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
13.3 °C
Humidity
80%
Wind
8.0 km/h
Pressure
1004.8 hPa

Moon
Latest preprints on astro-ph:
›
Extreme Stellar Death and Galaxy Feedback at z = 2: A Rest-frame Ultraviolet Characterization of the Strongly Lensed Superluminous Supernova 2025wny ›
KDG 162: A Nearby Isolated Star-forming Dwarf Galaxy ›
Modeling the nanohertz gravitational wave background with the t-process: Improved frequentist analysis of gravitational-wave power ›
Full-Shape Analysis of the Redshift-Space Galaxy Trispectrum in the EFTofLSS ›
Debye cooling of ultramassive white dwarfs ›
A Newly Identified Transient Ultraluminous X-ray Source in M31 ›
The BUFFALO Survey : The Subhalo Mass Function for Abell 2744 with Strong+Weak Gravitational Lensing ›
PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-Domain Field V: Unraveling X-ray Spectral Variability ›
Searching for hot water world candidates with CHEOPS: II. A low-density super-Earth orbiting the K dwarf TOI-2211 ›
Re-calibrated analytic stellar evolution formulae for the main sequence: Extension to massive stars and variations in $[\alpha/\mathrm{Fe}]$ ›
Early onset of the hot circumgalactic medium around Milky Way galaxies ›
Predictions for Short Gamma-Ray Burst Detections by COSI ›
Measuring the Clustering of tSZ-Selected Galaxy Clusters with SPT-3G ›
Turbulent viscosity in line-driven stellar winds ›
Can LISA See Inside the Little Red Dots? ›
CHemical Evolution in MassIve star-forming COres (CHEMICO). II. Molecular ions, electron fraction, and cosmic-ray ionisation rate ›
A method for multimodal analysis of TAIGA experiment data using essential features ›
Euclid Quick Data Release (Q1). Exploring the complexity of quenching processes across time, environment, and mass through recently quenched galaxies ›
(Monty Python and the) HoliGRALE: A Hybrid GRALE Lens Inversion Methodology Diagnostically Evaluated with Synthetic and Real Data ›
Assessment of sky brightness in central Portugal: the Dark Sky destination "Aldeias do Xisto" case study ›
Polarimetric Behaviour of (3200) Phaethon: New Observations with Implications for Surface Heterogeneity ›
Detection of escaping magnesium in the upper atmosphere of WASP-76b ›
The Impact of Galaxy Catalogue Completeness with GLADE+ on Dark Siren Cosmology: A Line-of-Sight Prior Analysis of GWTC-3 Events ›
Effects of Magnetic Fields on Solar Inertial Modes in Global Nonlinear Simulations ›
Constrained Diffusion for Data-Scarce Orbital Monte Carlo in Constellation Tasking ›
Scalar Perturbations and Induced Gravitational Waves from First-Order Phase Transitions in Lattice Simulations ›
The Fast Transient Foreground Fog of LSST ›
The Prompt Emission of Gamma-Ray Bursts from Population III Stars ›
Polarised X-ray emission from the accreting millisecond pulsar SAX J1808.4-3658 during an X-ray outburst and a type-I X-ray burst ›
Axion effects on hybrid stars: earlier hadron-quark phase transition and larger quark-matter cores ›
Complex Organic Molecules in Protostars with ALMA Spectral Surveys (COMPASS) V. Tracing cavity walls and shocked knots with nonthermally desorbed CH$_3$OH in BHR71-IRS1 ›
ASTRAL: A Framework for Optimal Placement and Emulation of Stellar Evolution Models ›
Light curve spectral energy distribution fitting of 13 carbon-rich Mira variables stars in the Small Magellanic Cloud ›
Evidence for a Similar Physical Origin Between Prompt Emission and X-Ray Flares of Gamma-Ray Bursts ›
$r$-Process as Production of Lanthanides from Compact Object Mergers ›
SAGE26 Paper I: Modelling the baryon cycle from cosmic dawn to the present day ›
A comparison between particle and fluid approaches for streaming instability in global patch simulations ›
Remnant-wide mapping of heterogeneous presupernova burning histories in the O-rich ejecta of Cassiopeia A ›
LazyTB: Extended LTB-solutions with Multiple Interacting Fluids ›
Registering Gaia positions on VLBI images: constraining opacity-driven core shift in B 1038+528 / B 1038+529 ›
A Novel Approach to Identify Unseen Companions: An In-Depth study of GDR3 220_28 ›
Gamma-rays from black hole coronae: disentangling the leptonic and hadronic contributions ›
A Deep Learning Approach to Improving the Arrival-Direction Accuracy of Gamma-Ray Air-Shower Measurements with the Tibet-III Air-Shower Array ›
Cosmic Birefringence from Large Lepton Asymmetry ›
Star Formation in the Low Surface Brightness Galaxies: a Comparison with the Outer Regions of Normal Galaxies ›
Dynamical pairing in gravitational wave populations ›
A Jupiter-like radio aurora in the L3.5 dwarf LSPM J0036+1821 ›
A faint dust ring beyond the compact disk of Sz 76 ›
The existence of null points of flow and magnetic fields as prerequisites for the presence of astropauses and their co-location ›
The GAPS Programme at TNG. LXXX. Characterisation of the 400 Myr old multi-planet system K2-233 ›
Astrometric planet search around southern ultracool dwarfs: V. Discovery of the exoplanet candidate PALTA-1 b ›
On the origin of the short-period Blue Straggler Stars in Collinder 261: a binary evolution approach ›
Composition $g$-modes and $f$-modes of neutron stars with gravitationally coupled dark matter: degeneracy with the symmetry energy ›
Wave-Growth-Limited Particle Confinement in a Near-Parallel Interplanetary Shock Observed by Parker Solar Probe ›
Quasi-periodic eruption spectral-timing: EMRIs crossing warped accretion disks ›
MUSE-ALMA Haloes XIV: The ALMA Large Programme Data Release ›
MUSE-ALMA Haloes XV: Cold molecular, ionised, and stellar kinematics of HI-rich galaxies at z $\sim$ 0.5 ›
MUSE-ALMA Haloes XVI: a census of the condensed baryons in z~0.5 HI absorption-selected galaxies ›
A Recurrent Infrared Modulation in the Warm Post-impact Debris Disk NGC 2547 ID8 ›
Effective Neutrino Mass and Apparent Phantom Crossing ›
Angular Baryon Acoustic Oscillations with DESI DR1 ›
IMFIT-MW: Multiwavelength photometric decomposition with IMFIT ›
A Gravitationally Lensed Low-Luminosity AGN From The Cosmic Noon ›
A relativistic inflow candidate in a quasar at cosmic noon ›
Two Low-Mass-Ratio Microlensing Planets from High-Magnification Events: KMT-2021-BLG-0247 and MOA-2023-BLG-169 ›
ROSE (Red-giant Oscillations Spectra Estimator): A Modular Machine-Learning Framework for Automated Asteroseismic Characterisation. I. $\nu_{\max}$ and $\Delta\nu$ from TESS ›
Changing-look Active Galactic Nuclei from the Dark Energy Spectroscopic Instrument. VII. Testing Disk-Corona Diagnostics with eROSITA ›
Photometric and Spectroscopic Study of Young Stellar Objects in IC 1848E Region ›
A Decade-Scale Ionization Echo of Black-Hole Accretion in Galactic Nuclei ›
Deep Learning for Cherenkov Astronomy: Performance of GammaLearn on LST-1 ›
The NANOGrav 15 yr Dataset: Modified Functional Forms for Profile-Evolution Time Delays in Pulsar Timing Models ›
BOLT: Imaging Lightning and Terrestrial Gamma-ray Flashes at the Pierre Auger Observatory ›
Widespread steep X-ray spectra of luminous $z\simeq5.85-7.5$ quasars and their implications for future X-ray surveys ›
Constraints on Primordial Oscillatory Features from the Power Spectrum and Bispectrum of Redshift-Space Galaxy Clustering in DESI DR1 ›
Phase transitions, shadows, and microstructure of Reissner-Nordstr\"om-Anti-de-Sitter black holes from a geometrothermodynamic perspective ›
A Common $\sim$55 GeV Inelastic Dark Matter Origin of the LZ, Fermi-LAT, and AMS-02 Excesses and Paleo-Detector Prospects ›
An early $Z'$ dominance: dark matter, gravitational waves & collider probes ›
Convergence of Roberts flow dynamos in Eulerian and Lagrangian codes ›
Toward a complete understanding of the properties of GW190521 ›
Anisotropic Fluid Model for Massive Boson Stars: Spherically Symmetric Configurations ›
The contribution of Soviet scientists to the emergence of high-energy neutrino astrophysics: from the Cherenkov effect to underwater and in-ice telescopes ›
Phenomenology of axion-meson mixing and scattering processes ›
Analytic parity-violating greybody factors of a dynamical Chern-Simons black hole ›
Water-rich sub-Neptunes and rocky super Earths around different Stars: Radii shaped by Volatile Partitioning, Formation, and Evolution ›
Solar Vortices as Conduits for Magnetoacoustic Waves: Multi-Layer Coupling and Their Role in Atmospheric Heating ›
A Unified Charge-Dependent Modulation Model for AMS-02 Proton and Antiproton Fluxes during Solar Minimum ›
Detecting the neutrino mass via the cross-correlation between matter tracers and the ISWRS effect? ›
Revisiting Ca II Activity Indices in FGK Stars: Systematic Biases in Infrared Triplet Measurements ›
Multi-wavelength study of EP250416a / GRB 250416C: An Optically Dark Long GRB with a Late Jet Break ›
Cosmic gas accretion from filaments onto galaxy clusters using the IllustrisTNG simulation ›
Coverage is not enough: Frequentist tests of simulation-based inference for primordial non-Gaussianity ›
Gravitational wave emission from nonspherical collapse in an early matter-dominated era using N-body simulations ›
Continuous mass ablation of planets engulfed in stellar envelopes ›
Transitions in the Mass-ratio and Spin Properties of Binary Black Holes in GWTC-5 ›
Fermi-eROSITA cross-correlations suggest annihilation lines of $\sim70$ GeV WIMPs ›
A Covariance-Aware Framework for Spatially Resolved Exoplanet Biosignature Inference with the Solar Gravitational Lens ›
Investigating the star formation histories of galaxies from Cosmic Dawn to the Epoch of Reionization with the Santa Cruz SAM ›
Contribution of White Dwarf Formation Kicks to the Free-Floating Planet Population ›
Cold Stream Penetration of Virial Shocks: Fragmentation, Coagulation, and Disruption in the Hot Circumgalactic Medium ›
Very Large Telescope observations of interstellar comet 3I/ATLAS III: High-resolution monitoring of CN and forbidden oxygen emission across the perihelion passage with ESPRESSO ›
On the Separation Between the Brightest Cluster Galaxy and the Intracluster Light ›
Comparing the Near-infrared Spectral Energy Distributions from Different Stellar Population Synthesis Models with SPHEREx Observations ›
Shock breakout from mildly relativistic ejecta in a dense wind: the case of EP260321a/SN 2026gzf ›
Growth, geometry, and early-universe split of the matter density parameter $\Omega_{\rm m}$ ›
Eclipses by Artificial Satellites to Measure the Angular Sizes of Stars ›
Reconstructing orbits of galaxies in extreme regions (roger v2.0): an extension to intermediate mass systems ›
Tidal disruption of stellar binaries as a pathway to exotic transients ›
Scatter, bias, and chaos of satellite orbits in triaxial dark matter haloes ›
POSEIDON III: The Aligned Orbit of the Hot Neptune Around the Hot Star WASP-195 ›
An Updated Model for Epsilon Eridani b and Prospects for Imaging with the Roman Coronagraph ›
ALMA Chemical Evolution (ACE) survey: The gas fundamental metallicity relation at cosmic noon ›
JWST Observations of Starbursts: The motion of dust - PAH kinematics of M82 and NGC 253 with JWST/MIRI spectroscopy ›
Unravelling the Nature of AT 2025abao: From Precursor to Final Fate ›
BRAHMa: Bar Recognition And Hatching using Machine learning -- a framework for oriented bounding box detection of galactic bars ›
Exploring Leptogenesis, WIMP Dark Matter, and Gravitational Waves in an extended Scalar Framework ›
Looking for non-gaussianity in Pulsar Timing Arrays through the four point correlator ›
Gauge Theoretic Signal Processing I: The Commutative Formalism for Single-Detector Adaptive Whitening ›
Cosmological perturbations of TDiff fields ›
The decay rate of metastable cosmic strings beyond the thin-string approximation ›
A simple solution to the monopole problem: SU(5) GUT with symmetry breaking into special subgroup ›
Massive scalar fields in eccentric regime: Detectability and constraints from LISA observations of extreme mass-ratio inspirals ›
Quark and hybrid stars with renormalization group improvement of NNLO perturbative QCD ↓↑