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

S Webcam

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S Sky
Temperature
19.8 °C
Humidity
69%
Wind
0.0 km/h
Pressure
1007.7 hPa

Moon
Latest preprints on astro-ph:
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Astro-Hunters: Machine Learning for Exoplanet Transit Detection in TESS Photometry ›
Supernova remnant 0509-67.5 is consistent with an explosion inside an old planetary nebula (SNIP) ›
The Mass Function of Neutron Stars from Core-Collapse Supernova Simulations ›
Heating Up the Black Hole X-ray Binary Accretion Disk by Superradiance ›
The impact of recombination during tidal disruption events ›
The fraction of periodic SN Ib/c light curves ›
A deep learning algorithm for black hole spin estimation using hot-spot secondary images ›
Recurrent Multi-year Mg II BAL Variability in SDSS J1333+0012 ›
Quasar Impostors: Two Extremely UV-Bright ($M_{\rm UV}\approx-23.5$) Reionisation-Epoch Galaxies Powered by Very Massive Stars ›
Radiation damage to the Hubble Space Telescope has been several years out of phase with the Solar cycle ›
Automated Assignment and Prediction of Molecules in Astronomical Line Surveys Using Machine-Learning-Based Chemical Embeddings ›
Mapping the Information Geometry of an Unresolved Dark Matter Population using a Differentiable Strong Lensing Simulator ›
Testing MOND-like modifications to gravity using growth-rate measurements and one-loop corrections to the matter power spectrum ›
Accretion of AGN Stars under Influence of Disk Geometry II: The Adiabatic Regime and Runaway Collapse Induced by Self-gravity ›
Asteroseismic analysis of red giants in eclipsing binaries using two methods: implications for scaling relations and chemical composition ›
The VLA and High-Frequency SETI: Expanding the Search for Life ›
CosmoPyro: Gradients for Gravitational-Wave Cosmology ›
Continuum Variability in AGN: Evidence for Systematically Suppressed Fluctuations in the BAL Population ›
The Tidal Venus Phenomenon: Demographics and Case Studies ›
PowerFull: fast and accurate computation of the relativistic angular galaxy power spectrum including local primordial non-Gaussianity ›
High-Redshift Type Ia Supernovae Exhibit Enhanced Calcium Abundances ›
Modeling the Gravitational Wave Signal from the X-ray Pulsar Her X-1 ›
The Atacama Cosmology Telescope: Passband Measurements with an Analysis of Systematic Errors ›
The Inbound Gas and Dust Evolution of Interstellar Comet 3I/ATLAS from Optical Spectroscopy and Multi-band Photometry ›
Dynamics of tidal dwarf galaxies in the system Arp 72 ›
An invariant energy release hierarchy in a repeating fast radio burst ›
Stellar Abundances as Probes of Rocky Exoplanet Interiors: The Mantle Composition and Mineralogy of GJ 486b ›
The MAGPI Survey: Emission Line Products Data Release and the Role of Spectroscopic Aperture Covering Fraction on the Balmer Decrement-Stellar Mass Relation ›
A model for the enhanced production rate of early-type hypervelocity stars in the Galactic halo ›
Time-dependent Evolution of Proton Spectra in Supernova Remnants and Their Contribution to Galactic Cosmic Rays ›
On coordinate frames relevant for pulsar physics ›
Beyond Idealized PAHs: Infrared Signatures of Carbon-Chain Defects from Shock Synthesis ›
Kinematics and Dynamics of the Open Cluster NGC 2302 ›
Investigating the properties of nearby young moving groups using GaiaDR3 ›
Hybrid disc geometry for shocked accretion flows: Unveiling QPOs in black hole X-ray binaries ›
An Empirical Effective-Temperature Calibrations for Galactic B/A Supergiants ›
Hector Galaxy Survey: Falling in Between - Infalling Galaxies in the Midst of the Abell 3667 Merger ›
Looking for TRAPPIST-1 external planets' emission in JWST archival data ›
Broadband Chiral Primordial Gravitational Waves from Constant-roll Inflation in Parity-violating Symmetric Teleparallel Gravity ›
The Total and Polarized Radio Emission from the Innermost Jets of a High-Redshift Quasar and a Candidate at Parsec-Scale Resolution ›
A generalized quadratic balance relation for nonradial nonadiabatic pulsations ›
Multi-zone Modeling of Blazar Jets: Constraints from GeV-Optical Correlation and Short-Timescale Variability ›
Size-Mass Relation Shows Its Colours: Contrasting Physical Imprints of Galaxy Evolution in Rest-Frame UV and Optical ›
Millimeter and sub-millimeter characterization of polymers used for infrared filters in high-sensitivity cryogenic microwave telescopes ›
Automatically distinguishing Rubin transients from AGN using variability metrics ›
A metallicity sweet spot for disc fragmentation and planet formation ›
Simulation of advective accretion flows around black holes under various outer boundary conditions ›
Estimation of systematic error from bulk deformation of end test mass induced by photon calibrator for LIGO post-O5 gravitational wave projects ›
VERITAS 2.3.1: Optimisation and Characterisation of the Enhanced Readout ASIC for the NewAthena Wide Field Imager ›
The efficient star-forming regions of stripped-envelope supernovae ›
First demonstration of a multimode-to-multimode photonic lantern for astronomy ›
Asgard/NOTT: Status of laboratory nulling performance ›
Constraining Cosmic-Ray Acceleration and Escape in Middle-Aged Supernova Remnants with GeV-TeV Gamma-Ray Observations ›
Towards end-to-end Bayesian forward models in global 21-cm cosmology: surrogate modelling and marginalisation of beam uncertainty ›
Quadrupole White-light Sources in an X1.2 Flare Observed by ASO-S/LST/WST and SDO/HMI ›
Physical Optics Analysis of Polarization Effects in SO LAT Reflectors ›
The progenitors of $z\gtrsim10$ JWST galaxies in the COLIBRE simulations ›
Quantifying uncertainty in the neutron-star equation of state using point estimates and posterior distributions ›
A Search for helium in the atmospheres of three sub-Neptunes and a super-Earth around M-dwarfs ›
The Ultrafast Line-Driven Wind from the Double-Degenerate Merger Remnant WD J005311 ›
Dipolar power asymmetry in wide-angle correlations of galaxy density, velocity and ellipticity ›
Asteroseismology of the multiperiodic field SX Phe pulsator BL Camelopardalis ›
Wet Removal and Cloud Enhancement: The Microphysics of Cloud-Haze Interactions on Sub-Neptunes ›
Real-Time RFI Mitigation in SPOTLIGHT: A Two-Stage Approach for Transient Searches ›
The Effective Velocity of Transferred Mass: How Momentum Prescriptions Determine Binary Orbital Evolution ›
No Persistent Helium Absorption in LHS 1140 b: Four JWST/NIRISS SOSS Transits and Multi-epoch Stellar He I Variability ›
Inferring the Dark from the Observable: Estimating Halo Masses Using Galaxy Properties ›
A comprehensive SKA Survey of lensing clusters and lensed galaxies ›
Tracing gas outflows in molecular gas-rich galaxies with the SKA ›
Effects of manufacturing tolerances on the performance of metamaterial microwave anti-reflection coatings ›
Diffuse HI emission in the circumgalactic medium of NGC891 and NGC4565 - III: azimuthal profiles ›
A Diagnostic Inverse-PINN Study of Identifiability in Reduced Black-Hole Spin Inference ›
JW-SSD: A Multimodal Benchmark Dataset for Fine-Grained Sunspot Classification ›
JW-FD: A Long Horizon Multimodal Solar Flare Forecasting Dataset ›
An axion constraint from the diffuse supernova neutrino background indicated by Super-Kamiokande ›
Safe Domain Adaptation for Physics: Overcoming Nuisances, Label Shifts, and Simulation Priors ›
Towards Quantum-Dot Detectors as Barcodes for Dark Matter Interactions ›
Evolution of lunar wake potentials: structure, energy conversion, and their imprints on velocity distributions ›
Probing Sub-GeV Dark Matter with the Migdal Effect at JUNO ›
Technical Proposal for the Atom Interferometer CERN Experiment (AICE) Facility ›
Could John Ellard Gore have pre-empted the Hertzsprung-Russell diagram? ›
Identifying Cost-Favorable Locations for Cosmic Explorer ›
Cosmology with the angular cross-correlation of gravitational-wave and galaxy catalogs: Forecasts for next-generation interferometers and the Euclid survey ›
Probing dipolar power asymmetry with galaxy clustering and intrinsic alignments ›
A Microphysical Probe of Neutron Star Interiors: Constraining the Equation of State with Glitch Dynamics ›
$\mbox{H}$ $\mbox{I}$ 21-cm Absorption Spectra Classification using Machine Learning ›
Magnetohydrodynamic Simulations of Transonic Accretion Flows ›
Cosmological Dynamics of Multi-Axion Quintessence ›
pop-cosmos: Redshifts and physical properties of KiDS-1000 galaxies ›
Synthetic Spectral Library of Optically Thick Atmospheres for Little Red Dots ›
Conditions for planetesimal formation via the streaming instability persist under turbulence driven by magnetorotational instability ›
The dominance of turbulence over magnetism in the formation of massive star cluster seeds ›
Nonthermal Velocity Dispersion in the Outer Disk of HL Tau ›
Nexae in caverna: the secular evolution of disks via collectively excited, transient spiral structure ›
Model-independent reconstruction of cosmic thermodynamics and dark energy dynamics ›
A Cosmological Uncertainty Relation and Late-Universe Acceleration ›
Particle Acceleration, Coronal Neutrino Production, and the Diffuse Extragalactic Neutrino Background from Supermassive Black Holes ›
Observation of spontaneous N-bearing PAH formation using ion trap: a new formation pathway in the interstellar medium ›
Spectral energy-loss bump and $\gamma$-ray pulsar halos ›
Inferring Globular Cluster Initial Mass Function from Stellar Streams ›
Hybrid neural denoising for resource-efficient near- and sub-threshold radio triggering of extensive air showers ›
DELOS: Contrastive Deep Learning for Low-SNR Blind Transit Searches in Kepler Photometry ›
The baryonic Tully-Fisher relation as an independent direct probe of cosmology and of the nature of dark matter ›
Latent thermal instability ›
How can we finally see the first light? Status and perspective in the search for Population III stars ›
The Best Guess: Testing new and old formalisms for the common envelope against observations ›
The Age-Thickness Relation as a Tracer of the Merger History of Disk Galaxies ›
JWST/NIRCam Imaging of Young Stellar Objects. IV. Detailed Imaging of the Protoplanetary Disk around TW Hya ›
A Sequentially-Valid Reanalysis of DESI's Dynamical Dark Energy Signal ›
Turbulent Convection: Modal Equations and Energy Pathways ›
Investigation of Calcium Dust in the Interstellar Medium ›
Reconstruction of ASO-S/HXI Solar Flare Hard X-ray Source Images with Physics-Constrained Deep Network ›
SPURS: Massive Stars, Dense Gas, and Ly$\alpha$ Escape in GN-z11 at $z = 10.6$ ›
Performance Analysis of the Asgard/NOTT Nulling Interferometer: Optimizing Observing Modes for High-contrast Detection ›
A NuSTAR Reflection-Spectroscopy Survey of Cygnus X-1 ›
Inflationary thermal Krylov complexity ›
Toward Efficient and Accurate EMRI Parameter Estimation: A Machine Learning-Enhanced MCMC Framework ›
Rotating neutron stars within the macroscopic effective-surface approximation ›
New Spallation Background Rejection Techniques to Greatly Improve the Solar Neutrino Sensitivity of JUNO ›
Towards First Detection of the Solar MSW Transition With JUNO ›
Compact Stars as Portals to Extra-Dimensional Dark Matter ›
Leveraging rapid parameter estimates for efficient gravitational-wave Bayesian inference via posterior repartitioning ›
Scalar shortcut to beyond-Kerr ringdown tests and their complementarity with black-hole shadow observations ›
Thermodynamic behavior of cosmological models with fractional entropy ›
Scalar Photon Coupling and Modified Photon Evolution: CMB Signatures and Cosmological Constraints ↓↑