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

View to Mt. Babia Gora

S Webcam

N Webcam

S Sky
Temperature
-3.6 °C
Humidity
93%
Wind
0.0 km/h
Pressure
1011.7 hPa

Moon
Latest preprints on astro-ph:
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Revisiting the missing mass problem in MOND for nearby galaxy clusters ›
Exploring Cosmological Tensions with Hubble Parameter Tomography via Linear Cosmography ›
Correlation Calibration: A Hybrid Calibration Technique for Radio Interferometric Arrays ›
Consistency of standard cosmologies using Bayesian model comparison and tension quantification ›
The Host Galaxies of Active Galactic Nuclei with Direct Black Hole Mass Measurements ›
Modelling the photometric and morphological evolution of disc galaxies in the cluster environment ›
Searching for dark matter signals with high energy astrophysical neutrinos in IceCube ›
Probing habitable regions with SRG/eROSITA ›
Satellites and small bodies with ALMA: Insights into Solar System formation & evolution ›
The imprint of AGN-driven outflows on the CGM: the case of Ly{\alpha} nebulae around high-z quasars ›
Ne and Fe abundances in the ISM: Archival Study of Fe-L and Ne-K edges in Chandra and XMM-Newton ›
Dynamic Zoom Simulations of structure formation beyond standard cosmology ›
How Neutron Star Observations Point Towards Exotic Matter: Existing Explanations and a Prospective Proposal ›
On the radial velocity wave in the Galactic disk ›
Hypersoft X-ray Sources: A New Class of Luminous Cosmic Emitters ›
Compact HII Regions as Clocks of Massive-Star Formation: Evidence for Long Formation Timescales ›
Dwarf Galaxy Number Counts within 25 Mpc: Predictions from Local Group Analogues in TNG50 ›
Disk-Regulated Mass Transfer Between Rotating Non-Degenerate Stars: Insights from Be and sdOB Binaries ›
On the Difficulties with Late-Time Solutions for the Hubble Tension ›
Treecode2: The Power of Pluralism. I. Static Tests ›
Simulated LSST Observations of Real Metre-scale Impactors ›
An Archival Optical Counterpart Search for Extragalactic Fast X-Ray Transients Discovered by Einstein Probe ›
Characterization of the Polarization Beam Response of SPT-3G Using Point Sources ›
Reversal of Spin: Comet 41P/Tuttle-Giacobini-Kresak ›
Primordial Black Hole signatures from femtolensing and spectral fringe of Gamma Ray Bursts ›
Super-knee cosmic rays from interacting supernovae ›
The Massive and Distant Clusters of WISE Survey 2: Splashback Radii to z=1.65 from Galaxy Density Profiles ›
The Massive and Distant Clusters of WISE Survey 2: Detection of splashback radii in galaxy cluster total light stacks ›
ELUCID-DESI I: A Parallel MPI Implementation of the Initial Condition Solver for Large-Scale Reconstruction Simulations ›
The Walkaway Star HP Tau/G2: Evidence for a Stellar Merger ›
A Demonstration of a Neural Network as a Bridge Between Galaxy Simulations and Surveys ›
The Non-Eruptive Reconfiguration of a Quiescent Filament After a Nearby Active Region Emergence ›
Joint optical-digital design strategy for adaptive optics systems: application to wavelength selection for satellite imaging ›
AB Aur, a Rosetta stone for studies of planet formation (IV): C/O estimates from CS and SO interferometric observations ›
Universality of Primordial Anisotropies in Gravitational Wave Background ›
SF2A Environmental Transition Commission: Summary of the 2025 workshop ›
Mobile neutron monitor for latitude cosmic ray monitoring ›
Studies on the spin and magnetic inclination evolution of magnetars Swift J1834.9-0846 under wind braking ›
Rotational Behaviour of Exotic Compact Objects ›
Introducing a new generation Adaptive Optics simulation framework: from PASSATA to SPECULA ›
Galaxies caught in transition: the role of group environment in shaping the mass-size relation in the local Universe ›
The effect of JWST/NIRSpec data reduction on the retrieval of WASP-39b atmospheric properties ›
Dilution of accreted planetary matter in hot DA white dwarfs according to their mass ›
Sensipy: simulate gamma-ray observations of transient astrophysical sources ›
Heavy interstellar scattering toward the near end of the Galactic bar ›
Forecasting Supermassive Black Hole Binary Gravitational Wave Probes: Prospects for Future Pulsar Timing Array and Space-Borne Detectors ›
The X-ray properties of the most luminous quasars with strong emission-line outflows ›
Primordial Black Hole Abundance from Reionization ›
Merger Driven or Internal Evolution? A New Morphological Study of Tidal Disruption Event Host Galaxies ›
Asteroseismic ages for 17,000 stars in Kepler, K2 and TESS ›
Antenna for the detection of electromagnetic audio-band disturbances on-board LISA ›
Magnetohydrodynamic instabilities in stellar radiative regions. I. Linear study of shear-driven instabilities ›
Astrometric follow-up of near-Earth asteroid 2024 YR4 during a Torino scale level 3 alert ›
Non-spherical BUFFALOs: a weak lensing view of the Frontier Field clusters and associated systematics ›
Optical spectral characterization of OP 313. Constraining the contribution of thermal and non-thermal optical emission ›
Towards a Fully Automated Pipeline for Short-Term Forecasting of In Situ Coronal Mass Ejection Magnetic Field Structure ›
Mapping plasma properties of Cassiopeia A with XRISM/Resolve: a Bayesian analysis via UltraSPEX ›
Spectral Appearance of Self-gravitating AGN Disks Powered by Stellar Objects: Universal Effective Temperature in the Optical Continuum and Application to Little Red Dots ›
Dark Matter Heating of Compact Stars Beyond Capture: A Relativistic Framework for Energy Deposition by Particle Beams ›
Scalar Tsunamis from Black Hole Formation ›
Chiral phase transition with primordial black holes: Distinct phase structure and catalysis ›
Gravastar on the brane with a timelike extra dimension ›
Bayesian Constraints on the Neutron Star Equation of State with a Smooth Hadron-Quark Crossover ›
Spin Light of neutrino in polarized matter ›
Accelerating TTL noise post-processing via combined coefficients and alternative TDI configuration ›
Real time, cross platform visualizations with zero dependencies for the N-body package REBOUND ›
Many-body effects on dense matter with hyperons at finite temperature ›
Parametric-Resonance Production of QCD Axions ›
Gravitational Raman Scattering: a Systematic Toolkit for Tidal Effects in General Relativity ›
The density-bounded twilight of starbursts in the early Universe ›
Investigating cosmic strings using large-volume hydrodynamical simulations in the context of JWST's massive UV-bright galaxies ›
Investigating the role of nuclear parameters in Neutron Star oscillations: a model comparison ›
The THESAN-ZOOM project: Burst, quench, repeat -- unveiling the evolution of high-redshift galaxies along the star-forming main sequence ›
The THESAN-ZOOM project: central starbursts and inside-out quenching govern galaxy sizes in the early Universe ›
The Shape of FIREbox Galaxies and a Potential Tension with Low-mass Disks ›
ECHO21: a tool for modelling global 21-cm signal from dark ages to reionization ›
Galaxy-scale lens search in the PEARLS NEP TDF and CEERS JWST fields ›
Overmassive black holes in the early Universe can be explained by gas-rich, dark matter-dominated galaxies ›
Tracing Missing Baryons in the Cosmic Filaments with tSZ and CMB-Lensing Stacking ›
The THESAN-ZOOM project: Mystery N/O more -- uncovering the origin of peculiar chemical abundances and a not-so-fundamental metallicity relation at $3 ›
From Redshift to Real Space: Combining Linear Theory With Neural Networks ›
The spin-orbit alignment hypothesis in millisecond pulsars ›
Resolving the Planck-DESI tension by non-minimally coupled quintessence ›
CLASH-VLT: The variance in the velocity anisotropy profiles of galaxy clusters ›
The New Status Qvo? SN 2021qvo is Another 2003fg-like Type Ia Supernova with a Rising Light-Curve Bump ›
Can an Anti-de Sitter Vacuum in the Dark Energy Sector Explain JWST High-Redshift Galaxy and Reionization Observations? ›
Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future ›
The Simons Observatory: Characterization of the 220/280 GHz TES Detector Modules ›
An Explicit M1 Radiation-hydrodynamics Scheme for Three-dimensional Protostellar Evolution ›
Revisiting electron-capture decay for Galactic cosmic-ray data ›
Probing AGN-ISM Feedback through Extended X-ray Emission in ESO 137-G034 ›
A Light-Cone Approach to Higher-Order Cosmological Observables ›
VENUS: A Strongly Lensed Clumpy Galaxy at $z\sim11-12$ behind the Galaxy Cluster MACS J0257.1-2325 ›
Stellar streams around dwarf galaxies in the Local Universe ›
Magnetic Field Amplification and Particle Acceleration in Weakly Magnetized Trans-relativistic Electron-ion Shocks ›
ALMAGAL VI. The spatial distribution of dense cores during the evolution of cluster-forming massive clump ›
Transformation of orientation and rotation angles of synchronous satellites: Application to the Galilean moons ›
The Birth of Be Star Disks II. A High-Resolution Spectroscopic Campaign and TESS Observations of an Outburst of the Classical Be star {\lambda} Pavonis ›
Ultimate large-$Rm$ regime of the solar dynamo ›
The WINTER Observatory: A One-Degree InGaAs Survey Camera to study the Transient Infrared Sky ›
Quantifying sunspot group nesting with density-based unsupervised clustering ›
Lyman Continuum escaping from in-situ formed stars in a tidal bridge at z = 3 ›
A comprehensive study of the relations between the properties of planetary systems and the chemical compositions of their host stars ›
Perihelion Asymmetry in the Water Production Rate of the Interstellar Object 3I/ATLAS ›
A dynamical systems approach to studying the equivalence principle in dilaton gravity ›
A quiescent galaxy in a gas-rich cosmic web node at z~3 ›
Investigating the origin of radio emission in candidate super-Eddington accreting black holes ›
Connecting the Dots: UV-Bright Companions of Little Red Dots as Lyman-Werner Sources Enabling Direct Collapse Black Hole Formation ›
Broadband infrared spectroscopy of methanol isotopologues in pure, H2O-rich, and CO-rich ice analogues ›
Clustering of z~6.6 Quasars and [O III] Emitters Constrains Host Halo Masses and Duty Cycles in 25 ASPIRE Fields ›
Sulfur Enrichment in Close-in Exoplanet Atmospheres Induced by Pebble Drift across the Salt Line ›
The Double-Burst Nature and Early Afterglow Evolution of Long GRB 110801A ›
Fundamental oscillations as a tool to distinguish boson stars from neutron stars and black holes ›
Probing Boson Clouds with Supermassive Black Hole Binaries ›
Reheating after the Supercooled Phase Transitions with Radiative Symmetry Breaking ›
Time-Frequency Analysis of Non-Uniformly Sampled Signals via Sample Density Adaptation ›
Metastable Strings and Gravitational Waves in One-Scale Models ›
$Q$-balls, neural networks and galaxy rotation curves ›
Numerical tiling-based simulations of decoherence in multifield models of inflation ›
Strong lensing cosmography using binary-black-hole mergers: Prospects for the near future ›
New Multi-messenger Probe of Dark Matter-Nucleon Interactions from Ultra-high Energy Cosmic Ray Acceleration ›
Exact black holes and black branes with bumpy horizons supported by superfluid pions ›
On the stability of viscous Riemann ellipsoids ↓↑