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

Big Dipper over the dome

S Webcam

N Webcam

S Sky
Temperature
16.3 °C
Humidity
70%
Wind
6.4 km/h
Pressure
1012.3 hPa

Moon
Latest preprints on astro-ph:
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PyCBC Live Search for Compact Binary Mergers in Advanced LIGO and Virgo's Fourth Observing Run ›
The X-ray-to-UV relation does not evolve in homogeneous quasar samples ›
The Effects of Cosmic Ray Protons on Galactic Nonthermal Filaments ›
Clumps in a Cocoon: Geometry and Mixing Set the Universal X-ray to H$\alpha$ Surface Brightness Ratio ›
CMBolic: Symbolic emulators for the Cosmic Microwave Background. I. Lensing ›
Euclid Quick Data Release (Q1): The impact of AGN emission on SED-derived physical properties ›
A Colour-colour Fingerprint Links the UV Upturn in Early-type Galaxies to Second-generation Stars from Dissolved Globular Clusters ›
MORFEO wavefront error budget ›
SynIM: a high-performance GPU-accelerated Python library for synthetic interaction and tomographic reconstruction matrices in next-generation adaptive optics ›
Towards Instrument-Agnostic Exoplanet Candidate Prioritization ›
Beyond Point Estimates: Benchmarking Uncertainty Quantification Methods on the AION-1 Astronomical Foundation Model ›
Do Vision-Language Models See Dwarf Galaxies the Way We Do? ›
Extending asteroseismic magnetometry across the diverse landscape of magnetic structures ›
Dynamic Range Beyond Bit Depth of a CMOS Image Sensor Using Interleaved Row Readout ›
Measurements of the Angular Homogeneity Scale from DESI DR1 ›
Faraday Complexity and Depolarisation in a High-Rotation-Measure Radio Galaxy from the Spectra and Polarisation In Cutouts of Extragalactic Sources (SPICE-RACS) DR2 ›
Effective Bayesian ranking of low order monomial potentials in low temperature warm inflation ›
Modern Time-Series and Spectral Methods for Analyzing Solar and Stellar Oscillatory Signals ›
Sunrise III: Instrument, mission, data, and first results ›
Isolated neutron star candidates from the fourth generation XMM-Newton catalogues ›
Detector Development for HUBS I: Initial Testing of Small-Area TES Microcalorimeters ›
XRISM Observations of Abell 1795: Evidence for Low Turbulence and Resonant Scattering ›
Population synthesis of Galactic middle-aged pulsar wind nebulae II. Observational signatures of superefficiency ›
Single-dish observations and non-LTE analysis of CH3OH, HCN, and CO line emission in the Oort cloud comet C/2017 K2 (PANSTARRS) ›
Fast Astronomical Transients in Archival Photographic Plates: Using optical aberrations as a tool for discerning real images, from plate artifacts ›
Old pulsar wind nebulae and the role of the thermal filaments ›
Reconciling large-scale Lyman-$\alpha$ correlations with the SCRIPT Semi-numerical Model ›
Dust to Dust: Prospects for Passive Technosignatures as Relics of ETI ›
$\delta$-CDM: A Minimal Deformation of $\Lambda$CDM with Scalar Field Reconstruction ›
Virial-based extraction of structures in numerical simulations: The vibes tool ›
Photometric light curves analysis of SU UMa-type dwarf novae: the case of RZ LMi and KV Dra ›
Post-Merger Gravitational-Wave Uncertainties of Binary Neutron Stars under Multi-Messenger EOS Constraints ›
Bayesian Reconstruction of the Local Universe from 2MRS: Testing the Gravitational Flow with Cosmicflows-4 ›
Discovery of a Candidate 2 keV Cyclotron Resonance Scattering Feature in the HLX NGC 3583 X-1 ›
ALMA High-resolution Observation of the HH46/47 Outflow/disk/envelope System ›
Thermal emission from dark matter-heated neutron stars in the Galactic Center ›
Reconstructing Synthetic SDO/AIA 193 A EUV Images from He I 10830 A Observations with Diffusion Model Translator ›
On The Nature of Einstein Probe Transient EP250916a: Insights from X-ray, Optical, and Radio Observations ›
Mapping the Landscape of M Dwarf X-ray Flares: New Discoveries in Context ›
From filaments to clumps: filament properties with synthetic Herschel observations ›
JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe ›
A Framework to Model Stellar Irradiated Disks with Frequency-dependent Absorption and Scattering Opacities in Athena++ ›
Disk reflection as the origin of the X-ray polarization of NGC 4151 with IXPE ›
Mock Catalogs of Strongly Lensed Gravitational Waves via a Halo Model Approach with Space-borne Detectors ›
Relativistic Thermal Emission from Accretion Disks in Kerr-MOG Spacetimes ›
Discovery of CO Clouds Associated with the X-ray Jets of SS 433: Evidence for Shock-Cloud Interaction Enhancing Nonthermal X-ray Emission ›
Rapid intermediate-mass black hole formation via runaway mergers of black holes ›
Precise scaling relations for self-interacting bosonic dark matter stars ›
The complex kinematics of the young stars orbiting the supermassive black hole in the Galactic center can be explained by the presence of an intermediate mass companion of Sgr A$^\star$ ›
The origin of WHAM Point Source~46 ›
Parameter Effects in Circumplanetary Disk Spectra and Prospects for Spectral Fitting ›
Statistical Estimation and Correction of Model-Measurement Bias in Time-Dependent Correction Factors of KAGRA ›
CORALIE radial-velocity search for companions around evolved stars (CASCADES) V. Three planetary companions and achievable precision ›
On the Nonlinear Dependence of Underground Muon Rate on Atmospheric Temperature Observed at Daya Bay ›
Ages and ZAMS spin distribution of stars in detached eclipsing binaries ›
Optimising ultra-light dark matter searches with ground-based interferometers ›
Predictability of a solar flare in May 2024 using observational data-driven MHD simulations ›
GRB 250706B/C: Insight-HXMT Discovery of a High-Luminosity Burst as a Candidate for Fallback-Regulated Accretion in the Prompt Emission ›
Bayesian analysis of the shear modulus in the neutron-star crust ›
A consistency check for the calibration of 5303{\AA} solar coronal emission line observations with Aditya-L1/VELC ›
Disentangling chemical evolution histories with phylogenetic trees ›
A Unified Ionization Framework for the Spectroscopic Diversity of Tidal Disruption Events ›
TYC 170-1218-1: A new r-process-enhanced extremely metal-poor star, rich in Th ›
Towards a consistent framework of determining active galactic nucleus contribution fraction and host galaxy properties ›
Fast Radio Bursts produced during collapse of macroscopic X-mode in magnetized pair plasma ›
Class I CH3OH Maser Emission from Bar-Driven Inflow Colliding with the Central Molecular Zone ›
Modifying $\Lambda$CDM dynamics via out-of-equilibrium axions: reconciling SH0ES and DESI $H_0$ values ›
Eccentricity as a probe of mass-transfer physics. Eccentric mass transfer as a solution to the wide eccentric binary problem ›
MRI-triggered instability at the inner dead zone edge: disc evolution and burst modes tied to magnetic field strengths ›
Quantifying isochrone-based age uncertainties for rapidly rotating A-type stars ›
Spectral distortion anisotropies from photon to dark photon conversions ›
Control problem in millimeter-wave adaptive optics ›
Apparent Transverse Motion of Light Bridges Coupled to Coronal Loop Dynamics ›
Characterizing Stellar Streams with Error-Aware Machine Learning ›
A thousand looks at X Persei: X-ray spectroscopy at high time resolution ›
Modelling Galactic neutrino emission: contributions from massive star clusters and interstellar cosmic rays ›
Blowing star formation away in AGN hosts (BAH) -- V: The Feeding-Feedback Cycle in local AGNs as reveled by their stellar populations ›
Measuring the radii of merging neutron stars with asteroseismology ›
Peristaltic Flow in Compressible, Ideal Magnetohydrodynamics: A Mechanism For Solar Spicules ›
Balmer decrements as a new diagnostic for period-bounce Cataclysmic Variable stars ›
A differentiable forward model for weakly perturbed stellar streams: substructure forecasts from density and kinematics spectra ›
Pantheon+ supernovae corrected for progenitor age indicate the universe is decelerating ›
Star Formation Drives Production of Low Energy Cosmic Rays ›
A Meta-Learning Framework for Multitask Reverberation Mapping in Active Galactic Nuclei ›
Stochastic constant-roll inflation beyond the hilltop with the spectral method ›
NEXUS: Abundance, Environments, and Spectral Diversity of Little Red Dots from the NIRSpec MSA Sample ›
A Scaling Relation of LRDs between Broad H$\alpha$ and Bolometric Luminosities: Enhanced Broad H$\alpha$ Emission Relative to Low-$z$ Type 1 AGN ›
Mapping Interstellar Ice Inventory toward Class 0 Protostars in Star-forming Region Orion A with JWST Data ›
Universal Suppression of Gravitational Waves from Black Hole Evaporation Dynamics ›
Inflationary interpretation of the gravitational-wave signal in the European Pulsar Timing Array DR2 with constraints ›
ALMA measurements of mass loss and wind clumping in the massive stars of the Arches cluster ›
Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation ›
Evolution of Coronal Mass Ejection Properties through Superposed Epoch Analysis from 0.2 to 2.2 au ›
On an Airborne Proton Accelerator for Enhancing Cloud Formation or Inducing their Precipitation ›
A Landscape of Cosmological Decoherence ›
NICER Constraints on Low density Interpolation and High density Continuation in Neutron Star Equations of State ›
Core Composition Effects on the QCD Axion Mass Limit from Neutron Star Cooling ›
Hybrid simulations of the proton beam instabilities in the young solar wind. The formation of hammerhead-like distributions ›
Does Eternal Inflation Violate the Smeared Null Energy Condition? ›
A New Route to the Annihilation of Multi-Wall String Topological Configurations ›
Stimulated Emission from Boson Clouds ›
On the effect of higher order symmetry energy corrections in Skyrme models for neutron star matter ›
Fire at the Tip of the Throat: Hagedorn Phase after brane-antibrane inflation? ›
Classifying galaxies in the Galaxy10 DECals dataset using Inception and Residual CNNs ›
Line-of-sight acceleration in compact binaries with higher harmonics and eccentricity ›
A Polarization-Decomposed Method for Simulating Inhomogeneous Birefringence in Laser-Interferometric Gravitational-Wave Detectors ›
Semi-supervised Source Detection in Astronomical Images: New Benchmark and Strong Baseline ›
Detectability to extreme mass ratio inspirals with alternative space-based detector networks ›
Satellite gravity constraints on inner core viscosity and LLVPs density anomalies ›
High-Efficiency Broadband Mid-Infrared Absorption in Asymmetrically Matched Metallic Meanders: Development of Ti40V60 Alloy based LEKIDs for Mid-Far IR ›
Primordial Black Holes from Slow Phase Transitions with Delayed Reheating: A Peak-Theory Approach ›
PTA-Compatible Domain Walls at LISA and Taiji: Bayesian Reconstruction and Multiband Inference ›
A Numerical Experiment on Oscillatory Magnetic Reconnection in a Laboratory Plasma System Driven by Alternating Currents ›
The integral and correlation scales of solar wind turbulence ›
Neutron stars in Poincar\'e gauge gravity with quadratic torsion ›
Linear Ricci-Trace Deformations and Operational Equivalence in Rastall-Type Gravity ›
A stellar dynamical mass measurement of an inactive black hole at redshift 2 ›
To CPL, or not to CPL? What we have not learned about the dark energy equation of state ›
Probing gravity with non-linear clustering in redshift space ›
Gravitational Lenses in UNIONS and Euclid (GLUE) I: A Search for Strong Gravitational Lenses in UNIONS with Subaru, CFHT, and Pan-STARRS Data ›
Robustness of pairwise kinematic Sunyaev-Zel'dovich effect to optical-cluster-selection bias ›
The 2MIG isolated AGNs -- 2. X-ray general properties and peculiarities ›
Non-Gaussian Expansion of Minkowski Tensors in Redshift Space ›
X-ray polarization of reflected thermal emission ›
Spatially resolved gas-phase metallicity at z~2-3 with JWST/NIRISS ›
Dark Matter and the Early Formation of Supermassive Black Holes ›
Les Houches on Dark Universe 2025: Elements of cosmology beyond FLRW ›
Probing initial isocurvature perturbation with 21cm one-point statistics ›
Aligned hierarchical black hole mergers in active-galactic-nuclei disks revealed by GWTC-4 ›
The Colors of Ices: Measuring ice column density through photometry ›
Resolving Star Cluster Formation in Galaxy Simulations with Cosmic Ray Feedback ›
The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- I. A golden thread through time and space ›
The chemodynamical memory of a major merger in a NIHAO-UHD Milky Way analogue -- II. Were Splash stars heated or already born hot? ›
Positive AGN Feedback Enhances Star Formation in Starburst Dwarf Galaxies ›
CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA ›
Searching for Electromagnetic Counterpart Candidates to GW231123 ›
Detection of Multiband Lensed Gravitational Waves from Dark Matter Halos with Deep Learning ›
Ultra-extreme high-frequency-peaked BL Lacs: A potential population of MeV synchrotron blazars ›
Where Galaxies Point: First Measurement of the Large-Scale Axial Intrinsic Alignment ›
Impact of Cosmic Ray Distribution on the Growth and Saturation of Bell Instability ›
Wavelet-Scattering Signatures of Fuzzy Dark Matter in Simulated 21 cm Brightness-Temperature Maps ›
NICER Perspective on TeV Blazar Mrk~421: X-ray Variability and Particle Acceleration ›
National Mapping and Testing of Astronomical Sites in Ethiopia (NMTASE) ›
Bayesian Smooth-Fit Extrapolation of the $^{12}\mathrm{C}+{}^{12}\mathrm{C}$ Astrophysical $S$ Factor ›
The rotation-magnetism relationship in solar-type stars. Constraining magnetic flux emergence rates ›
Parity-odd Four-Point Correlation Function from DESI Data Release 1 Luminous Red Galaxy Sample ›
Assessing systematic uncertainties from spectral re-analysis of Cyg X-1 with different coronal geometries ›
Widespread Extended [CII] Emission in High-Redshift Galaxies: Insights from the FIRE-2 Cosmological Zoom-in Simulations ›
Quintom Dark Energy: Future Attractor and Phantom Crossing in Light of DESI DR2 Observation ›
MeV absorption in gamma-ray bursts as a probe of their progenitor environments ›
Fast, dust-poor outflows in the local candidate dual AGN MCG-03-34-64 observed with VLT/ERIS ›
Dynamical Systematics for Time Delay Lenses and the Impact on the Hubble Constant ›
A simple mechanism for the enhancement of the inflationary power spectrum ›
Cosmo3DFlow: Wavelet Flow Matching for Spatial-to-Spectral Compression in Reconstructing the Early Universe ›
Cosmological Simulation with Population III Stellar Feedback and Metal Enrichment I: Model Description And Convergence Test ›
The spectral state transition of Mkn 590, a potential link between AGNs and X-ray binaries? ›
ATLAS100 -- I. A volume-limited sample of supernovae and related transients within 100 Mpc ›
Neutrino mass limits and decaying dark matter: background evolution versus perturbations ›
Probing the Dispersion and Rotation Measure Contributions from Supernova Remnants in Fast Radio Burst Source Environments with 1D SNR Simulation ›
The In Situ Growth of Stellar-mass "Light" Seed Black Holes in Nuclear Star Clusters ›
Sensitivity to Axion-like Particle dark matter with very-high-energy gamma-ray observations of Active Galactic Nuclei located behind Galaxy Clusters ›
Bayesian analysis of $\alpha$-Starobinsky model with Planck, ACT and DESI data ›
Data-driven discovery of dynamo cycle equations ›
Learning What's Real: Disentangling Signal and Measurement Artifacts in Multi-Sensor Data, with Applications to Astrophysics ›
A Salpeter-like filament linear density function across nearby molecular clouds ›
Constraining Quintessential Inflation with ACT: A Gauss-Bonnet Gateway ›
Stellar nucleosynthesis in the era of large surveys: s-process polluted binaries in GALAH DR4 ›
Forecasts of CMB $E$-mode anomalies for AliCPT-1 ›
Diversity in Evolutionary Status and Magnetic Activity among Solar-Type Twin Detached Eclipsing Binaries ›
Strong Gravitational Lensing with the James Webb Space Telescope ›
From inter-filamentary gas to filaments and hubs: gas flows in the Mon R2 hub-filament system ›
Solar Vortices: Catalysts of Magnetoacoustic Wave Dissipation and Atmospheric Heating ›
The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars ›
Cosmological constraints from neighbor-density-weighted marked correlation functions ›
Imaging spectroscopy reveals spike-like repeating radio burst pairs in the solar corona ›
The Persistent Missing Mass Problem in Planet Formation ›
From Images to Orbits: A Hubble 2030s Astrometric Legacy for the M31-M33 Star Cluster Systems ›
Choosing the right MCMC sampler: a systematic benchmark of gradient-free methods ›
Eigenvalue formulation of Stochastic Inflation and application to large perturbation generating inflationary features ›
Some Thoughts on the Future of Technosignature Searches: Constraining the Fermi Paradox ›
One Transit Is All You Need: Detecting Exoplanets Through Learned Stellar Behaviour with EXOVEIL ›
Possible explanation of primordial $^7$Li deficit ›
A Model Selection Criterion for Multidimensional Gaussian Processes: Application to Radial Velocities ›
Joint Multi-Period Fermi-LAT and LHAASO Constraints on Axion-Like Particles from Mrk 421 Using Profile Likelihood with Gaussian Copula Correlation ›
Mass-Orbital Period Distribution of Massive White Dwarfs Formed Through Stable Mass Transfer ›
EPISODE II: Variability in the CO and H$_2$O rovibrational absorption lines in a periodically variable protostar EC 53 ›
Angular momentum evolution in the CIELO simulations. I. Temporal evolution of gas-stellar misalignments and baryonic merger timing ›
The Universe Observed with Particle Detectors: Astrophysical Legacy of Guido Barbiellini Amidei ›
Phenomenology of bubble size distributions in a first-order phase transition ›
Bayesian Deep Gaussian Processes for Correlated Functional Data: A Case Study in Cosmological Matter Power Spectra ›
Influence of Rotation on Fingering Convection in Planetary Cores ›
Prospects for Neutrino Observation and Mass Measurement from Binary Neutron Star Mergers ›
Revisited apparent horizon entropy and GSL in modified gravity ›
Dark Dimension Right-handed Neutrinos Confronted with Long-Baseline Oscillation Experiments ›
Sterile Neutrino Dark Matter as a Probe of Inflationary Reheating ›
DC response of an interferometer topology with an L-shaped cavity: a tabletop study ›
High-bandwidth frequency domain multiplexed readout of transition-edge sensors for neutrinoless double beta decay searches ›
UV-complete and stable Quintom Dark Energy models in the light of DESI DR2 ›
Big Bang revisited ›
X-ray Response of the Fully-Depleted, p-Channel SiSeRO-CCD ›
Energy-momentum and dark energy in $\boldsymbol{SU(\infty)}$-QGR quantum gravity ›
Irreducible Gravitational Wave Background as a Particle Detector ›
Rotation-Induced Effective Anisotropy in White Dwarfs as a Newtonian Benchmark with Relativistic Scale Assessment ↓↑