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

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Astronomia w Krakowie
Zdjecie: Aurora 10 May 2024
Aurora 10 May 2024
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 Wiadomości z astronet.pl

› Pixinsight cz.VI – Łączenie zdjęć monochromatycznych w kolorowy obraz
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› Rozsiewanie nasion za pomocą satelity – projekt Greenstar
› Katalog Caldwella: C98
› Niebo w styczniu 2026 roku
› Podsumowanie roku 2025 w astronomii i astronautyce
› Katalog Caldwella: C19
RSS  Najnowsze prace na astro-ph:

› 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

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