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A robust, empirical approach to determine line-by-line convective blueshift strengths from F to M stars

Liebing, Florian


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{
  "description": "<p>Presentation slides for a recorded talk for the PLATO Conference 2021.</p>\n\n<p>&nbsp;</p>", 
  "creator": [
    {
      "affiliation": "Institute for Astrophysics, University of G\u00f6ttingen, Germany", 
      "@type": "Person", 
      "name": "Liebing, Florian"
    }
  ], 
  "url": "https://zenodo.org/record/5552141", 
  "datePublished": "2021-10-14", 
  "contributor": [
    {
      "affiliation": "Max Planck Institute for Solar System Research, G\u00f6ttingen, Germany", 
      "@type": "Person", 
      "name": "Jeffers, Sandra"
    }, 
    {
      "affiliation": "Institute for Astrophysics, University of G\u00f6ttingen, Germany", 
      "@type": "Person", 
      "name": "Reiners, Ansgar"
    }, 
    {
      "affiliation": "Institute for Astrophysics, University of G\u00f6ttingen, Germany", 
      "@type": "Person", 
      "name": "Zechmeister, Mathias"
    }
  ], 
  "@context": "https://schema.org/", 
  "identifier": "https://doi.org/10.5281/zenodo.5552141", 
  "@id": "https://doi.org/10.5281/zenodo.5552141", 
  "@type": "PresentationDigitalDocument", 
  "name": "A robust, empirical approach to determine line-by-line convective blueshift strengths from F to M stars"
}
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