October 11, 2021 Poster Open Access

de Almeida, Leandro; Velloso, Eduardo Nunes; do Nascimento, José Dias Jr; Silva, Francys Anthony da; Costa, Jefferson Soares da; Samadi, Réza

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  <identifier identifierType="DOI">10.5281/zenodo.5560822</identifier>
  <creators>
    <creator>
      <creatorName>de Almeida, Leandro</creatorName>
      <givenName>Leandro</givenName>
      <familyName>de Almeida</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0001-8179-1147</nameIdentifier>
      <affiliation>Laboratório Nacional de Astrofísica, Rua Estados Unidos 154, 37504-364, Itajubá - MG, Brazil</affiliation>
    </creator>
    <creator>
      <creatorName>Velloso, Eduardo Nunes</creatorName>
      <givenName>Eduardo Nunes</givenName>
      <familyName>Velloso</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-9668-5547</nameIdentifier>
      <affiliation>Universidade Federal do Rio Grande do Norte, Natal, RN, Brazil</affiliation>
    </creator>
    <creator>
      <creatorName>do Nascimento, José Dias Jr</creatorName>
      <givenName>José Dias Jr</givenName>
      <familyName>do Nascimento</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0001-7804-2145</nameIdentifier>
      <affiliation>Departamento de Física Teórica e Experimental, Universidade Federal do Rio Grande do Norte, Natal, RN, Brazil</affiliation>
    </creator>
    <creator>
      <creatorName>Silva, Francys Anthony da</creatorName>
      <givenName>Francys Anthony da</givenName>
      <familyName>Silva</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0003-1963-636X</nameIdentifier>
      <affiliation>Departamento de Física Teórica e Experimental, Universidade Federal do Rio Grande do Norte, Natal, RN, Brazil</affiliation>
    </creator>
    <creator>
      <creatorName>Costa, Jefferson Soares da</creatorName>
      <givenName>Jefferson Soares da</givenName>
      <familyName>Costa</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-9830-0495</nameIdentifier>
      <affiliation>Escola de Ciências e Tecnologia, ECT, Universidade Federal do Rio Grande do Norte, Natal, RN, Brazil</affiliation>
    </creator>
    <creator>
      <creatorName>Samadi, Réza</creatorName>
      <givenName>Réza</givenName>
      <familyName>Samadi</familyName>
      <affiliation>LESIA, Observatoire de Paris, Université PSL, CNRS, Sorbonne Université, Univ. Paris Diderot, Sorbonne, Paris Cité, France</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Unraveling Solar analogs from PLATO mission: Rotation and activity recovery from simulated light curves</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2021</publicationYear>
  <subjects>
    <subject>Rotation modulation</subject>
    <subject>Transits</subject>
    <subject>Light Curve</subject>
  </subjects>
  <dates>
    <date dateType="Issued">2021-10-11</date>
  </dates>
  <language>en</language>
  <resourceType resourceTypeGeneral="Text">Poster</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/5560822</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.5560821</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/plato2021</relatedIdentifier>
  </relatedIdentifiers>
  <version>V1</version>
  <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;We performed a validation exercise to recover the rotational modulation for 1,000 simulated PLATO light curves. We created a powerful simulation tool built upon the PLATO Solar-like Light-curve Simulator combining astrophysical (starspot rotation and evolution, planetary transits, oscillations, and granulations) and systematic instrumental effects. The simulated light curves follow specifications from the PLATO telescope in order to closely reproduce the expected raw data. We present a method of stitching and detrending to recover the original signal while also separating the rotational signal from the transit/eclipsing one. We find that a precise determination of rotation periods using this pre-processing pipeline is possible at every level of activity. From the stars with clear rotation determination, 92% of the values we recover are within the 10% confidence interval of the inputs.&lt;/p&gt;</description>
    <description descriptionType="Other">{"references": ["de Almeida, L. et al. 2020 https://doi.org/10.1007/s10686-020-09664-x", "Samadi, R. et al. 2019  https://doi.org/10.1051/0004-6361/201834822"]}</description>
  </descriptions>
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