Gaia FGK Benchmark Stars - Metallicity
| hal.structure.identifier | M2A 2014 | |
| dc.contributor.author | JOFRE, P. | |
| dc.contributor.author | HEITER, U. | |
| hal.structure.identifier | M2A 2014 | |
| dc.contributor.author | SOUBIRAN, C. | |
| hal.structure.identifier | M2A 2014 | |
| dc.contributor.author | BLANCO-CUARESMA, S. | |
| dc.contributor.author | PANCINO, E. | |
| dc.contributor.author | BERGEMANN, M. | |
| dc.contributor.author | CANTAT-GAUDIN, T. | |
| dc.contributor.author | HERNÁNDEZ, J. I. González | |
| dc.contributor.author | HILL, V. | |
| dc.contributor.author | LARDO, C. | |
| dc.contributor.author | DE LAVERNY, P. | |
| dc.contributor.author | LIND, K. | |
| dc.contributor.author | MAGRINI, L. | |
| dc.contributor.author | MASSERON, T. | |
| dc.contributor.author | MONTES, D. | |
| dc.contributor.author | MUCCIARELLI, A. | |
| dc.contributor.author | NORDLANDER, T. | |
| dc.contributor.author | RECIO-BLANCO, A. | |
| dc.contributor.author | SOBECK, J. | |
| dc.contributor.author | SORDO, R. | |
| dc.contributor.author | SOUSA, S. G. | |
| dc.contributor.author | TABERNERO, H. | |
| dc.contributor.author | VALLENARI, A. | |
| dc.contributor.author | VAN ECK, S. | |
| dc.contributor.author | WORLEY, C. C. | |
| dc.date.created | 2013-09-04 | |
| dc.date.issued | 2014 | |
| dc.identifier.issn | 0004-6361 | |
| dc.description.abstractEn | To calibrate automatic pipelines that determine atmospheric parameters of stars, one needs a sample of stars -- ''benchmark stars'' -- with well defined parameters to be used as a reference We provide a detailed documentation of the determination of the iron abundance of the 34 FGK-type benchmark stars selected to be the pillars for calibration of the one billion Gaia stars. They cover a wide range of temperatures, surface gravities and metallicities. Up to seven different methods were used to analyze an observed spectral library of high resolution and high signal-to-noise ratio. The metallicity was determined assuming a value of effective temperature and surface gravity obtained from fundamental relations, i.e. these parameters were known a priori independently from the spectra. We present a set of metallicity values obtained in a homogeneous way for our sample of Benchmark Stars. In addition to this value, we provide a detailed documentation of the associated uncertainties. Finally, we report for the first time a value of the metallicity of the cool giant psi Phe. | |
| dc.language.iso | en | |
| dc.publisher | EDP Sciences | |
| dc.subject.en | Galaxy Astrophysics | |
| dc.subject.en | Astrophysics | |
| dc.subject.en | Solar and Stellar Astrophysics | |
| dc.title.en | Gaia FGK Benchmark Stars - Metallicity | |
| dc.type | Article de revue | |
| dc.identifier.doi | 10.1051/0004-6361/201322440 | |
| dc.subject.hal | Physique [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR] | |
| dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Astrophysique stellaire et solaire [astro-ph.SR] | |
| dc.identifier.arxiv | 1309.1099 | |
| bordeaux.journal | Astronomy and Astrophysics - A&A | |
| bordeaux.page | id.A133 | |
| bordeaux.volume | 564 | |
| bordeaux.peerReviewed | oui | |
| hal.identifier | hal-00858346 | |
| hal.version | 1 | |
| hal.popular | non | |
| hal.audience | Internationale | |
| hal.origin.link | https://hal.archives-ouvertes.fr//hal-00858346v1 | |
| bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Astronomy%20and%20Astrophysics%20-%20A&A&rft.date=2014&rft.volume=564&rft.spage=id.A133&rft.epage=id.A133&rft.eissn=0004-6361&rft.issn=0004-6361&rft.au=JOFRE,%20P.&HEITER,%20U.&SOUBIRAN,%20C.&BLANCO-CUARESMA,%20S.&PANCINO,%20E.&rft.genre=article |
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