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 from south-east

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Temperature
4.2 °C
Humidity
93%
Wind
0.0 km/h
Pressure
1011.4 hPa

Moon
Latest preprints on astro-ph:
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Interpretation of Nanohertz Gravitational Waves via Cosmic Strings in Post-BBN Matter and Kination Domination ›
Kinematic and Dynamical Properties of Solar Neighborhood White Dwarfs from SDSS DR19 and Gaia DR3 ›
Global and Local Infall in the ASHES Sample (GLASHES). III. Physical Parameters of Contracting Motion onto Dense Cores in 70 $\mu$m Dark Massive Clumps ›
Primordial black holes as a natural consequence of scale-invariance ›
Exemplary Merging Clusters II: XMM-Newton and Chandra X-ray Observations of MACS J1752.0+4440 and ZwCl 1856.8+6616 ›
Wind-Fed Magnetic Flux and the Emergence of X-ray Coronae in Active Galactic Nuclei ›
A Multi-dimensional Analysis of the Open Clusters NGC 2423 and NGC 2482 with Gaia DR3 ›
Neutrino flavor conversion alters the lepton-emission self-sustained asymmetry in core-collapse supernovae ›
Cosmic Duets II. Growth and accretion in Gaia Multi-Peak dual AGN at Cosmic Noon ›
Discovery of a Nearby Ultra-fast Magnetic White Dwarf Propeller: Common Pathways to Magnetic Cataclysmic Variables ›
Accreting Neutron Stars in Low-Mass X-ray Binaries ›
The Origin of the Fermi Halo-like Emission: A New Model of the Fermi Bubbles ›
A "universal" supernova efficiency to drive the HI turbulence in nearby star-forming galaxies ›
Atypical White Dwarfs in Open Clusters ›
EK Cha b: multi-tracer detection of a protoplanet candidate in a gas-rich environment ›
Prevalence of radio Active Galactic Nuclei in galaxy groups since z=3.5 in the COSMOS-Web field ›
NGC 4936: abundant multi-phase medium in the central weak X-ray cool core and optically dark H I clouds in the group ›
First uGMRT Constraints on Rotation Measure in the Radio-Quiet Seyfert Galaxy NGC 4235 ›
Descalarization bursts from Galactic supramassive neutron stars: a kHz continuous-wave target ›
Population II Post-AGB Stars. I. Methodology, Initial Results, and the First Luminosity Function ›
Feedback-Conditional 3D Reconstruction of Cosmic Baryons with Flow Matching ›
Primordial black holes ›
Pushing Variability Searches to Extreme Dwarf Galaxies with the Vera C. Rubin Observatory Data Preview 2 ›
Microwave Loss in Low-Temperature ICPCVD Silicon Nitride: Dependence on Precursor Ratio and RF Substrate Bias ›
Debiasing Local Cluster Infall Reveals $\boldsymbol{H_0}$: Application to the Virgo Cluster ›
The progenitor galaxies of the intracluster light ›
Shortening the Baseline: Characterising Type Ia Supernovae Using $\Delta m_{10}(X)$ ›
Systematic non-compliance of satellite megaconstellations with IAU brightness limits ›
Mass Proxy Quality of Halo Properties in IllustrisTNG and FLAMINGO Simulations: II. Galaxies, Stars, and Black Holes ›
Understanding how Coronal Heating and Magnetic Field Scaling Affect Global Properties of the Low and Middle Corona ›
Stochastic Snowball States in Planetary Climate ›
The conditional colour-magnitude distribution: III. A study of galaxy colour- and luminosity-dependent counts-in-cells statistics ›
Central stellar depletion in the Draco dwarf from Subaru photometry ›
Flux Dependence of the 1\,keV Soft X-ray Feature in SAX J1808.4-3658 with \textit{NICER} ›
DeepDISC on LSST Data Preview 1: Scene-Level Detection, Deblending, and Star/Galaxy Classification in the ECDFS and EDFS Fields ›
NGC 6426: Colour-Magnitude diagram and variable star population as indicators of metallicity, distance, and age ›
Galaxy Clustering Can Reveal Host-Galaxy Properties of Binary Black Hole Mergers ›
The Binary Fraction of Milky Way Field Stars in DESI: Dependence on Chemical Abundance ›
Improved analysis of time delays between radio wavelengths and X-ray of Sgr A* flares in the shock oscillation model ›
Direct Numerical Comparison of Data Driving Strategies for Solar Flux Emergence in Magnetohydrodynamics: B-driving vs E-driving ›
Pinpointing the cosmic web between massive galaxy clusters I. The incidence of HI and OVI as WHIM tracers ›
Oxygen isotopic ratio in open cluster RGB stars: A new method for accurate mass and age estimations ›
radio-astro-tools: linking radio astronomical data to the astronomical Python ecosystem ›
Neutron star cooling with $\Delta$ dUrca processes ›
Pseudo Closed-Loop Bootstrapping for Reinforcement Learning Based AO Control ›
Gaseous SiO and Silicate Clouds in Three Benchmark Early-L Dwarfs ›
Isotopic ratios as probes of star formation and the origin of molecular gas in the Central Molecular Zone ›
Measuring radial flows in disc galaxies ›
Radio Continuum Study of One of the Brightest Large Magellanic Cloud Supernova Remnants N 132D ›
Gravitational Microlensing ›
A Coherent Harmonic Summing Pulsar Search Code ›
Probing Massive Star Formation with Intrinsic Multiplicity Constraints from TESS Eclipsing Binaries ›
Metallicity does not reorder line-to-line sensitivity to granulation in solar-like stars ›
What powers the most energetic flares in the Kepler field? Revisiting the superflaring star KIC 2852961 ›
The Hand of God Revisited: Revealing the Shell Structure and Jet-Supernova Remnant Interaction in MSH 15-52 ›
Investigating the nature of magnetic turbulence in Tycho's SNR using X-ray observation ›
From GeV to PeV: Orbital Modulation and Wind-Regulated Ultrahigh-energy Emission in Cygnus~X-3 ›
Magnetic flux cancellation in a 3D magnetohydrodynamic simulation of an emerging flux tube with a non-uniform twist ›
Size, Shape, and Geometric Albedo of Dwarf Planet Quaoar's Largest Satellite Weywot ›
Volume Dependence of Helicity-based Eruption Diagnostics in Recurrent Coronal Jets ›
On-chip filled array hyperspectral kinetic inductance detectors (FHYKID) for line intensity mapping ›
Binding Energies of Astrophysically Relevant Molecules on CO$_2$ Clusters: Benchmarking and the Donor-Acceptor Origin of Surface-Dependent Binding ›
A New Era for Supernova Science with the James Webb Space Telescope ›
An updated model of neutrino emission from proto-neutron stars ›
EWOCS-XI: Anisotropic expansion and shear in the cluster Westerlund 1. A 2D kinematic analysis with Gaia DR3 ›
Too many or too bright? Status and perspectives in the study of the UV Luminosity Function at z>10 ›
Discovery of the Slowest Radio Pulsar in the Small Magellanic Cloud ›
HI intensity mapping with MeerKAT: A measurement of the 21-cm auto-spectrum on cosmological scales ›
Modeling CO Line Luminosity Using FIRE Simulations: I. Methodology and Validation of Molecular Gas and CO Abundance ›
Autocorrelation in black hole flare movies: Departures from Kerr ›
Evidence for orbital eccentricity supports a hierarchical origin for GW231123 ›
An analytical model for non-local stochastic field-level galaxy bias on the sphere ›
Gen-EBM: an energy balance model for terrestrial planets. Climate multistability from snowball to post-runaway greenhouse climates ›
Longitudinal distribution of Io's dayside atmospheric density ›
Opening the Black Box: What Neural Networks Learn from Pulsar Timing Array Data ›
Data Representation Matters: Optimizing Machine Learning for X-ray Source Classification by Leveraging Spatio-Spectral Information ›
JWST CAPERS: Spectroscopic evaluation of very high redshift galaxy candidates ›
Rotation period of the O giant xi Persei: Coexistence of cyclic and periodic variability. A weakly magnetic candidate star ›
A morphological search for stable year-scale modulation in gamma-ray blazars ›
Funnel Leakage of the Wien Fireball in the Early Nebula after a Binary Neutron Star Merger ›
Inflow-driven galaxy evolution - II: A hierarchy in the scaling relations of star-forming galaxies ›
ACORN I. Massive Black Hole Seeding and Tidal Disruption Events from Star Clusters in Cosmological Simulations ›
Cosmic topology. Part IId. Eigenmodes and correlation matrices of lens spaces ›
Discovery of Hidden Extragalactic Pulsars in the Parkes Archival Data ›
Disk Structure May Determine AGN Variability and Explain the Accretion Disk Size Problem: No Broad Line Region Required ›
The neutrino magnetic moment and supernovae with strong magnetic fields ›
A weakly modelled view of the joint compact-binary mass plane: population structure and spectral-siren cosmology ›
Impact of site-dependent noise configurations on Einstein Telescope science at low frequency ›
Matter-Antimatter Asymmetry from Dirac-Majorana Flip-Flop ›
Observational Signatures of Dyonic Black Holes in Non-Linear Electrodynamics ›
Massive de Sitter Correlators as Finite Mellin-Barnes Integrals ›
Accounting for detector calibration uncertainty in black-hole ringdown analysis ›
Systematic Uncertainties in Ultralight Boson Constraints from Superradiance ›
Production Memory of the $^{225}\mathrm{Ra}$-$^{225}\mathrm{Ac}$ Clock in Neutron-Star Merger Ejecta ›
Analysis of p-Wave Sommerfeld Resonance Behavior in Finite-Size Dark Matter ›
Implications of tachyonic phase transition in classically scale invariant general $U(1)_{X}$ models ›
Reference-Filter-Driven Transition Probabilities for IMM-Based Satellite Maneuver Detection ›
Holographic dark energy from generalized entropies and extended infrared cut-offs ›
Nonreciprocal black holes with primary hair in beyond Horndeski gravity: Exact solutions and stability ›
Testing Extra-Dimensional Gravitational-Wave Polarizations with Compact-Binary Observations ›
Testing General Relativity with Binary Lens Microlensing Events ›
Gas-phase chemistry of $\mathrm{C}_3\mathrm{H}_3^+$: a key building block for carbon mass growth in space ›
Cavity Characterization for the Princeton Axion Search ›
Quantum Co-Design of Inhomogeneous Many-Body Neutrino Fast Flavor Transformation ›
A Pairwise Surrogate for Gravitational-Wave Spectra from Highly Relativistic Vacuum Bubble Collisions ›
Listening to the Horizon: Probing Near-Horizon Reflectivity with GW250114 ›
A scalar-extended ${\rm U(1)_{L_{\mu}-L_{\tau}}}$ explanation of the LUX-ZEPLIN 248 keV excess ›
Revising the Spin and Kick Connection in Isolated Binary Black Holes ›
DESI results and Dark Energy from QCD topological sectors ›
Rapid bulge assembly in young galaxy disks at Cosmic Dawn ›
New Signs Pointing Toward a Correlation Between Astrophysical Neutrinos and Radio Flares ›
Stable mass transfer in massive binaries leading to merging black holes ›
High-resolution Very Large Array Radio Observations of the Boomerang Pulsar Wind Nebula ›
Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole ›
Superposition model for energy reconstruction and mass identification in cosmic ray spectra ›
Velocity dispersion of Solar Energetic Particles in turbulent heliosphere ›
Learning to See Sharper: A Physics-Informed Artificial Intelligence Framework for Super-Resolving Galaxy Spectra ›
Point-like Off-pulse GeV Emission from the Millisecond Pulsar PSR J0437-4715 ›
Shape of the direct-method mass-metallicity relation with JWST: Fast-Track Nitrogen and Helium Enrichment ›
From protogalaxy through thick and thin: Why did the Milky Way evolve in three kinematic phases? ›
Phase-space averaging for stellar convection II. Maximum-entropy closures for mixed radiative-convective envelopes ›
The age of the Universe from a large sample of the oldest Galactic stars ›
Long-Baseline VLF Observations of Solar Flares from Antarctica ›
Will a Supernova explode in CD-30{\deg}11223? ›
Cosmological constraining power of the redshifts, heights, and angular clustering of weak gravitational lensing peaks ›
Spectroscopic follow-up of compact object binary candidates from Gaia DR3: White dwarfs, neutron stars, black holes, and the parallax zeropoint ›
Collisionless Shock Driven by a Supersonic Velocity Shear ›
Multi-Height Spectropolarimetric Signatures of Magnetoacoustic Waves in Solar Plage ›
Examining Temporal Characteristics of GCRs in the AMS-02 era ›
Characterizing the hierarchical structure of filaments I. On the origin of the length-mass (L-M) scaling relation ›
Why most neutron star low-mass X-ray binaries accrete transiently: an evolutionary study of transient and persistent phases ›
Gravitational-Susceptibility Dip Behind DESI's results: Addressing the Phantom Crossing by Local limit of Nonlocal Gravity ›
N/O-enhanced chemical enrichment by massive stars: the interplay of optically-thick winds and rotation ›
Discovery of thermal radio recombination line emission toward the high-mass protostar IRAS18162$-$2048 ›
Relaxation of a Vlasov gas to an inhomogeneous state due to phase space mixing in an axisymmetric potential: A Newtonian analogy of the Kerr orbital motion ›
High-Angular-Resolution Survey of Stars within 18 pc of the Sun: Part I ›
Mitigating prior-volume effects in galaxy clustering by adopting Mpc over Mpc/h units ›
PEARLS: NuSTAR and XMM-Newton Extragalactic Survey of the JWST North Ecliptic Pole Time-Domain Field V: Unraveling X-ray Spectral Variability ›
Two Low-Mass-Ratio Microlensing Planets from High-Magnification Events: KMT-2021-BLG-0247 and MOA-2023-BLG-169 ›
Widespread steep X-ray spectra of luminous $z\simeq5.85-7.5$ quasars and their implications for future X-ray surveys ›
Effect of ultralight dark matter on compact binary mergers ›
Optimized numerical evolution of perturbations across sharp background trajectory turns in multifield inflation ›
Probing soft signals of gravitational-wave memory with space-based interferometers ›
Reviving primordial black hole formation in slow first-order phase transitions ›
Exploring neutrino loss with diffuse astrophysical neutrino fluxes ›
Matter Flavor Conversion Mediated by Pseudo-Sterile States as the Possible Origin of Neutrino Oscillation Anomalies ›
Production of Leptophilic Bosons in Ultradegenerate Relativistic Matter ›
Neutron Star Bounds on Muonic Fifth Forces from Picometer to Meter Scales ›
Inflation with vector fields revisited: non-Gaussianities ›
Stochastic gravitational-wave background from self-interacting superradiant clouds ›
Heavy Higgsino Dark Matter With Low Reheating in View of the LZ High-Recoil Event ›
Kilopixel Performance of the Kinetic Inductance Detectors for the Terahertz Intensity Mapper ›
Convergence of Roberts flow dynamos in Eulerian and Lagrangian codes ↓↑