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

Stars over the dome

Cloud

Rainfall

S Sky
Temperature
-2.1 °C
Humidity
94%
Wind
0.0 km/h
Pressure
1018.3 hPa

Moon
Latest preprints on astro-ph:
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Emergent Complexity in Nuclear Reaction Networks: A Study of Stellar Nucleosynthesis through Chemical Organization Theory ›
Exoplanet characterization with NASA's Habitable Worlds Observatory ›
Transiting exoplanets as the immediate future for population-level atmospheric science ›
Characterizing turbulence in galaxy clusters: defining turbulent energies and assessing multi-scale versus fixed-scale filters ›
Formation of massive multiple-star systems: early migration and mergers ›
Masers and Broad-Line Mapping Favor Magnetically-Dominated AGN Accretion Disks ›
GA-NIFS: high prevalence of dusty and metal-enriched outflows in massive and luminous star-forming galaxies at $z\sim3-9$ ›
Cosmological back-reaction of baryons on dark matter in the CAMELS simulations ›
Ultraviolet observations of atmospheric escape in exoplanets with the Habitable Worlds Observatory ›
Spectral Signatures of Spinning Dust from Grain Ensembles in Diverse Environments: A Combined Theoretical and Observational Study ›
The Energy-Duration Relationship in Astrophysical Self-Organized Criticality Systems ›
VLBI Observations of SN 2012au Reveal a Compact Radio Source a Decade Post Explosion ›
CAMELS Environments: The Impact of Local Neighbours on Galaxy Evolution across the SIMBA, IllustrisTNG, ASTRID, and Swift-EAGLE Simulations ›
Star formation quenching precedes morphological transformation in COSMOS-WEB's richest galaxy groups ›
The Role of Interferometric Phase in Measuring Black Hole Photon Rings ›
Incorporating Wavefront Error, Wavefront Sensing and Control, and Sensitivities into Exposure Time Calculations for Future Space Missions with the Error Budget Software (EBS) ›
Collision between molecular clouds IV: The role of feedback and magnetic field in head on collisions ›
Exploring the internal structure of a neutron star and the associated magnetic fields aided by the mass-radius relationship ›
NASA Decadal Astrobiology Research and Exploration Strategy (NASA-DARES 2025) White Paper -- Habitable Worlds Observatory Living Worlds Science Cases: Research Gaps and Needs ›
Generalized Bondi Accretion Flow with and without Outflow ›
Radio Signatures of Cosmic-Ray Particle Showers in Deep In-Ice Antennas ›
In-ice Radio Signatures of Cosmic Ray Particle Cascades ›
Radio Morphing: Fast computation of inclined air shower radio emission ›
Simulations of Electron Beam Interactions in Brown Dwarf Atmospheres ›
Brahe: A Modern Astrodynamics Library for Research and Engineering Applications ›
Ruling Out Compact Jets as the Dominant Source of Radio Emission in Radio-quiet, High Eddington-ratio Active Galactic Nuclei ›
High-order expansions of multi-revolution elliptic Halo orbits in the elliptic restricted three-body problem ›
A binary merger product as the direct progenitor of a Type II-P supernova ›
AstroSat UV Deep Field IV. An Extended UV disk around a massive spiral galaxy at z=0.67 ›
Constraining Inflation Models with Spinning Voids ›
Impact of a negative cosmological constant on the reconstruction of dark energy in light of DESI BAO data ›
Evaluating the efficacy of a data cube treatment procedure for kinematic analyses: application to NGC 3115 and NGC 4699 ›
SPHEREx Re-Observation of Interstellar Object 3I/ATLAS in December 2025: Detection of Increased Post-Perihelion Activity, Refractory Coma Dust, and New Coma Gas Species ›
Joint Optical-HI mock catalogs and prospects for upcoming HI surveys ›
Computing Natural Magnitudes in the Photometric Systems of Astronomical Plates using Gaia DR3 SEDs ›
Turbulent Properties of Interplanetary Coronal Mass Ejections Observed by Solar Orbiter in the Inner Heliosphere ›
The Isaac Newton Telescope Monitoring Survey of Local Group Dwarf Galaxies-VIII. A Census of Long-Period Variable Stars across the Andromeda Dwarf Satellite System ›
Nitrogen abundances in star-forming galaxies 2.2 Gyr after the Big Bang are not elevated ›
Rings around irregular bodies. II. Numerical simulations of the 1/3 spin-orbit resonance confinement and applications to Chariklo ›
Magnetic winds in resistive compact binary discs ›
The Structure of Poloidal Fields Embedded in Thin Disks ›
A New Consistency Test for the $\Lambda$CDM Model using Radial and Transverse BAO Measurements ›
Magma Ocean Waves and Thermal Variability on Lava Worlds ›
On the 3D time evolution of the dust size distribution in protostellar envelopes ›
More power on large scales ›
The Hierarchical Structure of the Open Cluster NGC 752 ›
The Potential Impact of Neuromorphic Computing on Radio Telescope Observatories ›
Slow White Dwarf Mergers as a New Galactic Source of Trans-Iron Elements ›
Limit cycles and the climate history of Mars ›
First Submillimeter Lights from Dome A: Tracing the Carbon Cycle in the Feedback of Massive Stars ›
A Study Revealing Physical Attributes of Supernova Remnant in G321.3-3.9 ›
Does the radio-active phase of XTE~J1810$-$197 recur following the same evolutionary pattern? ›
The stellar initial mass function of nearby young moving groups ›
Broad line regions behind haze: Intrinsic shape of Br$\gamma$ line and its origin in a type-1 Seyfert galaxy ›
The magnetic helicity driven solar-type dynamo ›
What can be learnt from UHECR anisotropies observations Paper III: Update with new data and Galactic magnetic fields models ›
Photometric Redshift Estimation Using Scaled Ensemble Learning ›
WISE/CatWISE Constraints on Dysonian Waste-Heat Technosignatures in Nearby Galaxies ›
Emulator-Based Inference of Cosmological Subgrid Models ›
Multi-wavelength properties of changing-state active galactic nuclei: I. the evolution of soft excess and X-ray continuum ›
New $H(z)$ measurement at Redshift = 0.12 with DESI Data Release 1 ›
Direct detection of the non-thermal X-ray emission from the Arches star cluster ›
Strong Evidence for Dark Sector Interactions ›
Expanding the C$_3$H$_6$O$_2$ Isomeric Interstellar Inventory: Discovery of Lactaldehyde and Methoxyacetaldehyde in G+0.693-0.027 ›
Possible evidence for a pair-instability supernova nature of ultra-early JWST sources ›
Temporal variability of polarization in blazars ›
Asymmetric distribution of Fe-peak elements in Cassiopeia A revealed by XRISM ›
The converging gas flow around the infrared dark cloud G28.3 ›
Characterization of two new transiting sub-Neptunes and a terrestrial planet around M-dwarf hosts ›
A free-fall-based switching criterion for P^3 T N-body methods in collisional stellar systems ›
Advanced computing for reproducibility of astronomy Big Data Science, with a showcase of AMIGA and the SKA Science prototype ›
A Study of Two Type IIb Supernovae: SNe 2008aq and 2019gaf ›
Functionalization of Benzene Ices by Atomic Oxygen ›
Exoplanet transit search at the detection limit: detection and false alarm vetting pipeline ›
Instantaneous thermally-driven erosion can explain dearth of dark near-Sun asteroids ›
A Guided Unconditional Diffusion Model to Synthesize and Inpaint Radio Galaxies from FIRST, MGCLS and Radio Zoo ›
Modified Gravity and the Origin of the Excess Radio Galaxy Number-Count Dipole ›
The combined X-ray and $\gamma$-ray modeling of millisecond pulsars PSR J0030+0451 in the dissipative magnetospheres ›
High-resolution simulations of non-thermal emission from LS 5039 ›
Revealing the diversity of Type IIn supernova progenitors through their environments ›
CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations IV. Testing warm dark matter cosmologies with galaxy scaling relations: A joint simulation-observation study using DREAMS simulations ›
Isochrone Fitting of Galactic Globular Clusters -- VII. NGC\,1904 (M79), NGC\,4372, and revision of NGC\,288, NGC\,362, NGC\,5904 (M5), NGC\,6205 (M13), and NGC\,6218 (M12) ›
Uniform models of neutron and quark (strange) stars in General Relativity ›
Cosmic rays, gamma rays and neutrinos from discrete black hole X-ray binary ejecta ›
Timing Gamma-ray Pulsars using Gibbs Sampling ›
Deep Search for Joint Sources of Gravitational Waves and High-Energy Neutrinos with IceCube During the Third Observing Run of LIGO and Virgo ›
Galaxy Mergers in UNIONS -- II: Predicting Timescales in the Post-Merger Regime ›
Impact of Nuclear Reaction Rates on Calcium Production in Population III Stars: A Global Analysis ›
A Unified Charge-Dependent Modulation Model for AMS-02 Proton and Antiproton Fluxes during Solar Minimum ›
CHEX-MATE: Relationship between X-ray and millimetre inferences of galaxy cluster temperature profiles ›
Tachyonic gravitational dark matter production after inflation ›
Brightest GRB flare observed in GRB 221009A: bridge the last gap between flare and prompt emission in GRB ›
Brightness Characterization and Modeling for Amazon Leo Satellites ›
Induced gravitational waves - beyond linear cosmological perturbation theory ›
A COLIBRI Photometric Study of SN 2025bvm: A Normal, Slowly Declining Type Ia Supernova ›
Core Scouring Dynamics and Gravitational Wave Consequences: Constraints on Supermassive Black Hole Binary Hardening ›
Popcorn in the sky: Identifying primordial black holes in the gravitational-wave background ›
Euclid preparation. Testing analytic models of galaxy intrinsic alignments in the Euclid Flagship simulation ›
Euclid preparation. Calibrated intrinsic galaxy alignments in the Euclid Flagship simulation ›
Testing subhalo abundance matching with galaxy kinematics ›
Cosmoglobe DR2. V. Spatial correlations between thermal dust and ionized carbon emission in Planck HFI and COBE-DIRBE ›
Cosmoglobe DR2. VII. Towards a concordance model of large-scale thermal dust emission for microwave and infrared frequencies ›
Cosmoglobe DR2. IV. Modelling starlight in DIRBE with Gaia and WISE ›
Axion misalignment as a synchronization phenomenon ›
First Multi-Constellation Observations of Navigation Satellite Signals in the Lunar Domain by Post-Processing L1/L5 IQ Snapshots ›
Temperature-Dependent CPT Violation: Constraints from Big Bang Nucleosynthesis ›
Cosmological Dynamics on a Novel $f(Q)$ Gravity Model with Recent DESI DR2 Observation ›
Spec-o3: A Tool-Augmented Vision-Language Agent for Rare Celestial Object Candidate Vetting via Automated Spectral Inspection ›
Mati\`ere noire et (ou) gravitation modifi\'ee : une approche historique et \'epist\'emologique ›
Kerr-Newman-de Sitter black holes in $f(R)$ gravity with constant curvature: horizon structure and extremality ›
Limits of vacuum-template subtraction for LISA massive black hole binary sources in realistic environments ›
Numerical Study of Polytropes with n=1 and Differential Rotation ›
Strong Einstein-Hilbert Gravity Inflation and ACT Phenomenology ›
Viable f(R) Scenarios Unifying Inflation with Realistic Dynamical Dark Energy ›
IndIGO-D: Probing Compact Binary Coalescences in the Decihertz GW Band ›
Oscillatory Freeze from Inertial Holographic Dark Energy ›
Chiroptical effect induced by gravitational waves ›
Bringing Computation to the data: Interoperable serverless function execution for astrophysical data analysis in the SRCNet ›
Coordinate Systems and Transforms in Space Physics: Terms, Definitions, Implementations, and Recommendations for Reproducibility ›
Landau damping of disturbances in nearly inviscid inflectional shear flows ›
Multi-Physics Bayesian Analysis of Neutron Star Crust Using Relativistic Mean-Field Model ›
Learning the relations between neutron star and nuclear matter properties with symbolic regression ›
Rotation-dependent $I$-Love-$Q$-$\delta M$ relations in perturbation theory ›
Systematic Biases in Gravitational-Wave Parameter Estimation from Neglecting Orbital Eccentricity in Space-Based Detectors ›
Exploring Lorentz Invariance Violation from Ultra-high-energy Gamma Rays Observed by LHAASO ›
Self-consistent 3D radiative transfer for kilonovae: directional spectra from merger simulations ›
Exploring the interplay between star formation efficiency and dust in regulating the UV luminosity of early systems in the JWST and ALMA era ›
A model of the heliocentric dust ring on Venus orbit ›
Time-evolving coronal modelling of the solar maximum around the solar storms in May 2024 by COCONUT ›
The PAU Survey: Measuring intrinsic galaxy alignments in deep wide fields as a function of colour, luminosity, stellar mass and redshift ›
PEARLS: 21 Transients Found in the Three-Epoch NIRCam Observations in the Continuous Viewing Zone of the James Webb Space Telescope ›
JWST Reveals a Candidate Jellyfish Galaxy at z=1.156 ›
Bayesian constraints on quark stars from multi-messenger observations ›
Angular correlation functions of bright Lyman-break galaxies at $\mathbf{3 \lesssim z \lesssim 5}$ ›
Confronting Mukhanov Parametrization of Inflationary Equation-of-State with ACT-DR6 ›
MrMARTIAN: A Multi-resolution Mass Reconstruction Algorithm Combining Free-form and Analytic Components ›
Little Red Dots and their Progenitors from Direct Collapse Black Holes ›
What determines the $\gamma$-ray luminosities of classical novae? ›
COCONUT: A coronal model with an energy decomposition strategy ›
Accelerated calibration of semi-analytic galaxy formation models ›
Needlets and foreground removal for SKAO hydrogen intensity maps ›
$\texttt{Jipole}$: A Differentiable $\texttt{ipole}$-based Code for Radiative Transfer in Curved Spacetimes ›
A Pristine Star-Forming Complex at z=4.19 ›
Gaia Barium Dwarfs and Their Ostensibly Ordinary Counterparts ›
Measuring the Central Dark Mass in NGC 4258 with JWST/NIRSpec Stellar Kinematics ›
SymBoltz.jl: a symbolic-numeric, approximation-free and differentiable linear Einstein-Boltzmann solver ›
Modeling gravitational wave sources in the MillenniumTNG simulations ›
New ultralight scalar particles and the mass-radius relation of white dwarfs -- the important role of Sirius B ›
MESA-QUEST: Tracing the formation of direct collapse black hole seeds via quasi-stars ›
Born to be recycled: a comprehensive population synthesis of the Galactic millisecond pulsars ›
Implications of Joint Spectral Analysis of Gamma-Ray Bursts detected by Fermi Large Area Telescope and Gamma-ray Burst Monitor on Phenomenological Correlations ›
Evolutionary Tracks and Spectral Properties of Quasi-stars and Their Correlation with Little Red Dots ›
Stellar Wind-Blown Bubbles as Environments for Late-Time Rebrightening of Gamma-Ray Burst Afterglows ›
Cosmic Vine: High abundance of massive galaxies and dark matter halos in a forming cluster at z=3.44 ›
First Cosmological Constraints from the Joint Analysis of Galaxy Clustering and the Kinetic Sunyaev-Zel'dovich Effect ›
Machine-Learning Estimation of Energy Fractions in MHD Turbulence Modes ›
SN 2016iog: A fast declining Type II-L supernova with an ultra-faint tail, persistently interacting with circumstellar material ›
The HITRAN2024 methane update ›
JCMT Constraints on the Early-Time HCN and CO Emission and HCN Temporal Evolution of 3I/ATLAS ›
Large Language Models for Limited Noisy Data: A Gravitational Wave Identification Study ›
The Narrow Emission Lines of Seyfert 1 Galaxies: Comparisons with a Large SDSS Sample ›
ExoMol line lists -- LXIII: ExoMol line lists for 12 isotopologues of CO$_2$ ›
Ultralight Dark Matter Constraints from NanoHertz Gravitational Waves ›
First reverberation mapping of a Bowen fluorescence line ›
Einstein Probe Discovery of an X-ray Flare from K-type Star PM J23221-0301 ›
Pre-supernova O-C shell mergers could produce more $^{44}\mathrm{Ti}$ than the explosion ›
Multiband Gravitational Wave Detection Prospects for M31 UCXB-1 System in Low and Middle Frequency Band ›
Particle production and Higgs reheating ›
A global view of post-interaction white dwarf-main sequence binaries ›
Vetting and False Positive Analysis of TOI 864.01: Evidence for a Likely Hierarchical Eclipsing Binary Masked by Dilution ›
A Long Tidal Feature Extending from a Low-Redshift Galaxy Revealed in Rubin Data Preview 1 Imaging ›
Energetic particles accelerated via turbulent magnetic reconnection in protoplanetary discs - I. Ionisation rates ›
Hidden pattern of self-invariant cosmic expansion: Empirical evidence from Hubble diagram of supernovae ›
Corrections to the Black hole entropy from a Bose Einstein condensate: a semi-classical phenomenological approach ›
Supernova constraints on lepton flavor violating ALPs ›
Sound waves from primordial black hole formations ›
Enhancing gravitational-wave detection: a machine learning pipeline combination approach with robust uncertainty quantification ›
Dark Matter in X-rays: Revised XMM-Newton Limits and New Constraints from eROSITA ›
Diffuse astrophysical neutrinos from dark matter around blazars ›
Stability of Thin Shell and Wormhole Configurations: Schwarzschild, Schwarzschild -- (Anti-) de Sitter, and FLRW Spacetimes ›
Quasi-Normal Modes and Nonlinear Electrodynamics in Black Hole Phase Transitions ›
Color-superconducting quarkyonic matter ›
Uncertainty in predicting the stochastic gravitational wave background from compact binary coalescences ›
Infrared Quantum Electrodynamics and the Rayleigh-Jeans Physics ›
Cavity Multimodes as an Array for High-Frequency Gravitational Waves ›
Machine learning for radiative hydrodynamics in astrophysics ↓↑