How many stars form in compact clusters in the local Milky Way? ›
Photospheric radius expansion thermonuclear burst and X-ray reflection from the neutron star X-ray binary 4U 1702-429 ›
Energy relaxation in superthermal collisions of carbon with oxygen: the influence of isotopic substitution ›
PEARLS: Globular Clusters and Ultra-Compact Dwarfs in the El Gordo Galaxies at z=0.87 ›
An empirical determination of the Cosmic Shoreline ›
A bird's eye view of stellar evolution through populations of variable stars in Galactic open clusters ›
Adaptive Uniform Weighting: Pre-conditioning to Improve Image Fidelity ›
TIRAMISU: Non-LTE radiative transfer for molecules in exoplanet atmospheres ›
Planetary Nebulae in the eROSITA eRASS1 catalog ›
Stochasticity in Stellar Yields Reflected in Theoretical Dust Masses Estimates Across all Type II Supernova Progenitors ›
Self-Consistent Heating of the Magnetically Closed Solar Corona: Generation of Nanoflares, Thermodynamic Response of the Plasma and Observational Signatures ›
Using Doppler Imaging to model stellar activity and search for planets around Sun-like stars ›
Energy Conversion and Electron Acceleration and Transport in 3D Simulations of Solar Flares ›
Comparing X-ray Emission Line Fluxes of NGC 5548 to NGC 1068 ›
Size Distributions of Arcsecond-Scale Properties of Solar Flare Ribbons ›
A test of Ca ii H & K photometry for isolating massive globular clusters below the metallicity floor ›
EP250207b is not a collapsar fast X-ray transient. Is it due to a compact object merger? ›
A 15 Mpc rotating galaxy filament at redshift z = 0.032 ›
Double-Peaked Optical Afterglows with X-ray Shallow Decay Inferring a Magnetized Thick Shell Ejecta ›
Molecular Hydrogen in High-redshift Damped Lyman-{\alpha} Absorbers ›
Activity in White Dwarf Debris Disks I: Spitzer Legacy Reveals Variability Incompatible with the Canonical Model ›
The ALPINE-CRISTAL-JWST survey: spatially resolved star formation relations at $z\sim5$ ›
Aligned Stellar Obliquities for Two Hot Jupiter-hosting M Dwarfs Revealed by MAROON-X: Implications for Hot Jupiter Formation ›
Impact of Non-Thermal Leptogenesis from Early Matter Domination on Gravitational Wave from FOPT ›
A New Paradigm for Testing Gravity: Theory-Independent Constraints Using Data From All Astrophysical and Cosmological Scales ›
Spacetime Perspective of Gravitational Lensing in Perturbed Cosmologies ›
High-Energy Neutrinos from Cosmic-Ray Scatterings with Supernova Neutrinos ›
Energy extraction from the accelerating Kerr black hole via magnetic reconnection in the plunging region and circular orbit region ›
Wavelets for power spectral density estimation of gravitational wave data ›
GW200105: A detailed study of eccentricity in the neutron star-black hole binary ›
Scalarized neutron stars with a highly relativistic core in scalar-tensor gravity ›
A Neural-Network Framework for Tracking and Identification of Cosmic-Ray Nuclei in the RadMap Telescope ›
Completing Axion Double Level Crossings ›
Morphological classification of eclipsing binary stars using computer vision methods ›
Current sheet formation under radiative cooling ›
Stellar metallicity is a key parameter for the search of Life in the Universe ›
Partial tidal disruptions of spinning eccentric white dwarfs by spinning intermediate mass black holes ›
Dust attenuation evolution in $z \sim 2$-$12$ JWST galaxies ›
In-Flight Performance of Spider's 280 GHz Receivers ›
A reassessment of LVE method and hemispherical power asymmetry in CMB temperature data from Planck PR4 ›
Estimating the gravitational wave background anisotropy: a Bayesian approach boosted by cross-correlation angular power spectrum ›
NutMaat: A Python package for stellar spectral classification on the MK system ›
High-cadence observations of galactic nuclei by the future two-band UV-photometry mission QUVIK ›
Exploring lensing signatures through spectrotemporal correlations: implications for black hole parameter estimation ›
The cosmological Mass Varying Neutrino model in the late universe ›
Cosmic Strings-induced CMB anisotropies in light of Weighted Morphology ›
Primordial black holes and scalar induced gravitational waves from sound speed resonance in non-minimal derivative coupling inflation model ›
Massive Double White Dwarf Binary Mergers from the Moon: Extending the Reach of Multi-messenger Astrophysics ›
XL-Calibur measurements of polarised hard X-ray emission from the Crab ›
Evolution of Shock Structures and QPOs After Halting BHL Accretion onto Kerr Black Hole ›
A non-uniform metal distribution in the ram-pressure stripped circumgalactic medium of M86 ›
JWST/NIRSpec Observations of High Ionization Emission Lines in Galaxies at High Redshift ›
Bayesian pulsar timing and noise analysis with Vela.jl: the wideband paradigm ›
Exploring the Interior Structure and Mode of Tidal Heating in Enceladus ›
Wavelet Flow For Extragalactic Foreground Simulations ›
Mass-feeding of jet-launching white dwarfs in grazing and common envelope evolution ›
Direct High-Resolution Imaging of Earth-Like Exoplanets ›
Head-on collisions of fuzzy/cold dark matter subhalos ›
Differentiation, the exception not the rule -- Evidence for full miscibility in sub-Neptune interiors ›
First release of LiteBIRD simulations from an end-to-end pipeline ›
The z=1.03 Merging Cluster SPT-CL J0356-5337: New Strong Lensing Analysis with HST and MUSE ›
The impact of natal kicks on black hole binaries ›
Quasi-periodic variation during a fast X-ray outburst of a high-mass X-ray binary MAXI J0709-159 / LY CMa observed by NICER ›
The $z=7.08$ quasar ULAS J1120+0641 May Never Reach a "Normal" Black Hole to Stellar Mass Ratio ›
Tightening constraints on primordial oscillations with latest ACT and SPT data ›
Hubble Space Telescope Observations of the Interstellar Interloper 3I/ATLAS ›
The role of migration traps in the formation of binary black holes in AGN disks ›
Meridional circulation molecular-weighted ›
Evidence For Turbulent Concentration In Particle-Laden Midplane Layers of Planet-Forming Disks ›
The Compilation and Validation of the Spectroscopic Redshift Catalogs for the DESI-COSMOS and DESI-XMMLSS Fields ›
Starobinsky in Stereo: SKA-CMB Synergy in SBI ›
Evidence for Evolving Dark Energy from LRG1 and Low-$z$ SNe Ia Data ›
New black hole mergers in the LIGO-Virgo O3 data from a gravitational wave search including higher-order harmonics ›
No-hair and almost-no-hair results for static axisymmetric black holes and ultracompact objects in astrophysical environments ›
Self-consistent microscopic calculations for electron captures on nuclei in core-collapse supernovae ›
Generalizing the Bogoliubov vs Boltzmann approaches in gravitational production ›
A Distribution-Free Approach to Testing Models for Angular Power Spectra ›
The Discriminant Power of Bubble Wall Velocities: Gravitational Waves and Electroweak Baryogenesis ›
Cosmic strings in the complex symmetron model ›
Extreme mass ratio inspirals in rotating dark matter spikes ›
Self-Tracking Solutions for Asymptotic Scalar Fields ›
SPLENDOR: a novel detector platform to search for light dark matter with narrow-gap semiconductors ↓↑