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

In the dome

Cloud

Rainfall

S Sky
Temperature
12.2 °C
Humidity
56%
Wind
0.0 km/h
Pressure
1028.3 hPa

Moon
Latest preprints on astro-ph:
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Diffusion Models for Polarimetric Reconstruction of Circumstellar Environments in Correlated Speckle Noise ›
Multi Kernel Gaussian Process Guiding: Predictive Correction for Mounts with Several Gear Stages ›
The orbital dynamics of the LMC and SMC about the Milky Way ›
Not So Heavy Metal I: Low Metallicity Enhances the Rate of high-redshift Superluminous Supernovae ›
Nearby Supernova Science in the Era of High Cadence, Deep Time Domain Surveys ›
Close Pulsar Pairs See Dark Matter Substructure through the Gravitational-Wave Background ›
Testing Offsets Between Cluster-Scale Halos and BCGs in Strong Lensing Models Using the Jackknife Method ›
Gestalt: a meta-foundation model for astronomy ›
An Infant Sub-Saturn in Scorpius-Centaurus ›
Surveying for Close Binaries among Lithium-rich Giants ›
An X-ray Extremely wide-field Spectroscopic Surveyor (XESS, or "chess") ›
Revealing the accretion disc structure in Changing State AGN: NGC1566 ›
Learning Gaia: A Generative Model Trained on the Gaia Data Release 3 Source Catalog ›
Cosmic-neighbor-associated distances to VHE and candidate VHE BL Lacs via SDSS photometric redshifts ›
HESS J1507-622: A Plausible Young Galactic Kilonova Remnant ›
VLBI Astrometric Procedure and Performance with CHIME/FRB Outriggers ›
A New Hope for AGN SED Fitting: X-Ray Spectral Analysis of 12MGS AGN with the C2PO-Torus Model ›
NEXUS: Discovery of a Luminous Young Transient at $z=5$ ›
PTED: A multi-dimensional two-sample test for scientific inference and generative machine learning ›
Fisher and DALI posterior approximations for testing gravity with gravitational waves ›
AdS - de Sitter transition in interacting dark energy models ›
Cosmic Collisions I: Optical Morphologies for MIRI-selected galaxies from the PRIMER survey ›
Space Journey Beyond Earth: Exploring the properties of exoplanets and multi-planetary systems ›
Toward Detecting the Moving Lens Effect with Optical Spectroscopy ›
Migration and Evolution of giant ExoPlanets (MEEP). III. Twenty-Nine Giant Planets from the TESS Mission ›
Relativistic Spherical Accretion in Nonrotating Black Hole Spacetimes: Astrophysical Implications ›
Modeling of the Yarkovsky effect. I. Thermal dependence ›
A triple-induced merger in T Ori C, solves the proplyd lifetime problem and the curiously young shell of M42 ›
Nonthermal hotspot orbiting the supermassive black hole Sgr A* ›
aRieL - Reinforcement Learning for the Ariel Space Telescope Scheduling ›
Angular structure of finite-field vacuum birefringence in magnetars ›
Sunrise III/SUSI reveals extended and spectrally structured Ca II K emission above the solar limb ›
Chandra X-ray Spectral Evidence of the Dual AGN Nature of the Gravitational lens MG B2016+112 at z=3.273 with 175 pc separation ›
A Probabilistic Trajectory and Dispersion Study of Martian Tumbleweed Rover Swarms in Global Dust Storm Conditions ›
New Constraints on $r$-process Nucleosynthesis in Neutron Star Mergers from GW170817 Late-Phase Spectra ›
HLX-1 as a Repeating Partial Tidal Disruption Event around an Intermediate-Mass Black Hole ›
Magnetic field diagnostics of a solar active region filament ›
Pulsar glitches triggered by quakes when stress reaches a threshold ›
MATCH: Performance Characterization and Scientific Observations of the Wuhan University 1-m Optical Telescope ›
Planetesimal Formation under Realistic Gas Dynamics: Dust Concentration in Turbulent and Windy Protoplanetary Disks ›
The impact of the turbulent Mach number on star formation and the initial mass function ›
The "Fork" Geometry in the DESI Main Survey DR1: Implications of Target Selection for Galaxy Evolution Studies ›
Metastable Dark Energy on the Phantom Brane ›
Stacked strong and weak lensing united: Improved measurement of the stellar and dark matter distributions in massive early-type galaxies at $z\sim 0.5$ ›
Improved Population and EOS Joint Inference for Binary Neutron Star Systems ›
The Simons Observatory: Design and Initial Performance of the Detector Readout System for the Large-Aperture Telescope ›
AGC 322753: a Dark Galaxy Candidate detected by ALFALFA and FASHI ›
Probing Helical Primordial Magnetic Fields via Chiral Gravitational Waves in the LISA-TAIJI Network ›
Electromagnetic Counterparts of Stellar-mass Binary Black Hole Mergers in AGN Accretion Disks: Theoretical Models and Observational Status ›
The Astronomical Hub: A Unified Ecosystem for Modern Astronomical Research ›
The impact of primordial magnetic fields on the formation of galaxies ›
Correlating Surface Magnetic Field Decay with Internal Field Depth of Isolated Neutron Stars ›
Exploring the Primordial Power Spectrum with Dark-Age 21 cm fluctuations ›
The AI crisis for teaching: "Train your own neural network!" ›
Early Planet Formation in Embedded Disks (eDisk). XXV. Inclination-Induced Minor-Axis Brightness Asymmetries Reveal Limited Dust Settling in Embedded Protostellar Disks ›
FAIR-Compliant Architecture for Heterogeneous Astronomical Data: KazVO Framework ›
ArxSP: A Python-Based Modular Application for the Reduction of Digitized Archival Spectra ›
An LSST-DESC Precursor Project: Hyper Suprime-Cam Year 1 $3\times2$pt in Harmonic Space ›
Internal Structure, Not Environment, Shapes Metallicity Gradients in Low-Mass Galaxies from MaNGA ›
Deep radio characterization of the supernova remnant G343.1-00.7 ›
High velocity dust grains produced by a supernova explosion ›
Effects of a central dark matter core on time-delay cosmography with galaxy clusters ›
An improved standardization framework for Type II-P supernovae using a hierarchical Bayesian approach ›
XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary ›
The Cosmological Correlation Dimension Beyond the Linear Regime: Analytical Approximation and Parameter Sensitivity ›
Towards breaking the degeneracy between stellar ages and unresolved multiplicity ›
Raising the Optical Depth to Reionization with Dark Matter Decay ›
High-Priority Compact-Object Candidates in Young Clusters from the \textit{Gaia} DR3 Non-Single-Star Catalog ›
The role of velocity dispersion in the Kennicutt-Schmidt relation ›
A New Sample of Closely Separated Dual and Binary AGN Candidates Revealed with the Radio Fundamental Catalog ›
Toward the Italian Astronomical Community's Contribution to HWO: Science, Technology, and Instrument Concepts ›
Project CERES: Nuclear Thermal Transportation and In-Situ Propellant Production A Foundational Architecture for Solar System Logistics ›
Tracing star formation across the Rosette nebula using deep Spitzer imaging ›
MAGiDiff: Sampling the Photospheric Vector Field from UV/EUV Filtergrams ›
When Streams Curve Away: a Test of Dark Matter from Extragalactic Stellar Stream Populations ›
Flow dynamics of cryolava or impact melt on Titan's surface ›
A machine learning-based method for populating dark matter halos in N-body simulations with substructure ›
Improved Constraints on Cosmic Microwave Background Circular Polarization with CLASS ›
The assembly history of NGC 1365 through chemical archaeology ›
A new method for inspiral-to-ringdown waveforms of compact binaries: Helmholtz orbits and spherical-Bessel flux ›
Is DESI Seeing Dynamical Dark Energy, or a Cosmic Glitch in Gravity? ›
Sub-kiloparsec Test of the Kennicutt-Schmidt Relation in a Strongly Lensed Dusty Star-Forming Galaxy at z~2.78 ›
Two bits about lossy compression: On the limits of compression in cosmology ›
Probing the Reionization History and Bubble Sizes with JWST Lyman-$\alpha$ Fraction Measurements ›
Slowly rotating Black Holes in DHOST Theories ›
A Strong Cosmologically Coupled Mass Growth Solution in Linearized General Relativity ›
Searching for BSM Experimental Signatures with Large Lagrangian Models ›
How collective modes terminate in the dispersion relation of neutrino plasmas ›
Constraints on Complex Electroweak WIMPs from Solar Capture ›
Kilopixel Performance of the Kinetic Inductance Detectors for the Terahertz Intensity Mapper ›
Primordial Tensor Signatures and Gravitational Wave Constraints in Lorentz Violating Inflation with Non-Canonical Kinetics ›
Heavy Dark Baryons at Large $N$: Self-Interactions across All Scales ›
Heavy Dark Baryons as Self-Interacting Dark Matter: A GeV-Scale Coincidence ›
MADGRAV: a multilevel anomaly-detection pipeline for gravitational-wave searches applied to LIGO data ›
Enhancing Constraints on Ultralight Axion Dark Matter from Gravitational Capture ›
Interpreting the High-Recoil LUX-ZEPLIN Event with Bino-/Singlino-like and Higgsino Dark Matter ›
Clash of the Titans: ultra-high energy KM3NeT event versus IceCube data ›
Euclid preparation CIX. Baryon acoustic oscillation analysis of photometric galaxy clustering in configuration space ›
Spatio-Temporal Log-Gaussian Cox-Hawkes Processes with Inhibition and Excitation for Stochastic Star Formation ›
The Einstein Gap: an unrecognised strong lensing feature in weak lensing mass density profiles ›
Effects of primordial magnetic fields on 21 cm multifrequency angular power spectra ›
Relativistic jets from millisecond proto-magnetars ›
Factorized neural posterior estimation for rapid and reliable inference of parameterized post-Einsteinian deviation parameters in gravitational waves ›
Heavy-particle production during inflation and its gravitational-wave signal ›
Reconstruction of cosmic-ray direction and energy in radio arrays using deep ensemble graph neural networks ›
Starbursts hiding in the main sequence: a pathway toward quenching? ›
Proto-NUX: A prototype telescope for ground-based near-ultraviolet observations ›
CMB constraints on dark matter-proton scattering: investigating prior-volume effects using profile likelihoods ›
Non-LTE Ionization Modeling for Helium and Strontium in Neutron Star Merger Ejecta ›
Galactic tides and the outer density profile of the Sculptor and Ursa Minor dwarf spheroidals ›
Bayesian power spectrum estimation with modelling of systematic effects in delay-fringe rate space ›
Galaxy luminosity functions from far-UV to submillimetre at $z=0$ in the COLIBRE simulations ›
Exploring the Transitional Parameter Space of Blazars using Gamma-ray and X-ray Population Diagnostics ›
Cosmic web stripping and starvation of low-mass filament galaxies in TNG50 ›
Observations of stable pickup He$^+$ tori in a magnetic flux rope at 0.85 au ›
Hybrid neural denoising for resource-efficient near- and sub-threshold radio triggering of extensive air showers ›
A Consistent Implementation of Cluster Strong Lensing in Cosmological Simulation Light Cones ›
Gas-induced gravitational-wave dephasing and accretion periodicities of live post-Newtonian massive black hole binaries: warm disk ›
DANTE: A Reference-Guided Unsupervised Pipeline for Extended-Transient Anomaly Characterization in LIGO O4a ›
Characterization of the RF Board for microwave SQUID multiplexing readout electronics ›
Modeling Uncertainties in Modified Gravity Predictions for the Stochastic Gravitational-Wave Background ›
Radiation-hydrodynamics of star-disc collisions: From system parameters to outflows and lightcurves ›
Circumstellar Disc and X-ray Variability in the Be/X-ray Binary SXP 5.05 During its 2024 Outburst ›
Propagation Diagnostics of Supernova Remnant Environments around Young Repeating Fast Radio Bursts. I. Hydrodynamic Evolution of the Source-local Dispersion Measure ›
SPT-3G D1: Foreground-Robust Lensing Templates for Primordial Gravitational Wave Searches ›
On the Acceleration of Pulsar Timing computations using Normalising Flows and Parallelisation ›
JW-FD: A 15-Year Multimodal Dataset for Solar Flare Forecasting ›
Do DESI-DR2 BAO data imply a coupling of dark matter and dark energy? ›
Connecting Dynamo Theory with DNS Data: A Computational Analysis of $\alpha$ and $\beta$ effects ›
Forecasting Coupled Dark Energy Parameters with the One-Loop Galaxy Power Spectrum ›
Inelastic scattering effects on polarization predictions for cold and warm atmospheres in the X-rays ›
K-dwarf starspot hunters: how to directly characterize spot and faculae properties with UV-IR panchromatic transit spectra ›
Slow-roll inflation in $f\left(R, T, R_{ab}T^{ab}\right)$ gravity ›
Primordial black hole formation in matter domination ›
Bounds on massive graviton-like particles from searches for axion-like particles coupling to photons ›
Development of Neutron Transmutation Doped Germanium (NTD-Ge) for Cryogenic Applications ›
Infrared Screening of the Cosmological Constant ↓↑