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iSpec: Stellar atmospheric parameters and chemical abundances
hal.structure.identifier | M2A 2014 | |
dc.contributor.author | BLANCO-CUARESMA, S. | |
hal.structure.identifier | M2A 2014 | |
dc.contributor.author | SOUBIRAN, C. | |
dc.contributor.author | HEITER, U. | |
hal.structure.identifier | M2A 2014 | |
dc.contributor.author | JOFRE, P. | |
dc.date.issued | 2014-09 | |
dc.description | Astrophysics Source Code Library, record ascl:1409.006 | |
dc.description.abstractEn | iSpec 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.iso | en | |
dc.title.en | iSpec: Stellar atmospheric parameters and chemical abundances | |
dc.type | Autre document | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM] | |
dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM] | |
bordeaux.page | 09006 | |
hal.identifier | hal-01071925 | |
hal.version | 1 | |
hal.audience | Non spécifiée | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-01071925v1 | |
bordeaux.COinS | ctx_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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