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Table 3

A selection of the strongest Ni xii lines.

ij Levels Int gf Aji (s-1) λexp (Å) λth (Å)

1–29 3s2 3p52P3/2–3s2 3p4 3d 2D5/2 1.0 4.35 2.1×1011 152.151 152.32
1–28 3s2 3p52P3/2–3s2 3p4 3d 2P3/2 0.58 (0.49) 2.50 1.8×1011 154.171 154.14
1–27 3s2 3p52P3/2–3s2 3p4 3d 2S1/2 0.25 (0.21) 1.17 1.5×1011 160.556 160.54
1–5 3s2 3p52P3/2–3s2 3p4 3d 4D7/2 0.20 (0.06) 91. 220.247 221.87 T
1–3 3s2 3p52P3/2–3s 3p62S1/2 0.14 (0.09) 0.13 5.1×109 295.321 295.10
1–4 3s2 3p52P3/2–3s2 3p4 3d 4D5/2 6.6 (2.4)×10-2 3.7×10-4 8.3×106 220.870 222.40 T
2–27 3s2 3p52P1/2–3s2 3p4 3d 2S1/2 6.2 (6.0)×10-2 0.31 3.7×1010 166.887 167.09
2–30 3s2 3p52P1/2–3s2 3p4 3d 2P1/2 5.6 (8.2)×10-2 1.00 1.3×1011 157.796 157.65
1–19 3s2 3p52P3/2–3s2 3p4 3d 2D5/2 4.8 (1.3)×10-2 6.1×10-3 1.8×108 194.73
1–17 3s2 3p52P3/2–3s2 3p4 3d 4P5/2 4.3 (0.6)×10-2 4.6×10-3 1.3×108 196.56
1–22 3s2 3p52P3/2–3s2 3p4 3d 2F5/2 3.9 (0.7)×10-2 9.5×10-4 3.0×107 189.02
2–31 3s2 3p52P1/2–3s2 3p4 3d 2D3/2 4.0 (13)×10-2 2.79 2.0×1011 152.697 152.92 T
2–3 3s2 3p52P1/2–3s 3p62S1/2 6.1 (4.0)×10-2 6.5×10-2 2.2×109 317.474 318.04
1–2 3s2 3p52P3/2–3s2 3p52P1/2 0.57 (0.65) 2.6×102 4232.09 4091.00
5–9 3s2 3p4 3d 4D7/2–3s2 3p4 3d 4F9/2 9.4 (3.4)×10-2 28. 3171.18 3014.08
9–21 3s2 3p4 3d 4F9/2–3s2 3p4 3d 2G9/2 3.8 (1.4)×10-2 2.0×102 2398.08 2258.57
5–18 3s2 3p4 3d 4D7/2–3s2 3p4 3d 2F7/2 2.5 (0.47)×10-2 90. 1686.74 1661.20
5–10 3s2 3p4 3d 4D7/2–3s2 3p4 3d 4F7/2 1.9 (0.66)×10-2 18. 2580.38 2492.77
9–18 3s2 3p4 3d 4F9/2–3s2 3p4 3d 2F7/2 1.8 (0.30)×10-2 57. 3603.34 3701.00
10–20 3s2 3p4 3d 4F7/2–3s2 3p4 3d 2G7/2 1.3 (0.28)×10-2 84. 2923.12 2783.65
9–24 3s2 3p4 3d 4F9/2–3s2 3p4 3d 2F7/2 1.1 (0.37)×10-2 2.3×102 1225.05 1235.02
3–462 3s 3p62S1/2–3s 3p5 4s 2P3/2 1.9×10-2 0.25 8.0×1010 72.52
1–282 3s2 3p52P3/2–3s2 3p4 4s 2D5/2 1.2×10-2 0.30 6.7×1010 71.378 71.39
1–262 3s2 3p52P3/2–3s2 3p4 4s 2P3/2 1.1×10-2 0.45 1.4×1011 72.770 72.87
1–435 3s2 3p52P3/2–3s2 3p4 4d 2D5/2 5.8×10-3 1.00 3.1×1011 60.020 60.07
1–246 3s2 3p52P3/2–3s2 3p4 4s 4P3/2 4.5×10-3 0.10 3.0×1010 73.93
1–242 3s2 3p52P3/2–3s2 3p4 4s 4P5/2 3.7×10-3 1.5×10-2 2.9×109 74.60
22–526 3s2 3p4 3d 2F5/2–3s2 3p4 4f 2G7/2 3.1×10-3 2.33 3.3×1011 76.38
2–283 3s2 3p52P1/2–3s2 3p4 4s 2D3/2 2.4×10-3 0.27 8.6×1010 72.570 72.57
2–273 3s2 3p52P1/2–3s2 3p4 4s 2P1/2 2.4×10-3 0.17 1.0×1011 73.423 73.45
9–483 3s2 3p4 3d 4F9/2–3s2 3p4 4f 4G11/2 2.3×10-3 6.47 6.3×1011 75.618 75.73
1–273 3s2 3p52P3/2–3s2 3p4 4s 2P1/2 2.1×10-3 0.15 9.3×1010 72.171 72.15
14–498 3s2 3p4 3d 4F5/2–3s2 3p4 4f 4G7/2 2.1×10-3 2.33 3.4×1011 75.78
5–477 3s2 3p4 3d 4D7/2–3s2 3p4 4f 4F9/2 1.9×10-3 4.44 5.4×1011 74.440 74.35

Notes. Column 3 shows the relative intensities (photons) I = NjAji/Ne of the strongest lines, relative to the main transition. The intensities were calculated at an electron density of 109 cm-3 and log T [K] = 6.25, the temperature of peak ion abundance in equilibrium. Values in brackets are those calculated with the CHIANTI database. Columns 4 and 5 show the gf and A values calculated in this work with TECs. The λexp (Å) are our experimental wavelengths (in vacuum), while the λth (Å) values are our theoretical values obtained with the TECs. A “T” in the last column indicates a tentative new experimental wavelength.

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