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
15.0 °C
Humidity
74%
Wind
4.8 km/h
Pressure
1012.4 hPa

Moon
Latest preprints on astro-ph:
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Multimessenger Constraints on the Central Engine in SN 2023ixf: Neutron Star or Black Hole? ›
CHARA Array Observations of the Evolved Components in Symbiotic Star Systems ›
A first-principles binary neutron star merger model of GW170817, GRB170817A, and AT2017gfo ›
Discovering Substellar Dark Matter Halos with Astrometric Weak Lensing of Multiply Imaged Quasars ›
Resolved Dust in $z\approx1$ Galaxies with JWST/MIRI MRS: Survey Description and First View on PAHs, Mid-IR Atomic Emission, and Warm H$_2$ ›
TDCOSMO. XXVII. JWST-based Lens Models and H$_0$ Measurement of WFI2033, HE0435, and PG1115 ›
Exploring the capabilities of combined modelling strategies for supernova with relativistic jets using Redback ›
Dust and PAHs in late-stage galaxy evolution: Imprints of TP-AGB dust injection, grain growth and AGN feedback in high-z quiescent galaxies with JWST and ALMA ›
Stellar Flares Rather than High $T_{int}$ As Possible Cause for the Missing Methane in Young Exoplanets: The Case Study of V1298~Tau\,b ›
Measuring Extragalactic Microlens Masses and Motions in Strongly Lensed Quasar Systems with Intensity Interferometry ›
The Limited Lifetime of Self-Gravitating Accretion Disks In Galactic Centers ›
Dynamical formation of high-eccentricity compact binaries through BH--BH*/TZO collisions ›
Formation of black hole stars via star--black hole collisions ›
BSN-VIII: Detailed Photometric Modeling of Ten W UMa Contact Binaries and a Revised Empirical Period-Mass Relationship ›
Why is there cold gas inside the Local Bubble? ›
Cluster Ages to Reconstruct the Milky Way Assembly (CARMA). V. The chronological merger tree of the Milky Way ›
Spectral Synthesis for Classical Ae Stars: H${\alpha}$ and CaII ›
Toward a realistic test of black-hole movie correlations as a probe of extreme lensing ›
A 500 pc volume-limited sample of hot subluminous stars III. The short-period binary population ›
Spin-disc misalignment drives periodic accretion and pulse profile asymmetry in X-ray pulsars ›
Magnetospheric birefringence breaks the rotating-vector model and depolarises X-ray pulsars ›
Overmassive supermassive black holes in SDSS close galaxy pairs ›
The Impact of Errors in the Shape Function of Rotating Neutron Stars in the Oblate Schwarzschild Approximation ›
Near-Infrared Spectroscopy of Low-Redshift Palomar-Green Quasars and Composite Spectra ›
PolPy: A universal tool for X-ray/gamma-ray polarimetry using common data format standards ›
High Dispersion Measure Fast Radio Bursts from Young, Dust-Poor H II Regions ›
JUG: JAX-based Unified pulsar timinG ›
Low-energy antinuclei measurements for background-free indirect dark matter searches and PBH signatures ›
Quiescent and Interacting Compact Remnant Binary Populations in the Space Telescope Era ›
A Unified Tracer Analysis of DESI DR2 Baryon Acoustic Oscillations ›
Dynamically driven collapse of a thermally stable accretion disk in a nova-like system ›
Modeling Carbon-Based Planets with MAGRATHEA ›
Dense Cores in the Vicinity of an HII Region ›
Rapid Variability and Broadband Spectral Modeling in the Flaring Activity of BL Lacertae ›
Learning the averaged history of an inhomogeneous universe from its present day density field ›
From Inspiral to Expansion: The Wake-Driven Torque on Binary Black Holes in Gaseous Medium ›
Hyperon bulk viscosity effects in neutron-star inspirals ›
Cooling-regulated gas accretion onto gap-opening planets ›
The Geometry of Ultra-Fast Outflows Probed by Soft X-ray Variability in PDS 456 ›
A decade of radial-velocity monitoring of rho Leo: moment analysis and periodic variability ›
Spherical Accretion onto Konoplya Zhidenko Black Holes: Sonic Point Analysis and Fluid Dynamics ›
CoBiToM project. III. Physical characterisation of the potential merger candidates AL Lep, ASAS J082243+1927.0, and ZZ PsA ›
Extremely Low Mass Ratio Contact Binaries. III. Photometric and Spectroscopic Investigations of Eleven Systems ›
Broadband heterodyne interferometry with a chirped femtosecond laser in the H-band ›
Dissecting ultra-diffuse galaxies in the field ›
On the theoretical instability strips of {\gamma}-Doradus stars including the effect of the metallicity and rotation ›
The Canadian Galactic Emission Mapper: A New 8-10 GHz Telescope to Map the Polarization of the Northern Sky ›
A High Velocity SiO Jet from S255N SMA3 ›
Design and implementation of an SLM-driven coherent differential imaging scheme ›
The PLACID active coronagraphic imager instrument: commissioning status ›
Search for magnetic fields in seven slowly rotating A stars ›
Guide for the Hubble Tension: Mid-Time Solutions and Generalized PAge Parameterizations ›
Development, Configuration and Performance Characterization of a Scalable BETA ASIC-Based Readout System for Multi-Channel SiPM Detectors ›
Probing magnetic fields in stars: A 2D oscillation framework including rotation and magnetism ›
Correction of the influence of rolling shutter detectors on determining the velocity of meteors from video recordings ›
JWST telemetry combined with active coronagraphy: raw contrast predictions for exoplanet imaging with the Habitable Worlds Observatory ›
Deep VISTA observations of the Magellanic Clouds (VMCDeep) ›
Explicit gauge-invariant variables in multifield inflation beyond linear order and Hamiltonian dynamics ›
On the Origin of a Dusty Circumstellar Medium around Red Supergiants ›
Inversion Framework of Internal Mass Distribution Parameters of Asteroid Apophis from Dynamical Observations ›
Three-dimensional Core-Collapse Supernova Simulations: From shell burning to shock revival ›
A high-frequency type II radio burst associated with an X2.3 class flare ›
PIFFLE: Characterizing the Foreground Contributions from 4 Decades in Halo Mass to the FRB20230907D Dispersion Measure ›
Dynamical Modeling of Kinematically Decoupled Galaxies: Structural Components ›
Astrophysical Sensitivity Projections for the IceCube Upgrade ›
Follow-up of SN 2025wny I: Space-based Observations of the First Multiply-imaged Superluminous Supernova ›
Follow-up of SN 2025wny II: Superluminous Supernova Physics at Cosmic Noon ›
Follow-up of SN 2025wny III: Spectroscopic Time-delay Measurements of a Strongly Gravitationally Lensed Superluminous Supernova ›
Follow-up of SN 2025wny IV: Photometric Time-delay Measurements of a Strongly Lensed Superluminous Supernova ›
Follow-up of SN 2025wny V: Lens Modelling and Cosmography of a Strongly Lensed Superluminous Supernova at $z = 2.015$ using Space Data ›
Characterising the Globular Cluster Systems of Three Local Group Dwarf Galaxies: NGC6822, NGC147 and NGC185 ›
Reassessing the contribution of long-GRB high-energy afterglows to the isotropic gamma-ray background after GRB 221009A ›
pyEDITH: the coronagraphic exposure time calculator for the Habitable Worlds Observatory ›
Enhancing Cosmological Constraints from Foreground-Cleaned CMB Maps Using Large-Scale Structure Surveys ›
Relativistic outflows power a quasi-periodic eruption: constraints on energetics, mass loss, and emission mechanisms ›
Fast and efficient nested sampling with BEST ›
An All-Sky Catalog of 6.5 Million Primary Red Clump Stars from Gaia DR3 XP Spectra ›
Distinct Modes of Pulsar Glitch Activity Revealed by the Waiting-Time--Amplitude Morphology ›
Exploring the sensitivity of in-ice radio detectors to cosmic ray mass composition ›
A Clearer View of HAT-P-1 b: JWST NIRSpec G395H Reveals Water, Carbon Dioxide, and Possibly Hydrogen Sulfide ›
ExoMOD I. A Forward Model for the Orbital Architecture of Kepler Multi-Planet Systems ›
ExoMOD II. A Statistical Model of Transit Timing Variations in Kepler Multi-Planet Systems ›
A Similarity Theorem and Its Breakdown in Atomic Black Hole Accretion ›
Detecting Axion-Like Particles With Coiled Optical Fibers I: Silica Fibers ›
A microwave SQUID multiplexing concept for macro-cryogenic calorimeter arrays ›
Creation of an inflationary epoch from an Emergent Universe through quantum tunneling ›
Horizon-Dependent Tube MPC for Elliptical-Orbit Rendezvous Under Mass Uncertainty ›
Future of Artificial Intelligence for Science in Japan 2024 Community Report ›
Dynamical friction on black holes in scalar field environment ›
Devoured by a Hairy Gargantua: Probing Massive Scalar Charges with Non-minimal Curvature Coupling with Extreme-Mass-Ratio Inspirals ›
Editorial: Promoting Green Computing in High Energy Physics and Astrophysics ›
Solar Magnetic Configuration Control over Radiation Belt Electrons ›
Separate universe in multifield inflation: a phase-space approach ›
DESI Data Release 1: Stellar Catalogue ›
Reappraising the Elatina series: What if the Solar Interpretation Were Correct? ›
One-Loop Galaxy Bispectrum: Consistent Theory, Efficient Analysis with COBRA, and Implications for Cosmological Parameters ›
Renormalization group corrections to $\Lambda$CDM model and observational consequences for $H_0$ tension ›
A Practical Study of Lightweight Neural Gravitational-Wave Detection in Real LIGO Noise: Models, Ablations, and Open Software ›
Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy ›
Spectroscopic analysis and RHD modeling of the first Ca II H and H-epsilon flare spectra from DKIST/ViSP ›
The Binary Populations of Stellar Streams are Set by Cluster Dynamics ›
Fast modelling of ionization balance in the intergalactic medium: I- implications for the IGM metallicity ›
NOEMA3D: Extended CO, [C I] and dust in massive star-forming main-sequence galaxies at cosmic noon ›
Probing the IMF in the Early Universe -- Direct measurements in the Bo\"otes I UFD with JWST/NIRCam ›
Co-evolution of Supermassive Black Holes and their Host L* galaxies: implications for Milky Way and M31 ›
A Steep-Extinction Quasi-stellar Object at z=4.6: JWST Evidence for Abundant Small Dust Grains ›
GATOS XV: A JWST/MIRI survey of extended circumnuclear dust emission in nearby Seyfert galaxies ›
A self-consistent single-fluid framework for neutron stars admixed with mirror dark matter ›
The Stellar Observations Network Group (SONG) -- A Legacy Archive of Stellar Time-Domain Spectroscopy ›
On the astrophysical origin of cosmic rays: Constraining the Ultra-High-Energy Cosmic Ray Horizon through Nearby Galaxy Distributions ›
Constraints on the magnetic field in the hadronic scenario for the origin of the radio halo in the A1795 galaxy cluster ›
A Systematic Trend in the Observed vs. Predicted Radii of Transiting Brown Dwarfs ›
Distinct Jet Properties in the X-Ray-Obscured State of GRS 1915+105 ›
Qualification pathways for Photonic Integrated Circuits in Astrophotonic Space Missions ›
A bestiary of low-level electrical artifacts in SPHEREx flight data ›
Exact spherical-wave forward model for radio reflection from stratified media and implications for the anomalous-polarity events observed by ANITA ›
Assessing the Impact of High-Resolution Imaging on Statistical Validation of TESS Planet Candidates ›
Supernova 1987A was a "failed supernova" twenty thousand years before its jet-driven explosion ›
Magnesium silicate condensation in sub-Neptune envelopes: the fundamental link between chemistry, structure, and observables ›
Status of BICEP Array and Integration of the 220/270 GHz Receiver ›
Distinguishing cold and self-interacting dark matter through topological analysis ›
The MegaWave Radio Surveyor ›
Primordial black holes from Q-balls produced in a first-order phase transition ›
WimPyC: an extension module of WimPyDD for the calculation of WIMP capture in celestial bodies ›
A parameterized equation of state for dark energy and Hubble Tension ›
Assessing astrophysical foreground subtraction in DECIGO using compact binary populations inferred from the first part of the LIGO-Virgo-KAGRA's fourth observation run ›
Can UV meet IR in the Swiss cheese? ›
Optimized numerical evolution of perturbations across sharp background trajectory turns in multifield inflation ›
An Asymptotically Causal Metamodel for Neutron Star Equations of State ›
Irreducible Gravitational Wave Background as a Particle Detector ›
Model-Building Implications from Light Magnetic Monopoles: A Case Study of Flavour Deconstruction ›
Determination of the metric of a Schwarzschild black hole surrounded by a halo of dark matter ›
Photon Acceleration in Magnetized Plasma: A Mechanism for Fast Radio Bursts ↓↑