Atomic energy level diagrams

Erbium-166 energy level diagram

Energy levels and transitions of neutral 166Er (Er I, nuclear spin I = 0): the 90 strongest classified lines below 2 µm from the NIST Atomic Spectra Database and the 73 levels they connect, each line with its vacuum wavelength, frequency and, for 87 of them, the reduced dipole matrix element. Level energies come from NIST and refer to the natural isotope mixture; transition rates are 78 measured, 9 NIST, 1 theory. Hyperfine constants and measured frequencies are those of this isotope.

Hover a line or a level to isolate it, click to keep it selected. Scroll to zoom, drag to move.

Erbium-166 energy level diagram with transition wavelengths and dipole matrix elements

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

Key transitions of 166Er

Transitionλ vac (nm)λ air (nm)ν (THz)|⟨J‖er‖J′⟩| (ea₀)A (s⁻¹)Γ/2π up. (MHz)branch (%)Use
3H6 – (24943)°7400.9097400.7964747.78059.4451.870e+0829.75100broad cooling line: Zeeman slower, transverse cooling, im…
3H6 – (6,1)°7582.8421582.6805514.36311.3101.170e+060.1851100narrow-line MOT
3H6 – (13/2,3/2)°7631.0522630.8778475.06760.5791.800e+050.02842100narrow line proposed for cooling / spin manipulation
3H6 – (15/2,5/2)°7841.2196840.9884356.37840.4695.000e+040.0079581008 kHz narrow-line cooling / narrow-line MOT
3H6 – (15/2,3/2)°71299.21491298.8596230.74890.0105.600e+008.941e-0799.7ultranarrow inner-shell
3H6 – 3F41986.02121985.4791150.9513–4.700e-057.493e-1299.8proposed E2 optical clock transition within the 4f12 6s2…

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)
3H6 – (24943)°7400.910170-166-1681(14)
3H6 – (24943)°7400.910168-166-840(14)
3H6 – (24943)°7400.910167-166-297(6)
3H6 – (24943)°7400.910164-166849(17)
3H6 – (24943)°7400.910170-168-866.5(15)
3H6 – (24943)°7400.910166-164-859.3(16)
3H6 – (24943)°7400.910164-162-1028.7(28)
3H6 – (6,1)°7582.842170-166-1966(14)
3H6 – (6,1)°7582.842168-166-975(15)
3H6 – (6,1)°7582.842167-166-337(11)
3H6 – (15/2,3/2)°71299.215164-168-2732.290(3)
3H6 – (15/2,3/2)°71299.215166-168-1371.710(3)
3H6 – (15/2,3/2)°71299.215170-1681414.920(5)

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

Closed and nearly closed transitions of 166Er

Transitionλ vacuum (nm)Lower levelA (s⁻¹)Leak per scattered photonPhotons before a leakWhere the leak goes
3H6 → (13/2,3/2)°7631.0522ground1.800e+05 measuredclosed–no other level can be reached by electric-dipole decay
3H6 → (15/2,5/2)°7841.2196ground5.000e+04 measuredclosed–no other level can be reached by electric-dipole decay
3H6 → (15/2,3/2)°71299.2149ground5.600e+00 measuredclosed–no other level can be reached by electric-dipole decay
3F3 → (37971)°4390.7305metastable6.411e+07 measured9 % from measured data113H5 4.2 % (long-lived); 3H4 4.1 % (long-lived); 3F4 0.5 % (long-lived); 1 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 166Er 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
3F4(37290)°3310.0352309.9453966.9626E10.737 measured5.271e+06 measured9.4Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3F4(36931)°3313.5242313.4334956.2020E11.084 measured1.103e+07 measured15.5Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°9(39843)8320.2781320.1856936.0379E11.684 measured1.029e+07 measured18.2Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°9(39526)8323.5718323.4785926.5097E11.254 measured5.535e+06 measured10.2Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°6(37715)7327.4597327.3653915.5095E11.602 measured9.867e+06 measured10.8Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°8(39843)8327.9406327.8462914.1668E11.262 measured5.382e+06 measured9.5Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°7(37715)7333.1373333.0415899.9067E11.311 measured6.280e+06 measured6.9Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°9(38254)8337.4602337.3633888.3786E11.340 measured5.565e+06 measured15.5Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°8(38664)7341.1323341.0344878.8159E11.714 measured1.000e+07 measured37.6Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°9(39526)8345.2122345.1134868.4294E11.710 measured8.471e+06 measured15.7Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°8(38254)8345.9779345.8788866.5075E12.451 measured1.729e+07 measured48.2Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°6(36027)6346.6161346.5169864.9121E11.738 measured1.131e+07 measured79.8Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°6(35963)6347.3807347.2812863.0084E11.226 measured5.585e+06 measured33Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°6(35918)6347.9235347.8239861.6620E11.343 measured6.677e+06 measured50.6Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°7(36418)7348.1719348.0722861.0473E12.269 measured1.647e+07 measured50Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°6(35834)7348.9514348.8516859.1238E11.849 measured1.087e+07 measured24.6Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°6(40334)6350.4616350.3614855.4217E11.439 measured7.500e+06 measured22.1Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°8(37807)7351.4089351.3084853.1157E11.492 measured6.933e+06 measured64.8Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°7(40334)6351.5424351.4419852.7918E11.893 measured1.285e+07 measured37.7Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°8(37715)7352.5533352.4525850.3465E14.738 measured6.920e+07 measured76.1Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°8(39843)8353.5348353.4338847.9857E12.654 measured1.900e+07 measured33.6Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°7(35963)6353.7768353.6757847.4057E11.672 measured9.846e+06 measured58.1Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°9(38734)8354.9079354.8065844.7050E12.850 measured2.165e+07 measured45.3Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°7(35834)7355.4060355.3045843.5210E11.969 measured1.167e+07 measured26.5Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°8(39526)8357.5523357.4503838.4575E11.821 measured8.647e+06 measured16.1Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°7(39843)8357.7059357.6038838.0976E11.449 measured5.471e+06 measured9.7Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°5(39351)6357.7906357.6885837.8992E11.853 measured1.169e+07 measured9.6Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°8(39360)7359.6862359.5836833.4834E16.772 measured1.331e+08 measured63.9Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3H5(34684)°5360.6723360.5694831.2046E12.141 measured1.800e+07 measured80.1Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°5(39076)6361.3410361.2380829.6662E12.751 measured2.500e+07 measured48.5Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°7(39526)8361.8194361.7162828.5694E13.530 measured3.135e+07 measured58Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°5(39010)6362.1975362.0942827.7044E12.392 measured1.877e+07 measured41.6Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°8(39145)7362.4793362.3760827.0608E12.195 measured1.367e+07 measured30Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°6(39351)6362.9668362.8634825.9500E14.479 measured6.538e+07 measured53.6Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°7(39360)7364.0046363.9009823.5952E14.942 measured6.840e+07 measured32.8Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°7(39351)6364.1263364.0225823.3201E13.472 measured3.892e+07 measured31.9Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°6(39145)7365.6886365.5844819.8026E11.785 measured8.800e+06 measured19.3Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°5(38703)5366.2757366.1714818.4886E12.124 measured1.691e+07 measured35.7Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°6(39076)6366.6213366.5169817.7171E12.132 measured1.438e+07 measured28Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°7(39145)7366.8655366.7610817.1727E12.433 measured1.620e+07 measured35.6Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°6(38987)7367.8230367.7183815.0454E12.166 measured1.273e+07 measured41Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°8(38734)8367.9640367.8592814.7332E12.543 measured1.547e+07 measured32.3Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°8(38664)7368.9141368.8091812.6348E11.516 measured6.187e+06 measured23.3Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°7(34757)8369.5543369.4491811.2271E11.640 measured6.353e+06 measured64.5Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°6(38787)6370.5520370.4466809.0428E11.502 measured6.908e+06 measured35Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°6(38703)5371.7022371.5965806.5394E12.816 measured2.845e+07 measured60Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,5/2)°6(38668)6372.1897372.0838805.4830E11.325 measured5.308e+06 measured11.9Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3H4(37290)°3376.8095376.7025795.6075E11.057 measured6.043e+06 measured10.7Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(15/2,3/2)°8(35834)7377.5910377.4838793.9608E12.445 measured1.500e+07 measured34Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3H4(36931)°3381.9757381.8673784.8470E12.175 measured2.457e+07 measured34.3Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3H6(25880)°6386.3947386.2851775.8711E16.553 NIST1.160e+08 NIST–NIST ASD (accuracy n/a)
3H6(25682)°5389.3788389.2685769.9250E14.830 NIST7.280e+07 NIST–NIST ASD (accuracy n/a)
3F3(37971)°4390.7305390.6199767.2614E14.122 measured6.411e+07 measured91Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3H4(36280)°4391.7107391.5998765.3416E12.430 measured2.211e+07 measured69.7Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3H6(25393)°6393.8127393.7013761.2564E13.383 NIST2.920e+07 NIST–NIST ASD (accuracy n/a)
3F4(30380)°5394.5538394.4421759.8266E1––––
3H6(25163)°5397.4160397.3036754.3544E14.040 NIST4.790e+07 NIST–NIST ASD (accuracy n/a)
3H6(25159)°7397.4698397.3574754.2521E14.125 NIST3.660e+07 NIST–NIST ASD (accuracy n/a)
(13/2,3/2)°5(40334)6397.6424397.5299753.9248E11.573 measured6.131e+06 measured18Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3H4(35784)°4399.4771399.3641750.4622E11.229 measured5.333e+06 measured81.6Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3H5(31926)°6400.5179400.4047748.5120E11.943 measured9.154e+06 measured100Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3H6(24943)°7400.9097400.7964747.7805E19.445 measured1.870e+08 measured100A. Frisch, PhD thesis 'Dipolar quantum gases of erbium', Univ. Innsbruck (2014), Table 2.4
3F3(37290)°3401.4120401.2986746.8447E13.151 measured4.443e+07 measured79.1Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3H5(31824)°6402.1650402.0513745.4465E1––––
3F3(37125)°3404.0784403.9643741.9165E12.487 measured2.714e+07 measured100Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3F3(36931)°3407.2801407.1652736.0842E11.273 measured6.943e+06 measured9.7Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3H6(24457)°6408.8786408.7632733.2066E13.645 NIST3.030e+07 NIST–NIST ASD (accuracy n/a)
3H6(24083)°5415.2278415.1107721.9951E16.108 NIST9.600e+07 NIST–NIST ASD (accuracy n/a)
3F3(36280)°4418.3664418.2485716.5788E11.343 measured5.544e+06 measured17.5Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3F2(36931)°3419.5906419.4724714.4880E12.721 measured2.900e+07 measured40.5Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(13/2,3/2)°6(38407)6447.6802447.5546669.6577E12.526 measured1.108e+07 measured18Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(6,0)°6(38407)6452.7681452.6412662.1324E13.138 measured1.654e+07 measured26.8Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3H4(32695)°3455.6974455.5697657.8762E11.581 measured7.643e+06 measured84.2Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(6,1)°6(39010)6455.8582455.7305657.6441E12.388 measured9.385e+06 measured20.8Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3H6(11/2,5/2)°6460.7895460.6604650.6061E12.176 NIST7.540e+06 NIST–NIST ASD (accuracy n/a)
(6,1)°6(38752)7461.3010461.1718649.8848E13.999 measured2.200e+07 measured43.8Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(11/2,3/2)°7(40159)7467.6154467.4846641.1090E15.344 measured3.773e+07 measured78.5Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(6,1)°7(38407)6470.5846470.4530637.0639E12.655 measured1.054e+07 measured17.1Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(6,2)°5(39194)6500.1946500.0551599.3517E13.343 measured1.392e+07 measured32.9Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(6,2)°6(39194)6503.3481503.2078595.5967E13.449 measured1.454e+07 measured34.2Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(6,2)°7(38752)7509.5186509.3766588.3837E14.670 measured2.227e+07 measured44.3Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(6,2)°6(38668)6517.0310516.8870579.8346E14.012 measured1.815e+07 measured40.7Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(6,2)°7(38407)6518.6126518.4682578.0663E14.014 measured1.800e+07 measured29.1Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
(21979)°8(39843)8559.7773559.6219535.5567E14.098 measured1.141e+07 measured20.2Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 4 (machine-readabl…
3H6(6,1)°7582.8421582.6805514.3631E11.310 measured1.170e+06 measured100Den Hartog et al. 2010 / Lawler et al. 2010, as quoted in A. Frisch, PhD thesis 'Dipolar …
3H6(13/2,3/2)°6622.2739622.1017481.7693E11.140 NIST8.400e+05 NIST–NIST ASD (accuracy n/a)
3H6(13/2,3/2)°7631.0522630.8778475.0676E10.579 measured1.800e+05 measured100Ban, Jacka, Hanssen, Reader, McClelland, Opt. Express 13, 3185 (2005)
3H6(15/2,5/2)°7841.2196840.9884356.3784E10.469 measured5.000e+04 measured100Ban, Jacka, Hanssen, Reader, McClelland, Opt. Express 13, 3185 (2005)
3H6(15/2,3/2)°71299.21491298.8596230.7489E10.00954 measured5.600e+00 measured99.7A. Patscheider, PhD thesis 'Controlling and Understanding of Dipolar Quantum Gases of Erb…
3H63F41986.02121985.4791150.9513clock–4.700e-05 theory99.8Kozlov, Dzuba, Flambaum, "On the prospects of building optical atomic clocks using Er I o…

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.

166Er energy levels

LevelEnergy (cm⁻¹)JParityLifetimegJHyperfine A (MHz)Hyperfine B (MHz)Lifetime sourceHyperfine source
3H60.0006evenstable1.1638––––
3F45035.1934even2.124e+04 s theory1.147––Kozlov, Dzuba, Flambaum, "On the prospects of building optical atomic clocks using Er I o…–
3H56958.3295even–1.031––––
(15/2,3/2)°67176.5036odd–1.302––––
(15/2,3/2)°77696.9567odd178 ms measured1.266––Patscheider, Yang, Natale, Petter, Chomaz, Mark, Hovhannesyan, Lepers, Ferlaino, Phys. Re…–
(15/2,3/2)°98620.5659odd–1.15––––
(15/2,3/2)°89350.1068odd–1.18––––
(15/2,5/2)°910557.9169odd–1.178––––
3H410750.9824even–0.936––––
(15/2,5/2)°511401.1975odd–1.205––––
(15/2,5/2)°811557.6708odd–1.178––––
(15/2,5/2)°611799.7786odd–1.19––––
(15/2,5/2)°711887.5037odd20 µs measured1.153––Ban, Jacka, Hanssen, Reader, McClelland, Opt. Express 13, 3185 (2005)–
3F312377.5343even–1.065––––
3F213097.9062even–0.75––––
(13/2,3/2)°515185.3525odd–1.16––––
(13/2,3/2)°715846.5497odd5.6 µs measured1.07––Ban, Jacka, Hanssen, Reader, McClelland, Opt. Express 13, 3185 (2005)–
(13/2,3/2)°616070.0956odd–1.2––––
(6,0)°616321.1106odd–1.22––––
(6,1)°617073.8006odd–1.07––––
(6,1)°717157.3077odd860 ns measured1.195––Den Hartog, Chisholm, Lawler, J. Phys. B 43, 155004 (2010), as quoted in A. Patscheider, …–
(11/2,3/2)°718774.1237odd–0.965––––
(6,2)°719125.2537odd–1.235––––
(6,2)°519201.3435odd–1.06––––
(6,2)°619326.5986odd–1.18––––
(11/2,5/2)°621701.8856odd–1.055––––
(21979)°821979.1818odd–1.295––––
(24083)°524083.1665odd–1.128––––
(24457)°624457.1396odd–1.05––––
(24943)°724943.2727odd5.35 ns measured1.16––A. Frisch, PhD thesis 'Dipolar quantum gases of erbium', Univ. Innsbruck (2014), Table 2.…–
(25159)°725159.1437odd–1.17––––
(25163)°525162.5535odd–1.01––––
(25393)°625392.7796odd–1.075––––
(25682)°525681.9335odd–1.175––––
(25880)°625880.2746odd–1.15––––
(30380)°530380.2825odd–1.175––––
(31824)°631823.7486odd–1.045––––
(31926)°631926.0036odd109 ns measured1.215––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(32695)°332695.3703odd111 ns measured0.955––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(34684)°534684.3295odd44.6 ns measured1.08––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(34757)834756.5808even102 ns measured1.14––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(35784)°435783.7074odd153 ns measured1.12––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(35834)735833.7887even22.7 ns measured1.05––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(35918)635918.4546even75.8 ns measured1.095––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(35963)635963.3666even59.1 ns measured1.085––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(36027)636026.8646even70.6 ns measured1.185––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(36280)°436280.0294odd31.5 ns measured1.145––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(36418)736418.4027even30.3 ns measured1.13––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(36931)°336930.6593odd14 ns measured1.01––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(37125)°337125.2063odd36.8 ns measured0.935––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(37290)°337289.5923odd17.8 ns measured1.09––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(37715)737714.6137even11 ns measured1.205––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(37807)737806.9837even93 ns measured1.09––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(37971)°437970.6214odd14.2 ns measured1.02––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(38254)838253.6858even27.9 ns measured1.16––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(38407)638407.4706even16.2 ns measured1.32––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(38664)738664.2497even37.7 ns measured1.17––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(38668)638667.7996even22.4 ns measured1.15––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(38703)538703.0375even21.1 ns measured1.11––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(38734)838734.2438even20.9 ns measured1.135––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(38752)738751.6227even19.9 ns measured1.18––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(38787)638786.5426even50.7 ns measured1.005––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(38987)738986.7657even32.2 ns measured1.075––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(39010)639010.4456even22.2 ns measured1.05––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(39076)639075.8836even19.4 ns measured1.145––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(39145)739145.4507even22 ns measured1.13––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(39194)639193.5646even23.6 ns measured1.115––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(39351)639350.5056even8.2 ns measured1.155––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(39360)739359.6837even4.8 ns measured1.175––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(39526)839525.6038even18.5 ns measured1.11––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(39843)839843.4298even17.7 ns measured1.18––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(40159)740159.2187even20.8 ns measured1.185––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–
(40334)640333.5766even29.4 ns measured1.02––Yu, Wang, Li, Li, Dai, Astrophys. J. Suppl. Ser. 240, 25 (2019), Table 2 (pp. 3-4), colum…–

Er⁺ ionisation limit 49262.00 cm⁻¹ = 6.10771 eV (202.996 nm)

Sources

Isotope shifts are nu(first)-nu(second), keys as printed in the sources (reference isotope 166 for 401/583 nm, 168 for 1299 nm). Hyperfine A, B 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); 167Er (I=7/2) has negative A (inverted structure). Extra fields beyond SCHEMA.md: top-level ionization_limit; level fields lifetime_other, hyperfine_other, level_energy_measured; transition fields linewidth_MHz / linewidth_kHz / linewidth_Hz, wavenumber_cm, leak_to_metastable, isotope_shift_other, g_factor_difference, alternatives (each alternative names its quantity). rme_J_ea0 values are all derived from the A coefficient in the same entry (schema convention, J' = upper level) and inherit its method. A_s for the narrow lines is 1/tau of the upper level (no E1 leak channel exists below them, Ban et al. 2005). g_J without a literature source is copied from the NIST levels file. The 401 nm lifetime entry is the linewidth-derived value; the direct lifetime measurement (Den Hartog 2010) could only be read second-hand. Second pass: added the proposed 3H6 - 3F4 E2 clock transition (theory only) and use annotations from arXiv:2406.16146 and arXiv:2405.01499; no new measured numbers could be sourced. Third pass: added 103 measured lifetimes of high-lying Er I levels (31926-44526 cm^-1) and 356 branching fractions / transition probabilities of their decay lines from Yu et al., Astrophys. J. Suppl. Ser. 240, 25 (2019) (open access); A_s there is

Atoms with measured data

All elements: periodic table