Obserwatorium Astronomiczne na Suhorze Strona główna
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RSS  Najnowsze prace na astro-ph:

› Sustainable, Local Socio-Economic Development Through Astronomy
› Exploring Metal Additive Manufacturing in Martian Atmospheric Environments
› Charge Migration and Residual Non-Linearity in NIRSpec BOTS Observations
› Search for Precessing Binary Black Holes in Advanced LIGO's Third Observing Run using Harmonic Decomposition
› A New Bayesian Framework with Natural Priors to Constrain the Neutron Star Equation of State
› Morphologies arising from the gas flow in the innermost kiloparsec of barred galaxy models
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› Neutrino decays as a natural explanation of the neutrino mass tension
› The early Universe with JWST and ALMA
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› Simulating the Formation of the Young "Fermi Bubbles" in the Circinus Galaxy
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› Investigating HII Regions in the Disk of NGC 7331 with the Circumgalactic H$\alpha$ Spectrograph
› KL Dra as a Benchmark Laboratory for Accretion-Disk Physics: Constraints from TESS and Ground-Based Surveys
› Polarization of decayless kink oscillations in a 3D MHD coronal loop model
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› The Impact of Robotic Telescopes on Time-Domain Astronomy
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› A catalogue of Type 2 active galactic nuclei in the 6dF Galaxy Survey
› Propagating Uncertainties from Nuclear Physics to Gamma-rays in Core Collapse Supernovae
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› J-PLUS: The planetary nebula population of M 33
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› Explainable machine learning classification of \textit{Chandra} X-ray sources: SHAP analysis of multi-wavelength features
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› Probing Trans-Planckian Signatures in the Early Universe: A Bayesian Analysis of the Generalized Sasaki-Mukhanov Equation
› The effect of metallicity on the Leavitt Law using phase-dependent properties of classical Cepheids
› Optimization of Deep Learning Models for Radio Galaxy Classification
› First measurement of the Hubble constant from a combined weak lensing and gravitational-wave standard siren analysis
› Euclid preparation. Galaxy 2-point correlation function modelling in redshift space
› A change of the rotation period of asteroid (65803) Didymos caused by the DART impact
› Long-term evolution of cyclotron resonant scattering features in the accreting pulsar Vela X-1: A pulse-to-pulse approach
› Tidal encounters of close white dwarf binaries with spinning black holes
› Temporal Variations in Pulsar Spectro-Polarimetry: Findings from millisecond pulsar J2144-5237 using Parkes UWL receiver
› Three-equation turbulent convection models in classical variables
› Multi-Messenger Studies with High-Energy Neutrinos and Gamma Rays: The WST Opportunity
› Triaxial Magnetars as Sources of Fast Radio Bursts
› Rapid emergence of overmassive black holes in the early Universe
› Through Thick and Thin: The Cosmic Evolution of Disk Scale Height
› Probing millisecond magnetar formation in binary neutron star mergers through X-ray follow-up of gravitational wave alerts
› Mutual Orbit Alignment in Resolved Triple Systems
› Jet launching from the Kerr black hole magnetosphere: An electrogeodesic approach
› Energetic particles accelerated via turbulent magnetic reconnection in protoplanetary discs -- I: ionisation rates
› Constraining the Primoridal Black Hole Abundance with Space-Based Detectors
› Surveying exogenous species in Saturn with ALMA I. Detecting and Mapping CO
› Multigroup Radiation Diffusion on a Moving Mesh: Implementation in RICH and Application to Tidal Disruption Events
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› How deep can a cosmic void be? Voids-informed theoretical bounds in Galileon gravity
› Symbolically regressing dark matter halo profiles using weak lensing
› Addressing Known Challenges in Solar Flare Forecasting I: Limb-Flare Prediction with a 4-pi Full-Heliosphere Framework
› Mitigating Simulator Dependence in AI Parameter Inference for the Epoch of Reionization: The Importance of Simulation Diversity
› Three-dimensional scene reconstruction using Roman slitless spectra
› Mimicking Phantom Dark Energy with Evolving Dark Matter Mass
› Unveiling the 3D structure of the central molecular zone from stellar kinematics and photometry: The 50 and 20 km/s clouds
› The dynamical and thermodynamic effects of turbulence on the cosmic baryonic fluid
› Color-Singlet and Color-Octet Quark Matters
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› Metastable cosmic strings are broken at the start
› Future Rip Scenarios in Fractional Holographic Dark Energy
› Search for Ultralight Axion Dark Matter with a Levitated Ferromagnetic Torsional Oscillator
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› Multi-messenger standard-siren cosmology for third-generation gravitational-wave detectors: forecasts considering observations of gamma-ray bursts and kilonovae
› On the Presence of Angular-Velocity Offsets in Disk Galaxies
› Modelling the evolution and influence of dust in cosmological simulations that include the cold phase of the interstellar medium
› Non-Parametric Attenuation Curves in Local Star-Forming Galaxies: Geometry Effect, Dust Evolution, and ISS
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› Investigating non-Keplerian motion in flare events with astrometric data
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› In-orbit Spectral Calibration Prospects for the COSI Space Telescope
› Euclid: Early Release Observations -- The star cluster systems of the Local Group dwarf galaxies IC 10 and NGC 6822
› Distance measurements from the internal dynamics of globular clusters: Application to the Sombrero galaxy (M104)
› Biasing from galaxy trough and peak profiles with the DES Y3 redMaGiC galaxies and the weak lensing mass map
› Dark-Matter-Deficient Galaxies from Collisions: A New Probe of Bursty Feedback and Dark Matter Physics
› A z ~ 0.4 Galaxy Reflecting the high-redshift Little Red Dots: An Extended Starburst with an Overmassive Black Hole
› On the Possibility of Melting Water Ice during the Recent Past of Mars: Application to the Formation of Gullies
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› A User-Friendly Python Interface for Numerical Relativity Program AMSS-NCKU
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