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Mount Suhora Astronomical Observatory

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Astronomia w Krakowie
Photo: view from south-east
view from south-east
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Allsky

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Temperature
9.2 °C

Humidity
 37%

Wind
1.6 km/h

Pressure
1019.7 hPa

Moon

Moon

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RSS  Latest preprints on astro-ph:

› Gender equality activities in Astronomical Society of Japan
› Verifying the STIS Time Dependent Sensitivity Trends with the Primary CALSPEC Standards
› The Effects of Complex Accretion Disk Geometry on Broadened Iron K$\alpha$ Lines
› The Simons Observatory: Improved Cryogenic Struts for use in the Large Aperture Telescope Receiver
› Euclid Quick Data Release (Q1). AstroVink: A vision transformer approach to find strong gravitational lens systems
› Fast, Stable, and Physical: Hyperbolic, Magnetic Field-Aligned Diffusion in SPH
› A SPHEREx Pipeline and Spectral Library for Ultracool Dwarfs
› An Extended Parametric Model for Self-interacting Dark Matter Halos
› Understanding HWO's Field of Regard and Characterization Requirement Trade Space with a Dynamic Observation Scheduling Algorithm
› Differentiable Forward Modeling for Efficient and Accurate Shear Inference
› Electromagnetic Precursors to Binary Neutron Star Mergers: Kinetic Simulations of Magnetospheric Flaring
› Large language models are not the problem
› CCAT: Silicon-Platelet Feedhorns for Submillimeter Wavelengths
› Downward ultra-high-energy neutrino detection in the air with radio antennas at ground-based observatories
› Backlighting the Cosmic Web with Fast Radio Bursts: An Anthology of Dispersion Measure Cross-Correlations with Large-Scale Structure and Baryon Tracers
› FPGA-based Matched Filter Group Optimisation for SKA Pulsar Search Engine
› Short timescale variation in the submillimeter flux of Sagittarius A*
› Repeated Sunspot Light Bridge Jets Associated with Slipping Base Brightenings
› The science from asteroid sample return missions
› Formalizing Galaxy Population Evolution: Drift and Mergers as Transport Processes on Manifolds
› Caustic Skeleton and the Local Cosmic Web: the Coma Cluster node and the Pisces-Perseus ridge
› The circumstellar environment of the young, low-mass dipper star JH 223. Accretion and large-scale magnetic field topology
› Asteroseismic rotation rates of hot subfwarf B stars hint at transient accretion from leftover common envelope matter
› Non-LTE corrections for determinations of europium abundances in F-G-K stars in a broad metallicity range
› Quiescent and flaring states of three active stars: V834 Tau, LQ Hya, and BY Dra
› Signature of iron line profile from a Kerr-like wormhole
› The Leiden/ESA Astrophysics Program for Summer Students (LEAPS)
› A Morphological Identification and Study of Radio Galaxies from LoTSS DR2. I. The "Winged'' Radio Galaxies
› Thermal background reduction for mid-infrared imaging by low-rank background and sparse point-source modelling
› A study of the spatial evolution of the Radcliffe wave in a sample of young open star clusters
› Testing $\Lambda$CDM with ANN-Reconstructed Expansion History from Cosmic Chronometers
› Quiescent fractions in high-redshift galaxy groups reflect their hot-or-cold state of gas accretion
› How lonely are the Binary Compact Objects Detected by the LIGO-Virgo-KAGRA Collaboration?
› Spatially resolved metallicity and ionization in the merging system Gz9p3 at z=9.3
› Radial evolution of Alfv\'en wave Parametric Decay Instability in the near-Sun solar wind: Effects of Temperature Anisotropy
› A Quasar--Companion System Without AGN Outflow at $z \sim 6$: The Case of PSO J083+11
› A homogeneous three-dimensional view of Molecular Cloud kinematics out to 2.5 kpc. Using Young Stellar Objects and Open Clusters as complementary tracers
› Synchrotron polarization of anisotropic electron distribution in GRB prompt emission
› The Effect of Mass Loss and Convective Overshooting on the Pre-Collapse Structure, Composition, and Neutrino Emission of Red Supergiants
› MUSE-DARK III: The evolution of the radial acceleration relation at intermediate redshifts
› Ultra-high-energy $\gamma$-ray imprints from PeV particles accelerated by supernova remnants
› Constraints on the Primordial Black Hole Abundance using Pulsar Parameter Drifts
› Variability of Sagittarius A* at 3 GHz on minute-scale with MeerKAT
› Radiative feedbacks as drivers for quasi-periodic-oscillation activity in black-hole X-ray binaries
› From core to envelope: revealing the deep dynamics of stars with two convective zones
› The Sound of the Universe: A Resonant Gravitational Instability Driven by Baryon-Dark Matter Relative Drift
› Exploring the diversity of kilonovae with 3D radiative transfer I. The polar direction
› Dense Matter and Compact Stars in Strong Magnetic Fields
› CosmicDancePro -- Measuring LEO satellite's orbital decay and network connectivity implications during solar storms
› WAsp: The Wideband (W) Adaptive-Scale Pixel (Asp) Deconvolution Algorithm for Interferometric Imaging
› Forecasting the occupancy of satellite megaconstellations in SKA observations
› First Statistical Study of Over 100 Magnified Stellar Events at Redshift $z \approx 0.725$ with JWST
› Reionization, UV Luminosity and 21$\,$cm Sensitivity to Primordial Magnetic Fields: Impact of Energy Losses
› Simulation of a protoplanetary disk accretion activity due to a collision with a gas stream
› Precision Analysis for $\boldsymbol{H_0}$ Using Upcoming Multi-band Gravitational Wave Observations
› On the redshift evolution of the spin parameter in cosmological simulations
› Describing the swdatatoolkit: A Space Weather Data Analysis Library
› From Anomaly to Candidate Technosignature: The Threshold Problem of the Loeb Scale
› Determination of the sensitivity of the DEAP-3600 experiment to supermassive charged gravitinos
› Gradient-Produced Neutrinos
› Cosmic-Ray Signatures of Annihilating and Semi-Annihilating Dark Matter via One-Step Cascades
› Solar Reflection of Inelastic Dark Matter
› Data-Driven Acceleration of Eccentricity Reduction for Binary Black Hole Simulations
› Simulation-based Inference for Gravitational Waves from Binary Neutron Stars: Application of Summary Data from Heterodyning
› Machine Learning for Multi-messenger Probes of New Physics and Cosmology: A Review and Perspective
› Gauge-independent approach to inflation in quadratic gravity
› The Decoupling of Binaries from Their Circumbinary Disks
› On the Relationship of Dichotomy of Mars and Occurrence of Dust Devils with Crustal Magnetic Fields
› The Large Smooth Patch on Comet 9P/Tempel 1: Remnant of a Recent Past Event
› A Mysteriously Tight H$\alpha$-[O III] Correlation and Non-Case B Balmer Decrements Revealed by the Spectra from the James Webb Space Telescope NIRSpec Instrument
› The Missing Hard Photons of Little Red Dots: Their Incident Ionizing Spectra Resemble Massive Stars
› Probing dense environments around Sgr A* with S-stars dynamics
› Cross-correlations between the CLAMATO Lyman-alpha forest and galaxies within the COSMOS field
› Crosschecking Cosmic Distances from DESI BAO and DES SNe
› Generalized Distributions of Host Dispersion Measures in the Fast Radio Burst Cosmology
› $O_k$ null test with multi-task Gaussian processes: cosmic curvature and data compatibility
› Most Rocky Sub-Neptunes are Molten: Mapping the Solidification Shoreline for Gas Dwarf Exoplanets
› Anisotropic diffusion modeling of cosmic-ray lepton propagation
› Comprehensive study of solar type II radio bursts and the properties of the associated shock waves
› Cosmic Collider Gravitational Waves sourced by Right-handed Neutrino production from Bubbles: Testing Seesaw, Leptogenesis and Dark Matter
› Magma Ocean Waves and Thermal Variability on Lava Worlds
› Expanding the High-z Supernova Frontier: "Wide-Area" JWST Discoveries from the First Two Years of COSMOS-Web
› Subsolar mass black holes from stellar collapse induced by primordial black holes
› Probing Compact Objects in Wide-Orbit Binaries with Joint LAMOST LRS and MRS
› Oxygen left behind: Atmospheric Enrichment due to Fractionation in Sub-Neptunes using BOREAS
› Effects of the symmetry energy slope on magnetized neutron stars
› The no-hair theorems at work in the tidal disruption event AT2020afhd
› Probing Physics Beyond the Standard Model through Combined Analyses of Next-Generation Type Ia Supernova, CMB, and BAO Surveys
› The Pristine HeII Emitter near GN-z11: Constraining the Mass Distribution of the First Stars
› Automatic search for transiting planets in TESS-SPOC FFIs with RAVEN: over 100 newly validated planets and over 2000 vetted candidates
› Big Bang Nucleosynthesis Constraints on the CCC+TL Cosmology
› Multi-scale Gas Structure and Dynamics in an Extragalactic Central Molecular Zone
› The GMRT archive atomic gas survey -- IV. Consistency of the dark matter halo perturbation parameter from morphological and kinematic lopsidedness of galaxies
› JOYS: Launching and destruction of dust in protostellar jets. The case of BHR71-IRS1 with JWST/MIRI
› VLTI-GRAVITY observations of blazars
› X-Shooting ULLYSES: Massive stars at low metallicity XV. On the metallicity dependence of B-supergiant mass-loss rates
› Sensing Gravity with Polarized Electromagnetic Radiation
› Gravitational Wave Birefringence from Fuzzy Dark Matter
› Consistent $N_{\rm eff}$ fitting in big bang nucleosynthesis analysis
› A Compact Story of Positivity in de Sitter
› Electron Heat Flux and Whistler Instability in the Earth's Magnetosheath
› Dynamical response of twin stars to perturbations
› Design of low-energy transfers in cislunar space using sequences of lobe dynamics

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