October 8, 2021 Presentation Open Access

Amaury H.M.J.Triaud

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  <identifier identifierType="DOI">10.5281/zenodo.5557315</identifier>
  <creators>
    <creator>
      <creatorName>Amaury H.M.J.Triaud</creatorName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-5510-8751</nameIdentifier>
      <affiliation>University of Birmingham</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Confirming &amp; detecting circumbinary planets using radial-velocities.</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2021</publicationYear>
  <subjects>
    <subject>Exoplanets</subject>
    <subject>Circumbinary exoplanets</subject>
    <subject>Binary stars</subject>
    <subject>PLATO</subject>
    <subject>Radial-velocities</subject>
    <subject>Antarctica</subject>
    <subject>Transit</subject>
  </subjects>
  <dates>
    <date dateType="Issued">2021-10-08</date>
  </dates>
  <language>en</language>
  <resourceType resourceTypeGeneral="Text">Presentation</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/5557315</alternateIdentifier>
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    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.5557314</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>
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  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;Thanks to its long photometric stares, PLATO will likely identify multiple&amp;nbsp;transiting circumbinary planets. However the duration of its long stares are&amp;nbsp;insufficient to measure circumbinary planet masses accurately using eclipse&amp;nbsp;timing variations of the central binary. In this talk I show our efforts&amp;nbsp;on HARPS and SOPHIE to detect circumbinary planets orbiting single-lined&amp;nbsp;eclipse binaries. I will show the first ground-based detections of&amp;nbsp;circumbinary planets made by SOPHIE, HARPS in radial-velocities, and the&lt;br&gt;
first circumbinary planet transit obtained from ground, using ASTEP in&amp;nbsp;Antarctica. The methods we are developing are key to prepare for the&amp;nbsp;confirmation of PLATO&amp;#39;s circumbinary planets.&lt;br&gt;
&lt;br&gt;
&amp;nbsp;&lt;/p&gt;</description>
  </descriptions>
  <fundingReferences>
    <fundingReference>
      <funderName>European Commission</funderName>
      <funderIdentifier funderIdentifierType="Crossref Funder ID">10.13039/100010661</funderIdentifier>
      <awardNumber awardURI="info:eu-repo/grantAgreement/EC/H2020/803193/">803193</awardNumber>
      <awardTitle>Binaries Escorted By Orbiting Planets</awardTitle>
    </fundingReference>
    <fundingReference>
      <funderName>Research Councils UK</funderName>
      <funderIdentifier funderIdentifierType="Crossref Funder ID">10.13039/501100000690</funderIdentifier>
      <awardNumber awardURI="info:eu-repo/grantAgreement/RCUK/STFC/ST%2FS00193X%2F1/">ST/S00193X/1</awardNumber>
      <awardTitle>Red-enhanced cameras to seek rocky planets transiting Ultra-Cool Dwarfs</awardTitle>
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