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
18.2 °C
Humidity
68%
Wind
8.0 km/h
Pressure
1009.3 hPa

Moon
Latest preprints on astro-ph:
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On the Image Profiles of Transients in the Palomar Sky Survey ›
A Generative Model for Disentangling Galaxy Photometric Parameters ›
Physical parameter regression from black hole images via a multiscale adaptive neural network ›
The VISCACHA Survey: XIII. The extended main-sequence turn-off in intermediate-age low-mass clusters ›
oLIMpus: An Effective Model for Line Intensity Mapping Auto- and Cross- Power Spectra in Cosmic Dawn and Reionization ›
Hidden binaries in star-forming regions ›
A Late-time Radio Search for Highly Off-axis Jets from PTF Broad-lined Ic Supernovae in GRB-like Host Galaxy Environments ›
Orbital and Physical Properties of the Pleiades Binary 27 Tau (Atlas) ›
Converging on the Cepheid Metallicity Dependence: Implications of Non-Standard Gaia Parallax Recalibration on Distance Measures ›
GRB 241105A: A test case for GRB classification and rapid r-process nucleosynthesis channels ›
The HETDEX Survey: Probing neutral hydrogen in the circumgalactic medium of ~88,000 Lyman Alpha Emitters ›
Measuring and modelling the Splash with APOGEE/Gaia and ARTEMIS ›
Carbon burning cannot explain puffy hypervelocity white dwarfs ›
A Semi-Empirical Estimate of Solar EUV Evolution from 10 Myr to 10 Gyr ›
Stellar evolution through the Red Supergiant phase ›
The Red and Yellow Hypergiants ›
Host galaxy identification of LOFAR sources in the Euclid Deep Field North ›
Red Supergiants in the Milky Way and Nearby Galaxies ›
Red Supergiants -- The Other Side of the H-R Diagram ›
Betelgeuse, the Prototypical Red Supergiant ›
Resolving Black Hole Family Issues Among the Massive Ancestors of Very High-Spin Gravitational-Wave Events Like GW231123 ›
Molecules and Chemistry in Red Supergiants ›
Red Supergiant Mass Loss and Mass-Loss Rates ›
Red Supergiants as Supernova Progenitors ›
Relativistic X-ray reflection and thermonuclear burst from accreting millisecond X-ray pulsar SRGA J144459.2-604207 ›
Double-offset Cassegrain telescopes for the Ultraviolet Type Ia (UVIa) mission concept ›
Prospects for GeV Neutrino Transient Searches with the IceCube Upgrade ›
Interplanetary magnetic correlation and low-frequency spectrum over many solar rotations ›
Building Earth with pebbles made of chondritic components ›
Applying multimodal learning to Classify transient Detections Early (AppleCiDEr) I: Data set, methods, and infrastructure ›
The project of a ground-based wide-angle EAS Cherenkov light imaging detector for PCR mass composition study in the 1-1000 PeV energy range ›
Testing gravitational physics by combining DESI DR1 and weak lensing datasets using the E_G estimator ›
Extensive Air Shower Registration at Two Depths with SPHERE-3 Detector ›
The results of the development of the SPHERE-3 detector for studying the PCR mass composition in the 1-1000 PeV energy range. The status of 2025 ›
Dissecting Reionisation with the Cosmic Star Formation and AGN Luminosity History ›
Simba Simulation: The Effect of Feedback Physics on Matter Distribution in the Cosmic Web ›
Waiting Time Distribution of Supra-Arcade Downflows ›
A Comprehensive Analysis of Rovibrational CO in the Era of JWST ›
Central Concentration and Escape of Ionizing Photons in Galaxies at the Epoch of Reionization ›
The VISCACHA survey XIV. Chemical evolution history of the SMC: The Southern Bridge Clusters ›
Observational constraints on phenomenological emergent dark energy and barotropic dark matter characterized by a constant equation of state parameter ›
Ionized gas in NGC 4258: Exploring the AGN -- Star formation connection ›
An AI super-resolution field emulator for cosmological hydrodynamics: the Lyman-{\alpha} forest ›
Can GRB Empirical Correlations Be Used for Population Studies? ›
TOI-880 is an Aligned, Coplanar, Multi-planet System ›
Galaxy Evolution in the Local Universe: Group Richness Effects on Mergers and Non-Mergers ›
Early-type Galaxies on the Star Formation Main Sequence: Internal Star Formation Geometry Revealed with MaNGA and Their Environmental Origin ›
The mass of TOI-654 b: A short-period sub-Neptune transiting a mid-M dwarf ›
Ly$\alpha$ Emission from [OIII] Emitters Near Reionization: The role of environment in galaxy Ly$\alpha$ detection ›
Observations of microwave emission from solar jets and comparison with MHD simulations ›
The THESAN project: environmental drivers of Local Group reionization ›
Understanding the magnetic field and plasma-$\beta$ along umbral fan loops traced using 3-min slow waves ›
Challan: Solar Full-disk Imaging-Spectroscopic Telescope using the Drift-Scanning Technique ›
ANTIHEROES-PRODIGE: Quantifying the connection from envelope to disk with the IRAM 30m telescope and NOEMA I. Attack of the streamers: L1448N's fight for order in the chaos ›
Investigating Interacting Dark Energy Models Using Fast Radio Burst Observations ›
Lunar Orbital VLBI Experiment: motivation, scientific purposes and status ›
Deep Chandra X-ray observation of the isolated black hole OGLE-2011-BLG-0462 ›
A Unified Volumetric Rate-Energy Relation from Magnetar Radio Bursts to Fast Radio Bursts ›
The Large Magellanic Cloud as a source of the highest energy cosmic rays ›
Recent advances on multimessenger astrophysics: Centaurus A, GW 170817, and KM3-230213A ›
Observation of VER J2019+368 with the SST-1M stereoscopic system ›
Sometimes they come back: pulsations in A 0538-66 at 69 ms rediscovered with NICER ›
Modelling gyrosynchrotron emission from coronal energetic electrons in a CME flux rope ›
The effect of stellar magnetic activity on measurements of morning and evening asymmetry of planetary terminator ›
Fast magneto-acoustic waves in the solar chromosphere: Comparison of single-fluid and two-fluid approximations ›
Intra-night optical variability and radio characteristics of extremely radio-loud narrow-line Seyfert 1 galaxies ›
The SST-1M stereoscopic system ›
Very-high-energy observations of the Seyfert galaxy NGC 4151 with MAGIC -- Indication of another gamma-ray obscured candidate neutrino source ›
A $6.37\,{\rm Hz}$ quasi-periodic oscillating photospheric emission in GRB~240825A ›
Exploring the properties of newborn pulsars with high-energy neutrinos ›
Low D/H ratio for benzonitrile in TMC-1: Implication for the origin of polycyclic aromatic hydrocarbons in cold dark clouds ›
Cosmological Preference for a Positive Neutrino Mass at 2.7$\sigma$: A Joint Analysis of DESI DR2, DESY5, and DESY1 Data ›
Inference of matter power spectrum at z=0 using DESI DR1 Full-Shape data ›
The Event Rate and Luminosity Function of Fermi/GBM Gamma-Ray Bursts ›
Forecast constraints on null tests of the $\Lambda$CDM model with SPHEREx ›
The gravitational potential of spiral perturbations. I the 2D (razor-thin) case ›
Stereo performance of SST-1M at different altitudes ›
Assessing robustness and bias in 1D retrievals of 3D Global Circulation Models at high spectral resolution: a WASP-76 b simulation case study in emission ›
The GHOSDT Simulations: II. Missing Molecules in Simulations of a Self-Regulated Interstellar Medium ›
Simulating realistic Lyman-$\alpha$ emitting galaxies including the effect of radiative transfer ›
Planck constraints on the scale dependence of isotropic cosmic birefringence ›
Hybrid concept of detection for a wide-field gamma-ray observatory using Cherenkov telescopes ›
Weinberg's theorem, phantom crossing and screening ›
Considering contact forces during the formation of planetesimals by gravitational collapse: mutual orbits, spin states, and shapes ›
Artifacts in Halo Shapes: Imprints of the Initial Condition ›
A double-degenerate scenario with a merger to explosion delay time to explain type Ia supernova SN 2020aeuh ›
Discovery of SiC and Iron Dust Around AGB Stars in the very Metal-Poor Sextans A Dwarf Galaxy with JWST: Implications for Dust Production at High Redshift ›
The SOFIA Massive (SOMA) Radio Survey. II. Radio Emission from High-Luminosity Protostars ›
Silicate mineralogy and bulk composition of exoplanetary material in polluted white dwarfs ›
Primordial black holes with anisotropic hair ›
Stellar Mass-Dispersion Measure Correlations Constrain Baryonic Feedback in Fast Radio Burst Host Galaxies ›
Mixture-of-Expert Variational Autoencoders for Cross-Modality Embedding of Type Ia Supernova Data ›
Weyl-invariant Einstein-Cartan gravity with a heavy ALP: Higgs Inflation and $\alpha$-attractors ›
Probing displaced (dark)photons from low reheating freeze-in at the LHC ›
Wino and Real Minimal Dark Matter Excluded by Fermi Gamma-Ray Observations ›
Testing Real WIMPs with CTAO ›
Distinguishing Neutron Star vs. Low-Mass Black Hole Binaries with Postmerger Gravitational Waves $-$ Sensitivity to Transmuted Black Holes and Non-Annihilating Dark Matter ›
Sub-GeV Dark Matter Under Pressure from Direct Detection ›
dot-PE: Sampler-free gravitational wave inference using matrix multiplication ›
ARTEMIS observations of electrostatic shocks inside the lunar wake ›
Probing Double-Peaked Gamma-Ray Spectra from Primordial Black Holes with Next-Generation Gamma-Ray Experiments ›
Split supersymmetry and hybrid inflation in light of Atacama Cosmology Telescope DR6 data ›
Towards a theory of coupled sociopolitical events-planetary boundaries, crises, policrisis and Earth System syndromes ›
Impact of cavities on the detection of quadratically coupled ultra-light dark matter ›
Dark matter explanations for the neutrino emission from the Seyfert galaxy NGC 1068 ›
Multiple ALPs and enhanced echoes ›
Gravitational Wave Scattering on Magnetic Fields ›
Alpha clustering in warm and dense nuclear matter from heavy-ion collisions ›
Cosmology with a Non-minimally Coupled Dark Matter Fluid I. Background Evolution ›
Multi-field TDiff theories: the mixed regime case ›
Evidence for Extended Hydrogen-Poor CSM in the Three-Peaked Light Curve of Stripped Envelope Ib Supernova ›
JWST/MIRI reveals the true number density of massive galaxies in the early Universe ›
Multi-Zone Modeling of Black Hole Accretion and Feedback in 3D GRMHD: Bridging Vast Spatial and Temporal Scales ›
LIGO Detector Characterization in the first half of the fourth Observing run ›
Kinetic simulations of the cosmic ray pressure anisotropy instability: cosmic ray scattering rate in the saturated state ›
Impact of Low ell's on Large Scale Structure Anomalies ›
Exploring the interaction between the MW and LMC with a large sample of blue horizontal branch stars from the DESI survey ›
Reconciling PTA and JWST and preparing for LISA with POMPOCO: a Parametrisation Of the Massive black hole POpulation for Comparison to Observations ›
A Novel Bispectrum Estimator of the Kinematic Sunyaev-Zel'dovich Effect using Projected Fields ›
Can decaying vacuum solve the H_0 Tension? ›
Euclid: Early Release Observations of diffuse stellar structures and globular clusters as probes of the mass assembly of galaxies in the Dorado group ›
The Local Galactic Transient Survey Applied to an Optical Search for Directed Intelligence ›
The Type Ia Supernova and AGB-Regulated Interstellar Medium of Massive Galaxies ›
Nuclear Neural Networks: Emulating Late Burning Stages in Core Collapse Supernova Progenitors ›
The effects of projection on measuring the splashback feature ›
What's the matter with $\Sigma m_{\nu}$? ›
The rise of the galactic empire: luminosity functions at $z\sim17$ and $z\sim25$ estimated with the MIDIS$+$NGDEEP ultra-deep JWST/NIRCam dataset ›
Enhancement of primordial curvature perturbations in $R^3$-corrected Starobinsky-Higgs inflation ›
Characterizing 3D Magnetic Fields and Turbulence in H I Clouds ›
Learning novel representations of variable sources from multi-modal $\textit{Gaia}$ data via autoencoders ›
The Kick Velocity Distribution of Isolated Neutron Stars ›
Is Ozone a Reliable Proxy for Molecular Oxygen? II. The impact of N$_2$O on the O$_2$-O$_3$ relationship for Earth-like atmospheres ›
Neutrino pair annihilation driven jets from black-hole torus systems ›
IIb or not IIb: A Catalog of ZTF Kilonova Imposters ›
Detection of positron in-flight annihilation from the Galaxy ›
Cosmic structure from the path integral of classical mechanics and its comparison to standard perturbation theory ›
Model-independent observational constraints with fast radio bursts ›
X-SHOOTER Spectrum of Comet 3I/ATLAS: Insights into a Distant Interstellar Visitor ›
Roles of SN and AGN Feedback in Shaping the Baryonic Content in a Wide Range of Dark Matter Halo Mass ›
Supermassive Stars Match the Spectral Signatures of JWST's Little Red Dots ›
Multi-wavelength study of the high Galactic latitude supernova remnant candidate G118.4+37.0 associated with the Calvera pulsar ›
AMICO galaxy clusters in KiDS-1000: cosmological constraints and mass calibration from counts and weak lensing ›
Identifying the Quadrupolar Nature of Gravitational Wave Background through Space-based Missions ›
Dirac Leptogenesis in Left-Right Symmetric Models ›
On Formation of Primordial Naked Singularities ›
Pre-thermalized Gravitational Waves ›
Rotating Einstein-Maxwell-Dilaton Black Hole as a Particle Accelerator ›
Detectability of gravitational atoms in black hole binaries with the Einstein Telescope ›
Scale separation, rolling solutions and entropy bounds ›
Soft Oscillons ›
Evolution of a black hole cluster in full general relativity ›
Universal Cosmologies ›
Galactic double neutron stars as dual-line gravitational-wave sources: Prospects with LISA and Cosmic Explorer ›
Time as a test-field: the no-boundary universe in motion and a smooth radiation bounce ↓↑