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

In the dark

S Webcam

N Webcam

S Sky
Temperature
1.3 °C
Humidity
93%
Wind
6.4 km/h
Pressure
1009.2 hPa

Moon
Latest preprints on astro-ph:
›
Uniform Reinterpretation of Rocky Exoplanet Secondary Eclipse Observations and the Impact of Stellar and Orbital Uncertainties ›
The CARMENES search for exoplanets around M dwarfs. A homogeneous catalogue of projected rotational velocities accounting for limb-darkening ›
GRMHD accretion beyond the black hole paradigm: Light from within the shadow ›
PySCo-EFT and ECOSMOG-EFT: a tandem of N-body simulation codes for the Effective Field Theory of Dark Energy ›
Surveying the Whirlpool at Arcseconds with NOEMA (SWAN). IV. Extent of active galactic nucleus feedback on the interstellar medium ›
Probing the large-scale structure with 21cm-galaxy cross-bispectrum: Estimates from simulations and forecasts for upcoming cosmological surveys ›
Detectability of Gravitationally Lensed Kilonovae in the Rubin LSST ›
Joint Detection and Characterization of the Standing Accretion Shock Instability for Core-Collapse Supernovae with cWB XP ›
Refined Constraints on the Hard X-ray Polarization of the Crab Pulsar and Nebula Derived from an Extended XL-Calibur Dataset ›
The Effect of External Photoevaporation on the Disk Fraction in M17 ›
Sequential and non-sequential Zemax Dynamic Link Libraries for generating image slicer integral field units ›
On the contribution of the bow shock pulsar wind nebula PSR J0437-4715 to the observed fluxes of GeV-TeV positrons and antiprotons ›
ExoNet: Multimodal Deep Learning for TESS Exoplanet Candidate Identification via Phase-Folded Light Curves, Stellar Parameters, and Multi-Head Attention Fusion ›
The ubiquity of turbulence in the expanding kinematics of the ionized shells of Galactic planetary nebulae ›
The Impact of the Bar on Dense Gas and Star Formation in M83 ›
Distances to molecular clouds in the Galactic longitude l=10-20 deg from the MWISP 12CO 1-0 survey ›
Circular polarization images of Sgr A* for different magnetic field geometries ›
Radiation-driven stellar winds at the fast-slow transition: new hydrodynamic solutions ›
A New Cloud-Cloud Collision Source N68 toward the G35 Molecular Cloud Complex ›
A universal relationship between the variability timescale and black hole mass in black hole jetted and non-jetted accreting systems ›
Inverting Fisher biases for fast systematics exploration ›
Induced Scattering of Strong Waves in Pair Plasmas ›
Asteroid modelling by starlight diffraction: The shape of Dimorphos, the satellite of (65803) Didymos ›
A gem system with a lava world and a habitable zone sub-Neptune orbiting TOI-1752 ›
Benchmarking Two Chemical Networks used in General Circulation Models of Hot Jupiters ›
PISP: Projected-Space Inference of Stellar Parameters ›
Beyond the mass-radius plane: Integrated radiative-convective and interior structure simulations of the exoplanet continuum ›
The Reaction between Atomic Carbon and Molecular Nitrogen as a Source of Cyanamide and Carbodiimide on Interstellar Ices ›
Inferring Halo Mass and Scale Radius of Galaxy Clusters Using Convolutional Neural Networks and Uchuu-UniverseMachine Catalogs ›
Revisiting the Galactic age-metallicity relation from wide white dwarf-main-sequence binaries ›
Missing pairs in open cluster catalogs ›
Relativistic time scales in the Solar system ›
Binary and neutron star evolution in low-mass X-ray binaries on the evolutionary tracks of accreting millisecond X-ray pulsars ›
Kinematically cold and warm planetary nebulae samples, HII regions and supernovae remnants in the disc of the face-on spiral galaxy NGC 628 (M74) -- The Planetary Nebulae Spectrograph with the H$\alpha$ arm ›
Machine learning isotope shifts in molecular energy levels ›
JWST and Keck observations of the off-nuclear tidal disruption event TDE 2025abcr: An evolving reprocessing layer ›
Towards a Robust Estimate of the Solar Photospheric Poynting Flux and Helicity Flux ›
The 0.9 Megasecond XRISM/Resolve Spectrum of the Seyfert-1 AGN NGC 4151 ›
Probing Primordial Black Holes with upcoming Radio Telescopes: a case study for LOFAR2.0, FAST Core Array and BINGO ›
A ready-to-fit inhomogeneous cosmological model: the axially symmetric Szekeres spacetime ›
Magnetic switchback formation: a review of proposed mechanisms ›
Extending Galactic foreground emission with neural networks ›
On the relationship between the ellipticity of Galactic globular clusters and their X-ray luminosity ›
Euclid: Scaled-up little red dots and other sources with v-shaped spectral energy distributions at z>4 ›
Solar Cycle Prediction: Challenges, Progress, and Future Perspectives ›
Constraining the Pulsar Beaming Fraction with TeV-Selected Galactic Pulsar Wind Nebulae and unidentified TeV Sources ›
High-Frequency Gravitational Waves from the Galactic Pulsar Population ›
FastQSL 2: A Comprehensive Toolkit for Magnetic Connectivity Analysis ›
A XRISM Study of Highly Ionized Iron Emission Lines from the Low-Eddington-ratio AGN in NGC 7213 ›
Degradation mechanisms and efficiency of heavily cratered regions on Ceres ›
Relative frequencies of core-collapse supernovae as a function of metallicity: observations vs theoretical predictions ›
Prebiotic Chemistry Insights for Dragonfly II: Thermodynamic Favorability of Nucleobases, Ribose, and Fatty Acids in Selk Crater on Titan ›
Challenge in Arrokoth's single merger to achieve the shape's principal axis configuration ›
The DESIRED strong-line calibrations: I. New empirical metallicity relations for the local and high-redshift universe ›
The hydrodynamical response of cold circumgalactic clouds to quasar radiation ›
TTV-Not-So-Fast: Uniqueness and Degeneracy in Perturbing Planet Parameters ›
The Neptunian ridge as a natural outcome of high-eccentricity tidal migration ›
Electro-Weak Phase Transitions and Collider Signals in the Aligned 2-Higgs Doublet Model ›
OverCite: Add citations in LaTeX without leaving the editor ›
Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms ›
Geometrically Regular Black Holes with Hedgehog Scalar Hair ›
Mechanical Long Baseline Differential Gradiometers as Low Frequency Gravitational Wave Detectors ›
Gravitational-wave astronomy requires population-informed parameter estimation ›
Improved Constraints on Non-Kerr Deviations from Binary Black Hole Inspirals Using GWTC-4 Data ›
Measuring the rate of glitches in interferometric gravitational wave detectors with a hierarchical Bayesian model ›
Thermal effects on Dark Matter production during cosmic reheating ›
Experimental evidence for coronal mass ejection suppression in strong stellar magnetic fields ›
Post-Newtonian Constraints on Scalar-Tensor Gravity ›
Recent progress on inflation and dark energy from string theory ›
Euclid Quick Data Release (Q1): The evolution of the passive-density and morphology-density relations between $z=0.25$ and $z=1$ ›
A Homogeneous Catalog of Oscillating Solar-Type Stars Observed by the Kepler Mission and a New Amplitude Scaling Relation Including Chromospheric Activity ›
Influence of penetration depth on jets on giant planets: equatorial jet direction, jet numbers, and jet energy fraction ›
Tomographic Alcock-Paczynski Test with Marked Correlation Functions ›
Cosmic filaments confirm unexplained CMB temperature decrements in two independent redshift ranges ›
Unraveling the Secrets of the lower Solar Atmosphere: One year of Operation of the Solar Ultraviolet Imaging Telescope (SUIT) on board Aditya-L1 ›
Sensitivity of spectral lines to granulation: The Sun ›
Bulk viscosity from neutron decays to dark baryons in neutron star matter ›
Robust Measurement of Stellar Streams Around the Milky Way: Correcting Spatially Variable Observational Selection Effects in Optical Imaging Surveys ›
Sub-Snowline Formation of Gas-Giant Planets in Binary Systems ›
Study of Neutron Star Properties under the Two-Flavor Quark NJL Model ›
Kinematic scaling relations of disc galaxies from ionised gas at $z\sim1$ and their connection with dark matter haloes ›
Forecasting synchrotron spectral parameters with QUIJOTE-MFI2 in combination with Planck and WMAP ›
Readdressing the contribution of photonuclear reactions to the muon content of extensive air showers: a heuristic approach ›
Weakened Inspirals I: High Mass Ratio Common Envelope Interactions in RGB Stars ›
The contribution from small scales on two-point shear analysis: comparison between power spectrum and correlation function ›
Improved lanthanide constraints for the kilonova AT 2017gfo ›
Operational Non-identifiability of Single-epoch Low-rank RFI Mitigation: Controlled Failure-mode Analysis and HERA Evidence ›
How deep can a cosmic void be? Voids-informed theoretical bounds in Galileon gravity ›
A Dynamo Confinement Scenario for the Solar Tachocline and its Implications for Spin-down in the Radiative Spreading Regime ›
The long-term evolution of Ultra Faint Dwarf Galaxies and observational implications ›
Towards a Fully Automated Pipeline for Short-Term Forecasting of In Situ Coronal Mass Ejection Magnetic Field Structure ›
Bayesian Cosmic Void Finding with Graph Flows ›
Kinematics of Wolf-Rayet Stars in the LMC: Clues to Subtype Origins ›
A unified harmonic framework for dark siren cosmology ›
Measurements on the kinetic physics in streamer dynamics ›
Retrieving the Red Edge on Earth-like Planets with Heterogeneous Clouds and Surfaces ›
A New Method to Simulate Dark Matter-Baryon Interactions and Application to an Isolated Disk Galaxy ›
Magnetic-Field-Induced Inspiral of Binaries with Circumbinary Disk: Black Hole and Protostellar Systems ›
Coupled Dark Energy and Dark Matter for DESI: An Effective Guide to the Phantom Divide ›
Prospects for GRB Afterglow Discovery with the Eric and Wendy Schmidt Observatory System ›
The Damping and Instability of Ion-acoustic Waves in the Solar Wind: Solar Orbiter Observations ›
The physics of gravitational waves ›
Chiral global embedding of Fibre Inflation with $\overline{\rm D3}$ uplift ›
TLS and Quasiparticle Loss in Thin-Film Aluminum CPW Resonators: A Modified Model and Design Implications ›
Conformal form-invariant parametrization of scalar-tensor gravity theories: A critical analysis ›
Classical constant electric fields and the Schwinger effect in de Sitter ›
Inferring neutron-star Love-Q relations from gravitational waves in the hierarchical Bayesian framework ›
Comparing next-generation detector configurations for high-redshift gravitational wave sources with neural posterior estimation ›
Analytic Approximations for Fermionic Preheating ›
Novel ringdown tests of general relativity with black hole greybody factors ↓↑