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

Stars over the dome

S Webcam

N Webcam

S Sky
Temperature
8.8 °C
Humidity
73%
Wind
0.0 km/h
Pressure
1017.3 hPa

Moon
Latest preprints on astro-ph:
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Consistent Treatment of Muons in Binary Neutron Star Mergers ›
Could the high-mass black holes from gravitational-wave observations be explained by lensing? ›
Deep Imaging Meets Motion: Complementing Stream Photometry Through Planetary Nebula Kinematics ›
Cold vs. Hot Gas Accretion and Angular Momentum in FIRE Simulations: From Halo to Galaxy Scales ›
Combining spectroscopy and wavefront control at deep contrast with photonic lanterns ›
Stream on: Evolution of stellar shells and streams - A case study ›
The splash beneath the largest radio bubble in a cluster core ›
Rapid-response 1.3 mm Observations of GRB 260127A with the Submillimeter Array ›
The Damping and Instability of Ion-acoustic Waves in the Solar Wind: Solar Orbiter Observations ›
An Improved Fit for Linear Halo Bias at High Redshift ›
The azimuthal structure of magnetically arrested disks during flux eruption events ›
The Atacama Cosmology Telescope: A Test of the Gravitational Force Law on Cosmological Scales Using the Kinematic Sunyaev-Zeldovich Effect ›
A fast X-ray transient with chromatic flares: signatures of violent collisions induced by late-time central engine reactivation ›
A Fast and Physically Grounded Ocean Model for GCMs: The Dynamical Slab Ocean Model of the Generic-PCM (rev. 3423) ›
GRB 210704A: A Luminous Fast Blue Transient in a GRB Afterglow at $z = 2.34$ ›
Simulating the interplay between the snowline pebble flux and ongoing planet formation and migration ›
Thermophysical Properties of Europa's Surface Constrained by Galileo Photopolarimeter-Radiometer Temperature Measurements ›
Synchrotron-cooled plasma distribution in the outer magnetosphere of a neutron star ›
FAIR Universe Weak Lensing ML Uncertainty Challenge: Handling Uncertainties and Distribution Shifts for Precision Cosmology ›
The Last Galactic Firework: Timing the last significant merger with stars, globular clusters and $\omega$Centauri ›
Forecasting neutrino mass constraints from the Nancy Grace Roman Space Telescope ›
Ultrahigh-energy cosmogenic neutrino emissions in the high-redshift universe ›
The GECKOS survey: Resolving the molecular and ionised gas in the galactic outflow of ESO~484-036 ›
Discovery of low-redshift analogues to "Little Red Dots" in DESI: A later evolutionary stage of compact LRDs? ›
Misaligned circumbinary discs around unequal-mass eccentric binaries: alignment, morphology, and binary accretion variability ›
Impact of Baseline, Cadence, and Host Contamination on AGN Variability Metrics: A Systematic Study with ZTF ›
Disk-like galaxies at 4 < z < 7.7 : JWST/NIRCam morphologies revealed by denoising VAE-GCNN classification ›
Upper bound of ejecta mass in a nova outburst ›
Revisiting Ca II Activity Indices in FGK Stars: Systematic Biases in Infrared Triplet Measurements ›
Closing the Observational Gap in Cosmic Dynamics: AI-Enabled Reconstruction of the Universe's Vorticity and Rotational Flow Morphology ›
Constraining Quintessential Inflation with ACT: A Gauss-Bonnet Gateway ›
A simple yet effective model of galaxy mergers ›
Tracking ionization balance in intergalactic medium and its implications towards metallicity ›
Systematic assessment of disk truncation in the black hole X-ray binary Swift J1727.8-1613 using NICER ›
FAST and Dark: A catalogue of Dark Galaxy Candidates within 50 Mpc ›
Influence of winds on shocked magnetized viscous accretion flows around rotating black holes ›
NOMAI : A real-time photometric classifier for superluminous supernovae identification. A science module for the Fink broker ›
Deeper analysis of Fermi-LAT unassociated 4FGL J2112.5-3043 for possible identification ›
Euclid. Populating a dark universe with galaxies using SciPIC ›
Numerical investigation of particle acceleration at interplanetary shocks: diffusive and superdiffusive scenarios ›
Sky background accounting in spectral infrared observations of extended objects at the Caucasus Mountain Observatory of the SAI MSU ›
Microscopic primordial black holes as macroscopic dark matter from large extra dimensions ›
ALMA-IMF XXII. Role of core subfragmentation in the IMF origin: Hierarchical fragmentation cascade and CMF in W43-MM1 ›
Enhanced activity in close dual-AGN systems in the local Universe ›
A simple relation: Neutron star magnetic field strength and spectral shape at low mass accretion rates ›
Do galaxy mergers increase star formation and turbulence at cosmic noon? ›
Cosmology of Inelastic Self-Interacting Dark Matter: Linear Evolution and Observational Constraints ›
A Generalized Algorithmic Framework for Detecting Faraday Rotation Measure Flares in Repeating Fast Radio Bursts ›
The multi-planet system TOI-5624: four transiting sub-Neptunes with an outer companion revealed by transit-timing variations ›
Structure and Large-Scale Kinematics of Young Stellar Populations in the NGC 6357 and NGC 6334 Giant Molecular Cloud Complex ›
Continuing to Advance European High Contrast Imaging Research and Development towards HWO and LIFE ›
An FUor-like Outbursting Class I Protostar in NGC 7538 ›
Photometric Metallicities for 367,324 stars of Omega Centauri ›
Localization and Confidence Region Estimation of Short GRBs with the COSI BGO Shield Using a HEALPix-Based Deep Learning Approach ›
Las Cumbres Observatory Gravitational-Wave Follow-up in O3 and O4: Strengths and Weaknesses of a Rapid Response Galaxy Targeted Strategy ›
Radiation doses during extreme solar energetic particle events ›
Understanding the regulation of star formation within TNG100 galaxies on kpc-scales using machine learning I: Global versus local ›
Stellar nucleosynthesis in the era of large surveys: s-process polluted binaries in GALAH DR4 ›
Photometry and physical characterization of near-Earth asteroid 2025 FA$_{22}$ from one apparition ›
Tracing evolutionary pathways of bar-driven quenching in local Universe disc galaxies ›
Nonperturbative stochastic inflation in perturbative dynamical background ›
Age bimodality in pseudo-bulges of barred spiral galaxies: Bar-driven evolution across cosmic time ›
Neutrino self-interactions in post-reionization era: Lyman-$\alpha$, 21-cm and cross-spectra ›
Cloudy with a chance of metals: Indications of CO$_2$ in the atmosphere of GJ 1214 b from high-resolution K-band spectroscopy ›
A Validated Low-to-Intermediate Mass Planetary Interior Structure Model and New Mass-Radius Relations ›
Gravitational-wave lensing beyond rays: a disordered-system approach ›
Correlative Microstructural Analysis of a Weathered Nantan Meteorite Fragment ›
Fast neural network surrogate for multimodal effective-one-body gravitational waveforms from generically precessing compact binaries ›
Quantum correction to the diffusion term in stochastic inflation from composite-operator matching in Soft de Sitter Effective Theory ›
Emergent structure in the binary black hole mass distribution and implications for population-based cosmology ›
Astrophysical bounds on the high-energy evolution of neutrino mixing ›
Inflaton Regeneration via Scalar Couplings: Generic Models and the Higgs Portal ›
Exploring non-equilibrium effects in sequential freeze-in ›
Nonlinear backstepping with saturation for low-thrust station-keeping of libration point orbits ›
Static Tidal Perturbations of Relativistic Stars: Corrected Center Expansion and Love Numbers-I ›
Boson star-black hole binaries: initial data and head-on collisions ›
Echoes of Global Cosmic Strings ›
DESI Dark Secrets ›
Disentangling the galactic and intergalactic components in 313 observed Lyman-alpha line profiles between redshift 0 and 5 ›
Initial Characterization of Stellar Photometry of Roman images from the OpenUniverse Simulations ›
From the Densest Clusters to the Emptiest Voids: No Evidence For Environmental Effects on the Galaxy Size-Mass Relation at Low Redshift ›
Multidimensional Nebular-Phase Calculations of Dynamically-Driven Double-Degenerate Double-Detonation Models for Type Ia Supernovae ›
A Systematic Search for Active Galactic Nucleus Flares in ZTF Data Release 23 ›
Using Symbolic Regression to Emulate the Radial Fourier Transform of the S\'ersic profile for Fast, Accurate and Differentiable Galaxy Profile Fitting ›
Constraining Gas Mass Fractions in Galaxy Groups and Clusters with the First CHIME/FRB Outrigger ›
The evolution of the galaxy stellar mass function and star formation rates in the COLIBRE simulations from redshift 17 to 0 ›
Improving radial velocity precision with CARMENES-PLUS:An upgrade of the near-infrared spectrograph cooling system ›
WaveDriver: a Laser Guide Star AO System for HWO ›
Impact of Cosmic Filaments on Galaxy Morphological Evolution and Predictions of Early Cosmic Web Structure for Roman ›
GravSphere2: A higher-order Jeans method for mass-modeling spherical stellar systems ›
Finding Supermassive Black Hole Binary Mergers in Pulsar Timing Array Data ›
Image reconstruction with the JWST Interferometer ›
The THESAN project: Lyman-alpha emitters as probes of ionized bubble sizes ›
High-resolution radio imaging of TGSSJ1530+1049, a radio galaxy in a dense environment at z=4 ›
Nested Sampling for ARIMA Model Selection in Astronomical Time-Series Analysis ›
Cosmic Duets I. High-spatial resolution spectroscopy of dual and lensed AGN with MUSE-NFM ›
Observational constraints on the origin of the elements. X. Combining NLTE and machine learning for chemical diagnostics of 4 million stars in the 4MIDABLE-HR survey ›
Constraining primordial non-Gaussianity from DESI DR1 quasars and Planck PR4 CMB Lensing ›
New $H(z)$ measurement at Redshift = 0.12 with DESI Data Release 1 ›
Closed-Form Statistical Relations Between Projected Separation, Semimajor Axis, Companion Mass, and Host Acceleration ›
Polarimetry and albedo of the Near-Earth Asteroid 2025 FA22 ›
PDRs4All XVIII. JWST-NIRCam Photometric properties of protoplanetary disks in the Orion Nebula Cluster ›
Spectral Hardening Revealed by Geometric De-boosting in the Masked Jet of PKS 2155$-$304 ›
CTAO Simulations for Potential PeVatron Candidates ›
New black hole mass calibrations and the fundamental plane of the broad-line region size, luminosity, and velocity ›
Predictions of Stellar Occultations by Haumea and the Event of 4 May 2026 ›
Atmospheric Supply of Hydrogen Cyanide Is Not the Rate-limiting Step for Prebiotic Chemistry across Rocky Exoplanets ›
Finding the elusive RR Lyrae companions via speckle imaging ›
Holmberg IX: A Unique, Infant but Inactive Galaxy as Revealed via a Multiwavelength Approach ›
Wide Jets or Low Rates: Reconciling Short GRB and Gravitational-Wave Neutron Star Merger Rates ›
Low-ionization Metal Absorption at $0.7 \lesssim z \lesssim 2$ Confronting Cosmological Simulations with Observations ›
Reionization Topology as a Probe of Self-Interacting Dark Matter ›
Finite temperature effects on g-modes of inviscid neutron stars ›
The Identification of CS2 and Evidence for Carbon-Sulfur Chemical Coupling in a Warm Giant Exoplanet Atmosphere ›
The DECam MAGIC Survey: Investigating the Jet Stellar Stream with Photometric Metallicities ›
CHARA Interferometry and TESS Asteroseismology of the Core-Helium Burning Red Giant $\kappa$ Cyg ›
CHILES XII: The H I evolution of Luminous Compact Blue Galaxies between 0 ›
Radiative cooling effects on black hole hot accretion flows around the sub-Bondi radius ›
A Salpeter-like filament linear density function across nearby molecular clouds ›
Dark matter and modified gravity: Einstein clusters from a non-minimally coupled vector field ›
WIMP/FIMP dark matter and primordial black holes with memory burden effect ›
Asymmetric Cannibal Dark Matter: Constraints from Neutron Star ›
Imperfect dark matter with higher derivatives ›
Exact black holes and black branes with bumpy horizons supported by superfluid pions ›
On the Cuspy Structure of Rotating Wormhole Shadows ›
Towards a complete theory of thermal leptogenesis in the SM and MSSM ↓↑