Atomic energy level diagrams

Cobalt energy level diagram

Energy levels and transitions of neutral cobalt (Co I): the 70 strongest classified lines below 2 µm from the NIST Atomic Spectra Database and the 51 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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Cobalt energy level diagram with transition wavelengths and dipole matrix elements

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Strongest transitions of cobalt

Transitionλ vac (nm)λ air (nm)ν (THz)|⟨J‖er‖J′⟩| (ea₀)A (s⁻¹)Γ/2π up. (MHz)branch (%)Use
a 4F3/2 – w 4F°3/2233.9379233.86621281.50421.5259.200e+0736.1740.5
a 4F9/2 – x 4G°11/2240.7983240.72511244.99406.3914.940e+0879.5898.8
a 4F5/2 – x 4G°7/2241.5191241.44571241.27874.8564.240e+0875.7989
a 4F3/2 – x 4G°5/2241.6024241.52901240.85063.9993.830e+0869.288.1
a 4F9/2 – x 4F°9/2242.5668242.49311235.91725.1123.710e+0863.6692.8
a 4F7/2 – x 4F°7/2243.2947243.22091232.21934.2593.190e+0858.9586.1
a 4F5/2 – x 4F°5/2243.7396243.66571229.97023.3132.560e+0856.8471.7
a 4F3/2 – x 4F°3/2243.9778243.90381228.76952.8382.810e+0854.8881.5
b 4F9/2 – w 4F°9/2251.1774251.10181193.54872.6539.000e+0728.4250.4
a 4F9/2 – x 4D°7/2252.2122252.13631188.65194.2422.840e+0851.3488
a 4F7/2 – x 4D°5/2252.9727252.89671185.07813.5372.610e+0849.7483.5
a 4F5/2 – x 4D°3/2253.6724253.59611181.80972.7232.300e+0846.8178.2
a 4F3/2 – x 4D°1/2254.5017254.42531177.95862.1502.840e+0846.8196.6
b 4F9/2 – y 4F°9/2340.6091340.5114880.16584.6741.120e+0823.0777.3
b 4F9/2 – y 4G°11/2345.4498345.3508867.83235.6771.320e+0821.5197.7
b 4F7/2 – y 4D°5/2350.7315350.6312854.76353.4849.500e+0718.2982.7

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).

59Co hyperfine structure (I = 7/2)

LevelA (MHz)B (MHz)Shift of each F level from the centre of gravity (MHz)
a 4F9/2450.2835(9)139.22(3)F=1: -8604.15 F=2: -7723.47 F=3: -6398.31 F=4: -4623.69 F=5: -2392.99 F=6: +302.08 F=7: +3471.47 F=8: +7126.77
a 4F7/2490.5678(21)94.50(3)F=0: -7675.82 F=1: -7194.90 F=2: -6231.12 F=3: -4780.62 F=4: -2837.64 F=5: -394.44 F=6: +2558.61 F=7: +6033.08
a 4F5/2613.348(3)67.54(6)F=1: -6863.99 F=2: -5656.59 F=3: -3838.25 F=4: -1400.30 F=5: +1668.86 F=6: +5383.68
a 4F3/21042.9828(9)67.618(18)F=2: -7003.91 F=3: -3923.26 F=4: +229.35 F=5: +5492.56
b 4F9/2828.800(3)-118.7(3)F=1: -16008.82 F=2: -14334.26 F=3: -11825.95 F=4: -8488.14 F=5: -4326.47 F=6: +651.99 F=7: +6438.75 F=8: +13023.92
b 4F7/2668.918(3)-79.23(21)F=0: -10577.91 F=1: -9900.90 F=2: -8548.51 F=3: -6523.97 F=4: -3832.13 F=5: -479.45 F=6: +3525.97 F=7: +8174.44
z 4F°9/2810.0(24)-60.000F=1: -15620.77 F=2: -13992.12 F=3: -11550.93 F=4: -8299.34 F=5: -4240.21 F=6: +622.89 F=7: +6285.67 F=8: +12743.13
z 4F°7/2655.4(24)30.000F=0: -10305.69 F=1: -9653.40 F=2: -8348.21 F=3: -6388.90 F=4: -3773.62 F=5: -499.93 F=6: +3435.23 F=7: +8035.54
z 4G°11/2772.0(21)210.000F=2: -17475.45 F=3: -15193.91 F=4: -12144.21 F=5: -8319.81 F=6: -3712.54 F=7: +1687.43 F=8: +7891.56 F=9: +14912.92
z 4F°5/2559.1(21)30.000F=1: -6273.92 F=2: -5164.27 F=3: -3496.58 F=4: -1267.00 F=5: +1529.62 F=6: +4899.71
z 4G°9/2517.1(27)180.000F=1: -9872.44 F=2: -8863.88 F=3: -7345.67 F=4: -5311.40 F=5: -2752.49 F=6: +341.78 F=7: +3984.26 F=8: +8189.95
z 4D°7/2751.0(27)–F=0: -11827.93 F=1: -11076.95 F=2: -9575.00 F=3: -7322.06 F=4: -4318.14 F=5: -563.24 F=6: +3942.64 F=7: +9199.50
z 4G°7/2448.2(15)150.000F=0: -6978.64 F=1: -6545.75 F=2: -5676.92 F=3: -4366.03 F=4: -2603.88 F=5: -378.23 F=6: +2326.21 F=7: +5527.83
z 4D°5/2696.1(27)30.000F=1: -7815.28 F=2: -6431.61 F=3: -4352.89 F=4: -1575.27 F=5: +1906.40 F=6: +6098.55
z 4G°5/2398.4(18)150.000F=1: -4401.87 F=2: -3647.89 F=3: -2500.84 F=4: -941.45 F=5: +1056.01 F=6: +3523.68
z 4D°3/2705(6)30.000F=2: -4739.37 F=3: -2647.27 F=4: +162.20 F=5: +3706.18
z 2G°9/2495(3)–F=1: -9522.20 F=2: -8532.89 F=3: -7048.90 F=4: -5070.27 F=5: -2596.97 F=6: +371.00 F=7: +3833.61 F=8: +7790.90
z 2F°7/2448.8(18)180.000F=0: -6972.01 F=1: -6541.59 F=2: -5677.07 F=3: -4371.11 F=4: -2612.68 F=5: -387.10 F=6: +2324.01 F=7: +5542.68
y 4D°7/2478.2(24)150.000F=0: -7450.82 F=1: -6987.96 F=2: -6059.17 F=3: -4658.33 F=4: -2776.26 F=5: -400.72 F=6: +2483.61 F=7: +5895.08
y 4G°11/2300(6)–F=2: -6820.22 F=3: -5920.85 F=4: -4721.69 F=5: -3222.74 F=6: -1424.00 F=7: +674.53 F=8: +3072.85 F=9: +5770.96
y 4G°9/2334.3(27)–F=1: -6434.70 F=2: -5766.16 F=3: -4763.35 F=4: -3426.27 F=5: -1754.92 F=6: +250.70 F=7: +2590.59 F=8: +5264.75
y 4D°5/2465(6)–F=1: -5227.65 F=2: -4298.29 F=3: -2904.25 F=4: -1045.53 F=5: +1277.87 F=6: +4065.95
y 4F°9/2297(3)240.000F=1: -5603.21 F=2: -5043.91 F=3: -4197.83 F=4: -3056.38 F=5: -1608.15 F=6: +161.16 F=7: +2268.69 F=8: +4734.44
(33173)°7/2508.1(21)–F=0: -8003.36 F=1: -7495.21 F=2: -6478.91 F=3: -4954.46 F=4: -2921.86 F=5: -381.11 F=6: +2667.79 F=7: +6224.84
y 2G°9/2441.6(18)–F=1: -8500.61 F=2: -7617.43 F=3: -6292.66 F=4: -4526.30 F=5: -2318.35 F=6: +331.19 F=7: +3422.32 F=8: +6955.04
(33467)°7/2387(6)–F=0: -6091.00 F=1: -5704.27 F=2: -4930.81 F=3: -3770.62 F=4: -2223.70 F=5: -290.05 F=6: +2030.33 F=7: +4737.44
y 4G°5/2804.9(27)-120.000F=1: -9119.86 F=2: -7475.69 F=3: -5022.30 F=4: -1775.12 F=5: +2245.30 F=6: +7013.23
(33946)°5/2603(3)–F=1: -6779.02 F=2: -5573.86 F=3: -3766.12 F=4: -1355.81 F=5: +1657.10 F=6: +5272.57
y 4F°3/21190.8(24)-60.000F=2: -8070.04 F=3: -4454.79 F=4: +325.56 F=5: +6236.70
x 4D°7/2303.7(21)–F=0: -4783.12 F=1: -4479.43 F=2: -3872.05 F=3: -2960.98 F=4: -1746.22 F=5: -227.77 F=6: +1594.37 F=7: +3720.20
x 4D°5/2355.2(27)30.000F=1: -3980.49 F=2: -3278.56 F=3: -2222.45 F=4: -808.31 F=5: +969.01 F=6: +3115.94
x 4D°3/2528(6)–F=2: -3561.50 F=3: -1978.61 F=4: +131.91 F=5: +2770.06
x 4D°1/21673(9)–F=3: -3763.80 F=4: +2927.40
x 4F°9/2441(6)–F=1: -8483.28 F=2: -7601.90 F=3: -6279.83 F=4: -4517.07 F=5: -2313.62 F=6: +330.52 F=7: +3415.35 F=8: +6940.87
x 4G°11/2237(6)240.000F=2: -5288.84 F=3: -4617.59 F=4: -3713.87 F=5: -2570.19 F=6: -1177.20 F=7: +476.32 F=8: +2403.45 F=9: +4619.17
x 4F°7/2513(6)–F=0: -8074.24 F=1: -7561.59 F=2: -6536.29 F=3: -4998.34 F=4: -2947.74 F=5: -384.49 F=6: +2691.41 F=7: +6279.96
x 4G°9/2330(9)–F=1: -6348.07 F=2: -5688.53 F=3: -4699.22 F=4: -3380.14 F=5: -1731.29 F=6: +247.33 F=7: +2555.72 F=8: +5193.88
x 4F°5/2660(24)–F=1: -7419.82 F=2: -6100.74 F=3: -4122.12 F=4: -1483.96 F=5: +1813.73 F=6: +5770.98
x 4F°3/21019(9)–F=2: -6880.27 F=3: -3822.38 F=4: +254.82 F=5: +5351.32
x 4G°7/2537(27)–F=0: -8451.92 F=1: -7915.29 F=2: -6842.03 F=3: -5232.14 F=4: -3085.62 F=5: -402.47 F=6: +2817.31 F=7: +6573.72
x 4G°5/2929(9)–F=1: -10455.30 F=2: -8596.58 F=3: -5808.50 F=4: -2091.06 F=5: +2555.74 F=6: +8131.90
w 4D°5/2681(6)60.000F=1: -7623.82 F=2: -6279.90 F=3: -4257.60 F=4: -1549.19 F=5: +1855.60 F=6: +5969.64
w 4F°9/2983(6)-150.000F=1: -18997.66 F=2: -17009.59 F=3: -14031.95 F=4: -10070.10 F=5: -5131.18 F=6: +775.88 F=7: +7640.37 F=8: +15449.79
w 4D°7/2711(6)–F=0: -11190.53 F=1: -10480.02 F=2: -9059.00 F=3: -6927.47 F=4: -4085.43 F=5: -532.88 F=6: +3730.18 F=7: +8703.75
x 2F°7/2711(9)-150.000F=0: -11270.89 F=1: -10545.07 F=2: -9096.50 F=3: -6931.30 F=4: -4058.65 F=5: -490.79 F=6: +3756.96 F=7: +8666.25
(43848)°7/2779(3)–F=0: -12276.50 F=1: -11497.03 F=2: -9938.11 F=3: -7599.73 F=4: -4481.90 F=5: -584.60 F=6: +4092.16 F=7: +9548.39
w 4G°11/2982.1(27)-150.000F=2: -22405.28 F=3: -19434.37 F=4: -15478.62 F=5: -10542.69 F=6: -4632.44 F=7: +2245.13 F=8: +10081.83 F=9: +18868.31
(44202)°5/2660(24)–F=1: -7419.82 F=2: -6100.74 F=3: -4122.12 F=4: -1483.96 F=5: +1813.73 F=6: +5770.98
w 4G°7/2546(12)–F=0: -8593.51 F=1: -8047.90 F=2: -6956.65 F=3: -5319.80 F=4: -3137.32 F=5: -409.21 F=6: +2864.51 F=7: +6683.85
w 4F°3/2435(9)180.000F=2: -2837.80 F=3: -1662.27 F=4: +25.10 F=5: +2327.18

Measured A, B constants; sources in the data file.

Closed and nearly closed transitions of cobalt

Transitionλ vacuum (nm)Lower levelA (s⁻¹)Leak per scattered photonPhotons before a leakWhere the leak goes
a 4F9/2 → x 4G°11/2240.7983ground4.940e+08 measured≥ 0.924 % from semi-empirical calc.≤ 108b 4F9/2 ≈ 0.924 % (long-lived); a 2G9/2 ≈ 9.1 × 10−7 (long-lived); b 2G9/2 ≈ 2.79 × 10−8 (long-lived); 1 weaker lines; 1 more possible path without a listed rate
b 4F9/2 → y 4G°11/2345.4498metastable1.320e+08 measured2 % from semi-empirical calc.50a 4F9/2 2 % (long-lived); a 2H11/2 ≈ 7.64 × 10−7 (long-lived); a 2G9/2 ≈ 4.44 × 10−7 (long-lived); 2 weaker lines
a 4F9/2 → z 4G°11/2346.6779ground1.060e+07 measured3.02 % from semi-empirical calc.33b 4F9/2 3.01 % (long-lived); a 2G9/2 ≈ 2.78 × 10−5 (long-lived); a 2H11/2 ≈ 3.5 × 10−7 (long-lived); 2 weaker lines
a 4F7/2 → z 4G°9/2351.4478metastable8.800e+06 measured5.48 % from semi-empirical calc.18b 4F9/2 ≈ 2.78 % (long-lived); b 4F7/2 2.12 % (long-lived); a 2F7/2 0.286 % (long-lived); 7 weaker lines
a 4F9/2 → z 4F°9/2352.7852ground1.380e+07 measured6.19 % from semi-empirical calc.16a 4F7/2 3.55 % (long-lived); b 4F9/2 2.39 % (long-lived); b 4F7/2 ≈ 0.26 % (long-lived); 7 weaker lines
a 4F9/2 → x 4F°9/2242.5668ground3.710e+08 measured6.9 % from semi-empirical calc.14b 4F9/2 ≈ 4.63 % (long-lived); b 4F7/2 1.38 % (long-lived); a 4F7/2 ≈ 0.889 % (long-lived); 7 weaker lines
a 4F3/2 → x 4D°1/2254.5017metastable2.840e+08 measured7 % from semi-empirical calc.14b 4P1/2 ≈ 3.53 % (long-lived); b 4P3/2 ≈ 1.76 % (long-lived); b 4F3/2 ≈ 1.68 % (long-lived); 9 weaker lines
a 4F3/2 → z 4G°5/2353.4364metastable8.300e+06 measured8.35 % from semi-empirical calc.12a 4F5/2 2.78 % (long-lived); b 4F7/2 2.44 % (long-lived); b 4F3/2 1.55 % (long-lived); 18 weaker lines
a 4F5/2 → z 4G°7/2353.0034metastable8.500e+06 measured8.6 % from semi-empirical calc.12b 4F7/2 3.13 % (long-lived); a 4F7/2 1.94 % (long-lived); b 4F9/2 1.62 % (long-lived); 14 weaker lines
a 4F3/2 → x 4G°5/2241.6024metastable3.830e+08 measured9.96 % from semi-empirical calc.10a 4F5/2 8.51 % (long-lived); b 4F3/2 ≈ 0.787 % (long-lived); a 4F7/2 ≈ 0.403 % (long-lived); 18 weaker lines

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 Co 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
b 4F7/26°7/2228.8513228.78081309.9878E12.017 NIST8.600e+07 NIST97.2NIST ASD (accuracy D)
a 4F9/2x 2F°7/2229.5936229.52291305.7526E1 (intercombination)1.095 measured2.510e+07 measured21.6Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F9/2w 4F°9/2230.9718230.90081297.9610E11.973 measured6.400e+07 measured35.8Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F7/2(43848)°7/2232.3853232.31401290.0663E11.710 measured5.900e+07 measured34.8Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F5/2w 4G°7/2232.6251232.55371288.7367E10.683 measured9.400e+06 measured21.9Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F5/2(44202)°5/2233.6717233.60011282.9642E11.493 measured5.900e+07 measured31.9Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F3/2w 4F°3/2233.9379233.86621281.5042E11.525 measured9.200e+07 measured40.5Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F7/2w 4F°9/2235.4087235.33661273.4980E11.005 measured1.570e+07 measured8.79Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F5/2(43848)°7/2235.6204235.54841272.3534E10.874 measured1.480e+07 measured8.73Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F3/2(44202)°5/2235.8903235.81821270.8979E10.796 measured1.630e+07 measured8.8Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F9/2x 4G°9/2236.5782236.50591267.2023E11.085 measured1.800e+07 measured3.78Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F5/2x 2F°7/2237.2570237.18461263.5766E1 (intercombination)0.620 NIST7.300e+06 NIST6.28NIST ASD (accuracy D)
a 4F9/2x 4F°7/2238.5587238.48591256.6823E11.225 measured2.800e+07 measured7.56Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F5/2x 4G°5/2239.2756239.20271252.9169E11.225 measured3.700e+07 measured8.51Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F7/2x 4F°5/2240.2793240.20621247.6832E11.609 measured6.300e+07 measured17.6Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F9/2x 4G°11/2240.7983240.72511244.9940E16.391 measured4.940e+08 measured98.8Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F3/2w 4D°5/2241.3499241.27651242.1487E11.471 measured5.200e+07 measured44.7Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F5/2x 4G°7/2241.5191241.44571241.2787E14.856 measured4.240e+08 measured89Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F3/2x 4G°5/2241.6024241.52901240.8506E13.999 measured3.830e+08 measured88.1Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F9/2x 4F°9/2242.5668242.49311235.9172E15.112 measured3.710e+08 measured92.8Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F7/2x 4F°7/2243.2947243.22091232.2193E14.259 measured3.190e+08 measured86.1Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F5/2x 4F°5/2243.7396243.66571229.9702E13.313 measured2.560e+08 measured71.7Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F3/2x 4F°3/2243.9778243.90381228.7695E12.838 measured2.810e+08 measured81.5Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F3/2x 4F°5/2246.1545246.08001217.9039E10.761 measured1.310e+07 measured3.67Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F5/2x 4F°7/2246.8431246.76841214.5063E10.645 measured7.000e+06 measured1.89Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F9/2w 4G°11/2247.1013247.02661213.2373E11.146 measured1.470e+07 measured82.2Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F9/2(43848)°7/2247.7384247.66361210.1171E11.115 measured2.070e+07 measured12.2Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F9/2w 4D°7/2250.5274250.45191196.6456E10.997 measured1.600e+07 measured29.8Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F9/2w 4F°9/2251.1774251.10181193.5487E12.653 measured9.000e+07 measured50.4Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F9/2x 4D°7/2252.2122252.13631188.6519E14.242 measured2.840e+08 measured88Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F7/2x 4D°5/2252.9727252.89671185.0781E13.537 measured2.610e+08 measured83.5Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F5/2x 4D°3/2253.6724253.59611181.8097E12.723 measured2.300e+08 measured78.2Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F7/2x 2F°7/2253.7262253.65001181.5588E1 (intercombination)1.632 measured4.130e+07 measured35.5Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F3/2x 4D°1/2254.5017254.42531177.9586E12.150 measured2.840e+08 measured96.6Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F3/2x 4D°3/2256.2891256.21231169.7434E11.228 measured4.540e+07 measured15.4Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F5/2x 4D°5/2256.8112256.73431167.3652E11.259 measured3.160e+07 measured10.1Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F7/2x 4D°7/2257.5119257.43481164.1889E11.129 measured1.890e+07 measured5.86Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F7/2x 4F°9/2269.6646269.58461111.7234E10.730 measured5.500e+06 measured1.38Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F9/2y 4F°9/2304.4882304.3997984.5781E11.678 measured2.020e+07 measured13.9Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F7/2(33467)°7/2306.2706306.1815978.8485E11.300 measured1.490e+07 measured10.9Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F5/2(33946)°5/2307.3230307.2337975.4965E11.113 measured1.440e+07 measured9.94Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F3/2y 4F°3/2308.7670308.6774970.9342E11.023 measured1.800e+07 measured12.8Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F7/2(33946)°5/2335.5340335.4376893.4787E11.089 measured1.060e+07 measured7.31Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F9/2(33173)°7/2336.8076336.7109890.1000E10.903 measured5.400e+06 measured4.54Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F7/2y 4G°5/2338.6189338.5218885.3387E11.023 measured9.100e+06 measured6.73Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F9/2y 4F°9/2340.6091340.5114880.1658E14.674 measured1.120e+08 measured77.3Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F7/2(33467)°7/2341.0152340.9173879.1177E12.589 measured4.280e+07 measured31.2Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F7/2y 2G°9/2341.3312341.2333878.3038E1 (intercombination)3.572 measured6.500e+07 measured53.3Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F9/2z 4D°7/2341.3608341.2629878.2276E11.478 measured1.390e+07 measured39.8Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F7/2z 4D°5/2343.2562343.1578873.3782E11.189 measured1.180e+07 measured37.6Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F5/2z 4D°3/2344.3907344.2920870.5011E11.004 measured1.250e+07 measured42.6Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F7/2(33173)°7/2344.4629344.3642870.3185E13.337 measured6.900e+07 measured58Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F9/2y 4G°9/2345.0428344.9440868.8558E11.937 measured1.850e+07 measured17.9Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F9/2y 4G°11/2345.4498345.3508867.8323E15.677 measured1.320e+08 measured97.7Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F9/2z 4G°11/2346.6779346.5786864.7579E11.617 measured1.060e+07 measured96.8Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F7/2y 4F°9/2348.4402348.3405860.3843E11.052 measured5.300e+06 measured3.66Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F9/2y 4D°7/2350.3280350.2278855.7480E13.865 measured8.800e+07 measured88Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F7/2y 4D°5/2350.7315350.6312854.7635E13.484 measured9.500e+07 measured82.7Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F7/2z 4G°9/2351.4478351.3473853.0214E11.373 measured8.800e+06 measured93.3Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F9/2z 2F°7/2352.2574352.1567851.0607E1 (intercombination)1.451 measured1.220e+07 measured62.3Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F9/2z 4F°9/2352.7852352.6844849.7875E11.729 measured1.380e+07 measured94.2Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F5/2z 4G°7/2353.0034352.9025849.2623E11.215 measured8.500e+06 measured91.8Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F7/2y 4G°9/2353.0815352.9806849.0743E13.428 measured5.410e+07 measured52.5Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F3/2z 4G°5/2353.4364353.3354848.2217E11.042 measured8.300e+06 measured92.1Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F7/2z 4F°7/2357.6375357.5355838.2578E11.275 measured9.000e+06 measured71.1Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F7/2y 4D°7/2358.6178358.5155835.9665E11.145 measured7.200e+06 measured7.2Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
a 4F5/2z 4F°5/2359.5890359.4864833.7087E11.016 measured7.500e+06 measured61.7Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F7/2z 2G°9/2362.8838362.7804826.1390E1 (intercombination)1.018 measured4.390e+06 measured18.5Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F9/2z 4D°7/2387.4212387.3114773.8153E11.850 measured1.490e+07 measured42.6Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), Table 3
b 4F7/2z 4D°5/2387.5053387.3955773.6474E11.414 measured1.160e+07 measured37Lawler, Sneden, Cowan, Astrophys. J. Suppl. Ser. 220, 13 (2015), 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.

Co energy levels

LevelEnergy (cm⁻¹)JParityLifetimegJHyperfine A (MHz)Hyperfine B (MHz)Lifetime sourceHyperfine source
a 4F9/20.0009/2evenstable1.3329450.283139.22–Childs & Goodman, Phys. Rev. 170, 50 (1968) (atomic-beam magnetic resonance), as tabulate…
a 4F7/2816.0007/2even–1.2378490.56894.495–Childs & Goodman, Phys. Rev. 170, 50 (1968) (atomic-beam magnetic resonance), as tabulate…
a 4F5/21406.8405/2even–1.0283613.34867.543–Childs & Goodman, Phys. Rev. 170, 50 (1968) (atomic-beam magnetic resonance), as tabulate…
a 4F3/21809.3303/2even–0.39941042.9867.618–Childs & Goodman, Phys. Rev. 170, 50 (1968) (atomic-beam magnetic resonance), as tabulate…
b 4F9/23482.8209/2even–1.3334828.8-118.72–Childs & Goodman, Phys. Rev. 170, 50 (1968) (atomic-beam magnetic resonance), as tabulate…
b 4F7/24142.6607/2even–1.2366668.918-79.235–Childs & Goodman, Phys. Rev. 170, 50 (1968) (atomic-beam magnetic resonance), as tabulate…
z 4F°9/228345.8609/2odd68.3 ns measured1.33810.04-60Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
z 4F°7/228777.2707/2odd79 ns measured1.247655.3530Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
z 4G°11/228845.22011/2odd91.3 ns measured1.276771.97210Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
z 4F°5/229216.3705/2odd82.3 ns measured1.033559.1130Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
z 4G°9/229269.7309/2odd106 ns measured1.175517.14180Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
z 4D°7/229294.5207/2odd28.6 ns measured1.425750.98–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
z 4G°7/229735.1807/2odd108 ns measured0.995448.19150Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
z 4D°5/229948.7605/2odd31.9 ns measured1.359696.1230Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
z 4G°5/230102.9605/2odd111 ns measured0.577398.42150Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
z 4D°3/230443.6303/2odd34.1 ns measured1.192704.5130Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
z 2G°9/231699.6909/2odd42.1 ns measured1.126494.66–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
z 2F°7/231871.1507/2odd51.1 ns measured1.777448.79180Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
y 4D°7/232027.5007/2odd10 ns measured1.395478.17150Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
y 4G°11/232430.59011/2odd7.4 ns measured1.287299.79–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
y 4G°9/232464.7309/2odd9.7 ns measured1.154334.27–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
y 4D°5/232654.5005/2odd8.7 ns measured1.366464.68–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
y 4F°9/232841.9909/2odd6.9 ns measured1.313296.79240Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
(33173)°7/233173.3607/2odd8.4 ns measured1.039508.15–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
y 2G°9/233439.7209/2odd8.2 ns measured1.165441.59–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
(33467)°7/233466.8707/2odd7.3 ns measured1.155386.73–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
y 4G°5/233674.3805/2odd7.4 ns measured0.704804.94-120Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
(33946)°5/233945.9005/2odd6.9 ns measured0.9602.58–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
y 4F°3/234196.2103/2odd7.1 ns measured0.431190.8-60Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
x 4D°7/239649.1607/2odd3.1 ns measured1.428303.69–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
x 4D°5/240345.9505/2odd3.2 ns measured1.37355.2530Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
x 4D°3/240827.7703/2odd3.4 ns measured1.24527.63–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
x 4D°1/241101.8001/2odd3.4 ns measured0.0261672.8–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
x 4F°9/241225.7609/2odd2.5 ns measured1.319440.69–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
x 4G°11/241528.53011/2odd2 ns measured1.291236.84240Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
x 4F°7/241918.4107/2odd2.7 ns measured1.248512.65–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
x 4G°9/242269.3209/2odd2.1 ns measured1.169329.77–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
x 4F°5/242434.2305/2odd2.8 ns measured1.024659.54–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
x 4F°3/242796.6703/2odd2.9 ns measured0.4061019.3–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
x 4G°7/242811.4407/2odd2.1 ns measured1.004536.63–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
x 4G°5/243199.6505/2odd2.3 ns measured0.649929.36–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
w 4D°5/243242.9505/2odd8.6 ns measured1.101680.5360Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
w 4F°9/243295.3209/2odd5.6 ns measured1.295983.32-150Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
w 4D°7/243398.6207/2odd18.6 ns measured1.334710.51–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
x 2F°7/243555.2207/2odd8.6 ns measured1.229710.51-150Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
(43848)°7/243847.9807/2odd5.9 ns measured1.197779.46–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
w 4G°11/243952.06011/2odd55.9 ns measured1.279982.12-150Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
(44202)°5/244201.9205/2odd5.4 ns measured0.95659.54–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
w 4G°7/244394.4707/2odd23.3 ns measured1.004545.62–Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
w 4F°3/244555.7103/2odd4.4 ns measured0.415434.7180Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…Pickering, Astrophys. J. Suppl. Ser. 107, 811 (1996), Table 2 (Fourier-transform line-pro…
6°7/247839.1507/2odd11.3 ns measured–––Nitz, Bergeson, Lawler, J. Opt. Soc. Am. B 12, 377 (1995), Table 2 (time-resolved laser-i…–

Co⁺ ionisation limit 63564.60 cm⁻¹ = 7.88101 eV (157.320 nm)

Sources

Level energies are the site's NIST values; Lawler 2015 and Pickering 1996 use the Pickering & Thorne (1996) energies, which differ by <0.1 cm-1 (matched on energy within 0.3 cm-1 and J). Hyperfine constants were printed in mK (1 mK = 0.001 cm-1) and converted to MHz. Pickering's B values carry no uncertainty and are approximate. Pickering 1996 was read from the ADS scan (OCR text checked against page images for Tables 1 and 2, pages 814, 817, 818). Nitz 1995 lifetimes could only be read through an automated reader of the publisher's page; each carries its cross-check. rme_J_ea0 derived from A (S = A g_upper lambda_vac^3 / 2.0261e18). NIST labels '°7/2' at 33173.36, 33466.87, 33945.9, 43847.98, 44201.92 correspond to Pickering's y4F7/2, y4G7/2, y4F5/2, w4F7/2, w4F5/2. WebSearch was unavailable in this session (budget exhausted).

Atoms with measured data

All elements: periodic table