An effective temperature calibration for solar type stars using equivalent width ratios - A fast and easy spectroscopic temperature estimation

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Table 1:

Spectral lines added to the lists of lines presented in Sousa et al. (2008) and in Neves et al. (2009).
$\lambda$ (Å)	$\chi_{l}$	$\log{gf}$	Ele.
6318.72	5.11	-1.996	MgI
5621.60	5.08	-2.500	SiI
5690.43	4.93	-1.790	SiI
6414.99	5.87	-1.100	SiI
6583.71	5.95	-1.640	SiI
6604.60	1.36	-1.160	ScII
5866,45	1.07	-0.840	TiI
6330.13	0.94	-2,92	CrI
5703.59	1.05	-0.460	VI
5727.05	1.08	0.000	VI
6039.73	1.06	-0.650	VI
6090.21	1.08	-0.150	VI
6111.65	1.04	-0.715	VI
6135.36	1.05	-0.746	VI
6216.35	0.28	-0.900	VI
5578.72	1.68	-2.650	NiI
5682.20	4.10	-0.39	NiI
5754.68	1.94	-2.33	NiI
6007.31	1.68	-3.330	NiI

Source LaTeX | All tables | In the text

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