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

over the clouds

S Webcam

N Webcam

S Sky
Temperature
5.6 °C
Humidity
94%
Wind
16.1 km/h
Pressure
1017.7 hPa

Moon
Latest preprints on astro-ph:
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Solver-in-the-Loop Applications in Astrophysical (Magneto)hydrodynamics ›
Searching for Transit Timing Variations in young transiting systems ›
Revealing the accelerating wind in the inner region of the colliding-wind binary WR 112 ›
SN 2024afav: A Superluminous Supernova with Multiple Light Curve Bumps and Spectroscopic Signatures of Circumstellar Interaction ›
Do Low-Mass, Low-Luminosity AGNs Deviate from the Quasar Main Sequence? ›
An Ancient Brown Dwarf Transiting a Metal-Poor Thick Disk Star ›
The quenched fraction of satellites around simulated Milky Way-mass galaxies ›
Lyman-$\alpha$ Visibility During the Epoch of Reionization: Combining JWST FRESCO Grism Data with Keck Archival Spectroscopy ›
A Galactic Transformation -- Understanding the SMC's Structural and Kinematic Disequilibrium ›
A Song of Lines and Winds: Tracing the Signatures of AGN Outflows in X-rays ›
Globular clusters in \textsc{OrbIT}: complete dynamical characterisation of the globular cluster population of the Milky Way through updated orbital reconstruction ›
A Test of Substellar Evolutionary Models with High-Precision Ages from Asteroseismology and Gyrochronology for the Benchmark System HR 7672AB ›
The THESAN project: Lyman-alpha intensity mapping of cosmic reionization ›
Generalized tension metrics for multiple cosmological datasets ›
SHORES II: Multi-frequency Characterisation of the Sub-mJy Radio Population in FIR-selected Fields ›
Black hole merger rates for LISA and LGWA from semi-analytical modelling of light seeds ›
On the Origin of Intracluster Light based on the High-resolution Simulation, NewCluster ›
Formation of cold giant planets around late M dwarfs via core accretion and the fate of inner rocky worlds ›
Exploring Exoplanet Dynamics with JWST: Tides, Rotation, Rings, and Moons ›
ExoNAMD: Leveraging the spin-orbit angle to constrain the dynamics of multiplanetary systems ›
The eROSITA Final Equatorial-Depth Survey (eFEDS): X-ray stacking analysis of Subaru's optically selected clusters spanning low richness regime ›
yieldplotlib: A unified library for exoplanet yield code visualizations ›
From the Intergalactic to the Interstellar Scales -- EQUALS: a High-resolution Legacy Survey of Gas in the Distant Universe Using ESPRESSO ›
The Milky Way Project: Bridging Intermediate- and High-Mass Star Formation with the MIRION Catalog of Yellowballs ›
Effects of helium sedimentation on late star formation in galaxy clusters ›
A pan-galaxy study of synthetic giant molecular filaments: a turbulence-dominated life cycle ›
FIP-TOI: Fast Imaging Pipeline for Pulsar Localisation with a Transient-Oriented Radio Astronomical Imager ›
CLASSY XIV: The Nitrogen Exception -- Multi-Phase Enrichment and Feedback in High-$z$ Analogs ›
Revealing Hidden Repeaters in the CHIME/FRB Catalog: Semi-Supervised Insights into the Fast Radio Burst Population ›
A Fully Photometric Approach to Type Ia Supernova Cosmology in the LSST Era: Host Galaxy Redshifts and Supernova Classification ›
Photometric Analysis of TCP J20171288$+$1156589 -- WZ Sge Type Dwarf Nova with Delayed Ordinary Superhumps Emergence ›
Rebrightenings of gamma-ray burst afterglows from an increasing magnetic inclination angle of a nascent magnetar ›
Modelling dust coagulation, dynamical drag and turbulent mixing during star and disc formation ›
Water vapor emission at the warm cavity wall of the HD 100546 disk as revealed by ALMA ›
Testing the Distance Duality Relation with Cosmological Observations at high Redshift using Artificial Neural Network ›
Unified models revisited I: modelling the effect of source geometry on radio galaxy/quasar unification ›
Deciphering transmission spectra by exploring the solar paradigm ›
Optical Study of TRAPUM Pulsars and Modelling of the Redbacks: PSR J1036$-$4353 and PSR J1803$-$6707 ›
Venus as an exoplanet analog: extended UV transit signatures and coronal occultations ›
The impact of surface acetylene cyclotrimerization on the abundance of aromatic hydrocarbons in carbon-rich asymptotic giant branch stars ›
A New Torus Generator for AGAMA ›
Actions of highly eccentric orbits ›
Exoplanets synchronization: Learning from Venus' retrograde rotation ›
Angular BAO Forecasts for the IBIS Medium-Band Survey ›
Rotational Spectra and Search for Aromatic Imines: 9-Iminofluorene and Benzophenone imine ›
Probing Cosmic Magnetism with Rotation Measure-Squared-Galaxy Cross-Correlations ›
NEO and imminent impactor discoveries from Hungary: recent results and lessons learnt ›
A XRISM/Resolve view of the dynamics in the hot gaseous atmosphere of M87 ›
Fast X-ray Variability from the Coronae of Supermassive Black Holes ›
What Galaxy Clusters Have to Say About Dynamical Dark Energy and $H_0$ ›
An Extended WZDR Model with Interacting Scalar Field Dark Matter and Stepped Dark Radiation ›
A Fast, Parallelized, GPU-Accelerated Photochemical Model, XODIAC, with Built-in Equilibrium Chemistry and Multiple Chemical Networks for Exoplanetary Atmospheres ›
Revisiting the atmosphere of HAT-P-70b with CARMENES high-resolution transmission spectroscopy ›
The influence of external environment at cosmic noon on the subsequent evolution of galaxy stellar mass ›
Non-thermal Synchrotron Emission and Polarization Signatures during Black Hole Flux Eruptions ›
Multicolour Validation of Two Temperate Mini-Neptunes Around M-dwarf Habitable Zones ›
TOI-7166 b: A Habitable Zone mini-Neptune planet around a nearby low-mass star ›
Precise determination of circumstellar disk lifetimes: Disk evolution in a single star-forming region ›
Probing memory-burdened Primordial Black Holes with global 21 cm signal ›
The GLEAM 4-Jy (G4Jy) Sample: III. Further host-galaxy identification, and redshift assessment ›
Anisotropic Diffusion Modeling of Cosmic-Ray Lepton Propagation ›
Over-abundant gamma-like signals around Solar disk shadows by twin bent and smeared muon and electron pairs secondaries, versus rare local TeV gamma ›
SS433 PeV neutron jet feeding the far TeV gamma beam ›
Core-halo scaling relations in self-interacting scalar field dark matter ›
Understanding the Planetary Formation and Evolution in Star Clusters(UPiC)-II: Catalog of planets/candidates in Open Clusters and Moving Groups ›
Paucity of downward UHE neutrino tracks in IceCube versus unexpected huge KM3-230213A event: solving the puzzles? ›
Giant outbursts of clumpy material preceding Type II supernova 2024qiw ›
JWST reveals extended stellar disks for ALMA-bright dusty star-forming galaxies in the Spiderweb protocluster ›
A Multi-Probe ISW Study of Dark Energy Models with Negative Energy Density: Galaxy Correlations, Lensing Bispectrum, and Planck ISW-Lensing Likelihood ›
Trends in gravitational wave emission in axisymmetric simulations of rotating core-collapse supernovae ›
Dynamical Dark Energy in light of DESI BAO and Full-Shape Data ›
Universal relation involving fundamental modes in two-fluid dark matter admixed neutron stars ›
Vision Transformers for Cosmological Fields: Application to Weak Lensing Mass Maps ›
Statistics of the projected angles between the black-hole spin and the host-galaxy rotation axes from NewHorizon ›
Evidence of young magnetars in massive binary embedded in a supernova remnant as sources of active fast radio bursts ›
Simulation Study of Binary Mergers of Galaxy Clusters I: Properties of Merger Shocks and Radio Emission ›
FEASTS Compared with Simulations: Abnormally Irregular and Extended HI Morphologies at a Column Density of $10^{18}\,\text{cm}^{-2}$ in TNG50 and Auriga ›
EP241217a: a likely Type II GRB with an achromatic bump at z = 4.59 ›
Inference of $B$-mode polarization in the presence of non-Gaussian foregrounds ›
Counting voids and filaments: Betti Curves as a Powerful Probe for Cosmology ›
Interplay between Escaping Cosmic Rays and Interstellar Medium: Driving of Galactic Winds and Shaping the Local Proton Spectrum ›
Dynamical Dark Energy and the Unresolved Hubble Tension: Multi-model Constraints from DESI 2025 and Other Probes ›
Small EUV Brightenings in the Quiet Solar Atmosphere: New Insights from the Solar Orbiter Mission ›
Diagnosing Interstellar Magnetic Turbulence with TeV Pulsar Halos ›
Revisiting PBH Accretion, Evaporation and Their Cosmological Consequences ›
Squeezed Limit non-Gaussianity Estimation with Cosmic Shear ›
Back-End System of BURSTT ›
SPHEREx Pre-Perihelion Mapping of $\mathrm{H_2O}$, $\mathrm{CO_2}$, and $\mathrm{CO}$ in Interstellar Object 3I/ATLAS ›
Generating LSB-optimised synthetic images for simulated galaxies ›
Limits on Unintended Radio Emission from Geostationary and Geosynchronous Satellites in the SKA-Low Frequency Range ›
BSN: Light Curve Modeling and Orbital Evolution of the Total-Eclipse Contact Binary EZ Oct ›
Phase-space perturbation theory for cosmic large-scale structure ›
Revisiting the Evolutionary Status of Massive Stars at the central parsec of the Milky Way ›
Prospects for independent measurement of $\boldsymbol{\ell}$=1,2,3 CMB anisotropy multipoles using the anisotropic Sunyaev-Zel'dovich effect ›
The influence of Parker spiral on the reflection-driven turbulence ›
Surface temperature of an accretion disk around a wormhole Kerr-mimicker ›
Relationship between Poincar\'e Sections and Spectral Characteristics of Orbits of Globular Clusters in the Central Region of the Galaxy ›
Chemical complexity in star formation induced by stellar feedback: cores shock-formed by the supernova remnant W44 ›
Interstellar Medium in Extremely High Star-Formation Regions: A Prospect of Observations on the Millimetron ›
Two-stage primary acceleration in filament initial eruption under a fan-spine magnetic configuration ›
Systematic determination of dust properties for a sample of 133 spatially resolved debris discs ›
Diverse stages of star formation in the IRAS 18162-2048 region. Emergence of UV Feedback ›
Determining the Detectability of H2O with Photometric Observations using Bayesian Analysis for Remote Biosignature Identification on exoEarths (BARBIE) ›
The shape-velocity alignment of satellites forged by tidal locking and dynamical friction ›
Spatial and Dynamical Relations between Spicules and Network Bright Points ›
Observability of eccentricity in a population of merging compact binaries ›
JWST TRAPPIST-1 e/b Program: Motivation and first observations ›
ZTF-SEDm Type Ia supernova sample for Twins Embedding spectrophotometric standardisation ›
A 43 day transiting Neptune and two 25 day Saturns from TESS, NGTS and ASTEP ›
Multi-Wavelength Afterglows as Diagnostic Probes of Dense Circumburst Medium in GRBs ›
X-ray Analysis of Gamma-Ray Burst Flares and Underlying Afterglows: Insights into Origin of Flares ›
The heartbeat of stellar halos: Insights from the stellar halo mass-metallicity relation ›
Microquasar remnants as hidden PeVatrons ›
Hot, Photoionized X-ray Gas in Two Luminous Type 2 Quasars: Chandra-HST Evidence for a Wind-Driven Sequence ›
DESI Strong Lens Foundry V: A Sample of HST-Observed Strong Lenses Modeled with GIGA-Lens ›
The phases of QCD reached in terrestrial and cosmic colliders ›
Widen the Resonance at Ultra-High Energies: Novel Probes of Neutrino Self-interactions in the High-Mass Regime ›
Possible $\nu$ Source Class: 3-sigma Detection of High-Energy Neutrinos from Supermassive Black Hole Binary Candidates ›
Quenching factors for Na recoils as a function of Tl dopant concentrations in NaI(Tl) crystals ›
A few ideas to promote inclusion ›
Investigating all-sky Frequency Hough performances for neutron stars ›
Apparent Phantom Crossing in Gauss-Bonnet Gravity ›
Constraining meV Axion Dark Matter with ALMA Observations of the Galactic Center Magnetar SGR 1745-2900 ›
Masked Autoencoder Pretraining on Strong-Lensing Images for Joint Dark-Matter Model Classification and Super-Resolution ›
Extreme mass ratio inspirals in the cold vector dark matter environment ›
Shock trapping and inertial escape: Dust-particle clustering in compressible turbulence ›
Genesis of Axion Dark Matter via Black Hole and Cosmic String Dynamics ›
Evaporation of Primordial Black Holes in a Thermal Universe: A Thermofield Dynamics Approach ›
Long-wavelength UV-LEDs and charge management in the detection of gravitational waves in space ›
A short review on joint weak and strong cluster lens-mass reconstruction ›
Signatures of Massive Black Hole Merger Host Galaxies from Cosmological Simulations II: Unique Stellar Kinematics in Integral Field Unit Spectroscopy ›
Galactokinetics ›
Probing Primordial Black Hole Formation from Domain Wall Isocurvature Perturbations: Constraints and Implications ›
Simulations of Shapiro, Gravitational, and Doppler time delays in pulsar networks for ultralight dark matter ›
Primordial Black Hole Formation from Power Spectrum with Finite-width ›
Micro-Tidal Disruption Events at Galactic Centers ›
Seasonal Variations of the Atmospheric Muon Neutrino Spectrum measured with IceCube ›
Gamma-ray Burst Empirical Correlation between Peak Luminosity and Peak Energy in The ICMART Model ›
Using Wavelet Decomposition to Determine the Dimension of Structures from Projected Images ›
Bridging Quasars and Little Red Dots: Insights into Broad-Line AGNs at $z=5-8$ from the First JWST COSMOS-3D Dataset ›
Axion Dark Matter Archaeology with Primordial Gravitational Waves ›
The Tantalizing Case of the Quasar J0950+5128 -- I. Presentation of the Data and Detailed Exploration of the Binary Supermassive Black Hole Scenario ›
Merger History of Clustered Primordial Black Holes ›
Black Hole - Neutron Star and Binary Neutron Star Mergers from Population III and II stars ›
Unveiling the small-scale web around galaxies with miniJPAS and DESI ›
Probing the peak of star formation with the stochastic background of binary black hole mergers ›
Characterization of the Cherenkov Photon Background for Low-Noise Silicon Detectors in Space ›
Cosmic Rays Masquerading as Cool Cores: An Inverse-Compton Origin for Cool Core Cluster Emission ›
The NANOGrav 15-year Data Set: Search for Gravitational Scattering of Pulsars by Free-Floating Objects in Interstellar Space ›
On the origins of oxygen: ALMA and JWST characterise the multi-phase, metal-enriched, star-bursting medium within a 'normal' $z > 11$ galaxy ›
SHELLQs-JWST perspective on the intrinsic mass relation between supermassive black holes and their host galaxies at z > 6 ›
Effective Phantom Divide Crossing with Standard and Negative Quintessence ›
Detecting False Positives With Derived Planetary Parameters: Experimenting with the KEPLER Dataset ›
Disformal interactions in the Dark Sector: From driving Early Dark Energy to confronting cosmological tensions ›
Quasi-Periodic Eruptions as a Probe of Accretion Disk in Tidal Disruption Events ›
The role of peculiar velocity uncertainties in standard siren cosmology ›
PRIMER & JADES reveal an abundance of massive quiescent galaxies at 2 < z < 5 ›
Disclosing Submillimeter Galaxy Formation: Mergers or Secular Evolution? ›
Magnetic White Dwarf - M Dwarf Binaries in Pre-mCV Phase as Special Population of Long-Period Radio Transients ›
Early Stages of Dusty Tori: The First Infrared Spectra from a Highly Multiscale Quasar Simulation ›
A Short Introduction to Cosmology and its Current Status ›
Understanding post-red giant branch binaries through stable mass transfer ›
Inferring Cosmological Parameters with Evidential Physics-Informed Neural Networks ›
Rare Transients in Nearby Galaxies Explain Ultra-high-energy Cosmic Rays ›
The JWST-NIRCam View of Sagittarius C. III. The Extinction Curve ›
Combining spectral analysis and narrow band pass filtering to predict solar cycle parameters in the next solar grand minimum ›
Assessing the Distance for Probing the Nuclear Equation of State with Supernova Gravitational Waves ›
XRISM Observations of The Prototypical Cold Front in Abell 3667 ›
jFoF: GPU Cluster Finding with Gradient Propagation ›
Igniting galaxy formation in the post-reionization universe ›
A Mass-Independent Damping Timescale in Black Hole Accretion Systems ›
Simultaneous detection of the size and velocity of the largest ejecta particles with velocities exceeding 1 km s$^{-1}$ ›
Accuracy and Applicability of the Hartle-Thorne and Komatsu-Eriguchi-Hachisu Methods for Modeling Rotating Neutron Stars ›
Effects of New Forces on Scalar Dark Matter Solitons ›
Hidden metallic iron in amorphous silicate dust? Insights from condensation experiments and mid-infrared spectroscopy ›
Projections of Earth's Technosphere: Strategies for Observing Technosignatures on Terrestrial Exoplanets ›
Spatial Phonons: A Phenomenological Viscous Dark Energy Model for DESI ›
OASIS Survey Direct Imaging and Astrometric Discovery of HIP 71618 B: A Substellar Companion Suitable for the Roman Coronagraph Technology Demonstration ›
SCExAO/CHARIS and Gaia Direct Imaging and Astrometric Discovery of a Superjovian Planet 3--4 lambda/D from the Accelerating Star HIP 54515 ›
Cosmology after Phantom Crossing by Horndeski Gravity ›
A three-dimensional model for the reversal in the local large-scale interstellar magnetic field ›
An Analysis of LIGO Glitches Using t-SNE During the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run ›
JWST Exoplanetary Worlds and Elemental Survey (JEWELS) I: High-Precision Chemical Abundances of 20 FGK Planet-Hosting Stars from JWST Cycle 2 ›
Absorption in the 21 cm Hydrogen Line at $z>10$ as a Sensitive Tool for the Construction of a Cosmological Model on Small Scales ›
Constraining the competition between the deconfinement and chiral phase transitions in light of the multimessenger era ›
Nuclear Production and Analytic Attenuation of Energetic MeV Solar Dark Matter ›
Gravitational Wave Mountains: current-carrying domain walls ›
Gravitational lensing by non-self-intersecting vortons ›
Axion forces in axion backgrounds ›
Insights into the highest natural scale: Finite naturalness challenges inflationary dynamics ›
Dark Walker in the Early Universe: A Strongly Coupled Sector Model ›
Model-agnostic gravitational-wave background characterization algorithm ›
Binary black hole population inference combining confident and marginal events from the $\tt{IAS\text{-}HM}$ search pipeline ›
Sterile neutrino dark matter from a TeV Scale Seesaw ›
A synchronization-free one-way ranging observable for detecting and characterizing coherent orbital-period systematics in GRACE-FO laser ranging data ›
Bayesian Analysis of the Complex Singlet Model with Phase Transition Gravitational Waves ›
Klein Bottle Cosmology ›
Large/small eddy simulations: A posteriori analysis in high Reynolds number isotropic turbulence ›
Quasinormal modes of a static black hole in nonlinear electrodynamics ›
Popcorn EMRIs: Transient Gravitational Wave Signals and Their Analysis in Schwartz Space ↓↑