Open Access

Table A.1

Impact of orthogonal operator parameters on gA values for selected Ni II lines

Odd Level Even Level Transition Probability (s−1) Exp. Intensity




λair(Å) Eodd (cm−1) Levelodd Jodd Eeven (cm−1) Leveleven Jeven gA(o) gA(o=0) gA(K)a gA(T=15kK) CF UVb Shen.c
2376.037 10663.81 3d8(3F)4s 4F 1.5 52738.30 3d8(3F)4p 4D 2.5 4.68(6) 4.83(6) 5.78(6) 3.51(4) 0.085 45 75
2376.751 99154.62 3d8(3F)4d 4F 4.5 57080.38 3d8(3F)4p 2F 3.5 9.66(5) 1.25(7)! 1.48(7) 7.15(1) 0.001
2122.989 101365.91 3d8(3F)4d 4G 2.5 54262.52 3d8(3F)4p 4G 3.5 3.95(5) 2.62(7)! 2.41(7) 2.33(1) 0.000
2988.536 101144.63 3d8(3F)4d 4H 3.5 67694.64 3d8(1D)4p 2F 2.5 4.09(2) 5.38(3) 4.08(4) 2.50(−2) 0.000
2258.074 101365.91 3d8(3F)4d 4G 2.5 57080.38 3d8(3F)4p 2F 3.5 1.30(6) 2.14(7) 2.78(7) 7.82(1) 0.010
3064.48 24788.05 3d8(3P)4s 4P 1.5 57420.01 3d8(3F)4p 2D 2.5 6.08(4) 5.87(4) 1.89(5) 2.81(2) 0.013
3064.651 101365.91 3d8(3F)4d 4G 2.5 68735.77 3d8(1D)4p 2D 2.5 2.79(3) 1.97(5) 3.25(5) 1.67(−1) 0.000
2332.479 101365.91 3d8(3F)4d 4G 2.5 58493.07 3d8(3F)4p 2F 2.5 2.90(6) 8.74(7) 1.19(8) 1.74(2) 0.016 45 10
2337.808 23796.02 3d8(1D) 4s 2D 1.5 66571.13 3d8(3P)4p 4P 2.5 2.52(7) 1.32(8) 1.47(8) 2.78(5) 0.043 50 30
2337.358 99154.62 3d8(3F)4d 4F 4.5 56371.28 3d8(3F)4p 2G 3.5 7.60(5) 4.96(6) 5.78(6) 5.63(1) 0.002
2274.762 100331.93 3d8(3F)4d 4H 4.5 56371.28 3d8(3F)4p 2G 3.5 1.06(8) 3.91(7) 1.55(7) 7.02(3) 0.023 25 5
2170.98 100619.10 3d8(3F)4d 2G 4.5 54556.95 3d8(3F)4p 4F 4.5 3.07(7) 1.62(4)! 3.24(6) 1.97(3) 0.012 5
2158.416 100592.79 3d8(3F)4d 4F 3.5 54262.52 3d8(3F)4p 4G 3.5 4.84(8) 8.42(7) 8.77(7) 3.12(4) 0.154 45 18
2251.625 98969.31 3d8(3F)4d 4H 5.5 54556.95 3d8(3F)4p 4F 4.5 1.56(8) 5.07(7) 6.34(7) 1.18(4) 0.052 20 3
2123.392 101356.98 3d8(3F)4d 2H 4.5 54262.52 3d8(3F)4p 4G 3.5 4.38(7) 2.44(7) 9.16(6) 2.62(3) 0.007 5 0

Notes. Scientific notation is abbreviated as x(y) for compactness. a values from Kurucz (2011), b line intensity estimates of photographic plate blackening from unpublished grating spectra of a Ni-He hollow cathode lamp measured by the lead author in 2016, c line intensity estimates of photographic plate from Shenstone (1970). Note: UV and Shenstone should not be directly compared.

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