October 4, 2021 Poster Open Access

Mortier, A

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  <identifier identifierType="DOI">10.5281/zenodo.5547910</identifier>
  <creators>
    <creator>
      <creatorName>Mortier, A</creatorName>
      <givenName>A</givenName>
      <familyName>Mortier</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0001-7254-4363</nameIdentifier>
      <affiliation>University of Cambridge</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Exploring the variety of small planets with HARPS-N</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2021</publicationYear>
  <dates>
    <date dateType="Issued">2021-10-04</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Poster</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/5547910</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.5547909</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/plato2021</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/licenses/by/4.0/legalcode">Creative Commons Attribution 4.0 International</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;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&amp;#39;s leading efforts to fill and interpret the mass-radius diagram of small planets.&amp;nbsp;&lt;br&gt;
&amp;nbsp;&lt;/p&gt;</description>
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