hal.structure.identifier	FORMATION STELLAIRE 2011
dc.contributor.author	BROUILLET, N.
dc.date.issued	2011
dc.description	Workshop GAIA CU8 : Calibration meeting, Bordeaux, 15-16 nov. 2011
dc.description.abstractEn	Work is being done on NARVAL spectra of Arcturus and the Sun with several line lists available in order to define the one most suited for the analysis of AP reference stars already observed with that instrument. This involves much tedious work of visualization to keep or reject lines, and select continuum windows. Definition of good fit to be refined as well as objective criteria to select enough lines for a high quality analysis. Another goal is to select select more lines in Sun and Arcturus which are a priori rejected because they are strongly damped, but which become more relevant in metal poor stars.
dc.language.iso	en
dc.title.en	Optimization of line lists for the analysis of reference stars.
dc.type	Autre document
dc.subject.hal	Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
dc.subject.hal	Physique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR]
bordeaux.page	-
hal.identifier	hal-00669937
hal.version	1
hal.audience	Non spécifiée
hal.origin.link	https://hal.archives-ouvertes.fr//hal-00669937v1
bordeaux.COinS	ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2011&rft.spage=-&rft.epage=-&rft.au=BROUILLET,%20N.&rft.genre=unknown

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Optimization of line lists for the analysis of reference stars.