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
over the clouds
S Webcam
N Webcam
S Sky
Temperature
2.0 °C
Humidity
95%
Wind
6.4 km/h
Pressure
1002.3 hPa
Moon
Latest preprints on astro-ph:
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Exploring Radio Emissions from Confirmed Exoplanets Using SKA ›
Finding the unusual red giant remnants of cataclysmic variable mergers ›
JWST ERS Program Q3D: The pitfalls of virial BH mass constraints shown in a z = 3 quasar with an ultramassive host ›
APPLE: An Evolution Code for Modeling Giant Planets ›
Paicos: A Python package for analysis of (cosmological) simulations performed with Arepo ›
A Strong Gravitational Lens Is Worth a Thousand Dark Matter Halos: Inference on Small-Scale Structure Using Sequential Methods ›
Impact of main-sequence mass loss on the appearance, structure and evolution of Wolf-Rayet stars ›
An Excess of AGNs Triggered by Galaxy Mergers in MaNGA Galaxies of Stellar Mass $\sim10^{11}$ $M_{\odot}$ ›
Stochastic prior for non-parametric star-formation histories ›
Death of the Immortal Molecular Cloud: Resolution Dependence of the Gas-Star Formation Relation Rules out Decoupling by Stellar Drift ›
Formation of low mass protostars and their circumstellar disks ›
The SAGA Survey. III. A Census of 101 Satellite Systems around Milky Way-mass Galaxies ›
The SAGA Survey. IV. The Star Formation Properties of 101 Satellite Systems around Milky Way-mass Galaxies ›
The SAGA Survey. V. Modeling Satellite Systems around Milky Way-mass Galaxies with Updated UniverseMachine ›
The extent and power of "maintainance mode" feedback in MaNGA AGN ›
The CO-to-H$_2$ Conversion Factor in the Barred Spiral Galaxy M83 ›
Evolution of the disk in the Be binary $\delta$ Scorpii probed during three periastron passages ›
Imprints of Supermassive Black Hole Evolution on the Spectral and Spatial Anisotropy of Nano-Hertz Stochastic Gravitational-Wave Background ›
Instrument Signature Removal and Calibration Products for the Rubin Legacy Survey of Space and Time ›
Magnetic amplification in pre-merger neutron stars through resonance-induced magnetorotational instabilities ›
SMARTY: The mileS Moderate resolution neAr-infRared sTellar librarY ›
Loss of coherence and change in emission physics for radio emission from very inclined cosmic-ray air showers ›
Frequency Dispersed Ion Acoustic Waves in the Near Sun Solar Wind: Signatures of Impulsive Ion Beams ›
When are galactic winds molecular? ›
A Blueprint for the Milky Way's Stellar Populations. V. 3D Local Dust Extinction ›
VLBI with SKA: Possible Arrays and Astrometric Science ›
Spectropolarimetric Radio Imaging of Faint Gyrosynchrotron Emission from a CME : A Possible Indication of the Insufficiency of Homogeneous Models ›
Variation in Path Lengths of Turbulent Magnetic Field Lines and Solar Energetic Particles ›
On the X-ray efficiency of the white dwarf pulsar candidate ZTF J190132.9+145808.7 ›
Black hole-neutron star binaries ›
Isochrone Fitting of Galactic Globular Clusters -- VI. High-latitude Clusters NGC5024 (M53), NGC5053, NGC5272 (M3), NGC5466, and NGC7099 (M30) ›
NuSTAR detection of a broad absorption line in IGR J06074+2205 ›
Planetary nebula morphologies indicate a jet-driven explosion of SN 1987A and other core-collapse supernovae ›
X-ray detection of astrospheres around three main-sequence stars and their mass-loss rates ›
The Solar System: structural overview, origins and evolution ›
On the impact of the vertical structure of Martian water ice clouds on nadir atmospheric retrievals from simultaneous EMM/EXI and TGO/ACS-MIR observations ›
Solar flare observations with the Radio Neutrino Observatory Greenland (RNO-G) ›
Three dimensional end-to-end simulation for kilonova emission from a black-hole neutron-star merger ›
1-bit raw voltage recording system for dedicated observations of transients at low radio frequencies ›
Quantum study of the CH$_3^+$ photodissociation in full dimension Neural Networks potential energy surfaces ›
Confronting Dark Matter Capture Rate with Continuous Gravitational Wave Probe of Local Neutron Stars ›
Uncovering an Excess of X-ray Point Sources in the Halos of Virgo Late-type Galaxies ›
Resolving Red Giant Winds with the Hubble Space Telescope ›
Vanilla Inflation Predicts Negative Running ›
What can cosmic-ray knees reveal about source populations? ›
Life Cycle Assessment of the Athena X-ray Integral Field Unit ›
Signature of Particle Diffusion on the X-ray Spectra of the blazar Mkn 421 ›
A Unified Treatment of Kepler Occurrence to Trace Planet Evolution II: The Radius Cliff Formed by Atmospheric Escape ›
The Sensitivity of NEO Surveyor to Low-Perihelion Asteroids ›
Dark Radiation with Baryon Acoustic Oscillations from DESI 2024 and the $H_0$ tension ›
Interacting Dark Energy after DESI Baryon Acoustic Oscillation measurements ›
Leading Axion-Photon Sensitivity with NuSTAR Observations of M82 and M87 ›
Enhanced Muonization by Active-Sterile Neutrino Mixing in Protoneutron Stars ›
Inflaton decay in No-Scale Supergravity and Starobinsky-like models ›
LIGO operates with quantum noise below the Standard Quantum Limit ›
Lifetime-Limited Linewidth Measurements of the 3C and 3D Soft X-ray Transitions in Ni XIX ›
Bring the Heat: Tidal Heating Constraints for Black Holes and Exotic Compact Objects from the LIGO-Virgo-KAGRA Data ›
First Mapping the Canopy Height of Primeval Forests in the Tallest Tree Area of Asia ›
The unstable null circular geodesic features the spherically symmetrical asymptotically flat black hole ›
Asymmetric self-interacting dark matter with canonical seesaw ›
Impacting the dayside Martian ionosphere from above and below: Effects of the impact of CIRs and ICMEs close to aphelion (April 2021) and during dust storms (June-July 2022) seen with MAVEN ROSE ›
QCD topology and axion properties in an isotropic hot and dense medium ›
A Parameter-Free Tour of the Binary Black Hole Population ›
The Maximum Energy of Shock-Accelerated Cosmic Rays ›
Testing General Relativity with Black Hole X-Ray Data and ABHModels ›
Variability in SSTc2d J163134.1-240100, a brown dwarf with quasi-spherical mass loss ›
Iterative removal of sources to model the turbulent electromotive force ›
CLEANing Cygnus A deep and fast with R2D2 ›
Beyond the Background: Gravitational Wave Anisotropy and Continuous Waves from Supermassive Black Hole Binaries ›
A JWST investigation into the bar fraction at redshifts 1 < z < 3 ›
MaNGA DynPop -- V. The dark-matter fraction versus stellar velocity dispersion relation and stellar initial mass function variations in galaxies: dynamical models and full spectrum fitting of integral-field spectroscopy ›
Gravitational to Coulomb force ratio and the origin of the Cosmic magnetic field ›
MIDIS: Unveiling the Role of Strong Ha-emitters during the Epoch of Reionization with JWST ›
The relation between the cool-core radius and the host galaxy clusters: thermodynamic properties and cluster mass ›
First direction sensitive search for dark matter with a nuclear emulsion detector at a surface site ›
Winds and Disk Turbulence Exert Equal Torques on Thick Magnetically Arrested Disks ›
Confirmation of a Substantial Discrepancy between Radio and UV--IR Measures of the Star Formation Rate Density at 0.2 < z < 1.3 ›
Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties ›
The Survival and Entrainment of Molecules and Dust in Galactic Winds ›
Bidimensional Exploration of the warm-Temperature Ionised gaS (BETIS) I. Showcase sample and first results ›
Data-Driven Constraints on Cosmic-Ray Diffusion: Probing Self-Generated Turbulence in the Milky Way ›
Weighing neutrinos with Lyman-$\alpha$ observations ›
JWST Reveals a Surprisingly High Fraction of Galaxies Being Spiral-like at $0.5\leq z\leq4$ ›
Multi-tracing the primordial Universe with future surveys ›
Bridging relativistic jets from black hole scales to long-term electromagnetic radiation distances: A moving-mesh general relativistic hydrodynamics code with the HLLC Riemann solver ›
Electron-capture supernovae in NS+He star systems and the double neutron star systems ›
Hierarchical binary black hole mergers in globular clusters: mass function and evolution with redshift ›
Cosmological Prediction of the CSST Ultra Deep Field Type Ia Supernova Photometric Survey ›
The Impact of an AGN on PAH Emission in Galaxies: the Case of Ring Galaxy NGC 4138 ›
A perspective on the Milky Way Bulge-Bar as seen from the neutron-capture elements Cerium and Neodymium with APOGEE ›
Using Rest-Frame Optical and NIR Data from the RAISIN Survey to Explore the Redshift Evolution of Dust Laws in SN Ia Host Galaxies ›
Atmospheric entry and fragmentation of small asteroid 2024 BX1: Bolide trajectory, orbit, dynamics, light curve, and spectrum ›
Improved modeling of in-ice particle showers for IceCube event reconstruction ›
Simulations of galaxies in an expanding Universe with modified Newtonian dynamics (MOND) and with modified gravitational attractions (MOGA) ›
The role of heating on the formation and the dynamics of YSO jets : I. A parametric study ›
Does the Earth's rotation speed really tend to accelerate for a long time? ›
A short review of the pulsar magnetic inclination angles (II) ›
A short review on the pulsar magnetic inclination angles ›
Improved Treatment of Dark Matter Capture in Neutron Stars III: Nucleon and Exotic Targets ›
4D Weyl Anomaly and Diversity of the Interior Structure of Quantum Black Hole ›
Quantum Gravity Effects on Fermionic Dark Matter and Gravitational Waves ›
Testing Axionic Dark Matter during Gravitational Reheating ›
Generalized Lomb-Scargle Analysis of 22 years of Super-Kamiokande solar $^8$B neutrino data ↓↑