ul. Podchorążych 2, 30-084 Kraków.
tel.: (+48 12) 662 6301;
fax: (+48 12) 637 2243;
Obs. tel.: (+48) 502 113714
Obserwatorium Astronomiczne na Suhorze

Aurora 10 May 2024

Kamerka S

Kamerka N

Niebo
Temperatura
1.3 °C
Wilgotność
36%
Wiatr
0.0 km/h
Ciśnienie
1030.2 hPa

Księżyc
Najnowsze prace na astro-ph:
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The Ghana Radio Astronomy Observatory ›
Simulating cosmic ray electron spectra and radio emission from an AGN jet outburst in a cool-core cluster ›
Astrometric microlensing probes of the isolated neutron star population with Roman ›
Metal Pipe: A Broadly-Applicable Stellar Abundance Pipeline Using Isochronal Parameters ›
Euclid: Galaxy SED reconstruction in the PHZ processing function: impact on the PSF and the role of medium-band filters ›
Diagnosing the Effects of Spectroscopic Training Set Imperfection on Photometric Redshift Performance ›
POLAMI Multi-Wavelength Polarization Study of AGN Jets: A Millimeter-Optical Comparison ›
Checking It Twice: Using [C/N]-Masses and Asteroseismic Masses as a Diagnostic of Mass Loss and Transfer on the RGB ›
The impact of ram pressure on the radio spectral index and magnetic field of NGC 4522: A high-resolution VLA continuum study ›
The impact of disc photoevaporation on the long-term evolution of giant planets in mean motion resonances ›
A Closer Look at the Dynamical State of the High-redshift Galaxy Cluster SPT-CL J2215-3537 ›
Tracking the Evolution of Plasma Instabilities from the Prominence-Corona Transition Region into Interplanetary Space with Total Solar Eclipse and WISPR/PSP White Light Images ›
Asteroseismology of the ZZ Ceti star WD 1310+583 using the Transiting Exoplanet Survey Satellite ›
Rotation Period of 3I/ATLAS After Perihelion from Jet Position Angle Wobble and Photometric Variability ›
Optimal and Unbiased Fluxes from Up-the-Ramp Detectors under Variable Illumination ›
From a Network to a Networking: The Evolution of the Latin American Giant Observatory ›
The Deeper, Wider, Faster programme's first DECam optical data release ›
Pink Dwarfs and the Paths to Stardom: How Brown Dwarfs Pushed Above the Hydrogen Burning Limit Evolve ›
X-ray and radio observations of the AMXP MAXI J1957+032 covering the 2022-2025 outbursts ›
Radiative Cooling Effects on Plasmoid Formation in Black Hole Accretion Flows with Multiple Magnetic Loops ›
A Novel, Beam-based Formalism for Active Impedance of Phased Arrays ›
How To Use Thermal Dust Continuum Emission To Measure The Physical Properties Of Dusty Astrophysical Objects ›
Curvature Effect on the Speed of Sound ›
CHILES XI: Resolved HI morphologies and the evolution of the H2/HI ratio over the last five billion years ›
An 11-Year Catalog of Gamma-Ray Transients: A Comprehensive Search with Fermi Gamma-ray Burst Monitor Data ›
Searching for Galaxy Cluster-Scale Strong lenses from the DESI Legacy Imaging Surveys ›
A Portrait of the Cosmic Reionisation History in the Context of the Early Dark Energy Model ›
Multifrequency evolution of the Integrated pulse profile of radio pulsars by implementing the inverse Compton mechanism ›
Investigating Pulsar Wind Nebula DA 495: Insights from LHAASO and Multi-Wavelength Observations ›
Magnetic Topology and Loop Statistics in Observed Coronal Holes Using Potential Field Modeling ›
Emission-line Diagnostics at $z\gtrsim 2$: A Probe of the Ionizing Spectrum and $\alpha$ Enhancement Beyond Cosmic Noon ›
ALMA Polarization Study of the Magnetic Fields in Two Massive Clumps in the 20 km s$^{-1}$ Cloud of the Central Molecular Zone ›
Broadband study of the Be/X-ray binary pulsar eRASSU J012422.9-724248 in the Magellanic Bridge, near the Eastern Wing of the Small Magellanic Cloud ›
The Role of Plasma Lensing in Fast Radio Bursts ›
Discovery of a gas-enshrouded broad-line AGN at z $\sim$ 7 ›
Molecular gas and star formation in central rings across nearby galaxies ›
Unveiling Ionized Jet Morphologies: Sub-arcsecond VLA Observations of Compact Radio Sources ›
Study of the anisotropy of cosmic expansion on ZTF type Iasupernovae simulations ›
Bayesian optimisation for Bayesian evidence (BOBE) -- a fast and efficient likelihood emulator for model selection ›
Deep Submillimeter and Radio Observations in the SSA22 Field. IV. Spectral Energy Distributions, Star Formation Histories, and the Infrared-Radio Correlation of the 850 $\mu$m-selected SMGs ›
Spectral evolution of hot hybrid white dwarfs: II. Photometry ›
The test and calibration system for the Elementary Cells of the Cherenkov Camera in the PBR Mission ›
Little Red Dots as Hidden Neutrino Sources ›
Deep Submillimeter and Radio Observations in the SSA22 Field. III. Multiwavelength Identifications and Properties of the 850 $\mu$m-selected Submillimeter Galaxies ›
KiDS-Legacy: WIMP dark matter constraints from the cross-correlation of weak lensing and Fermi-LAT gamma rays ›
Mobile Intensity Interferometer for Stellar Observations (MI$^2$SO) ›
Cluster number counts in dark energy model with energy and momentum coupling to dark matter ›
Suppression of Fast Flavor Conversion by Red Turbulence in Supernovae ›
Detection of four cold Jupiters through combined analyses of radial velocity and astrometry data ›
Aligned, Misaligned and Polar Orbits of Hot Jupiters: Measuring Spin-Orbit Angles via Doppler Tomography with HARPS-N ›
Extragalactic planetary nebulae -- tracers of kinematics and stellar populations out to 100 Mpc ›
Rescaling Transforms for Local Models of Spherical Flows ›
Constraining the inflaton potential with gravitational waves from oscillons ›
Central flashes during stellar occultations. Effects of diffraction, interferences, and stellar diameter ›
Star-forming compact groups: Tracing the early evolutionary stages of compact group environments ›
Zero-Shot Detection of Elastic Transient Morphology Across Physical Systems ›
FEAST: Probing Hierarchical Star Formation with the Spatial Distributions of Young Star Clusters ›
Impact of baryons on the population of Galactic subhalos and implications for dark matter searches ›
Five Years of Mini-EUSO Observations from the ISS: Summary of Key Results ›
Pseudo Little Red Dot: an Active Black Hole Embedded in a Dense and Dusty, Metal-Poor Starburst Galaxy at z=5.96 ›
KMT-2025-BLG-1616Lb: First Microlensing Bound Planet From DREAMS ›
Fundamental Properties of Novae in M31 ›
Galactic core-tail structure in BEC dark matter with Kapitza potential ›
Analytical approaches to the study of the phase of the visibility function ›
Spectroscopic confirmation of a large and luminous galaxy with weak emission lines at $\mathbf{z = 13.53}$ ›
X-ray Polarization of the Intrabinary Shock in Redback Pulsar J1723$-$2837 ›
The gravitational wave landscape of cosmic string networks with varying tension ›
Shadow signatures and energy accumulation in Lorentzian-Euclidean black holes ›
Gravitational perturbations of nonlocal black holes ›
Fine-tunings in radiative $\alpha$-particle capture on $^{12}$C at astrophysical energies ›
Rapid inference of gravitational-wave signals in the time domain using a heterodyned likelihood ›
Light Dark Matter Search with 7.8 Tonne-Year of Ionization-Only Data in XENONnT ›
Circumbinary disks in post common envelope binary systems with compact objects ›
Ultra High-Redshift or Closer-by, Dust-Obscured Galaxies? Deciphering the Nature of Faint, Previously Missed F200W-Dropouts in CEERS ›
Current Theories of Lunar Ice ›
Unified and consistent structure growth measurements from joint ACT, SPT and \textit{Planck} CMB lensing ›
Amaryllis: a digital twin of the earliest galaxies in the Universe ›
Discovery of a dwarf planet candidate in an extremely wide orbit: 2017 OF201 ›
The Properties of Little Red Dot Galaxies in the ASTRID Simulation ›
Critical Metallicity of Cool Supergiant Formation. II. Physical Origin ›
Characterising the Standardisation Properties of Type Ia Supernovae in the z band with Hierarchical Bayesian Modelling ›
Optical and near-infrared nebular-phase spectroscopy of SN 2024ggi: constraints on the structure of the inner ejecta, progenitor mass, and dust ›
Dual-Backend Multibeam Position Switching Targeted SETI Observations toward Nearby Active Planet-Hosting Systems with FAST ›
GW231109_235456: A Sub-threshold Binary Neutron Star Merger in the LIGO-Virgo-KAGRA O4a Observing Run? ›
M^3D: Mosaicking M33 with MUSE datacubes I. Unveiling the diversity of HII regions in M33 with MUSE ›
Cosmological constraints on Galileon dark energy with broken shift symmetry ›
Simulating Image Coaddition with the Nancy Grace Roman Space Telescope. IV. Hyperparameter Optimization and Experimental Features ›
A supermassive black hole under the radar: Repeating X-ray variability in a Seyfert galaxy ›
The ExoGRAVITY survey: A K-band spectral library of giant exoplanet and brown dwarf companions ›
Leveraging Photometry for Deconfusion of Directly Imaged Multi-Planet Systems ›
Simulation-calibrated Bayesian inference for progenitor properties of the microquasar SS 433 ›
A JWST Transit of a Jupiter Analog I: Constraints on the Oblateness of Kepler-167e ›
Exploring Cosmological Constraints of the Void-Lensing Cross-Correlation in the CSST Photometric Survey ›
Study of Flat Spectrum Radio Quasars and BL Lacertae Objects as Sources of Diffusive Ultra High-Energy Cosmic Rays ›
Verifying the failing supernova constraint on dark photons with two-dimensional hydrodynamic simulations ›
Non-Gaussianity in SMICA ›
Spectroscopic characterization of a remarkable temporally varying, triple-lensed quasar at z=2.67 ›
Water Production of Interstellar Comet 3I/ATLAS from SOHO/SWAN Observations after Perihelion ›
The steep redshift evolution of the hierarchical binary black hole merger rate may cause the $z$-$\chi_{\rm eff}$ correlation ›
The maximum mass ratio of hierarchical binary black hole mergers may cause the $q$-$\chi_{\rm eff}$ correlation ›
Isochrone Fitting of Galactic Globular Clusters -- VII. NGC1904 (M79), NGC4372, and revision of NGC288, NGC362, NGC5904 (M5), NGC6205 (M13), and NGC6218 (M12) ›
Brightest GRB flare observed in GRB 221009A: bridge the last gap between flare and prompt emission in GRB ›
The influence of magnetic fields in Cloud-Cloud Collisions ›
The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations ›
Time delay interferometry with minimal null frequencies and shortened time span ›
A Step in Flux to Suppress Axion Isocurvature ›
Challenging a binary neutron star merger interpretation of GW230529 ›
Dynamical Prevention of Topological Defect Formation ›
Photon Accelerator in Magnetized Plasma ›
Reinforcement Learning to Discover a NorthEast Monsoon Index for Monthly Rainfall Prediction in Thailand ↓↑