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

Dome at sunrise

S Webcam

N Webcam

S Sky
Temperature
19.9 °C
Humidity
51%
Wind
4.8 km/h
Pressure
1020.3 hPa

Moon
Latest preprints on astro-ph:
›
Magnus mountains on spinning neutron stars ›
Synchrotron and Inverse-Compton Signatures of Black to White Hole Explosions: Weibel-Mediated External Shocks in the Interstellar Medium ›
Microscopic Interaction versus Purely Gravitational Coupling in Strange Quark Stars Admixed with Dark Matter: A One-Fluid and Two-Fluid Comparison ›
Climates of Gl 514 b ›
The \^G Infrared Search for Extraterrestrial Civilizations with Large Energy Supplies. V. When Galaxies Glow with Industry ›
Recycled Gas Dominates the Metal-rich Fuel of Supermassive Black Holes ›
Interacting Supernovae: a Radio and X-ray Strategy to Constrain the Structure of the Circumstellar Medium ›
Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics ›
Don't Cut Corners: How Training Outside the Prior Makes Simulation-Based Inference More Robust ›
FLAGS II: Constraining Galaxy Formation Models with Dimensionality Reduction of Direct Observables ›
Trace the Self-Gravitating Gas Using CO Isotopologues ›
Astronomical Cardiology II: A Search For Heartbeat Stars Using APOGEE and TESS ›
CLASSY. XV. Kinematics and Spatial Distributions of Outflows in Local Highly Star-Forming Galaxies ›
Ripples in the OCEANS: Broad Line Variability of Little Red Dots ›
3D Radiative Transfer of Lyman-series Lines with SKIRT ›
Large-Scale Dynamos Driven by Shear-Flow-Induced Jets ›
Observing Co-Located Neutral and Ionized Gas-Phase Iron Depletion in the Magellanic Clouds ›
Laser-micromachined silicon-platelet feedhorns for large-scale submillimeter and millimeter-wave focal planes ›
The Wave-Regulated Precursor of a Near-Parallel Interplanetary Shock Observed by Parker Solar Probe ›
Gaia parallax bias via spherical harmonics: A Python tool and discussion of possible causes ›
How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition ›
Titanium Oxide Absorption as a Proxy to Detect Long term Variation and Activity Cycle in Proxima Centauri ›
An Evolving Leptonic Jet Model for Delayed Radio Flares in Neutrino Blazars ›
SPURS: Massive Stars, Dense Gas, and Ly$\alpha$ Escape in GN-z11 at $z = 10.6$ ›
ALMA observations of pre-JWST z ~ 10 galaxy candidates: A CO(J = 9-8) line from a ULIRG at z = 2.54 and revisit of the photometric redshifts with JWST photometry ›
Are Near Resonant Multiple-planet Systems from Kepler Young? ›
Are Hot Jupiters Tidally Disrupted During Stellar Main Sequence? ›
Photospheric Kelvin--Helmholtz Vortices as Possible Drivers of Coronal Heating: Implications of the DKIST Observations ›
Waterfall-modulated $\alpha$-attractors ›
Tropospheric Ducting Prediction based on GFS Model Data at Inyarrimanha Ilgari Bundara, the CSIRO Murchison Radio-astronomy Observatory ›
X-ray signals converted from high-frequency gravitational waves emitted by spinning light primordial black hole dark matter ›
Elemental Composition Evolution during the 2024 September 30 Solar Eruption: A Comparison of Hot and Cool Plasma Components with Solar Orbiter/SPICE, Hinode/EIS, and Chandrayaan-2/XSM ›
Chondrule formation in the outer disk from the primary three-dimensional chemical composition of CM chondrules ›
Gal3D: Superellipsoid Modeling of Radial 3D Galaxy Structure in IllustrisTNG and EAGLE Simulations ›
Cross-spectral Analysis of the Type-C Quasi-periodic Oscillation Shoulder Component in GX 339-4 ›
SNIFFLES I: Intended Emission, Unwanted Emission, and Unintended Radiation from Low-Earth Orbiting Satellites Impacting Radio Astronomy from 1-26 GHz ›
AT 2024qfm: a luminous fast blue optical transient at a redshift of z = 0.2267 identified by Lasair-ZTF ›
TIC 433545934: The first 2+2 type doubly eclipsing binary with extra, mutual eclipses ›
Revisiting gravitational instability in protostellar discs with improved radiative cooling models ›
Complex Energy-Dependent Behaviour of Quasi-Periodic Oscillation Observed in GRS 1915+105 ›
Cosmic Structures in CDM and SIDM ›
Forecast for the detectability of patchy hydrogen reionization in WEAVE-QSO measurements of the Lyman-$\alpha$ forest power spectrum at redshift $z \geq 4$ ›
The atmospheric vertical structure of Uranus and Neptune from thermochemical models: the impact of model assumptions ›
A Radon-Transform Perspective on Exoplanet Transits ›
Cosmography with DESI-DR1 Cosmic Chronometers: Direct H(z) measurements from Luminous Red Galaxy ages ›
FOSSIL's preliminary thermal architecture ›
Optical development of the BISOU breadboard ›
Assessing Planetary Stability and Long-Term Habitability in Nearby Stellar Binaries: 70 Oph, 36 Oph, $\gamma$ Leo ›
Optical concept model of the future cosmology project BISOU ›
The low luminosity end of Galactic HMXBs with eROSITA: Establishing a luminosity floor for accreting BeXRBs ›
Stellar tidal systematics in apsidal-motion searches for circumbinary planets: CH Ind and SW CMa ›
X-ray Flaring and Variability in NGC 1275, the Heart of the Perseus Cluster ›
Radio Properties of Narrow-Line and Broad-Line Seyfert 1 Galaxies ›
Differential Reddening and Extinction Law Analyses of Galactic Open Clusters ›
JWST Detects a Dusty AGB-like Source Before the Type Ia-CSM Supernova 2026sqf ›
Radio Monitoring of Classical Novae using the ASKAP Variable and Slow Transients Survey ›
Automatic detection of fast oscillations of dark matter scalar field and updated cosmological constraints on QCDM ›
The Most Probable Outer Density Profile from Excursion Set Theory ›
Widefield Arecibo Virgo Extragalactic Survey: II. Characterizing the HI properties and environment of the WAVES South region ›
The Production of Electron-Capture Elements in Thermonuclear Supernovae: Theory vs. Observations ›
JWST MIRI Medium Resolution Spectrometer Point Fixed Pattern Corrections: Cleaner and Higher Signal-to-Noise Spectra of Point Sources ›
Strict Limits on Helium Absorption from LHS 1140 b from Four JWST NIRISS Transits ›
No Helium Detected in LHS 1140 b from Four JWST NIRISS/SOSS Transits ›
Higher-Order Analytical Expansion of Thawing Dark Energy with an Exponential Potential ›
Numerical Model Simulation of the Carruthers GCI Images ›
The sensitivity of TESS to transiting planets in TOIs with close-in stellar companions ›
Production of Primordial Black Holes in the Double D3-Brane - anti-D3-Brane Inflation Model ›
Gas Flows and Mass Accretion Rates in Eight Dippers: HD 142666, HD 143006, HD 145718, V935 Sco, DoAr 25, EPIC 204638512, EPIC 205151387, and EPIC 203850058 ›
Learned proposals in trans-dimensional inference are optimal at equilibrium, not during assembly ›
Effects of Quantum Spin-Connection Foam in the Solar System, Galaxies, and the Universe ›
Thermal false vacuum decay near black holes is aspherical ›
Singlet-Doublet fermion origin of dark matter, neutrino mass and inverse first-order electroweak phase transition ›
Spontaneous Scoto-leptogenesis ›
Massive cold hybrid stars in a modified Polyakov-Nambu-Jona-Lasinio model ›
Scalar induced gravitational waves as probes of dark QCD ›
Temperature effects on white dwarfs in modified gravity ›
Long-term 3+1 simulations of primordial black hole formation during radiation domination ›
Vector Perturbations in Ghost-Free Quasidilaton Massive Gravity ›
Development of an Embedded Receiver for Space Exploration Missions ›
Deep Investigation of Neutral Gas Origins (DINGO): Options for the Processing and Storage of Radio Astronomy Data for robust Deep Spectral Line Imaging in the SKA-Era using uv-Grids ›
The origin of the galaxy size-stellar metallicity relation: A semi-analytical perspective ›
StarEmbed: Benchmarking Time Series Foundation Models on Astronomical Observations of Variable Stars ›
Dark Matter profiles of "in silico" galaxies: deep learning inference ›
Gravitational potential drives the concentration dependence of the stellar mass-halo mass relation ›
Discovery of Isolated, Quenched Candidate Backsplash Dwarf Galaxies near M101 ›
Cosmic Chance Superpositions: Largest Catalog of Quasar-Galaxy Pairs at a Projected Separation of $D \lesssim 20$ kpc ›
Probing Dark Matter Halos of High-redshift Quasars via Wide-Field Clustering ›
McFACTS. IV. Electromagnetic Counterparts to AGN-disk-embedded Binary Black Hole Mergers ›
Filling The Pockets: The Spherical Nature of 3D Deflagration in Thermonuclear Supernovae ›
Sound Speed Resonance in the Gravitational Wave Background as a probe for non-standard early universe cosmologies ›
Nonminimally coupled quintessence with sign-switching interaction ›
Measurement of the minimum cold dark matter halo mass with strong gravitational lensing ›
Theoretical Constraints on Neutron Star Superfluidity from Her X-1 Precession ›
A Unified [CII] Morpho-Kinematic Corpus for 31 Star-Forming Galaxies at z = 4.26-5.68: The High-z Kinematic Corpus Z1 ›
The EPS Research Astro-RAG Platform: A Unified Open-Science Infrastructure for Cross-Epoch Astrophysical Kinematic Analysis, LLM-Assisted Research Workflows, and Educational Outreach ›
The Delta Resonance in the Neutrino Sky ›
Probing Baryonic Feedback Effect with CSST Weak Lensing and Future FRB Measurements ›
Pulsed Infrared Emission from Magnetar 4U 0142+61 Detected by JWST ›
A Model Context Protocol Server for Astrophysical RAG: Unified Access to HI, Dwarf, Globular Cluster, IntZ, and ALPINE Kinematic Corpora with FAISS Semantic Search ›
The emergence of X-ray emission lines during relativistic radio-jet formation in the changing-look active galactic nucleus 1ES 1927+654 ›
MOA-2020-BLG-108Lb: A Giant Planet Beyond the Snow Line of a Low-Mass Lens Near the Lower Boundary of the Mass-Ratio Desert ›
Planet-moon ejections in close stellar encounters ›
Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars ›
Environmental Noise Challenges for the Einstein Telescope - A Review ›
Lunar Reflective Interferometry ›
Gauge-Invariant Bubble Nucleation and Gravitational Waves from First-Order Electroweak Phase Transitions ›
Towards Accurate Gravitational Wave Predictions: Gauge-Invariant Nucleation in the Electroweak Phase Transition ›
Sub-Leading Logarithms for Scalar Potential Models on de Sitter ›
Forbidden dark matter assisted by first-order phase transition and associated gravitational waves ›
Not So Minimal Warm Inflation ›
Can Primordial Black Holes Be Seeds for Early Galaxies in Models Satisfying the Covariant Entropy Bound? ↓↑