October 11, 2021 Poster Open Access

Rojas-Ayala, Bárbara

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  <dc:creator>Rojas-Ayala, Bárbara</dc:creator>
  <dc:date>2021-10-11</dc:date>
  <dc:description>We present a method to derive stellar parameters for M dwarfs using high-resolution H-band spectra via spectrum synthesis using iSpec, Turbospectrum, MARCS 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 (Teff, [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.</dc:description>
  <dc:identifier>https://zenodo.org/record/5560090</dc:identifier>
  <dc:identifier>10.5281/zenodo.5560090</dc:identifier>
  <dc:identifier>oai:zenodo.org:5560090</dc:identifier>
  <dc:relation>doi:10.5281/zenodo.5560089</dc:relation>
  <dc:relation>url:https://zenodo.org/communities/plato2021</dc:relation>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>https://creativecommons.org/licenses/by/4.0/legalcode</dc:rights>
  <dc:title>Stellar Parameters Via Spectrum Synthesis Of APOGEE DR 16 H-band Spectra Of M Dwarf Stars</dc:title>
  <dc:type>info:eu-repo/semantics/conferencePoster</dc:type>
  <dc:type>poster</dc:type>
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