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
-1.0 °C
Humidity
80%
Wind
0.0 km/h
Pressure
1002.2 hPa

Moon
Latest preprints on astro-ph:
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OmniSpectra: A Unified Foundation Model for Native Resolution Astronomical Spectra ›
LISA and the LISA Science Team ›
Non-uniform Antenna Loading Effect on Embedded Element Patterns and Application to Fault Detection ›
Digging into the Interior of Hot Cores with ALMA (DIHCA). VII. Disk candidates around high-mass stars and evidence of anisotropic infall ›
Hierarchical bayesian inference: constraining population distribution of dark matter halo shapes via stellar streams ›
What factors shape the radio luminosity of star-forming galaxies? A new calibration from LoTSS-DR2 ›
The Back-in-time Void Finder: dynamical identification of cosmic voids through optimal transport reconstruction ›
Optimizing Optical Searches for Supermassive Black Hole Binaries in AGN Light Curves: Fourier versus Bayesian Periodicity Detection ›
Blazars define a stable celestial reference frame ›
A Stratification in Magnetic Field Structures: The Radio Outflow in NGC 4151 ›
An Investigation of 5-year Simultaneous X-ray and Radio Light Curves of the Dwarf Seyfert Galaxy UGC 6728 ›
An Analysis of AGN Feedback in the Compact Galaxy Group Stephan's Quintet ›
Solar twins in Gaia DR3 GSP-Spec I. Building a large catalog of Solar twins with ages ›
Dynamic shocks powered by a wide, relativistic, super-Eddington outflow launched by an accreting neutron star in the mid-20th century ›
The age sequence of young clusters in Perseus: Estimating ages from mass distributions ›
Spin-down changes in PSR B0540-69 induced by a drift of the magnetic axis ›
Supernova interactions with aspherical circumstellar material I: calculations of light curves, AB magnitudes, spectra, and polarisation ›
The role of gas stripping in the quenching of satellite galaxies using SHARK v2.0 ›
Perihelion Asymmetry in the Water Production Rate of the Interstellar Object 3I/ATLAS ›
The long quest for vacuum birefringence in magnetars: 1E 1547.0-5408 and the elusive smoking gun ›
Constraining nonminimal f(T) gravity from Primordial Nucleosynthesis to Late-Universe observations ›
Two Fluid Quantum Bouncing Cosmology I: Theoretical Model ›
Source identification for the Swift-BAT 150-month hard X-ray catalog using soft X-ray observations ›
Mapping dark matter and the emergence of large-scale structure ›
Multi-band Reconstruction of Sixteen Gravitational Lens Systems using PISCO data ›
A compact object with a K type star companion in the solar neighborhood: a wide post common envelope binary with a white dwarf candidate ›
The initial spin matters: the impact of rapid rotation on magnetic-field amplification at merger ›
K-DRIFT Science Theme: Galactic Cirrus Clouds and Circumgalactic Medium ›
The reason for the occurrence of W-type contact binaries ›
Development of an early warning method incorporating pre-supernova neutrino light curves ›
Evidence for stellar contamination and water absorption in NGTS-5b's transmission spectra with GTC/OSIRIS ›
Hydrodynamic simulations of the recurrent nova T Coronae Borealis: Nucleosynthesis predictions ›
Fuzzy dark matter soliton core hosting a supermassive black hole as a dense low-mass perturber in strong gravitational lensing ›
Interaction between the ejecta, the accretion disk, and the secondary star in the recurrent nova system U Sco ›
GRB~250704B/EP250704a a Short Gamma-Ray Burst Powered by a Magnetar ›
Nucleosynthesis in Type Ia Supernovae, Classical Novae, and Type I X-Ray Bursts. A Primer on Stellar Explosions ›
Redshift-Binned Constraints on the Hubble Constant under $\Lambda$CDM, CPL, and Pad\'e Cosmography ›
Deuteration of HC3N and CH3CCH in the pre-stellar core L1544 ›
Distance-Independent Atmospheric Refraction Correction for Accurate Retrieval of Fireball Trajectories ›
Failed ejection and oscillations of a current-carrying filament balanced by gravity ›
Radio-Interferometric Image Reconstruction with Denoising Diffusion Restoration Models ›
Intrinsic alignments in the FLAMINGO simulations with two-point statistics ›
Does the solar oxygen abundance change over the solar cycle? An investigation into activity-induced variations of the O I infrared triplet ›
Out-of-Sample Validation of MagNet ›
Hot and cloudy: High temperature clouds in super-Earths and sub-Neptunes ›
Enhancing Thermal Sunyaev-Zel'dovich Analyses with Digital Twins of the Local Universe ›
A 2 au resolution view by ALMA of the planet-hosting WISPIT 2 disk ›
JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: NIRCam Imaging in GOODS-S and GOODS-N ›
JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: MIRI Coordinated Parallels in GOODS-S and GOODS-N ›
JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Photometric Catalog ›
JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Catalogs of inferred morphological properties of galaxies from JWST/NIRCam imaging in GOODS-N and GOODS-S ›
JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Wisp Subtraction with the Non-negative Matrix Factorization Algorithm ›
JWST Advanced Deep Extragalactic Survey (JADES) Data Release 5: Photometrically Selected Galaxy Candidates at z > 8 ›
JADES: A Prominent Galaxy Overdensity Candidate within the First 500 Myr ›
JADES: Discovery of Large Reservoirs of Small Dust Grains in the Circumgalactic Medium of Massive Galaxies at $z\sim3.5$ through Deep JWST/NIRCam Imaging and Grism Spectroscopy ›
Undermassive Hosts of $z = 4-6 $ AGN from JWST/NIRCam Image Decomposition with CONGRESS, FRESCO, and JADES ›
There Is More to Outshining: 2D Dust Effects on Stellar Mass Estimates at $3 \leq z < 9$ with JWST in the JADES Field ›
JADES: Evolution of nitrogen abundances in star-forming galaxies from z ~ 1.5-7 ›
Clump-like Structures in High-Redshift Galaxies: Mass Scaling and Radial Trends from JADES ›
Gaia20fnr: A binary-lens microlensing event with full orbital motion revealed by four space telescopes ›
HE0144-4657: A Carbon-Enhanced Ultra Metal-Poor Star ([Fe/H] ~ -4.1) from the Helmi Stream Disrupted Dwarf Galaxy ›
Extreme line profile variations in the repeating changing-look active galactic nucleus IRAS23226-3843 ›
A multi-wavelength approach of AGN feedback in LINERs: The case of NGC 4438 ›
SVOM discovery of a strong X-ray outburst of the blazar 1ES~1959+650 and multi-wavelength follow-up with the Neil Gehrels Swift observatory ›
Spatially resolved stellar-to-total dynamical mass relation: Radial variations, gradients and profiles of galaxy stellar populations ›
Modeling the Impact of Unresolved Stellar Companions on Detection Sensitivity in Kepler's Small Planet Occurrence Rates ›
Unveiling the Spectral Morphological Division of Fast Radio Bursts with CHIME/FRB Catalog 2 ›
Constraining Nuclear Molecular Gas Content with High-resolution CO Imaging of GOALS Galaxies ›
Formation and X-ray emission from hot bubbles in planetary nebulae - III. The impact of [Wolf-Rayet]-type winds ›
Cis--Trans Rotational Isomerism of Seleno-, Thio-, and Formic Acids and Their Dimers: Chemical Kinetics under Interstellar Conditions ›
Magnetar fraction in Core-Collapse Supernovae ›
Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy ›
The FarView Low Frequency Radio Array on the Moon's Far Side: Science and Array Architecture ›
A general spectral solver for the axisymmetric Jeans equations: fast galaxy modelling with arbitrary anisotropy ›
Evolution of the recent high-accretion state of the recurrent nova T CrB: HST, Swift, NuSTAR, and XMM-Newton observations ›
On the Missing Red Giants near the Galactic Center ›
Constraining dark energy models using Jackknife and Bootstrap resampling ›
A multiwavelength ALMA view of gas and dust in binary protoplanetary system AS 205: Evidence of dust asymmetric distribution ›
Cyclic sunspot activity during the first millennium CE as reconstructed from radiocarbon ›
Dynamical Origin of (469219) Kamo`oalewa of Tianwen-2 Mission from the Main-Belt: $\nu_6$ Secular Resonance, Flora Family or 3:1 Resonance with Jupiter ›
Gravitational Waves and Primordial Black Holes produced by Dark Meta Stable Vacuum Decay ›
Single-wave solutions of the neutrino fast flavor system. Part I. Mechanical properties ›
Compact Stars Sourced by Dark Matter Halos and Their Frozen States ›
Determination of the longitude difference between Baghdad and Khwarezm using a lunar eclipse (the method of Abu Rayhan al-Biruni and Abu al-Wafa al-Buzjani) ›
Neutrino-Induced Polarization Rotation in Active Galactic Nuclei Plasmas ›
Natural Language-Driven Global Mapping of Martian Landforms ›
Photon-dark photon oscillation in M87 and Crab Nebula environments ›
Different effects of the Lorentz and Gaussian bump functions on the formation of primordial black holes and secondary gravitational waves ›
Evidence for GeV emission of the superluminous supernova SN 2017egm ›
Running the small-correlated-against-large estimator at scale: Applications of small-scale CMB lensing estimators on realistic simulations ›
Cosmic acceleration and the Hubble tension from baryon acoustic oscillation data ›
Turbulent dynamos in a collapsing cloud ›
WINTER on S250206dm: A near-infrared search for an electromagnetic counterpart to a gravitational-wave event ›
Distinguishing the Origin of Eccentric Black Hole Mergers with Gravitational-wave Spin Measurements ›
The AURORA Survey: Tracing Galactic Outflows at $z\gtrsim2.5$ with JWST/NIRSpec NUV Absorption Lines ›
Self-bound hybrid stars with strong phase transitions can relieve major compact star observation tensions ›
Machine-learning correction for the calorimeter saturation of cosmic-ray ions with the Dark Matter Particle Explorer: towards the PeV scale ›
AT2019cmw: A highly luminous, cooling featureless TDE candidate from the disruption of a high mass star in an early-type galaxy ›
The role of magnetic fields in shaping $\gamma$-ray emission from the Fermi bubbles ›
Group Therapy for Halos: Advancing Halo Mass Estimation for Galaxy Groups ›
One latent to fit them all: a unified representation of baryonic feedback on matter distribution ›
Enhancing the detectability of ionized Regions during the Epoch of Reionization ›
Multi-color characterization of optically invisible FU Orionis-type outbursts: Demonstration and prospects for the WINTER survey ›
Rapid jet production and suppression during fast state transitions in the black hole X-ray binary MAXI J1348$-$630 ›
STRAWBERRY: Finding haloes in the gravitational potential ›
Probing the millisecond pulsar origin of the $\gamma$-ray excess in the Galactic centre with LISA ›
The effect of matter discreteness on gravitational wave propagation in post-geometrical optics ›
Polarimeter to Unify the Corona and Heliosphere (PUNCH) ›
AGN spectral variability across activity states and searches for axion-like particles ›
Light Travel Time Effects in Kilonova Models ›
The choice of Planck CMB likelihood in cosmological analyses ›
Gamma-ray Orbital Modulation in Spider Pulsars: Three Discoveries and a Universal Modulated Fraction ›
On the Short Dissipation Scales and Current-Sheet Properties of Low-Coronal EUV Brightenings ›
NEOForCE: Near-Earth Objects' Forecast of Collisional Events ›
Bars in low-density environments rotate faster than bars in dense regions ›
Diagnosing Interstellar Magnetic Turbulence with TeV Pulsar Halos ›
Hidden pattern of self-invariant cosmic expansion: Empirical evidence from Hubble diagram of supernovae ›
Digging into the Interior of Hot Cores with ALMA. VI. The Formation of Low-mass Multiple Systems in High-mass Cluster-forming Regions ›
Resonant Scattering of the He I 1.0833$\mu$m Triplet in H II Regions: Emission Spectra ›
Updated Metallicity Diagnostics for Precision Oxygen Abundance Measurements in High-redshift Galaxies with JWST ›
Unveiling Hidden Clustering: An Unsupervised Machine Learning Study of Repeating FRB 20220912A ›
A Not-So-Compact Companion: Massive, Oversize White Dwarf in a Post-Common Envelope Eclipsing Binary ›
The Supernova Remnant G284.3$-$1.8 and Its Relation to the Gamma-ray Binary 1FGL J1018.6$-$5856 ›
Probing Heavily Obscured AGN in Major Galaxy Mergers Using the mm-X-ray Correlation ›
Constraining electromagnetic couplings of ultralight scalars from compact stars ›
Constraining light dark matter in vector-scalar portals with COSI and AMEGO-X ›
Maximal GW amplitude from bubble collisions in supercooled phase transitions ›
Asymptotics of spherical dynamos exhibiting a small-scale MAC balance ›
Uncertainty in predicting the stochastic gravitational wave background from compact binary coalescences ›
Pulsar timing array analysis in a Legendre polynomial basis ›
Reconstructing and resampling: a guide to utilising posterior samples from gravitational wave observations ›
Development and Testing of a Modular Large-Area Cosmic Ray Telescope Using Scintillator-Fiber Hybrid Design for Millimeter-Level Muon Tracking ›
Multipole moments do not uniquely characterize spacetimes beyond general relativity ›
Two-Dimensional Pulsar Distance Inference from Nanohertz Gravitational Waves ›
A Framework for Lorentz-Dirac Dynamics and Post-Newtonian Interaction of Radiating Point Charges ›
Calibration Method of Spacecraft-Inertial Sensor Center-of-Mass Offset for the Taiji Gravitational Wave Detection Mission under Science Mode ›
Resonant Photon-Axion Mixing Driven by Dark Matter Oscillations ›
On flying through the base of a pseudo-streamer ↓↑