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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Temperatura
7.3 °C

Wilgotność
 37%

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3.2 km/h

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1025.2 hPa

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 Wiadomości z astronet.pl

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RSS  Najnowsze prace na astro-ph:

› Parameter estimation of eccentric massive black hole binaries with LISA and its cosmological implications
› SNAPPY CubeSat Control Script Generation and Data File Processing
› NASA's Pandora SmallSat Mission: Simulated Modeling and Retrieval of Near-Infrared Exoplanet Transmission Spectra
› The erasure of Galactic bar resonances by dark matter subhaloes
› When self-similarity meets mass spectrum and anisotropy
› The Drivers of Cosmic Dust Temperature Evolution
› Low-resolution spectroscopic characterisation of five poorly known Galactic stellar clusters
› The dark fate of ultra-faint dwarfs: gravothermal collapse in action
› The Far-Ultraviolet Extragalactic Legacy (FUEL) Survey: Hubble Far-UV Images and Catalogs of the Extragalactic Legacy Fields
› MXDFz4.4: A LyC emitter 250Myr after the epoch of reionization and a first test of Ly-alpha morphology as a tracer of LyC escape at high redshift
› NASA's $\textit{Pandora SmallSat Mission}$: Simulating the Impact of Stellar Photospheric Heterogeneity and Its Correction
› Detection of non-thermal radio emission components from the Orion Nebula: stellar jets, cloud collision or feedback from stellar winds?
› Coexistence of Chromatic Flares and an Achromatic QPO in the Gamma-ray Blazar PG 1553+113
› Spectral Hardening Revealed by Geometric De-boosting in the Masked Jet of PKS 2155$-$304
› Geometric masking in AGN jets and its implications for unification and blazar physics
› A Fast Generative Framework for High-dimensional Posterior Sampling: Application to CMB Delensing
› Aromatic Species in the Molecular Universe
› Beyond21: A Global Framework for Cosmic Dawn and Reionization Within and Beyond the Standard Model
› EBLM XVII - Tidal Synchronization and Circularization in Tight Stellar Binaries
› Examining the Effects of Magnetic Field Extrapolation on MHD Flare Simulations
› A Comparative Study of the Streaming Instability: Unstratified Models with Marginally Coupled Grains
› Repeating Nuclear Transients from Repeating Partial Tidal Disruption Events
› The Age of the R127 & R128 Clusters: Implications for the LBV
› The First Detection of Forbidden Emission Lines at the Outskirts of the AGN Broad Line Region?
› NEXUS: Quick Release Notes
› PulSKASim: A Pulsar Simulator for SKA-Scale Interferometric Observations
› X-ray Doppler tomography of Fe K$\alpha$ emission in a low-mass X-ray binary 4U 1822-371 - a localized reflector at the accretion stream-disk overflow
› 3D Rotation of the Open Cluster NGC 2516
› AstroInspect: a web-based system to organize, assess, and visually inspect astronomical objects
› Early Planet Formation in Embedded Disks (eDisk). XVIII. Indication of a possible spiral structure in the dust-continuum emission of the protostellar disk around IRAS 16544-1604 in CB 68
› Could the interaction of jet and SN ejecta be the cause of X-ray knots observed in a radio galaxy?
› Accelerating massive galaxy formation with primordial black hole seed nuclei
› Resolving diffusion signatures in distant pulsar halos with current and future experiments
› A New Method for Identifying Contaminating Sources and Locating Target Sources through the Cross-Arm Features of Micro Pore Optics
› Probing Dark Energy on the Moon
› STOchastic LAttice Simulation of hybrid inflation
› The Age of the Universe with Globular Clusters IV: Multiple Stellar Populations
› Long-period magnetic activity in the K dwarf GJ 1137 and a new super-Earth on a 9-day orbit
› Influence of Solar Polar Magnetic Fields on the Propagation of Coronal Mass Ejection
› Euclid: A blue galaxy population and a brightest cluster galaxy in the making in a $z\sim1.74$ MaDCoWS2 galaxy cluster candidate
› MWA tied-array processing V: Super-resolved localisation via amplitude-only maximum likelihood direction finding
› Sensitivity of a closed dielectric haloscope to axion dark matter
› Fusion of JWST data - Demonstrating practical feasibility
› Stochastic Particle Acceleration during Pressure-Anisotropy-Driven Magnetogenesis in the Pre-Structure Universe
› Neural blind deconvolution to reconstruct high-resolution ground-based solar observations
› Accelerated size evolution in the FirstLight simulations from z=14 to z=5
› Sound Mode and Scale-Dependent Growth in Two-Fluid Dynamical Dark Energy
› Simultaneous Misalignment and Mode Mismatch Sensing in Optical Cavities Using Intensity-Only Measurements
› Exploring the chemical evolution in hot molecular cores
› HC$_3$N, H$^{13}$CN, and HN$^{13}$C in molecular cores evolving towards star-forming regions
› Reassessing the SIGW Interpretation of PTA Signal: The Role of Third-Order Gravitational Waves and Implications for the PBH Overproduction
› Probing the properties of active regions in the solar interface region using full-disk spectroheliograms
› Comparing First Ionisation Potential bias diagnostics in the solar atmosphere
› Stellar contents and Star Formation in IRAS 18456-0223
› EMU/GAMA: A statistical perspective on active galactic nuclei diagnostics
› The Local Tremaine-Weinberg Method for Galactic Pattern Speed: Theory and its Application to IllustrisTNG
› ULTIMATE deblending I. A 50-band UV-to-MIR photometric catalog combining space- and ground-based data in the JWST/PRIMER survey
› HD 188101: A Spotted B Star with Abundance Anomalies
› Hydrodynamic outflows of proto-lunar disk volatiles
› Scientific performance of on-board analyses for the SVOM X-ray telescope MXT
› GASTON-GP: Source catalogue and millimetre variability of massive protostellar objects
› Nuclear Physics of X-ray Bursts
› Detection of C3 in Titan with VLT-ESPRESSO
› Trans-Neptunian Binary Mutual Events in the 2020s and 2030s
› Resolving the sub-parsec circumnuclear density profiles of quiescent galaxies: Evidence for Bondi accretion flows in tidal disruption event hosts
› Surprising increase of electron temperature in metal-rich star-forming region
› TILARA: Template-Independent Line-by-line Algorithm for Radial velocity Analysis. I. Description of the code and application on a Sun-like star
› A likelihood analysis for gamma-ray background models
› The Bayesian view of DESI DR2: Evidence and tension in a combined analysis with CMB and supernovae across cosmological models
› A FAST Survey of H I Absorption in Low-power Radio Sources
› Experiments towards a neutron target for measurements in inverse kinematics
› Augmenting representations with scientific papers
› Search for continuous gravitational waves from neutron stars in five globular clusters in the first part of the fourth LIGO-Virgo-KAGRA observing run
› On curvature corrections for field theory cosmic strings
› High Tide or Riptide on the Cosmic Shoreline? A Water-Rich Atmosphere or Stellar Contamination for the Warm Super-Earth GJ~486b from JWST Observations
› Boltzmann Equation Field Theory I: Ensemble Averages
› The size and shape dependence of the SDSS galaxy bispectrum
› Data Release 1 of the Dark Energy Spectroscopic Instrument
› Discovery of a 0.8-mHz quasi-periodic oscillation in the transient X-ray pulsar SXP31.0 and associated timing transitions
› Unveiling the Sagittarius Dwarf Spheroidal Galaxy Core with Gaia DR3: A Red Clump Distance Precise to 2%
› A Multimessenger Search for the Supermassive Black Hole Binary in 3C 66B with the Parkes Pulsar Timing Array
› Investigating the Gamma-Ray Emission from Explosive Dispersal Outflows with Fermi-LAT
› Time-Dependent Modeling of the Sub-Hour Spectral Evolution During the 2013 Outburst of Mrk 421
› Towards a foundation model for astrophysical source detection: An End-to-End Gamma-Ray Data Analysis Pipeline Using Deep Learning
› Large-scale peculiar velocities in the universe
› Estimation of intrinsic fast radio burst width and scattering distributions from CRAFT data
› Lanthanide Impact on the Infra-Red Spectra of Nebular Phase Kilonovae
› A merger within a merger: Chandra pinpoints the short GRB 230906A in a peculiar environment
› Slow neutrinos: non-linearity and momentum-space emulation
› Smoothed Particle Hydrodynamics in pkdgrav3 for Shock Physics Simulations I: Hydrodynamics
› Large Language Model-driven Analysis of General Coordinates Network (GCN) Circulars
› Broad-band temporal and spectral study of TeV blazar TXS 0518+211
› Solar Cycle Variation of Sustained Gamma Ray Emission from the Sun
› The Preliminary Mauve Science Programme: Science themes identified for the first year of operations
› Spectral Signatures of Spinning Dust from Grain Ensembles in Diverse Environments: A Combined Theoretical and Observational Study
› The multiple coherence scales of C IV at cosmic noon
› Three-dimensional mapping of coronal magnetic field and plasma parameters in a solar flare
› Shock-induced chiral magnetic effect
› GA-NIFS: Dissecting The Alchemised: NIRSpec/IFU reveals turbulent gas inflows in a complex system at $z=10.17$
› Matched Filtering for the Canadian Hydrogen Observatory and Radio-Transient Detector Galaxy Search
› Weak Lensing by Photometric Density Ridges
› Megahertz Gravitational Waves from Neutron Star Mergers
› Unified Gas Heating Constraints on Extended Dark Matter Compact Objects
› Probing Light Primordial Black Holes through Non-cold Dark Matter
› Stochastic gravitational wave from graviton bremsstrahlung in inflaton decay into massive spin 3/2 particles
› Thermodynamic Gravity with Non-Extensive Horizon Entropy and Topological Calibration
› Magnetic monopoles and high frequency gravitational waves from quasi-stable strings

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