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

Before observations ...

Cloud

Rainfall

S Sky
Temperature
3.8 °C
Humidity
83%
Wind
6.4 km/h
Pressure
1019.0 hPa

Moon
Latest preprints on astro-ph:
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Reconstruction of the dark matter density profile from cosmic positron anomaly data ›
An Improved Machine Learning Approach for RFI Mitigation in FAST-SETI Survey Archival Data ›
Milky Way disc & Bulge in situ populations: ESO white paper - Expanding horizons call ›
Asteroseismology of white dwarfs in the 2040s ›
Sailing to the next safe harbour in our trip to the early Universe: The massive star population of metal-poor galaxies ›
Nova Explosions in 2040 ›
Accretion and Ejection Physics at High Time Resolution ›
The Simons Observatory: forecasted constraints on primordial gravitational waves with the expanded array of Small Aperture Telescopes ›
What Builds and Quenches the Most Massive Galaxies in the Early Universe? ›
Galaxies as stochastic systems: why the next breakthrough in galaxy evolution requires one hundred million spectra ›
A JWST Transmission Spectrum of the Temperate Sub-Neptune TOI-732 c ›
Self-confinement of relativistic pair beams in magnetized interstellar plasmas: the case of pulsar X-ray filaments ›
Revealing Callisto's Near Subsurface Thermophysical Properties with ALMA Calibration Data ›
From "The Cliff" to "Virgil": Mapping the Spectral Diversity of Little Red Dots with JWST/NIRSpec ›
The AIDA-TNG project: 3D halo shapes ›
Hunting exomoons with a kilometric baseline interferometer ›
A second planetesimal collision in the Fomalhaut system ›
The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models ›
Dark Acoustic Oscillations as an Early-Universe Explanation of the DESI Anomaly ›
In-plane Black-hole Spin Measurements Suggest Most Gravitational-wave Mergers Form in Triples ›
Bright Long Secondary Period Stars for Follow-up Observations ›
Shedding the envelope: JWST reveals a kiloparsec-scale [OIII]-weak Balmer shell around a z=7.64 quasar ›
The AIDA-TNG project: abundance, radial distribution, and clustering properties of halos in alternative dark matter models ›
Cored galaxies in cuspy dark matter halos ›
Observational constraints on the origin of the elements. X. Combining NLTE and machine learning for chemical diagnostics of 4 million stars in the 4MIDABLE-HR survey ›
The Next Generation Fornax Survey (NGFS).VIII. A Support Vector Machine Approach for Disentangling Globular Clusters from other Sources ›
Dust evolution across cosmic times as seen through DUSTY-GAEA ›
Binarity Beyond Gaia: The case for a dedicated spectroscopic survey of binary stars ›
The Era of Binary Supermassive Black Holes: Coordination of Nanohertz-Frequency Gravitational-Wave Follow-up ›
2D or not 2D? Exploring 3D relativistic magnetic reconnection dynamics with highly accurate numerical simulations ›
DESI-DR1 $3 \times 2$-pt analysis: consistent cosmology across weak lensing surveys ›
Joint cosmological fits to DESI-DR1 full-shape clustering and weak gravitational lensing in configuration space ›
Cosmological Constraints from Full-Scale Clustering and Galaxy-Galaxy Lensing with DESI DR1 ›
Clustering redshift distribution calibration of weak lensing surveys using the DESI-DR1 spectroscopic dataset ›
The Power of DESI for Photometric Redshift Calibration: A Case Study with KiDS-1000 ›
The Sesquinary Catastrophe on Deimos can reconcile its excited past with its dynamically cool present ›
MAGellanic Outflow and chemistry Survey (MAGOS): Hot cores in the LMC ›
ASKAP discovery of a 30 kpc bipolar outflow from the edge-on disk of the nearby spiral galaxy ESO 130-G012 ›
IPA. Accretion rate of a low-mass Class 0 protostar, measured via mid-infrared fluorescent OH emission ›
HEGS : Revisiting a decade of H.E.S.S. extragalactic observations ›
Exploring the Galactic Plane: A Comparative Study of Fermi-LAT Sources and HESS's Non-Detection at TeV Energies ›
LSTM-MDNz: Estimating Quasar Photometric Redshifts with an LSTM-Augmented Mixture Density Network ›
Direct calculation of steady-state hydrodynamic solar wind solutions with newtonian viscosity ›
Astrometric and Spectroscopic Analysis of IC 2714: An Open Cluster Hosting a Lithium-Rich Giant ›
Gas Accretion from a Neighbouring Galaxy Fuels the Low-luminosity AGN in NGC 4278 ›
Graph Neural Networks for Interferometer Simulations ›
Axisymmetric Modeling of DSHARP Dusty Disks: Asymmetric Structures and Inner-Disk Dispersal ›
Inferring the Intrinsic Energy Function of FRB 20220912A ›
Pulsar Science with the SKA Observatory ›
A Square Kilometre Array Pulsar Census ›
Pulsars in Globular Clusters With the SKAO ›
Galactic Centre Pulsars with the SKAO ›
Understanding the Neutron Star Population with the SKAO telescopes ›
Understanding pulsar magnetospheres with the SKAO ›
Exploring Galactic plasma with pulsars in the SKA era ›
Exploring the magnetic field structure of the Milky Way with pulsars in the SKA era ›
Understanding Pulsar Wind Nebulae with the SKA ›
Testing Gravity with Binary Pulsars in the SKA Era ›
Probing neutron star interiors and the properties of cold ultra-dense matter with the SKAO ›
The SKAO Pulsar Timing Array ›
Bayesian Smooth-Fit Extrapolation of the $^{12}\mathrm{C}+{}^{12}\mathrm{C}$ Astrophysical $S$ Factor ›
Physics-Informed Neural Networks for Modeling the Martian Induced Magnetosphere ›
Fastest or Significant: A Systematic Framework for Validating Global Minimum Variability Timescale Measurements of Gamma-ray Bursts ›
Unveiling the properties and origin of massive quenched galaxies at $z\ge2$ in the COLIBRE hydrodynamical simulations ›
Infrared SED Modeling of Velocity-Excess Maser Sources: Identifying Incipient Water-Fountain Candidates ›
ALMA and JWST Identification of Faint Dusty Star-Forming Galaxies up to z~8 ›
Weakened Inspirals I: High Mass Ratio Common Envelope Interactions in RGB Stars ›
Expanding Horizons - Transforming Astronomy in the 2040s Time-Domain Multi-Messenger Astronomy in the 2040s: EM Follow-up of LGWA Sources ›
Radio frequency interference identification using eigenvalue decomposition for multi-beam observations ›
Astrophysical Implications of Eccentricity in Gravitational Waves from Neutron Star-Black Hole Binaries ›
The dominant role of dark matter halo in quenching central galaxies ›
Multi-Energy Proton Events and Geomagnetic Storms in Solar Cycles 23 and 24 ›
Discovery of a rapidly evolving global magnetic field in the M-dwarf YZ Cet and constraints on the magnetic field of its planet YZ Cet b ›
Hydrodynamic Evolution and Detectability of Nova Remnants in the Galactic Center ›
New methods to improve the decontamination of slitless spectra ›
Maximizing the sensitivity of ELT to habitable worlds with a space-based starshade ›
Observational methods for solar origin diagnostics of energetic protons ›
The AGN nature of strong CIII emitters in the Early Universe with JWST ›
High mass accretion rates onto evolved stripped-envelope massive stars by jet-induced mass removal ›
Transformational astrophysics and exoplanet science with Habitable Worlds Observatory's High Resolution Imager ›
Understanding the chemistry of temperate exoplanets atmospheres through experimental and numerical simulations ›
MUSE Analysis of Gas around Galaxies (MAGG) - VII. Emission line galaxies near strong blended Ly$\alpha$ absorption systems at $z\gtrsim3$ ›
A direction-dependent framework for visibility plane mosaicing and primary beam correction ›
Classification of the equation of state of neutron stars via sparse dictionary learning ›
Uniform Rolling: An LSST Observing Cadence Offering Sufficient Survey Uniformity for Comprehensive Cosmological Analysis ›
How massive neutrinos reshape the cosmic web ›
XMM-Newton multi-year campaign on NGC 55 ULX-1: Resolving the wind and its variability with RGS ›
Pulsar B1237+25 at 111~MHz: average profile, mode switching, nullings, microstructure ›
Galaxy evolution in compact groups - III. Structural analysis of galaxies and dynamical state of non-isolated compact groups ›
N-emitters as possible sign-posts of GC formation ›
Warm Jupiter Tidal Migration Can Spare Inner Planets; Hot Jupiter Tidal Migration May Not ›
Decoupling perturbations from background in $f(Q)$ gravity: the square-root correction and the alleviation of the $\sigma_8$ tension ›
Double shell structure in supernova 2024ggi ›
Prompt Searches for Very-High-Energy {\gamma}-Ray Counterparts to IceCube Astrophysical Neutrino Alerts ›
A Tidal Disruption Event from an Intermediate-mass Black Hole Revealed by Comprehensive Multi-wavelength Observations ›
Probing thermal gradients of habitable-zone rocky planets using direct imaging as an anti-indicator of a global surface ocean ›
JWST MIRI color classification of mid-infrared selected galaxies: MIRI color classification toward cosmic noon ›
An effective $\boldsymbol{\Lambda}$-Szekeres modelling of the local Universe with Cosmicflows-4 ›
Closed Form Expressions for the Potentials and Accelerations of Generalized Ring Models ›
Observing spatial and temporal variations in the atmospheric chemistry of rocky exoplanets: prospects for mid-infrared spectroscopy ›
The high-redshift radio galaxy 3C 294 at low frequencies: radio detection of the X-ray Ghost ›
Cygnus X-3: A variable petaelectronvolt gamma-ray source ›
The Preliminary Mauve Science Programme: Science themes identified for the first year of operations ›
Einstein Probe Discovery of an X-ray Flare from K-type Star PM J23221-0301 ›
Comparison of General Circulation Models of the Venus upper atmosphere ›
Discovery of two new millisecond pulsars towards the Galactic bulge ›
On the Origin of Kinematic Structure in the Young Association Serpens OB2 ›
Simulation-based inference with neural posterior estimation applied to X-ray spectral fitting - III Deriving exact posteriors with dimension reduction and importance sampling ›
Multiwavelength identification of millisecond pulsar candidates in the Galactic bulge ›
Evidence of Possible Spectral Variability in the Patroclus-Menoetius Binary System ›
A finite temperature framework for quark matter with color-superconducting phases ›
A faint M$_{\rm UV} = -14.5$ Lyman continuum leaker in the reionization epoch: unprecedented Ly$\alpha$ properties at z=5.725 ›
Current observations favour phantom-enhanced nature of dark energy ›
The WINTER Observatory: A One-Degree InGaAs Survey Camera to study the Transient Infrared Sky ›
N-body interactions and collisions in circumstellar disks for planar and inclined binary star configurations ›
Strategies for Accurate Effective Point Spread Function (ePSF) Modelling on Undersampled Images ›
Dark energy and neutrinos along the cosmic expansion history ›
SNR 1987A : Spitzer data from days 6000 to 8000 revisited ›
Future Dark Energy Constraints from Atomic Clocks ›
Connecting current and future dual AGN searches to LISA and PTA gravitational wave detections ›
BeppoSAX-WFC catalog of fast X-ray transients ›
A Radio Search for Star-Planet Interaction in TOI-540 and SPECULOOS-3 ›
Robust CMB B-mode analysis with Needlet-ILC and simulation-based inference ›
Discovering gravitational waveform distortions from lensing: a deep dive into GW231123 ›
Density reconstruction from biased tracers: Testing the equivalence principle through consistency relations ›
Towards First Detection of the Solar MSW Transition With JUNO ›
Multiple mountains on a pulsar: implications for gravitational waves and the spin-down rate ›
GRHayL: a modern, infrastructure-agnostic, extensible library for GRMHD simulations ›
Cosmological Neutron Stars Produce Diffuse Axion X-Ray Signatures ›
Particle Production by Time-Varying Dark Energy and the End of Cosmic Expansion ›
Kination and the Inert Doublet Model ›
Modeling the frequency-domain ringdown amplitude of comparable-mass mergers with greybody factors ›
Fifty shades of grayness: parameterizations of spectral distortions and applications in cosmology ›
Introduction to Symbolic Regression in the Physical Sciences ›
Unraveling the anomaly in the production of $^{60}$Fe nucleus in massive stars ›
Modeling Ultra-High-Energy Cosmic Rays propagation using the input from Configuration Interaction Shell Model ›
Modified light-cylinder and centrifugal acceleration in Schwarzschild geometry ›
GWTC-4.0: Searches for Gravitational-Wave Lensing Signatures ›
Implementing F (T ) Gravity in Boltzmann Codes: A Framework for Power Spectrum Computation ›
Constraining the nuclear equation of state from terrestrial experiments and neutron star observations using relativistic mean-field models ›
Cosmology with non-linear barotropic Israel-Stewart fluid with causal relaxation time ›
Chiral magnetic effect amplified baryogenesis at first-order phase transitions ›
Photon Accelerator in Magnetized Plasma ›
On Non-Minimal Couplings to Gravity and Axion Isocurvature Bounds ›
Impact of Supercooling on Direct Searches for Dark Matter and Gravitational Wave Backgrounds ›
Exponential plateaus and inflation in metric-affine gravity ›
Delayed Scaling of Multi-Type Cosmic F- and D-strings in VOS Models ›
Multiple Axions in Laboratory Experiments ›
Science Requirement Document (SRD) for the European Solar Telescope (EST) (3rd Edition, December 2025) ›
Binary Black Hole Mergers: Spin and mass ratio effects on gravitational waveforms ›
Radiation-driven dusty outflows from early galaxies ›
Benchmarking field-level cosmological inference from galaxy redshift surveys ›
LITMUS: Bayesian Lag Recovery in Reverberation Mapping with Fast Differentiable Models ›
Unveiling the Ionized and Neutral ISM at z > 10 : The Origin of [O III] /[C II] Ratios from a Sub-parsec Resolution Radiative Transfer Simulation ›
Spatial and velocity anisotropies of stellar halos across cosmic web environments: Insights from IllustrisTNG simulation ›
Inferring and Interpreting the Visual Geometric Albedo and Phase Function of Earth ›
Spiral Structure Properties, Dynamics, and Evolution in MW-mass Galaxy Simulations ›
Design and Commissioning of an LWA Swarm Station: The Long Wavelength Array -- North Arm ›
The Hidden Role of Anisotropies in Shaping Structure Formation in Cosmological N-Body Simulations ›
Linear map-making with LuSEE-Night ›
J-VAR: Analysis of RR Lyrae light curves in seven optical bands ›
Segmentation and Tracking of Eruptive Solar Phenomena with Convolutional Neural Networks ›
A Spatial Gap in the Sky Distribution of Fast Radio Burst Detections Coinciding with Galactic Plasma Overdensities ›
SN 2024aecx: a fast-evolving Type IIb supernova with a prominent shock-cooling peak ›
Backtracking Bipolar Magnetic Regions to their emergence: Two groups and their implication in the tilt measurements ›
JWST occultation reveals unforeseen complexity in Chariklo's ring system ›
What is the contribution of gravitational infall on the mass assembly of star-forming clouds? A case study in a numerical simulation of the interstellar medium ›
Eclipsing Stellar Flare on the Demon Star Algol Binary System Observed during the MAXI-NICER Follow-up Campaign in 2018 ›
Variance of dust temperature and spectral index in Planck polarization data using spin-moment expansion ›
An accurate measure of the size of dark matter halos using the size of galaxies ›
A volcanic chronosequence as a time-resolved paleo-detector array to study the cosmic-ray flux in the Late Pleistocene and Holocene ›
Rapid Brightening of 3I/ATLAS Ahead of Perihelion ›
Oscillations of dark matter halos in galaxies and their effects on motion of stars ›
Dynamical Dark Energy and the Unresolved Hubble Tension: Multi-model Constraints from DESI 2025 and Other Probes ›
First Resolution of a Main Sequence G-Star Astrosphere Using Chandra ›
Stellar properties and chemical features of the Gaia Catalogue of Nearby Stars observed by GALAH DR4 ›
Super-resolving Herschel - a deep learning based deconvolution and denoising technique ›
From ASTRID to BRAHMA -- The role of overmassive black holes in little red dots in cosmological simulations ›
Characterisation of the Bedretto Underground Site for Fundamental Physics Experiments ›
Stellar Morphology of Optically Dark or Faint Galaxies at $z>3$ with JWST ›
Dual-coding contrastive learning based on ConvNeXt and ViT models for morphological classification of galaxies in COSMOS-Web ›
An updated efficient galaxy morphology classification model based on ConvNeXt encoding with UMAP dimensionality reduction ›
Robustness Analysis of USmorph: I. Generalization Efficiency of Unsupervised Strategies and Supervised Learning in Galaxy Morphological Classification ›
Ultralight Dark Matter Constraints from NanoHertz Gravitational Waves ›
JWST NIRSpec finds no clear signs of an atmosphere on TOI-1685 b ›
Searching potential astronomical sites in Ethiopia ›
Numerical simulations of density perturbation and gravitational wave production from cosmological first-order phase transition ›
No Dark Matter Axion During Minimal Higgs Inflation ›
Lensing by black holes within astrophysical environments ›
Wave Front Sensing demodulated at the difference frequency between two phase-modulation sidebands in a compound interferometer configuration for a gravitational-wave detector ↓↑