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

Telescope

Cloud

Rainfall

S Sky
Temperature
-4.5 °C
Humidity
93%
Wind
0.0 km/h
Pressure
1010.4 hPa

Moon
Latest preprints on astro-ph:
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Foiling Black Hole Foils: Revealing Horizon Alternatives with Baryonic Atmospheres ›
Supermassive black holes swallow stellar objects at high rates: from Little Red Dots to Black Hole Stars ›
A targeted machine learning approach for detecting diffuse radio emission with Astronomaly: Protege ›
What does it mean to take the mean? The effect of the averaging scale on the characterization of interstellar turbulence ›
CLASH-VLT velocity anisotropy profiles in a stack of massive galaxy clusters ›
Little Red Dots as Globular Clusters in Formation ›
Exploring the Near Galactic Centre: A Comprehensive Study of Bulge OCs HSC 25, HSC 37, HSC 2878 Utilising Gaia DR3 Data ›
Implications of the nanoHertz Gravitational-Wave Background for Galactic Feedback and Massive Black Hole Growth ›
The large cores of dark matter and globular clusters in AS1063. Possible evidence of self-interacting dark matter. Or not ›
The LOFAR Two-metre Sky Survey: VII. Third Data Release ›
MadEvolve: Evolutionary Optimization of Cosmological Algorithms with Large Language Models ›
Gas Accretion versus BH Merger driven Growth Modes of Supermassive Black Holes and Implications for the Little Red Dots ›
Is the overconcentration of pristine populations in Galactic globular clusters real? An N-body approach to the problem ›
Stellar microlensing as a probe of Primordial Black Holes: status and prospects ›
Early Results from the Coma Legacy IFU Survey (CLIFS): Ram Pressure Induced Shocks and Ionization in Jellyfish Tails ›
Planet-Disk Interactions and the Convective Overstability. I. Low Mass Planets ›
Multiwavelength Campaign Observations of a Young Solar-type Star, EK Draconis. III. Comparison between Starspot Mapping, Zeeman Doppler Imaging, and Multiwavelength Variability ›
CHARA Array Delay Lines: Upgrades, Performance and Future Directions ›
Molecular diagnostics for the mid-infrared emission of planet-forming disks. Carbon and oxygen elemental abundances ›
Diffusive Instabilities in Dusty Disks: Linear Growth and Nonlinear Breakdown ›
Direct contact binary planetesimal formation from gravitational collapse ›
The Carousel Lens II: Cosmological Constraints with GIGA-Lens ›
Evolution of Low-Mass Population III Stars: Convection, Mass Loss, Nucleosynthesis, and Neutrinos ›
Three Saturn-mass Microlensing Planets Identified through Signals from Peripheral-caustic Perturbations ›
Effects of Symmetron on growth and RSD multipoles ›
Graph--Based Event Fingerprints for Classifying Geomagnetic Storm--Driven Forbush Decreases ›
First Detection of the Baryon Acoustic Oscillation (BAO) Feature in the 3-Point Correlation Function of DESI DR1 Luminous Red Galaxies ›
Investigating Ionospheric TEC Variations in Solar and Geomagnetic Influences Across Solar Activity Phases ›
Cosmic Ray Spectra and Metal Budget Regulated by the Galactic Wind ›
Reinterpreting the sunward electron deficit: Implications for solar wind acceleration and core population formation ›
The Enigmatic Type Icn Supernova 2024abvb Located ~22 kpc from Its Host Galaxy ›
Propagation Characteristics of the April 21, 2023 CME ›
A XRISM View of the Iron Line Complex in NGC 1068: Rethinking the Prototypical Compton-Thick AGN ›
PDRs4All XXI. JWST-NIRCam Photometric properties of protoplanetary disks in the Orion Nebula Cluster ›
SPT-CL J0417-4748: A Deep Chandra Study of a Relaxed Galaxy Cluster Without Central Star Formation ›
Numerical analysis of Lyapunov Times for Trans-Neptunian Objects and Main-Belt Asteroids: stability, accuracy, and methodological comparisons ›
High significance detection at 4.8 GHz of the radio halo in the Coma galaxy cluster with the Sardinia Radio Telescope ›
Localized $^{18}$O production in white dwarf mergers ›
Accretion Disk Magnetic Braking ›
Deepest ever photographed Geminid with small but not negligible terminal mass ›
A fast radio burst cyclone in technicolour: evidence of plasma lensing ›
The Astronomical Telescope of the University of Stuttgart (ATUS): Development, Optimization, and Lessons Learned ›
Euclid preparation. Impact of galaxy intrinsic alignment modelling choices on Euclid 3x2pt cosmology ›
Benchmarking Photolysis Rates with Socrates (24.11): Species for Earth and Exoplanets ›
Resolving the Multiple Component Outflows in PG 1211+143: II. The Soft X-ray View of the Ultra Fast Outflow ›
The role of radiative torques in the molecular cloud core L43 ›
New self-consistent theoretical descriptions for mass-loss rates of O-type stars ›
Searching for White Dwarf Candidates Formed Through Binary evolution in Star Clusters ›
GOTO identification and broadband modelling of the counterpart to the SVOM GRB 250818B ›
Chiral gravitational waves from multi-phase magnetogenesis ›
Meteor statistics I: The distribution of instrumental magnitudes ›
HOLISMOKES XX. Lens models of binary lens galaxies with five images of Supernova Winny ›
Two warm sub-Saturn mass planets identified from the TESS Full Frame Images ›
Interpreting the HI 21-cm cosmology maps through Largest Cluster Statistics III: Impact of the lightcone effect ›
Investigating Nonlinear Quenching Effects on Polar Field Buildup in the Sun Using Physics-Informed Neural Networks ›
Updated Constraints on Infrared Cutoff Models and Implications for Large-Scale CMB Anomalies ›
Orbital Motions of Binaries in Orion South ›
How Bursty is Star Formation at z>5? ›
Particle-in-Cell Methods for Simulations of Sheared, Expanding, or Escaping Astrophysical Plasma ›
New formula for Asymptotic behavior of the Synchrotron function ›
Statistics of Daily Modulation in Dark Matter Direct Detection Experiments ›
Solving BDNK diffusion using physics-informed neural networks ›
Rotating Black Holes with Primary Scalar Hair: Shadow Signatures in Beyond Horndeski Gravity ›
Prediction of Major Solar Flares Using Interpretable Class-dependent Reward Framework with Active Region Magnetograms and Domain Knowledge ›
Gravitational Waves from Primordial Black Holes formed by Null Energy Condition Violation during Inflation ›
Characterization of an MPPC-Based Scintillator Telescope and Measurement of Cosmic Muon Angular Distribution ›
Comet-type periodic motions and their out-of-plane bifurcations in the Earth-Moon CR3BP: a computational symplectic analysis ›
Prompt And Delayed Radio Bangs At Kilohertz By SN 1987A: A Test For Graviton-Photon Conversion ›
Precessing Gamma Jets in extended and evaporating galactic halo as a source of GRB ›
Inverse Compton Scattering onto BBR in High Energy Physics and Gamma (MeV-Tev) Astrophysics ›
The role of \nu_{\tau} ultrahigh energy astrophysics in Km^3 detectors ›
Adiabatic or Non-Adiabatic? Unraveling the Nature of Initial Conditions in the Cosmological Gravitational Wave Background ›
Dark Energy Survey: Galaxy Sample for the Baryonic Acoustic Oscillation Measurement from the Final Dataset ›
AbacusPNG: A modest set of simulations of local-type primordial non-Gaussianity in the DESI era ›
Novel Physics of Escaping Secondary Atmospheres May Shape the Cosmic Shoreline ›
The Effect of Foreground Galaxies on the Estimation of the Hubble Constant from Type Ia Supernovae ›
X-ray emission in IllustrisTNG circum-cluster environments. II -- Possible origins of the soft X-ray excess emission ›
Inflationary Fossils Beyond Perturbation Theory ›
Can GW231123 have a stellar origin? ›
Sound-Horizon-Agnostic Inference of the Hubble Constant and Neutrino Mass from BAO, CMB Lensing, and Galaxy Weak Lensing and Clustering ›
A novel algorithm for GPU-accelerated particle-mesh interactions implemented in the QUOKKA code ›
The warm outer layer of a Little Red Dot as the source of [Fe II] and collisional Balmer lines with scattering wings ›
Millimeter-Wavelength Lens-Absorber-Coupled Ti/Al Kinetic Inductance Detectors ›
StarEmbed: Benchmarking Time Series Foundation Models on Astronomical Observations of Variable Stars ›
An Explicit M1 Radiation-hydrodynamics Scheme for 3D Protostellar Evolution ›
Radiation-dominated polar emitting region of an accreting X-ray pulsar -- I. Polarization- and spectrum-dependent structure, and the emergent continuum ›
Dark Energy Survey Year 3 results: Simulation-based $w$CDM inference from weak lensing and galaxy clustering maps with deep learning: Analysis design ›
Data-driven Radiative Magnetohydrodynamics Simulations with the MURaM Code: the Emergence of Active Region 11158 and the X2.2 Flare ›
Dust destruction by the supernova remnant forward shock in a turbulent interstellar medium ›
JOYS: JWST MIRI/MRS spectra of the inner 500 au region of the L1527 IRS bipolar outflow ›
A Universal CMB $B$-Mode Spectrum from Early Causal Tensor Sources ›
JWST imaging of the Pleiades: anisotropy of turbulence in the cold neutral medium ›
Exploring Cosmological Tensions with Hubble Parameter Tomography via Linear Cosmography ›
TIC-65910228 b / NGTS-38 b, a 180 day transiting warm super-Jupiter ›
The James Webb Space Telescope Absolute Flux Calibration. V. Near-Infrared Camera Wide Field Slitless Spectroscopy ›
Production of Jets before Neutron Star Mergers ›
Hipparcos period-luminosity relations for Miras and semiregular variables ›
Relativistic magnetohydrodynamics in the early Universe ›
Cosmic Axions Revealed via Amplified Modulation of Ellipticity of Laser (CARAMEL) ›
High-Precision Measurement of D($\gamma$, $n$)$p$ Photodisintegration Reaction and Implications for Big-Bang Nucleosynthesis ›
Shadow of rotating black holes with consistent thermodynamics ›
Photon Accelerator in Magnetized Electron-Ion Plasma ›
Post-Newtonian Dynamics of Radiating Charges: Canonical Formulation and Binary Inspiral Laws ›
Dark Matter Heating of Compact Stars Beyond Capture: A Relativistic Framework for Energy Deposition by Particle Beams ›
Some phenomenological aspects of a quantum-corrected Reissner-Nordstr\"{o}m black hole: quasi-periodic oscillations, scalar perturbations and thermal fluctuations ↓↑