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

Before observations ...

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Temperature
-2.8 °C
Humidity
94%
Wind
0.0 km/h
Pressure
1009.2 hPa

Moon
Latest preprints on astro-ph:
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A New Plotly-Dash-based Query Infrastructure for the Keck Observatory Archive ›
Resonant Axion-Photon Conversion in the Early Inspiral of Neutron Star Binaries ›
GW-FALCON: A Novel Feature-Driven Deep Learning Approach for Early Warning Alerts of BNS and NSBH Inspirals in Next-Generation GW Observatories ›
Coupled Map Lattice for Astronomical Object Formation: A Scenario for Evolution from Star to Disk, Arms, and Companions ›
Well-being and career instability across genders in the Spanish Astronomical Society ›
PSR J0024$-$7204ai: a massive, eccentric binary system in the globular cluster 47 Tucanae ›
Intracluster globular clusters as tracers of the mass assembly of the Hydra I galaxy cluster ›
UV and Optical Signatures of Late-time Disk Instabilities in Tidal Disruption Events ›
ABCMB: A Python+JAX Package for the Cosmic Microwave Background Power Spectrum ›
Searching for Extragalactic Exoplanets: A Survey of the Sagittarius Dwarf Galaxy Stream with TESS ›
Barium Stars Across the Milky Way: Probing Their Origins via the GALAH Survey ›
The diverse nature of spiral arms in the Auriga Superstars cosmological hydrodynamic simulations ›
The dependence of triggering mechanisms on radio AGN sub-types: the role of galaxy mergers ›
Measuring Pulsar Distances from Chirping Orbital Periods ›
Orbital eccentricity can make neutron star g-mode resonances observable with current gravitational-wave detectors ›
Detection horizon for the neutrino burst from the stellar helium flash ›
Magnetohydrodynamic Precipitation ›
AGN in massive galaxies identified via optical broadband variability: lessons from VST-COSMOS for future LSST science ›
Mimicking the large-scale structure of the Local Universe. Synthetic pre-labelled galaxies in large-scale structures ›
Mechanisms Affecting Galaxies Nearby and Environmental Trends (MAGNET) ›
The eruptive young star IRAS 21204+4913 ›
Three-Dimensional Kinematics of the Oxygen-rich Supernova Remnant G292.0+1.8 ›
A Response to paper Critical Evaluation of Studies Alleging Evidence for Technosignatures in the POSS1-E Photographic Plates by Watters et al. (2026) ›
Helium superluminous SN 2021bnw : an explosion of a massive star with a pre-outburst ›
Vertical Temperature Structure in Io's Atmosphere from ALMA SO$_2$ Observations ›
Multi-Arrival Infrasound from Meteoroids: Fragmentation Signatures versus Propagation Effects in a Fine-Scale Layered Atmosphere ›
GPS constellation search for exotic physics messengers coincident with the binary neutron star merger GW170817 ›
New Insights from Revisiting the Rotation Period of the Strongly Magnetic O Star, NGC 1624-2 ›
On the dynamics, thermodynamics and fine structure of virtual erupting filaments ›
Calibrating the Tip of the Red Giant Branch and measuring Magellanic Cloud distances to 2% exclusively with Gaia ›
The First Instrumentally Documented Fall of an Iron Meteorite: atmospheric trajectory and ground impact ›
Cosmological Averaging in Nonminimally Coupled Gravity ›
A Quantum Genetic Algorithm with application to Cosmological Parameters Estimation ›
Coronal Non-Thermal and Doppler Plasma Flows Driven by Photospheric Flux in 28 Active Regions ›
Scaling solutions in three-form cosmology ›
Precise measurement of WASP-31 b's Rossiter-McLaughlin effect and characterization of the planet transmission spectra ›
Upper atmosphere dynamics and drivers of volatiles loss from terrestrial-type (exo)planets ›
Cosmic topology. Part IIc. Detectability with non-standard primordial power spectrum ›
A homogeneous view of asymptotic giant branch carbon stars as seen by Gaia ›
An observational test of the plasma lensing effect using QSOs with and without MgII absorption ›
Bridging Scales in Black Hole Accretion and Feedback: Subgrid Prescription from First Principles ›
Inference of horizontal velocity fields from the induction equation in the solar atmosphere. I. Analytical and numerical solutions in 2D ›
Dust measurements with the Mars Dust Counter on board Nozomi (PLANET-B) ›
Morphological variations of solar granules in the presence of magnetic fields ›
Aligned and misaligned metallicity gradients in young stars and star-forming regions in the EAGLE discs ›
Fast computation of temperature and polarization coupling matrices ›
Searching for Axion-like particle Dark Matter with Time-domain Polarization: Constraints from a protoplanetary disk ›
Bayesian parameter study of the Seyfert-starburst composite galaxies NGC 1068 and NGC 7469 ›
Spectroscopic analysis and RHD modeling of the first Ca II H and H-epsilon flare spectra from DKIST/ViSP ›
Detecting the neutrino mass via the cross-correlation between matter tracers and the ISWRS effect? ›
Hot subdwarf stars from the Hamburg Quasar Survey ›
The Montreal Open Clusters and Associations (MOCA) Database: A Census of Nearby Associations, Open Clusters, and Young Substellar Objects within 500 pc of the Sun ›
Impact of rotation on the amplitude of acoustic modes in solar-like stars: Insights from hydrodynamical simulations ›
Slow focus sensor for the Keck I laser guide star adaptive optics system using focal plane wavefront sensing ›
Deep Learning for Point Spread Function Modeling in Cosmology ›
Between Plateaus and Slopes: A Data-Driven Exploration of Spectral Diversity Across Type IIP/L Supernovae ›
WISDOM Project - XXVII. Giant molecular clouds of the lenticular galaxy NGC 1387: similarities with spiral galaxy clouds ›
Nearest Neighbour-Based Statistics for 21cm-Galaxy Cross-Correlations in the Epoch of Reionization ›
Exploring Chaotic Motion of a Particle in the Centre of a Galaxy with a Prolate Halo ›
Venting and Outgassing Simulations of Pressurized Lunar Modules: Contamination of the Lunar Environment ›
Model selection with the Pantheon+ Type Ia SN sample ›
Blackening Cryosphere: Revealing Hotspot Shifts and HGB-Based Forecasting of Absorbing Aerosol Threats over the Himalayan Frozen Frontiers ›
May Negative Mass Objects exist in the sky? ›
IT-DPC-SRI: A Cloud-Optimized Archive of Italian Radar Precipitation (2010-2025) ›
The Sun Can Strongly Constrain Spin-Dependent Dark Matter Nucleon Scattering Below the Evaporation Limit ›
Enhanced Cosmic-Ray Antinuclei Fluxes with Dark Matter Annihilation into SUEPs ›
Primordial black hole evaporation in a thermal bath and gravitational waves ›
Some phenomenological aspects of a quantum-corrected Reissner-Nordstr\"{o}m black hole: quasi-periodic oscillations, scalar perturbations and thermal fluctuations ›
Radial oscillations of pulsating neutron stars: The UCIa equation-of-state case ›
Hubble-Scale Tachyonic Shocks from Low-Scale Inflation -- A New Gravitational-Wave Window on Inflation ›
Probing neutrino emission at GeV energies from compact binary mergers with the IceCube Neutrino Observatory ›
Revisiting bright delta Scuti stars and their period-luminosity relation with TESS and Gaia DR3 ›
WISDOM project -- XVIII. Molecular gas distributions and kinematics of three megamaser galaxies ›
Identifying 850 delta Scuti pulsators in a narrow Gaia colour range with TESS 10-minute full-frame images ›
Astrometric constraints on stochastic gravitational wave background with neural networks ›
Gravitational waves from cosmic strings for pedestrians ›
The HST-Hyperion Survey: Companion Fraction and Overdensity in a z ~ 2.5 Proto-supercluster ›
Influence of finite-temperature effects on CMB power spectrum ›
Stochastic analysis of finite-temperature effects on cosmological parameters by artificial neural networks ›
Late-blooming magnetars: awakening as long period transients after a dormant cooling epoch ›
The Single-Degenerate Channel Leads to Type Iax and Not Type Ia Supernovae due to Premature Ignition ›
Characterizing bright $\delta$ Scuti pulsators using TESS lightcurves ›
The Diversity and Evolution of Dust Attenuation Curves from Redshift z ~ 1 to 9 ›
Investigating the Gamma-Ray Emission from Explosive Dispersal Outflows with Fermi-LAT ›
A hybrid active galactic nucleus feedback model with spinning black holes, winds and jets ›
Carnegie Supernova Project: Fast-Declining Type Ia Supernovae as Cosmological Distance Indicators ›
Dark-to-black super accretion as a mechanism for early supermassive black hole growth ›
Beyond CPL: Evidence for dynamical dark energy in three-parameter models ›
Crosschecking Cosmic Distances from DESI BAO and DES SNe Points to Systematics ›
JWST/MIRI-MRS view of the metal-poor galaxy CGCG 007-025: the spatial location of PAHs and very highly ionized gas ›
Ephemeris and Almanac Design for Lunar Navigation Satellites ›
Formation Channels of Magnetars ›
Synchrotron radiation from NGC 470 HLX1 - a hidden hyperluminous accreting neutron star? ›
Non-Gaussianity in SMICA ›
JWST observations of three long-period AM CVn binaries: detection of the donors and hints of magnetically truncated disks ›
Fluctuation dynamos in supersonic turbulence at ${\rm Pm} \gtrsim 1$ ›
Multigroup Radiation Diffusion on a Moving Mesh: Implementation in RICH and Application to Tidal Disruption Events ›
Digging into the Interior of Hot Cores with ALMA (DIHCA). VI. The Formation of Low-mass Multiple Systems in High-mass Cluster-forming Regions ›
Prediction of Multi-Wavelength Afterglows Associated with FRB 20200120E and FRB 20201124A ›
WLM: Dynamics of an isolated Dwarf Irregular Galaxy Under Ram Pressure in the Local Group ›
Dynamics of the coronal magnetic field in the 2022-10-02 X-class flare ›
Seasonal Variation of Polar Ice: Implications for Ultrahigh Energy Neutrino Detectors ›
First statistical constraints on galactic scale outflows properties traced by their extended Mg II emission with MUSE ›
Is cosmic birefringence due to dark energy or dark matter? Simulation-based inference ›
Self-Consistent Direct Method for Chemical Abundances in High-z Galaxies with JWST ›
Microphysical Model of Jupiter's Great Red Spot Upper Chromophore Haze ›
The Numerics of VMEC++ ›
Deflection angle in the strong deflection limit: A perspective from local geometrical invariants and matter distributions ›
Explaining the PeV Neutrino Fluxes at KM3NeT and IceCube with Quasi-Extremal Primordial Black Holes ›
Secluded Dark Composites and Remnant Binding Fields ›
Gravothermal Pile-Up of Collisional Dark Matter Around Compact Objects ›
Testing Real WIMPs with CTAO ›
Nonstrange and strange quark matter at finite temperature within modified NJL model and protoquark stars ›
Coordinate Systems and Transforms in Space Physics: Terms, Definitions, Implementations, and Recommendations for Reproducibility ›
Multibanded Reduced Order Quadrature Techniques for Gravitational Wave Inference ↓↑