October 4, 2021 Poster Open Access

Mortier, A

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  <dc:creator>Mortier, A</dc:creator>
  <dc:date>2021-10-04</dc:date>
  <dc:description>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's leading efforts to fill and interpret the mass-radius diagram of small planets. 
 </dc:description>
  <dc:identifier>https://zenodo.org/record/5547910</dc:identifier>
  <dc:identifier>10.5281/zenodo.5547910</dc:identifier>
  <dc:identifier>oai:zenodo.org:5547910</dc:identifier>
  <dc:relation>doi:10.5281/zenodo.5547909</dc:relation>
  <dc:relation>url:https://zenodo.org/communities/plato2021</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by/4.0/legalcode</dc:rights>
  <dc:title>Exploring the variety of small planets with HARPS-N</dc:title>
  <dc:type>info:eu-repo/semantics/conferencePoster</dc:type>
  <dc:type>poster</dc:type>
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