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 dome

S Webcam

N Webcam

S Sky
Temperature
-4.6 °C
Humidity
84%
Wind
11.3 km/h
Pressure
1006.3 hPa

Moon
Latest preprints on astro-ph:
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Pedagogic Null Tests of Dynamical Dark Energy Hints: Reconstructing LambdaCDM with Consistent BAO, CMB, and SNe Mocks ›
No Pulsar Detected in Reprocessed Archival Parkes Observations of SNR 1987A ›
Habitable from the start: How initial planetary formation conditions may create habitable worlds ›
The CO-to-H$_2$ conversion factor in the Milky Way's central parsec ›
The Surface and Interior Conditions of Temperate Sub-Neptune TOI-270 d ›
HIDES -- I. The population and diversity of HI-rich 'dark' galaxies in the Hestia and Auriga simulations ›
Radio-Continuum Spectra of Pulsars with Free-Free Thermal Absorption ›
Evolution mapping III: A new recipe for the halo mass function ›
A search for cold molecular outflows in cosmic noon galaxies ›
The 12CO Gas Structures of Protoplanetary Disks in the Upper Scorpius Region ›
Zooming into the water snowline: high resolution water observations of the HL Tau disk ›
A continuous parameterization of the cosmic web ›
Validation of optical pathlength stability in a LISA test-bench demonstrator ›
CLAWDIA: A dictionary learning framework for gravitational-wave data analysis ›
Finding He II: Testing Novel Models of Binary Populations across Cosmic Time ›
The ViSta method for stacking in the Fourier domain and its application to the dusty star-forming galaxies in the ALMA Science Archive ›
Data-Driven Stellar Spectral Modelling with GSPICE ›
Turbulence in Core-Collapse Supernovae ›
An Investigation of Systematic Effects from Background Priors on PSR J0740$+$6620 Radius Estimates using Synthetic NICER and XMM-Newton Data ›
Ionizing radiation of [WR] stars: atmospheres and photoionization models ›
The nature of UHE source 1LHAASO J1740+0948u and its connection to PSR J1740+1000 ›
Dynamical fractalization of ring systems ›
A Comprehensive Analysis of the Panchromatic Transmission Spectrum of the Hot-Saturn WASP-96 b: Nondetection of Haze, Possible Sodium Limb Asymmetry, Stellar Characterization, and Formation History ›
A study of transients from ground-based surveys reveals new AM CVn stars ›
Lord of the (sub-)Rings : Mapping the surface reflectance and spin-axis of Ajisai ›
Solar Cycle 25 Dynamics from Observational and Statistical Parameters: Characterization of the Maximum Phase and Rotational Behaviour ›
In-depth analysis of the clustering of dark matter particles around primordial black holes. Part II. Analytical prescriptions for spikes ›
Gray Spectral Variability in Three Brown Dwarfs Observed by HST/WFC3 Time-Series Observations ›
Quantifying the impact of selection effects on FRB DM-$z$ relation cosmological inference ›
Constructing Earth Formation History Using Deep Mantle Noble Gas Reservoirs ›
GSpyNetTreeS: a machine learning solution for glitch localization in time and frequency ›
Which active galaxies might be neutrino emitters? ›
Self-bound quark stars with a first-order two-to-three flavor phase transition ›
Exploring Emission Line Variability and Jet-Broad Line Region Interaction in the Blazar TON 599 ›
CO Multi-line Imaging of Nearby Galaxies (COMING). XI. Azimuthally averaged star formation rate and stellar mass relation with molecular gas amount ›
A deep ALMA Band 3 survey of HDFS/MUSE3D: Survey description and initial results ›
Exploring the Cosmological Model Degeneracy with a new evaluate factor G ›
Fully self-consistent nova explosion models reproducing light curves of KT Eri, V339 Del, V597 Pup, and SMC NOVA 2016-10a ›
Fast far-sidelobe modeling for centimeter to sub-millimeter astrophysical observations ›
A novel double-rim forebaffle design for centimeter to sub-millimeter astrophysical observations ›
Probing Dark Matter Substructure with Image Number Anomaly in Strong Lensing Systems ›
TRAO Survey of the Nearby Filamentary Molecular Clouds, the Universal Nursery of Stars (TRAO-FUNS). IV. Filaments and Dense Cores in the W40 and Serpens South Regions of Aquila ›
Multiphase Astrophysics to Unveil the Virgo Environment (MAUVE) ›
Comparing galaxy merger orbits in hydrodynamical simulation and in dark-matter-only simulation ›
Morphological Image Similarity Search on the ALMA Science Archive Query Interface Using Deep Unsupervised Contrastive Representation Learning ›
Spectral synthesis techniques for supernovae and kilonovae ›
RUBIX: Differentiable forward modelling of galaxy spectral data cubes for gradient-based parameter estimation ›
Dark Matter Admixed White Dwarfs: A Single-Fluid Approach ›
RGB Tip distance to the faint gas-rich dwarf KK 153 ›
Magnetized particle motion and accretion process with shock cone morphology around a decoupled hairy black holes ›
From Ground to Space: An Overview of the JEM-EUSO Program for the Study of UHECRs and Astrophysical Neutrinos ›
Arp@VST: Legacy Survey of the Arp Peculiar Galaxies with the VST ›
Orbital parameters of the bright binary alpha Draconis based on amateur spectra from the STAROS database ›
Constraining non-minimally coupled squared-Quartic Hilltop Inflation in light of ACT observations ›
An Alternative Explanation for the Helium Star Pulsar Binary J1928$+$1815: The Most Heavyweight Black Widow System to Date ›
Far-infrared to centimeter emission of very nearby galaxies with archival data ›
Covariance spectrum of MAXI J1820+070: On the nature of the Comptonizing flow ›
Deep Investigation of Neutral Gas Origins (DINGO): Options for robust Deep Spectral Line Imaging in the SKA-Era ›
Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4 ›
On the baryon budget in the X-ray-emitting circumgalactic medium of Milky Way-mass galaxies ›
Effect of the Memory Burden on Primordial Black Hole Hot Spots ›
Simulating Disky Broad Line Region Reverberation ›
A XRISM View of Relativistic Reflection in Cygnus X-1 ›
Deep Learning Analysis of Ions Accelerated at Shocks ›
Discovering periodic and repeating nuclear transients in the XMM-Newton archives ›
Accelerating the CLEAN algorithm of radio interferometry with convex optimization ›
Quasar clustering and duty cycle measurements at $0\leq z\leq 4$ with the Gaia-unWISE Catalog ›
Moving superfluids in the rotating universe ›
Performance Simulations for Kola: Achieving High-Resolution, Visible-Light AO Correction Over a 1 Arcminute Field ›
Effect of local environment on Ly$\alpha$ line profile in DESI/ODIN LAEs ›
How Significant are Cosmological Collider Signals in the Planck Data? ›
Growth of Cosmic Strings with Field-Dependent Tension ›
WIMP Meets ALP: Coherent Freeze-Out of Dark Matter ›
The 59th Karl Jansky Lecture: Discovering the Radio Universe ›
Numerical tiling-based simulations of decoherence in multifield models of inflation ›
Accelerating parameter estimation for parameterized tests of general relativity with gravitational-wave observations ›
Exceptional line and pseudospectrum in black hole spectroscopy ›
Distributed Acoustic Fiber Sensing for Research Campuses and Large Scientific Infrastructures -- The Hamburg WAVE proto-network ›
Cosmological perturbations on an averaged background ›
A battle of designs: triangular vs. L-shaped detectors and parity violation in the gravitational-wave background ›
Constraining tachyonic inflationary \beta-exponential model with Continuous Spontaneous Localization collapse scheme ›
Generalized framework for likelihood-based field-level inference of growth rate from velocity and density fields ›
Proto-neutron star oscillations including accretion flows ›
The contribution of turbulent AGN coronae to the diffuse neutrino flux ›
The Tantalizing Case of the Quasar J0950+5128 -- I. Presentation of the Data and Detailed Exploration of the Binary Supermassive Black Hole Scenario ›
DESI DR1 Ly{\alpha} 1D power spectrum: The Fast Fourier Transform estimator measurement ›
Did the Corona Borealis-A2142 supercluster binary-like system originate as a proto-cluster binary embedded in a primordial cloud of galaxies? ›
A systematic search for AGN obscuration variability in the Chandra archive ›
The properties of primordially-seeded black holes and their hosts in the first billion years: implications for JWST ›
$w_{dm}$-$w_{de}$ cosmological model with new data samples of cosmological observations ›
Revealing Limitation in the Standard Cosmological Model: A Redshift-Dependent Hubble Constant from Fast Radio Bursts ›
Direct High-Resolution Imaging of Earth-Like Exoplanets ›
Gravitational lensing of fast radio bursts: prospects for probing microlens populations in lensing galaxies ›
Fast and "lossless" propagation of relativistic electrons along magnetized non-thermal filaments in galaxy clusters and the Galactic Center region ›
Stable Collisionless Tori Around Kerr Black Holes ›
The resummation model in FLAMINGO: precisely predicting matter power suppression from observed halo baryon fractions ›
Death by Impact: Evidence for Merger-Driven Quenching in a Collisional Ring Galaxy at Cosmic Noon ›
Can GRB 250702B be explained as the tidal disruption of a white dwarf by an intermediate mass black hole? Yes ›
LATIS Data Release: $\sim4200$ Spectra of $z \sim 2-3$ Galaxies, Redshifts, and Intergalactic Medium Tomography Maps ›
PAH Spectral Diversity in NGC 7027 and the Evolution of Aromatic Carriers ›
Multiple shells in supernova 2023ixf support the jittering jets explosion mechanism (JJEM) ›
Uncertainties in the production of iron-group nuclides in core-collapse supernovae from Monte Carlo variations of reaction rates ›
Primordial Black Holes from Kinetic Preheating ›
Redshift-Frame Systematics and Their Impact on the Hubble Constant from Pantheon+ Supernovae ›
Orbit Elements from Kepler Solutions in Projective Coordinates ›
Reheating and Inflationary dynamics driven by an inverse tangent potential ›
Deep-learning mitigation of foregrounds and beam effects in 21-cm intensity mapping using hybrid frequency differencing and PCA ›
Iron Nuclei in Ultra-High Energy Cosmic Rays Near the Earth ›
The MeerKAT Fornax Survey VI. The collapse of the galaxy HI Mass Function in Fornax ›
Ion-Scale Solitary Structures in the Solar Wind Observed by Solar Orbiter and Parker Solar Probe ›
The early universe is $\textit{ACT}$-ing $\textit{warm}$ ›
Dynamical dark energy parameterizations in VCDM ›
Observable signature of magnetic tidal coupling in hierarchical triple systems ›
Divergence in tracing the flavors of astrophysical neutrinos: can JUNO help IceCube? ↓↑