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Table 3

List of the strongest Ni xi lines.

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

CHIANTI BL11

1–13 3s23p61S0–3s23p53d 1P1 1.0 1.0 2.72 2.7 × 1011 2.8 × 1011 148.377 144.66 (–3.7)
5–95 3s23p53d 3F4–3s23p43d23G5 5.1 × 10-2 4.7 × 10-2 5.12 1.2 × 1011 1.3 × 1011 152.54
5–106 3s23p53d 3F4–3s23p43d23D3 3.8 × 10-2 3.7 × 10-2 5.05 2.0 × 1011 2.3 × 1011 143.87
5–114 3s23p53d 3F4–3s23p43d23F4 3.5 × 10-2 3.3 × 10-2 5.92 2.0 × 1011 2.2 × 1011 137.72
6–93 3s23p53d 3F3–3s23p43d23G4 3.2 × 10-2 2.9 × 10-2 3.85 1.1 × 1011 1.2 × 1011 153.95
6–107 3s23p53d 3F3–3s23p43d23D2 1.9 × 10-2 1.7 × 10-2 3.30 1.9 × 1011 2.1 × 1011 144.40
1–4 3s23p61S0–3s23p53d 3P2 0.19 0.12 1.4 × 102 1.4 × 102 207.922 205.01 (–2.9)
1–3 3s23p61S0–3s23p53d 3P1 9.1 × 10-2 5.0 × 10-2 3.8 × 10-4 1.9 × 107 2.3 × 107 211.430 208.58 (–2.8)
1–10 3s23p61S0–3s23p53d 3D1 4.4 × 10-2 2.3 × 10-2 8.2 × 10-3 5.1 × 108 5.7 × 108 186.975 183.60 (–3.4) (bl)
1–7 3s23p61S0–3s23p53d 3F2 2.2 × 10-2 1.3 × 10-2 5.9 5.6 198.42 195.01 (–3.4) R (bl)
1–9 3s23p61S0–3s23p53d 1D2 1.6 × 10-2 9.6 × 10-3 49. 51 188.435 184.87 (–3.6) R
5–16 3s23p53d 3F4–3s3p63d 3D3 1.3 × 10-2 2.0 × 10-2 0.38 4.2 × 109 4.4 × 109 288.41 276.51 TN (bl)
1–139 3s23p61S0–3s23p54s 1P1 2.3 × 10-2 4.9 × 10-3 0.20 7.1 × 1010 7.3 × 1010 77.393 74.41 (–3.0)
1–133 3s23p61S0–3s23p54s 3P1 1.4 × 10-2 4.1 × 10-3 0.13 4.6 × 1010 5.0 × 1010 78.744 75.63 (–3.1) (bl)
13–440 3s23p53d 1P1–3s3p64s 1S0 1.1 × 10-2 5.6 × 10-3 2.5 × 10-2 1.5 × 1010 7.9 × 109 104.67 100.25 TN
5–540 3s23p53d 3F4–3s23p54f 3G5 6.7 × 10-3 5.5 × 10-3 5.66 4.8 × 1011 4.6 × 1011 82.416 78.96 (–3.5)
13–599 3s23p53d 1P1–3s23p54f 1D2 5.5 × 10-3 2.8 × 10-3 1.93 3.4 × 1011 2.0 × 1011 93.849 89.49 (–4.4)
1–357 3s23p61S0–3s23p54d 1P1 4.0 × 10-3 3.7 × 10-4 0.58 3.1 × 1011 7.7 × 1010 62.730 61.40 (–1.3) ?
6–545 3s23p53d 3F3–3s23p54f 3G4 3.8 × 10-3 2.9 × 10-3 3.89 4.1 × 1011 3.8 × 1011 82.530 79.04 (–3.5)
5–187 3s23p53d 3F4–3s23p54p 3D3 3.5 × 10-3 2.9 × 10-3 0.30 2.2 × 1010 2.2 × 1010 106.60
10–577 3s23p53d 3D1–3s23p54f 3F2 2.5 × 10-3 2.5 × 10-3 1.51 2.7 × 1011 2.3 × 1011 80.43
6–186 3s23p53d 3F3–3s23p54p 3D2 2.4 × 10-3 2.2 × 10-3 0.17 1.8 × 1010 1.8 × 1010 107.49
10–599 3s23p53d 3D1–3s23p54f 1D2 1.9 × 10-3 1.3 × 10-3 0.52 1.1 × 1011 9.2 × 1010 83.010 79.11 (–3.9)
5–12 3s23p53d 3F4–3s23p53d 1F3 6.7 × 10-2 4.4 × 10-2 2.7 × 102 2.8 × 102 2001.20 1959.12 (–42)
4–8 3s23p53d 3P2–3s23p53d 3D3 5.5 × 10-2 3.8 × 10-2 34 37 2157.08 2021.38 (–136) R
4–11 3s23p53d 3P2–3s23p53d 3D2 4.2 × 10-2 2.6 × 10-2 1.7 × 102 1.9 × 102 1717.33 1627.83 (–89.5)
6–8 3s23p53d 3F3–3s23p53d 3D3 3.1 × 10-2 2.1 × 10-2 19 21 3339.46 3218.54 (–121) R
6–9 3s23p53d 3F3–3s23p53d 1D2 2.9 × 10-2 1.8 × 10-2 86 95 3000.93 2878.03 (–123) R
7–9 3s23p53d 3F2–3s23p53d 1D2 1.8 × 10-2 1.1 × 10-2 54 59 3743.07 3553.69 (–189) R

Notes. The first column lists the indices of the levels, as from Table 2. The second the spectroscopic notation. Columns 3 and 4 show the intensities (photons) of the strongest lines, relative to the resonance transition, calculated at log Ne [cm-3] = 9 and log Te [K] = 6.1, using the present and the CHIANTI ion models. The CHIANTI model uses the Aggarwal & Keenan (2007) collision strengths for the first 17 levels and for the rest those of Bhatia & Landi (2011). Column 5 lists the weighted oscillator strength gf and Col. 6 the A-values from our calculation. Column 7 lists the Bhatia & Landi (2011) A-values as given in the CHIANTI v.7.1 database. TN is a tentative new identification, R a revised wavelength (compared to NIST), bl a blend. All wavelengths are in vacuum.

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