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
16.8 °C
Humidity
64%
Wind
1.6 km/h
Pressure
1015.9 hPa

Moon
Latest preprints on astro-ph:
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G(2) Glueball Boson Stars as Restricted Kerr Mimickers in the Thomas--Fermi Limit ›
Magnetic destabilisation in disc galaxies: Filament/feather formation ›
AXIS Could Have Accessed Dark Matter Decays ›
Spatially-Resolved Spectra of Diffuse Galactic Light using 10.8 M DESI Sky Fibers ›
The GECKOS survey: Assembly history of the lenticular galaxy NGC 3957 ›
Super-Eddington Little Blue Dots May Reionize Helium Too Early ›
Galactic Science with Ultra-High Angular Resolution X-ray Imaging ›
Shock-heated Away: The Impact of Radiative Cooling on Gas-Phase Transitions in Supernova Remnants ›
On the Impact of Correlated Noise and Spectral Resolution on the Retrieval Analysis of the Habitable World Observatory ›
Impacts of Correlated Noise on Retrievals of Exo-Earth Atmospheres ›
Decisive evidence for a global cosmic-ray feature in gamma-ray data ›
Investigating the magnetic field in the inter-cluster filament between Abell 3667 and Abell 3651 with POSSUM ›
Comment on `Measuring the Hubble Constant Using Strongly Lensed Gravitational Wave Signals' ›
Radio-dust connection in quasars driven by powerful ionised outflows ›
Probing the Taxonomic Diversity of the Small Near-Earth Object Population ›
Reconstructing stochastic gravitational-wave signals from flavour deconstruction with LISA ›
X-ray grating spectroscopy as a mission enhancement ›
The Hot, Continuum-compact State of the Yellow Hypergiant V509 Cassiopeiae: CHARA Diameters, CO-band Angular-extension Constraints, and Companion Limits ›
Exploring the trade-space of distributed aperture telescopes for faint-object spectroscopy ›
96 kHz on-sky imaging on an adaptive optics system with a single-photon avalanche diode ›
Statistical Energy Budget of the Solar Wind with Parker Solar Probe and Solar Orbiter : 1 - Unbalanced Total Energy Radial Evolution ›
A Terrestrial Gamma-ray Flash with an Asymmetric Footprint Observed at the Pierre Auger Observatory ›
Pre-shipment optical characterization of the SCALES instrument ›
Magnitude of stable iron isotope fractionation limited by multiple stages of terrestrial core formation ›
A Self-Sustaining Black Hole Engine Powered by the Tidal Disruptions of Stars ›
Anomalous horizontal track-like events at the HAWC observatory: candidate neutrino-induced charged leptons from the Pico de Orizaba volcano ›
Little Red Dots as Shock-Powered High-Energy Neutrino Sources ›
Estimation of Dust Mass from Infrared Emission and Extinction of Supernova Remnants: G93.7-0.2, G109.1-1.0, G156.2+5.7, and G166.0+4.3 ›
Can Little Red Dots Contribute To The Early Universe Cosmic Dust Budget? ›
First overnight balloon flight of the GRAINE 2023 emulsion gamma-ray telescope enabled by a large-scale pressure-vessel gondola ›
Primordial black holes and induced gravitational waves from localized features in DBI inflation ›
Evidence for an accretion-driven subpopulation of black holes in GWTC-5.0 ›
Dynamical Mass Demography of Single S-type Planets Shaped by Stellar Companions ›
How nanoscale physics shapes ice formation in the Universe: Rethinking gas freeze-out on dust grains ›
The Cygnus Allscale Survey of Chemistry and Dynamical Environments: CASCADE: VI. Molecular outflows in the DR21 ridge ›
The onset of the strong backreaction regime in axion inflation, an analytical study ›
Evolution of Stellar Activity and Habitable Zone (EATEN): III. X-ray Activity of Dwarfs in Open Clusters and Field Stars ›
The refractory fraction of phosphorus in planet-forming discs ›
On the Effect of Large Scale Structures and Turbulence on Solar Eruptive Events: The Cross-Scale Challenge for Space Weather ›
Rapid Energy Dissipation by Colliding Waves in Strongly Magnetized Plasmas ›
Characterization of the stabilized nulling interferometry testbed PERS\'EE ›
BSN-VII: Photometric Light Curve Study of Three Cool, Large-Amplitude, Low Mass, W-Subtype Contact Binaries ›
A semi-analytical surrogate model for giant planet evolution: bypassing ordinary differential equation solvers with localised thermodynamics, softplus asymptotes, and B-spline photometry ›
MEGARA Stellar Spectral Library. Second Release ›
Photon--Dark Matter Elastic Scattering: An Effective-Operator Scan and First Operator-Resolved Sensitivity Estimates from the Galactic Halo ›
AO3k + SCExAO: on-sky wavefront quality and demonstration of novel WFS techniques with the double XAO system ›
Self-calibration of adaptive optics systems. Application to the THEMIS solar telescope ›
Tracing Radial Migration in the Outer Disk: A Comprehensive Analysis of the Old Open Cluster Berkeley 36 ›
Origin of small-scale evaporation flows deep in the chromosphere during a solar flare ›
Microchannel plate detector development for ultraviolet astronomy ›
The multi-frequency radio light curve of the sub-pc SMBH binary candidate PG 1302-102 ›
Spheroidal Resampling Analysis of High-Redshift Gamma-Ray Burst Spatial Densities ›
Gemini and Apache Point Multi-band Optical Imaging Characterization of Fragmenting Long-period Comet C/2025 K1 (ATLAS) ›
Primordial Black Hole Seeds for Little Red Dots in $f(R)$ Gravity ›
Soft proton experiments supporting the development of astronomical X-ray instrumentation ›
Type I Solar Radio Bursts Modulated by Solar Flares ›
Ion-Scale Waves Regulated by Plasma Beta and Cross Helicity: Observational Evidence for the Helicity Barrier in Imbalanced Solar Wind Turbulence ›
A generalized likelihood model for segmented muon counters ›
Probing Triton's Space Environment and Internal Structure: An Integrated Detection-and-Interpretation Framework ›
The Structural Abundance Crisis of Massive Galaxies in Current Cosmological Simulations ›
Multiscale Synthetic observations of Polarized dust emission: On the origin of Depolarization effect from Molecular clouds to Starless cores and Constraints on Dust Physics ›
Caught Napping by JWST UNCOVER+MegaScience: Constraining bursty star formation histories and number densities of mini-quenched galaxies at redshifts 4-7 ›
Vortex pinning and the elastic response of neutron-star crusts - I. Axisymmetric loading ›
The $\gamma$ Cephei System: Updated Orbits, Dynamical Architecture, and Limits on Additional Companions ›
Advancing Fundamental Physics and Cosmology with high-resolution X-ray imaging ›
Intermediate-mass runaway and hypervelocity star candidates in DESI DR1 ›
Host Dependence and Line-of-Sight Effects on Galaxy-Galaxy Strong Lensing in Clusters ›
CRUX: A topology-aware load balancer for mesh-based fluid dynamics codes on GPU clusters ›
Atmospheric escape fractionates secondary but not primary atmospheres ›
Moment-based formulas for the transport coefficients ›
Empirical Constraints on the CO Snowline Transition in HD 163296: The Local CO Column and $^{13}$C$^{18}$O Optical Depth ›
OB stars identified in LAMOST Data Release 10 ›
Systematic and Statistical Properties of Prominence Eruptions on the M-dwarf YZ CMi ›
SN 2019cqc: A Hydrogen-rich Superluminous Supernova Showing Electron-Scattering Signatures ›
Testing SALT Approximations with Numerical Radiative Transfer Code. II. Thermal and Microturbulent Line Broadening ›
Hunting the nature of the Seyfert 1 galaxy GRS 1734-292: can it be a gamma-ray emitter? ›
Planar Three-Body Problem: theoretical predictions and simulation results ›
Broad-band host measurements of little red dots and similar compact nuclei require source-conditioned polychromatic PSFs ›
SNAD: enabling discovery in the era of big data ›
Phosphorus abundances and multi-element co-enrichment in nearby FGK stars ›
ALMA Observations of DEM L241/LMC P3 in the Large Magellanic Cloud: Evidence for the Formation of Cool Molecular Jets Driven by a Microquasar ›
Photometric redshifts for active galactic nuclei with LePHARE for the Vera C. Rubin Observatory ›
Thermodynamic reconstruction in observationally constrained dynamical dark energy models ›
DINOspec: Efficient Multimodal Alignment of Vision and Spectral Foundation Models for Astronomy ›
Equilibrium \(\mathrm{H}_2^+/\mathrm{H}^-\) Abundance Ratios in MARCS Atmosphere Models ›
Joint Observations of PTPS Targets (JOTA). Combined spectroscopic and photometric analysis of 16 SB1 systems ›
Interferometric Survey of Stellar Parameters: Towards homogeneous FGK stars parameters and surface-brightness color relation in the context of PLATO space mission ›
Cascades from ultra-high-energy neutrinos ›
Learning Radio Astronomical Representations with LeJEPA and Very Small Models ›
TeV Gamma Rays and Neutrinos from Winds Driven by Radiatively Inefficient Accretion Flows of Low-Luminosity Active Galactic Nuclei ›
Not all those missing are lost: leveraging galaxy clustering in incomplete catalogs to unleash dark sirens cosmology ›
Astrometric modeling of unresolved variable binary systems. II. Application to Gaia epoch astrometry of nearby pulsating and convective red giants ›
On-sky demonstration of a vector Zernike wavefront sensor in a cascaded adaptive optics system ›
STOKES tables and KY codes ›
Constraining Baryonic Feedback at $z\sim 1$ with the H$\alpha$ Luminosity Function ›
The umbrella effect: Magnetic canopy topology modulates spatially averaged chromospheric three-minute power ›
Magnetohydrodynamics of charged interstellar dust. Multifluid models and study of the linear modes ›
A consistent, physical, and analytical model for CMB observables of reionisation I. Derivation, constraining power, and detectability of the auto-spectra ›
Radio measurements of air showers with the IceCube-Gen2 surface prototype station at the Pierre Auger Observatory ›
Stellar streams around dwarf galaxies are observationally rare in the local Universe ›
Study of Butterfly-Shaped Coronal Hole Evolution Across the Solar Disk ›
Cosmic variance and ergodicity in finite systems with correlations ›
Extremes of solar spectral irradiance in the SORCE/XPS record ›
Beyond $X_\mathrm{max}$ : Reconstructing Air Shower Profiles with Information Field Theory with SKA-Low ›
Measuring peculiar velocity and tomographic redshift dipole with DESI DR1 catalogs ›
The DSA/Chronoscope fast radio burst survey: forecasts and science overview ›
From spectroscopic abundances to evolutionary [$\alpha$/Fe] in stellar models ›
\"Opik-type collision frequency for Kozai-driven projectiles: Target bodies on eccentric and inclined orbits ›
Resonant Dynamics of Gravitational Wave and Chiral Alfv\'en wave in the Early Universe ›
METIS high-contrast imaging simulations: From instrument modelling to science readiness ›
The First Array-Wide Diffuse Flux Search for UHE Neutrinos with the Askaryan Radio Array ›
ALMA CO(2-1) Gas Dynamics in NGC 315: A Multi-Method Benchmark for Supermassive Black Hole Mass Measurement ›
The Auger Radio Infill SKALA Extension (ARISE): Science Case and Instrumentation (ARENA 2026) ›
Feasibility of Capillary-Driven Orbital Liquid Mirror Telescopes ›
Accretion Rates and Thermohaline Convection in Polluted White Dwarfs ›
SPT-3G D1: Quadratic-Estimator CMB Lensing Reconstruction and Cosmology ›
The impact of hot mode accretion and angular momentum conservation on metallicity gradients of galactic discs ›
The Analysis, not the Aperture: End-to-End Transformer Reconstruction for Imaging Atmospheric Cherenkov Telescopes ›
Slysh haloes: the waste heat of cold computing as a submillimetre technosignature ›
Ad Astra White Paper: A Pitch for the Next 25 Years of NASA's Physics of the Cosmos Program ›
Agentic research is oxymoronic ›
Geometrothermodynamics and critical behavior of regular black holes ›
Phase Transitions, Shadows, and Microstructure of Kerr-anti-de Sitter Black Holes from Geometrothermodynamics ›
Shadow and Thermodynamics of deformed Schwarzschild-AdS black hole with a Cloud of Strings embedded in Perfect Fluid Dark Matter ›
Probing Black Hole Thermodynamics and Microstructure via the Shadow of Sagittarius A* ›
Testing $f(Q)$ Gravity with DESI DR2 and Strong-Lensing Time Delays ›
Fluxes through a uniform double-diffusive staircase at low Prandtl number ›
Inspiralling Binary merger parameter reconstruction with lunar and satellite Laser Ranging ›
Internal heating in rapidly rotating convection is not a shortcut to geostrophic turbulence ›
Geochemical Hazard Assessment of Martian Regolith for Future Human Exploration ›
Strongly coupled quark matter in neutron stars and their mergers ›
Automated identification and subtraction of gravitational-wave glitches using boundary refinement ›
How much of the black hole ringdown is sourced within the light ring? ›
Imaging Stars at the Quantum Compatibility Limit ›
Seesaw and Axion in No-Scale Gravity ›
Building a Better Beta: Nucleation and Timescales in Cosmological Phase Transitions ›
NS-UNO: Neutron Star EoS Inference from an Unconstrained Number of Observations ›
Constraining equation of state of neutron star using neutron star-black hole mergers ›
Bekenstein--Hod Bound: A $3.3\sigma$ Confirmation from GW250114 ›
Evolution of Cosmic String Loops under Gravitational Backreaction ›
Accelerating Stochastic Gravitational Wave Backgrounds Parameter Estimation in Pulsar Timing Arrays with Flow Matching ›
The Stochastic Siren: Astrophysical Gravitational-Wave Background Measurements of the Hubble Constant ›
What we have not learned about the dark energy equation of state? ›
Gravitational Wave with Domain Wall Dominance ›
Euclid preparation. XCI. Validation method for the detections in the Euclid Catalogue of Galaxy Clusters using external data ›
Nulling baryonic feedback in weak lensing surveys using cross-correlations with fast radio bursts ›
Dark forces suppress structure growth ›
The Lensing Counter Narrative: An Effective Description of Small-Scale Clustering in Weak Lensing Power Spectra ›
The Sagittarius C Complex in the Mid-Infrared with SOFIA/FORCAST ›
How Primordial Black Holes Change BBN ›
A source-plane reassessment of the z=6--8 ultraviolet luminosity function behind Abell 2744: no requirement for additional faint-end curvature ›
Simulation Study of Binary Mergers of Galaxy Clusters I: Properties of Merger Shocks and Radio Emission ›
A Universal Bilinear Model for the Dependence of Void Asymmetry Distributions on $\Omega_{m}$ and $\sigma_{8}$ ›
Cosmogenic 10Be as a Tracer for Recent Heliospheric Encounters with Interstellar Cold Clouds ›
Direct Detection of Type II-P Supernova Progenitors with the $\textit{Euclid}$ and CSST Surveys ›
Intracluster light as a dark matter tracer: how their spatial and kinematic relationship is shaped by satellite demographics ›
Efficient reduction of stellar contamination and noise in planetary transmission spectra using neural networks ›
Constraining Axion-like Particles through Multi-epoch Monitoring of Strong Gravitational Lenses ›
The origin of isolated millisecond pulsars in globular clusters ›
Accretion in Binary Systems with Slow Stellar Winds ›
Thermal enhancement of inflationary magnetic fields ›
Three-band dark-siren cosmology with intermediate mass black hole binaries: Synergy of Taiji, LGWA, and the Einstein Telescope ›
Mapping of the Cold Neutral Medium via HI Phase Separation in an Atomic Cloud Undergoing Molecular Cloud Formation ›
Perturbative Effects of Dark Matter Environments on Black Hole Shadows ›
High-redshift physics from the acoustic scale ›
A Century of Radial Velocity and Astrometric Monitoring of 70 Oph AB: New PFS Data and Constraints on Planetary Companions ›
Revisiting the Claim for a Direct-Collapse Black Hole in UHZ1 at $z=10.05$ ›
A statistical study of the environmental age of core-collapse supernovae based on VLT/MUSE integral-field-unit spectroscopy ›
From NVSS to RACS: Identifying truly Compact Galactic and Extragalactic sources with Steep Spectra ›
SCAT Data Release 1: 1812 optical spectra of 1331 transients ›
The GMRT High-Resolution Southern Sky Survey for pulsars and transients -- VIII: Orbital Variability and the Evolution of a 1-Day He-WD Millisecond Pulsar J2101-4802 ›
Euclid preparation. Testing template-fitting models for the multipoles of the two-point clustering of galaxy clusters ›
Implications of SARAS3 data for Coulomb-like interacting dark matter ›
Joint XMM-Newton and NuSTAR Observations of Type I X-ray Bursts from the Dipping Low-Mass X-ray Binary 4U 1323-62 ›
The EDGES Analysis Pipeline: Description and Validation ›
QPEs from Warped Disk Collisions with EMRIs: Brightness-Recurrence Diagram and Gravitational-Wave Follow-up ›
Fast radio bursts, magnetars and earthquakes: their "family feud"? ›
Reconstructing the orbits of Milky Way dwarf galaxies: A Large Magellanic Cloud perspective ›
Misspecification in amortized X-ray spectral inference: a detection benchmark, a gain shift three schemes cannot see, and marginalizing it out ›
The Chirp-Mass Ladder: A New Rung Emerges ›
Compact Core, Extended Reach: A Bipolar kpc-Scale Elongation in a Little Red Dot at $z \approx 5.5$ ›
Solitary dwarf galaxy groups as tracers of dark matter halos in the local Universe ›
Statistical Field Theory for Weak Gravitational Lensing ›
Photochemical Production of CS2 in Temperate-to-Warm Gas Giant Exoplanet Atmospheres ›
An SKA-Low RM Grid for constraining the origin of cosmic magnetism ›
How Low Can We Go? Minimum Spectroscopic Requirements For Supernova Subtype Classification ›
A Universal Relation Between Primordial Density-Potential Cross-correlation Coefficient and Spin Factor Distribution ›
Rolling Galileons: Evolving Braiding Strength for Viable Dark Energy ›
Probing Dark Matter Substructure with Wave-Optics Distortions of Strongly Lensed LISA Gravitational Waves ›
From compact jets to extended lobes: radio morphologies of distant quasars at z > 4 ›
Multi-branch classification of diffuse cluster radio emission from the LOFAR two-metre sky survey ›
Investigating radio source population and spatial characteristics of diffuse Galactic synchrotron emission in the GAMA-23 field with uGMRT Band-3 ›
Determining low-$\ell$ p-mode frequency shifts in Sun-like stars: Enhancing the cross-correlation technique with filters ›
Constraining Cosmic-Ray Acceleration and Escape in Middle-Aged Supernova Remnants with GeV-TeV Gamma-Ray Observations ›
Inferring the Dark from the Observable: Estimating Halo Masses Using Galaxy Properties ›
ALMA high resolution observations of Betelgeuse: Persistent structure spanning the inner atmosphere ›
A Prediction for DESI Full-Shape: Increasing Tomographic $\Omega_m(z)$ Trend ›
A Highly Reflective Atmosphere on the Lava World TOI-561b Revealed by JWST/NIRSpec Phase Curve ›
BlueBird 6 is Fainter than Block 1 Satellites ›
The solitary star cluster of the Andromeda XXV dwarf spheroidal ›
Dynamically driven collapse of a thermally stable accretion disk in a nova-like system ›
Examining the possibility of a thick crust in the compact stellar object HESS J1731-347 ›
Towards First Detection of the Solar MSW Transition With JUNO ›
The gravitational wave landscape of cosmic string networks with varying tension ›
Spin Light of neutrino in polarized matter ›
Primordial features as probes of baryogenesis from supersymmetric flat directions ›
Collisionless relaxation as the origin of the anisotropic, non-thermal, and multi-temperature momentum distributions observed in space plasmas ›
Electroweak Doublet Dark Matter for a Galactic Halo Gamma-Ray Excess ›
Cosmological Collider Signals at Strong Mixing ↓↑