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

Cloud

Rainfall

S Sky
Temperature
9.8 °C
Humidity
94%
Wind
0.0 km/h
Pressure
1021.2 hPa

Moon
Latest preprints on astro-ph:
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The Role of the Core in Setting Massive Neutron-Star Radii ›
A Framework for Evaluating Forward Contamination Risk for Bio-ISRU Microorganisms ›
Continuous Learning of Gravity Field Irregularities Around Small Bodies via Neural Hamiltonian ODEs ›
An unresolved extreme warm infrared excess toward a nearby low-mass star ›
Impact of galaxy intrinsic alignments on non-Gaussian weak lensing statistics for modified gravity ›
Clustering-based halo mass assignment for high-redshift galaxies: method, validation, and application to JWST ›
Constraining dark matter using 20-year INTEGRAL/IBIS observations I: Primordial black holes ›
Little Red Dots are Direct-Collapse Black Hole-Forming Galaxies ›
Reconsidering the role of bright and dark gravitational-wave standard sirens for cosmology ›
Time-Integrated Searches for Sub-TeV Neutrino Sources with IceCube-DeepCore ›
Resolved SED Modeling with JWST and ALMA: The Role of Stellar Mass Surface Density in Regulating Star Formation in Cosmic Noon Galaxies ›
Galaxies in the first two billion years: Earlier formation and quenching with surface-density modulated star formation and feedback ›
BAQARO: Tracing Stochastic Black Hole Growth Histories and Quasar Lightcurves in a Cosmological Context ›
Unified modelling of broad and narrow optical-UV emission lines from massive black holes: interpreting high-redshift JWST observations ›
The Role of Big Bang Nucleosynthesis in Joint Cosmological Analyses ›
Long-term X-ray spectral analysis of Cygnus X-1 using AstroSat ›
Which Type Ia supernova observables best indicate the ages of their progenitor stars? ›
Probing Lorentz Invariance Violation in Cosmogenic Neutrino Propagation with KM3-230213A ›
A Proliferated Space Architecture for Time-Domain Astrophysics ›
Probabilistic characterization of blending with LSST and application to cluster lensing cosmology ›
Hidden structures in the UHE sky: unveiling potential sources via spectral signatures ›
NOEMA probes the [CII] and dust content in a 2175{\AA} UV Bump Galaxy at $z=7.1$ ›
Plasma Heating and Energization in Hot-Onset Flare Precursor Events ›
Steepening Optical Slopes in Exoplanet Transmission Spectra with Charged Hazes ›
OSIRIS-REx Returned a Pristine Sample of Asteroid Bennu: Takeaways from the Mission's Contamination Control and Knowledge Program ›
Electromagnetic Probes of the Supernova Engine ›
Mapping the Quasar Main Sequence in the UV range: A Connection with the UV Fe III Emission ›
Stellar bar occurrence in TNG50 and TNG100: disentangling environmental effects and assembly history at z = 0 ›
High water D/H ratio of the interstellar object 3I/ATLAS is consistent with a low-metallicity origin ›
A Localized Current-Sheet Magnetic-Diffusion and Heating Prescription for Ideal-GRMHD Simulations of M87*-like Accretion Flows ›
Evolution of first-interaction second-harmonic anisotropy in cosmic-ray air showers ›
A systematic study of the long-term mid-infrared color variations of Seyfert 1 galaxies ›
KMT-2026-BLG-0083L: A Two-Jovian-Planet System Orbiting an M Dwarf Discovered by Microlensing ›
Superoutbursts and Superhumps of Cataclysmic Variables observed with TESS ›
The constrainability of galaxy positions in the $M_*$ -- SFR plane from SED fitting ›
Magnetic Fields and Asymmetric Accretion in the Class 0 Protostellar System L1527 IRS ›
Terminal instability of the Solar System triggered by stochastic solar mass loss ›
Spin-polarization of the neutron ocean in magnetar crusts ›
E-INSPIRE - II. Finding relics from wide-sky multi-band surveys: A proof-of-concept machine learning regression algorithm ›
Optical Follow-Up of Two Spider Pulsar Candidates: An Irradiated Redback and a Possible Double Giant Impostor ›
Heavy Seed Black Hole Growth in Metal-Enriched Halos through Disk-Induced Stellar Disruptions: A Semi-Analytical Modelling ›
Large-Scale Latitude-time Relationships Between the Green-Line Corona and Sunspot Activity During Solar Cycles 18-24 ›
Plasmoid-Trapped Condensation Associated with a Transient Thermal-Instability-Like Process in Chromospheric Magnetic Reconnection ›
Identification of Cosmic Chronometers in the GAMA Survey ›
Limits on a Host Star around a Saturn-mass Free-floating Planet Candidate KMT-2024-BLG-0792/OGLE-2024-BLG-0516 ›
Probing Inflationary Origins of Primordial Black Holes with LIGO--Virgo--KAGRA O1--O4a data ›
The influence of free-free absorption on the radio spectrum of Particle-Accelerating Colliding-Wind Binaries ›
The Infrared Glow of Galactic Outskirts: A New Window with NASIM ›
XMST: An Extended Minimum Spanning Tree Framework with Objective Fracture-Scale Selection ›
Late-Time Evolution of the Massive Stellar Merger M101 OT2015-1 ›
Magnetized interstellar molecular clouds - III. Filament Collisions and Core Formation: Insights into Substructures and Evolution ›
An efficient approach to resistive GRMHD simulations of binary neutron star mergers ›
High-redshift supermassive black hole population from core-collapse in self-interacting dark matter halos ›
The atomic C/O ratio of KELT-9b ›
Spectro-polarimetry of HAbitable Planet Earth (SHAPE) on Chandrayaan-3: Instrument characteristics, calibration and onboard performance ›
The Nature of Small-Scale Perturbation Modes in a Nonstationary Self-Gravitating Disk ›
JWST/MIRI Imaging Search for Kinematically Detected Protoplanetary Candidates ›
Big Bang For Your Helium Buck ›
Implications of the LISA stochastic signal from eccentric stellar mass black hole binaries in vacuum ›
Constraining Ultralight Scalars with Black Hole Binary Mergers in Galactic Nuclei ›
Accretion onto a moving black hole for stiff equations of state ›
Path-Degenerate Quantum Interferometry for Decoherence Mitigation in Gravitational-Wave Detectors ›
A semicoherent resampling method for long-transient gravitational wave searches with applications to subsolar-mass primordial black-hole binaries ›
Experimental Ni II Oscillator Strengths for Transitions from $3d^84d$ to $3d^84p$ Levels Measured Using High-resolution Fourier Transform Spectroscopy ›
Intrinsic pressure anisotropy in spherical Proca stars ›
Constraints on Galactic Dark Photons from a DALI Prototype ›
The DALI Haloscope: A Magnetized Phased Array Coupled to a Semi-Open Fabry--P\'erot Resonator ›
The Wavelet Detection Filter: a real time unmodeled pipeline for gravitational wave transients, ranking coincidences with a graph neural network ›
Reconstructing the Dark Matter Equation of State with Compact Object Inspirals ›
\texttt{cWB-space}: A time-frequency transient-search pipeline for LISA ›
Probing Two-dimensional Asymmetries of an Exoplanet Atmosphere from Chromatic Transit Variation ›
Renormalization group corrections to $\Lambda$CDM model and observational consequences for $H_0$ tension ›
The Power of DESI for Photometric Redshift Calibration: A Case Study with KiDS-1000 ›
Hedorah, the first yellow supergiant Kaiju star candidate at $z=3.7$ revealed by JWST behind AS1063 ›
Gas distributions inside and around haloes in the alternative dark matter simulations AIDA-TNG ›
ABCMB: A Python+JAX Package for the Cosmic Microwave Background Power Spectrum ›
A Wide and Deep Exploration of Radio-detected Active Galactic Nuclei with Subaru HSC (WERGS). XIII. High-z Radio Quasar Selection from HSC--VLASS over $\sim1200$ deg$^2$ ›
The Heavy Tailed Non-Gaussianity of the Supermassive Black Hole Gravitational Wave Background ›
Induced Scattering of Strong Waves in Pair Plasmas ›
Hessian-based photometric substructure as an evolutionary tracer of OB cluster candidates in M31 ›
Revisiting primordial black hole dark matter from axion inflation ›
Nonuniform Particle Injection into Black Hole Jets by Radiative Magnetic Reconnection ›
Cooling of Isolated Neutron Stars with Hyperon-mixed Kaon-Condensation Matter ›
Mass-Orbital Period Distribution of Massive White Dwarfs Formed Through Stable Mass Transfer ›
The quasi-star model for Little Red Dots: potential and challenges ›
The dynamics of the Anglerfish cluster ›
Comparing gravitational wave background predictions from cosmological simulations to pulsar timing observations ›
Environmental dependence of Type Ia supernova standardization on the local luminosity-weighted age ›
Detection of cosmic strings by gravitational wave lensing. Predictions for Einstein Telescope ›
Identifying Kilonovae in the Presence of Optical Afterglow for the Wide Field Survey Telescope ›
Population synthesis of delta Scuti stars: the instability strip, period-luminosity relation, and large-separation distribution ›
Time-Domain Dust Astrophysics. I. Polarization Flares, Polarization-Angle Reverberation, and Fossil Imprints in Supernova-Illuminated Clouds ›
Solar Wind Proton Heating and its Effect on Temperature Anisotropy Evolution between 0.05 and 1 au ›
The Non-Principal-Axis Rotation and Convex Shape Model of Earth Quasi-Satellite and the Target of China's Tianwen-2 Mission (469219) Kamo`oalewa ›
A Radon Transform Perspective on Exoplanet Transits ›
Generation of TeV Photons by PeV Neutrinos in Dense Astrophysical Environments ›
Active nests at solar maximum: How nested flux emergence dominated flaring activity and structured the heliosphere ›
Bumpy inflation from explosive particle production ›
Origin of small-scale evaporation flows deep in the chromosphere during a solar flare ›
That's no moon: Exomoon survival and detection limitations ›
Centaur Longevity Revisited: Reclassification of the Bailey and Malhotra Sample with Modern Orbital Solutions and Astrometric Constraints ›
Milky Way Structure from Double White Dwarf Gravitational-Wave Sources ›
Magnetising the quokka code with fast, second-order accurate, error-correcting schemes for magnetohydrodynamics on GPUs ›
Testing Chemical Tagging with LAMOST: Intrinsic Abundance Dispersion of Subgiant Stars in the Galactic Disk ›
From Stars to Waves: Non-deterministic Inference of Microlensed Gravitational Waves ›
On the Theory of Bulk Viscosity of Cold Plasmas and Thermodynamics of Alkali-Noble Gas Cocktails ›
Spectral sirens cosmology from binary black holes populations with sharper mass features ›
Branching Universes ›
Extreme, transient bursts of energy in the auroral ionosphere. I. Predictive radar tracking ›
Orbital evolution of asymmetric binaries within accreting environments ›
Enhanced electron-beam lithography to reduce the frequency scatter of 200-400 GHz superconducting microstrip resonators for on-chip filterbank spectrometers ›
Oscillations of Dissipative Neutron Stars: The Impact of Hyperonic Reaction Rates ›
Theoretical Aspects of Direct Waves in Kerr Black Holes: Pole-Splitting Method for Ringdown Analysis ↓↑