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Table 3

List of the strongest Ni xv lines.

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

CHIANTI

1–20 3s2 3p23P0–3s2 3p 3d 3P1 1.0 1.0 0.83 5.9×1010 176.741 174.21 (–2.5)
1–7 3s2 3p23P0–3s 3p33D1 0.28 0.25 7.7×10-2 1.9×109 298.151 299.60 (1.4)
3–14 3s2 3p23P2–3s 3p33S1 0.26 0.23 0.90 4.1×1010 221.895 219.17 (–2.7)
3–24 3s2 3p23P2–3s2 3p 3d 3D3 0.16 0.11 2.50 7.4×1010 179.273 176.35 (–2.9)
2–14 3s2 3p23P1–3s 3p33S1 0.12 0.11 0.41 2.0×1010 215.925 213.24 (–2.7)
2–23 3s2 3p23P1–3s2 3p 3d 3D1 0.10 9.3×10-2 0.64 4.6×1010 176.105 173.59 (–2.5)
3–20 3s2 3p23P2–3s2 3p 3d 3P1 9.9×10-2 0.10 9.1×10-2 5.8×109 185.727 182.81 (–2.9)
2–11 3s2 3p23P1–3s 3p33P1 8.8×10-2 7.5×10-2 9.2×10-2 2.8×109 269.87 269.66 (–0.2) N
3–12 3s2 3p23P2–3s 3p33P2 6.2×10-2 3.3×10-2 0.26 4.4×109 278.386 278.37 (–0.0)
1–14 3s2 3p23P0–3s 3p33S1 5.4×10-2 4.8×10-2 0.17 8.6×109 209.187 206.92 (–2.3)
1–11 3s2 3p23P0–3s 3p33P1 5.1×10-2 4.3×10-2 4.9×10-2 1.6×109 259.63
3–16 3s2 3p23P2–3s2 3p 3d 3F3 4.9×10-2 2.9×10-2 2.7×10-2 5.8×108 207.49
3–25 3s2 3p23P2–3s2 3p 3d 3D2 5.0×10-2 3.5×10-2 0.89 3.7×1010 178.890 176.19 (–2.7)
4–17 3s2 3p21D2–3s 3p31P1 4.4×10-2 3.9×10-2 0.83 3.7×1010 224.057 221.79 (–2.3)
2–19 3s2 3p23P1–3s2 3p 3d 3P2 4.2×10-2 3.4×10-2 0.62 2.4×1010 184.884 181.81 (–3.1)
4–21 3s2 3p21D2–3s2 3p 3d 1D2 4.0×10-2 2.4×10-2 1.15 4.0×1010 195.536 192.86 (–2.7)
3–19 3s2 3p23P2–3s2 3p 3d 3P2 3.7×10-2 2.7×10-2 0.58 2.2×1010 189.243 186.11 (–3.1)
2–8 3s2 3p23P1–3s 3p33D2 0.11 6.8×10-2 0.15 2.0×109 311.755 312.73 (1.0)
3–9 3s2 3p23P2–3s 3p33D3 8.9×10-2 5.0×10-2 0.17 1.6×109 319.063 320.45 (1.4)
2–7 3s2 3p23P1–3s 3p33D1 5.3×10-2 4.4×10-2 1.6×10-2 3.5×108 312.030 313.03 (1.0)
1–2 3s2 3p23P0–3s2 3p23P1 1.4 1.0 57. 6703.54 6983.71 (280)
2–3 3s2 3p23P1–3s2 3p23P2 0.81 0.61 23. 8026.33 7879.71 (–147)
3–4 3s2 3p23P2–3s2 3p21D2 0.18 9.8×10-2 2.0×102 2818.84 2720.34 (–98.5)
2–4 3s2 3p23P1–3s2 3p21D2 0.17 9.1×10-2 1.9×102 2086.18 2022.21 (–64.0)
2–5 3s2 3p23P1–3s2 3p21S0 4.5×10-2 2.1×10-2 2.6×103 1033.04 1004.17 (–28.9)
7–376 3s 3p33D1–3s 3p2 4s 3P0 1.6×10-2 0.12 2.3×1011 59.59 59.37 (–0.2) N (bl)
20–439 3s2 3p 3d 3P1–3s2 3p 4f 3F2 1.2×10-2 1.3×10-2 1.63 5.4×1011 63.57 62.88 (–0.7) TN
7–328 3s 3p33D1–3s2 3p 4p 3P0 1.0×10-2 1.3×10-2 3.1×10-2 4.7×1010 65.90 65.20 (–0.7) TN
20–328 3s2 3p 3d 3P1–3s2 3p 4p 3P0 8.1×10-3 1.1×10-2 3.5×10-2 3.8×1010 77.73 77.31 (–0.4) TN
1–383 3s2 3p23P0–3s2 3p 4d 3D1 7.5×10-3 7.9×10-3 0.45 4.1×1011 49.58? 49.11 (–0.5)
3–271 3s2 3p23P2–3s2 3p 4s 3P1 4.5×10-3 2.7×10-3 0.20 1.3×1011 58.94
23–439 3s2 3p 3d 3D1–3s2 3p 4f 3F2 3.6×10-3 3.9×10-3 0.52 1.7×1011 63.53
3–389 3s2 3p23P2–3s2 3p 4d 3D3 3.1×10-3 3.1×10-3 1.04 3.9×1011 50.173 49.68 (–0.5)
16–327 3s2 3p 3d 3F3–3s2 3p 4p 3D2 3.1×10-3 3.3×10-3 0.25 6.1×1010 74.11
11–376 3s 3p33P1–3s 3p2 4s 3P0 2.8×10-3 2.3×10-2 4.1×1010 61.23
2–383 3s2 3p23P1–3s2 3p 4d 3D1 2.8×10-3 2.8×10-3 0.17 1.5×1011 49.45
7–439 3s 3p33D1–3s2 3p 4f 3F2 2.6×10-3 2.9×10-3 0.28 1.2×1011 54.63
1–271 3s2 3p23P0–3s2 3p 4s 3P1 2.4×10-3 1.5×10-3 0.11 6.9×1010 58.02
14–436 3s 3p33S1–3s 3p2 4s 3P0 2.3×10-3 7.0×10-2 1.3×1011 59.56
20–376 3s2 3p 3d 3P1–3s 3p2 4s 3P0 2.3×10-3 2.5×10-2 3.4×1010 69.24
16–435 3s2 3p 3d 3F3–3s2 3p 4f 3G4 2.4×10-3 2.3×10-3 3.80 7.6×1011 61.152 60.49 (–0.7)
8–378 3s 3p33D2–3s 3p2 4s 3P1 1.9×10-3 0.30 1.9×1011 59.08
9–388 3s 3p33D3–3s 3p2 4s 3P2 2.2×10-3 0.44 1.7×1011 58.83
15–439 3s2 3p 3d 3F2–3s2 3p 4f 3F2 1.9×10-3 2.0×10-3 0.24 8.7×1010 60.05
2–385 3s2 3p23P1–3s2 3p 4d 3D2 1.8×10-3 1.3×10-3 0.73 3.9×1011 49.913 49.44 (–0.5)
2–271 3s2 3p23P1–3s2 3p 4s 3P1 1.7×10-3 1.0×10-3 7.7×10-2 4.9×1010 58.51
3–279 3s2 3p23P2–3s2 3p 4s 3P2 1.6×10-3 6.2×10-4 0.39 1.5×1011 58.709 58.19 (–0.5)

Notes. The first and second columns indicate the level indices and spectroscopic notation. Columns 3, 4, show the intensities Int = NjAji/Ne (photons) relative to the strongest transition (in the EUV), displayed in decreasing order of intensity. The intensities were calculated at log Ne [cm-3] = 9 and log Te [K] = 6.4, with the present and the CHIANTI v.7 data, which are from Landi & Bhatia (2012). Columns 5 and 6 display the weighted oscillator strength (gf) and the spontaneous radiative transition probability. The last two columns show the wavelengths (in vacuum) corresponding to the experimental and target energies. Values in parentheses list the corresponding wavelength difference. N: new identification, TN: a tentative one.

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