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Non-seismic (and Non-LTE) stellar parameters for the PLATO core sample

Bergemann, Maria


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{
  "description": "<p>Accurate stellar parameters, Teff and chemical composition, are imperative for the determination of masses, radii, and ages of PLATO stars. I will present the architecture and input physics of the SAPP pipeline that will be used to determine non-seismic stellar parameters for the PLATO core sample.<br>\nIn this talk, I will discuss how we cope with rapid yet painstaking developments in stellar atmosphere modelling, including radiation hydrodynamics theory, atomic and molecular physics, machine learning and numerical analysis methods, - the developments that form the basis of the unique diagnostic capabilties of the SAPP. I will highlight our successes and challenges, and close with the prospects for PLATO and other future projects that aim to capitalise on unprecendeted data available from ground- and space-based observations.</p>\n\n<p>&nbsp;</p>", 
  "license": "https://creativecommons.org/licenses/by/4.0/legalcode", 
  "creator": [
    {
      "affiliation": "MPIA, NBIA", 
      "@type": "Person", 
      "name": "Bergemann, Maria"
    }
  ], 
  "url": "https://zenodo.org/record/5568759", 
  "datePublished": "2021-10-14", 
  "@context": "https://schema.org/", 
  "identifier": "https://doi.org/10.5281/zenodo.5568759", 
  "@id": "https://doi.org/10.5281/zenodo.5568759", 
  "@type": "PresentationDigitalDocument", 
  "name": "Non-seismic (and Non-LTE) stellar parameters for the PLATO core sample"
}
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