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

Cloud

Rainfall

S Sky
Temperature
1.2 °C
Humidity
85%
Wind
6.4 km/h
Pressure
1014.8 hPa

Moon
Latest preprints on astro-ph:
›
How Dark is Dark Energy? A Lightcones Comparison Approach ›
COSMOS-3D: Two obscured X-ray AGNs with hot dust and He I$\lambda$10830 absorption at z~3 ›
Photon (Non)Conservation in the Reduced Speed of Light Approximation and How to (Almost) Fix It ›
The DREAMS Project: Disentangling the Impact of Halo-to-Halo Variance and Baryonic Feedback on Milky Way Satellite Galaxies ›
Discovery of two little red dots transitioning into quasars ›
Possible $\nu$ Source Class: 3-sigma Detection of High-Energy Neutrinos from Supermassive Black Hole Binary Candidates ›
JCMT Constraints on the Early-Time HCN and CO Emission and HCN Temporal Evolution of 3I/ATLAS ›
The Dependence of Earth Milankovitch Cycles on Martian Mass ›
Cosmic chronometers with galaxy clusters: a new avenue for multi-probe cosmology ›
Slow-Light Effect in the Jet-Launching Region of M87 ›
Image simulations of highly magnified clumpy galaxies ›
Determining the Milky Way gravitational potential without selection functions ›
Hidden in Plain Sight II: Characterizing the luminous companion to Kappa Velorum with VLTI/GRAVITY ›
VENUS: When Red meets Blue -- A multiply imaged Little Red Dot with an apparent blue companion behind the galaxy cluster Abell 383 ›
SEAMLESS Survey: Four Faint Dwarf Galaxies Tracing Low-Mass Galaxy Evolution Across Environments ›
Untangling the Sources of Abundance Dispersion in Low-metallicity Stars II: Neutron Capture Elements ›
Kinematics of young stellar objects in NGC 2024 based on infrared proper motions ›
A value-added catalogue of neural network-based europium abundances for GALAH DR4 ›
OASIS Survey Direct Imaging and Astrometric Discovery of HIP 71618 B: A Substellar Companion Suitable for the Roman Coronagraph Technology Demonstration ›
Ripples in the baryon to dark matter ratio in $\Lambda$CDM: implications for galaxy formation ›
Dynamo and Jet interconnections in GRMHD simulations of black hole accretion disks ›
Constraining the Occurrence of ZLK-Induced White Dwarf Pollution with Dissipative Precession ›
AT2022zod: An Unusual Tidal Disruption Event in an Elliptical Galaxy at Redshift 0.11 ›
Inefficient Circularization, Delayed Stream-Disk Interaction and Reprocessing: A Five-Stage Model for the Intermediate-Mass Black Hole Tidal Disruption Event EP240222a ›
SCExAO/CHARIS and Gaia Direct Imaging and Astrometric Discovery of a Superjovian Planet 3--4 lambda/D from the Accelerating Star HIP 54515 ›
Impact of Nuclear Reaction Rate Uncertainties on Type I X-ray Burst Nucleosynthesis: A Monte Carlo Study ›
High-Energy Extractions from Horizonless Compact Objects ›
Dynamics of Streamers and Pseudostreamers and Implications for the Solar Wind ›
$S^5$: Tidal Disruption in Crater 2 and Formation of Diffuse Dwarf Galaxies in the Local Group ›
Convective Heat Transport Asymptotic Law in an $\alpha^2$ dynamo model ›
Evolution of the Accretion Rate of Young Intermediate Mass Stars: Implications for Disk Evolution and Planet Formation ›
Evaluating the Prospects of Cyclic Deconvolution across 312 Pulsars ›
The SPHINX M dwarf Spectral Grid. II. New Model Atmospheres and Spectra to Derive Fundamental Properties of mid-to-late type M-dwarfs ›
Solitary Alfv\'en Waves ›
Driving mechanisms of solar active region geysers: The role of interacting magnetic flux ›
Observing binary neutron star subpopulations with the Einstein Telescope ›
How much gas and dust is in the $z=5.7$ Lyman Break Galaxy HZ10? An ALMA Band 10 to 4 and JWST/NIRSpec study of its interstellar medium ›
Segmented-Polynomial-fitting Least Squares (SPLS): An optimized algorithm to find Earth twins ›
Pad\'e Approximants for Fast Radio Bursts Diffuse Dispersion Measure ›
The first extragalactic ultra-compact X-ray binary : a candidate black hole-white dwarf system ›
"SNe Ia twins" in the Hubble flow, and the determination of H0 ›
High-Precision Amplitude-Modulated Continuous-Wave Lunar Laser Ranging ›
The exotic black hole-neutron star binaries in our Galaxy ›
Evolution and Mass Dependence of UV-to-near-IR Color Gradients up to z=2.5 from HST+JWST ›
Updates on dipolar anisotropy in local measurements of the Hubble constant from Cosmicflows-4 ›
The near-Sun Heliospheric Current Sheet, fluid and kinetic properties ›
Modeling Particle Acceleration and MWL Emission of a PeVatron Microquasar V4641 Sgr ›
Quantification of abundance uncertainties in chemical models of exoplanet atmospheres ›
A Statistical Analysis of Fluence and Energy Distributions of Non-repeating Fast Radio Bursts Detected by CHIME ›
Radio, X-ray, and EUV signatures of internal and external reconnection of an erupting flux rope ›
Stellar chemistry and planet size: insights from GALAH DR4 ›
Stranger Things: A Grid-based Survey of Strange Modes in Post-Main Sequence Models ›
Silicate emission in a type-2 quasar: JWST/MIRI constraints on torus geometry and radiative feedback ›
The role of the galaxy stellar mass function in determining the cosmological distribution of astrophysical transients with applications to fast radio bursts and merging binary black holes ›
KM3NeT/ARCA stacking search for high-energy neutrinos from blazars ›
Peculiar SN Ic 2022esa: An explosion of a massive Wolf-Rayet star in a binary as a precursor to a BH-BH binary? ›
Search for persistent radio emission towards selected localised Fast Radio Burst positions using the MeerKAT Telescope ›
Spectropolarimetric characterisation of exoplanet host stars in preparation of the $Ariel$ mission II. The magnetised wind environment of TOI-1860, DS Tuc A, and HD 63433 ›
SDSS-V LVM: Resolving Physical Conditions in the Trifid Nebula ›
Direct observational evidence that higher-luminosity type 1 active galactic nuclei are most commonly triggered by galaxy mergers ›
The Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey: Quasar Properties from Data Release 10 to 12 ›
VHE FSRQs with Fermi-LAT: VHE and even brighter states in high-z FSRQs due to an HBL-like component? ›
On Constraining the Proposed Hierarchical Triple Scenario for an Eccentric Milli-Second Pulsar Binary PSR J1618-3921 ›
Insights into Extragalactic Background Light constraints with MAGIC archival data ›
Distinguishing ram pressure from gravitational interactions: Applying the Size-Shape Difference method to real galaxies ›
The suppression of the matter power spectrum: strong feedback from X-ray gas mass fractions, kSZ effect profiles, and galaxy-galaxy lensing ›
The Composite Spectrum of QSO Absorption Line Systems in DESI DR2 ›
MIRI spectrophotometry of GN-z11: Detection and nature of an optical red continuum component ›
A new constraint on the $y$-distortion with FIRAS: implications for feedback models in galaxy formation and cosmic shear measurements ›
Effect of the avoided crossing on the rovibrational energy levels, resonances, and predissociation lifetimes within the ground and first excited electronic states of lithium fluoride ›
Linearly Polarized Gravitational Waves from Bubble Collisions ›
Properties of Stable Massive Quark Stars in Holography ›
Thermoelectric coefficients of two-flavor quark matter from the Kubo formalism ›
Exploring Leptogenesis, WIMP Dark Matter, and Gravitational Waves in an extended Scalar Framework ›
Quasinormal modes of a static black hole in nonlinear electrodynamics ›
Inflationary assessment of $F(\mathcal{R},\tilde{\mathcal{R}})$ Einstein-Cartan models ›
Limiting Reduction and Modified Gravity ›
Flexible Gravitational-Wave Parameter Estimation with Transformers ›
Singular $\alpha$-attractors ›
Modeling dark matter halos with self-interacting fermions ›
Topological Shell Structures in Neutron Stars: Effects on Equilibrium, Oscillations, and Gravitational-Wave Signatures ›
Neutron stars in $f(\mathbb{Q})$ gravity ›
WASP-39b: exo-Saturn with patchy cloud composition, moderate metallicity, and underdepleted S/O ›
The Case for Hot-Mode Accretion in Abell 2029 ›
Extremely luminous optical afterglow of an energetic gamma-ray burst GRB 230204B ›
Concept integral field unit spectrometer instrument for the next-generation mm-wave cosmological surveys ›
REBELS-IFU: Dust Build-up in Massive Galaxies at Redshift 7 ›
Feedback and dynamical masses in high-$z$ galaxies: the advent of high-resolution NIRSpec spectroscopy ›
Scaling relations, dynamical heating and tidal disruption in spin $s$ ultralight dark matter models ›
Probing the Distance Duality Relation with Machine Learning and Recent Data ›
Time-resolved spectro-polarimetric analysis of extremely bright GRB 230307A: Possible Evidence of evolution from photospheric to synchrotron dominated emission ›
Analyzing type Ia supernovae near-infrared light curves with Principal Component Analysis ›
Polarization Angle Orthogonal Jumps in Fast Radio Bursts ›
MINDS. Anatomy of a water-rich, inclined, brown dwarf disk: lack of abundant hydrocarbons ›
The fate of the progenitors of luminous red novae: Infrared detection of LRNe years after the outburst ›
Impact of magnetic field gradients on the development of the MRI: Applications to binary neutron star mergers and proto-planetary disks ›
Structure and Magnetic Field of the Bright-rimmed Cloud IC 1396E/SFO 38 ›
Dark Classification Matters: Searching for Primordial Black Holes with LSST ›
Planck Constraints on Axion-Like Particles through Isotropic Cosmic Birefringence ›
Low-metallicity massive single stars with rotation. III. Source of ionization and C-IV emission in I Zw 18 ›
A systematic search for dormant galaxies at z~5-7 from the JWST NIRSpec archive ›
A general polynomial emulator for cosmology via moment projection ›
Testing Photometric Techniques for Measuring the Rest-Frame UV Spectral Slope Against JWST PRISM Spectroscopy ›
Deep Learning Improves Photometric Redshifts in All Regions of Color Space ›
Dark energy constraints in light of theoretical priors ›
The Fate of Transonic Shocks around Black Holes and their Future Astrophysical Implications ›
Spatially resolved gas-phase metallicity at z~2-3 with JWST/NIRISS ›
XMAGNET : Kinetic, Thermal and Magnetic AGN Feedback in Massive Galaxies at Halo Masses $\sim 10^{13.5}$ M$_\odot$ ›
HD 44892: The youngest (or oldest?) gas-harbouring debris disc around an intermediate mass star ›
Radiation damage to the Hubble Space Telescope during two Solar cycles, and correction of Charge Transfer Inefficiency using ArCTIc ›
Macromodel-free flux-ratio prediction in quadruply imaged quasars with local constraints from lensed arcs ›
LIMFAST. IV. Learning High-Redshift Galaxy Formation from Multiline Intensity Mapping with Implicit Likelihood Inference ›
WIYN Open Cluster Study. XCVII. An Extended Radial-Velocity Survey and Spectroscopic Binary Orbits in the Open Cluster NGC 188 ›
Radiative hydrodynamic simulations of FIP fractionation in solar flares ›
SN 2025coe: A Multiple-Peaked Calcium-Strong Transient from A White-Dwarf Progenitor ›
No Observational Evidence for Dark Matter Nor a Large Metallicity Spread in the Extreme Milky Way Satellite Ursa Major III / UNIONS 1 ›
Multi-faceted light pollution modelling and its application to the decline of artificial illuminance in France ›
Formation of protostars and the launching of stellar core outflows with moving-mesh radiation non-ideal magnetohydrodynamics ›
On the Dusty Proximate Damped Lyman-{\alpha} System toward Q2310-3358 at z = 2.40 ›
Properties of Carbon-rich AGB Stars in the LMC and the Milky Way ›
Kinematic scaling relations of disc galaxies from ionised gas at $z\sim1$ and their connection with dark matter haloes ›
Low-energy Radio Bursts from Magnetar XTE J1810$-$197: Implications for Fast Radio Bursts ›
Kinematic Mapping of Giant Arcs: A New Method to Locate Lensing Critical Curves ›
On the planetary forcing of the Solar dynamo: Evidence from a Lagrangian framework ›
Sequential Convex Programming for Multimode Spacecraft Trajectory Optimization ›
Revisiting wideband pulsar timing measurements ›
The Milky Way stellar halo is twisted and doubly broken: insights from DESI DR2 Milky Way Survey observation ›
Holographic complexity and the Hubble tension: a quantum gravity portrayal for the large scale structure of the cosmos ›
The Dynamics of Reheating in Loop Quantum Cosmology ›
Superheavy dark matter from the natural inflation in light of the highest-energy astroparticle events ›
Equation of state and Fermi liquid properties of dense matter based on chiral effective field theory interactions ›
Precision predictions of Starobinsky inflation with self-consistent Weyl-squared corrections ›
Gravitational scattering of two neutron stars ›
MaxWave: Rapid maximum likelihood wavelet reconstruction of non-Gaussian features in gravitational wave data ›
Eccentricity evolution consistency test to distinguish eccentric gravitational-wave signals from eccentricity mimickers ›
The Great Impersonation: $\mathcal{W}$-Solitons as Prototypical Black Hole Microstates ›
Chaotic Inflation RIDES Again ↓↑