October 4, 2021 Poster Open Access

Mortier, A

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{
  "description": "<p>To understand exoplanetary systems, we can study their mass-radius relationship or lack thereof. Kepler, K2, and TESS discover thousands of exoplanet candidates providing precise transit photometry which are then followed up by ground-based spectroscopy to characterise their masses and internal composition. The expertise gained from this process will be invaluable for the PLATO mission when pushing to longer-period small planets. In this poster, I give an overview of the HARPS-N Collaboration&#39;s leading efforts to fill and interpret the mass-radius diagram of small planets.&nbsp;<br>\n&nbsp;</p>", 
  "license": "https://creativecommons.org/licenses/by/4.0/legalcode", 
  "creator": [
    {
      "affiliation": "University of Cambridge", 
      "@id": "https://orcid.org/0000-0001-7254-4363", 
      "@type": "Person", 
      "name": "Mortier, A"
    }
  ], 
  "url": "https://zenodo.org/record/5547910", 
  "datePublished": "2021-10-04", 
  "@context": "https://schema.org/", 
  "identifier": "https://doi.org/10.5281/zenodo.5547910", 
  "@id": "https://doi.org/10.5281/zenodo.5547910", 
  "@type": "CreativeWork", 
  "name": "Exploring the variety of small planets with HARPS-N"
}