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iSpec: Stellar atmospheric parameters and chemical abundances

hal.structure.identifierM2A 2014
dc.contributor.authorBLANCO-CUARESMA, S.
hal.structure.identifierM2A 2014
dc.contributor.authorSOUBIRAN, C.
dc.contributor.authorHEITER, U.
hal.structure.identifierM2A 2014
dc.contributor.authorJOFRE, P.
dc.date.issued2014-09
dc.descriptionAstrophysics Source Code Library, record ascl:1409.006
dc.description.abstractEniSpec is an integrated software framework written in Python for the treatment and analysis of stellar spectra and abundances. Spectra treatment functions include cosmic rays removal, continuum normalization, resolution degradation, and telluric lines identification. It can also perform radial velocity determination and correction and resampling. iSpec can also determine atmospheric parameters (i.e effective temperature, surface gravity, metallicity, micro/macroturbulence, rotation) and individual chemical abundances by using either the synthetic spectra fitting technique or equivalent widths method. The synthesis is performed with SPECTRUM (ascl:9910.002).
dc.language.isoen
dc.title.eniSpec: Stellar atmospheric parameters and chemical abundances
dc.typeAutre document
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
bordeaux.page09006
hal.identifierhal-01071925
hal.version1
hal.audienceNon spécifiée
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01071925v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2014-09&rft.spage=09006&rft.epage=09006&rft.au=BLANCO-CUARESMA,%20S.&SOUBIRAN,%20C.&HEITER,%20U.&JOFRE,%20P.&rft.genre=unknown


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