Gaia FGK benchmark stars: new candidates at low metallicities

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Volume 592 (August 2016)

A&A, 592 (2016) A70

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Table A.1

Online table format.

Column	Label	Unit

(1)	Element
(2)	Absorption line wavelength	Å
(3)	Mean EW	mÅ
(4)	Mean abundance (A)	dex
(5)	NLTE correction^a	dex
(6)	EW (EPI)	mÅ
(7)	EW (BOL)	mÅ
(8)	EW (ULB)	mÅ
(9)	EW (iSpec)	mÅ
(10)	A(EPI)	dex
(11)	A(BOL)	dex
(12)	A(ULB)	dex
(13)	A(iSpec)	dex

Notes. This table is only available in electronic form at CDS. For the EW and abundances, the node is noted in the parentheses. For example EW (EPI) denotes the EW measurement of a specific line from the EPINARBO node while A(BOL) is the log(abundance) of a specific line for the Bologna node.

^(a)

In the online table, the lines with NLTE corrections of −0.000 are those that do not have corrections available. This is done for identification purposes. In these cases, the median of the NLTE corrections of the other lines is assumed.

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