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

Sunset view from dome

S Webcam

N Webcam

S Sky
Temperature
15.2 °C
Humidity
76%
Wind
3.2 km/h
Pressure
1009.9 hPa

Moon
Latest preprints on astro-ph:
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Engineering of titanium transition edge sensor wafers for the BA4-90/150 receiver of BICEP Array ›
Best practices for obtaining astrometric observations from JWST (274) NIRCam data ›
Alfred: A Flexible, User-Friendly Python Package for Exoplanet Confirmation ›
Radio Monitoring of the Changing-look AGN Mrk 590 I: VLA Observations Reveal A Bow-shock Driven Radio Brightening Event ›
Primordial Black Holes as Cosmic Architects: Imprints of an extended mass function ›
Scatter, bias, and chaos of satellite orbits in triaxial dark matter haloes ›
SOAR TESS Survey III: Mapping the Stellar Companion Deficit around TESS Planet Candidates ›
Barren but not Empty: The Impact of Void Environments on Galaxy and Halo Populations ›
A Broken Clock Is Right Twice a Day: [Ce/Mg] Is Not a Universal Chemical Clock ›
Assembly bias from nuisance to probe II: Salvaging linear clustering from DESI and SDSS data ›
The origin of the stellar mass-size relation of satellite galaxies in the COLIBRE simulations ›
$\texttt{SPINE}$: Symbolic Models to Predict the Evolution of the $\Lambda$CDM Nonlinear Power Spectrum ›
Using CFHT's SITELLE to Probe the Long-Sought Supernova Remnant Shell in the Crab Nebula ›
The host galaxies of 2003fg-like type Ia supernovae ›
Paleo-Detectors as a Novel Probe of Dark Matter-Nucleus Effective Interactions ›
Synchrotron self-Compton Reverse Shock in Energy-Injection and Radiative Scenarios ›
Phase-Space Diagnostics for Dwarf Galaxies in Cluster Environments ›
The Impact of Magnitude Uncertainties and K-corrections on Standard Siren Measurements of the Hubble Constant ›
Active nests at solar maximum: How nested flux emergence dominated flaring activity and structured the heliosphere ›
Non-equilibrium condensation of the first Solar System solids ›
The MegaWave Radio Surveyor ›
RadialPaths: Radial profiles in multi-centred astronomical structures ›
HOLISMOKES -- XVIII. Cosmology with strongly lensed type II supernovae: Effects of instrumental setups on $H_0$ ›
COSMOS-Web: From early star-formation enhancement to late suppression in galaxy groups ›
Cross-simulator transfer with foundation model summaries: Towards robust SKA-era reionization inference ›
Microscopy assessment of two multiple-transient candidates ›
Diversity of stripped-envelope supernova light curves from interaction with binary-driven circumstellar material ›
Path to Black Hole Astrometric Microlensing from 10-Year KMTNet Database ›
Numerical modelling of recombination-driven stellar winds ›
Fine-scale flare structures and their energetic implications from short-exposure extreme-ultraviolet imaging ›
Systematic uncertainties on DESI Tully-Fisher distances constrained with Integral Field Spectroscopy ›
A radio continuum view of Stephan's Quintet: age, dynamics and origin of the shock ›
Revisiting the Hubble tension with an inverse power-law early dark energy ›
Visualizing Disequilibrium: Tracing Two-Point Correlations to Specific Spatial Structures in the Milky Way ›
Background Intensity Estimation for Cassini-ISS Image Using Deep Learning-Based Diffusion Model ›
Two Predicted, Concentric Nova Shells Surround the Prototype Dwarf Nova U Geminorum ›
FRB 121102: No supernova-like ejecta or magnetar power, hinting at a binary WD merger ›
Approximating the peculiar velocity distribution of dark matter halos with Tsallis statistics ›
Investigating the disappearance of a type-C QPO in black hole X-ray binary Swift J151857-572147 with AstroSat ›
Bifrost spectral inversions, Fast non-LTE solar chromospheric diagnostics from 3D simulations ›
Spectro-Polarimetric Properties of CHIME FRB Sources ›
Optical Discovery of New and Candidate Galactic Supernova Remnants Plus Optical Imaging of the Monogem Ring Supernova Remnant ›
ELUCID-DESI II. Revealing dark matter mass, tidal, and velocity (MTV) fields using galaxy group phase information ›
ANRe-M1: a GPU-accelerated numerical relativity code with multi-energy M1 neutrino transport ›
SERENADE III: Insight into the Origin of the High Dust Temperature and High [O III]/[C II] Ratio at $z\gtrsim6$ ›
Carbon in J0815+4729: Casting A Shadow of Doubt on the Interpretation of CH Absorption in the Most Primitive Stars ›
Classical Cepheids in the JWST and Roman Era: A New Theoretical Framework and its Metallicity Dependence ›
Study on the Venusian Atmospheric Thermal Structure: A Comparative Analysis between VEX/Akatsuki and Venus-GRAM/VCD ›
Derivative hierarchy as the origin of kernel-dependent trends in Gaussian process reconstructions of the hubble parameter ›
Alkali lines at extreme densities and their impact on giant planet interior structure ›
Energy-dependent slow collective flavor conversion of supernova neutrinos ›
A Bayesian Framework for Constraining Magnetar Magnetic Fields from Repeating FRB Statistics ›
The true masses of radial-velocity exoplanets constrained by stability ›
Bumpy inflation from explosive particle production ›
Not so typical doubly eclipsing systems ›
Anisotropy-driven constraints on the transition from Galactic to extragalactic cosmic-ray sources ›
Three-dimensional SPH simulations of the Caloris basin-forming impact: basin scaling, the gravity anomaly, and antipodal effects ›
The solitary star cluster of the Andromeda XXV dwarf spheroidal ›
HURACAN: A comparison of stellar and interstellar proper motions inside L1688 ›
Source models of ultrahigh-energy cosmic rays ›
Catastrophic tidal disruption of heterogeneous rubble piles: a tale of two regimes ›
Narrow-Shell Stochasticity in Source-Sink Models of the Low Earth Orbit Environment ›
NGTS clusters survey - VI: Stellar rotation in seven young open clusters within the PLATO LOPS2 field ›
Optimal transport regularized dynamic radio interferometric reconstruction ›
Testing Narrow-jet Gamma-Ray Bursts as Sources of Ultrahigh-Energy Cosmic Rays ›
Bright Metal-Poor Star Survey - I. Tomo-e Gozen narrow-band photometric survey and medium-resolution spectroscopic follow-up ›
Towards the exploration of astrophysical datacubes through volumetric rendering within CARTA ›
Revisiting the enigmatic sixth star cluster in the Fornax dwarf spheroidal galaxy ›
Exploring the survivability of higher-order multiple protostellar systems -- The case of VLA1623 ›
Panchromatic Spectra of Nearby Low-mass and Sun-like Stars with Directly Imageable Habitable Zones ›
Dust torques for realistic dust size distributions ›
$N$-body simulations of the open cluster population in the Milky Way and the impact of GMC encounters ›
Non-isothermal vertical distribution functions for the Milky Way ›
Near universality of nonlinear transverse and radial velocity responses in spherical collapse with arbitrary radial profiles ›
The MICADO first light imager for the ELT: first on-bench performance tests of the SCAO hybrid LQG+Integrator controller ›
LightCube: A Parsec-Resolution 3D Model of the Local Far-Ultraviolet Interstellar Radiation Field ›
Map of the Interstellar Continuum FUV Field within 800 Parsecs ›
An Equation of State for Supercritical Silicate-Hydrogen Mixtures at Sub-Neptune Interior Conditions ›
The JWST/NIRCam Scattered Light Disks GTO 2780 program: panchromatic coronagraphic imaging of the HD 10647, HD 32297, HD 61005, HD 107146, and HD 181327 debris disk systems ›
The Atacama Cosmology Telescope: Constraints on the anisotropic screening and birefringence effects with DR6 ›
Deuterium Production in an Effective Field Theory Constructed from On-Shell Amplitudes ›
Spatially Scanned STIS Spectra of the Exoplanet Host Star 55 Cnc ›
Impact of Nuclear Level Density on $r$-Process Rare-Earth Peak Nucleosynthesis ›
Getting Warmer: IceCube Nears Freeze Out ›
Effects of the interaction of dark matter and neutron-star matter on extreme and intermediate mass-ratio inspirals ›
Direct and Indirect searches for DM-electron interactions in sub-GeV DM models ›
$\mu$DM: a new mechanism for the baryon-dark matter coincidence ›
Scale Invariance and Compact Star Matter ›
Quantum Selection of Classical Histories ›
Mixed Dark Matter and Galaxy Clustering: The Importance of Relative Perturbations ›
Lyman-alpha emission at the end of reionization: line strengths and profiles from MMT and JWST observations at z~5-6 ›
Assessing Self-Absorbed Molecular Lines as Tracers of Gravitational Collapse ›
Updated constraints on interacting dark energy: A comprehensive analysis using multiple CMB probes, DESI DR2, and supernovae observations ›
Quantifying Systematic Age Discrepancies in Very Young Star Clusters ›
On Lorentz Variability of Magnetically Dominated Relativistic Outflows ›
Fisher Forecasts for Cosmological Yields from $3\!\times\!2$pt Analysis of the Roman Space Telescope High Latitude Imaging Survey ›
Cluster number counts in dark energy model with energy and momentum coupling to dark matter ›
The origin of isolated millisecond pulsars in globular clusters ›
Impact and interplay of $\Lambda$CDM analysis choices for LSST cosmic shear ›
Redshift evolution of the Hubble constant: Constraints and new insights from an interacting dark energy model ›
Effects of resolution and local stability on galactic disks: Halo resolution and softening on bar formation ›
The baryon content of magnetically arrested black hole disks and jets ›
Weak-lensing Analysis of Intracluster Filaments in Abell 2744: Matched-filter Scans and Stepwise 2D Tracing ›
The Neptunian ridge planet WASP-156 b does not have a polar orbit ›
TRINITY: A coupled model of winds, radiation, and photoionised gas in molecular clouds. I. Methods and validation ›
SMUGGLE-Ring: Evolutionary link between nuclear star cluster and nuclear disk ›
Probing a new subclass of llGRB-SN transients: Insights from EP250304a and its associated supernova ›
Angular momentum evolution in the CIELO simulations. I. Temporal evolution of gas-stellar misalignments and baryonic merger timing ›
AutoClassMK: A public neural network for automatic 2D MK classification of normal stars in basic Python ›
The limits of lattice inflation: a cautionary tale ›
Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data ›
Lower Your Rates: On Claims of a Binary Black Hole Merger-Rate Crisis ›
The Impact of Non-Gaussian Line Spread Functions on Stellar Kinematic Recovery: Consequences for Dynamical Models ›
Archival Diagnostics for Potential Background Contaminantsof Project Hephaistos Dyson Sphere Candidates ›
Refined reduction and standardisation of 53 years of UBV photometry at Hvar ›
Tracing black hole and galaxy growth across environments since cosmic noon ›
Atmosphere mitigation in CMB observations using multi-frequency time-domain component separation ›
Exploration of Exoplanet Atmospheres with the James Webb Space Telescope ›
The Tidal Venus Phenomenon: Demographics and Case Studies ›
Dipolar power asymmetry in wide-angle correlations of galaxy density, velocity and ellipticity ›
The First X-Ray Polarimetry of the Typical Accretion Disk Corona Source 4U 1822-37 ›
Energy Partition in AGN-driven Bubbles of NGC 4438: From Nuclear Bubbles to a Galaxy-scale Outflow ›
Indirect Searches for Dark Photon-Photon Tridents in Celestial Objects ›
How light can ALP dark matter be? ›
Generalized JMN Naked Singularity Models ›
Gravitational wave signal and noise response of an optically levitated sensor in a Fabry-P\'erot cavity ›
Primordial Magnetogenesis and Gravitational Waves from ALP-assisted Phase Transition ›
Gravitational-wave astronomy with a space-based optical clock network ›
When Do Autoregressive Sequence Models Forecast Physical Wavefields? A Controlled Study on Synthetic Seismograms ›
Tunable responsivity and bandwidth in microwave kinetic inductance detectors via readout current nonlinearity ↓↑