Table 2: Spectral lines having their origin mainly in the primary and spectral lines with the strongest contributions of the secondary (wavelength in Å, ions, and RMT number of transition).

primary			secondary
5183.604	Mg I	2	6102.722	Ca I	3
5528.398	Mg I	9	6122.219	Ca I	3
5275.994	Fe II	49	4957.453	Fe I	318
5284.092	Fe II	41	5615.652	Fe I	686
5316,693	Fe II	48+49	5658.684	Fe I	685
4911.205	Ti II	114
5226.534	Ti II	70