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

Cloud

Rainfall

S Sky
Temperature
5.7 °C
Humidity
84%
Wind
4.8 km/h
Pressure
1012.4 hPa

Moon
Latest preprints on astro-ph:
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Controlled Tension Forecasting: Quantifying Cross-Probe Biases in $\omega_0\omega_a$CDM ›
Pleiades Binary Fraction Revisited ›
Minuet: A Diffusion Autoencoder for Compact Semantic Compression of Multi-Band Galaxy Images ›
The evolutionary history of ultra-compact accreting binaries. I. Chemical abundances and formation channel of the eclipsing AM CVn system ZTF J225237.05-051917.4 from HST spectroscopy ›
Resolving the terrestrial planet-forming region of HD 172555 with ALMA: I. Post-impact dust distribution ›
Testing warm dark matter with kinematics of the smallest galaxies ›
The DREAMS Project: Disentangling the Impact of Halo-to-Halo Variance and Baryonic Feedback on Milky Way Dark Matter Speed Distributions ›
Tighter constraints on the atmosphere of GJ 436 b from combined high-resolution CARMENES and CRIRES$^+$ observations ›
Galactic bars are already mature at Cosmic Noon: bar strength and flatness at z ~ 1.5 ›
JWST Confirmation of a Runaway Supermassive Black Hole via its Supersonic Bow Shock ›
Eight New Ultramassive Black Hole Masses confirm Best Correlation with Galaxy Core Sizes ›
The dispersion in pulsar $\gamma$-ray efficiency ›
A bottleneck for star formation: the importance of magnetic fields during the formation of cold gas in galaxies ›
Fractal Aggregate Aerosols in the Virga Cloud Code II: Exploring the Effects of Key Cloud Parameters in Warm Neptune, Hot Jupiter and Brown Dwarf Atmospheres ›
Stellar Bars in Jellyfish Galaxies: Statistical Insights into the Combined Role of Bars and Environment ›
Primordial Black Holes from Inflation with a Spectator Field ›
Warped & Hooked: Mapping the Magellanic Clouds in 3D using Red Clump stars ›
The impact of strong feedback on galaxy group scaling relations ›
Machine Phenomenology: A Simple Equation Classifying Fast Radio Bursts ›
A Black-Hole Envelope Interpretation for Cosmological Demographics of Little Red Dots ›
Confronting cosmic shear astrophysical uncertainties: DES Year 3 revisited ›
LEBS Toolkit for Addressing Development Challenges through Astronomy ›
Separating flare and secondary atmospheric signals with RADYN modeling of near-infrared JWST transmission spectroscopy observations of TRAPPIST-1 ›
Reanalyzing DESI DR1: 3. Constraints on Inflation from Galaxy Power Spectra & Bispectra ›
The DESI Single Fiber Lens Search. I. Four Thousand Spectroscopically Selected Galaxy-Galaxy Gravitational Lens Candidates ›
A review on fundamental bounds and estimators for photometry and astrometry of celestial point sources using array detectors, from first principles ›
A distance measurement for blazar TXS 0506+056 using its radio variability and very long baseline images ›
An Analysis of a Coronal Mass Ejection Leading Edge by Means of Multi-Spacecraft-in-Beam Phase Scintillation ›
Asymptotic constraints for 1D planar grey photon diffusion from linear transport with special-relativistic effects ›
Solar Cycle Variation of Sustained Gamma Ray Emission from the Sun ›
ELG$\times$LRG distribution through dark matter halo dynamics ›
Design and dynamics experiment of filter wheel mechanism of space coronagraph ›
Mini-supernovae from white dwarf-neutron star mergers: Viewing-angle-dependent spectra and lightcurves ›
JWST Exoplanetary Worlds and Elemental Survey (JEWELS) I: High-Precision Chemical Abundances of 20 FGK Planet-Hosting Stars from JWST Cycle 2 ›
The Binary Fraction of Stars in the Dwarf Galaxy Ursa Minor via Dark Energy Spectroscopic Instrument ›
Chlorine and Potassium Enrichment in the Cassiopeia A Supernova Remnant ›
A Morpho-kinematic Study of Galactic High-ADF PNe Based on the VLT/UVES Deep Spectroscopy ›
Constraining regular primordial black holes with isocurvature gravitational waves ›
Towards Baikal-Top: Feasibility study of an onshore detector system for the joint registration of EAS with Baikal-GVD ›
Investigating the H i mass-size relation using the Simba cosmological simulations ›
The role of distant pulsars in the detectability of continuous gravitational waves ›
The dynamical memory of tidal stellar streams: Joint inference of the Galactic potential and the progenitor of GD-1 with flow matching ›
The GAPS programme at TNG LXXI. HD 128717 B/Gaia-6 B: a long-period eccentric low-mass brown dwarf from astrometry and radial velocities ›
Connections between the cycle-to-cycle light curve and O-C variations of the Blazhko RR Lyrae stars ›
Characterizing the Low-Mass Pre-Main-Sequence Population in the Low-Metallicity Star-Forming Region Dolidze 25 Using VLT-MUSE ›
Velocity Dispersion Functions of Pressure-supported Galaxies in EAGLE Simulations with Varying AGN Feedback ›
Progress towards a microchannel plate detector with AlGaN photocathode and cross-strip anode for ultraviolet astronomy ›
FAUST XXIX. OCS line emission: a new method for measuring the luminosity of embedded protostars in binary systems ›
A Chandra view of SPT-CL J0217-5014: a massive galaxy cluster at a cosmic intersection at z=0.53 ›
The ejection velocities of interstellar objects signpost their progenitor system architectures ›
On the magnetic field evolution of interplanetary coronal mass ejections from 0.07 to 5.4 au ›
ALMA-QUARKS: Few-Thousand-Year Hatching out of "Egg": The Supersonic Breakout of a Hypercompact H II Region from Its Parental Hot Core ›
Formation of the Dormant Black Holes with Luminous Companions from Binary or Triple Systems ›
287,872 Supermassive Black Holes Masses: Deep Learning Approaching Reverberation Mapping Accuracy ›
Unveiling gravitational waves from core-collapse supernovae with MUSE ›
Spaceflight KID Readout Electronics for PRIMA ›
Long-term X-ray variability of the multiple-planet host L 98-59: Hints of an activity cycle ›
aim-resolve: Automatic Identification and Modeling for Bayesian Radio Interferometric Imaging ›
The MALATANG survey: star formation, dense gas, and AGN feedback in NGC 1068 ›
Probing TeV Afterglow Emission of GRB~221009A with Gaussian Structured jet in Wind-driven medium ›
Local mixing length theory with compositional effects:\ First application to asymptotic giant branch evolution ›
Long-term Mid-infrared Color Variations of Narrow-Line Seyfert 1 Galaxies ›
Oxygen Isotope Constraints on the Importance of Photochemical Processing in Protoplanetary Disks ›
MALLORN: Many Artificial LSST Lightcurves based on Observations of Real Nuclear transients ›
Intertwined birth and death: a Herbig-Haro outflow resolves the distance to Vela Junior ›
Internal superfluid response and torque evolution in the giant glitch of PSR J1718-3718 ›
Inflationary relics from an Ultra-Slow-Roll plateau ›
The critical role of clumping in line-driven disc winds ›
Spectrum and anisotropies of Galactic cosmic rays: a laboratory for magnetic fields ›
Probing AGN Feedback in Dwarf Galaxies with Spatially Resolved NIR Coronal Lines from JWST ›
Dust destruction by the supernova remnant forward shock in a turbulent interstellar medium ›
The position and resolvability of blended point sources ›
Line-of-sight shear in SLACS strong lenses II: validation tests with an extended sample ›
Sensitivity of Hongmeng 21cm experiment on scattering dark matter ›
Improving Posterior Inference of Galaxy Properties with Image-Based Conditional Flow Matching ›
Resolving the molecular gas emission of the z~2.5-2.8 starburst galaxies SPT0125-47 and SPT 2134-50 ›
Highly-ionized gas in lensed z = 6.027 Little Red Dot seen through [OIII] 88$\mu$m with ALMA ›
PSR J0952-0607: Tightening a Record-High Neutron Star Mass ›
The spectrum of $n_s$ constraints from DESI and CMB data ›
Searching for EeV photons with Telescope Array Surface Detector and neural networks ›
Responsible Discovery in Astrobiology: Lessons from Four Controversial Claims ›
Questions related to the Deflection of Light by Gravity determined by Soldner, Einstein and Schwarzschild ›
A new connection between WIMP dark matter and the hierarchy problem ›
Popcorn EMRIs: Transient Gravitational Wave Signals and Their Analysis in Schwartz Space ›
Electroweak phase transition in SMEFT: Gravitational wave and collider complementarity ›
Inflation with a Growing Fifth Dimension ›
Nucleon Short-Range Correlations and High-Momentum Dynamics: Implications on the Equation of State of Dense Matter ›
Z' portal dark matter from post-inflationary reheating: WIMPs, FIMPs, and UFOs ›
Gravitational Waves from Isocurvature Perturbations of Spectator Scalar Fields ›
A simple procedure for generating a Kappa distribution in PIC simulation ›
Linear stability of nonrelativistic Proca stars ›
On angular dependent response to gravitational-wave signals for time-delay interferometry combinations ›
A Quarkyonic Quark-Meson Coupling Model for Nuclear and Neutron Matter ›
Searching for binary black hole mergers with deep learning in Advanced LIGO's third observing run ›
Extreme-Mass-Ratio Inspirals Embedded in Dark Matter Halo II: Chaotic Imprints in Gravitational Waves ›
Detecting relativistic black hole collisions near a massive black hole ›
Adaptive Optics-Enhanced Michelson Interferometer for Spectroscopy of Narrow-Band Light Sources ›
Constraints on Genesis Cosmology from the Smeared Null Energy Condition ›
Thermodynamics vs Teleodynamics: A Cosmological Divide? ›
Geophysical intensity problems: the axisymmetric case ›
On the treatment of thermal effects in the equation of state on neutron star merger remnants ›
Resonant neutrino self-interactions and the $H_0$ tension ›
Mapping Dark Matter in the Milky Way using Normalizing Flows and Gaia DR3 ›
Sweeping the Dust Away - Correcting the Phase Space Density of the Milky Way with Unsupervised Machine Learning ›
Modeling APOKASC-3 red giants: I. The first dredge-up and red giant branch bump ›
Line-of-sight shear in SLACS strong lenses I: shear and mass model parametrisations ›
Progenitor Dependence of Neutrino-driven Supernova Explosions with the Aid of Heavy Axion-like Particles ›
Unveiling the Coma Cluster Structure: From the Core to the Hubble Flow ›
Gaia FGK Benchmark Stars: spectral library, metallicities and abundances of $\alpha$ and Fe-peak elements of the third version ›
Type Ia supernova growth-rate measurement with LSST simulations: intrinsic scatter systematics ›
Viability of general relativity and modified gravity cosmologies using high-redshift cosmic probes ›
Power Spectrum Emulators from Neural Networks and Tree-Based Methods ›
Resonant neutrino self-interactions: Insights from the full shape galaxy power spectrum ›
Global magnetohydrodynamic simulations of the inner regions of protoplanetary discs. I. Zero-net flux regime ›
A Virgo Environmental Survey Tracing Ionised Gas Emission (VESTIGE). XIX. The discovery of a spectacular 230 kpc Halpha tail following NGC 4569 in the Virgo cluster ›
Continued radio observations of the persistent radio source associated with FRB20190520B provides insights into its origin ›
Semi-empirical Framework of Supermassive Black Hole Evolution: Highlighting a possible tension between Demographics and Gravitational Wave Background ›
One-Loop Galaxy Bispectrum: Consistent Theory, Efficient Analysis with COBRA, and Implications for Cosmological Parameters ›
PSR J0614-3329: A NICER case for Strange Quark Stars ›
Memoirs of mass accretion: probing the edges of intracluster light in simulated galaxy clusters ›
JWST/NIRSpec Observations of Salacia-Actaea and M\'ani: Exploring Population-level Trends among Water-ice-rich Kuiper Belt Objects ›
Silane-Methane Competition in Sub-Neptune Atmospheres as a Diagnostic of Metallicity and Magma Oceans ›
What is the most massive gravitational-wave source? ›
Rotating twisted magnetosphere of magnetars: approximate analytical solutions ›
Cislunar Resonant Transport and Heteroclinic Pathways: From 3:1 to 2:1 to L1 ›
Exploring dark matter with quantum-enhanced haloscopes and time projection chambers ›
Star Formation under a Cosmic Microscope: Highly magnified z = 11 galaxy behind the Bullet Cluster ›
Turbulence and dust fragility in protoplanetary discs ›
Vz-GAL: Probing Cold Molecular Gas in Dusty Star-forming Galaxies at z=1-6 ›
Testing new-physics scenarios with the combined LHAASO and Carpet-3 fluence spectrum of GRB 221009A: axion-like particles and Lorentz-invariance violation ›
GALACTICNUCLEUS: A high angular resolution JHKs imaging survey of the Galactic centre. V. Toward the GNS Second Data Release: Methodology, Photometric and Astrometric Performance ›
Detecting Population III Gamma-Ray Bursts with Einstein Probe and Space-Based Multi-band Astronomical Variable Objects Monitor ›
Solar flare forecasting with foundational transformer models across image, video, and time-series modalities ›
Galaxy Spin Alignment with Tidal Fields in the SDSS-IV MaNGA Survey ›
Finite Lifetime Fragment Model 4 for Striae Formation in the Dust Tails of Comets (FLM 4) Acceleration by Lorenz-force ›
Numerical implementation of flat FLRW models of cosmic expansion with Planck 2018 cosmological parameters ›
The Dependence of Earth Milankovitch Cycles on Martian Mass ›
VENUS: When Red meets Blue -- A multiply imaged Little Red Dot with an apparent blue companion behind the galaxy cluster Abell 383 ›
Enhanced magnetostrophic waves with magnetic field orthogonal to the rotation axis ›
An Ancient Descendant of the First Galaxies ›
Statistical and Temporal Analysis of Multi-component Burst-clusters from the Repeating FRB 20190520B ›
Tracing the Cosmic Evolution of the Cool Circumgalactic Medium of Luminous Red Galaxies with DESI Year 1 Data ›
The Importance of Heat Flux in Quasi-Parallel Collisionless Shocks ›
Long-living Equilibria in Kinetic Astrophysical Plasma Turbulence ›
Investigating the competition between the deconfinement and chiral phase transitions in light of the multimessenger observations of neutron stars ›
Supercooled Audible Axions ›
From Capture to Collapse: Revisiting Black Hole formation by Fermionic Asymmetric Dark Matter in Neutron Stars ›
Constraints on cosmological parameters and CMB first acoustic peak in conformal Killing gravity ›
Extraction of neutron-capture cross sections on $^{92}$Zr using the charge-exchange Oslo method ›
Natural inflation in Palatini $F(R)$ ↓↑