Poster Open Access
<?xml version='1.0' encoding='UTF-8'?> <record xmlns="http://www.loc.gov/MARC21/slim"> <leader>00000nam##2200000uu#4500</leader> <controlfield tag="005">20211011121159.0</controlfield> <controlfield tag="001">5560090</controlfield> <datafield tag="856" ind1="4" ind2=" "> <subfield code="s">1599218</subfield> <subfield code="z">md5:28c8b69537478deb7dddd7d1b4b294c6</subfield> <subfield code="u">https://zenodo.org/record/5560090/files/RojasAyala_poster_PLATO2021_18_32.pdf</subfield> </datafield> <datafield tag="542" ind1=" " ind2=" "> <subfield code="l">open</subfield> </datafield> <datafield tag="260" ind1=" " ind2=" "> <subfield code="c">2021-10-11</subfield> </datafield> <datafield tag="909" ind1="C" ind2="O"> <subfield code="p">openaire</subfield> <subfield code="p">user-plato2021</subfield> <subfield code="o">oai:zenodo.org:5560090</subfield> </datafield> <datafield tag="100" ind1=" " ind2=" "> <subfield code="u">IAI-UTA</subfield> <subfield code="0">(orcid)0000-0002-0149-1302</subfield> <subfield code="a">Rojas-Ayala, Bárbara</subfield> </datafield> <datafield tag="245" ind1=" " ind2=" "> <subfield code="a">Stellar Parameters Via Spectrum Synthesis Of APOGEE DR 16 H-band Spectra Of M Dwarf Stars</subfield> </datafield> <datafield tag="980" ind1=" " ind2=" "> <subfield code="a">user-plato2021</subfield> </datafield> <datafield tag="540" ind1=" " ind2=" "> <subfield code="u">https://creativecommons.org/licenses/by/4.0/legalcode</subfield> <subfield code="a">Creative Commons Attribution 4.0 International</subfield> </datafield> <datafield tag="650" ind1="1" ind2="7"> <subfield code="a">cc-by</subfield> <subfield code="2">opendefinition.org</subfield> </datafield> <datafield tag="520" ind1=" " ind2=" "> <subfield code="a"><p>We present a method to derive stellar parameters for M dwarfs using high-resolution H-band spectra via spectrum synthesis using <em>iSpec</em>, <em>Turbospectrum</em>, <em>MARCS</em> 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<sub>eff</sub>, [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.</p></subfield> </datafield> <datafield tag="773" ind1=" " ind2=" "> <subfield code="n">doi</subfield> <subfield code="i">isVersionOf</subfield> <subfield code="a">10.5281/zenodo.5560089</subfield> </datafield> <datafield tag="024" ind1=" " ind2=" "> <subfield code="a">10.5281/zenodo.5560090</subfield> <subfield code="2">doi</subfield> </datafield> <datafield tag="980" ind1=" " ind2=" "> <subfield code="a">poster</subfield> </datafield> </record>
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