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

Dome at sunrise

Cloud

Rainfall

S Sky
Temperature
2.3 °C
Humidity
87%
Wind
8.0 km/h
Pressure
1022.9 hPa

Moon
Latest preprints on astro-ph:
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Experimental investigation of O2 diffusion and entrapment in interstellar amorphous solid water (ASW) ›
Stellar physics at sub-nanoradian angular resolution ›
Geometry of non-Gaussianity in transient non-attractor inflation ›
An Active Galaxy Cluster Merger at Cosmic Noon Revealed by JWST Weak Lensing and Multiwavelength Probes ›
Chemical composition and enrichment of the Centaurus cluster core seen by XRISM/Resolve ›
Impact of in-situ nuclear networks and atomic opacities on neutron star merger ejecta dynamics, nucleosynthesis, and kilonovae ›
Dynamical disequilibrium in dwarf galaxies: rethinking gas dynamics, rotation curves, and dark matter inference ›
The abundance of thin dwarf galaxies: a challenge for cosmological hydrodynamical simulations ›
Intermediate Mass Black Hole Binary Evolution in Nuclear Star Clusters: the effect of the stellar mass black hole population ›
KiDS-Legacy: Constraints on Horndeski gravity from weak lensing combined with galaxy clustering and cosmic microwave background anisotropies ›
KiDS-Legacy: Constraining dark energy, neutrino mass, and curvature ›
MIRACLE III. JWST/MIRI expose the hidden role of the AGN outflow in NGC 1068 ›
Seeking Spectroscopic Binaries with Data-Driven Models ›
Dynamical constraints on the S2 (S0-2) star possible companions ›
Balmer Transition Signatures from Gas-Enshrouded, Dust-Poor Active Galactic Nuclei ›
Globular Clusters GMRT Pulsar Search (GCGPS) II: Discovery of five MSPs in M69 and M70 ›
Milky Way Globular Clusters: Nurseries for Dynamically-Formed Binary Black Holes ›
Effects of Varied Cosmic Ray Feedback from AGN on Massive Galaxy Properties ›
An Open Benchmark of One Million High-Fidelity Cislunar Trajectories ›
Connection Between Dwarf Galaxies and Globular Clusters: Insights from the Perseus Cluster Using Subaru Imaging and Keck Spectroscopy ›
The Crab Nebula Revisited Using HST/WFC3 ›
First Detection of an Ultracool Dwarf at 340 MHz: VLITE Observations of EI Cancri AB ›
Constraints on the intergalactic magnetic field from Fermi-LAT observations of GRB 221009A ›
libyt: an In Situ Interface Connecting Simulations with yt, Python, and Jupyter Workflows ›
Asteroid Occultations with VERITAS: Observations and Considerations ›
The magnetic origin of the outer boundary of sunspots ›
Classifying High-Energy Celestial Objects with Machine Learning Methods ›
Insights for Early Dark Energy with Big Bang Nucleosynthesis ›
The Interplay of Stellar Evolution and Collisions in Galactic Nuclei ›
Mantle Differentiation, Mixing and Interior-Exterior Exchange ›
Free Energy Sources of Ion-scale Waves Observed by Parker Solar Probe ›
amc: The Automated Mission Classifier for Telescope Bibliographies ›
On the Border: Searching for Cometary Activity Near the Centaur-JFC Transition Line ›
Synthetic polarization observations of magnetized pillars in HII regions: The limitations of the Davis-Chandrasekhar-Fermi method ›
The Response of Rotating Stellar Convection to Latitudinally-Varying Heat Flux ›
Probable Quasi-Periodic Oscillations in the {\tt TESS} observations of blazars in the Swift X-ray Survey ›
The energy structure function of fast radio bursts supports a stochastic origin model ›
CPI-C: Cool Planet Imaging Coronagraph on Chinese Space Station Survey Telescope ›
Kennicutt-Schmidt relation of galaxies over 13 billion years in the COLIBRE hydrodynamical simulations ›
The Simons Observatory: Development of a Pipeline to Detect Rapid Transients in Time-Ordered Data ›
Cosmological Implication of Cross-correlation between Galaxy Clustering and 21-cm Line Intensity Mapping ›
Varying core-envelope coupling efficiency identified from stellar rotation--activity relation ›
Observational evidence of tidal torque in the primordial Universe ›
Intergalactic magnetic field lower limits up to the redshift $z\approx3$ ›
Impacts of hydrogen envelope on supernova fallback and the resulting compact remnant masses ›
The Influential Roles of Gravity, Turbulence, and Magnetic Fields in Shaping the Physical Evolution of Dense Massive Clumps ›
Measurement of the cosmic ray nickel energy spectrum from 10 GeV/n to 2 TeV/n with the DAMPE ›
The hydrogen-free circumstellar interaction in the Type Ib supernova 2021efd: A clue to the mechanism of the helium-layer stripping ›
Type II and Type III Solar Radio Burst Classification Using Transfer Learning ›
The Polarized X-ray Universe: Insights and Discoveries ›
Laboratory rotational spectroscopy and interstellar search for the protein precursor 4-oxobutanenitrile (HCOCH$_2$CH$_2$CN) ›
Dynamical evolution of massless particles in star clusters with NBODY6++GPU-MASSLESS: II. The long-term evolution of free-floating comets ›
The magnitude of the dark ages 21-cm signal in the context of existing early and late time constraints on $\Lambda$CDM ›
JWST and HST observations of the host galaxy and supernova, SN 2024aihh in EP240801a at z=1.67 ›
UK White Paper on Magnetic Reconnection ›
Dark sector interactions in the $w \rightarrow -1$ limit: velocity locking in pure momentum exchange models ›
The multiphase interstellar medium as a common origin for magnetic misalignment and TB parity violation ›
Rapid sinking and efficient mergers of supermassive black holes in compact high-redshift galaxies ›
One-loop power spectrum corrections in interacting dark energy cosmologies ›
Transformer Embeddings for Fast Microlensing Inference ›
A Spatially Resolved Evolutionary Sequence of Multi-wavelength AGN Host Galaxies ›
The Domain Adaptation problem in photometric redshift estimation: a solution applied to the HSC Survey ›
Looking into the faintEst WIth MUSE (LEWIS): on the nature of ultra-diffuse galaxies in the Hydra I cluster. V. Integrated stellar population properties ›
The Impact of Initial Mass Dependent Convective Boundary Mixing on the Structure and Fates of Massive Stars ›
The low-mass and structured stellar halo of M83 argues against a merger origin for its starburst and extended neutral hydrogen disk ›
The Effect of a Non-universal Extinction Curve on the Wesenheit Function and Cepheid Distances ›
GLIMPSE-D: An Exotic Balmer-Jump Object at z=6.20? Revisiting Photometric Selection and the Cosmic Abundance of Pop III Galaxies ›
Solving the Cosmological Vlasov-Poisson Equations with Physics-Informed Kolmogorov-Arnold Networks ›
Ultra-relativistic journeys through compact astrophysical objects ›
The AURORA Survey: Constraining Chemical Enrichment Pathways at Cosmic Noon with Argon Abundances ›
Constraints on light QCD and CP-violating axions from the death line of rotation-powered pulsars ›
Vibration Isolation for the Laser Interferometer Lunar Antenna ›
Temporal Substepping Scheme for Magnetohydrodynamics with Cell-based Adaptive Mesh Refinement on Staggered Grid ›
A review on combinatorial approach to aggregation ›
Gravitational Foundations and Exact Solutions in $n$--Dimensional Fractional Cosmology ›
Portable Adaptive Optics for Exoplanet Imaging ›
Microphysics of diffusive shock acceleration: impact on the spectrum of accelerated particles ›
Modeling reflection spectra of super-Eddington X-ray sources ›
Dynamical Galactic Halo Reconstruction from Rotation Curves in Self-Interacting Fuzzy Dark Matter ›
Neutrino quantum kinetics in three flavors ›
The Luminosity Function and Clustering of H$\alpha$ Emitting Galaxies at $z\approx4-6$ from a Complete NIRCam Grism Redshift Survey ›
Extreme Neutral Outflow in a non-AGN Quiescent Galaxy at z~1.3 ›
Optimal intrinsic alignment estimators in the presence of redshift-space distortions ›
The Large-scale Environments of Low-luminosity AGNs at $3.9 < z < 6$ and Implications for Their Host Dark Matter Halos from a Complete NIRCam Grism Redshift Survey ›
Patterns of X-ray and $\gamma$-ray Flares: from Blazar to Maganetar and Sun ›
Dynamical Properties and Velocity Dispersion-Mass Relation of $z \sim 1$ Galaxy Clusters from the GOGREEN and GCLASS Surveys ›
Constraining the Extragalactic Magnetic Field: Auger Data Meet UHECR Propagation Modeling ›
Sensitivity of the redshifted 21 cm signal from the Dark Ages to parameters of primordial magnetic fields ›
Fuzzy dark matter halos with repulsive self-interactions: coherent soliton and halo vortex network with moderate self-coupling ›
The Discovery of Little Red Dots in the Local Universe: Signatures of Cool Gas Envelopes ›
Detection of low-luminosity X-ray pulsations from the accreting millisecond pulsar IGR J17511-3057: An ever-thinning thread between bright accretion and sub-luminous states ›
Euclid: Photometric redshift calibration with self-organising maps ›
Data-driven dust inference at mid-to-high Galactic latitudes using probabilistic machine learning ›
Slantwise convection and heat transport in icy moon oceans ›
The impact of radial migration on disk galaxy star formation histories I. Biases in spatially resolved estimates ›
Spatially resolved broad line region in a quasar at z=4: Dynamical black hole mass and prominent outflow ›
Estimation of Temporal Muon Signals in Water-Cherenkov Detectors of the Surface Detector of the Pierre Auger Observatory ›
Spatial Profiles of 3I/ATLAS CN and Ni Outgassing from Keck/KCWI Integral Field Spectroscopy ›
Non-linear spiral waves in accretion discs ›
A Mass-Independent Damping Timescale in Black Hole Accretion Systems ›
Forecasting the Constraint on the Hu-Sawicki $f(R)$ Modified Gravity in the CSST $3\times2$pt Photometric Survey ›
A sudden fine-scale bright kernel captured by Hi-C Flare in 11 MK emission during an M1.6-class solar flare's post-maximum phase ›
AT2022zod: An Unusual Tidal Disruption Event in an Elliptical Galaxy at Redshift 0.11 ›
Characterization of debris disks observed with SPHERE ›
Interpretable machine learning of halo gas density profiles: a sensitivity analysis of cosmological hydrodynamical simulations ›
Galaxy Cluster Detection and Dynamical Analysis in the VIPERS High-Redshift Spectroscopic Survey ›
Decisively Demonstrating Roman CGI's TTR5 Requirement by Reimaging a Newly-Discovered Brown Dwarf Orbiting a Bright Accelerating Star ›
Wind-mediated Eddington-limited emission in a $10^{4}M_\odot$ Black Hole Tidal Disruption Event ›
Fast LISA Likelihood Approximations by Downsampling ›
The Role of the Schwinger Effect in Superradiant Axion Lasers ›
$F$-term Multi-Field Inflation in Supergravity without Stabiliser Superfields ›
Lensing Stability and Scattering Phenomena in Anisotropic Black Hole Spacetimes in Plasma ›
Misspecification-robust amortised simulation-based inference using variational methods ›
The $\mu$-deformed Einstein field equations with $\mu$-dependent effective cosmological constant ›
BinaryGFH-v2: Improved method to search for gravitational waves from sub-solar-mass, ultra-compact binaries using the Generalized Frequency-Hough Transform ↓↑