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 ...

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Temperature
13.8 °C
Humidity
68%
Wind
3.2 km/h
Pressure
1015.5 hPa

Moon
Latest preprints on astro-ph:
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Gas Motions in Hydra-A: XRISM Constraints on ICM Kinematics Across Jet-Inflated Cavities ›
Search for Planetary-mass Black Holes with an Improved Viterbi Algorithm ›
Dissecting the Scalar Cosmological Collider with the Cosmic Microwave Background ›
Late-infall-induced formation of giant planets, multi-generational planetesimals, and disk substructures ›
Dark Energy Bubble as Dynamical Dark Energy: Properties and CMB Constraints ›
Probing large mass-splitting inelastic Dark Matter with RES-NOVA ›
Bispectrum BAO and the baryon-dark matter relative velocity ›
Star formation powers optical line emission from the CGM ›
GUEST: Gravitational Universe Exploration with Satellite Tracking. A passive satellite laser-ranging mission for the dark gravitational Universe ›
Characterizing Microlensing Planetary System OGLE-2014-BLG-0676L with High-Resolution Image Constrained Light Curve Modeling ›
Precise Determination of the Metallicity and C/O of WASP-39~b From a Single JWST Instrument Mode with Phase-Resolved Cross-Correlation Retrievals ›
The Next Generation Virgo Cluster Survey (NGVS). II. A Catalog of Galaxies in the Virgo Cluster ›
Nancy Grace Roman Space Telescope Wide Field Instrument: Bright Point Source Saturation Response and Persistence Properties from Thermal-Vacuum Testing ›
First results for second generation SiSeRO CCD devices ›
Can We Find the Emission Mechanism Behind the Extremely Bright GRB 230812B? ›
Vz-GAL Dusty Star-Forming Galaxies: Revisiting the CO-H2 Conversion Factor Tension ›
Detection of cosmic strings by gravitational wave lensing. Predictions for Einstein Telescope ›
Chondrite Parent Bodies as Escaped Satellites of Proto-Planetary Embryos ›
The impact of Hawking radiation from primordial black holes on recombination and the Hubble tension ›
Capture of interstellar objects during stellar encounters ›
Stream-Driven Ignition of a Realistic Undisturbed Helium Shell on a White Dwarf ›
A multiwavelength light curve analysis of the very fast nova V1723 Sco ›
Time-Domain Axion Searches with Magnetic White Dwarfs ›
Morphology-spin connection in the SAMI Galaxy Survey ›
Examining the stellar-merger origin of the blue main sequence in the open cluster NGC\,3532 with N-body simulations ›
Azimuthal molecular variations in the AB Aur planet-forming disk ›
Universal scaling between magnetar field and initial spin period for short gamma ray bursts ›
Estimating stellar metallicities from Gaia DR3 XP data using LAMOST DR10 ›
The XMM-Newton Line Emission Analysis Program (X-LEAP) III: Earth's Magnetospheric X-ray Emission Revealed by 22-Year XMM-Newton Observations ›
Semi-Analytical Model for the Evolution of Stellar Binaries in the Empty Loss Cone of Massive Black Holes ›
Enhanced Astrometry of the Rapid ASKAP Continuum Survey: Mid and High Frequency Epochs ›
Searching for $\gamma$-ray emission from a bona fide Compact Symmetric Object sample: a $\gamma$-ray signal near GB6 J0906+4124 ›
KIC 6464285: A Solar-type Eclipsing Binary in a Hierarchical Triple System with Quasi-periodic Out-of-eclipse Modulations ›
Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity ›
Forward Modeling of the $\delta$ Sct Star V1790 Ori: $\Delta \nu$, $\Omega$, Resolution and Non-adiabatic Effects ›
Influence of local and global solar magnetic fields on medium-term forecasting of the number and parameters of coronal mass ejections ›
A Type Ia Supernova Candidate at $z\sim4.3$: A Transient Interloper in the Search for $z\sim14$ Galaxies ›
Molecular gas hidden in plain sight in the early Universe ›
Be/X-Ray Binaries: Phenomenology, Variability, and Accretion~Dynamics ›
Consistent Multi-Wavelength Spectral Modeling of Cool White Dwarfs with Carbon-Polluted Atmospheres ›
An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars ›
Modes in Transitional Millisecond Pulsars: Evidence of Pulsar Wind-Induced Disk Heating from GRMHD and Radiative Transfer ›
Dynamical formation of long-period exoplanets systems in evolving binary stars ›
Optical Spectroscopy and Temporal Evolution of the Nova V1405 Cas ›
Physical Properties of 6.7 Million Galaxies from the DESI Bright Galaxy Survey: Spectral Fitting and Systematic Tests with Mock Spectra ›
Determination of the horizontal velocity field in the solar atmosphere: Method validation using 3D MHD model ›
Identifying and Determining Atmospheric Parameters of BHB Stars Based on LAMOST DR11 ›
Will a Supernova explode in CD-30{\deg}11223? ›
Testing Theories of Solar Coronal Heating with Three-Dimensional Forward Modeling ›
NAPTIME: A Neural-Process Framework for Rubin Alert Classification ›
Decaying Dark Matter Halo Abundance from a Revised Spherical Collapse Model ›
The Large Magellanic Cloud through the lens of the James Webb Space Telescope: Binaries and the mass function in the galaxy's outskirts ›
Astrophysics on GPUs: introducing AGILE 1.0 ›
Euclid: Inferring star-formation history via cross-correlations of photometric clustering and shear with the cosmic infrared background ›
Three-Dimensional Dust Distribution in the Jovian System from Juno/Waves Observations: Insights into the Halo Ring and Magnetospheric Dust ›
Refined parameters, formation, and dynamical stability of the wild exoplanet system K2-312=HD 80653 ›
Gravitational-Wave Sky Mapping with Pulsar Timing Arrays: The Full Earth-Pulsar Response and Fundamental Resolution Limits ›
Beyond the $\alpha$ model: scaling the wind-driven accretion rate in protoplanetary disks using systematic non-ideal magnetohydrodynamical simulations ›
Search for continuous gravitational waves from the pulsar J0435+3233 ›
Electron Temperature Gradients Regulate the Duration of Two-Stage Plasmasphere Refilling ›
Gravitational waves from self-resonance during reheating with a quantum-corrected inflaton potential ›
Hawking emission of massive vector fields by Kerr black holes ›
Detecting Cosmological Stasis with Future Gravitational Wave Observatories ›
Modified Cosmology from Mass-to-Horizon Relation: Observational Bounds ›
Stochastic template banks for GW searches using low-discrepancy sequences ›
Domain Walls From Confining Bubbles: $SU(N_{c})$ Yang Mills at Finite $\theta$ ›
Accretion of multipolar massive complex scalar field packets by a Schwarzschild black hole ›
Quarkyonic Stars with Strangeness ›
Astrophysical Neutrino Sources as Colliders ›
GWTC-5.0: Tests of General Relativity ›
Gravitational wave echoes as probes of the maximum mass of strange stars in quadratic curvature-matter coupled gravity ›
Optomechanical transfer factors for scattered light noise estimations in the beamtubes of ground-based gravitational wave detectors ›
Dark matter searches with a 13 meV threshold superconducting sensor array ›
X-ray and Radio campaign of the Z-source GX 340+0: discovery of X-ray polarization and its implications ›
Evidence for a $\sim 43$ GeV $\gamma$-ray line signal in a stacking analysis of the Virgo, Fornax, and Ophiuchus Galaxy clusters ›
Polarization Measurement of Gamma-ray Bursts with Fermi-GBM: The Case of GRB 180720B ›
Revealing the $\chi_{\rm eff}$-$q$ Correlation among Coalescing Binary Black Holes and Tentative Evidence for AGN-driven Hierarchical Mergers ›
Seeing the Outer Edge of the Infant Type Ia Supernova 2024epr in the Optical and Near Infrared ›
Simulating the Solar Corona with Multiple Solar Photospheric Magnetic Maps during the 8 April 2024 Total Solar Eclipse ›
GA-NIFS: Powerful and frequent outflows in moderate-luminosity active galactic nuclei at $z\sim3-6$ ›
VLBI Diagnostics of Off-axis Jets in Radio Flares of Tidal Disruption Events ›
Hypersoft X-ray Sources as a Low-Energy Class of Luminous Cosmic Emitters ›
Monitoring the upper atmospheric temperature and interplanetary magnetic field with the GRAPES-3 muon telescope ›
Cosmic voids evolution in modified gravity via hydrodynamics ›
A Realistic Pulsar -- Supermassive Black Hole Timing Model ›
ALMA High-J CO Spectroscopy of High-Redshift Galaxies. II. 0.03" Resolution CO Kinematics Reveal Super-Eddington Accretion in a Dust-Obscured Galaxy at z=3.111 ›
Interpreting Swift and NuSTAR Observations of the Low-Luminosity Active Galactic Nucleus NGC 4278 with Radiatively Inefficient Accretion Flows and Implications for Neutrino Emission ›
Very long-term relaxation of harmonic 1D self-gravitating systems ›
Enhanced foreground mitigation in thermal SZ Compton-$y$ maps via polarization and deprojection ›
The tidal evolution of satellite galaxies in cosmological simulations: insights from COLIBRE ›
Deriving volume density profiles of filaments from observed surface densities ›
Breaking Free from the Swampland of Impossible Universes through the DESI Portal ›
HWO Target Stars and Systems: Activity and Rotation Catalog (ARC) of Potential Target Stars for the Habitable Worlds Observatory ›
On the Faint Early-time Radio and X-ray Emissions in TDE2025aarm ›
The Role of Stellar Spin in Repeating Partial Tidal Disruption Events ›
Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution ›
Amortized Simulation-Based Inference of Colliding-Wind Binaries from Short, Noisy Image Time Series ›
The Hubble Missing Globular Clusters Survey IV. Ultra-faint compact satellites of the Milky Way. The case of Koposov 2 ›
Nebular_AGN: A CIGALE module for fitting AGN emission lines ›
Pushing the Primordial Frontier: Exact Linear Solutions in Multifield Inflation ›
The Effects of Energy Conservation in Simulating Solar Eruptions ›
Thermal Sunyaev-Zel'dovich cross-correlations with unWISE galaxies: disentangling radio contamination, dust properties, and electron pressure ›
Numerical polology: towards next-generation model-building for cosmology ›
Deep Learning for Astrophysics: An Open Textbook from the NASA Cosmic Origins AI/ML Science and Technology Interest Group ›
Assembly bias from nuisance to probe I: the relation between galactic conformity and the linear matter clustering ›
The Three Hundred Project: Validating $H_0$ inference from mock X-ray and millimetre analyses of galaxy clusters ›
Pushing the Primordial Frontier: Cosmological Collider Signatures at Strong Mixing ›
Enabling Cosmic Web Analysis at Gigaparsec Scales: A Multi Block Approach for DisPerSE ›
Eccentricity as a Magnifying Glass: Precision Population Inference Enabled by Eccentric Neutron Star-Black Hole Mergers ›
Unveiling dark energy properties with high-sensitivity cross-correlations of neutral hydrogen intensity mapping and galaxy surveys ›
Constraints on Primordial Black Hole Dressed by Dark Matter Halo from Microlensing Effect of Fast Radio Bursts ›
CW Cas: A solar-type contact binary system with an unseen third companion in a hierarchical quadruple system ›
Solar, Heliospheric and Ionospheric Physics: Pathfinders, Precursors and SKAO Perspective ›
An Unsupervised Search for Novel Instrumental Glitches in LIGO O4a: Multi-Scale Sensitization, Empirical Physical Vetoes, and Rate Upper Limits ›
Regression to the Mean can Explain Saturation of Geomagnetic Storms ›
Galaxy dynamics, gravitational Vlasov-Poisson system, Landau damping, and scattering theory ›
Static horizons in cosmology ›
Cryogenic sub-Hz cROss torsion bar detector with quantum NOn-demolition Speed meter (CHRONOS) for gravitational wave detection ›
Renormalization-Group Invariant Parity-Doublet Model for Nuclear and Neutron-Star Matter ›
Measuring Primitive Accumulation: An Information-Theoretic Approach to Capitalist Enclosure in PIK2, Indonesia ›
GWTC-4.0: Tests of General Relativity. II. Parameterized Tests ›
Seidr update: photonic 'black magic' for high-contrast interferometry using kernel-nulling and photonic lanterns ↓↑