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

Big Dipper over the dome

Cloud

Rainfall

S Sky
Temperature
1.4 °C
Humidity
95%
Wind
0.0 km/h
Pressure
1011.5 hPa

Moon
Latest preprints on astro-ph:
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Independent Replication of Nuclear Test-Transient Correlations and Earth Shadow Deficit in POSS-I Photographic Plates ›
Large Scale Structure and Environmental Effects on Dwarf Galaxy Growth ›
Non-Cold Dark Matter from Memory-Burdened Primordial Black Holes ›
A Solar Probe of Dark Matter Decay in the Galaxy ›
Revealing the stellar population of the ultra-obscured Galactic globular cluster Glimpse-C02 ›
Lagrangian Bias as a Gaussian Random Field ›
The multi-age stellar populations of Terzan 5 as revealed by JWST ›
Imladris: a detailed and flexible model for galaxy simulations with individual stars ›
Searching for unresolved massive black hole pairs through AGN photometric variability ›
The Kormendy Relation in the First Billion Years: Evidence from $JWST$ ›
Optimisation of calibration sources for global 21-cm experiments: the REACH case ›
Generalized Predictions for the Electromagnetic Signatures of Mirror Stars ›
The Impact of Seyfert Jets on Galaxy Evolution Across Major Scaling Relations ›
Eppur non si trovano Vol. 2: No Planetary-mass Primordial Black Holes toward the Andromeda Galaxy ›
The Star Formation Factory revisited I. The impact of metallicity on collapsing star-forming clouds ›
Pegasi Ascendant: Ranking Constellation Genitives on their Aesthetic Merit ›
Formation of dust grains in the winds of cool giants, PhD thesis 1992 ›
Traces of Helium Detected in Type Ic Supernova 2014L ›
Resistive MHD Simulations of Stellar Wind-Magnetosphere Coupling in TRAPPIST-1e ›
Radiative Feedback in Population III Protostellar Growth: The Impact of HI Shielding ›
Predictions of the LSST Solar System (non-)Yield ›
A Comprehensive Analysis of WISE Mid-Infrared Colors for Obscured AGN Selection ›
A Novel Method to Construct Frequency-Domain Gravitational Waveform for Accelerating Sources ›
Planetary Radar at the Arecibo Observatory ›
A large misalignment between continuous jet and discrete ejecta in microquasar GRS 1915+105 during its obscured phase ›
Calibrating optical galaxy cluster projection effects with sparse spectroscopic samples: A clustering redshift approach ›
Relic Magnetic Fields from Non-Adiabatic Photon Freeze-Out at Recombination ›
FAST Observations of Wave-like Structures in the Radio Dynamic Spectrum of AD Leo ›
X-ray variability of SDSS J000532.84+200717.4: from a normal state to an X-weak state ›
Global asteroseismology of 19,000 red giants in the TESS Continuous Viewing Zones ›
Twists in the flow: revisiting convective mixing in rotating stellar models. I. Effect on the stellar structure ›
Three-Dimensional Ocean Dynamics and Detectability of Tidally Locked Lava Worlds ›
Revisiting Marked Galaxy Clustering from a Joint Point Process Perspective ›
A Universal 1.5 GeV Gamma-Ray Line in Active Galactic Nuclei ›
A Geometric Theory of Cosmological Structure via Entropic Curvature in Wasserstein Space ›
Misaligned rings around minor planets with moons ›
The complex dependencies of Wolf-Rayet winds -- Insights from detailed radiative transfer models ›
A comparison of pendulum models for large-amplitude longitudinal prominence oscillations ›
OJAL\'A: Optimizing J-PAS Astronomy for Large-scale Analysis. A foundation model for the SED of galaxies, QSOs and stars ›
Arches of chaos, heteroclinic connections of first-order MMRs and the chaotic transport of small bodies in the Sun-Jupiter system ›
Predicting CO and dust emission of star-forming galaxies ›
An updated picture of pre-solar history from short-lived radioactive isotopes and inferences on the birth of the Sun ›
Euclid preparation. Impact of redshift distribution uncertainties on the joint analysis of photometric galaxy clustering and weak gravitational lensing ›
Transport-Geometric Formulation of Peak Statistics: Curvature-Conditioned Point Processes and Response Hierarchy ›
20 years of monitoring: PKS 2155-304 and PKS 1510-089 in the eyes of Swift and Fermi. I. The case of PKS 2155-304 ›
Waiting time distribution of solar flares from a global perspective ›
20 years of monitoring: PKS 2155-304 and PKS 1510-089 in the eyes of Swift and Fermi. II. PKS 1510-089 and comparison ›
Imaging magnetically driven astrospheres: a forward modelling approach ›
Near-Earth asteroids in Main Belt-crossing orbits ›
Resolving Oblique Star-Disk Collisions in Quasi-Periodic Eruptions: Numerical Requirements and the Importance of Geometry ›
On the variability of the reflection nebula Van den Bergh 27 surrounding RY Tau ›
A subgrid model for chemical enrichment in cosmological simulations ›
High-Precision Near-Infrared Abundances of Solar Analogs in the YJ Bands ›
Focal plane wavefront control with model-based reinforcement learning ›
Addressing the open flux problem with a non-spherical solar coronal magnetic field model ›
Universal Non-Gaussian Signatures from Transient Instabilities ›
Distance and [Fe/H] of Galactic bulge clusters from member RR Lyrae I-band light curves ›
Curvature-induced electroweak symmetry breaking and phase transition of a Higgs-portal dark scalar field ›
ALMA Band 2 line survey of a $z = 3.44$ clumpy strongly-lensed submillimetre galaxy ›
The radial component of the local Galactic magnetic field in 3D ›
Approximate Energy-Integration Method for Identifying Collisional Neutrino Flavor Instabilities ›
Cosmological zoom-in perturbation theory as a consistent beyond point-particle approximation framework ›
First results of AMBRA: Abundant Seeds and Early Mergers as a Pathway to the First Massive Black Holes ›
Delayed Radio Flares in Neutrino-associated Blazars: The Case of TXS 0506+056 ›
The RRATalog: a Galactic census of rotating radio transients ›
Beaming of polarized radiation in subcritical X-ray pulsars ›
Information content of JWST transmission spectroscopy of the exoplanet HAT-P-12b from the optical to the mid-infrared ›
Multimessenger Constraints on Production Sites of High-Energy Neutrinos from NGC 1068 ›
Number Theory in Quantum Physics: Minicharged Particles and the Prouhet-Tarry-Escott Problem ›
Dark energy from string theory: an introductory review ›
Analytical Scaling of Relativistic Drag in the Interstellar Medium ›
Cherenkov plasmons emission by primordial neutrinos ›
Wormhole Dynamics: Nonlinear Collapse and Gravitational-Wave Emission ›
Lectures on Light Particles and Compact Objects ›
Does a wormhole survive a cosmological bounce? ›
An Asymptotically Causal Metamodel for Neutron Star Equations of State ›
Next-to-Minimal Freeze-in Dark Matter ›
Optical frequency comb Fourier transform spectroscopy of the CH$_2$$^{79}$Br$^{81}$Br, CH$_2$$^{79}$Br$_2$, and CH$_2$$^{81}$Br$_2$ isotopologues in the 1180-1210 cm$^{-1}$ region ›
Gravitational wave spectrum from first-order QCD phase transitions based on a parity doublet model ›
Baryogenesis in $SU(2)_{L}$ multiplet models ›
Topological defect induced phase separation in a holographic system ›
Stability analysis and double critical phenomenon in the Einstein-Maxwell-scalar theory ›
Modeling the refractive index profile n(z) of polar ice for ultra-high energy neutrino experiments ›
Differentiable Optics with dLux II: Optical Design Maximising Fisher Information ›
Joint Electromagnetic and Gravitational Wave Inference of Binary Neutron Star Merger GW170817 Using Forward-Modeling Ejecta Predictions ›
Higher multipoles of the cow ›
Unveiling the Coma Cluster Structure: From the Core to the Hubble Flow ›
Insights into the structure and kinematics of a Milky Way-like galaxy ›
SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field ›
Evidence for a Spectral Break or Curvature in the Spectrum of Astrophysical Neutrinos from 5 TeV--10 PeV ›
Super-Eddington accretion in protogalactic cores ›
Primordial Physics in the Nonlinear Universe: mapping cosmological collider models to weak-lensing observables ›
MARTA: The connection between chemical enrichment, feedback, and dust in a Wolf-Rayet galaxy at z${\sim}$2 ›
A galactic tug-of-war: how (not) to simultaneously fit the Milky Way satellite luminosity function and the mass-metallicity relation ›
Reverberation lags viewed in hard X-rays from an accreting stellar-mass black hole ›
CURLING -- III. Identifying Candidates of Wide-separation Gravitationally Lensed Quasars from the CatNorth Catalogue ›
Gravitational Waves from Hyperbolic Encounters of Primordial Black Holes in Dwarf Galaxies ›
Strong gravitational-wave lensing posterior odds ›
Reexamining Evidence of a Pair-Instability Mass Gap in the Binary Black Hole Population ›
Constraints on Axion-photon coupling from the Global 21-cm Signal ›
Precise Measurement of the Cosmic Ray Helium Spectrum above 0.1 PeV ›
Topological Signatures of Heating and Dark Matter in the 21 cm Forest ›
Impact of in situ nuclear networks and atomic opacities on neutron star merger ejecta dynamics, nucleosynthesis, and kilonovae ›
Primordial black holes: constraints, potential evidence and prospects ›
Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn ›
Multi-Tracer Cross-Correlations of the Unresolved $\gamma$-Ray Sky ›
The early r-process nucleosynthesis scenarios ›
Supernova interactions with aspherical circumstellar material I: calculations of light curves, AB magnitudes, spectra, and polarisation ›
Direct Abundance Maps and Radial Metallicity Gradients of two Galaxies at z~4-5 in the GARDEN Survey ›
Resolution Dependence in Magnetohydrodynamic Simulations of Neutrino-Driven Core-Collapse Supernovae ›
Physics-Informed Neural Networks for Modeling Galactic Gravitational Potentials ›
The compositions of the HR 8799 planets reflect accretion of both solids and metal-enriched gas ›
AT 2025abao: The fourth luminous red nova in M 31 ›
Single- and double-headed odd radio circles in the LOFAR surveys ›
Pulsar Discoveries from the TRAPUM UHF Survey of Fermi-LAT Sources ›
TESS Planet Occurrence Rates Reveal the Disappearance of the Radius Valley Around Mid-to-Late M Dwarfs ›
Stochastic Particle Acceleration during Pressure-Anisotropy-Driven Magnetogenesis in the Pre-Structure Universe ›
Gravitational-Wave Propagation Through the Axiverse ›
Advanced Virgo Plus for O5 -- Design Report Overview ›
Data-calibrated point spread function prediction: General description of the method and demonstration on MUSE-NFM ›
e-CALLISTO FITS Analyzer: A Software Framework for CALLISTO Solar Radio Data ›
Single vs. Binary Origin: The Diversity of Stripped-Envelope Supernova Remnants ›
Formation and disruption of wide binaries in star clusters revealed by N-body simulations ›
Enabling fundamental understanding of Nature with novel binning methods for 2D histograms ›
Searches for continuous gravitational waves from neutron stars: A twenty-year retrospective ›
The Highest-Energy Neutrino Event Constrains Dark Matter-Neutrino Interactions ›
Unique gravitational wave signatures of GLPV scalar-tensor theories ›
Investigating Production of TeV-scale Muons in Extensive Air Shower at 2400 Meters Underground ›
High-Q Superconducting Lumped-Element Resonators for Low-Mass Axion Searches ›
Development and Testing of a Modular Large-Area Cosmic Ray Telescope Using Scintillator-Fiber Hybrid Design for Millimeter-Level Muon Tracking ›
The phases of QCD reached in terrestrial and cosmic colliders ›
Probing the Scalar Hair of Rotating Horndeski Black Holes through Thick Disk Images ›
Linear stability of nonrelativistic Proca stars ›
Microscopic Description of Critical Bubbles ›
Analytic force-free jet from disk-fed rotating black holes ›
Conventional and Unitarity-Conserving Peccei-Quinn Inflation Models and ACT ↓↑