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

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Latest preprints on astro-ph:
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Decisively Demonstrating Roman CGI's TTR5 Requirement by Reimaging a Newly-Discovered Brown Dwarf Orbiting a Bright Accelerating Star ›
UV Luminosity Functions from HST and JWST: A Possible Resolution to the High-Redshift Galaxy Abundance Puzzle and Implications for Cosmic Strings ›
Rhea-RT: Dynamical impact of Central Molecular Zone conditions on ISM properties and stellar feedback coupling ›
KURVS: chemical properties from multiple strong line calibrations for star-forming galaxies at $z\sim1.5$ ›
Clues from $\mathcal{Q}$--A null test designed for line intensity mapping cross-correlation studies ›
Orbital migration and heating history of the Galactic disc: a transition between the bimodal discs ›
ClearPotential: Revealing Local Dark Matter in Three Dimensions ›
The mysterious Globular Cluster population of MATLAS-2019 ›
Observational constraints on 3-forms dark energy ›
Characterizing the Roman Grism Redshift Efficiency of Type Ia Supernova Host Galaxies for the High-Latitude Time-Domain Survey ›
GA-NIFS: Powerful and frequent outflows in moderate-luminosity AGN at $z\sim3-6$ ›
Transient protostellar cores in high mass star forming regions revealed by time-resolved synthetic imaging of dust emission ›
The Space-Based Time-Domain Revolution in Astrophysics ›
Detailed Chemical Abundance Analysis of the Brightest Stars in the Turranburra and Willka Yaku Stellar Streams ›
Validation of a Third Earth-sized Planet in the TOI-2267 Binary System ›
The SPace-based InterFerometer Feasibility (SPIFF) Project: Enabling Future High-Resolution Astronomy Across the EM Spectrum ›
Formation of circumstellar material during double-white-dwarf mergers and the early excess emissions in Type Ia supernovae ›
Beyond prewhitening: detection of gravity modes and their period spacings in slowly pulsating B stars using the multitaper F-test ›
Classification of a New X-ray Catalog of Likely Counterparts to 4FGL-DR4 Unassociated Gamma-ray Sources Using a Neural Network ›
Stellar properties and chemical features of the Gaia Catalogue of Nearby Stars observed by GALAH DR4 ›
High-energy astrochemistry in the molecular interstellar medium ›
Hipparcos, Gaia, and RVs reveal that the radio emitting F star HD 220242 has an M dwarf companion, a likely source of the radio emission ›
The AURORA Survey: Constraining Chemical Enrichment Pathways at Cosmic Noon with Argon Abundances ›
Deuterium fractionation and CO depletion in Barnard 5 ›
Discovery of Weak O VI Absorption in Underdense Regions of the Low-Redshift Intergalactic Medium ›
Strong Bars, Strong Inflow: The Effect of Bar Strength on Gas Inflow ›
Spectrally Resolved Gas Kinematics in Cygnus A: XRISM Detects AGN Jet-induced Velocity Dispersion in Multi-temperature Gas ›
The Narrow Emission Lines of Seyfert 1 Galaxies: Comparisons with a Large SDSS Sample ›
Galaxy Phase-Space and Field-Level Cosmology: The Strength of Semi-Analytic Models ›
FEADME: Fast Elliptical Accretion Disk Modeling Engine ›
EP250827b/SN 2025wkm: An X-ray Flash-Supernova Powered by a Central Engine and Circumstellar Interaction ›
$^{12}$CO $J$=3--2 Observations of Tycho's supernova remnant: constraints on the environmental gas properties ›
Irregularity in Active Fast Radio Burst Repeaters and Magnetar Periodic Radio Pulses: Time, Energy, and Frequency Analyses ›
Relaxation of time-variable neutron-loaded relativistic jets across the photosphere and their GeV-TeV neutrino counterparts ›
Hybrid corona and transient soft X-ray lags in Fairall 9 ›
Detectability of Atmospheric Biosignatures in Earth Analogs with Varying Surface Boundary Conditions: Prospects for Characterization in the UV, Visible, Near-Infrared, and Mid-Infrared Regions ›
MorphZ: Enhancing evidence estimation through the Morph approximation ›
Tracking Protostellar Variability in Massive Protoclusters with ALMA: I. Insights from QUARKS and MaMMOtH ›
Refined M-type Star Catalog from LAMOST DR10: Measurements of Radial Velocities, $T_\text{eff}$, log $g$, [M/H] and [$\alpha$/M] ›
Improved Identification of Strongly Lensed Gravitational Waves with Host Galaxy Locations ›
Estimating stellar atmospheric parameters and elemental abundances using fully connected residual network ›
The LEGA-C galaxy survey: multiple quenching channels for quiescent galaxies at $z\sim1$ ›
A Systematic Study of Magnetic Fields Impacts on Neutrino Transport in Core-Collapse Supernovae ›
Detailed theoretical analysis of core Helium-burning stars: Mixed mode patterns I. Impact of the He-flash discontinuity and of induced semi-convection ›
Multi-wavelength emission in resistive pulsar magnetospheres ›
FAUST XXX: Dust enhancement in the young binary L1551 IRS 5 ›
Scintillating insights into PSR~J0737$-$3039A and the interstellar plasma of the Gum Nebula from MeerKAT ›
Does the Babcock-Leighton dynamo operate in rapidly rotating solar-type stars? Exploration using a 3D dynamo model at different rotation rates ›
Isotopomer-Specific Carbon Isotope Ratio of Complex Organic Molecules in Star-Forming Cores ›
The SALT survey of helium-rich hot subdwarfs: final sample and classification ›
Application of time-series analysis methods to a multiple-sector TESS observations: the case of the radio-loud blazar 3C 371 ›
Near Ultraviolet Transient Explorer (NUTEx): A CubeSat-Based NUV Imaging Payload for Transient Sky Surveys ›
Stellar Evolution in Close Binaries: Processes and Outcomes ›
Wind-mediated Eddington-limited emission in a 1e4 Black Hole Tidal Disruption Event ›
MAUVE-MUSE: A Star Formation-driven Outflow Caught in the Act of Quenching the Stripped Virgo Galaxy NGC 4064 ›
An analytical framework for atmospheric tides on rocky planets. I. Formulation ›
FAST-MEPSA: an optimised and faster version of peak detection algorithm MEPSA ›
Is Dark Energy Dynamical in the DESI Era? A Critical Review ›
Inflation at the End of 2025: Constraints on $r$ and $n_s$ Using the Latest CMB and BAO Data ›
nDspec: a new Python library for modelling multi-dimensional datasets in X-ray astronomy ›
Stellar masses and mass ratios for Gaia open cluster members ›
OutLines: Modeling Spectral Lines from Winds, Bubbles, and Outflows ›
Can accreting isolated neutron stars be detected? ›
Constraints on the Population of Common Sources of Gravitational Waves and High-Energy Neutrinos with IceCube During the Third Observing Run of the LIGO and Virgo Detectors ›
Model independent approach towards measuring expansion and growth factor from next generation galaxy clustering and lensing angular power spectrum ›
A "New Hope" for Moon Formation: Presenting a Multiple Impact Pathway ›
Applying the BF method on the DESI evidence for dynamical dark energy models ›
Hidden No More: Spotlight on tidal disruption events in active galactic nuclei ›
Chemical enrichment in LINERs from MaNGA. II. Characterizing the shape of their radial metallicity gradients ›
Pressure and Star Formation in LITTLE THINGS Dwarf Irregular Galaxies ›
Reaching diffraction-limited localization with coherent PTAs ›
On the validity of the continuity equation in a modified gravity framework with CMB, DES 3x2pt and tomographic ISW data ›
A remarkable Gaia-assisted discovery of a temporally varying, triple-lensed quasar at z=2.67 ›
Resolving the ionizing photon budget crisis with JWST/NIRCam HII clumping constraints at z=6 ›
Inflation in light of ACT/SPT: a new perspective from Weyl gravity ›
Diversity in the haziness and chemistry of temperate sub-Neptunes ›
Weighing the Milky Way's Satellite Galaxies Using Pulsar Accelerations ›
Impact of geometry on 1D molecular-kinetics simulations of acoustic-gravity wave propagation into the exosphere ›
The LISA Astrophysics "Disc-IMRI" Code Comparison Project: Intermediate-Mass-Ratio Binaries in AGN-Like Discs ›
Updated and Projected Cosmic Microwave Background Bounds on WIMP Annihilation ›
A vision for ground-based astronomy beyond the 2030s: How to build ESO's next big telescope sustainably ›
A Stellar Magnesium to Silicon ratio in the atmosphere of an exoplanet ›
Shedding Light on Large Space-Based Telescopes: Modeling Stray Light due to Primary Mirror Damage from Micrometeoroid Impacts ›
Detection prospects for heavy WIMP dark matter near supermassive black holes, particularly in M31 ›
Signatures of star formation inside galactic outflows ›
Evidence of galaxy cluster rotation in the cosmic microwave background ›
CWTHF: Subhalo Identification with Continuous Wavelet Transform ›
Lateral Deformation of Large-scale Coronal Mass Ejections during the Transition from Non-radial to Radial Propagation ›
Two-dimensional PIC simulation of collective Thomson scattering in a beam-plasma system ›
The meaning of "Big Bang" ›
Blandford-Znajek Jets and the Total Angular Momentum Evolution of a Black Hole Connected to a Cosmic String ›
The Eschatian Hypothesis ›
Can the 3 neutrino masses really be found using SN 1987A data? ›
Gravitational-wave parameter estimation to the Moon and back: massive binaries and the case of GW231123 ›
Dark matter mounds from the collapse of supermassive stars: a general-relativistic analysis ›
Constraining Gravitational Dark Matter with LHAASO and Fermi-LAT ›
Stationary Stars Are Axisymmetric in Higher Curvature Gravity ›
Generation of proton beams at switchback boundary-like rotational discontinuities in the solar wind ›
Identification and Characterization of the Topside Bulge of the Venusian Ionosphere ›
A Nonlocal Realization of MOND that Interpolates from Cosmology to Gravitationally Bound Systems ›
Nonlinear evolution of the ergoregion instability: Turbulence, bursts of radiation, and black hole formation ›
Cosmological and lunar laser ranging constraints on evolving dark energy in a nonminimally coupled curvature-matter gravity model ›
BinaryGFH-v2: Improved method to search for gravitational waves from sub-solar-mass, ultra-compact binaries using the Generalized Frequency-Hough Transform ›
Subtracting compact binary foregrounds utilizing anisotropic statistic for third-generation gravitational-wave detectors ›
Efficient pulsar distance measurement with multiple nanohertz gravitational-wave sources ›
Exploring New Propagation Scales With Galactic Neutrinos ›
Measuring the neutron star equation of state from EMRIs in dark matter environments with LISA ›
Heterogeneous Cosmological Phase Transitions: Seeded by Domain Walls and Junctions ›
Comprehensive survey of hybrid equations of state in neutron star mergers and constraints on the hadron-quark phase transition ›
Bringing together African & European research communities with an inclusive astronomy conference ›
Tidally Delayed Spin-Down of Very Low Mass Stars ›
Probing Spin-Orbit Resonances with the Binary Black Hole Population ›
Retrograde predominance of small saturnian moons reiterates a recent retrograde collisional disruption ›
Euclid Quick Data Release (Q1): VIS processing and data products ›
The dark side of the universe may be more harmonic than we thought ›
On Validating Angular Power Spectral Models for the Stochastic Gravitational-Wave Background Without Distributional Assumptions ›
SpiderCat: A Catalog of Compact Binary Millisecond Pulsars ›
fftvis: A Non-Uniform Fast Fourier Transform Based Interferometric Visibility Simulator ›
Caustic fringes for wave dark matter ›
Pulsar Sparking: What if mountains on the surface? ›
Cosmic sign-reversal: non-parametric reconstruction of interacting dark energy with DESI DR2 ›
Metal-poor single Wolf-Rayet stars: The interplay of optically thick winds and rotation ›
Duration and properties of the embedded phase of star formation in 37 nearby galaxies from PHANGS-JWST ›
Earliest Galaxy Evolution in the CANUCS+Technicolor fields: Galaxy Properties at $z\sim10-16$ seen with the Full NIRCam Medium and Broad Band Filters ›
Collapsar Disk Outflows III: Detectable Neutrino and Gravitational Wave Signatures ›
The z = 9.625 Cosmic Gems Galaxy was a "Compact Blue Monster" Propelled by Massive Star Clusters ›
Eccentricity distribution of extreme mass ratio inspirals ›
A milliarcsecond localization associates FRB 20190417A with a compact persistent radio source and an extreme magneto-ionic environment ›
First Light for the GRAVITY+ Adaptive Optics: Extreme Adaptive Optics for the Very Large Telescope Interferometer ›
The Most Probable Behaviour of the Dark Energy Equation of State Indicates a Thawing Quintessence Field: Tomographic Alcock-Paczy\'nski Test with Redshift-Space Correlation Function II ›
Pre-flight Background Estimates for COSI ›
Investigating episodic mass loss in evolved massive stars IV. Comprehensive analysis of dusty red supergiants in NGC 6822, IC 10, and WLM ›
Direct multi-model dark-matter search with gravitational-wave interferometers using data from the first part of the fourth LIGO-Virgo-KAGRA observing run ›
Dynamical Masses and Radiative Transfer Modeling of HD 698: a Be Binary in Evolutionary Transition ›
On the Exoplanet Yield of Gaia Astrometry ›
Finite Lifetime Fragment Model 4 for Striae Formation in the Dust Tails of Comets (FLM 4) Acceleration by Lorenz-force ›
High-impact Scientific Software in Astronomy and its creators ›
High-Precision Multi-Period Analysis of the Ellipsoidal Variable Candidate TIC~470127886 from TESS Photometry ›
Advancing Identification method of Gamma-Ray Bursts with Data and Feature Enhancement ›
The FAST-SETI Milky Way Globular Cluster Survey I: A Pilot Multibeam On-the-Fly Search of Five Globular Clusters at L-Band ›
Resolving Interchange Reconnection Dynamics in a Fan-Spine-like Topology Observed by Solar Orbiter ›
Interstellar Medium in Extremely High Star-Formation Regions: A Prospect of Observations on the Millimetron Space Observatory ›
The Milky Way Imaging Scroll Painting Survey: Data Release 1 ›
Self-lensing of moving gravitational-wave sources can break the microlensing crossing timescale degeneracy ›
The impact of AGN environmental effects on testing general relativity with space-borne gravitational wave detector ›
Massive Star Clusters as sources of high-energy gamma radiation ›
Clumpy, dense gas in the outflow of NGC 1266 ›
Testing models for angular power spectra: A distribution-free approach ›
Angular momentum of vacuum bubbles in a first-order phase transition ›
Modelling cosmic-ray transport: magnetised versus unmagnetised motion in astrophysical magnetic turbulence ›
Black Hole Thermodynamics: Established Results, Unresolved Paradoxes, and Speculative Resolutions ›
Trustworthy scientific inference with generative models ›
A Markov Decision Process Framework for Early Maneuver Decisions in Satellite Collision Avoidance ›
The complementary of CTAO, direct detection and collider searches for dark matter in Effective Field Theories and Simplified models ›
High Energy Particle Production from Proton Synchrotron Radiation in Strong Magnetic Fields in Relativistic Quantum Field Theory ›
Restrictions on Initial Conditions in Cosmological Scenarios and Implications for Simulations of Primordial Black Holes and Inflation ›
Progress on the ALETHEIA project and a new approach to mitigate events overlap ›
Questions related to the Deflection of Light by Gravity determined by Soldner, Einstein and Schwarzschild ›
Bayesian Model Selection with an Application to Cosmology ↓↑