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

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S Sky
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1019.3 hPa

Moon
Latest preprints on astro-ph:
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A Missing Latent, Not a Missing Simulator: Radius-Augmented Inference for Real JWST Retrieval ›
Generation of UL-Axions by a Kerr Black Hole. Part III: The fate of its Axion Wind ›
Comment on: "The Preprint Evolution: The Rise of Unreviewed Drafts on arXiv and its Implications for Astronomy" ›
Testing internal dynamics in neutron stars with radio pulsar timing ›
Optimizing spectral-matching component separation for measuring CMB B-mode polarization with a satellite mission ›
Towards robust simulations of the galactic dynamo: a cross-code comparison between Eulerian and Lagrangian schemes ›
Point spread function requirements for dark matter subhalo detection with the Habitable Worlds Observatory ›
Inferring magnetic field strengths in high-redshift lensing galaxies from Faraday rotation measure observations ›
Neutrino flavor instabilities intermediate between slow and fast ›
Full orbital solution and dynamical masses for a new shell-Be + sdOB binary AN Col ›
Collapse-accelerated small-scale dynamos in the first stars and galaxies ›
Extending the Pulsar radio population through Quantum Vacuum Cherenkov Emission ›
TOI-1408: the limb darkening models, photometric and Doppler noises, and the exoplanetary system ›
Learning Approximate Isometric Embeddings for Efficient Template Placement ›
Separating the Optical to Near-Infrared Light of AGN and Their Host Galaxies ›
X-ray Characterization of Galaxy Groups and Hickson Groups in COSMOS-Web to z~3.8 I. X-ray Luminosity Function Evolution ›
Suppression of spiral density waves in collisionless accretion flows ›
Super-resolving Polarized Dust Emission with Transformer-Based Multi-Tracer Fusion ›
DESI Interacting Dwarfs Survey: Multiple Evolutionary Channels of Dwarf Galaxies Driven by Major Dwarf Interactions ›
The Largest Catalog of Dwarf Galaxy Groups: Transient Structures or Building Blocks of the Universe? ›
Star Cluster Populations in 38 Spiral Galaxies: Evidence for Near-Universal Mass and Age Distributions from PHANGS ›
Do Astronomical Foundation Models Know When They Will Fail? ›
The 200-300 GHz Survey for 18 Class II Disks in the Ophiuchus Star-Forming Complex ›
Performance of AutoRegressive Planet Search methodology on simulated PLATO lightcurves ›
A Refined Analytic Oblate--Schwarzschild Model for Thermal X-Ray Pulse Profiles of Rotating Neutron Stars ›
Distinguishing the origin of cosmic birefringence: dark energy, dark matter, and neutrino asymmetry ›
Mesoscale Turbulence in Type Ia Supernova Deflagrations II. Evidence for Fuel Preheat Due to Flame Thermal Expansion from Lagrangian Analysis ›
The Structure in the Structure Function of Black Hole Light Curves ›
A New Analysis Tool for Radial Pulsations ›
Robust Bayesian non-linear pulsar timing and noise analysis using a sequential data-tempered ensemble sampler ›
Formation and Eruption of a Vortex-driven Magnetic Flux Rope in the Simulated Quiet Sun ›
Joint RV-Astrometric Analysis of two-planet system HD 65216: Prospects for Gaia DR4 ›
Study of the Ultra-Long GRB 220627A: Exploring a Possible Blue Supergiant Collapsar Origin ›
Plato benchmark stars I. The initial benchmark sample ›
Candidate X-ray Counterparts of Ultra-High-Energy Emission of the Galactic Microquasar V4641 Sgr Revealed by Einstein Probe ›
XMM-Newton Resolves Parsec-scale X-ray Jets in the PeVatron Microquasar V4641 Sgr ›
Comparing the size evolution of GRB 221009A with afterglow models ›
No Convincing Evidence for Tidal Binary Clusters in the Galaxy ›
The 2015-2017 Large EVPA Rotation in OJ 287: Dominant Propagating Component in a Helical Magnetic Field with Time-Dependent Viewing Geometry ›
Twins in the Shadow: Phase Transitions in Proto-Neutron Stars ›
A two-stage settling of the Milky Way disk revealed by precise ChronoGal ages ›
Merger remnant in TXS 1033+026 - I: $\rm H\alpha$ and HI 21-cm observations suggest counter-rotating gas ›
Discovery of thermal radio recombination line emission toward the high-mass protostar IRAS18162$-$2048 ›
A multi-scale view of molecular gas and magnetic fields in the Antennae galaxies ›
Guide field effects on particle acceleration in three-dimensional relativistic magnetic reconnection ›
The origin of dispersion in the wind mass-loss rate--luminosity relation of massive O stars ›
Dark Energy Survey Year 6 Results: fast and interpretable posterior predictive checks for correlated cosmic probes ›
Forward Bayesian Inference for the Binary Black Hole Populations ›
A novel, fast, and accurate code for cosmological loop calculations ›
Design, Fabrication, and Free-Space Characterization of a Two-Photon-Polymerized Nano-printed Photonic Lantern ›
Probing Early Phases of the Epoch of Reionization with the $\mathrm{kSZ}^{2}\times21\,\mathrm{cm}^{2}$ Cross-Correlation ›
Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on 28 model parameters in the CAMELS suite ›
Searching for Green Pea Galaxies in the SFACT Survey ›
Temporal Variability of Titan's Middle-Atmospheric Zonal Winds from Southern Fall to Late Winter (2016-2023) ›
Charged anisotropic white dwarfs in $f\left({R}, {T}\right)$ gravity ›
Toward Resolution Convergence for Star Formation and Galactic Winds in Galaxy Simulations ›
Chaotic signatures in extreme-mass-ratio systems surrounded by bosonic environments ›
FlashSinkhorn 2: Block-Sparse Entropic Optimal Transport ›
High Energy Neutrinos, Gravitational Waves, and Dark Matter from a Cosmological First Order Phase Transition ›
Post-Training Quantization of Autoregressive Weather Models ›
Multi-Band Constraints on Cosmic Strings: Unifying Harmonic and Burst Spectra ›
Non-Gaussian timing residual skewness in pulsar timing arrays ›
Kinetic Equilibrium between SIMP Dark Matter and Radiation via Internal Bremsstrahlung ›
First strength measurements of low-energy resonances in the $^{45}$Sc($p,\gamma$)$^{46}$Ti reaction and its astrophysical implications ›
Big Bang Nucleosynthesis Constraint on $B$-mesogenesis ›
Higgsino dark matter compatible with the LUX-ZEPLIN high-energy nuclear-recoil event and IceCube constraints ›
Cosmological implications of tracker scalar fields: Testing the evidence for dynamical dark energy with recent data ›
Dark Energy Survey Year 6 Results: Redshift Calibration of the MagLim++ Lens Sample ›
Growth of Aromatic Hydrocarbon Dust Particles in the Extremely Metal-poor Galaxy Sextans A ›
An Effective Theory for Biased Tracers via the Boltzmann-Equation Approach ›
Non-adiabatic Effect on Convective Mode ›
Dark Energy Survey Year 6 Results: Galaxy-galaxy lensing ›
Learning to See Sharper: A Physics-Informed Artificial Intelligence Framework for Super-Resolving Galaxy Spectra ›
Primitive recovery methods for binary neutron star mergers with tabulated equations of state in SPHINCS_BSSN ›
JWST Nebular Spectroscopy of SN 2023qov: Circumstellar Dust Emission in a Normal Type Ia Supernova ›
SVOM/C-GFT: Instrumentation and Performances on the SVOM Alerts ›
A New Record Census of Dwarf AGN and a Bimodal $M_{\rm BH}$-$M_{\star}$ Scaling Relation with DESI DR1 ›
Diverse Histories and Common Origins of Nitrogen-enhanced JWST Galaxies ›
Probing the molecular gas content of galaxies in an over-dense group at z~0.7: A test case for environmental quenching ›
Cosmology with Multi-Wavelength Line Intensity Mapping Synergies in the SKAO Era ›
Diameters and Temperatures VII: High-angular resolution measurements of Solar-type stars with the CHARA Array ›
Supernovae Ia ejecta velocities and host galaxy environments: the role of survey-selection effects ›
Quantitative Links between Formation and Atmospheric Composition for Giant Planets ›
Discovering Substellar Dark Matter Halos with Astrometric Weak Lensing of Multiply Imaged Quasars ›
Reassessing the contribution of long-GRB high-energy afterglows to the isotropic gamma-ray background after GRB 221009A ›
First Light of Neutron Star Mergers: Off-axis Cocoon Cooling X-ray Emission from Short Gamma-Ray Burst Jets ›
hyprfine: simulating the 21-cm signal from the Dark Ages through to the Epoch of Reionization on a GPU ›
Physical properties of compact star-like systems harboring traversable wormholes: Effects of chaotic magnetic fields and anisotropic matter ›
Deep Learning Search for Gravitational Waves from Compact Binary Coalescence ›
$\xi R\phi^2$ non-minimal coupling, and the long range gravitational potential for different spin fields from 2-2 scattering amplitudes ›
A Vector-Like Lepton Interpretation of the High-Energy Nuclear Recoil Candidate in LUX-ZEPLIN ↓↑