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

Cloud

Rainfall

S Sky
Temperature
0.5 °C
Humidity
83%
Wind
0.0 km/h
Pressure
1025.3 hPa

Moon
Latest preprints on astro-ph:
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From Early Concepts to Lunar Hypertelescopes Roadmap for Next-Generation Optical Astronomy on the Moon ›
From Earth's Harshest Landscapes to Lunar Horizons: Engineering NEA Telescopes for Extreme Environments ›
HLA-Net: A Physics-Guided Skeleton-Based Framework for Automatic Gravitational Arc Detection in Astronomical Images ›
The PAU Survey: Self-supervised image denoising for flux-preserving photometry ›
Brewing another binary in the Teapot: Nandou=Phi Sagittarii ›
Characterizing Gravitational Wave Electromagnetic Counterparts with the Schmidt Observatory System ›
How sky subtraction scales affect Intracluster light measurements ›
CosmoVerse Data Challenge: How Tip of the Red Giant Branch Analysis Choices Shape the Inferred Hubble Constant ›
Searching for Signatures of i-process Nucleosynthesis in Metal-Rich, Lead-rich Barium Stars ›
Dynamics of self-gravitating halos with decaying dark matter ›
CHEX-MATE: Density profile reconstruction in galaxy clusters ›
Euclid. Predicting scaling relations for emission-line galaxies using simulated data ›
Euclid: Forecasting the number counts of bright line emitters in the Euclid Wide Survey and Euclid Deep fields ›
The M87 Black Hole Mass from JWST and Keck Stellar Kinematics Spanning 10 pc to 10 kpc ›
A pocket of oxygen in a near-pristine galaxy at z=4.2: chemical inhomogeneity at 10-parsec scales in LAP2 ›
She Sees Shells by the Stellar Shore: A Kinematic View of NGC 253's Stellar Halo ›
ReveaLLAGN 2: Exploring the Nuclear Gas and Stellar Kinematics of Nearby LLAGNs with JWST/NIRSpec IFU ›
Gravitational waves flooding the Universe after wall domination ›
Fast and accurate false-alarm probabilities for linear detection statistics in Poisson noise ›
DESI DR2 Results III: The Mass of the Milky Way ›
Mock catalogues for the DESI DR2 Milky Way mass modeling effort ›
Constraining the Milky Way Mass profile with data driven distribution function using DESI DR2 halo stars ›
A distribution-function estimate of the Milky Way mass profile from outer halo stars in DESI DR2 ›
On the Detectability of Compact Multi-Planet Systems via Gravitational Microlensing ›
Identifying Compact Object Candidates using Gaia DR3 Astrometric Accelerations and Jerks ›
Revisiting the Stellar-Dynamical Mass of the Central Black Hole in NGC 3227 ›
An obstruction to cosmic acceleration from shift-symmetric dark sector interactions ›
PrimordialPy: A Python library for single-field inflation, primordial black holes, and scalar-induced gravitational waves ›
The impact of Population III stars on the elemental enrichment of ultra-faint galaxies in the FIRE-3 zoom-in simulations ›
One gravitational function across matter phases: compatibility and interface constraints in static $f(R,T)$ gravity ›
The spatial structure of solar magnetoconvection at scales up to $60$~Mm ›
A high-frequency turnover in the persistent radio source of FRB20201124A ›
Observational Test of the Maximum-Entropy Conjecture for Black-Hole Mergers with GW250114 ›
Constraining Ganymede's Interior Structure and Bulk Composition from Its Present-Day Magnetic Field Strength ›
The impact of M dwarf stellar convection on exoplanetary atmospheric signatures. A 3D radiation-hydrodynamics simulation analysis for high-resolution spectroscopy ›
How fast is the fastest-rotating O-type star in the Galaxy? ›
Insights on the mass composition of ultrahigh-energy cosmic rays from small-scale anisotropy with large-scale structure simulations ›
Unsupervised Neural Operators for Rotating Relativistic Stars: High-Fidelity Equation of State Inference and Pulsar Spin Evolution at Scale ›
A Laplace-Transform Green's Function for Two-Zone Diffusion with Energy Losses: Application to the Geminga Pulsar Halo ›
Photometric Study of a Distant SU UMa-type Dwarf Nova KSP-OT-201803a ›
Polarimetry with the Giant Magellan Telescope: A Scientific Justification & Technical Requirements Document ›
Mock CSST NUV-NIR imaging of TNG50 galaxies with resolved stellar populations ›
The kinematic Kelvin-Helmholtz instability-driven dynamo: implications for merging compact objects ›
Frequent Optical Flares in an M-type Detached Eclipsing Binary TIC 349005337 ›
Collective Characterization of Polar Crown Filament Eruptions ›
Tiny Quiet-Sun EUV Ejections Revealed by High-resolution Multiwavelength Observations ›
Gravitational-Wave Microlensing as a Probe of Compact Object Population ›
Longitudinal-field particle acceleration in channels generated by strong electromagnetic waves in pair plasma ›
Orbital Architecture of Super-Earth-Cold-Jupiter Systems from Transit Duration Ratios ›
Spectroscopic diagnostics of coronal fan loops using EIS/Hinode and AIA/SDO ›
Spectroscopy-informed Deep Learning Searches for Photometric Little Red Dots in JWST Surveys ›
Aperture-dependent [O III] profile variability: Clues to the nature of double-peaked narrow emission lines ›
Pushing the frontiers of low-frequency radio astronomy: An ultra-deep sub-arcsecond LOFAR image of ELAIS-N1 ›
Evolutionary Map of the Universe (EMU): Selection of active galactic nuclei and star-formation emission with machine-learning techniques ›
Orientation of the spin axes of large Kuiper belt bodies as an indicator of the mechanism of their origin ›
Optical linear polarization of the Be--X-ray pulsar binary LS V +44 17 ›
A brief overview of the baryon cycle in galaxies ›
A search for sterile neutrinos at ultrahigh energies at the Pierre Auger Observatory ›
Euclid: Survey mask effects on clustering of galaxy clusters ›
Primordial Black Holes and Induced Gravitational Waves from Inflation with History-Dependent Effective Dissipation ›
Horndeski Gravity as an Effective Dark Energy Fluid in Cosmological N-body Simulations ›
Quiescent galaxies at cosmic noon: from individual element abundances to star formation histories ›
Developing the Field Selector System for the SHARP Multi-IFU: Optomechanical Design and First Prototype Validation ›
Understanding galaxies and the origin of the golden mass through the study of scaling relations across cosmic history ›
Supermassive black holes and nuclear star clusters in galaxies: constraining formation and co-evolution with SHARP and MICADO ›
SHARP: A spectrograph proposal to fully exploit ELT capabilities ›
The Environment of High-Energy Transient Host Galaxies at High Redshifts as Observed by SHARP ›
Net Cooling Tables for Cosmological Simulations under Multiple UV/X-ray Background Models ›
Planting neutrino SE-EdS: A < 3% accurate clustering approximation for neutrinos and other hot dark matter ›
AGN Host Galaxies in COSMOS-Web: Linking Structural Evolution and Star Formation Quenching up to $z=5$ ›
Object-independent evaluation of small-data astronomical image classifiers: architecture, representation, and acquisition shortcuts ›
Gaia DR3 Reveals the Kinematics of Young Stellar Objects in the Carina Nebula: Peripheral Expansion and Central Rotation ›
Primary and Secondary Star Formation in the Spiral Waves of NGC 628 ›
The dwarf galaxy NGC 185: the flagship of Andromeda's dwarf galaxies for the study of evolved multiple stellar populations ›
Magnetism among the oldest white dwarfs in the solar neighbourhood ›
Population synthesis of substellar companions surviving common-envelope evolution ›
Living near filaments: How environment shapes age profiles in low-mass galaxies ›
APOLLO-Timing: Annealed Phase - Orbit Lattice Linking across Observations for Binary Pulsar Timing ›
Investigating the initial conditions of globular clusters via $N$-body simulations: I. half-mass radius and stellar density ›
The formation and evolution of Wolf-Rayet stars with temperature-dependent winds ›
Euclid Quick Data Release (Q1). Refining the strong lens sample with Space Warps crowd-sourced science ›
Adaptive Optics for the Extremely Large Telescope: overcoming Point Spread Function challenges with MORFEO ›
Probing Solar-Wind Structure During Crab Pulsar Conjunctions with Dispersion and Faraday Rotation ›
Can Magnetic Reconnection Accelerate Energetic Particles in the Heliosheath? ›
Energetic Nonthermal Electrons within the Above-the-looptop Regions in Solar Flares: Acceleration, Feedback, and Quasi-Periodic Pulsations ›
Migration and eccentricity damping timescales in overstable resonant planetary systems: hydrodynamic and N-body simulations ›
Constraining the white-dwarf mass in the intermediate polar IGR J17014-4306 using X-ray and optical spectroscopy ›
Cosmological Backreaction and the Separate Universe Conjecture: Dynamical volume partitioning of Newtonian cosmologies ›
Magnetic Properties of Galactic Molecular Clouds ›
Magnetohydrodynamics During Reheating ›
Tracking turbulence for wind-driven halo removal using MagAO-X pyramid wavefront sensor images ›
Preparing for the Gaia DR4 Epochalypse: Simulated Epoch Astrometry for Substellar Companion Orbit-Modeling Benchmarks ›
ReveaLLAGN 3: Revealing the Infrared Spectral Energy Distributions of Low Luminosity AGN ›
Shining LIMelight into the dark: Probing Dark matter - baryon interactions with Line Intensity Mapping ›
Estimating LuSEE-Night's Sensitivity to C{\alpha} Radio Recombination Lines ›
The Start Time of Ringdown ›
The Cosmology of Hawking Axions ›
Spacetime Evolution Induced by a Massive Cosmic String in Numerical Relativity ›
Inflationary attractors in metric-affine gravity ›
Near-Quantum-Limited Readout for the Princeton Axion Search using a sub-GHz Kinetic Inductance Traveling Wave Parametric Amplifier ›
Gravitational-Wave Constraints on $R^2$ Gravity ›
QUIJOTE scientific results -- XVIII. New constraints on the polarization of the Anomalous Microwave Emission in bright Galactic regions: $\rho$\,Ophiuchi, Perseus and W43 ›
Hard X-ray/Soft gamma-ray Laue Lenses for High Energy Astrophysics ›
Wide Area VISTA Extragalactic Survey (WAVES): Redshift-limited selection of targets for the Wide survey using decision-tree classification ›
Euclid: Modelling observational effects in cluster counts and cluster clustering ›
A Smooth Transition from Giant Planets to Brown Dwarfs from the Radial Occurrence Distribution ›
The Space-Based Time-Domain Revolution in Astrophysics ›
Inside the cocoon: a comprehensive explanation of the spectra of Little Red Dots ›
Investigating the Circumnuclear Medium of Tidal Disruption Events with Radio Observations ›
Axionlike dark-matter winds driven by galactic baryon redistribution ›
Accretion-powered flares from black hole-disk collisions in galactic nuclei ›
Paschen Jumps in Little Red Dots: Evidence for Nebular Continua ›
Einstein-Cartan pseudoscalaron inflation, reheating and nonthermal leptogenesis ›
Clumps in a Cocoon: Geometry and Mixing Set the Universal X-ray to H$\alpha$ Surface Brightness Ratio ›
MusE GAs FLOw and Wind (MEGAFLOW) XIV: Background-Galaxy Absorption Reveals Kiloparsec-Scale Structure in the Cool Circumgalactic Medium ›
IceCube Real-time Searches for High-energy Neutrinos Coincident with LIGO/Virgo/KAGRA Gravitational-Wave Alerts in O4a ›
Revisiting the Lyth bound constraints on inflation from ACT DR6 results ›
Effect of tidal gravity and planetary rotation on the retrieved atmospheric abundances of close-in exoplanets ›
Morpho-kinematic of galaxies at cosmic noon ›
SHARP -- A spectrograph proposal to fully exploit ELT capabilities and look beyond JWST ›
A new era for Dual AGN science with SHARP ›
A SHARP Look at Quenching and Bulge-Disk Growth in Massive Galaxies at Cosmic Noon ›
Probing IMF Variations in High-Redshift Early-Type Galaxies with SHARP ›
Fast Graph-based Higher-Order Clustering Statistics on the GPU ›
Inferring Properties of Rotating Core-Collapse Supernovae with Gravitational-Wave Detector Networks ›
A unified modeling of X-ray and gamma-ray spectro-polarimetric data: the case of Cygnus X-1 ›
Gemini and Apache Point Multi-band Optical Imaging Characterization of Fragmenting Long-period Comet C/2025 K1 (ATLAS) ›
Moment-based formulas for the transport coefficients ›
Composition gradients in sub-Neptunes: K2-18 b and TOI-270 d as case studies ›
Probing the dynamics of extreme galaxies I. Dark matter content in ultra-diffuse galaxies ›
Stellar bar occurrence in TNG50 and TNG100: disentangling environmental effects and assembly history at z = 0 ›
A derived evolution of dark energy from cosmic inhomogeneity confronted with baryon acoustic oscillations and type Ia supernovae ›
Correlated Signatures of Plasma Lensing in Fast Radio Bursts ›
TOI-6981 b: a transiting sub-Neptune at the water ice line ›
An ALMA sub-kiloparsec test of the Kennicutt--Schmidt relation in a strongly lensed dusty star-forming galaxy at $z\sim2.78$ ›
Boosted Odds: Lower-Point Probes of Parity Violation with Momentum Fields ›
Experimental evidence for a physical alteration of fine regolith on near-Sun asteroids ›
A breath of fresh air: Oxygen enhancement from silicate sublimation during early protostellar evolution ›
Beyond the Disc--Spheroid Dichotomy at $0.6 < z < 8.0$: Evidence for a Morphological Indeterminacy Regime from JWST ›
MACE: Multigroup-Multiangle Integrated Thermal Compton Scattering Kernel ›
Unveiling the nonthermal environments of NGC 3411 and NGC 5903 through new MeerKAT observations ›
Small-Scale Magnetic Fields of Hyades M Dwarfs: Evolution with Age from the Pleiades to Field Stars ›
Up in smoke: carbon-destruction in the terrestrial planet-forming region of a young Class I disk ›
Missing Outer Rings in the exoALMA Sample: Physical Mechanisms Suppressing Dust Ring Formation Despite Strong Pressure Bumps ›
Online learning of subgrid-scale models for quasi-geostrophic turbulence in planetary interiors ›
Direction-of-arrival estimation of a gravitational wave by correlations between quadrupole moments of pulsar timing data ›
Cosmologically viable non-polynomial quasi-topological gravity: explicit models, $\Lambda$CDM limit and observational constraints ›
Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM ›
Tachyonic Encore: A universal shift of inflationary observables ›
Primordial Black Holes from Vector-Induced Curvature Perturbations Sourced by Primordial Magnetic Fields ›
Stable Ballistic Prograde Cyclers in the Three-Body Problem ›
Precision Solar System Dynamics for Ultralight Dark Matter Search ›
Gravitational Wave Birefringence in generalized Palatini Chern Simons ›
Neutron star cooling with medium-modified Urca rates ›
IceCube data for astrophysical neutrinos exhibit q-statistical behavior ↓↑