Nickel energy level diagram
Energy levels and transitions of neutral nickel (Ni I): the 70 strongest classified lines below 2 µm from the NIST Atomic Spectra Database and the 55 levels they connect, each line with its vacuum wavelength, frequency and, for 70 of them, the reduced dipole matrix element derived from the NIST transition rate. Measured lifetimes, transition rates, hyperfine constants and isotope shifts from the literature are included, each with its citation.
Hover a line or a level to isolate it, click to keep it selected. Scroll to zoom, drag to move.

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Key transitions of nickel
| Transition | λ vac (nm) | λ air (nm) | ν (THz) | |⟨J‖er‖J′⟩| (ea₀) | A (s⁻¹) | Γ/2π up. (MHz) | branch (%) | Use |
|---|---|---|---|---|---|---|---|---|
| 3d84s2 3F4 – 3d84s4p 3G°5 | 323.3867 | 323.2933 | 927.0402 | 1.004 | 5.490e+06 | 0.8745 | 99.9 | 323 nm J=4 -> J'=5 line from the 3F4 ground level |
λ, ν from NIST level energies unless a measured frequency for this isotope is available. A: measured value or NIST. Γ/2π: natural linewidth of the upper level, 1/(2πτ).
Isotope shifts
| Transition | λ vac (nm) | Isotopes | Shift (MHz) |
|---|---|---|---|
| 3d94s 3D3 – 3d84s4p 5S°2 | 212.206 | 60-58 | -800(50) |
| 3d94s 3D2 – 3d84s4p 3D°1 | 214.846 | 60-58 | -710(50) |
| 3d94s 3D2 – 3d84s4p 3P°1 | 215.851 | 60-58 | -840(50) |
| 3d94s 3D3 – 3d84s4p 3P°2 | 215.898 | 60-58 | -770(50) |
| 3d94s 3D1 – 3d84s4p 3P°0 | 217.517 | 60-58 | -890(40) |
| 3d94s 3D2 – 3d84s4p 3P°2 | 219.091 | 60-58 | -750(40) |
| 3d94s 3D1 – 3d84s4p 3P°1 | 219.804 | 60-58 | -870(40) |
| 3d94s 3D2 – 3d84s4p 3F°2 | 224.522 | 60-58 | -1070(40) |
| 3d94s 3D3 – 3d84s4p 3G°3 | 225.427 | 60-58 | -1060(40) |
| 3d94s 3D3 – 3d84s4p 3D°2 | 225.885 | 60-58 | -1060(40) |
| 3d94s 3D1 – 3d84s4p 3F°2 | 228.803 | 60-58 | -1090(40) |
| 3d84s2 3F4 – (43655)°3 | 229.069 | 60-58 | 740(40) |
| 3d94s 3D2 – 3d84s4p 3D°2 | 229.383 | 60-58 | -970(40) |
| 3d94s 3D3 – (43655)°3 | 230.149 | 60-58 | -960(40) |
| 3d94s 3D1 – 3d84s4p 3D°1 | 230.365 | 60-58 | -1070(40) |
| 3d84s2 3F3 – 3d84s4p 3G°3 | 231.305 | 60-58 | 730(40) |
| 3d84s2 3F2 – 3d84s4p 3F°2 | 231.469 | 60-58 | 620(40) |
| 3d84s2 3F3 – 3d84s4p 3D°2 | 231.788 | 60-58 | 780(40) |
| 3d84s2 3F2 – 3d84s4p 3F°3 | 232.210 | 60-58 | 720(40) |
| 3d84s2 3F3 – 3d84s4p 3G°4 | 232.651 | 60-58 | 780(40) |
| 3d84s2 3F2 – 3d84s4p 3D°1 | 233.069 | 60-58 | 660(40) |
| 3d84s2 3F4 – 3d84s4p 3D°3 | 234.626 | 60-58 | 710(40) |
Shift = ν(first isotope) − ν(second isotope).
Closed and nearly closed transitions of nickel
| Transition | λ vacuum (nm) | Lower level | A (s⁻¹) | Leak per scattered photon | Photons before a leak | Where the leak goes |
|---|---|---|---|---|---|---|
| 3d84s2 3F4 → 3d84s4p 3G°5 | 232.0747 | ground | 6.900e+08 NIST | 1.06 × 10−7 from semi-empirical calc. | 9.43 × 106 | 3d84s2 1G4 ≈ 1.06 × 10−7 (long-lived) |
| 3d84s2 3F4 → 3d84s4p 3G°5 | 323.3867 | ground | 5.490e+06 measured | 3.93 × 10−6 from semi-empirical calc. | 254,000 | 3d84s2 1G4 ≈ 3.93 × 10−6 (long-lived) |
| 3d94s 3D1 → 3d84s4p 3P°0 | 217.5166 | metastable | 1.370e+08 measured | 0.512 % from semi-empirical calc. | 195 | 3d84s2 3P1 ≈ 0.395 % (long-lived); 3d95s 2[3/2]1 ≈ 0.12 % |
| 3d94s 3D1 → 3d94p 3P°0 | 351.1339 | metastable | 1.230e+08 measured | 0.606 % from NIST data | 165 | 3d84s2 3P1 0.607 % (long-lived) |
| 3d94s 3D3 → 3d84s4p 3F°4 | 305.1703 | metastable | 6.400e+07 measured | 2.63 % from semi-empirical calc. | 38 | 3d84s2 3F4 2.62 % (long-lived); 3d84s2 3F3 4.62 × 10−4 (long-lived); 3d84s2 1G4 ≈ 1.22 × 10−5 (long-lived) |
| 3d84s2 3F3 → (44336)°4 | 232.5369 | metastable | 1.800e+07 NIST | ≥ 3.36 % from NIST data | ≤ 30 | 3d84s2 3F4 3.36 % (long-lived); 3 more possible paths without a listed rate |
| 3d84s2 3F2 → 3d84s4p 3F°3 | 232.2096 | metastable | 5.450e+08 measured | 4.33 % from semi-empirical calc. | 23 | 3d94s 3D3 ≈ 1.57 % (long-lived); 3d84s2 3F3 0.936 % (long-lived); 3d94s 1D2 ≈ 0.761 % (long-lived); 8 weaker lines |
| 3d84s2 3F3 → 3d84s4p 3G°4 | 232.6515 | metastable | 3.410e+08 measured | 4.53 % from semi-empirical calc. | 22 | 3d84s2 3F4 ≈ 4.02 % (long-lived); 3d94s 3D3 0.667 % (long-lived); 3d95s 2[5/2]3 ≈ 1.92 × 10−6; 1 weaker lines |
| 3d84s2 3F2 → 3d84s4p 3F°2 | 231.4694 | metastable | 5.280e+08 measured | 5.39 % from semi-empirical calc. | 19 | 3d94s 3D1 1.67 % (long-lived); 3d84s2 3F3 1.44 % (long-lived); 3d94s 3D2 1.37 % (long-lived); 9 weaker lines |
| 3d94s 3D3 → 3d84s4p 3F°4 | 197.6890 | metastable | 1.100e+08 NIST | 5.92 % from semi-empirical calc. | 17 | 3d84s2 3F4 3.85 % (long-lived); 3d95s 2[5/2]3 ≈ 1.3 %; 3d84s2 3F3 ≈ 0.735 % (long-lived); 12 weaker lines |
| 3d84s2 3F4 → (44336)°4 | 225.5498 | ground | 9.600e+06 NIST | ≥ 6.3 % from NIST data | ≤ 16 | 3d84s2 3F3 6.3 % (long-lived); 3 more possible paths without a listed rate |
| 3d94s 3D3 → 3d94p 3P°2 | 352.5544 | metastable | 1.100e+08 measured | 7.98 % from NIST data | 12 | 3d94s 3D2 6.05 % (long-lived); 3d94s 3D1 0.672 % (long-lived); 3d84s2 3F3 0.512 % (long-lived); 5 weaker lines |
| 3d94s 3D3 → 3d94p 3F°4 | 341.5744 | metastable | 6.400e+07 measured | 9.55 % from semi-empirical calc. | 10 | 3d84s2 3F4 9.44 % (long-lived); 3d84s2 3F3 0.229 % (long-lived); 3d84s2 1G4 ≈ 3.79 × 10−7 (long-lived) |
A transition is closed when its upper level can decay only to the level it was excited from, so the atom keeps scattering photons. “closed”: among the levels NIST lists, no other level below the upper level has the opposite parity and |ΔJ| ≤ 1, so no other electric-dipole decay exists. Otherwise the leak is the sum of the branching ratios of the other decay lines of the upper level (or 1 − branching ratio where that of the line itself has been measured), and the number of photons is 1 / leak. “≥” and “≤”: at least one possible decay path has no listed rate, so the leak is a lower limit. These numbers are derived from the branching ratios, lifetimes and rates of this page, not measured as such; the tag names the weakest of the inputs, * marks theory and ≈ a model or semi-empirical calculation. Listed: lines that start on the ground level or on a metastable level and leak at most 10 %, unless more than three possible decay paths have no listed rate. Fine-structure levels only: hyperfine and Zeeman dark states and forbidden decays without a listed rate are not considered. Select a line in the diagram for the full list of its leak channels.
Listed Ni transitions below 2 µm
| Lower level | Upper level | λ vacuum (nm) | λ air (nm) | ν (THz) | Type | |⟨J‖er‖J′⟩| (ea₀) | A (s⁻¹) | Branching (%) | Source of matrix element / A |
|---|---|---|---|---|---|---|---|---|---|
| 3d94s 3D3 | 3d84s4p 3F°3 | 196.3870 | – | 1526.5394 | E1 | 0.536 NIST | 1.100e+07 NIST | – | NIST ASD (accuracy C) |
| 3d94s 3D3 | 3d84s4p 3F°4 | 197.6890 | – | 1516.4856 | E1 | 1.943 NIST | 1.100e+08 NIST | – | NIST ASD (accuracy C) |
| 3d94s 3D2 | 3d84s4p 3F°2 | 198.1621 | – | 1512.8646 | E1 | 0.500 NIST | 1.300e+07 NIST | – | NIST ASD (accuracy C) |
| 3d94s 3D2 | 3d84s4p 3F°3 | 199.0254 | – | 1506.3026 | E1 | 1.504 NIST | 8.300e+07 NIST | – | NIST ASD (accuracy C) |
| 3d94s 3D2 | 3d95p 3D°2 | 200.7642 | 200.6993 | 1493.2564 | E1 | 0.583 NIST | 1.700e+07 NIST | – | NIST ASD (accuracy C) |
| 3d94s 3D1 | 3d84s4p 3F°2 | 201.4892 | 201.4242 | 1487.8838 | E1 | 1.370 NIST | 9.300e+07 NIST | – | NIST ASD (accuracy C) |
| 3d84s2 3F3 | 3d95p 3D°2 | 202.6042 | 202.5390 | 1479.6954 | E1 | 0.687 NIST | 2.300e+07 NIST | – | NIST ASD (accuracy D) |
| 3d84s2 3F4 | 3d95p 3D°3 | 202.7240 | 202.6588 | 1478.8204 | E1 | 0.831 NIST | 2.400e+07 NIST | – | NIST ASD (accuracy C) |
| 3d94s 3D3 | 3d95p 1D°2 | 204.7999 | 204.7343 | 1463.8308 | E1 (intercombination) | 0.618 NIST | 1.800e+07 NIST | – | NIST ASD (accuracy C) |
| 3d84s2 3F4 | 3d95p 3F°4 | 205.2731 | 205.2074 | 1460.4565 | E1 | 0.611 NIST | 9.700e+06 NIST | – | NIST ASD (accuracy C) |
| 3d84s2 3F2 | 3d95p 3D°1 | 205.6147 | 205.5489 | 1458.0301 | E1 | 0.652 NIST | 3.300e+07 NIST | – | NIST ASD (accuracy C) |
| 3d94s 3D3 | 3d95p 3P°2 | 206.0560 | 205.9901 | 1454.9079 | E1 | 0.673 NIST | 2.100e+07 NIST | 45.8 | NIST ASD (accuracy D) |
| 3d94s 3D2 | 3d84s4p 3S°1 | 206.0854 | 206.0195 | 1454.7000 | E1 | 0.546 NIST | 2.300e+07 NIST | 54.5 | NIST ASD (accuracy E) |
| 3d94s 3D3 | 3d84s4p 5S°2 | 212.2061 | 212.1390 | 1412.7419 | E1 (intercombination) | 0.762 measured | 2.460e+07 measured | 81.2 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D2 | 3d84s4p 3D°1 | 214.8460 | 214.7784 | 1395.3831 | E1 | 0.817 measured | 4.540e+07 measured | 62.6 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D2 | 3d84s4p 3P°1 | 215.8506 | 215.7828 | 1388.8885 | E1 | 0.732 measured | 3.600e+07 measured | 27 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D3 | 3d84s4p 3P°2 | 215.8984 | 215.8306 | 1388.5811 | E1 | 1.241 measured | 6.200e+07 measured | 57.7 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D1 | 3d84s4p 3P°0 | 217.5166 | 217.4485 | 1378.2509 | E1 | 0.834 measured | 1.370e+08 measured | 100 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D2 | 3d84s4p 3P°2 | 219.0914 | 219.0229 | 1368.3442 | E1 | 0.897 measured | 3.100e+07 measured | 28.8 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D1 | 3d84s4p 3P°1 | 219.8041 | 219.7354 | 1363.9077 | E1 | 1.100 measured | 7.700e+07 measured | 57.8 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d84s2 3F2 | 3d84s4p 3P°1 | 222.2637 | 222.1946 | 1348.8142 | E1 | 0.598 NIST | 2.200e+07 NIST | 16.5 | NIST ASD (accuracy D) |
| 3d94s 3D2 | 3d84s4p 3F°2 | 224.5224 | 224.4528 | 1335.2453 | E1 | 0.461 measured | 7.600e+06 measured | 1.37 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D3 | 3d84s4p 3G°3 | 225.4270 | 225.3572 | 1329.8868 | E1 | 0.788 measured | 1.570e+07 measured | 3.14 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d84s2 3F4 | (44336)°4 | 225.5498 | 225.4800 | 1329.1628 | E1 | 0.700 NIST | 9.600e+06 NIST | 3.36 | NIST ASD (accuracy C) |
| 3d94s 3D3 | 3d84s4p 3D°2 | 225.8850 | 225.8151 | 1327.1906 | E1 | 0.675 measured | 1.600e+07 measured | 3.68 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D1 | 3d84s4p 3F°2 | 228.8030 | 228.7325 | 1310.2644 | E1 | 0.524 measured | 9.300e+06 measured | 1.67 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d84s2 3F4 | (43655)°3 | 229.0690 | 228.9984 | 1308.7432 | E1 | 2.939 measured | 2.080e+08 measured | 70.7 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D2 | 3d84s4p 3D°2 | 229.3826 | 229.3119 | 1306.9537 | E1 | 0.903 measured | 2.740e+07 measured | 6.3 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D3 | (43655)°3 | 230.1486 | 230.0778 | 1302.6038 | E1 | 1.563 measured | 5.800e+07 measured | 19.7 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D1 | 3d84s4p 3D°1 | 230.3654 | 230.2945 | 1301.3780 | E1 | 0.851 measured | 4.000e+07 measured | 8.4 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D2 | 3d84s4p 5D°3 | 230.8068 | 230.7358 | 1298.8893 | E1 (intercombination) | 0.824 NIST | 1.600e+07 NIST | 68 | NIST ASD (accuracy C) |
| 3d84s2 3F3 | 3d84s4p 3G°3 | 231.3055 | 231.2344 | 1296.0889 | E1 | 4.444 measured | 4.620e+08 measured | 92.4 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d84s2 3F2 | 3d84s4p 3F°2 | 231.4694 | 231.3983 | 1295.1710 | E1 | 4.020 measured | 5.280e+08 measured | 95 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d84s2 3F3 | 3d84s4p 3D°2 | 231.7877 | 231.7164 | 1293.3927 | E1 | 3.367 measured | 3.690e+08 measured | 84.9 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d84s2 3F4 | 3d84s4p 3G°5 | 232.0747 | 232.0034 | 1291.7930 | E1 | 6.843 NIST | 6.900e+08 NIST | – | NIST ASD (accuracy C) |
| 3d84s2 3F2 | 3d84s4p 3F°3 | 232.2096 | 232.1383 | 1291.0424 | E1 | 4.856 measured | 5.450e+08 measured | 98.1 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d84s2 3F3 | (44336)°4 | 232.5369 | 232.4655 | 1289.2256 | E1 | 1.003 NIST | 1.800e+07 NIST | 6.3 | NIST ASD (accuracy D) |
| 3d84s2 3F3 | 3d84s4p 3G°4 | 232.6515 | 232.5801 | 1288.5901 | E1 | 4.367 measured | 3.410e+08 measured | 98.9 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d84s2 3F2 | 3d84s4p 3D°1 | 233.0685 | 232.9970 | 1286.2845 | E1 | 2.776 measured | 4.110e+08 measured | 86.3 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d84s2 3F4 | 3d84s4p 3D°3 | 234.6262 | 234.5543 | 1277.7453 | E1 | 3.190 measured | 2.280e+08 measured | 95.8 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d84s2 3F3 | 3d84s4p 3P°2 | 234.7349 | 234.6631 | 1277.1532 | E1 | 1.058 measured | 3.510e+07 measured | 81.8 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d84s2 3F4 | 3d84s4p 3F°4 | 234.8233 | 234.7514 | 1276.6725 | E1 | 1.003 measured | 1.750e+07 measured | 78.4 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D3 | 3d84s4p 3F°3 | 234.9455 | 234.8736 | 1276.0086 | E1 | 0.177 measured | 7.000e+05 measured | 0.91 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d84s2 3F3 | 3d84s4p 3D°2 | 242.0048 | 241.9313 | 1238.7873 | E1 | 0.845 measured | 2.040e+07 measured | 59.4 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D2 | 3d84s4p 3D°1 | 298.2516 | 298.1646 | 1005.1663 | E1 | 1.018 measured | 2.640e+07 measured | 18.2 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D3 | 3d84s4p 1G°4 | 299.5326 | 299.4453 | 1000.8674 | E1 (intercombination) | 1.019 measured | 8.700e+06 measured | 83.5 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D3 | 3d84s4p 3D°3 | 300.3361 | 300.2485 | 998.1900 | E1 | 2.950 measured | 9.300e+07 measured | 86.5 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D2 | 3d84s4p 3F°2 | 300.4496 | 300.3621 | 997.8127 | E1 | 2.180 measured | 7.100e+07 measured | 73.8 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D3 | 3d84s4p 3F°3 | 303.8817 | 303.7932 | 986.5434 | E1 | 1.748 measured | 3.150e+07 measured | 28 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D3 | 3d84s4p 3F°4 | 305.1703 | 305.0816 | 982.3776 | E1 | 2.842 measured | 6.400e+07 measured | 98.6 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D2 | 3d84s4p 3D°2 | 305.5201 | 305.4312 | 981.2529 | E1 | 1.589 measured | 3.590e+07 measured | 28.7 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D1 | 3d84s4p 3D°1 | 305.8528 | 305.7639 | 980.1855 | E1 | 2.069 measured | 1.010e+08 measured | 69.7 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D2 | 3d84s4p 3D°3 | 306.5509 | 306.4619 | 977.9532 | E1 | 0.847 measured | 7.200e+06 measured | 6.7 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D2 | 3d84s4p 3F°3 | 310.2457 | 310.1557 | 966.3066 | E1 | 2.706 measured | 7.100e+07 measured | 63.2 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D1 | 3d84s4p 3D°2 | 313.5012 | 313.4104 | 956.2721 | E1 | 2.388 measured | 7.500e+07 measured | 60 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d84s2 3F4 | 3d84s4p 3G°5 | 323.3867 | 323.2933 | 927.0402 | E1 | 1.004 measured | 5.490e+06 measured | 99.9 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d84s2 3F4 | (29669)°3 | 337.0531 | 336.9563 | 889.4518 | E1 | 1.522 measured | 1.750e+07 measured | 29 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D3 | (29669)°3 | 339.3957 | 339.2983 | 883.3124 | E1 | 1.852 measured | 2.540e+07 measured | 42.2 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D3 | 3d94p 3F°4 | 341.5744 | 341.4764 | 877.6785 | E1 | 3.366 measured | 6.400e+07 measured | 91.5 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D1 | 3d94p 3D°1 | 342.4689 | 342.3707 | 875.3859 | E1 | 1.483 measured | 3.700e+07 measured | 71.4 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D3 | 3d94p 3F°3 | 343.4541 | 343.3556 | 872.8750 | E1 | 1.556 measured | 1.730e+07 measured | 21.4 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D2 | 3d94p 3D°2 | 344.7246 | 344.6259 | 869.6578 | E1 | 2.175 measured | 4.680e+07 measured | 73.5 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D2 | 3d84s4p 5F°3 | 345.3878 | 345.2889 | 867.9880 | E1 (intercombination) | 1.193 measured | 1.000e+07 measured | 71 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D1 | 3d94p 3F°2 | 345.9450 | 345.8460 | 866.5899 | E1 | 2.636 measured | 6.800e+07 measured | 82.3 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D3 | 3d84s4p 5F°4 | 346.2644 | 346.1652 | 865.7907 | E1 (intercombination) | 2.264 measured | 2.780e+07 measured | 86.5 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D2 | (29669)°3 | 347.3537 | 347.2542 | 863.0756 | E1 | 1.361 measured | 1.280e+07 measured | 21.2 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D2 | 3d94p 3P°1 | 349.3955 | 349.2956 | 858.0317 | E1 | 2.563 measured | 1.040e+08 measured | 86.3 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D1 | 3d94p 3P°0 | 351.1339 | 351.0335 | 853.7839 | E1 | 1.621 measured | 1.230e+08 measured | 99.6 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D2 | 3d94p 3F°3 | 351.6057 | 351.5052 | 852.6381 | E1 | 2.751 measured | 5.040e+07 measured | 62.5 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
| 3d94s 3D3 | 3d94p 3P°2 | 352.5544 | 352.4536 | 850.3438 | E1 | 3.449 measured | 1.100e+08 measured | 92.4 | Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3 |
Reduced dipole matrix elements follow the convention A = ω³|d|²/(3πε₀ħc³(2J′+1)), with J′ the upper level. Tags show where a number comes from: measured, NIST compilation, high-accuracy theory, a semi-empirical calculation (Kurucz line list, used only where no measurement or NIST value exists; typically within a factor 2), or a model calculation.
Ni energy levels
Ni⁺ ionisation limit 61619.77 cm⁻¹ = 7.63988 eV (162.286 nm)
Sources
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…
- NIST ASD
- NIST ASD level energies
- Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
Bergeson & Lawler 1993 lifetimes could only be read through an automated reader of the publisher's page (full text paywalled); every value carries its cross-check against Wood 2014, and the four without one (44206.099, 44336.1, 48735.29, 49403.386) should be verified against the PDF before being treated as final. Isotope shifts are nu(60Ni)-nu(58Ni), derived from compiled wavelengths, sign as computed. Wood 2014 level energies equal the NIST ones to <0.1 cm-1 (matched within 0.3 cm-1 and J). rme_J_ea0 derived from A (S = A g_upper lambda_vac^3 / 2.0261e18). 61Ni: I=3/2. WebSearch was unavailable in this session (budget exhausted).
Atoms with measured data
- Lithium-632 levels, 85 lines
- Lithium-732 levels, 85 lines
- Beryllium-917 levels, 26 lines
- Sodium-2336 levels, 106 lines
- Magnesium-2418 levels, 61 lines
- Magnesium-2518 levels, 61 lines
- Potassium-3934 levels, 84 lines
- Potassium-4034 levels, 84 lines
- Potassium-4134 levels, 84 lines
- Calcium-4035 levels, 61 lines
- Calcium-4335 levels, 61 lines
- Chromium-5256 levels, 87 lines
- Chromium-5356 levels, 87 lines
- Rubidium-8536 levels, 94 lines
- Rubidium-8736 levels, 94 lines
- Strontium-8440 levels, 70 lines
- Strontium-8640 levels, 70 lines
- Strontium-8740 levels, 70 lines
- Strontium-8840 levels, 70 lines
- Cadmium-11115 levels, 21 lines
- Cadmium-11315 levels, 21 lines
- Cadmium-11415 levels, 21 lines
- Caesium-13331 levels, 79 lines
- Barium-13744 levels, 89 lines
- Barium-13844 levels, 89 lines
- Dysprosium-16139 levels, 55 lines
- Dysprosium-16239 levels, 55 lines
- Dysprosium-16339 levels, 55 lines
- Dysprosium-16439 levels, 55 lines
- Erbium-16673 levels, 90 lines
- Erbium-16773 levels, 90 lines
- Erbium-16873 levels, 90 lines
- Thulium-16972 levels, 73 lines
- Ytterbium-17118 levels, 26 lines
- Ytterbium-17318 levels, 26 lines
- Ytterbium-17418 levels, 26 lines
- Mercury-19927 levels, 47 lines
- Mercury-20127 levels, 47 lines
- Mercury-20227 levels, 47 lines