Poster Open Access

Stellar Parameters Via Spectrum Synthesis Of APOGEE DR 16 H-band Spectra Of M Dwarf Stars

Rojas-Ayala, Bárbara


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    <subfield code="a">&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;</subfield>
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