The Gaia-ESO Survey: a new approach to chemically characterising young open clusters - I. Stellar parameters, and iron-peak, α-, and proton-capture elements

M. Baratella; V. D’Orazi; G. Carraro; S. Desidera; S. Randich; L. Magrini; V. Adibekyan; R. Smiljanic; L. Spina; M. Tsantaki; G. Tautvaišienė; S. G. Sousa; P. Jofré; F. M. Jiménez-Esteban; E. Delgado-Mena; S. Martell; M. Van der Swaelmen; V. Roccatagliata; G. Gilmore; E. J. Alfaro; A. Bayo; T. Bensby; A. Bragaglia; E. Franciosini; A. Gonneau; U. Heiter; A. Hourihane; R. D. Jeffries; S. E. Koposov; L. Morbidelli; L. Prisinzano; G. Sacco; L. Sbordone; C. Worley; S. Zaggia; J. Lewis

doi:10.1051/0004-6361/201937055

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Volume 634 (February 2020)

A&A, 634 (2020) A34

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Table 3

Atmospheric parameters and chemical composition of Gaia benchmarks stars.

Notes. We also report the value from the literature (i.e. ξ values from Jofré et al. 2015 -J15-, while T_eff, log g, [Fe/H] and [Ti/H] are from Jofré et al. 2018 -J18-) and from the Gaia-ESO iDR5 catalogue (GESiDR5). The numbers of the lines we used in the analysis are in square brackets. The uncertainties are calculated as the quadratic sum of the σ₁ and σ₂ contributions (see Sect. 4.4 for details). ^(*)The solar values are in log(X) scale.

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