The Gaia-ESO Survey: radial metallicity gradients and age-metallicity relation of stars in the Milky Way disk

M. Bergemann; G. R. Ruchti; A. Serenelli; S. Feltzing; A. Alves-Brito; M. Asplund; T. Bensby; P. Gruiters; U. Heiter; A. Hourihane; A. Korn; K. Lind; A. Marino; P. Jofre; T. Nordlander; N. Ryde; C. C. Worley; G. Gilmore; S. Randich; A. M. N. Ferguson; R. D. Jeffries; G. Micela; I. Negueruela; T. Prusti; H.-W. Rix; A. Vallenari; E. J. Alfaro; C. Allende Prieto; A. Bragaglia; S. E. Koposov; A. C. Lanzafame; E. Pancino; A. Recio-Blanco; R. Smiljanic; N. Walton; M. T. Costado; E. Franciosini; V. Hill; C. Lardo; P. de Laverny; L. Magrini; E. Maiorca; T. Masseron; L. Morbidelli; G. Sacco; G. Kordopatis; G. Tautvaišienė

doi:10.1051/0004-6361/201423456

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Volume 565 (May 2014)

A&A, 565 (2014) A89

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Fig. A.1

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Top four panels: stellar parameters recovered by BeSPP for the ideal synthetic stellar sample drawn from the tracks (see text). Bottom four panels: stellar parameters (T_eff, log g, [Fe/H]) recovered by BeSPP compared with the input spectroscopic values for the UVES stars. The total χ² was computed summing over the three spectroscopic parameters and using only the observational errors.

This figure is made of several images, please see below:

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