Iron energy level diagram
Energy levels and transitions of neutral iron (Fe I): the 71 strongest classified lines below 2 µm from the NIST Atomic Spectra Database and the 47 levels they connect, each line with its vacuum wavelength, frequency and, for 71 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.

Download: diagram (PDF) diagram (SVG) transitions (CSV) levels (CSV) source code
Key transitions of iron
| Transition | λ vac (nm) | λ air (nm) | ν (THz) | |⟨J‖er‖J′⟩| (ea₀) | A (s⁻¹) | Γ/2π up. (MHz) | branch (%) | Use |
|---|---|---|---|---|---|---|---|---|
| a 5F5 – z 5G°6 | 358.2215 | 358.1193 | 836.8913 | 5.662 | 1.087e+08 | 17.3 | 100 | 358 nm laser-cooling line of iron |
| a 5D4 – z 5F°5 | 372.0993 | 371.9934 | 805.6787 | 2.129 | 1.620e+07 | 2.631 | 99.6 | 372 nm resonance line: laser collimation / cooling of an… |
| a 5F5 – z 5F°5 | 501.3466 | 501.2068 | 597.9745 | ≈0.539 | 4.251e+05 | 2.631 | 2.57 | decay channel that completes optical pumping from the gro… |
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).
57Fe hyperfine structure (I = 1/2)
| Level | A (MHz) | B (MHz) | Shift of each F level from the centre of gravity (MHz) |
|---|---|---|---|
| a 5D4 | 38.0795(10) | – | F=7/2: -95.20 F=9/2: +76.16 |
| a 5F5 | 87.246(3) | – | F=9/2: -261.74 F=11/2: +218.12 |
| z 5F°5 | 81.7(9) | – | F=9/2: -245.07 F=11/2: +204.22 |
| z 5G°6 | 31.24(5) | – | F=11/2: -109.34 F=13/2: +93.72 |
Measured A, B constants; sources in the data file.
Isotope shifts
| Transition | λ vac (nm) | Isotopes | Shift (MHz) |
|---|---|---|---|
| a 5F5 – z 5G°6 | 358.221 | 56-54 | 592.3(6) |
| a 5F5 – z 5G°6 | 358.221 | 57-56 | 299.7(6) |
| a 5F5 – z 5G°6 | 358.221 | 58-56 | 566.0(5) |
| a 5D4 – z 5F°5 | 372.099 | 56-54 | 726(8) |
| a 5D4 – z 5F°5 | 372.099 | 57-56 | 365(6) |
| a 5D4 – z 5F°5 | 372.099 | 58-56 | 690(7) |
Shift = ν(first isotope) − ν(second isotope).
Closed and nearly closed transitions of iron
| Transition | λ vacuum (nm) | Lower level | A (s⁻¹) | Leak per scattered photon | Photons before a leak | Where the leak goes |
|---|---|---|---|---|---|---|
| a 5F5 → z 5G°6 | 358.2215 | metastable | 1.087e+08 measured | 9.61 × 10−6 from semi-empirical calc. | 104,000 | a 3H6 ≈ 5.42 × 10−6; a 3G5 ≈ 3.82 × 10−6; a 3H5 ≈ 2.65 × 10−7; 5 weaker lines |
| a 5F5 → y 5G°6 | 278.8927 | metastable | 5.920e+07 NIST | 2.3 × 10−4 from semi-empirical calc. | 4,350 | a 3H5 ≈ 1.36 × 10−4; a 3H6 ≈ 5.91 × 10−5; b 3G5 ≈ 2.06 × 10−5; 5 weaker lines |
| a 5D4 → z 5F°5 | 372.0993 | ground | 1.620e+07 NIST | 0.42 % from measured data | 238 | a 5F5 ≈ 2.57 % (long-lived); a 5F4 6.9 × 10−4 (long-lived); a 3F4 ≈ 1.73 × 10−5 (long-lived); 11 weaker lines; the listed lines add up to ≈ 2.64 % |
| a 5F5 → x 5G°6 | 258.5309 | metastable | 3.150e+07 NIST | 1.12 % from semi-empirical calc. | 89 | a 3H5 1.08 %; b 3H6 ≈ 2 × 10−4; a 3G5 ≈ 1.25 × 10−4; 6 weaker lines |
| a 5D4 → x 5F°5 | 248.4021 | ground | 4.800e+08 NIST | ≥ 3.89 % from semi-empirical calc. | ≤ 26 | a 5F5 3.4 % (long-lived); a 5F4 0.49 % (long-lived); a 3F4 ≈ 2.87 × 10−6 (long-lived); 16 weaker lines; 1 more possible path without a listed rate |
| a 5F5 → v 5F°5 | 245.8341 | metastable | 4.810e+07 NIST | 9.1 % from semi-empirical calc. | 11 | a 3G5 ≈ 2.72 %; b 3F24 2.22 %; a 5D4 ≈ 1.51 % (long-lived); 22 weaker lines |
| a 5D3 → z 5F°4 | 373.8194 | metastable | 1.410e+07 NIST | 9.31 % from semi-empirical calc. | 11 | a 5D4 8.75 % (long-lived); a 5F4 0.295 % (long-lived); a 5F3 0.152 % (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 Fe 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 |
|---|---|---|---|---|---|---|---|---|---|
| a 5D4 | u 5P°3 | 193.4535 | – | 1549.6875 | E1 | 0.791 NIST | 2.500e+07 NIST | – | NIST ASD (accuracy C+) |
| a 5D4 | u 5F°3 | 193.7268 | – | 1547.5010 | E1 | 0.743 NIST | 2.200e+07 NIST | – | NIST ASD (accuracy C+) |
| a 5D3 | u 5P°2 | 194.0660 | – | 1544.7961 | E1 | 0.685 NIST | 2.600e+07 NIST | – | NIST ASD (accuracy D+) |
| a 5D4 | w 5P°3 | 216.7453 | 216.6773 | 1383.1554 | E1 | 3.082 NIST | 2.700e+08 NIST | 86.4 | NIST ASD (accuracy D+) |
| a 5D2 | w 5P°2 | 219.2524 | 219.1839 | 1367.3393 | E1 | 1.767 NIST | 1.200e+08 NIST | 38.4 | NIST ASD (accuracy C+) |
| a 5D1 | w 5P°1 | 219.6728 | 219.6042 | 1364.7227 | E1 | 1.372 NIST | 1.200e+08 NIST | 42 | NIST ASD (accuracy C+) |
| a 5D0 | w 5P°1 | 220.1077 | 220.0390 | 1362.0263 | E1 | 1.185 NIST | 8.900e+07 NIST | 31.1 | NIST ASD (accuracy C) |
| a 5D1 | w 5P°2 | 220.1411 | 220.0724 | 1361.8194 | E1 | 0.859 NIST | 2.800e+07 NIST | 8.96 | NIST ASD (accuracy C) |
| a 5D3 | w 5D°3 | 229.8495 | 229.7787 | 1304.2991 | E1 | 0.777 NIST | 1.440e+07 NIST | 12.2 | NIST ASD (accuracy D+) |
| a 5D4 | w 5D°4 | 229.8877 | 229.8169 | 1304.0823 | E1 | 1.291 NIST | 3.090e+07 NIST | 22.9 | NIST ASD (accuracy D+) |
| a 5D3 | w 5D°4 | 232.1070 | 232.0357 | 1291.6130 | E1 | 0.885 NIST | 1.410e+07 NIST | 10.4 | NIST ASD (accuracy C) |
| a 5F5 | v 5F°5 | 245.8341 | 245.7597 | 1219.4911 | E1 | 1.970 NIST | 4.810e+07 NIST | 100 | NIST ASD (accuracy B) |
| a 5D4 | x 5F°4 | 246.3392 | 246.2647 | 1216.9905 | E1 | 1.971 NIST | 5.850e+07 NIST | 11.7 | NIST ASD (accuracy C+) |
| a 5F5 | w 5G°5 | 246.9626 | 246.8880 | 1213.9184 | E1 | 1.401 NIST | 2.400e+07 NIST | 48.5 | NIST ASD (accuracy B+) |
| a 5D3 | x 5F°3 | 247.3642 | 247.2895 | 1211.9476 | E1 | 2.607 NIST | 1.300e+08 NIST | 26 | NIST ASD (accuracy B) |
| a 5D2 | x 5F°2 | 248.0525 | 247.9776 | 1208.5846 | E1 | 2.560 NIST | 1.740e+08 NIST | 34.8 | NIST ASD (accuracy B) |
| a 5D4 | x 5F°5 | 248.4021 | 248.3271 | 1206.8839 | E1 | 6.320 NIST | 4.800e+08 NIST | 96 | NIST ASD (accuracy B) |
| a 5D1 | x 5F°1 | 248.4937 | 248.4187 | 1206.4388 | E1 | 2.266 NIST | 2.260e+08 NIST | 45.2 | NIST ASD (accuracy C+) |
| a 5D3 | x 5F°4 | 248.8893 | 248.8142 | 1204.5211 | E1 | 5.363 NIST | 4.200e+08 NIST | 84 | NIST ASD (accuracy B) |
| a 5D0 | x 5F°1 | 249.0503 | 248.9752 | 1203.7424 | E1 | 2.299 NIST | 2.310e+08 NIST | 46.2 | NIST ASD (accuracy C+) |
| a 5D2 | x 5F°3 | 249.1396 | 249.0644 | 1203.3114 | E1 | 4.287 NIST | 3.440e+08 NIST | 68.8 | NIST ASD (accuracy B) |
| a 5D1 | x 5F°2 | 249.1906 | 249.1155 | 1203.0647 | E1 | 3.333 NIST | 2.910e+08 NIST | 58.2 | NIST ASD (accuracy B) |
| a 5D4 | x 5D°3 | 250.1886 | 250.1132 | 1198.2660 | E1 | 1.932 measured | 6.900e+07 measured | 17.9 | Belmonte, Pickering, Ruffoni, Den Hartog, Lawler, Guzman, Heiter, Astrophys. J. 848, 125 … |
| a 5D3 | x 5D°2 | 251.1591 | 251.0835 | 1193.6357 | E1 | 2.246 NIST | 1.290e+08 NIST | 33.5 | NIST ASD (accuracy B) |
| a 5D2 | x 5D°1 | 251.8859 | 251.8101 | 1190.1914 | E1 | 2.090 measured | 1.845e+08 measured | 51.7 | Belmonte, Pickering, Ruffoni, Den Hartog, Lawler, Guzman, Heiter, Astrophys. J. 848, 125 … |
| a 5D4 | x 5D°4 | 252.3608 | 252.2849 | 1187.9517 | E1 | 3.900 NIST | 2.130e+08 NIST | 55.4 | NIST ASD (accuracy B) |
| a 5D1 | x 5D°0 | 252.5052 | 252.4292 | 1187.2726 | E1 | 1.602 NIST | 3.230e+08 NIST | 84 | NIST ASD (accuracy B) |
| a 5D3 | x 5D°3 | 252.8194 | 252.7434 | 1185.7967 | E1 | 3.202 measured | 1.836e+08 measured | 47.7 | Belmonte, Pickering, Ruffoni, Den Hartog, Lawler, Guzman, Heiter, Astrophys. J. 848, 125 … |
| a 5D2 | x 5D°2 | 252.9895 | 252.9135 | 1184.9995 | E1 | 1.990 NIST | 9.910e+07 NIST | 25.8 | NIST ASD (accuracy B) |
| a 5D1 | x 5D°1 | 253.0596 | 252.9835 | 1184.6715 | E1 | 0.869 measured | 3.148e+07 measured | 8.81 | Belmonte, Pickering, Ruffoni, Den Hartog, Lawler, Guzman, Heiter, Astrophys. J. 848, 125 … |
| a 5D0 | x 5D°1 | 253.6369 | 253.5607 | 1181.9751 | E1 | 1.520 measured | 9.563e+07 measured | 26.8 | Belmonte, Pickering, Ruffoni, Den Hartog, Lawler, Guzman, Heiter, Astrophys. J. 848, 125 … |
| a 5D1 | x 5D°2 | 254.1735 | 254.0972 | 1179.4796 | E1 | 1.971 NIST | 9.590e+07 NIST | 24.9 | NIST ASD (accuracy C+) |
| a 5D2 | x 5D°3 | 254.6743 | 254.5978 | 1177.1605 | E1 | 2.019 measured | 7.144e+07 measured | 18.6 | Belmonte, Pickering, Ruffoni, Den Hartog, Lawler, Guzman, Heiter, Astrophys. J. 848, 125 … |
| a 5D3 | x 5D°4 | 255.0378 | 254.9613 | 1175.4824 | E1 | 1.305 NIST | 2.310e+07 NIST | 6.01 | NIST ASD (accuracy B) |
| a 5F5 | x 5G°5 | 257.7462 | 257.6690 | 1163.1306 | E1 | 1.025 NIST | 1.130e+07 NIST | 31.8 | NIST ASD (accuracy B+) |
| a 5F5 | x 5G°6 | 258.5309 | 258.4536 | 1159.6000 | E1 | 1.869 NIST | 3.150e+07 NIST | 98.9 | NIST ASD (accuracy B+) |
| a 5F5 | w 5F°5 | 267.9857 | 267.9061 | 1118.6881 | E1 | 1.252 NIST | 1.500e+07 NIST | 58.5 | NIST ASD (accuracy B+) |
| a 5D4 | y 5P°3 | 271.9833 | 271.9027 | 1102.2459 | E1 | 3.142 NIST | 1.420e+08 NIST | 80.9 | NIST ASD (accuracy B+) |
| a 5D3 | y 5P°2 | 272.1708 | 272.0902 | 1101.4865 | E1 | 2.275 NIST | 1.040e+08 NIST | 62.4 | NIST ASD (accuracy B) |
| a 5D2 | y 5P°1 | 272.4384 | 272.3577 | 1100.4046 | E1 | 1.305 NIST | 5.690e+07 NIST | 35.3 | NIST ASD (accuracy B) |
| a 5F5 | w 5D°4 | 273.4389 | 273.3580 | 1096.3781 | E1 | 2.539 NIST | 7.100e+07 NIST | 52.5 | NIST ASD (accuracy C+) |
| a 5D1 | y 5P°1 | 273.8119 | 273.7309 | 1094.8847 | E1 | 1.484 NIST | 7.250e+07 NIST | 45 | NIST ASD (accuracy B) |
| a 5D2 | y 5P°2 | 274.3216 | 274.2405 | 1092.8502 | E1 | 1.547 NIST | 4.700e+07 NIST | 28.2 | NIST ASD (accuracy C+) |
| a 5D3 | y 5P°3 | 275.0953 | 275.0140 | 1089.7766 | E1 | 1.404 NIST | 2.740e+07 NIST | 15.6 | NIST ASD (accuracy B) |
| a 5F5 | y 5G°5 | 277.9040 | 277.8220 | 1078.7627 | E1 | 1.029 NIST | 9.080e+06 NIST | 21 | NIST ASD (accuracy B+) |
| a 5F5 | y 5G°6 | 278.8927 | 278.8105 | 1074.9384 | E1 | 2.870 NIST | 5.920e+07 NIST | 100 | NIST ASD (accuracy B+) |
| a 5D4 | y 5F°4 | 293.7762 | 293.6903 | 1020.4790 | E1 | 1.256 NIST | 1.400e+07 NIST | 10.8 | NIST ASD (accuracy C+) |
| a 5D3 | y 5F°3 | 294.8737 | 294.7876 | 1016.6807 | E1 | 1.273 NIST | 1.830e+07 NIST | 14.1 | NIST ASD (accuracy B) |
| a 5D2 | y 5F°2 | 295.4803 | 295.3940 | 1014.5937 | E1 | 1.097 NIST | 1.890e+07 NIST | 14.5 | NIST ASD (accuracy A) |
| a 5D4 | y 5F°5 | 296.7764 | 296.6898 | 1010.1626 | E1 | 1.965 NIST | 2.720e+07 NIST | 21.5 | NIST ASD (accuracy A) |
| a 5D3 | y 5F°4 | 297.4103 | 297.3235 | 1008.0097 | E1 | 1.462 NIST | 1.830e+07 NIST | 14.1 | NIST ASD (accuracy A) |
| a 5D4 | y 5D°3 | 298.4440 | 298.3569 | 1004.5183 | E1 | 1.601 NIST | 2.790e+07 NIST | 15.9 | NIST ASD (accuracy A) |
| a 5D3 | y 5D°2 | 299.5300 | 299.4427 | 1000.8763 | E1 | 1.706 NIST | 4.390e+07 NIST | 28.5 | NIST ASD (accuracy B+) |
| a 5F5 | x 5F°5 | 300.0386 | 299.9511 | 999.1797 | E1 | 1.579 NIST | 1.700e+07 NIST | 3.4 | NIST ASD (accuracy C) |
| a 5D2 | y 5D°1 | 300.1822 | 300.0948 | 998.7015 | E1 | 1.604 NIST | 6.420e+07 NIST | 37.2 | NIST ASD (accuracy A) |
| a 5D1 | y 5D°0 | 300.9015 | 300.8138 | 996.3144 | E1 | 1.199 NIST | 1.070e+08 NIST | 62.1 | NIST ASD (accuracy A) |
| a 5D2 | y 5D°2 | 302.1370 | 302.0491 | 992.2400 | E1 | 1.149 NIST | 1.940e+07 NIST | 12.6 | NIST ASD (accuracy B) |
| a 5D4 | y 5D°4 | 302.1519 | 302.0639 | 992.1914 | E1 | 3.050 NIST | 7.590e+07 NIST | 44.8 | NIST ASD (accuracy B) |
| a 5D3 | y 5D°3 | 302.1952 | 302.1072 | 992.0489 | E1 | 2.083 NIST | 4.550e+07 NIST | 25.9 | NIST ASD (accuracy A) |
| a 5D0 | y 5D°1 | 302.6723 | 302.5842 | 990.4852 | E1 | 1.195 NIST | 3.480e+07 NIST | 20.2 | NIST ASD (accuracy A) |
| a 5D1 | y 5D°2 | 303.8273 | 303.7389 | 986.7201 | E1 | 1.419 NIST | 2.910e+07 NIST | 18.9 | NIST ASD (accuracy B) |
| a 5D2 | y 5D°3 | 304.8491 | 304.7604 | 983.4127 | E1 | 1.667 NIST | 2.840e+07 NIST | 16.2 | NIST ASD (accuracy A) |
| a 5F5 | x 5D°4 | 305.8334 | 305.7445 | 980.2475 | E1 | 1.994 NIST | 3.130e+07 NIST | 8.14 | NIST ASD (accuracy B) |
| a 5D3 | y 5D°4 | 305.9975 | 305.9085 | 979.7220 | E1 | 1.440 NIST | 1.630e+07 NIST | 9.62 | NIST ASD (accuracy C+) |
| a 5D4 | z 5P°3 | 344.1592 | 344.0605 | 871.0867 | E1 | 1.552 NIST | 1.710e+07 NIST | 74.7 | NIST ASD (accuracy B) |
| a 5F5 | z 5G°6 | 358.2215 | 358.1193 | 836.8913 | E1 | 5.662 measured | 1.087e+08 measured | 100 | Belmonte, Pickering, Ruffoni, Den Hartog, Lawler, Guzman, Heiter, Astrophys. J. 848, 125 … |
| a 5D4 | z 5F°5 | 372.0993 | 371.9934 | 805.6787 | E1 | 2.129 NIST | 1.620e+07 NIST | 99.6 | NIST ASD (accuracy A) |
| a 5F5 | y 5F°5 | 373.5926 | 373.4863 | 802.4583 | E1 | 5.050 NIST | 9.010e+07 NIST | 71.2 | NIST ASD (accuracy A) |
| a 5D3 | z 5F°4 | 373.8194 | 373.7131 | 801.9714 | E1 | 1.809 NIST | 1.410e+07 NIST | 89.4 | NIST ASD (accuracy A) |
| a 5F5 | y 5D°4 | 382.1509 | 382.0425 | 784.4871 | E1 | 4.066 NIST | 6.670e+07 NIST | 39.4 | NIST ASD (accuracy A) |
| a 5F5 | z 5F°5 | 501.3466 | 501.2068 | 597.9745 | E1 | 0.539 semi-empirical | 4.251e+05 semi-empirical | 2.57 | Kurucz, R. L., Can. J. Phys. 89, 417 (2011); semi-empirical line list gf2600.pos of 2017-… |
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.
Fe energy levels
Fe⁺ ionisation limit 63737.70 cm⁻¹ = 7.90247 eV (156.893 nm)
Sources
- Belmonte, Pickering, Ruffoni, Den Hartog, Lawler, Guzman, Heiter, Astrophys. J. 848, 125 …
- Belmonte, Pickering, Ruffoni, Den Hartog, Lawler, Guzman, Heiter, Astrophys. J. 848, 125 …
- Childs & Goodman, Phys. Rev. 148, 74 (1966), quoted in Krins, Oppel, Huet, von Zanthier, …
- Dembczynski et al., Z. Phys. A 294, 313 (1980), quoted in Huet, Pettens, Bastin, 'Isotope…
- Huet, Pettens, Bastin, 'Isotope shifts and hyperfine structure of the laser-cooling Fe I …
- Krins, Oppel, Huet, von Zanthier, Bastin, Phys. Rev. A 80, 062508 (2009), Table II
- Kurucz, R. L., Can. J. Phys. 89, 417 (2011); semi-empirical line list gf2600.pos of 2017-…
- NIST ASD
- NIST ASD level energies
- O'Brian, Wickliffe, Lawler, Whaling, Brault, J. Opt. Soc. Am. B 8, 1185 (1991), Table 1 (…
- O'Brian, Wickliffe, Lawler, Whaling, Brault, J. Opt. Soc. Am. B 8, 1185 (1991), Table 1 (…
- O'Brian, Wickliffe, Lawler, Whaling, Brault, J. Opt. Soc. Am. B 8, 1185 (1991), Table 1 (…
- O'Brian, Wickliffe, Lawler, Whaling, Brault, J. Opt. Soc. Am. B 8, 1185 (1991), Table 1 (…
- O'Brian, Wickliffe, Lawler, Whaling, Brault, J. Opt. Soc. Am. B 8, 1185 (1991), Table 1 (…
- O'Brian, Wickliffe, Lawler, Whaling, Brault, J. Opt. Soc. Am. B 8, 1185 (1991), Table 1 (…
- O'Brian, Wickliffe, Lawler, Whaling, Brault, J. Opt. Soc. Am. B 8, 1185 (1991), Table 1 (…
- O'Brian, Wickliffe, Lawler, Whaling, Brault, J. Opt. Soc. Am. B 8, 1185 (1991), Table 1 (…
- O'Brian, Wickliffe, Lawler, Whaling, Brault, J. Opt. Soc. Am. B 8, 1185 (1991), Table 1 (…
Isotope shifts are nu(first)-nu(second) as in the source (delta nu_{56,54} = nu56 - nu54). 57Fe has I=1/2 so only A constants exist. O'Brian 1991 Table 1 was read from the scanned PDF (text layer checked against the page image). Lifetime uncertainties for O'Brian/Belmonte are the papers' blanket 'larger of 5 % or 0.2 ns'. rme_J_ea0 values are derived from measured A (S = A g_upper lambda_vac^3 / 2.0261e18, lambda in Angstrom). WebSearch was unavailable in this session (budget exhausted); sources were located through DOI/bibliographic lookups (Crossref, OpenAlex), VizieR, ADS and arXiv.
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