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 to the south-west

S Webcam

N Webcam

S Sky
Temperature
3.0 °C
Humidity
54%
Wind
0.0 km/h
Pressure
1026.3 hPa

Moon
Latest preprints on astro-ph:
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Learning Neural Operator Surrogates for the Black Hole Accretion Code ›
Measuring Apsidal Clustering ›
The GlimmIr: Spectroscopic Variability in a z~7 LRD Indicates Rapid Changes in Both the Narrow and Broad Line Regions ›
Properties of black hole mergers in disks of active galactic nuclei ›
Distortion of a relativistic jet echoing a magnetic flux eruption ›
A quantum theory of the alignment and polarization of very small dust grains ›
Determination of the Solar System contribution to the soft X-ray sky ›
Towards A Universal Analytical Model of Population III Star Formation: A Bridge Between Cosmological Scales and Protostars ›
Nature and nurture: the dynamical ages of in situ and accreted globular clusters in the Milky Way ›
Kinematic Lensing Ratio: Reviving Weak Lensing Cosmography as a Geometric Dark Energy Probe ›
Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos ›
Exploring the gaseous halos of z>3 radio galaxies with UVES and JWST/NIRSpec ›
Brightenings AnD Polarity Inversion Tracking (BADPIT) method for studying solar active region evolution before major solar flares ›
Blueberry and Green Pea galaxies live in low density environments ›
Caught in the Cosmic Web: Environmental Impacts on the Halo Substructure Boosts to Dark Matter Annihilation Signals ›
Sensitivity of binary pulsar timing to spin-0 and spin-1 ultralight dark matter ›
Charge diffusion and modulation transfer function in a Nancy Grace Roman Space Telescope detector ›
Label Propagation for Identifying Gamma-Ray Burst Progenitors from Prompt Emission ›
Parker Solar Probe Observations of Compound Reconnection Exhaust Boundaries and Mirror-Mode Structures in the Near-Sun Heliospheric Current Sheet ›
Evolving Low- and Intermediate-Mass Binaries: Departures from Classical Theory ›
Unique photometric variability in SDSS J134628.62+173659.5: clues for moving dust clouds as physical origin of changing-look AGN ›
The $\beta$-Dependence of Particle Spectra in Relativistic Turbulent Reconnection ›
Resolved Maps of Gas and Dust in a Massive Quiescent Galaxy at z=2 from INQUEST-JWST: Evidence of Accretion and Rejuvenation ›
Blinded Mock Data Challenge: Is the Spectral Siren Technique Robust for Measuring the Hubble Constant? ›
Prediction of Celestial Pole Offsets Based on Sliding Window and Bivariate Least Squares Fitting ›
Early Evolution of Earth-Directed Coronal Mass Ejections in the Vicinity of Coronal Holes ›
Double-Peaked Ly$\alpha$ Emission during Reionization Requires Nearby Voids and a Favorable Local Ionizing Background ›
Analytical Modeling of Far-Field Wavefront Error with Beam-Waist and Lateral-Shift Effects in Spaceborne Laser Interferometry ›
DINGO/GAMA /WAVES: HI-halo mass relation ›
Tidal Heating of Stellar Clusters in Fuzzy Dark Matter Halos ›
Effects of nucleon-nucleon short-range correlation and symmetry energy on the evolution of newly born magnetars ›
The Phenomenological Classification of TESS Eclipsing Binaries ›
RV and TTV Measurements of Two Transiting Long-Period Giants around TOI-4600 ›
Studying spherical collapse and its implications in the Eddington-inspired Born-Infeld gravity theory ›
TMC-1: probing the onset of chemical complexity in space ›
Point-like Off-pulse GeV Emission from the Millisecond Pulsar PSR J0437-4715 ›
A Systematic Search for Optical Outbursts in IPs Using ASAS-SN ›
TwinSpecNet: Extending APOGEE's chemical reach to low-S/N spectra via empirical paired learning ›
Transient Parity Violation during Inflation: Implications for PTA Gravitational Waves ›
The End of the First Act: Spectral Running, Interacting Dark Radiation, and the Hubble Tension in Light of ACT DR6 Data ›
Rotational characteristics of five photometrically variable stars ›
Cosmological evolution of fast radio bursts and its rapid decline relative to star formation rate ›
Normalizing flows for density estimation in multi-detector gravitational-wave searches ›
The intrinsic dispersion of elemental abundance ratios in nearby metal-poor halo stars ›
XVII. Nitrogen abundances in Galactic O-type stars: further hints for separating binary-interaction products from effectively single stars ›
36Cl Concentrations from Polar Ice Cores Set New Constraints on the Carrington Event ›
Turbulence and its Potential Impact on Solar Chromospheric and Coronal Heating ›
Euclid preparation. Refining input galaxy shape distributions for shear calibration simulations ›
Nonlinear Relativistic Effects on Cosmological Redshift Drift ›
Population synthesis of Be X-ray binaries in the Small Magellanic Cloud: angular momentum recycling and stable mass transfer ›
SRGA J115215.0$-$510656: an unusual long-period eclipsing dwarf nova with disc wind signatures ›
A short-period binary OGLE-BLG-ELL-006503 showing slow variations in brightness ›
Radial Profiles of Binary Fraction in Elliptical Galaxies ›
Shape and spin axis determination of the Tianwen-2 target asteroid (469219) Kamo'oalewa from lightcurve inversion ›
Invariant manifolds in barred galaxy simulations. I. Material density waves ›
A Rare Eddington-Limited, Heavily Obscured Low-Mass Active Galactic Nucleus Likely Triggered by a Galaxy Merger ›
Dust enrichment from core-collapse supernovae and extinction curves in the high-redshift universe ›
SPHEREx Ultracool Dwarf spectral Atlas (SUDA): Atmospheric and Fundamental Parameters of Ultracool Dwarfs ›
IQUEYE at Gemini South: instrument, science commission, and first results ›
Status of the KM3NeT real-time analysis framework ›
Coronal Diagnostics Via Modelling Periodic-Beaded Stripes of Solar Radio Bursts ›
The Influence of the Fractal Dimension on Dust Evolution in Protoplanetary Disks ›
Mujic{\Lambda}: Reconstructing Initial Conditions from Incomplete Redshift Surveys with Projected Optimization ›
Oxygen and nitrogen isotopologues on cold COCONUTS-2b observed with MIRI/MRS ›
Bayesian power spectrum estimation with modelling of systematic effects in delay-fringe rate space ›
Predicted number counts and clustering of Hi galaxies from future radio surveys ›
Bayesian component separation and power spectrum estimation for 21 cm intensity mapping data cubes ›
The tale of the 3 planets: 3D cloud feedback enhances the spectral diversity of warm Jupiters ›
Eccentricity as a signature of hierarchical subsolar-mass mergers in collapsar disks ›
Testing Scale-Dependent Modified Gravity with DESI DR1 ›
The effect of spectral resolution on biosignature detection via reflected light observations of the Earth through time ›
Energy-Dependent Polarization Angle Variability as a Robust Diagnostic for Blazar Flaring Mechanisms ›
The evolution of the baryonic content and mass profiles of satellite galaxies in the MTNG simulations ›
Bouncing cosmologies from Born-Infeld-type gravity ›
Strong-field signatures of a regular black hole in an Einasto dark matter halo ›
Revisiting Turner Window Axions: The Untapped Potential of NaI Dark Matter Detectors ›
Asteroid-mass Primordial Black Holes as Dark Matter from Supersymmetry ›
Parameter-estimation bias induced by transient orbital resonances in extreme-mass-ratio inspirals ›
Time-of-Flight Constraints on Neutrino Millicharge from Supernova Neutrinos in Galactic Magnetic Fields ›
Gravitational Properties of the Monopole Bag ›
Trapping, Irregular Waveforms, and Efficient Radiation in Ultra-relativistic Black Hole Encounters ›
Approximating Periodic Orbits with Algebraic Curves and Related Minimal Problems ›
A positive definite formulation of vacuum decay with reduced symmetry ›
Neutron Stars and Neutron Skins: Connecting Finite Nuclei to Dense Matter ›
Outer-Crust Equations of State for Neutron Stars ›
Implementing a Robust Test of Galaxy Catalogue Completeness for Dark Siren Measurements of the Hubble Constant ›
Simba Simulation: The Effect of Feedback Physics on Matter Distribution in the Cosmic Web ›
Tidal disruptions of close white dwarf binaries by intermediate mass black holes ›
AGN jet evolution simulation with GADGET4-OSAKA ›
Cosmic Rays on Galaxy Scales: Progress and Pitfalls for CR-MHD Dynamical Models ›
Clues to inside-out quenching in quiescent galaxies at $1.2\lesssim z\lesssim2.2$: Age, Fe-, and Mg-abundance gradients from JWST-SUSPENSE ›
Stochastic Gravitational Waves from Modulated Reheating ›
Time-Dilation Methods for Extreme Multiscale Timestepping Problems ›
AMIGO: a Data-Driven Calibration of the JWST Interferometer ›
Dynamics and observational signatures of core-collapse supernovae with central engines: hydrodynamics simulations with Monte Carlo post-processing ›
Imaging and Polarimetric Signatures of Konoplya-Zhidenko Black Holes with Various Thick Disk ›
Strong Lensing Model and Dust Extinction Maps of the Host Galaxy of Type Ia Supernova H0pe ›
Development of a planar cable-driven parallel robot for submillimeter and terahertz beam mapping measurements ›
Effects of Resolution and Local Stability on Galactic Disks: I. Multiple Spiral Mode Formation via Swing Amplification ›
ELG$\times$LRG distribution through dark matter halo dynamics ›
A new Gaia census of OB associations within 1 kpc ›
CPI-C: Cool Planet Imaging Coronagraph on Chinese Space Station Survey Telescope ›
Evolution of Massive Main-sequence Stars in Rapid Population Synthesis. I. Framework and Implementation ›
Astrophysical constraints on the cold equation of state of the strongly interacting matter ›
Mind the peak: improving cosmological constraints from GWTC-4.0 spectral sirens using semiparametric mass models ›
Accretion disc winds in X-ray binaries ›
Baryonification III: An accurate analytical model for the dispersion measure probability density function of fast radio bursts ›
Down-bending Breaks in Galactic Disks Are an Intrinsic Byproduct of Inside-out Growth ›
Impact of rotation on the amplitude of acoustic modes in solar-like stars: Insights from hydrodynamical simulations ›
Fermi-LAT 16-year Source List ›
Polarimetric Tomography Applied to Synthetic Multi-Spacecraft White-Light Images: Observing Coronal Mass Ejections in 3D ›
Spin-up and spin distribution of stellar black holes grown by gas accretion in proto-stellar clusters ›
From Detection to Host Galaxy Identification: Precision Continuous Gravitational Wave Localization with a Few Anchor Pulsars ›
The ZTF-ULTRASAT experiment: Characterizing the non-transients in ULTRASAT's high cadence survey ›
Reanalysing large-scale structure using an updated gamma-ray burst spatial density approach ›
Dark energy, spatial curvature, and star formation efficiency from JWST photometric and spectroscopic high-redshift galaxies ›
A Salpeter-like filament linear density function across nearby molecular clouds ›
Search for Anisotropic Pair Halos Associated with Blazar Jets ›
Circumbinary Discs as the Origin of Circumstellar Material around Interacting H-poor Supernovae and Fast Blue Optical Transients ›
Hill's level surfaces in the circular restricted three-body problem solved ›
Testing $\Lambda$CDM with ANN-Reconstructed Expansion History from Cosmic Chronometers ›
STVG-MOG Cluster Dynamics and the Cosmological $1/r^2$ Force Law from Pairwise kSZ Data ›
The FLAMINGO simulations data release ›
Cosmic gas accretion from filaments onto galaxy clusters using the IllustrisTNG simulation ›
Recovering cosmological parameters from the mock gravitational wave data of the Einstein Telescope ›
Probing modified gravitational-wave dispersion with bursts from eccentric black-hole binaries ›
Detecting gravitational wave background with equivalent configurations in the network of space based optical lattice clocks ›
Comet-type periodic motions and their out-of-plane bifurcations in the Earth-Moon CR3BP: a computational symplectic analysis ›
Stable black hole solutions with cosmological hair ›
Testing Dark Energy with Black Hole Ringdown ↓↑