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
view from south-west
S Webcam
N Webcam
S Sky
Temperature
2.8 °C
Humidity
72%
Wind
12.9 km/h
Pressure
1007.5 hPa
Moon
Latest preprints on astro-ph:
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PDS 70 unveiled by star-hopping: total intensity, polarimetry and mm-imaging modeled in concert ›
The Host Galaxy of a Dormant, Overmassive Black Hole at $z=6.7$ May Be Restarting Star Formation ›
IMBH Progenitors from Stellar Collisions in Dense Star Clusters ›
The impact of stellar bars on quenching star formation: insights from a spatially resolved analysis in the local Universe ›
Study of the $\sim 50$ kpc circumgalactic environment around the merger system J2057-0030 at $z$ $\sim$ 4.6 using ALMA ›
Beyond MACS: Physical properties of extremely X-ray luminous clusters at $z > 0.5$ ›
Modelling stochastic and quasi-periodic behaviour in stellar time-series: Gaussian process regression versus power-spectrum fitting ›
Searching for Free-Floating Planets with TESS: I. Discovery of a First Terrestrial-Mass Candidate ›
Joint r-Process Enrichment by Supernovae with a Metallicity Threshold and Neutron Star Mergers ›
Supermassive black holes from runaway mergers and accretion in nuclear star clusters ›
Probing the intergalactic medium during the Epoch of Reionization using 21-cm signal power spectra ›
Soft Photon Heating: A Semi-Analytic Framework and Applications to $21$cm Cosmology ›
Kinematic and metallicity of the dwarf spheroidal galaxy Andromeda XVIII ›
Future Perspectives for Gamma-ray Burst Detection from Space ›
Laser Irradiation of Carbonaceous Chondrite Simulants: Space Weathering Implications for C-complex Asteroids ›
Transitory tidal heating and its impact on cluster isochrones ›
Evidence for a nearly orthogonal rotator in GX 301--2 with phase-resolved cyclotron resonant scattering features ›
General non-linear fragmentation with discontinuous Galerkin methods ›
Delivery of Dust Particles from Protoplanetary Disks onto Circumplanetary Disks of Giant Planets ›
Gravitational waves from nonradial oscillations of stochastically accreting neutron stars ›
Finding the particularity of the active episode of SGR J1935+2154 during which FRB 20200428 occurred: Implication from a statistics of \textit{Fermi}/GBM X-ray bursts ›
Dark supernova remnant buried in the Galactic-Centre "Brick" G0.253+0.016 revealed by an expanding CO-line bubble ›
A Self-Consistent Treatment of the Line-Driving Radiation Force for Active Galactic Nuclei Outflows: New Prescriptions for Simulations ›
MINDS: Mid-infrared atomic and molecular hydrogen lines in the inner disk around a low-mass star ›
Coherent Inverse Compton Scattering in Fast Radio Bursts Revisited ›
The Fireball of November 24, 1970, as the Most Probable Source of the Ischgl Meteorite ›
Comparing the three-dimensional morphological asymmetries in the ejecta of Kepler and Tycho in X-rays ›
Generation of relativistic electrons at the termination shock in the solar flare region ›
Generation and annihilation of three dimensional magnetic nulls in extrapolated solar coronal magnetic field: Data-based Implicit Large Eddy Simulation ›
Resolved magnetohydrodynamic wave lensing in the solar corona ›
A method for non-linear inversion of the stellar structure applied to gravity-mode pulsators ›
Does dark energy really revive using DESI 2024 data? ›
Big Bang equivalence of $f(R)$ gravity with no cosmological lithium problem ›
Data reconstruction of the dynamical connection function in $f(Q)$ cosmology ›
Euclid preparation. Improving cosmological constraints using a new multi-tracer method with the spectroscopic and photometric samples ›
The 2018 outburst of MAXI J1820+070 as seen by Insight-HXMT ›
Detection and prebiotic chemistry of possible glycine precursor molecule methylenimine towards the hot molecular core G10.47+0.03 ›
A Photoionization model for the Infrared Coronal Line Emission in the Classical Nova V1716 Scorpii ›
The formation of transiting circumplanetary debris discs from the disruption of satellite systems during planet-planet scattering ›
Star-by-star dynamical evolution of the physical pair of the Collinder 135 and UBC 7 open clusters ›
Efficient Identification of Broad Absorption Line Quasars using Dimensionality Reduction and Machine Learning ›
A New Computational Method for Energetic Particle Acceleration and Transport with its Feedback ›
VELOcities of CEpheids (VELOCE) I. High-precision radial velocities of Cepheids ›
A Multiwavelength Survey of Nearby M dwarfs: Optical and Near-Ultraviolet Flares and Activity with Contemporaneous TESS, Kepler/K2, \textit{Swift}, and HST Observations ›
On the roles of stellar rotation and binarity in NGC 2423's main-sequence turnoff region ›
Gemini Near Infrared Spectrograph -- Distant Quasar Survey: Rest-Frame Ultraviolet-Optical Spectral Properties of Broad Absorption Line Quasars ›
Modeling nonlinear scales with COLA: preparing for LSST-Y1 ›
Radio Observations as an Extrasolar Planet Discovery and Characterization: Interior Structure and Habitability ›
Gravitational wave luminosity distance-weighted anisotropies ›
A link to the past: characterizing wandering black holes in Milky Way-type galaxies ›
CRIRES$^+$ transmission spectroscopy of WASP-127b. Detection of the resolved signatures of a supersonic equatorial jet and cool poles in a hot planet ›
First Search for High-Energy Neutrino Emission from Galaxy Mergers ›
The Field Theory Axiverse ›
Semiclassical bremsstrahlung from a charge radially falling into a Schwarzschild black hole ›
Cosmological Inflation and Dark Sector from 11D Supergravity ›
The relic density and temperature evolution of light dark sector ›
Improving inference on neutron star properties using information from binary merger remnants ›
Energetic particle acceleration and transport with the novel Icarus$+$PARADISE model ›
Helicity oscillations in Rayleigh-B\'enard convection of liquid metal in a cell with aspect ratio 0.5 ›
Images of Kerr-MOG black holes surrounded by geometrically thick magnetized equilibrium tori ›
floZ: Evidence estimation from posterior samples with normalizing flows ›
Sound speed as a source of the gravitational field in modified gravity ›
Missing Metals in DQ Stars; a Compelling Clue to their Origin ›
B-mode polarization forecasts for GreenPol ›
The Local Value of H$_0$ ›
Ciii]$\lambda1909$ emission as an alternative to Ly$\alpha$ in the reionization era: the dependence of Ciii] and Ly$\alpha$ at $3 ›
Project Dinos I: A joint lensing-dynamics constraint on the deviation from the power law in the mass profile of massive ellipticals ›
Variation of the stellar initial mass function in semi-analytical models III: testing the cosmic ray regulated integrated galaxy-wide initial mass function ›
Low-frequency pulse-jitter measurement with the uGMRT I : PSR J0437$-$4715 ›
Impact of anisotropic cosmic-ray transport on the gamma-ray signatures in the Galactic Center ›
The Kinematic and Chemical Properties of the Close-in Planet Host Star 8 UMi ›
Simulated host galaxy analogs of high-z quasars observed with JWST ›
Quantifying the escape of Ly$\alpha$ at $z\approx 5-6$: a census of Ly$\alpha$ escape fraction with H$\alpha$ emitting galaxies spectroscopically confirmed by JWST and VLT/MUSE ›
Some Old Globular Clusters (and Stars) Inferring That the Universe Is Older Than Commonly Accepted ›
Fast and Slow Crystallization-driven Convection in White Dwarfs ›
Deep Optical Emission-Line Images of Nine Known and Three New Galactic Supernova Remnants ›
The disappearance of the blue and luminous progenitor of the Type IIn SN 2010jl ›
The seeding of cosmic ray electrons by cluster radio galaxies: a review ›
Prospects of the multi-channel photometric survey telescope in the cosmological application of Type Ia supernovae ›
Exoplanet Detection : A Detailed Analysis ›
GHOST Commissioning Science Results III: Characterizing an iron-poor damped Lyman $\alpha$ system ›
Effect of Systematic Uncertainties on Density and Temperature Estimates in Coronae of Capella ›
Vorticity and magnetic dynamo from subsonic expansion waves II: Dependence on magnetic Prandtl number, forcing scale, cooling time ›
H$\alpha$ Reverberation Mapping from Broad-band Photometry of Dwarf Seyfert 1 Galaxy NGC 4395 ›
Sky location of Massive Black Hole Binaries in the foreground of Galactic white dwarf binaries ›
Singlet-doublet fermion dark matter with Dirac neutrino mass, $(g-2)_\mu$ and $\Delta N_{\rm eff}$ ›
Gravitational Wave Probe of Primordial Black Hole Origin via Superradiance ›
Nucleonic models at finite temperature with in-medium effective fields ›
Proto-strange quark stars from density-dependent quark mass model ›
The neutrino fog for dark matter-electron scattering experiments ›
Quantum tachyonic preheating, revisited ↓↑