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Table 3

Strategic lines and determined element abundances (mass fraction, error ± 0.2 dex).

Element Analyzed lines Abundance [X]

H optical H i lines 9 .12 × 10-1 0 .00
He optical He i–ii lines 7 .93 × 10-2 −0 .50
C C III λλ 1174 − 1176 Å C IV λλ 1118.41,1122.49,1168 − 1169 Å <1.04 × 10-7 <−4.36
N N III λλ 1182.97,1183.03,1184.51,1184.57 Å N III λλ 3998.63,4003.58,4379.11,4510.91,4514.86,4634.14,4640.64 Å N IV λλ 921.99,922.52,923.06,923.22,923.68,924.28 Å N V λλ 1238.82,1242.80 Å 1 .56 × 10-4 −0 .65
O O III λ 1153.78 Å O IV λλ 921.30,921.36,923.37,923.43 Å <1.78 × 10-6 <−3.51
Si Si III λ 1113.23 Å Si IV λ 1122.49 Å <3.96 × 10-7 <−3.23
P P IV λλ 1025.56,1028.09,1030.51,1030.51,1033.11,1035.52 Å P V λλ 1117.98,1128.01 Å 6 .67 × 10-6 0 .06
S S IV λλ 1062.66,1072.97,1073.52,1098.93,1099.48 Å S V λλ 1039.92,1122.03,1128.67,1128.78 Å S VI λλ 933.38,944.52 Å 9 .77 × 10-5 −0 .50
Ca optical Ca iv lines <9.27 × 10-5 <0.16
Sc Sc IV λ 931.42 Å Sc V λλ 939.40,944.04 Å <3.08 × 10-4 <3.82
Ti optical Ti iv lines, Ti IV λ 1183.63 Å Ti V λλ 1153.28,1163.52 Å 1 .77 × 10-4 2 .24
V V IV λ 1131.25 Å V V λλ 978.16,1142.74,1157.58 Å 5 .50 × 10-5 2 .06
Cr many Cr iv–vi lines in the FUV, e.g. Cr IV λλ 1043.46,1065.26,1072.10,1096.64,1126.35 Å Cr V λλ 1031.10,1035.04,1042.55,1045.04,1060.65 Å Cr VI λ 957.01 Å 1 .92 × 10-3 2 .06
Mn Mn V λλ 1040.04,1043.65,1048.63,1049.43,1055.98,1062.49,1172.06 Å Mn VI λλ 1081.09,1113.58 Å 1 .92 × 10-3 2 .25
Fe many Fe v–vi lines in the FUV, e.g. Fe V λλ 1002.87,1015.33,1020.36 Å Fe VI λλ 1000.93,1167.70 Å 1 .08 × 10-3 −0 .08
Co many Co v–vi lines in the FUV, e.g. Co V λλ 1179.59,1183.91,1184.60 Å Co VI λλ 1133.71,1142.77,1150.23,1169.55,1175.36 Å 8 .72 × 10-4 2 .32
Ni many Ni v–vi lines in the FUV, e.g. Ni V λλ 1124.30,1178.92 Å Ni VI λλ 1000.39,1157.55,1159.00,1178.37 Å 2 .28 × 10-3 1 .51
Zn Zn V λλ 1116.84,1120.33,1158.76 Å 9 .08 × 10-5 1 .72
Ge Ge V λλ 1016.67,1069.13,1072.66,1116.95,1165.26 Å 5 .38 × 10-5 2 .36

Notes. [X] = log (abundance/solar abundance) of species X (solar values from Asplund et al. 2009).

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