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

over the clouds

Cloud

Rainfall

S Sky
Temperature
3.4 °C
Humidity
68%
Wind
4.8 km/h
Pressure
1013.4 hPa

Moon
Latest preprints on astro-ph:
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Degeneracy in Accretion Disk Spectra from Naked Singularities and Kerr Black Holes: Application to the AGN MCG-06-30-15 ›
Advanced Virgo Plus for O5 -- Design Report Overview ›
GA-NIFS & JADES: Confirmation of pristine gas near GN-z11 ›
The search for Population III: Confirmation of a HeII emitter with no metal lines at z=10.6 ›
The Pristine HeII Emitter near GN-z11: Constraining the Mass Distribution of the First Stars ›
Probing Atomic Dark Matter with Stellar Streams in Milky Way-Mass Galaxies ›
Radial Velocity Orbital Solutions for Candidate Black Hole and Neutron Star Binary Systems in the Gaia Data Release 3 Catalog ›
Radiating Bondi Flows I: Dimensionless Framework and Constant Opacity Solutions ›
DETECT: A Pipeline to Quantify Detection Thresholds in Rubin for Nearby Targets Embedded in Bright Host Galaxies ›
SN 2024iss: A Multi-Wavelength Expos\'e of a Type IIb Supernova with an Early-Time Ultraviolet Spectrum and Shock Breakout Constraints ›
Radiating Bondi Flows II: Giant Planet Accretion Models ›
Probing the statistical correlation of optical tidal disruption events with high-energy neutrinos ›
Searching for Fast Astronomical Transients in Archival Photographic Plates ›
The impact of gamma-ray propagation effects on indirect dark matter searches ›
Cyclic light variations and accretion disk evolution in the LMC eclipsing binary OGLE-LMC-DPV-062 ›
Hide and Seek with Gaia. Detectability of Predicted Thin-Disc Metal-Rich RR Lyrae Binaries in Gaia DR3 and DR4 ›
Isolated or Dynamical? Tracing Black Hole Binary Formation through the Population of Gravitational-Wave Sources ›
Accurate and efficient simulation-based inference for massive black-hole binaries with LISA ›
Beyond compactness: a structural-dynamical-evolutionary manifold for the stellar-to-dynamical mass ratio in ultra-compact massive galaxies ›
Isotopic Signature of Organic Molecules from Beyond the Solar System: An Enriched Methane D/H Ratio in the Interstellar Object 3I/ATLAS ›
Astrophysics Research Organizations in the 21st Century: Database and Comparative Dashboards ›
Coma Physics of an Interstellar Object: JWST Spatial-Spectral Mapping of 3I/ATLAS ›
Refinement of Stellar Parameters for the Eclipsing Binary System KIC 8569819 using Stellar Modeling Approach ›
Circular polarization of gravitational waves from magnetorotational supernovae ›
Magnetic white dwarfs from DESI ›
A New Method of Measuring Magnetic Field Strength in Highly Structured Protostellar Envelopes ›
A Physical Model of Pulsar X-ray Filaments ›
Improved dark matter measurements with flexible modeling of resolved strongly-lensed quasar narrow-line emission ›
FAST Polarization Catalog of FRB 20240114A ›
Observations of DNC and DCO$^+$ toward the $\int$-shaped Filament and Starless Cores in the Orion Molecular Clouds ›
Synchrotron Self-Absorption Spectral Modeling Reveals a Magnetically Driven Shock-in-Jet Scenario in Blazar 1156+295 ›
Southern eROSITA bubble as a forward shock and the low-metallicity CGM. South-east side story ›
Probing the stochastic signal from primordial gravitational waves with pulsar timing arrays ›
Radiative Compression of Dense Cores in the Pillars of Creation as Revealed by JWST Extinction Mapping ›
Measurement of the Orbital Parameters, Spin and Spectral Evolution During the Main High State of Her X-1 with Insight-HXMT ›
X-Ray Polarization Study of Pulsar Wind Nebulae with eXTP: Simulation Results and Scientific Prospects ›
Field-Level Inference of Primordial Non-Gaussianity with the Quijote Simulation Suite ›
Modeling surface radiation of rotating neutron stars with Monk-NS ›
Rediscussion of Eclipsing Binaries. Paper XXX. The Slightly Evolved F-type System BK Pegasi ›
A generalized method for estimating solar wind speeds and densities using spectral broadening for a Kolmogorov turbulence spectrum ›
The Extinction Distance of Supernova Remnants in Combination with the CO Line Measurements ›
Pre-perihelion observations of comet P/2023 JN16 (Lemmon) at the 2024 apparition ›
Redshift Dipoles from Non-Geodesic Observer Congruences in Covariant Cosmology ›
Distributed accelerators in the jet of Centaurus A: the origin of the spectral hardening of very high energy gamma-rays ›
On the origin of the strong internal magnetic fields of central compact objects ›
The First GeV Gamma-Ray Flares from the CSO-like Source 4C 76.03 ›
Time-Domain Radio Loudness of Active Galactic Nuclei: Intermittency, Memory, and Jet Escape ›
Model-Independent Reconstruction of Quintessence Potential and Kinetic Energy from DESI DR2 and Pantheon+ Supernovae ›
Testing General Relativity on Galactic Scales via DESI-BAO and Strong Lensing: Circumventing Assumptions on the Hubble Constant, Sound Horizon, and Dark Energy ›
No evidence of polarization in the $11.3\,\mu$m PAH emission line by independent analyses ›
Q/W-band Observations toward Starless Cores in Orion (QWOSCO) I. Overview, Isotopologues, Isomers, and Complex Organics ›
Parallel Adaptive Reweighting Importance Sampling (PARIS) ›
First constraints on point-like astrophysical sources using Baikal-GVD muon neutrino events ›
High-resolution spectroscopic atmospheric studies of 5 hot Jupiters across the edge of the Neptune desert ›
Closed-form approximations of fundamental quantities of Lemaitre-Tolman-Bondi cosmologies from Symbolic Regression: I. Results on the Garcia-Bellido-Haugb{\o}lle parameterization ›
Revisiting the Excess of Bar-like Structures in TNG50 Early-type Galaxies: Consistency and Tension with Observations ›
Analytical Framework for Expanding Bubbles in a Hot Circumgalactic Medium ›
The precessing jet axis of the supernova remnant 3C 397 ›
Iron isotope anomalies and the origin of the Earth ›
Modelling solar radial velocities and photometric variability with SOAPv4 ›
Transient narrowband radio bursts from 1E 1547.0-5408 ›
ASKAP EMU detection of an Odd Radio Circle (ORC) candidate: J094412-751016 (Anglerfish) ›
Tracing Star Formation in Quasar Hosts via [O II] $\lambda$3727: A Kinematically Consistent Approach ›
Magnetic Field Measurements in the Solar Chromosphere Using the H$_{\beta}$ 4861\AA~Line I: Forward Modeling Based on 1D Models ›
Detection of a Molecular Cloud toward the Heartbeating Gamma-ray Source near the Microquasar SS 433 ›
Chemical Abundance Ratios of Nitrogen Rich Galaxies Identified at $z\sim 6-12$: Observational Demographics and Models ›
Research on the central region of quasars based on variability and structure function ›
Insights into the Exoplanet Radius Valley from Host-Star Ages, Activity, Chemistry, and Birth Radius ›
Investigating the propagation of small-scale flare energy in the lower and upper atmosphere of solar active region ›
Multimessenger Concordance for the Cygnus Region as the Source of the Cosmic-Ray Knee ›
The ALMA-QUARKS survey: Investigating Thermal Feedback of Massive Protostars in Hot Molecular Cores ›
Unimodular Diffusion and Interacting Vacuum Cosmology ›
Cherenkov Neutrino Telescopes: Recent Progress and Next Steps ›
A quasi-star is born: formation and evolution of accreting quasi-stars as a metallicity-independent pathway to Little Red Dots ›
Narrow iron- and nickel-K absorption lines from the eclipsing low-mass X-ray binary AX~J1745.6$-$2901 ›
The second H.E.S.S. gamma-ray burst catalogue: 15 years of observations with the H.E.S.S. telescopes ›
The fragility of the Uranian moons during the giant planet instability ›
Inflationary Phase Transitions in the Early Universe: A Bayesian Study with Space-Based Gravitational Waves Detectors ›
Are "Changing-Look" Active Galactic Nuclei Special in the Coevolution of Supermassive Black Holes and their Hosts? II. The Case of Changing-Look Narrow-Line Seyfert 1 Galaxies ›
X-ray transients in the Chandra archive: Introducing the cumulative distribution discriminator (CuDiDi) ›
Fine-tuning of light-time effect in triple systems ›
APOSTLE vs. AURIGA Simulations: How Subgrid Models Shape Milky Way Analogs ›
A joint MeerKAT and Parkes view of Omega Centauri: New TRAPUM Searches and Pulsar Timing ›
The MUSE Ultra Deep Field (MUDF) VIII. The cool gas distribution surrounding galaxies at redshifts z ~ 0.5-2 ›
Diffuse and specular brightness models applied to LEO satellites. Case study: The ONEWEB constellation ›
New surface composition and temperature maps of Pluto from New Horizons LEISA data ›
On the Constraints and Observational Manifestations of Failed Solar Eruptions in Toroidal Magnetic Cage ›
Planetary Architectures of Kepler Compact Multis with Binary Star Companions ›
H.E.S.S. observations of composite Seyfert-starburst galaxies ›
Observations of Early Black Holes Before and After JWST ›
A plug-and-play approach with fast uncertainty quantification for weak lensing mass mapping ›
JOYS: Linking the molecular ice and gas-phase composition towards the high-mass hot core IRAS 18089-1732 ›
Formation of black holes from He stars ›
Millihertz quasi-periodic oscillations in accreting X-ray pulsars ›
Lava Lakes on Io: crust age and implications for thermal output ›
Direct spectroscopic confirmation of the young embedded proto-planet WISPIT 2c ›
Solar Radio Burst in the metric to kilometric range ›
The full evolution of the type-C QPO in MAXI J1348-630 revealed by Insight-HXMT ›
Investigation of the Microquasar SS 433 with VERITAS ›
Probing the Cosmic Web with Fast Radio Bursts. I. Scattering ›
The SPHEREx Ices Investigation: An Overview ›
Using Global Gravitational Potential Weighted Correlation Function to Constrain Modified Gravity Models ›
Global Coronal Equilibria with Solar Wind Outflow II -- Optimizing the Outflow Model ›
J-PAS: unprecedented precision in stellar populations of diffuse tidal features ›
Simulations of massive star atmospheres and winds during giant eruptive and quiescent luminous blue variable phases ›
Characterizing Short-Timescale Optical Variability in Non-blazar Active Galactic Nucleus PKS~0521$-$36 Using TESS ›
Axionlike dark-matter winds driven by galactic baryon redistribution ›
QLP Data Release Notes 004: TESS-Gaia Light Curve Photometry Implementation ›
A bending in the size-mass relation of star-forming galaxies across $0.5 < z < 6.0$ at a critical stellar mass of $10^{10}M_\odot$ revealed by JWST ›
Two hot pre-white dwarfs inside the red-giant-branch planetary nebula Pa 13 -- Double core evolution or common envelope-induced rejuvenation? ›
Mainly on the Plane: Observing the Extended, Ionized Disks of Milky Way Analogs in IllustrisTNG ›
Little Red and Blue Dots: simply stratified Broad Line Regions ›
Theoretical Ion Sputtering Yields from Loose Powders using a Multiscale Monte Carlo Approach ›
White Dwarf Structure in $f(Q)$ Gravity ›
Nonlinear tails in the Kerr black hole ringdown ›
Inverse Electroweak Baryogenesis ›
Singular structures and causality of the Schwarzschild Green's function in the frequency domain ›
Breaking the degeneracy among regular black holes with gravitational lensing ›
Generalized JMN Naked Singularity Models ›
Non-local gravity effects in cosmological dynamics probed by IceCube/KM3NeT signals and dark matter relic abundance ›
Causal Structure of Spacetime Singularities and Their Observable Signatures ›
Polytropes, logotropes, the universal value of the surface density of dark matter halos, and the value of the cosmological constant ›
Dark energy and accelerating cosmological evolution in a Universe with a Weylian boundary ›
Observational Constraints on Noncoincident $f(Q)$-Gravity with Matter-Gravity Coupling ›
Kinky vortons in the 2HDM ›
S-wave kaon condensation in neutron-star matter within a chiral model framework with dynamical meson masses ›
Landau Damping of Collective Neutrino Oscillation Waves ›
Calibrating baryonic feedback with weak lensing and fast radio bursts ›
Accreting Primordial Black Holes: Dark Matter Constituents ›
Stellar angular momentum of intermediate redshift galaxies in MUSE surveys ›
SZ Lyncis: A Non-Accreting Neutron Star-delta Scuti Binary Candidate Discovered via Dynamics and Asteroseismology ›
Hic Sunt Dracones: Uncovering Dynamical Perturbers Within the Habitable Zone ›
Discovery of A Starburst in the Early Milky Way at [Fe/H] $< -2$ ›
Thermodynamics of sign-switching dark energy models ›
The maximum mass and rotational kinetic energy of rapidly rotating neutron stars ›
Probing Time-Varying Dark Energy with DESI: The Crucial Role of Precision Matter Density (\Omega_{m0}) Measurements ›
Shape of Dark Energy: Constraining Its Evolution with a General Parametrization ›
ALMA FACTS III. High-Resolution CO(2-1)/CO(1-0) Maps of Twelve Nearby Galaxies ›
Calculating the power spectrum in stochastic inflation by Monte Carlo simulation and least squares curve fitting ›
Diamond-loaded polyimide aerogel scattering filters and their applications in astrophysical and planetary science observations ›
Primordial Physics in the Nonlinear Universe: mapping cosmological collider models to weak-lensing observables ›
Primordial Physics in the Nonlinear Universe: signatures of inflationary resonances, excitations, and scale dependence ›
Constraining Brown Dwarf Desert Formation Mechanisms Through Bayesian Statistical Comparison of Observed and Simulated Populations ›
Probing small-scale dark matter clumping with the large-scale 21-cm power spectrum ›
Scalar-induced gravitational waves including isocurvature perturbations with lattice simulations ›
Dormant black hole candidates from Gaia DR3 summary diagnostics ›
State-Dependent X-ray Variability in Cygnus X-1: A 12-Year NuSTAR Timing Study of Accretion Flow Geometry ›
Three Birds with One Stone: Core-Collapsed SIDM Halos as the Common Origin of Dense Perturbers in Lenses, Streams, and Satellites ›
CHIME-o-Grav: Wideband Timing of Four Millisecond Pulsars from the NANOGrav 15-yr dataset ›
The Origin of Cross-Energy-Similar FRED Profiles in Gamma-Ray Bursts Pulses ›
On the acceleration of cosmic rays at the post-adiabatic shocks of supernova remnants ›
Machine Learning-Driven Analysis of kSZ Maps to Predict CMB Optical Depth $\tau$ ›
Simulations of the onset and dynamical evolution of inertial waves in solar/stellar interior ›
JWST observes the assembly of a massive galaxy at z~4 ›
Do z>6 quasars reside in protoclusters? ›
Synchronisation of a tidal binary by inward orbital migration. The case of Pluto and Charon ›
The dawn is quiet II: Gaia XP constraints on the Milky Way's proto-Galaxy from very metal-poor MDF tails ›
Toward testing gravity with LSST using $E_G$ ›
Guesswork in the gap: the impact of uncertainty in the compact binary population on source classification ›
Gamma-ray Time Delay and Magnification Ratio in the Gravitationally-Lensed Blazar PKS 1830-211 ›
TDCOSMO. XXIII. Measurement of the Hubble constant from the doubly lensed quasar HE1104-1805 ›
The position and resolvability of blended point sources ›
Measuring the diffuse Galactic synchrotron spectral index and curvature between 45 and 2300 MHz ›
One-loop power spectrum corrections in interacting dark energy cosmologies ›
NICER Magnetar Burst Catalog ›
The impact of non-Gaussianity when searching for Primordial Black Holes with LISA ›
Discovery of the First Five Carbon-Enhanced Metal-Poor Stars in the LMC ›
Optimal and Unbiased Fluxes from Up-the-Ramp Detectors under Variable Illumination ›
Impact of baryons on the population of Galactic subhalos and implications for dark matter searches ›
Global Magnetohydrodynamic Simulations of Monster Shocks in Neutron Star Magnetospheres ›
Energy Deposition by Galactic Cosmic Rays and Implications for Ozone Chemistry ›
Terraforming Mars: Mass, Forcing, and Industrial Throughput Constraints ›
Overmassive and Undermassive Massive Black Holes: The Role of Environment and Gravitational-Wave Recoils ›
Fuzzy Dark Matter and the Impact of Core-Halo Diversity on Its Particle Mass Constraints ›
Long-term outburst activity of comet 17P/Holmes and constraints on ejecta size distributions ›
Magnetic field measurements in a sample of Class I and flat-spectrum protostars observed with SPIRou ›
Proton Irradiation of Primitive Atmospheres of Young Exoplanets and early Earth: $N_{\mathrm{2}}O$ Greenhouse Warming and Prebiotic Synthesis ›
Gravitational collapse of a fluid with torsion into a universe in a black hole ›
Fusion and reactions of $\alpha$+$^8$Be in the Hoyle resonance and associated resonances region ›
New 511 keV line data provides strongest sub-GeV dark matter constraints ›
Search for QCD axion dark matter with transmon qubits and quantum circuit ›
Evolution of strangeness and hyperons in quarkyonic matter ›
From Stars to Molecules: AI Guided Device-Agnostic Super-Resolution Imaging ›
Composite Hybrid Inflation : Primordial Black Holes and Stochastic Gravitational Waves ›
Sub-keV dark matter can strongly ionize molecular clouds ›
Studying Ionospheric Phase Structure Functions Using Wide-Band uGMRT (Band-4) Interferometric Data ›
Super-heated first order phase transitions ›
Cooling of quark stars from perturbative QCD ›
Black Hole Superradiance of Interacting Multi-Field ›
Limits on the axion-photon coupling from Chandrayaan-2 observations ›
Influence of Fermionic Dark Matter on the Structural and Tidal Properties of Neutron Stars ›
GUT-Scale Smooth Hybrid Inflation with a Stabilized Modulus in Light of ACT and SPT Data ›
Gravitational waves from the sound shell model: direct and inverse phase transitions in the early Universe ›
Spin precession effects in the phasing formula of eccentric compact binary inspirals up to the second post-Newtonian order ›
Gravitational waves from the late inspiral, transition, and plunge of small-mass-ratio eccentric binaries ›
Dark matter mounds from the collapse of supermassive stars: a general-relativistic analysis ›
An approximate Kappa generator for particle simulations ›
Gravastar on the brane with a timelike extra dimension ›
Evidence for Multimodal Superfluidity of Neutrons ›
The Role of Inhomogeneities in the Turbulent Accretion of Black Holes ›
Environmental Measurements in the Sedrun Access Shaft to the Gotthard Base Tunnel -- a Promising Site for a Long-Baseline Atom Interferometer ›
ANNA: a toolbox for Newtonian Noise Analysis ↓↑