Atomic energy level diagrams

Europium energy level diagram

Energy levels and transitions of neutral europium (Eu I): the 90 strongest classified lines below 2 µm from the NIST Atomic Spectra Database and the 68 levels they connect, each line with its vacuum wavelength, frequency and, for 90 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.

Europium energy level diagram with transition wavelengths and dipole matrix elements

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

Key transitions of europium

Transitionλ vac (nm)λ air (nm)ν (THz)|⟨J‖er‖J′⟩| (ea₀)A (s⁻¹)Γ/2π up. (MHz)branch (%)Use
a 8S°7/2 – y 8P9/2459.5322459.4035652.38628.7811.610e+0826.0999.9broad blue line
a 8S°7/2 – y 8P7/2462.8522462.7226647.70677.8151.560e+0824.8799.8strong blue resonance line of the y8P triplet
a 8S°7/2 – y 8P5/2466.3183466.1878642.89236.7561.520e+0824.11100strong blue resonance line of the y8P triplet
a 10D°9/2 – y 10P11/2506.9356506.7943591.38172.0975.700e+0611.457.92507 nm: optical pumping a10D9/2
a 10D°11/2 – y 10P11/2513.0520512.9091584.33153.9591.960e+0711.4527.2513 nm: optical pumping a10D11/2
a 10D°13/2 – y 10P11/2521.6558521.5105574.69405.7703.960e+0711.4555521.5 nm: decay channel y10P11/2 -> a10D13/2 that populat…
a 10D°13/2 – z 10F15/2583.2594583.0977513.99518.9665.130e+078.162100quasi-cyclic 583 nm transition of the metastable a10D13/2…
a 10D°11/2 – z 10F13/2596.8767596.7114502.26876.7273.080e+077.26767.5decay channel z10F13/2 -> a10D11/2 used in the pump-back
a 10D°13/2 – z 10F13/2608.5535608.3850492.63134.5511.330e+077.26729.1609 nm
a 8S°7/2 – z 10P9/2686.6448686.4554436.60480.9635.800e+050.0970597.3narrow-line "red" MOT at 687 nm
a 10D°7/2 – y 8P9/21147.79461147.4805261.19000.1935.000e+0326.090.0032optical leak of the 460 nm line
a 10D°9/2 – y 8P9/21171.06711170.7467255.99940.3671.700e+0426.090.0108optical leak of the 460 nm line
a 10D°11/2 – y 8P9/21204.23171203.9022248.94920.5002.900e+0426.090.0178optical leak of the 460 nm line
a 8D°7/2 – y 8P9/21577.28461576.8537190.06870.2733.860e+0326.090.0024optical leak of the 460 nm line
a 8D°9/2 – y 8P9/21644.47181644.0227182.30320.6852.140e+0426.090.0133optical leak of the 460 nm line
a 8D°11/2 – y 8P9/21760.09861759.6180170.32711.5749.210e+0426.090.0572optical leak of the 460 nm line

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).

153Eu hyperfine structure (I = 5/2)

LevelA (MHz)B (MHz)Shift of each F level from the centre of gravity (MHz)
a 8S°7/2-8.85320(20)-1.785(4)F=1: +98.64 F=2: +81.45 F=3: +55.46 F=4: +20.45 F=5: -23.87 F=6: -77.91

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

Closed and nearly closed transitions of europium

Transitionλ vacuum (nm)Lower levelA (s⁻¹)Leak per scattered photonPhotons before a leakWhere the leak goes
a 10D°13/2 → z 10F15/2583.2594metastable5.130e+07 measuredclosed–no other level can be reached by electric-dipole decay
a 8S°7/2 → y 8P9/2459.5322ground1.610e+08 measured0.105 % from measured data952a 8D°11/2 5.72 × 10−4; a 10D°11/2 1.78 × 10−4 (long-lived); a 8D°9/2 1.33 × 10−4; 3 weaker lines
a 8S°7/2 → z 10P9/2686.6448ground5.800e+05 measured2.7 % from measured data37a 10D°9/2 1.21 % (long-lived); a 10D°7/2 0.738 % (long-lived); a 10D°11/2 0.738 % (long-lived)

A transition is closed when its upper level can decay only to the level it was excited from, so the atom keeps scattering photons. “closed”: among the levels NIST lists, no other level below the upper level has the opposite parity and |ΔJ| ≤ 1, so no other electric-dipole decay exists. Otherwise the leak is the sum of the branching ratios of the other decay lines of the upper level (or 1 − branching ratio where that of the line itself has been measured), and the number of photons is 1 / leak. “≥” and “≤”: at least one possible decay path has no listed rate, so the leak is a lower limit. These numbers are derived from the branching ratios, lifetimes and rates of this page, not measured as such; the tag names the weakest of the inputs, * marks theory and ≈ a model or semi-empirical calculation. Listed: lines that start on the ground level or on a metastable level and leak at most 10 %, unless more than three possible decay paths have no listed rate. Fine-structure levels only: hyperfine and Zeeman dark states and forbidden decays without a listed rate are not considered. Select a line in the diagram for the full list of its leak channels.

Listed Eu 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
a 8S°7/28P5/2237.3565237.28401263.0472E10.933 NIST2.200e+07 NIST66.9NIST ASD (accuracy C+)
a 8S°7/28P7/2237.6029237.53041261.7371E11.104 NIST2.300e+07 NIST69.9NIST ASD (accuracy C+)
a 8S°7/28P9/2238.0371237.96451259.4356E11.237 NIST2.300e+07 NIST70.6NIST ASD (accuracy C+)
a 8S°7/2y 8D9/2271.0790270.99861105.9230E11.254 NIST1.600e+07 NIST23.2NIST ASD (accuracy C+)
a 8S°7/2y 8D7/2272.4767272.39601100.2500E11.046 NIST1.370e+07 NIST21.6NIST ASD (accuracy C+)
a 8S°7/2(36601)7/2273.2178273.13701097.2653E10.538 NIST3.600e+06 NIST15.8NIST ASD (accuracy C+)
a 8S°7/2(36549)9/2273.6066273.52561095.7064E10.739 NIST5.400e+06 NIST13.5NIST ASD (accuracy C+)
a 8S°7/28P5/2274.4104274.32921092.4968E10.853 NIST1.190e+07 NIST42.7NIST ASD (accuracy C+)
a 8S°7/2(36411)5/2274.6426274.56141091.5731E10.591 NIST5.700e+06 NIST27.8NIST ASD (accuracy C+)
a 8S°7/2(36382)7/2274.8649274.78361090.6902E10.701 NIST6.000e+06 NIST15.1NIST ASD (accuracy C+)
a 8S°7/2x 8P9/2287.9702287.88581041.0536E10.614 NIST3.200e+06 NIST7.55NIST ASD (accuracy C+)
a 8S°7/28P7/2289.3362289.25141036.1388E11.053 NIST1.160e+07 NIST33.3NIST ASD (accuracy C+)
a 8S°7/28P5/2289.3869289.30201035.9574E10.908 NIST1.150e+07 NIST38NIST ASD (accuracy C+)
a 8S°7/28P9/2290.9842290.89901030.2707E10.993 NIST8.100e+06 NIST35.4NIST ASD (accuracy C+)
a 8S°7/26P7/2305.9870305.8980979.7556E1 (intercombination)0.670 measured3.970e+06 measured70.7Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8S°7/2z 8F9/2310.7071310.6170964.8715E10.981 measured6.500e+06 measured14.8Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8S°7/28P9/2311.2332311.1429963.2407E12.216 measured3.300e+07 measured69Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8S°7/2z 10D7/2321.1499321.0571933.4970E1 (intercombination)1.248 measured1.190e+07 measured21.7Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8S°7/28P7/2321.3741321.2813932.8456E12.114 measured3.410e+07 measured62.4Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8S°7/26P5/2321.4682321.3753932.5728E1 (intercombination)1.289 measured1.690e+07 measured86.7Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8S°7/28P5/2333.5279333.4320898.8527E12.128 measured4.120e+07 measured100Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°13/2y 8D11/2433.1187432.9969692.1716E1 (intercombination)2.011 measured8.400e+06 measured15.3Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8S°7/2y 8P9/2459.5322459.4035652.3862E18.781 measured1.610e+08 measured99.9Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8S°7/2y 8P7/2462.8522462.7226647.7067E17.815 measured1.560e+08 measured99.8Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8S°7/2y 8P5/2466.3183466.1878642.8923E16.756 measured1.520e+08 measured100Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
z 10P9/2e 10D°11/2501.4547501.3149597.8455E15.221 measured3.650e+07 measured51.1Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
z 10P9/2e 10D°9/2502.4310502.2909596.6838E15.313 measured4.510e+07 measured60.4Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°9/2y 10P11/2506.9356506.7943591.3817E12.097 measured5.700e+06 measured7.92Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°7/2y 10P9/2511.5767511.4342586.0166E13.487 measured1.840e+07 measured26.1Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°11/2y 10P11/2513.0520512.9091584.3315E13.959 measured1.960e+07 measured27.2Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°5/2y 10P7/2513.4912513.3482583.8317E14.607 measured3.970e+07 measured52.4Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°9/2y 10P9/2516.1485516.0047580.8260E14.452 measured2.920e+07 measured41.5Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°7/2y 10P7/2516.8132516.6693580.0789E13.669 measured2.470e+07 measured32.6Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°13/2y 10P11/2521.6558521.5105574.6940E15.770 measured3.960e+07 measured55Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°11/2y 10P9/2522.4906522.3452573.7758E13.667 measured1.910e+07 measured27.1Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°13/2z 8F13/2526.7855526.6389569.0978E1 (intercombination)3.693 measured1.350e+07 measured28.1Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
z 10P11/2e 10D°13/2527.3424527.1957568.4967E18.422 measured7.000e+07 measured100Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°11/2z 8F11/2527.3936527.2469568.4416E1 (intercombination)2.431 measured6.800e+06 measured16.6Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
z 10P11/2e 10D°11/2528.4303528.2833567.3264E15.205 measured3.100e+07 measured43.4Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°9/28P9/2528.8708528.7237566.8539E1 (intercombination)1.480 measured3.000e+06 measured6.27Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
z 6P3/2e 6D°3/2535.4319535.2831559.9077E13.389 measured3.790e+07 measured66.7Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°11/2z 10D13/2535.9088535.7598559.4094E14.978 measured2.330e+07 measured36.8Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8D°11/2x 8P9/2536.3066536.1575558.9945E14.755 measured2.970e+07 measured70.1Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8D°5/2x 8P5/2539.4386539.2887555.7490E13.205 measured2.210e+07 measured38Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°9/2z 10D11/2540.4269540.2767554.7327E15.401 measured3.120e+07 measured49.3Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8D°9/2x 8P7/2542.8440542.6931552.2627E13.778 measured2.260e+07 measured51.1Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°13/2z 10D13/2545.3032545.1517549.7720E16.108 measured3.330e+07 measured52.6Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°7/2z 10D9/2545.4433545.2918549.6308E14.983 measured3.100e+07 measured49.9Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°11/2z 10D11/2547.3837547.2317547.6825E13.148 measured1.020e+07 measured16.1Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°5/2z 10D7/2549.0165548.8640546.0537E13.410 measured1.780e+07 measured32.4Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°5/28P7/2549.6722549.5195545.4022E1 (intercombination)2.096 measured6.700e+06 measured12.3Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°7/2z 10D7/2552.8157552.6622542.3009E11.586 measured3.770e+06 measured6.86Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°5/2z 10D5/2554.8974554.7433540.2665E14.099 measured3.320e+07 measured57.4Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°13/2z 10D11/2557.1884557.0337538.0450E14.470 measured1.950e+07 measured30.8Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°11/2z 10D9/2557.8676557.7127537.3900E14.898 measured2.800e+07 measured45.1Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°9/2z 10D7/2558.1581558.0032537.1103E13.706 measured2.000e+07 measured36.4Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°7/2z 10D5/2558.7788558.6237536.5137E12.972 measured1.710e+07 measured29.6Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°9/28P7/2558.8359558.6808536.4588E1 (intercombination)2.420 measured8.500e+06 measured15.6Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°9/2z 8D11/2562.0365561.8805533.4039E1 (intercombination)1.653 measured2.600e+06 measured6.71Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°7/2z 8D5/2563.4069563.2506532.1064E1 (intercombination)2.510 measured1.190e+07 measured22.5Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°9/2z 8D7/2567.5385567.3810528.2328E1 (intercombination)2.403 measured8.000e+06 measured15.6Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°11/2z 8D9/2573.2423573.0833522.9769E1 (intercombination)2.261 measured5.500e+06 measured11.1Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
b 8D°11/2y 8D11/2574.0578573.8986522.2340E15.611 measured2.810e+07 measured51.1Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°13/2z 8D11/2580.1877580.0269516.7163E1 (intercombination)2.429 measured5.100e+06 measured13.2Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°13/2z 10F15/2583.2594583.0977513.9951E18.966 measured5.130e+07 measured100Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°11/2z 10F13/2596.8767596.7114502.2687E16.727 measured3.080e+07 measured67.5Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8D°11/2z 8F13/2599.4492599.2832500.1132E17.051 measured3.340e+07 measured69.5Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8D°5/2z 8F5/2601.4195601.2529498.4748E13.841 measured2.290e+07 measured52.9Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8D°7/2z 8F7/2603.0639602.8970497.1155E14.662 measured2.510e+07 measured57.5Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°13/2z 10F13/2608.5535608.3850492.6313E14.551 measured1.330e+07 measured29.1Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°9/2z 10F11/2610.1039609.9351491.3793E14.796 measured1.710e+07 measured41Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°11/2z 10F11/2618.9850618.8138484.3291E15.300 measured2.000e+07 measured48Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°7/2z 10F9/2619.6777619.5063483.7877E13.305 measured9.300e+06 measured23.7Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°9/2z 10F9/2626.3984626.2252478.5971E15.154 measured2.190e+07 measured55.9Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°7/2z 10F7/2630.1487629.9745475.7487E13.639 measured1.340e+07 measured53.7Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°7/28D7/2633.7565633.5813473.0404E1 (intercombination)2.746 measured7.500e+06 measured50Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°5/2z 10F5/2635.1759635.0003471.9833E13.485 measured1.600e+07 measured42.6Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°11/2z 10F9/2635.7639635.5881471.5469E12.442 measured4.700e+06 measured12Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°9/2z 10F7/2637.0997636.9236470.5581E12.454 measured5.900e+06 measured23.7Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°7/2z 10F5/2640.2668640.0898468.2305E13.688 measured1.750e+07 measured46.6Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°9/28D7/2640.7878640.6107467.8498E1 (intercombination)1.974 measured3.750e+06 measured25Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 10D°5/2z 10F3/2641.1798641.0026467.5638E14.169 measured3.340e+07 measured91.8Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8D°5/2z 8D7/2641.3040641.1267467.4733E14.926 measured2.330e+07 measured45.4Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)
a 8S°7/2z 10P9/2686.6448686.4554436.6048E1 (intercombination)0.963 measured5.800e+05 measured97.3NIST ASD Eu I lines table (local copy data/nist/Eu_I_lines_from1nm.tsv)
a 10D°7/2y 8P9/21147.79461147.4805261.1900E1 (intercombination)0.193 measured5.000e+03 measured0.0032Miyazawa, Inoue, Matsui, Takanashi, Kozuma, Phys. Rev. A 103, 053122 (2021)
a 10D°9/2y 8P9/21171.06711170.7467255.9994E1 (intercombination)0.367 measured1.700e+04 measured0.0108Miyazawa, Inoue, Matsui, Takanashi, Kozuma, Phys. Rev. A 103, 053122 (2021)
a 10D°11/2y 8P9/21204.23171203.9022248.9492E1 (intercombination)0.500 measured2.900e+04 measured0.0178Miyazawa, Inoue, Matsui, Takanashi, Kozuma, Phys. Rev. A 103, 053122 (2021)
a 8D°7/2y 8P9/21577.28461576.8537190.0687E10.273 measured3.860e+03 measured0.0024Miyazawa, Inoue, Nishida, Hosoya, Kozuma, Opt. Commun. 392, 171 (2017)
a 8D°9/2y 8P9/21644.47181644.0227182.3032E10.685 measured2.140e+04 measured0.0133Miyazawa, Inoue, Nishida, Hosoya, Kozuma, Opt. Commun. 392, 171 (2017)
a 8D°11/2y 8P9/21760.09861759.6180170.3271E11.574 measured9.210e+04 measured0.0572Miyazawa, Inoue, Nishida, Hosoya, Kozuma, Opt. Commun. 392, 171 (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, or a model calculation.

Eu energy levels

LevelEnergy (cm⁻¹)JParityLifetimegJHyperfine A (MHz)Hyperfine B (MHz)Lifetime sourceHyperfine source
a 8S°7/20.0007/2oddstable1.9934-8.8532-1.7852–Sandars, Woodgate, Proc. R. Soc. Lond. A 257, 269 (1960)
a 10D°5/212923.7205/2odd––––––
a 10D°7/213048.9007/2odd––––––
a 10D°9/213222.0409/2odd––––––
a 10D°11/213457.21011/2odd––––––
a 10D°13/213778.68013/2odd––––––
z 10P9/214563.5709/2even1.64 µs measured1.936––Fechner, Rinkleff, Steudel, Z. Phys. D 6, 31 (1987), linewidth as quoted by Inoue, Miyaza…–
a 8D°5/215248.7605/2odd––––––
a 8D°7/215421.2507/2odd––––––
z 10P11/215581.58011/2even––––––
a 8D°9/215680.2809/2odd––––––
a 8D°11/216079.76011/2odd––––––
z 6P3/217945.4903/2even––––––
b 8D°11/219447.19011/2odd––––––
y 8P5/221444.5805/2even6.6 ns measured2.272––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
y 8P7/221605.1707/2even6.4 ns measured1.929––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
y 8P9/221761.2609/2even6.1 ns measured1.772––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 10F3/228519.9703/2even27.5 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 10F5/228667.3905/2even26.6 ns measured2.194––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
8D7/228827.8307/2even66.7 ns measured1.811––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 10F7/228918.1707/2even40.1 ns measured1.841––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 10F9/229186.3209/2even25.5 ns measured1.7––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 10F11/229612.69011/2even24 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
8P5/229982.5005/2even24.3 ns measured2.06––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 10F13/230211.09013/2even21.9 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 8D5/230798.0605/2even18.9 ns measured2.14––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 8D7/230841.9907/2even19.5 ns measured1.824––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 8D9/230901.8409/2even20.1 ns measured1.706––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 10F15/230923.71015/2even19.5 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 10D5/230945.0705/2even17.3 ns measured2.49––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 8D11/231014.48011/2even25.8 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
6P5/231107.2805/2even51.3 ns measured1.954––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
8P7/231116.3807/2even18.3 ns measured1.928––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 10D7/231138.1107/2even18.2 ns measured2.006––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 10D9/231382.6109/2even16.1 ns measured1.86––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 10D11/231725.93011/2even15.8 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 8F5/231876.0905/2even23.1 ns measured1.719––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 8F7/232003.2407/2even22.9 ns measured1.628––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 10D13/232117.10013/2even15.8 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
8P9/232130.2509/2even20.9 ns measured1.747––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 8F9/232184.6509/2even22.7 ns measured1.615––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
y 10P7/232398.2507/2even13.2 ns measured2.195––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 8F11/232418.38011/2even24.4 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
y 10P9/232596.3109/2even14.2 ns measured1.93––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
6P7/232681.1307/2even178 ns measured1.729––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
z 8F13/232761.74013/2even20.8 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
y 10P11/232948.41011/2even13.9 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
x 8P5/233786.5505/2even17.2 ns measured2.276––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
x 8P7/234101.7807/2even22.6 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
8P9/234366.1309/2even43.7 ns measured1.803––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
e 10D°9/234466.8009/2odd13.4 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
e 10D°11/234505.55011/2odd14 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
e 10D°13/234544.59013/2odd14.3 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
8P5/234555.8205/2even33 ns measured2.27––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
8P7/234561.8707/2even28.7 ns measured1.91––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
x 8P9/234725.8109/2even23.6 ns measured1.719––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
(36382)7/236381.5107/2even25.2 ns measured1.841––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
(36411)5/236410.9605/2even48.7 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
8P5/236441.7705/2even35.9 ns measured2.224––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
(36549)9/236548.8309/2even25 ns measured1.81––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
(36601)7/236600.8307/2even43.8 ns measured1.91––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
e 6D°3/236622.0003/2odd17.6 ns measured–––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
y 8D7/236700.3907/2even15.8 ns measured1.83––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
y 8D11/236867.04011/2even18.2 ns measured1.662––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
y 8D9/236889.6209/2even14.5 ns measured1.729––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
8P9/242010.2509/2even30.7 ns measured1.771––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
8P7/242087.0207/2even30.4 ns measured1.86––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–
8P5/242130.7205/2even30.4 ns measured2.04––Den Hartog, Wickliffe, Lawler, Astrophys. J. Suppl. Ser. 141, 255 (2002)–

Eu⁺ ionisation limit 45734.74 cm⁻¹ = 5.67039 eV (218.652 nm)

Sources

Lifetimes (85 levels, Table 1) and transition probabilities (140 lines, Table 4) were parsed from the text layer of the publisher PDF of Den Hartog et al. 2002 retrieved through the Internet Archive (iopscience.iop.org itself is bot-blocked); the +- signs are lost in the text layer but value/uncertainty pairs are unambiguous, and the count of parsed rows (85, 140) matches the numbers stated in the abstract. Den Hartog level energies are those of Martin, Zalubas, Hagan (1978) and coincide with the NIST energies used as identifiers. NIST ASD already carries the Den Hartog A values (same numbers); they are repeated here with their uncertainties. rme_J_ea0 entries are derived from the measured A with the SCHEMA convention. Hyperfine constants follow E = A K/2 + B [3K(K+1)/4 - I(I+1)J(J+1)] / [2I(2I-1)J(2J-1)]; both ground-state A values are negative. Extra fields beyond SCHEMA.md: top-level ionization_limit, laser_cooling_scheme, conflicts; level fields lifetime_other, hyperfine_note, decay_to_metastable, trap_loss, magnetic_moment_muB; transition fields linewidth_MHz / linewidth_kHz, saturation_intensity_*, doppler_limit_uK, leak_to_metastable. Entries whose note says LOWER BOUND / UPPER BOUND / derived are not direct measurements of the stated quantity. The line the brief calls "1148 nm" is the y8P9/2 -> a10D7/2 leak / repumper.

Atoms with measured data

All elements: periodic table