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 from north-east

S Webcam

N Webcam

S Sky
Temperature
13.9 °C
Humidity
70%
Wind
1.6 km/h
Pressure
1023.8 hPa

Moon
Latest preprints on astro-ph:
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FPCA-Enhanced Simulation-Based Inference for Robust Type Ia Supernova Cosmology ›
Tails and Trails: Comets and NEOs Survive Co-addition in Rubin Early Data Preview 2 ›
A Self-Consistent Jeans Analysis of the Milky Way Rotation Curve ›
Non-linear dynamo waves in magnetized shear flows: a candidate mechanism for the solar cycle ›
Hidden in the Halo: New Diffuse Star Clusters in the M82 Starburst with JWST ›
TRICEPS. I. Tracing cold gas, dust, and stars at sub-kpc scales in massive star-forming galaxies at z = 4-5 ›
Saturation Mechanism of Cosmic Ray Streaming Instabilities with a Shell Distribution ›
Mass and spin properties of black-hole mergers reveal formation in triples ›
Selective state space model for photon energy estimation in microwave kinetic inductance detectors ›
Revealing Optically Hidden Companions to Intermediate-Mass Stripped Stars with Radial Velocities ›
Analyzing $\mu$ Parameter Range and the Duration of Reheating in the Polynomial $\alpha$-attractor Models using CMB Observations ›
Interaction of stellar dipole and disk magnetic fields in accretion-ejection systems ›
Machine Learning $\beta$-decay Half-lives and Their Application to $r$-Process Observables ›
SN Helios: A Multiply Imaged Type II Supernova Opening Time-Delay Cosmography beyond redshift of 3 ›
A tidal disruption event in a quasar at redshift 7.19 ›
Infrared Cavity Surrounding T Pyxidis: Evidence of a Nova Super-remnant? ›
Spectral and Polarization Properties of Coherent Radio Emission from Relativistic Magnetized Pair Plasma Shocks ›
Collisional excitation of E- and Z-ethanimine to model cold molecular clouds ›
The 91T/99aa-like Type Ia Supernova 2019vrq, Part II: 3D, Non-LTE, Low-Amplitude, Pulsating Delayed-Detonation Models of a Promising Standard Candle ›
FOTO: Figure-Level Semantic Search for Astronomy ›
Breaking the AGB Color Degeneracy with Variability and H$_2$O: A Consistent Picture of AGB Chemistry, Dust, and the J-Region Across Environments ›
Hot Rocks Survey VI: An anomalously hot dayside for the rocky planet GJ 357 b ›
The JWST Proto-PAH project. Computational modeling of the emission carriers ›
The JWST Proto-PAH project: Aromatic backbones with extensive aliphatic substitution account for both the aromatic and aliphatic emission ›
Evidence for the Typhon Stellar Stream as the Remnant of a Recently-disrupted Dwarf Galaxy ›
Tracing the Host-Galaxy Environments of FRBs with a New Sample of Localized Sources Detected with the DSA-110 ›
Deciphering the VHE gamma-rays spectra of Extreme High-Frequency peaked BL Lac Objects through a Photohadronic Model ›
A VLA Study of the Disturbed Massive Cluster PLCK G165.7 + 67.0 and Its Two Narrow Angle Tail Galaxies ›
A Cyanopolyyne-rich but COM-poor Massive Protostar: The First Hot Carbon Chain Chemistry Source G28.28-0.36 ›
A Comprehensive Study of the Long-Period Cataclysmic Variable V630 Cassiopeiae ›
A Sample of Long-Period Binaries with Dormant Compact-Object Candidates from LAMOST DR13 MRS and Gaia DR3 ›
Pulsed Accretion onto Eccentric Binaries in Highly Misaligned Circumbinary Disks ›
BS Cassiopeiae: A Contact Binary with Starspot-Driven Variability and Evidence for Additional Components ›
Long-term X-ray variability of the NLS1 Ark 564 ›
On the Compositions of Interstellar Objects ›
KBSS-InCLOSE II: First Detailed Insights on the Inner CGM of Low-Mass $z\sim2.3$ Galaxies ›
Near-infrared spectra of chemically peculiar stars and applications to kilonova spectra ›
Beating and coupling in pulsating stars: a unified Fourier description and observational diagnostics ›
TS23/McDonald and FIES/NOT strike again. Two new warm Jupiter systems and outer companions in a third ›
Convolutional non-parametric Gamma-Ray Signal and Background Separation ›
AKARI near-infrared spectroscopy of circumstellar hydrocarbon dust associated with young stellar objects ›
Simulating tidal disruption events in nuclear star clusters ›
Probing the cosmic web with fast radio bursts: II. Scintillation ›
The NEMESIS general YSO catalogue - I. Supervised classification with deep learning methods ›
Observational constraints on scalar-vector-tensor dark energy with phantom-divide crossing ›
JWST detection of methane emission from a young brown dwarf ›
ATLASGAL: The HCN-IR Star Formation Relation for the Milky Way ›
N-Body Dynamics as a Mechanism for Mean Motion Resonance Formation in the Post-Gas Era ›
MATISSE-py: a high-level Python interface for efficient, automated VLTI/MATISSE data reduction ›
H2 emission in the Orion Bar, NGC7023 and the Horsehead Nebula observed with the James Webb Space Telescope ›
A solution to the paradox of youth in the Galactic centre ›
SQuIGG$\vec{L}$E: Spatially resolved NIRSpec Pa$\alpha$ reveals that the most CO-luminous, $z\sim0.7$ post-starburst galaxies exhibit falling---but still active---star formation behind optically thick dust ›
SQuIGG$\vec{L}$E: Ubiquitous Cool Gas Outflows with Large Mass-Loading Factors in $z\sim0.7$ Post-starburst Galaxies ›
A statistical hardness classification of ultraluminous X-ray sources using long-term Swift/XRT monitoring ›
The Molecular Circumstellar Environments of Red Supergiants in Galactic Open Clusters ›
Kruglov-entropy cosmology from apparent-horizon thermodynamics: background dynamics and observational constraints ›
4FHL: The Fourth Catalog of Hard Fermi-LAT Sources ›
Neutron Economy and Freeze-out Dynamics in the Late-Time Cold r-Process ›
Physics-induced impact on the properties of Kepler/K2 solar analogs in the light of PLATO's requirements ›
The 91T/99aa-like Type Ia Supernova 2019vrq, Part I: Photometry, Spectroscopy, and Spectropolarimetry of a Nearly Standard Candle ›
Cosmic Heterogeneity Shapes the Evolution of Dark Energy and Time ›
A Comprehensive Study of the Magnetic White Dwarfs in DESI DR1 ›
Inclination of Miranda as a Constraint on the Tidal Dissipation of Uranus ›
A Multidimensional General-Relativistic Boltzmann Solver for Neutrino Transport: Implementation, Discretization and Optimization ›
MAGGIE: A Magnetic Gravitational Wave Induction Experiment ›
Metastable Neutron Stars as Transient-Rate Detectors of Heavy Dark Matter ›
Hybrid Partial Dressing: Correct Effective Potentials at All Temperatures ›
Tracing out massive fields in cosmology ›
Rotating Weyssenhoff fluids in linearized Einstein-Cartan theory ›
Propagation delays and regional intensity changes in lensed hotspot images ›
A Bonded-Particle Discrete-Element Model with Self-Gravity for the Collision and Reaccumulation of Rubble-Pile Asteroids: Formulation and Numerical Protocol ›
Sub-Horizon and Quasi-Static Approximations in Interacting Dark Sector Models Involving Scalar Field Dark Energy ›
Bayesian inference of non-Maxwellian distribution functions from collective Thomson scattering spectra ›
Set Transformer inference of the neutron star equation of state from stellar observations ›
Architecture Acceleration of Machine Learning Gravitational Waveform Surrogate Models ›
From Image Morphology to Multiphysics Earth Posteriors ›
Natural Saturation Of The Sterile Neutrino Dark Matter Resonant Production By a High Lepton Flavor Asymmetry In Primordial Plasma ›
Mind the second gap: The impact of gaps on noise and signal parameter inference ›
Dark Bondi Accretion Aided by Baryons and the Origin of JWST Little Red Dots ›
MEGATRON: the impact of non-equilibrium effects and local radiation fields on the circumgalactic medium at cosmic noon ›
MAGNUS I: A MUSE-DEEP Sample of Early-type Galaxies at Intermediate Redshift ›
MAGNUS II: Rotational support of massive early-type galaxies decreased over the past 7 billion years ›
VELOCE III. Reconstructing Radial Velocity Curves of Classical Cepheids ›
DESI-Like Hubble Expansion From Staged Symmetry Breaking: Constraints on Renormalizable Models ›
The Clustering of Little Red Dots from Ultra-Strongly Self-Interacting Dark Matter ›
Interpreting the diversity of afterglow emission from radio-detected tidal disruption events with instantaneous and delayed outflows ›
Partial Relief of the Hubble Tension and a Natural Self-Interacting Dark Matter Candidate From Staged Symmetry Breaking ›
Exploring Beyond {\Lambda}CDM with the Weak Lensing Power Spectrum and Bispectrum ›
Does supernova feedback regulate the star formation rate in dwarf galaxies? ›
Euclid preparation. XCV. Cosmology Likelihood for Observables in Euclid (CLOE). 2. Code implementation ›
Introducing SAGUARO -- Simulating IGM Evolution and Environments At High Resolution: Setup and First Results ›
Investigating the $H_0$ Tension and Expansion-History Mismatch with Diverse Dark Energy Parametrization Frameworks ›
TDCOSMO XXVI: Uniform lens modeling of eight doubly imaged quasars ›
Identifying the host of compact binary mergers ›
Vision-Language Model Ensembles Achieve Human-Expert Accuracy for Galaxy Merger Classification ›
Isochrones in primordial magnetic field evolution ›
SIDM and CDM interpretations of the million-solar-mass lensing perturber JVAS B1938+666-$\mathcal{V}$ ›
MOSAIC at ELT: Design and First Prototyping of Novel Robotic Optical-Relay Positioners ›
Signatures of photospheric convection throughout the solar atmosphere: the EVE Sun-as-a-star mHz continuum ›
Primordial Black Hole mass growth from neutrinos during the radiation era ›
Turbulent Transport of Galactic Magnetic Fields into Cosmic Voids: Insights from IllustrisTNG ›
Falsifiable anthropic model from the string landscape ›
Structural quasi-universality in highly magnetized differentially rotating neutron stars ›
J0011+3443: a GPS compact symmetric object, gravitational lens, or dual AGN? ›
On the formation of subdwarf B stars via engulfment of substellar companions I. Conditions for and occurrence of envelope ejection events ›
Volatile depletion in rocky planets as a chemical fingerprint of hybrid accretion ›
Early against Late: A contrast on dark energy in the light of DESI DR2 ›
A Spectral Framework for Testing the Quasi-Star Hypothesis in Little Red Dots I: Weighing LRDs by Their Super-Eddington Luminosity Ratios---No Signs of Overmassive Black Holes ›
First results on the search for the Galactic Center Excess in the sub-GeV band with the emulsion telescope in GRAINE 2023 ›
High Resolution Grid-based Simulations of the Warm-Hot Intergalactic Medium ›
Silencing the stellar glare with kernel-nulling and active phase control on photonic chips ›
Pushing high angular resolution and high contrast observations on the VLTI from Y to L band with the Asgard instrumental suite: integration status and plans ›
Formation of adducts of C$_6$H with Na$^+$, Mg$^+$ and Al$^+$ metal cations by radiative association ›
Gravitational and kinematic redshifts of black holes in nonlinear electrodynamics ›
Black hole binaries in shift-symmetric Einstein-scalar-Gauss-Bonnet gravity experience a slower merger phase ›
Addressing leakage and mode suppression in angular power spectrum estimation for gravitational-wave backgrounds using pulsar timing arrays ›
ThousandWorlds: A benchmark for climate emulation of potentially habitable exoplanets ›
Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures ›
Isochrone fitting of Galactic globular clusters - IX. Tip of the red-giant branch for 27 clusters and constraints on new particle physics ›
Promoting Green Computing in High Energy Physics and Astrophysics ›
Higgsino Dark Matter Interpretation of the LUX-ZEPLIN 248 keV Nuclear-Recoil Event ›
Sub-TeV Singlino Dark Matter in light from Sagittarius A$^\ast$ and LUX-ZEPLIN Nuclear-Recoil Event ↓↑