October 11, 2021 Poster Open Access

Rojas-Ayala, Bárbara

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  <identifier identifierType="DOI">10.5281/zenodo.5560090</identifier>
  <creators>
    <creator>
      <creatorName>Rojas-Ayala, Bárbara</creatorName>
      <givenName>Bárbara</givenName>
      <familyName>Rojas-Ayala</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-0149-1302</nameIdentifier>
      <affiliation>IAI-UTA</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Stellar Parameters Via Spectrum Synthesis Of APOGEE DR 16 H-band Spectra Of M Dwarf Stars</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2021</publicationYear>
  <dates>
    <date dateType="Issued">2021-10-11</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Poster</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/5560090</alternateIdentifier>
  </alternateIdentifiers>
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    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.5560089</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;We present a method to derive stellar parameters for M dwarfs using high-resolution H-band spectra via spectrum synthesis using &lt;em&gt;iSpec&lt;/em&gt;, &lt;em&gt;Turbospectrum&lt;/em&gt;, &lt;em&gt;MARCS&lt;/em&gt; models atmospheres, and a custom-made line list including over 1000000 water lines (Sarmento et al. 2021). The method was developed to provide reliable spectroscopic parameters from the spectra of current and future NIR high-resolution spectrographs. We derived the spectroscopic parameters (T&lt;sub&gt;eff&lt;/sub&gt;, [M/H], log g) for a sample of 313 M dwarfs in the APOGEE DR16 and compared them to the ones obtained by ASPCAP and previous values derived from NIR and optical data.&lt;/p&gt;</description>
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