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Table 4

Results of multiple analyses of solar spectra in the Gaia-ESO Survey for the iDR2 and iDR3 cycles.

Spectrograph Cycle T eff log  g [Fe/H] ξ log ϵ(Na) log ϵ(Al)
(K) (dex) (dex) (km s-1) (dex) (dex)

FLAMES/UVES iDR2 5826 ± 40 4.50 ± 0.05 0.03 ± 0.12 1.05 ± 0.00 6.31 ± 0.05 6.44 ± 0.01
FLAMES/UVES iDR3 5797 ± 85 4.45 ± 0.11 0.03 ± 0.03 0.70 ± 0.25 6.27 ± 0.07 6.43 ± 0.09
NARVAL iDR2 5810 ± 17 4.50 ± 0.08 0.00 ± 0.04 1.06 ± 0.08 6.29 ± 0.02 6.46 ± 0.01
NARVAL iDR3 5785 ± 40 4.44 ± 0.14 0.03 ± 0.12 0.94 ± 0.20 6.30 ± 0.13 6.43 ± 0.04
UVES stand-alone iDR2 5777 ± 31 4.43 ± 0.13 0.00 ± 0.06 1.04 ± 0.16 6.28 ± 0.02 6.45 ± 0.03
UVES stand-alone iDR3 5774 ± 25 4.43 ± 0.10 0.04 ± 0.04 0.95 ± 0.17 6.33 ± 0.07 6.44 ± 0.05

Average 5795 ± 20 4.46 ± 0.03 0.01 ± 0.03 0.96 ± 0.14 6.30 ± 0.02 6.44 ± 0.01

Notes. The metallicities, [Fe/H], are given with respect to log ϵ(Fe) = 7.45 from Grevesse et al. (2007).

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