Atomic energy level diagrams

Lutetium energy level diagram

Energy levels and transitions of neutral lutetium (Lu I): the 66 strongest classified lines below 2 µm from the NIST Atomic Spectra Database and the 41 levels they connect, each line with its vacuum wavelength, frequency and, for 45 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.

Lutetium energy level diagram with transition wavelengths and dipole matrix elements

Download: diagram (PDF) diagram (SVG) transitions (CSV) levels (CSV) source code

Key transitions of lutetium

Transitionλ vac (nm)λ air (nm)ν (THz)|⟨J‖er‖J′⟩| (ea₀)A (s⁻¹)Γ/2π up. (MHz)branch (%)Use
5d6s2 2D3/2 – 5d6s6p 2D°3/2451.9823451.8556663.28362.0302.260e+073.62599.4451.9 nm line of collinear laser spectroscopy at ISOLDE
5d6s2 2D3/2 – 5d6s6p 2D°5/2465.9316465.8011643.42600.9713.150e+061.94325.8first step
5d6s2 2D3/2 – 5d6s6p 4F°5/2540.4068540.2565554.75330.7491.200e+060.337256.6first step
5d6s2 2D3/2 – 5d6s6p 4F°3/2573.8130573.6539522.45670.8031.730e+060.287396first step

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).

175Lu hyperfine structure (I = 7/2)

LevelA (MHz)B (MHz)Shift of each F level from the centre of gravity (MHz)
5d6s2 2D3/2194.33162(9)1511.3987(7)F=2: -502.06 F=3: -998.64 F=4: -653.14 F=5: +1398.09
5d6s2 2D5/2146.7761860.656F=1: -654.46 F=2: -892.52 F=3: -1050.26 F=4: -888.44 F=5: -88.11 F=6: +1749.46
6s26p 2P°3/2221(8)2091(23)F=2: -370.22 F=3: -1201.39 F=4: -915.62 F=5: +1681.95
5d6s6p 4F°3/2-924.7(5)1767(6)F=2: +7188.33 F=3: +3152.09 F=4: -1051.57 F=5: -4412.93
5d6s6p 4F°5/2987.2(4)1117(6)F=1: -10507.61 F=2: -8852.35 F=3: -6249.79 F=4: -2556.30 F=5: +2419.59 F=6: +8917.25
5d6s6p 4F°7/21016(4)2531(22)F=0: -14653.98 F=1: -13895.75 F=2: -12327.62 F=3: -9846.31 F=4: -6296.84 F=5: -1472.61 F=6: +4884.66 F=7: +13084.88
5d6s6p 4D°1/2-2244(3)–F=3: +5049.00 F=4: -3927.00
5d6s6p 4D°3/21026(5)615(14)F=2: -6595.36 F=3: -3956.95 F=4: -29.06 F=5: +5539.73
5d6s6p 2D°5/21398.2(15)-689(30)F=1: -16098.86 F=2: -13105.60 F=3: -8689.54 F=4: -2939.25 F=5: +4027.14 F=6: +12062.00
5d6s6p 2D°3/2-1424.7(7)-501(6)F=2: +9348.33 F=3: +5432.09 F=4: -123.57 F=5: -7604.93
5d6s6p 4D°5/21092(3)855(30)F=1: -11826.96 F=2: -9887.25 F=3: -6886.07 F=4: -2713.50 F=5: +2777.04 F=6: +9768.75
6s27s 2S1/21170(3)–F=3: -2632.50 F=4: +2047.50
5d26s 2P3/2-1021(3)-1190(15)F=2: +6254.25 F=3: +4041.25 F=4: +297.25 F=5: -5657.75
6s6p2 4P5/21933.660-2509.260F=1: -23097.92 F=2: -18513.67 F=3: -11906.14 F=4: -3597.96 F=5: +5980.73 F=6: +16292.21

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

Isotope shifts

Transitionλ vac (nm)IsotopesShift (MHz)
5d6s2 2D3/2 – 5d6s6p 2D°3/2451.982175-176435(7)

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

Closed and nearly closed transitions of lutetium

Transitionλ vacuum (nm)Lower levelA (s⁻¹)Leak per scattered photonPhotons before a leakWhere the leak goes
5d6s2 2D5/2 → 5d6s6p 2F°7/2336.0526metastable2.440e+08 measured0.1 % from measured data1,000leak channels not listed
5d6s2 2D3/2 → 5d6s6p 2P°1/2311.9336ground2.030e+08 measured0.5 % from measured data200leak channels not listed
5d6s2 2D3/2 → 5d6s6p 2P°1/2299.0153ground1.280e+08 measured0.5 % from measured data200leak channels not listed
5d6s2 2D3/2 → 5d6s6p 2D°3/2451.9823ground2.260e+07 measured0.6 % from measured data1675d6s2 2D5/2 0.14 % (long-lived); the listed lines add up to 0.14 %
5d6s2 2D3/2 → 5d6s6p 2D°3/2337.7464ground1.680e+08 measured1 % from measured data1005d6s2 2D5/2 0.649 % (long-lived)
5d6s2 2D3/2 → 5d6s6p 2F°5/2331.3063ground1.850e+08 measured1.9 % from measured data535d6s2 2D5/2 1.39 % (long-lived)
5d6s2 2D5/2 → 5d6s6p 2D°5/2328.2694metastable3.050e+08 measured2.4 % from measured data425d6s2 2D3/2 2.29 % (long-lived)
5d6s2 2D5/2 → 5d6s6p 2P°3/2308.2370metastable2.620e+08 measured2.9 % from measured data345d6s2 2D3/2 2.92 % (long-lived)
5d6s2 2D5/2 → 5d6s6p 2F°7/2363.7287metastable6.400e+06 measured3 % from measured data33leak channels not listed
5d6s2 2D3/2 → 5d6s6p 4F°3/2573.8130ground1.730e+06 measured4 % from measured data255d6s2 2D5/2 4 % (long-lived)
5d6s2 2D3/2 → 6s27p 2P°1/2339.7772ground1.030e+08 measured5 % from measured data20leak channels not listed
5d6s2 2D3/2 → 5d6s6p 4D°1/2481.6383ground9.000e+05 measured5 % from measured data20leak channels not listed

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 Lu 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
5d6s2 2D3/26s25f 2F°5/2272.9752272.89441098.2405E11.182 measured2.320e+07 measured70Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D5/26s25f 2F°7/2288.5986288.51401038.7869E11.481 measured2.310e+07 measured70Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/25d6s6p 2P°3/2290.3896290.30461032.3800E10.618 measured7.900e+06 measured2.92Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/25d6s6p 2P°1/2299.0153298.92811002.5989E11.838 measured1.280e+08 measured99.5Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/25d6s6p 2D°5/2308.1028308.0133973.0274E10.790 measured7.200e+06 measured2.29Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D5/25d6s6p 2P°3/2308.2370308.1475972.6038E13.892 measured2.620e+08 measured97.1Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/25d6s6p 2P°1/2311.9336311.8432961.0777E12.466 measured2.030e+08 measured99.5Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/25d6s6p 2P°3/2317.2284317.1366945.0367E12.040 measured6.600e+07 measured56.2Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/26s27p 2P°3/2327.9912327.8967914.0258E12.639 measured1.000e+08 measured59Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D5/25d6s6p 2D°5/2328.2694328.1749913.2512E15.652 measured3.050e+08 measured97.6Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/25d6s6p 2F°5/2331.3063331.2110904.8801E14.463 measured1.850e+08 measured98.1Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D5/25d6s6p 2F°7/2336.0526335.9560892.0999E16.047 measured2.440e+08 measured99.9Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/25d6s6p 2D°3/2337.7464337.6495887.6258E13.575 measured1.680e+08 measured99Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D5/25d6s6p 2P°3/2338.6489338.5517885.2604E11.964 measured5.030e+07 measured42.8Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/26s27p 2P°1/2339.7772339.6797882.3207E11.997 measured1.030e+08 measured95Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D5/26s27p 2P°3/2350.9425350.8421854.2496E12.355 measured6.500e+07 measured38.5Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D5/25d6s6p 2F°5/2354.7404354.6390845.1038E10.586 measured2.600e+06 measured1.39Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/25d6s6p 2F°5/2356.8865356.7847840.0218E13.048 measured6.900e+07 measured72.1Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
6s26p 2P°3/26s6p2 4P5/2359.7367359.6341833.3664E1 (intercombination)––15.3–
5d6s2 2D5/25d6s6p 2D°3/2362.1340362.0307827.8496E10.321 NIST1.100e+06 NIST0.649NIST ASD (accuracy D)
5d6s2 2D5/25d6s6p 2F°7/2363.7287363.6250824.2200E11.103 measured6.400e+06 measured97Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
6s26p 2P°1/26s26d 2D3/2364.8821364.7782821.6145E12.970 measured9.200e+07 measured84.5Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
6s26p 2P°1/25d26s 2S1/2375.7820375.6753797.7828E1––34.9–
5d6s2 2D5/25d6s6p 2F°5/2384.2283384.1194780.2455E12.110 measured2.650e+07 measured27.8Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
6s26p 2P°1/25d26s 2P3/2387.5703387.4605773.5176E1––12.6–
6s26p 2P°3/26s6p2 4P1/2391.9996391.8886764.7775E1 (intercombination)––11.8–
5d6s2 2D3/25d6s6p 4P°5/2396.9583396.8461755.2240E1 (intercombination)0.640 measured2.210e+06 measured73.2Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
6s26p 2P°1/25d26s 2P1/2405.5596405.4450739.2070E11.150 measured2.010e+07 measured91.9Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/25d6s6p 4P°3/2411.3857411.2696728.7382E1 (intercombination)0.243 measured4.300e+05 measured70.6Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
6s26p 2P°3/26s26d 2D5/2412.5887412.4724726.6133E14.302 measured8.900e+07 measured100Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
6s26p 2P°3/26s26d 2D3/2415.5266415.4094721.4760E11.543 measured1.680e+07 measured15.5Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
6s26p 2P°3/25d26s 2S1/2429.7211429.6002697.6443E1––62.1–
5d6s2 2D5/25d6s6p 4P°5/2431.0783430.9571695.4478E1 (intercombination)0.396 measured6.600e+05 measured21.8Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
6s26p 2P°3/25d26s 2P3/2445.2060445.0811673.3791E1––75–
5d6s2 2D5/25d6s6p 4P°3/2448.1457448.0200668.9620E1 (intercombination)0.125 measured8.800e+04 measured14.4Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/25d6s6p 4D°5/2450.0110449.8848666.1892E1 (intercombination)0.186 measured1.280e+05 measured11Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/25d6s6p 2D°3/2451.9823451.8556663.2836E12.030 measured2.260e+07 measured99.4Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/25d6s6p 2D°5/2465.9316465.8011643.4260E10.971 measured3.150e+06 measured25.8Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
6s26p 2P°3/25d26s 2P1/2469.1085468.9772639.0685E10.367 measured1.320e+06 measured6.1Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/25d6s6p 4D°3/2471.8012471.6692635.4212E1 (intercombination)0.153 measured1.130e+05 measured27.7Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/25d6s6p 4D°1/2481.6383481.5037622.4432E1 (intercombination)0.315 measured9.000e+05 measured95Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
6s26p 2P°1/25d26s 2D3/2490.6249490.4879611.0421E1––96.8–
5d6s2 2D5/25d6s6p 4D°5/2494.3701494.2322606.4130E1 (intercombination)0.589 measured9.700e+05 measured84Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D5/25d6s6p 2D°3/2496.7503496.6117603.5074E10.0894 measured3.300e+04 measured0.14Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
6s26p 2P°1/26s27s 2S1/2500.2536500.1141599.2809E11.989 measured3.200e+07 measured39.3Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D5/25d6s6p 2D°5/2513.6513513.5082583.6498E11.911 measured9.100e+06 measured74.2Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D5/25d6s6p 4D°3/2520.7940520.6490575.6450E1 (intercombination)0.266 measured2.540e+05 measured62.3Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D3/25d6s6p 4F°5/2540.4068540.2565554.7533E1 (intercombination)0.749 measured1.200e+06 measured56.6Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D5/25d6s6p 4F°7/2542.3402542.1895552.7756E1 (intercombination)––100–
6s26p 2P°1/25d26s 4P3/2545.5112545.3596549.5625E1 (intercombination)––80.6–
5d6s2 2D3/25d6s6p 4F°3/2573.8130573.6539522.4567E1 (intercombination)0.803 measured1.730e+06 measured96Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
6s26p 2P°3/25d26s 2D3/2586.7887586.6261510.9036E1––2.18–
5d6s6p 4F°5/26s6p2 4P5/2596.3058596.1406502.7495E1––3.5–
6s26p 2P°3/26s27s 2S1/2600.6150600.4487499.1424E13.247 measured4.930e+07 measured60.7Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D5/25d6s6p 4F°5/2605.6693605.5016494.9771E1 (intercombination)0.778 measured9.200e+05 measured43.4Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
5d6s2 2D5/25d6s6p 4F°3/2647.9470647.7680462.6805E1 (intercombination)0.197 measured7.200e+04 measured4Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…
6s26p 2P°3/25d26s 4P3/2667.0593666.8752449.4240E1 (intercombination)––19.4–
5d6s6p 2D°5/26s6p2 4P5/2724.0018723.8023414.0769E1 (intercombination)––10.7–
5d6s6p 4D°3/26s6p2 4P3/2791.3840791.1664378.8204E1––17.7–
5d6s6p 4D°1/26s6p2 4P1/2818.0528817.8279366.4708E1––32.5–
5d6s6p 4D°3/26s6p2 4P1/2848.0865847.8535353.4928E1––29.7–
5d6s6p 4D°7/26s6p2 4P5/2851.0450850.8112352.2639E1––36.8–
5d6s6p 4D°5/26s6p2 4P3/2861.3428861.1062348.0525E1––47.8–
5d6s6p 4P°3/26s6p2 4P5/2911.8754911.6252328.7647E1––11.6–
5d6s6p 4P°5/26s6p2 4P5/2991.7742991.5024302.2789E1––17.9–
5d6s6p 4P°1/26s6p2 4P3/21028.51671028.2348291.4804E1––12.9–

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, or a model calculation.

Lu energy levels

LevelEnergy (cm⁻¹)JParityLifetimegJHyperfine A (MHz)Hyperfine B (MHz)Lifetime sourceHyperfine source
5d6s2 2D3/20.0003/2evenstable0.79921194.3321511.4–Brenner, Büttgenbach, Rupprecht, Träber, Nucl. Phys. A 440, 407 (1985) (atomic-beam magne…
5d6s2 2D5/21993.9205/2even–1.2004146.7761860.66–"Ref. 9" of Reddy & Rao 1989 (reference list not visible on the page read; magnetic-reson…
6s26p 2P°1/24136.1301/2odd–0.66––––
6s26p 2P°3/27476.3903/2odd–1.33220.82091–Reddy, Rao, J. Opt. Soc. Am. B 6, 1481 (1989), Table 2
5d6s6p 4F°3/217427.2803/2odd554 ns measured0.5-924.71767Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…"Ref. 11" of Reddy & Rao 1989 (reference list not visible; original not opened); quoted i…
5d6s6p 4F°5/218504.5805/2odd472 ns measured1.07987.21117Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…"Ref. 12" of Reddy & Rao 1989 (reference list not visible; original not opened); quoted i…
5d6s6p 4F°7/220432.5307/2odd–1.221016.52531–Reddy, Rao, J. Opt. Soc. Am. B 6, 1481 (1989), Table 2
5d6s6p 4D°1/220762.4701/2odd1.05 µs measured–-2244–Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…"Ref. 7" of Reddy & Rao 1989 (reference list not visible; original not opened); quoted in…
5d6s6p 4D°3/221195.3703/2odd2.45 µs measured1.191025.9615Kwiatkowski, Zimmermann, Biémont, Grevesse 1980 (quoted in Fedchak, Den Hartog, Lawler, P…Reddy, Rao, J. Opt. Soc. Am. B 6, 1481 (1989), Table 2
5d6s6p 2D°5/221462.3805/2odd81.9 ns measured1.231398.2-689Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…Vergès, Wyart, Phys. Scr. 17, 495 (1978) (Fourier-transform spectra; printed 46.64(5) mK …
5d6s6p 2D°3/222124.7603/2odd43.9 ns measured0.874-1424.7-501Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…Georg, Borchers, Keim, Klein, Neugart, Neuroth, Schulz, Rao, Eur. Phys. J. A 3, 225 (1998…
5d6s6p 4D°5/222221.6805/2odd862 ns measured1.391092855Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…"Ref. 7" of Reddy & Rao 1989 (reference list not visible; original not opened); quoted in…
5d26s 4P3/222467.5603/2even–1.73––––
5d6s6p 4D°7/223524.2407/2odd–1.41––––
5d6s6p 4P°1/224108.7201/2odd––––––
6s27s 2S1/224125.9901/2even12.3 ns measured2.051170–Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…"Ref. 10" of Reddy & Rao 1989 (reference list not visible; original not opened); quoted i…
5d6s6p 4P°3/224308.0903/2odd1.64 µs measured1.67––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
5d26s 2D3/224518.3003/2even––––––
5d6s6p 4P°5/225191.5605/2odd332 ns measured1.53––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
5d6s6p 2F°5/228020.1105/2odd10.5 ns measured0.88––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
5d26s 2P1/228793.4201/2even45.7 ns measured0.98––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
6s27p 2P°1/229431.0501/2odd9.2 ns measured–––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
5d6s6p 2F°7/229486.9407/2odd151 ns measured–––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
5d6s6p 2D°3/229608.0103/2odd5.9 ns measured–––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
5d26s 2P3/229937.9003/2even––-1021-1190–Vergès, Wyart, Phys. Scr. 17, 495 (1978) (printed -34.05(10) mK, -39.7(5) mK, converted t…
5d6s6p 2F°5/230183.5505/2odd5.3 ns measured–––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
6s27p 2P°3/230488.6203/2odd5.9 ns measured1.23––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
5d26s 2S1/230747.3001/2even–2.2––––
5d6s6p 2P°3/231523.0303/2odd8.5 ns measured–––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
6s26d 2D3/231542.2403/2even9.2 ns measured0.8––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
6s26d 2D5/231713.6005/2even11.2 ns measured1.23––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
5d6s6p 2F°7/231751.1707/2odd4.1 ns measured–––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
5d6s6p 2P°1/232058.1001/2odd4.9 ns measured–––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
5d6s6p 2D°5/232456.7005/2odd3.2 ns measured–––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
6s6p2 4P1/232986.6201/2even–2.62––––
5d6s6p 2P°1/233443.1001/2odd7.8 ns measured–––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
6s6p2 4P3/233831.4603/2even–1.75––––
5d6s6p 2P°3/234436.4903/2odd3.7 ns measured–––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
6s6p2 4P5/235274.5005/2even–1.511933.66-2509.26–Vergès, Wyart, Phys. Scr. 17, 495 (1978) (printed 64.5 mK, -83.70 mK); quoted in Suryanar…
6s25f 2F°5/236633.3605/2odd30.2 ns measured–––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–
6s25f 2F°7/236644.1207/2odd30.3 ns measured–––Fedchak, Den Hartog, Lawler, Palmeri, Quinet, Biémont, Astrophys. J. 542, 1109 (2000), Ta…–

Lu⁺ ionisation limit 43762.60 cm⁻¹ = 5.42587 eV (228.506 nm)

Sources

Hyperfine convention: E = A K/2 + B [3K(K+1)/4 - I(I+1)J(J+1)] / [2I(2I-1)J(2J-1)], K = F(F+1)-I(I+1)-J(J+1) (as in Georg et al.). 175Lu I = 7/2, 176Lu I = 7. Lifetimes, branching fractions and A values are from Fedchak et al. 2000 (PDF opened via the Internet Archive copy of the publisher file; table rows were extracted by script and matched to NIST levels by energy and J); Table 4 gives 65 branching fractions, Table 5 gives 44 A values, all entered; these A values are the ones NIST ASD already lists, here with their uncertainties. In Reddy & Rao the parenthesised uncertainties are in units of the last printed digit (195.6(40) = 195.6 ± 4.0 MHz); that table was read twice from the publisher abstract page (which embeds the tables) through an automated page reader, with identical results; the Engleman et al. table was read once the same way. Conversions from mK use 1 mK = 29.9792458 MHz and are marked "derived". Extra fields beyond SCHEMA.md: top-level ionization_limit; transition field use_source; "alternatives" inside lifetime and hyperfine entries. Isotope shift key "175-176" means nu(175) - nu(176).

Atoms with measured data

All elements: periodic table