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

Before observations ...

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S Sky
Temperature
2.6 °C
Humidity
55%
Wind
0.0 km/h
Pressure
1022.4 hPa

Moon
Latest preprints on astro-ph:
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JWST Constraints on Primordial Magnetic Fields ›
The Thermodynamic and Kinematic Evolution of Circumgalactic Gas around $z=1$ in the IllustrisTNG model ›
The evolution of the baryonic content and mass profiles of satellite galaxies in the MTNG simulations ›
spectroxide: A code package for computing cosmic microwave background spectral distortions ›
ORCHARD: A General Planetary Evolution Code ›
SN Ia Population Machine. I. A Unified Cosmological Simulation-Binary Synthesis Framework Establishing Non-universal Delay-time Distributions and Cosmic Progenitor-channel Dominance Crossover ›
Cosmic gas accretion from filaments onto galaxy clusters using the IllustrisTNG simulation ›
Galactic tides and the outer density profile of the Sculptor and Ursa Minor dwarf spheroidals ›
Multi-component, axisymmetric dynamical models of dSphs based on distribution functions: inferences on dark matter and intermediate-mass black holes in Draco and Ursa Minor ›
The Bulge Cluster Origin (BulCO) survey with CRIRES at the ESO-VLT: a chemical screening of the Globular Cluster NGC 6553 ›
A Monte Carlo method for tracking dust properties during coagulation in protoplanetary disks ›
The effects of image augmentations when training machine learning models in astronomy ›
Bound or blown: the fate of hot gas in galaxy groups ›
Seismic background mitigation with the Lunar Gravitational-wave Antenna ›
$N$-body modelling of the ED-2 stream progenitor shows Gaia BH3's formation involved dynamical interactions ›
Joint Multiband Photometry with crowdsource ›
Decoupling the AGN outflow and star-forming disk kinematics in the nuclear region of NGC 7582 with JWST NIRSpec and MIRI/MRS ›
Ultra-thick warm absorbers: Enlarging the parameter space of AGN ionised outflows ›
Can BLR line profile shape improve single-epoch black hole mass estimates? ›
TDCOSMO XXVI: Uniform lens modeling of eight doubly imaged quasars ›
Forward modeling solar spectra onto Doppler images of {\lambda} And ›
A Physics Informed Bayesian Neural Network for the Neutron Star Equation of State ›
Pair-Rich Corona of an Accreting Kerr Black Hole ›
Moving-Mesh Simulations of Mini-Common Envelope Ejection in Classical Novae ›
Galaxy mergers and disk angular momentum evolution: stellar halos as a critical test ›
Core Collapse Supernova Modeling: The Next Ten Years ›
Variance-aware model discrimination with the Sunyaev-Zel'dovich effect of the 21 cm background (SZE-21cm) ›
RSCL Earth Lookback Simulator: A Real-Time Multi-Physics Framework for Relativistic Signal Propagation from Confirmed Milky Way Exoplanets ›
Hourly radio variability of PDS70c from time-differential photometry ›
The Singular Behaviour of Ambipolar Diffusion Revealed by 1D Cartesian Solutions ›
The Unstable Chromosphere: Effects of the Thermal Farley-Buneman Instability Across a Broad Range of Solar Chromospheric Conditions ›
Exploring the Impact of Tilted Magnetic Dipoles on the Atmospheric Dynamics of Hot Jupiters: Towards an Improved Magnetohydrodynamic Framework ›
Symmetric kiloparsec-scale radio knots in NGC 7213: evidence for a confined weak jet and recurrent nuclear activity ›
V446 Cephei: a $\beta$ Cep pulsator in a multiple system ›
Non-Monotonic Rotation Imprint on Time-Integrated Neutrino Spectral Moments in a 15\,$M_\odot$ Core-Collapse Supernova Sequence ›
Constraining the nature of active galactic nuclei through circumgalactic Lya emission at z=2-3 ›
The Impact of Elliptical Broad-Line Regions on Reverberation-Based Black Hole Mass Estimates ›
Multi-tracers, multi-surveys: data-driven EFT prior calibration from the PFS--DESI overlap ›
Spectral Evolution and Transient Broad-Line Features in the Isolated AGN UNAM-KIAS 613 ›
Revealing a Systematic High-latitude Current Sheet at Jupiter ›
Oxygen Isotopic Compositions of Chondrules as Probes of Solar Protoplanetary Disk Formation ›
Disc lifetime distribution as a function of the mass of host star ›
The GMRT High-Resolution Southern Sky Survey for pulsars and transients -- VIII: Orbital Variability and the Evolution of a 1-Day He-WD Millisecond Pulsar J2101-4208 ›
Correlation Between Lunar Surface and Exospheric Sodium: Effects of Albedo-Driven Temperature on Multilayer Sodium Reservoirs Rather Than Surface Abundance Variations ›
Recovering cosmological parameters from the mock gravitational wave data of the Einstein Telescope ›
LAMOST J052016.79+345651.7: An EW-type Binary with Emission Line Spectra and Circumstellar Material ›
Generalizing the CPL Parametrization through Dark Sector Interaction ›
On the Relation Between Field-Level Posteriors, Correlators, and their Likelihoods ›
Effects on vsini determinations of O-stars from 3D model atmospheres with large turbulent velocities ›
Microlensing of fast and slow compact objects ›
Rotation Measure Substructures Induced by the Ponderomotive Force of Inertial \alfven Waves ›
Enabling real-time multi-messenger follow-up of transient events with Astro-COLIBRI ›
Compton-thick AGN Characterisation in a Multi-wavelength Context: Insights from the 70-Month \textit{SWIFT}/BAT Catalogue ›
Massive Black holes and their galaxies ›
HyGAL: Characterizing the Galactic ISM with observations of hydrides and other small molecules. III. The absorption lines of [O I], CH, and OH ›
Asteroseismic analysis of RY Leporis: the post-main sequence HADS in a binary system ›
The PHANGS-H{\alpha} survey. Ground-based narrow-band imaging of nearby star-forming galaxies ›
Environmental dependence of the Mass-Metallicity Star Formation Relations at z=4-10 with JWST ›
Intergalactic Magnetic Field constraints from detected very high-energy Gamma-Ray Bursts using the Cherenkov Telescope Array Observatory ›
Euclid: Asteroid rotation periods from the Euclid Ecliptic Survey ›
Impact of segmented deformable mirrors on high-contrast testbeds for exoplanet imaging with future large space telescopes: contrast stability assessment on the HiCAT bench ›
Suppression of Resonant Overstability at Sharp Migration Gradients ›
Characterisation of the Clouds' young stellar Bridge using Gaia DR3 ›
A multifluid approach for polydisperse pebble accretion: From particles to fluids, establishing the multifluid framework ›
Testing template-fitting models for the multipoles of the two-point clustering of galaxy clusters ›
Substructure in redMaPPer clusters and its impact on X-ray morphology and scaling relations ›
Homogeneous Stellar Parameters from Heterogeneous Spectra with Deep Learning ›
Equifinality of Venus-like CO$_2$ Atmospheres ›
Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension ›
Exploring the conditions for forming planetesimals by the streaming instability and planetary systems by pebble accretion ›
Fast radio burst dispersion is an unbiased tracer of matter on large scales ›
From short-lived to long-lived clouds: impact of star formation models on giant molecular cloud evolution in simulations of an NGC 300-like galaxy ›
JOYS+ analyses of OCN$^-$, N$_2$O, NO, and complex cyanides in ices -- Thermal processing results in modest enhancement of OCN$^-$ ice ›
3D Kinetic Simulations of Driven Reconnection in Merging Flux Tubes ›
Joint Estimation of Properties of the Lunar Subsurface and Galactic Foregrounds with LuSEE-Night ›
Peculiar velocities in the $\Lambda$CDM universe ›
Solar Energetic Particle Reflection by Precursor ICMEs: Multi-spacecraft Observations of Bi-Directional Electron Beams at 1 AU ›
A magnetotelluric image of the Curnamona Province and the adjacent Delamerian Orogen margin: new insights into the crustal architecture ›
Gauge Theoretic Signal Processing II: Zero-Latency Whitening for Early Warning Pipelines ›
Towards Seamless Lunar Mosaics: Deep Radiometric Normalization for Cross-Sensor Orbital Imagery Using Chandrayaan-2 TMC Data ›
Simple Analytical Solutions of the Wheeler-DeWitt Equation in the Classical Hamilton-Jacobi Limit ›
Plausible but Wrong: A case study on Agentic Failures in Astrophysical Workflows ›
Polarization-preserving wavefront rotator ›
Collective neutrino-antineutrino pair oscillations ›
$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity ›
The case for super-Eddington accretion in JWST broad-line AGN during the first billion years ›
Distinct Signatures of the Nature of Phase Transition in Binary Neutron Star Mergers ›
The Emergence of Little Red Dots from Binary Massive Black Holes ›
Dimensional reduction for sampled priors and application to photometric redshift distributions ›
Schwinger effect in axion inflation on a lattice ›
R-process heating implementation in hydrodynamic simulations with neural networks ›
Probing the scalar-induced gravitational waves with the Five-hundred-meter Aperture Spherical radio Telescope and the Square Kilometer Array ›
Resolving the Planck-DESI tension by nonminimally coupled quintessence ›
Reionization in Protocluster Environments at $z>7$ with JWST/NIRSpec ›
Spectral Uniformity of Little Red Dots: A Natural Outcome of Coevolving Seed Black Holes and Nascent Starbursts ›
CAZ catalog and optical light curves of 7918 blazar-selected active galactic nuclei ›
Association of the IceCube neutrinos with CAZ blazar light curves ›
SKYSURF-11: A New Zodiacal Light Model Optimized for Optical Wavelengths ›
$H_0$ Without the Sound Horizon (or Supernovae): A 2% Measurement in DESI DR1 ›
Coupling of neutrino beam-driven MHD waves and resonant instabilities in rotating magnetoplasmas with neutrino two-flavor oscillations ›
Diverse Emission Patterns from Precessing Super-Eddington Disks Formed in Tidal Disruption Events ›
Euclid Quick Data Release (Q1). The average far-infrared properties of Euclid-selected star-forming galaxies ›
Study of Flat Spectrum Radio Quasars and BL Lacertae Objects as Sources of Diffusive Ultra High-Energy Cosmic Rays ›
A Novel Parameterization for Rapid Cooling in Supernova Remnants, with applications to the Pa 30 nebula ›
Identification of Candidate Halos Hosting Massive Black Hole Seeds in the $\textit{Renaissance}$ Simulations with Support Vector Machines ›
Stochastic gravitational-wave background search using data from five pulsar timing arrays ›
The NIRISS PASSAGE Spectroscopic Redshift Catalog in COSMOS ›
Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing ›
Unprecedented Multipoint Observation of Spatially Varying ICME Turbulence of Different Ages during October 2024 Extreme Solar Storm at 1 AU ›
Chiral gravitational waves from multi-phase magnetogenesis ›
Willman 1 Revisited: The Kinematics, Chemistry, and Orbital Properties of a Potentially-Disrupting Dwarf Galaxy ›
Single-star optical turbulence profiling techniques for the SHIMM and other Shack-Hartmann instruments ›
An updated model for the Perseus Spiral Arm from Trigonometric Parallax and 3-dimensional kinematic distances of distant massive stars ›
Enhancing Gravitational Lens Study with Deep Learning: A Study on Effects of Dropout Regularization ›
ZTF J021804.16+071152.93: a dead cataclysmic variable and potential solution to the missing period bouncers ›
Asteroseismology of red giants in the globular cluster 47 Tuc using the HST ›
CIV wind properties of the SDSS-V X-ray selected quasars: strong optical-to-UV emission is key regardless of X-ray strength ›
Towards physically more comprehensive AGN modelling in cosmological simulations: A MACER-based modification of IllustrisTNG ›
High efficiency superconducting filterbanks with impedance-defined resolution for millimeter-wave spectroscopy ›
Do little red dots really form a distinct class of astronomical objects? ›
Nonperturbative stochastic inflation in perturbative dynamical background ›
Plate Sensitivity Is Invariant Across Geomagnetic Storm Intensity at Harvard and Palomar: A Protocol for Artifact Control in Historical Plate Archive Studies ›
The trigger and localization system of SVOM-GRM ›
Formalizing Galaxy Population Evolution: Drift and Mergers as Transport Processes on Manifolds ›
Asteroseismic rotation rates of hot subdwarf B stars hint at transient accretion from leftover common envelope matter ›
First Statistical Study of Over 100 Magnified Stellar Events at Redshift $z \approx 0.725$ with JWST ›
It\^o tracers: continuous-trajectory Lagrangian particles for Eulerian hydrodynamics ›
Nonparametric Variational Inference Reconstruction of the Cosmic Expansion History from SNe Ia -- the charm2 code ›
Connecting the dusty dots: dust depletion and extinction of local interstellar clouds ›
Thermodynamics of magnetized BPS baryonic layers and the effects of the Isospin chemical potential ›
Probing Heavy Dark Matter in Red Giants ›
Testing Viability of Benchmark Dark Matter Models for the Galactic Center Excess ›
Multimodal axion emissions from Abelian-Higgs cosmic strings ›
Impact of facility timing and coordination for next-generation gravitational-wave detectors ›
Characterization of field cage and cathode for low radioactivity operation with the CYGNO experiment ›
WIMP Meets ALP: Coherent Freeze-Out of Dark Matter ›
Quantum dynamics of cosmological particle production: interacting quantum field theories with matrix product states ›
A framework for LISA population inference ›
Plotting correlated data ›
Global structure of the time delay likelihood ›
Local Origin of Hidden Symmetry in Rotating Spacetimes ›
The read-out electronics for the FLASH experiment ↓↑