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

over the clouds

Cloud

Rainfall

S Sky
Temperature
2.6 °C
Humidity
94%
Wind
3.2 km/h
Pressure
1013.8 hPa

Moon
Latest preprints on astro-ph:
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SGNL: Scalable Low-Latency Gravitational Wave Detection Pipeline for Compact Binary Mergers ›
Combining CMB datasets with consistent foreground modelling ›
Large-Scale Structure Probes of the Post-Inflationary Axiverse ›
Heavy black hole seed survivors in dwarf galaxies: a case study of Leo I ›
SRGt 062340.2-265751 confirmed as a nova-like cataclysmic variable with a possible magnetic nature ›
Micrometeoroid Impact Rate Analysis for an Artemis-Era Lunar Base ›
Sub-Gyr variability around the SFMS and its contribution to the scatter ›
Dents in the Mirror: A Novel Probe of Dark Matter Substructure in Galaxy Clusters from the Astrometric Asymmetry of Lensed Arcs ›
The essential elements of dust evolution: a-C(:H) nanoparticle sub-structures and photo-fragmentation ›
HiSAXy: A fast methodology for solar wind structure identification in millions of time series ›
Secondary small-scale dynamics of a Rayleigh-Taylor unstable solar prominence ›
Machine Learning-Driven Analysis of kSZ Maps to Predict CMB Optical Depth $\tau$ ›
ALMA Sub-parsec Resolution Dense Molecular Line Observations of the NGC 1068 Nucleus ›
Kinematic and extinction analysis of a potential spiral arm beyond the Galactic bar ›
Synthetic JWST galaxy images in the TNG50 simulation - I. Model validation and comparison to observations ›
How Low Can You Go: Constraining the Effects of Catalog Incompleteness on Dark Siren Cosmology ›
Comprehensive Listing of 208 Nova White Dwarf Masses As the Primary Determinant of Spectral-Class and Light-Curve-Class ›
Blind Strong Gravitational Lensing Inversion: Joint Inference of Source and Lens Mass with Score-Based Models ›
Comparative Analysis of 10 - 50 MeV Solar Proton Events at Lagrange Point 1 and the Geostationary Orbit ›
FermiPhased: A tool for phase-resolved likelihood analysis of Fermi-LAT data ›
Using ML-based Regression Techniques to Mitigate GOES Energetic Proton Flux Data Contamination and Magnetospheric Effects ›
Empirical measures of the largest amounts of magnetically-induced radius inflation in low-mass stars ›
JWST provides a new view of cosmic dawn: latest developments in studies of early galaxies ›
The Dual Nature of Solar Wind Structuring: Resonant Standing Waves and Laval Nozzle Dynamics in Coronal Streamers ›
SCATTER Common Envelope Formalism for Triples ›
Calcium Excess in Novae: Beyond Nuclear Physics Uncertainties ›
On the Energetic Role of Forward Neutrino Scattering in Core-Collapse Supernovae ›
Investigation on the Predictive Potentiality of Photospheric Magnetic Parameters for Distinguishing Confined from Eruptive Solar Flares ›
Detecting FRB by DANCE: a method based on DEnsity ANalysis and Cluster Extraction ›
Precise Measurement of Cosmic Ray Light and Helium Spectra above 0.1 Peta-electron-Volt ›
LHAASO Detection of Ultra-High-Energy Gamma-Ray Emission toward the Giant Molecular Clouds ›
Unveiling the Nature of Superorbital Modulation of SMC X-1 using NinjaSat ›
Discovery of an X-ray Luminous Radio-Loud Quasar at $z=3.4$: A Possible Transitional Super-Eddington Phase ›
A deep X-ray look to the most obscured quasar at z~3.6 and its environment ›
Quokka-based understanding of outflows (QED) - IV. Limitations of H$\alpha$ as an outflow diagnostic ›
Probing Lorentz Invariance Violation at High Energies Using LHAASO Observations of GRB221009A via DisCan Algorithm ›
NGC 6860, Mrk 915, and MCG -01-24-012. II. Inflowing and outflowing cold molecular gas and the connection with ionized gas in Seyfert galaxies ›
Formation of millisecond pulsar-helium star binaries ›
Sym-EFT: Accelerating Effective Field Theory of Large Scale Structure with Symbolic Regression ›
Spatially-resolved PAH_3.3 emission and stellar ages in ram pressure stripped clumps at z~0.3 ›
Stellar Population Astrophysics (SPA) with the TNG 23 IR elemental abundances of 114 giant stars in 41 Open Clusters ›
The most distant optically polarised GRB afterglow: GRB 240419A at z = 5.178 ›
Searching for Electromagnetic Counterpart Candidates to GW231123 ›
Mass determination of the three long-period Neptune- and sub-Neptune-sized planets transiting TOI-282 ›
Upper limits on atmospheric abundances of KELT-11b and WASP-69b from a retrieval approach ›
High-spectral Resolution, Multi-wavelength Center-to-limb Observations of the Sun ›
On the possibility of using decayless kink oscillations of coronal loops to forecast powerful solar flares and coronal mass ejections ›
Co-existence of Internal Gravity Waves and Tayler-Spruit Magnetic Fields in the Radiative Core of Low-mass Stars ›
Multiplicity of stellar systems in the solar neighbourhood, wide binaries, and planet-hosting stars ›
The stellar mass function of quiescent and star-forming galaxies and its dependence on morphology in COSMOS-Web ›
A Mass-Independent Damping Timescale in Black Hole Accretion Systems ›
Focus Point on Tensions in Cosmology from Early to Late Universe: Part II: New Directions in the Light of Observations from the Most Modern Astronomical Facilities ›
Spectrum of PeV Cosmic-Ray Protons and Helium Nuclei with IceCube ›
Optimizing broadband microwave absorbers for applications in the 70-200 GHz range ›
Near-degeneracy effects in Quadrupolar Mixed Modes. From an Asymptotic Description to Data Fitting ›
A subpopulation of low-mass, spinning black holes: signatures of dynamical assembly ›
EMPEROR I. Exoplanet MCMC parallel tempering for RV orbit retrieval ›
Reviving Quadratic Inflation: Minimal Deformation for CMB Compatibility and Reheating Consistency ›
Intensive X-ray/UVOIR continuum reverberation mapping of the Seyfert AGN MCG+08-11-11 ›
Linking Warm Dark Matter to Merger Tree Histories via Deep Learning Networks ›
A scaling relationship for non-thermal radio emission from ordered magnetospheres - II. Investigating the efficiency of relativistic electron production in magnetospheres of BA-type stars ›
Modeling Solar Atmosphere Dynamics with MAGEC ›
Charge-dependent spectral softenings of primary cosmic-rays from proton to iron below the knee ›
Recovering Ion Distribution Functions: II. Gyrotropic Slepian Reconstruction of Solar Wind Electrostatic Analyzer Measurements ›
Crossing the veil of the brightest radio relic in the sky MACS J0717.6+3745 ›
Investigating the imprints of tidal features on simulated galaxy outskirts in LSST-like mock observations ›
Upper Limits on Radio Emission from the K2-18 System ›
Unsupervised Discovery of High-Redshift Galaxy Populations with Variational Autoencoders ›
$\texttt{unimpeded}$: A Public Nested Sampling Database for Bayesian Cosmology ›
Chemical Evolution and Kilonova Implications of Post-Merger Accretion Disk Winds ›
Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation ›
Dark Secrets of Baryons: Illuminating Dark Matter-Baryon Interactions with JWST ›
CATS: Empowering the next generation of rocket scientists through educational flight computers ›
Higgs inflation in Weyl-invariant Einstein-Cartan gravity ›
Effective Field Theories for Neutron Stars Physics ›
Fast and Flexible Neutrino Decoupling Part I: The Standard Model ›
Millicharged Particle Production in Pulsars via the Schwinger Effect ›
Novel Solar System Probes for Primordial Black Holes ›
Low-reheating scenario in dark Higgs inflation and its impact on dark photon dark matter production ›
Exact Renormalisation Group Evolution of the Inflation Dynamics: Reconciling $\alpha$-Attractors with ACT ›
Quantum Gravity, de Sitter Space, and Normalizability ›
One Galaxy Sample to Rule Them All: Halo Occupation Distribution Modeling of DES Year 3 Source Galaxies ›
The distribution of ultra-high-energy cosmic rays along the supergalactic plane measured at the Pierre Auger Observatory ›
Narrow line AGN selection in CEERS: spectroscopic selection, physical properties, X-ray and radio analysis ›
Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry ›
The radio properties of the JWST-discovered AGN ›
Constraining the potential of the Milky Way using stellar streams and the Inverse Time Integration method ›
Search for a diffuse flux of photons with energies above tens of PeV at the Pierre Auger Observatory ›
Dynamics of $Z_N$ domain walls with bias directions ›
Updated cosmological constraints on axion dark energy with DESI ›
Testing the Shock-cooling Emission Model from Star-disk Collisions for Quasi-periodic Eruptions ›
Super-Eddington accretion in high-redshift quasar hosts: Black-hole driven outflows, galaxy quenching, and the nature of little red dots ›
Jet-environment interaction after delayed collapse in binary neutron star mergers ›
One-loop kernels in scale-dependent Horndeski theory ›
On the calculation of p-values for quadratic statistics in Pulsar Timing Arrays ›
A deep dive down the broad-line region: permitted OI, CaII and FeII emission in an AGN Little Red Dot at z=5.3 ›
On the Interpretation of Velocity Residuals in Protoplanetary Disks ›
On the Efficiency of Producing Gamma-Ray Bursts from Isolated Population III Stars ›
Constraints on the progenitor and explosion of SN 2024ggi in harmony with pre-explosion detection and hydrodynamic simulations ›
Modelling the M68 stellar stream with realistic mass loss and frequency distributions in angle-action coordinates ›
Renormalization-Free Galaxy Bias in Unified Lagrangian Perturbation Theory ›
DiskMINT: Self-Consistent Thermochemical Disk Models with Radially Varying Gas and Dust -- Application to the Massive, CO-Rich Disk of IM Lup ›
Role of sunspot latitude versus tilt in determining the polar field and amplitude of the next cycle: Cause of the weak Solar Cycle 20 ›
The Hubble Tension resolved by the DESI Baryon Acoustic Oscillations Measurements ›
Not All Sub-Neptune Exoplanets Have Magma Oceans ›
Solar limb faculae: intensity contrast from two vantage points ›
Design and Scientific Prospects of the POLAR-2 Mission ›
AppleCiDEr II: SpectraNet -- A Deep Learning Network for Spectroscopic Data ›
Picoflares in the Quiet Solar Corona: Solar Orbiter Observations Halfway to the Sun ›
Estimating Orbital Parameters of Direct Imaging Exoplanet Using Neural Network ›
Evidence of Energy Injection in the Short and Distant GRB 250221A ›
The Missing Mechanism: Picoflare Heating in the Solar Corona ›
Wind-AE: A Fast, Open-source 1D Photoevaporation Code with Metal and Multi-frequency X-ray Capabilities ›
The Physical Origin of Periodic Density Structures in the Solar Wind: Coronal Streamers as Magnetohydrodynamic Resonators ›
Detection of the stochastic gravitational wave background with the space-borne gravitational-wave detector network ›
On the Inner Crusts of Neo-Neutron Stars: exotic light nuclei, diffusional and thermodynamical stability ›
Bright ring features and polarization structures in Kerr-Sen black hole images illuminated by radiatively inefficient accretion flows ›
Background stability and annual modulation test using PICOLON ultra-pure NaI(Tl) detector ›
Effects of the ekpyrotic mechanism on inflationary phase in loop quantum cosmologies ›
The importance of being non-minimally coupled: scalar Hawking radiation from regular black holes ›
Gravitational waves from the sound shell model: direct and inverse phase transitions in the early Universe ›
Cosmological and High Energy Physics implications from gravitational-wave background searches in LIGO-Virgo-KAGRA's O1-O4a runs ›
Geometric acceleration in $f(Q,C)$ theories ›
Conserved Quantities in Expanding G\"odel Cosmology ›
Computing the Full Earth System at 1 km Resolution ›
Observational tests of the conformal osculating Barthel-Kropina cosmological model ↓↑