Atomic energy level diagrams

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.

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Nickel energy level diagram with transition wavelengths and dipole matrix elements

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Key transitions of nickel

Transitionλ vac (nm)λ air (nm)ν (THz)|⟨J‖er‖J′⟩| (ea₀)A (s⁻¹)Γ/2π up. (MHz)branch (%)Use
3d84s2 3F4 – 3d84s4p 3G°5323.3867323.2933927.04021.0045.490e+060.874599.9323 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

Transitionλ vac (nm)IsotopesShift (MHz)
3d94s 3D3 – 3d84s4p 5S°2212.20660-58-800(50)
3d94s 3D2 – 3d84s4p 3D°1214.84660-58-710(50)
3d94s 3D2 – 3d84s4p 3P°1215.85160-58-840(50)
3d94s 3D3 – 3d84s4p 3P°2215.89860-58-770(50)
3d94s 3D1 – 3d84s4p 3P°0217.51760-58-890(40)
3d94s 3D2 – 3d84s4p 3P°2219.09160-58-750(40)
3d94s 3D1 – 3d84s4p 3P°1219.80460-58-870(40)
3d94s 3D2 – 3d84s4p 3F°2224.52260-58-1070(40)
3d94s 3D3 – 3d84s4p 3G°3225.42760-58-1060(40)
3d94s 3D3 – 3d84s4p 3D°2225.88560-58-1060(40)
3d94s 3D1 – 3d84s4p 3F°2228.80360-58-1090(40)
3d84s2 3F4 – (43655)°3229.06960-58740(40)
3d94s 3D2 – 3d84s4p 3D°2229.38360-58-970(40)
3d94s 3D3 – (43655)°3230.14960-58-960(40)
3d94s 3D1 – 3d84s4p 3D°1230.36560-58-1070(40)
3d84s2 3F3 – 3d84s4p 3G°3231.30560-58730(40)
3d84s2 3F2 – 3d84s4p 3F°2231.46960-58620(40)
3d84s2 3F3 – 3d84s4p 3D°2231.78860-58780(40)
3d84s2 3F2 – 3d84s4p 3F°3232.21060-58720(40)
3d84s2 3F3 – 3d84s4p 3G°4232.65160-58780(40)
3d84s2 3F2 – 3d84s4p 3D°1233.06960-58660(40)
3d84s2 3F4 – 3d84s4p 3D°3234.62660-58710(40)

Shift = ν(first isotope) − ν(second isotope).

Closed and nearly closed transitions of nickel

Transitionλ vacuum (nm)Lower levelA (s⁻¹)Leak per scattered photonPhotons before a leakWhere the leak goes
3d84s2 3F4 → 3d84s4p 3G°5232.0747ground6.900e+08 NIST1.06 × 10−7 from semi-empirical calc.9.43 × 1063d84s2 1G4 ≈ 1.06 × 10−7 (long-lived)
3d84s2 3F4 → 3d84s4p 3G°5323.3867ground5.490e+06 measured3.93 × 10−6 from semi-empirical calc.254,0003d84s2 1G4 ≈ 3.93 × 10−6 (long-lived)
3d94s 3D1 → 3d84s4p 3P°0217.5166metastable1.370e+08 measured0.512 % from semi-empirical calc.1953d84s2 3P1 ≈ 0.395 % (long-lived); 3d95s 2[3/2]1 ≈ 0.12 %
3d94s 3D1 → 3d94p 3P°0351.1339metastable1.230e+08 measured0.606 % from NIST data1653d84s2 3P1 0.607 % (long-lived)
3d94s 3D3 → 3d84s4p 3F°4305.1703metastable6.400e+07 measured2.63 % from semi-empirical calc.383d84s2 3F4 2.62 % (long-lived); 3d84s2 3F3 4.62 × 10−4 (long-lived); 3d84s2 1G4 ≈ 1.22 × 10−5 (long-lived)
3d84s2 3F3 → (44336)°4232.5369metastable1.800e+07 NIST≥ 3.36 % from NIST data≤ 303d84s2 3F4 3.36 % (long-lived); 3 more possible paths without a listed rate
3d84s2 3F2 → 3d84s4p 3F°3232.2096metastable5.450e+08 measured4.33 % from semi-empirical calc.233d94s 3D3 ≈ 1.57 % (long-lived); 3d84s2 3F3 0.936 % (long-lived); 3d94s 1D2 ≈ 0.761 % (long-lived); 8 weaker lines
3d84s2 3F3 → 3d84s4p 3G°4232.6515metastable3.410e+08 measured4.53 % from semi-empirical calc.223d84s2 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°2231.4694metastable5.280e+08 measured5.39 % from semi-empirical calc.193d94s 3D1 1.67 % (long-lived); 3d84s2 3F3 1.44 % (long-lived); 3d94s 3D2 1.37 % (long-lived); 9 weaker lines
3d94s 3D3 → 3d84s4p 3F°4197.6890metastable1.100e+08 NIST5.92 % from semi-empirical calc.173d84s2 3F4 3.85 % (long-lived); 3d95s 2[5/2]3 ≈ 1.3 %; 3d84s2 3F3 ≈ 0.735 % (long-lived); 12 weaker lines
3d84s2 3F4 → (44336)°4225.5498ground9.600e+06 NIST≥ 6.3 % from NIST data≤ 163d84s2 3F3 6.3 % (long-lived); 3 more possible paths without a listed rate
3d94s 3D3 → 3d94p 3P°2352.5544metastable1.100e+08 measured7.98 % from NIST data123d94s 3D2 6.05 % (long-lived); 3d94s 3D1 0.672 % (long-lived); 3d84s2 3F3 0.512 % (long-lived); 5 weaker lines
3d94s 3D3 → 3d94p 3F°4341.5744metastable6.400e+07 measured9.55 % from semi-empirical calc.103d84s2 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 levelUpper levelλ vacuum (nm)λ air (nm)ν (THz)Type|⟨J‖er‖J′⟩| (ea₀)A (s⁻¹)Branching (%)Source of matrix element / A
3d94s 3D33d84s4p 3F°3196.3870–1526.5394E10.536 NIST1.100e+07 NIST–NIST ASD (accuracy C)
3d94s 3D33d84s4p 3F°4197.6890–1516.4856E11.943 NIST1.100e+08 NIST–NIST ASD (accuracy C)
3d94s 3D23d84s4p 3F°2198.1621–1512.8646E10.500 NIST1.300e+07 NIST–NIST ASD (accuracy C)
3d94s 3D23d84s4p 3F°3199.0254–1506.3026E11.504 NIST8.300e+07 NIST–NIST ASD (accuracy C)
3d94s 3D23d95p 3D°2200.7642200.69931493.2564E10.583 NIST1.700e+07 NIST–NIST ASD (accuracy C)
3d94s 3D13d84s4p 3F°2201.4892201.42421487.8838E11.370 NIST9.300e+07 NIST–NIST ASD (accuracy C)
3d84s2 3F33d95p 3D°2202.6042202.53901479.6954E10.687 NIST2.300e+07 NIST–NIST ASD (accuracy D)
3d84s2 3F43d95p 3D°3202.7240202.65881478.8204E10.831 NIST2.400e+07 NIST–NIST ASD (accuracy C)
3d94s 3D33d95p 1D°2204.7999204.73431463.8308E1 (intercombination)0.618 NIST1.800e+07 NIST–NIST ASD (accuracy C)
3d84s2 3F43d95p 3F°4205.2731205.20741460.4565E10.611 NIST9.700e+06 NIST–NIST ASD (accuracy C)
3d84s2 3F23d95p 3D°1205.6147205.54891458.0301E10.652 NIST3.300e+07 NIST–NIST ASD (accuracy C)
3d94s 3D33d95p 3P°2206.0560205.99011454.9079E10.673 NIST2.100e+07 NIST45.8NIST ASD (accuracy D)
3d94s 3D23d84s4p 3S°1206.0854206.01951454.7000E10.546 NIST2.300e+07 NIST54.5NIST ASD (accuracy E)
3d94s 3D33d84s4p 5S°2212.2061212.13901412.7419E1 (intercombination)0.762 measured2.460e+07 measured81.2Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D23d84s4p 3D°1214.8460214.77841395.3831E10.817 measured4.540e+07 measured62.6Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D23d84s4p 3P°1215.8506215.78281388.8885E10.732 measured3.600e+07 measured27Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D33d84s4p 3P°2215.8984215.83061388.5811E11.241 measured6.200e+07 measured57.7Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D13d84s4p 3P°0217.5166217.44851378.2509E10.834 measured1.370e+08 measured100Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D23d84s4p 3P°2219.0914219.02291368.3442E10.897 measured3.100e+07 measured28.8Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D13d84s4p 3P°1219.8041219.73541363.9077E11.100 measured7.700e+07 measured57.8Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d84s2 3F23d84s4p 3P°1222.2637222.19461348.8142E10.598 NIST2.200e+07 NIST16.5NIST ASD (accuracy D)
3d94s 3D23d84s4p 3F°2224.5224224.45281335.2453E10.461 measured7.600e+06 measured1.37Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D33d84s4p 3G°3225.4270225.35721329.8868E10.788 measured1.570e+07 measured3.14Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d84s2 3F4(44336)°4225.5498225.48001329.1628E10.700 NIST9.600e+06 NIST3.36NIST ASD (accuracy C)
3d94s 3D33d84s4p 3D°2225.8850225.81511327.1906E10.675 measured1.600e+07 measured3.68Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D13d84s4p 3F°2228.8030228.73251310.2644E10.524 measured9.300e+06 measured1.67Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d84s2 3F4(43655)°3229.0690228.99841308.7432E12.939 measured2.080e+08 measured70.7Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D23d84s4p 3D°2229.3826229.31191306.9537E10.903 measured2.740e+07 measured6.3Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D3(43655)°3230.1486230.07781302.6038E11.563 measured5.800e+07 measured19.7Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D13d84s4p 3D°1230.3654230.29451301.3780E10.851 measured4.000e+07 measured8.4Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D23d84s4p 5D°3230.8068230.73581298.8893E1 (intercombination)0.824 NIST1.600e+07 NIST68NIST ASD (accuracy C)
3d84s2 3F33d84s4p 3G°3231.3055231.23441296.0889E14.444 measured4.620e+08 measured92.4Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d84s2 3F23d84s4p 3F°2231.4694231.39831295.1710E14.020 measured5.280e+08 measured95Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d84s2 3F33d84s4p 3D°2231.7877231.71641293.3927E13.367 measured3.690e+08 measured84.9Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d84s2 3F43d84s4p 3G°5232.0747232.00341291.7930E16.843 NIST6.900e+08 NIST–NIST ASD (accuracy C)
3d84s2 3F23d84s4p 3F°3232.2096232.13831291.0424E14.856 measured5.450e+08 measured98.1Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d84s2 3F3(44336)°4232.5369232.46551289.2256E11.003 NIST1.800e+07 NIST6.3NIST ASD (accuracy D)
3d84s2 3F33d84s4p 3G°4232.6515232.58011288.5901E14.367 measured3.410e+08 measured98.9Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d84s2 3F23d84s4p 3D°1233.0685232.99701286.2845E12.776 measured4.110e+08 measured86.3Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d84s2 3F43d84s4p 3D°3234.6262234.55431277.7453E13.190 measured2.280e+08 measured95.8Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d84s2 3F33d84s4p 3P°2234.7349234.66311277.1532E11.058 measured3.510e+07 measured81.8Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d84s2 3F43d84s4p 3F°4234.8233234.75141276.6725E11.003 measured1.750e+07 measured78.4Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D33d84s4p 3F°3234.9455234.87361276.0086E10.177 measured7.000e+05 measured0.91Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d84s2 3F33d84s4p 3D°2242.0048241.93131238.7873E10.845 measured2.040e+07 measured59.4Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D23d84s4p 3D°1298.2516298.16461005.1663E11.018 measured2.640e+07 measured18.2Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D33d84s4p 1G°4299.5326299.44531000.8674E1 (intercombination)1.019 measured8.700e+06 measured83.5Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D33d84s4p 3D°3300.3361300.2485998.1900E12.950 measured9.300e+07 measured86.5Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D23d84s4p 3F°2300.4496300.3621997.8127E12.180 measured7.100e+07 measured73.8Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D33d84s4p 3F°3303.8817303.7932986.5434E11.748 measured3.150e+07 measured28Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D33d84s4p 3F°4305.1703305.0816982.3776E12.842 measured6.400e+07 measured98.6Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D23d84s4p 3D°2305.5201305.4312981.2529E11.589 measured3.590e+07 measured28.7Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D13d84s4p 3D°1305.8528305.7639980.1855E12.069 measured1.010e+08 measured69.7Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D23d84s4p 3D°3306.5509306.4619977.9532E10.847 measured7.200e+06 measured6.7Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D23d84s4p 3F°3310.2457310.1557966.3066E12.706 measured7.100e+07 measured63.2Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D13d84s4p 3D°2313.5012313.4104956.2721E12.388 measured7.500e+07 measured60Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d84s2 3F43d84s4p 3G°5323.3867323.2933927.0402E11.004 measured5.490e+06 measured99.9Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d84s2 3F4(29669)°3337.0531336.9563889.4518E11.522 measured1.750e+07 measured29Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D3(29669)°3339.3957339.2983883.3124E11.852 measured2.540e+07 measured42.2Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D33d94p 3F°4341.5744341.4764877.6785E13.366 measured6.400e+07 measured91.5Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D13d94p 3D°1342.4689342.3707875.3859E11.483 measured3.700e+07 measured71.4Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D33d94p 3F°3343.4541343.3556872.8750E11.556 measured1.730e+07 measured21.4Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D23d94p 3D°2344.7246344.6259869.6578E12.175 measured4.680e+07 measured73.5Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D23d84s4p 5F°3345.3878345.2889867.9880E1 (intercombination)1.193 measured1.000e+07 measured71Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D13d94p 3F°2345.9450345.8460866.5899E12.636 measured6.800e+07 measured82.3Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D33d84s4p 5F°4346.2644346.1652865.7907E1 (intercombination)2.264 measured2.780e+07 measured86.5Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D2(29669)°3347.3537347.2542863.0756E11.361 measured1.280e+07 measured21.2Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D23d94p 3P°1349.3955349.2956858.0317E12.563 measured1.040e+08 measured86.3Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D13d94p 3P°0351.1339351.0335853.7839E11.621 measured1.230e+08 measured99.6Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D23d94p 3F°3351.6057351.5052852.6381E12.751 measured5.040e+07 measured62.5Wood, Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 211, 20 (2014), Table 3
3d94s 3D33d94p 3P°2352.5544352.4536850.3438E13.449 measured1.100e+08 measured92.4Wood, 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

LevelEnergy (cm⁻¹)JParityLifetimegJHyperfine A (MHz)Hyperfine B (MHz)Lifetime sourceHyperfine source
3d84s2 3F40.0004evenstable1.2496––––
3d94s 3D3204.7873even–1.3335––––
3d94s 3D2879.8162even–1.151––––
3d84s2 3F31332.1643even–1.0828––––
3d94s 3D11713.0871even–0.49804––––
3d84s2 3F22216.5502even–0.66956––––
3d94p 3P°228569.2032odd8.4 ns measured1.485––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 5F°429084.4564odd31.1 ns measured1.288––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d94p 3F°329320.7623odd12.4 ns measured1.287––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d94p 3F°429480.9894odd14.3 ns measured1.086––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d94p 3P°129500.6741odd8.3 ns measured1.426––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
(29669)°329668.9183odd16.6 ns measured1.3––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 5F°329832.7793odd71 ns measured1.208––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d94p 3D°229888.4772odd15.7 ns measured0.552––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d94p 3P°030192.2510odd8.1 ns measured–––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d94p 3F°230619.4142odd12.1 ns measured0.74––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d94p 3D°130912.8171odd19.3 ns measured–––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3G°530922.7345odd182 ns measured1.214––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3F°432973.3764odd15.4 ns measured1.222––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3F°333112.3343odd8.9 ns measured1.193––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3D°333500.8223odd9.3 ns measured1.198––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 1G°433590.1304odd96 ns measured–––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3D°233610.8902odd8 ns measured1.19––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3F°234163.2642odd10.4 ns measured0.973––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3D°134408.5551odd6.9 ns measured0.511––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3F°442585.2124odd44.8 ns measured1.346––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3D°342620.9943odd4.2 ns measured–––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3D°242653.6612odd29.1 ns measured–––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3F°342767.8533odd13 ns measured1.218––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3G°543089.5785odd–1.226––––
(43655)°343654.9743odd3.4 ns measured1.243––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3P°243933.4082odd23.3 ns measured1.476––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 5D°344206.0993odd42.5 ns measured–––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3G°444314.9044odd2.9 ns measured1.182––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
(44336)°444336.1004odd3.5 ns measured–––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3D°244475.0992odd2.3 ns measured0.566––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3G°344565.0373odd2 ns measured1.044––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3D°145122.3831odd2.1 ns measured–––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3F°345281.0893odd1.8 ns measured0.779––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3F°245418.8042odd1.8 ns measured0.677––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3P°246522.8662odd9.3 ns measured–––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3P°147208.1491odd7.5 ns measured–––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 5S°247328.7842odd33 ns measured–––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3D°147424.7851odd13.8 ns measured0.726––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d84s4p 3P°047686.5870odd7.3 ns measured–––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d95p 3F°448715.5864odd––––––
3d95p 3P°248735.2902odd21.8 ns measured–––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d95p 1D°249032.9262odd––––––
3d95p 3D°349328.1403odd––––––
3d84s4p 3S°149403.3861odd23.7 ns measured–––Bergeson & Lawler, J. Opt. Soc. Am. B 10, 794 (1993), Table 1 (time-resolved laser-induce…–
3d95p 3D°250689.4892odd––––––
3d84s4p 3F°450789.3034odd––––––
3d95p 3D°150851.1991odd––––––
3d84s4p 3F°351124.6623odd––––––
3d84s4p 3F°251343.5472odd––––––

Ni⁺ ionisation limit 61619.77 cm⁻¹ = 7.63988 eV (162.286 nm)

Sources

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

All elements: periodic table