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Benchmark stars for cross-calibration of Galactic stellar surveys

dc.contributor.authorHEITER, U.
dc.contributor.authorJOFRÉ, P.
hal.structure.identifierUppsala Astronomical 0bservatory [UAO]
dc.contributor.authorGUSTAFSSON, B.
dc.contributor.authorTHÉVENIN, F.
dc.contributor.authorKORN, A.
hal.structure.identifierM2A 2015
dc.contributor.authorSOUBIRAN, C.
hal.structure.identifierM2A 2015
dc.contributor.authorBLANCO-CUARESMA, S.
hal.structure.identifierUniversity of Amsterdam [Amsterdam] = Universiteit van Amsterdam [UvA]
dc.contributor.authorWALTON, N.A.
hal.structure.identifierBIOVERT [BIOVERT]
dc.contributor.authorFIGUERAS, F.
dc.contributor.authorBALAGUER-NÚÑEZ, L.
dc.date.issued2015
dc.date.conference2014-12-01
dc.description.abstractEnVarious Galactic stellar spectroscopic surveys are currently underway, and each is expected to achieve high internal accuracy in terms of stellar parameters and abundances. A number of questions related to the formation and evolution of the Galaxy may be addressed based on samples of stars observed within each survey. In addition, complementary samples of stars may be constructed by combining data from different surveys. The Gaia FGK Benchmark Stars provide the necessary link to bring the quantities measured from different spectra with different methods onto the same scale. We selected 28 FGK stars and 5 M giants with available angular diameter θ, bolometric flux Fbol, and distance. We used the fundamental relation Teff ∝ F/θ0.5 to determine a reference effective temperature. We used the fundamental relation g ∝ M/R2, where M is the mass and R the radius, to determine a reference surface gravity. A homogeneous analysis of a high resolution and high signal-to-noise spectral library provides a reference metallicity (Blanco-Cuaresma et al. 2014A&A...566A..98B, Jofré et al. 2014A&A...564A.133J). These stars serve as a reference for testing and homogenizing large stellar surveys such as the Gaia mission and the Gaia-ESO public spectroscopic survey and for improving models of FGK-star atmospheres. A detailed discussion of the fundamental Teff and logg values will be presented in Heiter et al. (to be submitted).
dc.language.isoen
dc.title.enBenchmark stars for cross-calibration of Galactic stellar surveys
dc.typeCommunication dans un congrès
dc.identifier.doi10.1051/eas/1567074
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Instrumentation et méthodes pour l'astrophysique [astro-ph.IM]
bordeaux.page375-375
bordeaux.volume67-68
bordeaux.conference.title- Published online: 17 July 2015 - DOI: http://dx.doi.org/10.1051/eas/1567074 EAS Publications Series - Vol. 67-68 (2014) - Barcelona, Spain, December 1–5, 2014 N.A. Walton, F. Figueras, L. Balaguer-Núñez and C. Soubiran (Eds.) - ISBN: 978-2-7598-1826-6
bordeaux.countryES
bordeaux.conference.cityBarcelona
bordeaux.peerReviewedoui
hal.identifierhal-01198908
hal.version1
hal.invitednon
hal.proceedingsnon
hal.conference.end2014-12-05
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01198908v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2015&rft.volume=67-68&rft.spage=375-375&rft.epage=375-375&rft.au=HEITER,%20U.&JOFR%C3%89,%20P.&GUSTAFSSON,%20B.&TH%C3%89VENIN,%20F.&KORN,%20A.&rft.genre=unknown


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