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

In the dome

S Webcam

N Webcam

S Sky
Temperature
16.3 °C
Humidity
69%
Wind
0.0 km/h
Pressure
1018.3 hPa

Moon
Latest preprints on astro-ph:
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Astrophysics in the Era of Artificial Intelligence powered by Large Language Models ›
An X-ray Data Primer: What I Wish I Knew When Starting X-ray Astronomy ›
The Loud Tail of the Supermassive Black Hole Binary Population: Multimessenger Candidates and Prospects for SKAO ›
Complete Second-Order Relativistic Derivation of the Observed Pulsar Timing Modulations ›
Reigniting the FUSE II: O VI Emission in Massive Elliptical Galaxies ›
Diffraction of gravitational waves by extended dark objects ›
Spinning Between Models: Continuum and Reflection Constraints in the Intermediate States of GRS 1716-249 and GRS 1739-278 ›
Chemo-dynamical Analysis of a CNO-Enhanced Ultra Metal-poor Star ($\rm[Fe/H] < -4$): Insights into Early Enrichment by Faint Population III Supernova ›
The GMRT CAT$z$1-COSMOS Survey: HI 21 cm emission from star-forming galaxies at $z\approx1$ in the COSMOS field ›
Classical Cases of Non-solar Mixing Length in Low Mass Stars ›
Gas absorption of soft X-rays strongly impacts the redshift distribution of dark Fast X-ray Transients ›
Mapping parameters of idealised hydrodynamic galaxy simulations to bar properties: a case study with the RAMSES code ›
The core-mantle mode of gravitational oscillation ›
Sinking Silicates I: Characterizing the benchmark system containing the T0 brown dwarf CWISE J210640.16+250729.0 using JWST ›
Host Galaxy UV Emission and Dust Reddening in Little Red Dots ›
SDSS-IV MaStar: Determination of Stellar Parameters Using Bayesian Averaging ›
Photonic Integrated Circuits for the Habitable Worlds Observatory: Science Drivers, Material Platforms, Arrayed-Waveguide Spectrographs, and a Space-Qualification Roadmap ›
Supernova Cousins: The Intrinsic Dispersion and Environmental Dependence of Type Ia Supernovae in Galaxy Groups with TITAN ›
Incompatibility of iron in post-perovskite and the stability of basal magma oceans in super-Earths ›
Observable Signatures of Supernova Shock Breakout in Confined Circumstellar Medium ›
Sensing ELT petal modes with a discrete beam combiner: an end-to-end theoretical model ›
CHEX-MATE: X-ray surface brightness discontinuities across a representative cluster sample ›
A Two-Stage Physically Grounded Optical Design Framework with Application to a Multi-Channel Focal Reducer ›
Examining Temporal Characteristics of GCRs in the AMS-02 era ›
Consistency and precision of very long baseline interferometry source coordinate time series ›
Multi-Instrument Analysis of NOAA AR 12781: Coupling Surface Evolution of the AR with Its In-Situ Solar Wind Signatures ›
Consistent treatment of flavour-specific neutrino self-interactions in cosmology ›
Investigating r-Process Diversity in Mildly Metal-Poor Stars Using the Th II 5989 Angstrom Line ›
Investigating Variability in Long-lived Protoplanetary Disks (>10 Myr) using NEOWISE ›
Measuring the spatio-temporal variation of fundamental physical constants using the OH sum rules ›
Recovering turbulent velocity statistics from noisy integral-field spectroscopy ›
The New Dark Matter Density Profile from JWST JADES Galaxies ›
A comprehensive assessment of weak-lensing inferred circular velocity profiles of isolated galaxies ›
A compact time-domain reduced order quadrature for gravitational wave inspirals with non-stationary noise ›
Reconstruction of pretelescopic and early telescopic solar activity cycles from auroral records ›
The Galactic Black Hole mass distribution ›
The LGRBs Redshift and Jet Opening Angle Distributions and the Hubble Constant $H_0$ ›
Exploring the dynamics of the Coma galaxy cluster by mapping its X-ray emission line profiles with XRISM ›
Supersonic flows observed by THEMIS related to a coronal bright point and filament ›
Decoding RR Lyrae light curves with deep learning for accurate absolute magnitude estimation ›
Thermodynamic exchange and mode stability in strongly nonadiabatic radial pulsations ›
Presence of Solar Neutral Atom Corona and Coronal Heating ›
High-energy spectral cutoffs in the prompt emission of Fermi gamma-ray bursts: bulk Lorentz factors, emission radii, and a cutoff-peak energy relation ›
Evolution of the High-Energy Excess in Swift J1727.8-1613 during Its 2023 Flare State ›
Nitrogen-Loud Quasars from the Dark Energy Spectroscopic Instrument. II. Broad-Line Region Metallicity and Relative Nitrogen Enrichment ›
The Connection between Halo Assembly History and the Stellar Distribution I: The Central Stellar Mass - Richness Plane ›
NICER neutron stars with dark energy and dark matter: effects on the inferred equation of state ›
First Light of Neutron Star Mergers: Off-axis Cocoon Cooling X-ray Emission from Short Gamma-Ray Burst Jets ›
Stripped helium stars in UV ›
Euclid: Data Release 1 (DR1) -- Fornax-7, an ultra-faint companion to the Fornax dwarf spheroidal galaxy? A remote star cluster or dwarf satellite of the Fornax dSph ›
First results on the search for the Galactic Center Excess in the sub-GeV band with the emulsion telescope in GRAINE 2023 ›
PRISMS. GHZ1. A standard tale of galaxy evolution with atypical ionizing conditions at $z=9.878$ ›
Bayesian Inference of the Tip of the Red Giant Branch: I. One-Dimensional Analysis ›
WINERED Detects a Strong Atmospheric Outflow on the Sub-Neptune GJ 3090b ›
Second Generation Planet Formation in Post-AGB Discs - II: Dust Coagulation and Core Accretion ›
Field-Level Baryon Acoustic Oscillation Reconstruction of the DESI DR1 Luminous Red Galaxies with Linear Field Transformer (LiFT) ›
Tracing Stellar Populations through the Mg-Al Anti-Correlation in Gaia-ESO Globular Clusters ›
Measurement of Cosmic-Ray Density in the Spiral Arms toward Galactic Anticenter ›
Forecasting Coupled Dark Energy Parameters with the One-Loop Galaxy Power Spectrum ›
Optical spectroscopy of the VHE flat-spectrum radio quasar PKS 0903-57 ›
Nexus-CDM: Isolated Galaxy Simulations with Cosmologically Evolving Dark-Matter Halos I. Method and Validation ›
The driving mode of turbulence in disc galaxy simulations with adaptive mesh refinement ›
Hardware-aware quantum attention for fast radio burst identification ›
Nii-MALA: A Fast Metropolis-Adjusted Langevin Sampler with Radial Velocity Benchmarks ›
A comparative analysis of the long-term optical variability characteristics of narrow and broad-line Seyfert 1 galaxies at z > 0.8 ›
Spectral Evolution of Ceres' Surface and Implications for Space Weathering ›
FOSSIL: Thermo-mechanical architecture ›
Riemann Map Operator for Solar Front Diagnostics ›
Results on young stellar clusters with the WEAVE LIFU ›
Physics-Informed Neural Networks and Data-Driven Models for GRB X-ray Light-Curve Gap Reconstruction ›
Discovery of Two Consecutive Profile Change Events in the Millisecond Pulsar PSR J0437-4715 ›
A new method to cleanly separate hot and cool populations using just Gaia and 2MASS photometry ›
The WISSH quasars project XIII. A multi-epoch study of ultra-fast broad absorption line outflows at cosmic noon ›
A Self-consistent Model for the Generation of Coronal Condensations: The Effects of Turbulent Wave Dissipation ›
Highly Ionized Oxygen in the Circumgalactic Medium of TNG100 Galaxies: Distributions, Thermal States, and Ionization Mechanisms ›
Spectro-polarimetric study of the black hole X-ray binary Swift J1727.8-1613 in the JED-SAD framework ›
SPAMMS: 3D spectroscopic modelling of stellar surfaces. II. Implementation of Kurucz and TLUSTY model atmospheres ›
PYRA and MYTHRA: new statistical analysis for image reconstruction ›
Assembly Bias in eRASS1 X-ray Galaxy Clusters: Accounting for Non-uniform Survey Exposure ›
2+1 is not 3: Angular bispectrum and Super-Sample Covariance on the light cone ›
MINCE IV. A detailed analysis of 37 metal-poor and subsolar metallicity stars ›
The effect of pressure confinement on the maximum mass of rapidly accreting supermassive stars ›
Influence of the large-scale structure velocity field on halo mass assembly within cosmic filaments ›
Gravitational-Wave Image Multiplicity as a Topological Probe of Dark-Matter Core Collapse ›
Detecting transiting exoplanets in simulated PLATO data: A comparison of light curve filter and transit search algorithms ›
Gnuastro: removing extended/diffuse outliers while coadding ›
ALMA-JELLY II. Constraining the radial profiles of the quenching timescales in ram-pressure-stripped galaxies ›
Anisotropic redshift distributions in photometric galaxy clustering and their cosmological impact ›
The Multiphase CGM in the Epoch of Reionization: CII and CIV absorbers around [OIII] Emitters ›
Calibrations for high precision differential astrometry onboard Theia and HWO ›
Constraining the Delay Time Distribution of the r- and s-Process from Stellar Ages at Solar Metallicity ›
Stellar activity in a post-merger Giant star ›
Compelling evidence of a link between the lags of the quasi-periodic oscillations and the radio jet in the black-hole X-ray binary GRS 1915+105 ›
Iron Nuclei with Energy of 10^19 eV in Extragalactic Cosmic Rays Near Earth ›
Automatic astrometric calibration of low-cost all-sky cameras ›
Using the Circumgalactic Medium of Dwarf Galaxies as a Calorimetric Dark Matter Detector ›
Toward Precision Kinetic Sunyaev-Zel'dovich Cosmology---1. The Matter - Momentum Bispectrum at One-Loop Order ›
Thermophysical characterization of the potentially hazardous near-Earth object 2024 YR4 ›
Modeling Gamma-Ray Bursts Using CRISP ›
Multi-chromatic observations of classical Cepheids using the CHARA Array interferometer: Surface brightness-colour relation, projection factor, and limb-darkening ›
Cosmological Signatures of Curvature-Coupled Dark Energy ›
Rubin Observatory Reveals a Dust-Shrouded Halo Globular Cluster in Ophiuchus ›
Impact of uncertainties on the cosmic optical and infrared backgrounds on the propagation of astroparticles ›
Ce II-IV emission in kilonovae with R-matrix collision strengths and distorted wave recombination rates ›
The JWST Proto-PAH Project: Detection of the methyl radical CH$_{3}$ in the highly evolved C-rich object SMP LMC 011 ›
Common Excitation Patterns of Star Formation, Active Galactic Nuclei, and Shocks in Seyfert Galaxies ›
Disentangling 3D Magnetic Field Geometry from Turbulence: A Polarization-Based Classification Method ›
NERV: Neural-network Enhanced Reconstruction of the UniVerse with Application to Baryon Acoustic Oscillations in the BOSS DR12 Galaxy Sample ›
MUSHY: Multimodal Flow-Based Amortized Bayesian Inference for Spectroscopic Data Fusion ›
Validating Inverse Fundamental-Plane IMBH Mass Estimates in the SKA/ngVLA Era ›
Can Isotropic Thermal Conduction Heat One of the Hottest Cool Cores? ›
A Standard Ultraviolet Continuum Can Hide Supercritical Accretion in GN-z11 ›
Constraining quantum-gravity predictions for evolving dark energy ›
Less isn't more: Cosmological bounds on the neutrino masses are robust to changes in the neutrino abundance ›
Elveslocation: A new approach for studying thunderstorm atmosphere ›
Opacity predictions in plasmas under stellar conditions using deep learning ›
Black Holes, Gravitational Waves and Space-Time Singularities Lemaitre Conference 2024 ›
Survey of Novel Deep Learning Architectures for Denoising Gravitational-wave Signals ›
Scale analysis for the Madden$-$Julian oscillation ›
Operational Range Bounding in Spectroscopy: A Safety Cage Framework for Machine Learning Models ›
Direct detection of right-handed fermionic dark matter: electron-recoil measurements in Xe atoms ›
A Unified Numerical Study of Axion Stars: From the Nonrelativistic Regime to General Relativity ›
Frequency shift in gravitational lensing by Kerr metric ›
The optimal-transport cartogram: world population as a Brenier map ›
Quantum black hole ringdown ›
Simulation of PBH formation in a matter-dominated universe ›
Parameter Estimation of Ringdown Quasinormal Modes with Autoencoder ›
From CMB to LHC: A hybrid inflation model with gauged scale symmetry ›
Convex Pursuit-Evasion Games for Spacecraft Proximity Operations on Circular and Elliptical Orbits ›
Probe of Solar Neutrino Magnetic Moments through Spin-Flavor Precession: Resonance Structure and Antineutrino Appearance ›
Full set of scenarios of high energy collision in the Schwarzschild background and kinematic censorship ›
Stability and Structural Properties of Hot Quark Stars within Perturbative QCD ›
Boosted or Inelastic? Discriminating Interpretations of the LZ 248 keV Event ›
Inelastic Dark Matter at LZ from Radiative Dirac Neutrino Mass Paradigm ›
Did LZ see modified gravity? ›
Testing the equivalence principle with lunar laser ranging residuals from different planetary and lunar ephemerides ›
Deterministic denoising of long-duration gravitational-wave signal candidates with $\alpha$-(de)blending ›
Self-field of a moving string ›
Magnetic Reconnection Heating of Thin Accretion Disks around Kerr Black Holes ›
Setup and performance of focal-plane characterization benches for high precision astrometry ›
Hadrophilic inelastic freeze-in dark matter in $q_1-q_2$ gauge extension and the high energy LZ event ›
Analysis of GWTC-3 with multiple quasicircular models ›
Neutron Skin Effects on Particle Emission in Heavy-Ion Collisions: A Topic Review with Astrophysical and Nuclear Structure Connections ›
Distinguishing cosmology, astrophysics and systematics: the Bayesian search for a primordial gravitational-wave background in next-generation observatories ›
Generative Learner for Distributional Causal Effects ›
Exploration of groups and outliers in Gaia RVS stellar spectra with metric learning ›
Stochasticity in Stellar Yields Reflected in Supernova Dust Masses Across All Massive-Star Progenitors ›
Search for Quintessence-Like Pseudoscalar Dark Energy Effects on $^{56}\text{Fe}$ Nuclear Transition Energies in Supernova 1991T ›
Impact of Large-Scale Structure along Line-of-Sight on Time-Delay Cosmography ›
Constraints on the Thomson optical depth to the CMB from the Lyman-$\alpha$ forest ›
ExTraSS: a Domain Decomposed 3D NLTE Radiative Transfer spectral synthesis code for nebular phase transients ›
Constraints on the canonical single-field slow-roll inflation model from observations ›
Tracing the Cosmic Evolution of the Cool Circumgalactic Medium of Luminous Red Galaxies with DESI Year 1 Data ›
3D Radiative MHD Modeling of Particle Beam Heating of the Solar Atmosphere ›
Late-Time Alleviation of the Hubble Tension in CPL Cosmology with Massive Neutrinos via Bayesian Physics-Informed Neural Networks ›
Reconstructing Gamma Ray Burst Energy Relations with Observational H(z) data in Neural Network Framework ›
Note on pulsar timing array correlation functions induced by peculiar velocities ›
Lightcurve Modelling of 2,205 ZTF DR2 Type~Ia Supernovae: Implications for SN Ia Physics and Cosmology ›
Improved Heavy Dark Matter Annihilation Search from Dwarf Galaxies with HAWC ›
Non-minimally Coupled Running Curvaton for DESI-motivated Dynamical Dark Energy ›
Observations of Binary Stars with the 1.3-m Devasthal Fast Optical Telescope Using Speckle Interferometry: An Attempt ›
Modeling Globular Cluster Stellar Streams with a Basis-Expansion N-body Code ›
Survival of ultraheavy nuclei in astrophysical sources: applications to protomagnetar outflows ›
Searching for Black Hole Candidates in Quiescence by Using Multi-band Observations in Globular Cluster M22 (NGC 6656) ›
TDCOSMO XXV: A "soup-to-nuts" 6.5% $H_0$ measurement -- strong lensing and dynamics with a maximally flexible mass sheet ›
Estimating galactic foreground with the population of resolved galactic binaries ›
The Deep Newtonian Regime in Late-Time Blast Waves: Inevitable Transition and Distinct Flux Signatures ›
On the Relation Between Field-Level Posteriors, Correlators, and their Likelihoods ›
J1248+4826: A diffuse radio source consistent with re-energized fossil plasma in a galaxy group ›
Gas Phase Distribution in the Neutral ISM: A Comparison between Observation and Numerical Simulation ›
From mass-loss histories to lightcurves: a generalised framework for interaction-powered transients ›
X-ray Polarization Signatures from Comptonization by Magnetic Reconnection Plasmoids ›
Agentic AI for Gravitational Wave Data Analysis: A Head-to-Head Comparison of Coding Agents Executing a Matched Filter Pipeline on Einstein Telescope Simulated Data ›
Tidal Disruption of Blanets by Supermassive Black Holes: From Test Particles to Planetary-Mass Bodies in Kerr Spacetime ›
Fast Astronomical Transients in Archival Photographic Plates: Using optical aberrations as a tool for discerning real images, from plate artifacts ›
Spatially Resolved Nebular-Stellar Reddening with JWST/NIRISS ›
The nature of `little blue dots' ›
Little Red Dots as Supermassive Counterparts of SS 433: A Hyper-Eddington Accretion Framework ›
When the black holes align: a subpopulation of aligned massive binary black holes observed via gravitational waves ›
Signatures of $^{56}$Ni Mixing and Neutron-rich Ejecta in Supernovae ›
A First Measurement of Circumgalactic Dust Reddening from Only 4.6 deg$^2$ of the Rubin Observatory's Data Preview 1 ›
Time-Domain Synthesis of Gravitational-Wave Detector Glitches using Class-Conditional Derivative Generative Adversarial Networks ›
Energy-Resolved Limits on Orbital X-ray Polarization Modulation in Cygnus X-1 ›
Chemical evolution of the Milky Way disc with radial gas flows: a Lagrangian approach ›
SGN: A python framework for stream-processing pipelines ›
Multi-messenger View of White Dwarf Tidal Disruption Events by Intermediate-Mass Black Holes: I. Gravitational Waves and Disk Photon and Neutrino Emissions ›
Effects of Rotation on 3D Core-Collapse Supernova Models for Low-Mass Progenitors ›
Early Near-Infrared Excess and Rapid Disk-Corona Evolution in the Tidal Disruption Event 2024aepd ›
Galactic constraints on spinning primordial black hole dark matter from interstellar dust heating ›
The extended globular cluster system of the archetypal "failed galaxy" Dragonfly-44 from deep white-light Hubble Space Telescope imaging ›
Optical Images of the Braneworld Black Hole Surrounded by an Optically Thin Accretion Disk ›
HST imaging, pipeline modeling, and time-delay predictions of 2 triply-imaged and 15 quadruply-imaged lensed quasars ›
The Rotation Curve of the Milky Way: State of the Art, the Keplerian Decline Debate, and Implications for Dark Matter ›
Exploring the long-term temporal variability in polarization through multi-epoch optical spectro-polarimetry - Part II: A sample of symbiotic and red-giant stars ›
An ALMA view of the Jet-Arc CO clouds toward the TeV $\gamma$-ray source HESS J1023-575 and Westerlund 2; Evidence for the footprints of microquasar jets, the very powerful cosmic-ray accelerator in the Galactic disk ›
Spectral Fingerprints Beyond Degeneracies in Primordial Gravitational-Wave Sources ›
Preparing for the Early eVolution Explorer: Photometric Diagnostics of Magnetospheric Accretion Geometry in Young Stellar Objects ›
Portraits of the young and old in X-ray: New millisecond pulsar detections and updated characterization of young neutron stars ›
Quantifying Sky Map Resolution Requirements for Beam Chromaticity Correction in Sky-Averaged 21 cm Experiments ›
GRINTA: a new Probe of the Dynamic Universe ›
Dispersion Measure Variability in Fast Radio Bursts from Photoionization ›
Connecting Dynamo Theory with DNS Data: A Computational Analysis of $\alpha$ and $\beta$ Effects ›
High water D/H ratio of the interstellar object 3I/ATLAS is consistent with a low-metallicity origin ›
DESI DR2 Constraints on Coupled Hu--Sawicki $f(R)$ Gravity with Interacting Neutrinos: Implications for the Hubble and \(S_8\) Tensions ›
Local relaxation and scale-dependent alignment in compressible, magnetized turbulence ›
Cosmic Overture Echoed in a Stellar Final Act: Implications of Nanohertz Gravitational Waves for Core Collapse Supernova Neutrinos ›
Cosmological Limits on Strong Dark Forces ›
Bayesian approach study of hybrid neutron stars ›
Circumstellar Medium of Supernovae as New Probes for Feebly Interacting Particles ›
Nonlinear tails in the Kerr black hole ringdown ›
No evidence of vorticity production from irrotational turbulent gravitational collapse yet ›
Probing Nonlinear Logarithmic Kalb-Ramond Black Holes: Particle Dynamics, Epicyclic Oscillations and Thermodynamic Signatures ›
Inelastic dark matter and baryon flavor symmetry in light of LUX-ZEPLIN (LZ) experiment ↓↑