October 10, 2021 Poster Open Access

Lacedelli Gaia; Malavolta Luca; Borsato Luca; Piotto Giampaolo; Nardiello Domenico; the HARPS-N team; the CHEOPS team

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  <identifier identifierType="DOI">10.5281/zenodo.5559862</identifier>
  <creators>
    <creator>
      <creatorName>Lacedelli Gaia</creatorName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-4197-7374</nameIdentifier>
      <affiliation>Università degli Studi di Padova, INAF-OAPD</affiliation>
    </creator>
    <creator>
      <creatorName>Malavolta Luca</creatorName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-6492-2085</nameIdentifier>
      <affiliation>Università degli Studi di Padova, INAF-OAPD</affiliation>
    </creator>
    <creator>
      <creatorName>Borsato Luca</creatorName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0003-0066-9268</nameIdentifier>
      <affiliation>INAF-OAPD</affiliation>
    </creator>
    <creator>
      <creatorName>Piotto Giampaolo</creatorName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-9937-6387</nameIdentifier>
      <affiliation>Università degli Studi di Padova, INAF-OAPD</affiliation>
    </creator>
    <creator>
      <creatorName>Nardiello Domenico</creatorName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0003-1149-3659</nameIdentifier>
      <affiliation>Laboratoire d'Astrophysique de Marseille</affiliation>
    </creator>
    <creator>
      <creatorName>the HARPS-N team</creatorName>
    </creator>
    <creator>
      <creatorName>the CHEOPS team</creatorName>
    </creator>
  </creators>
  <titles>
    <title>CHEOPS, HARPS-N and TESS: a joint effort to characterize the unexpected planetary system around TOI-561</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2021</publicationYear>
  <subjects>
    <subject>Exoplanets</subject>
    <subject>Exoplanets Detection And Characterization</subject>
    <subject>Transits</subject>
    <subject>Radial Velocity</subject>
    <subject>TOI-561</subject>
  </subjects>
  <dates>
    <date dateType="Issued">2021-10-10</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Poster</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/5559862</alternateIdentifier>
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  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo" resourceTypeGeneral="Text">10.5281/zenodo.5123553</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsDocumentedBy">10.1093/mnras/staa3728</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.5559861</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;Well-characterized multiplanetary systems offer a unique opportunity for comparative planetology, allowing for investigations of the formation and evolution processes.&amp;nbsp;I will present the analysis of a new multiplanetary system, TOI-561, initially discovered by the&amp;nbsp;TESS&amp;nbsp;mission through photometric observations, and further characterized using high-precision RV data collected with the HARPS-N spectrograph, that allowed us to obtain precise masses for all the four planets in the system, namely an ultra-short period super-Earth and three mini-Neptunes (Lacedelli et al. 2021).&amp;nbsp; I will show how in this case combining photometric and RV data has been essential to discriminate between various possible architectures, highlighting the importance of combining different techniques to obtain a better characterization of a planetary system. Additional insights on the planetary architecture and internal structure are coming from the ultra-high precision photometry of the CHEOPS satellite (Lacedelli et al., in prep), which additionally stresses the importance of synergies between various techniques and instruments.&lt;/p&gt;</description>
  </descriptions>
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