Table 2
Observed (J′ ← J′′ = 0 ← 1 at the PhLAM laboratory) and calculated (J′ ← J′′ = 2 ← 1 and 1 ← 1) frequencies (in MHz) of the N = 1 ← 0 ground-state rotational transition of 15NH (), given together with the base-10 logarithm of the Einstein coefficient for spontaneous emission (in s-1).
J′ ← J′′ | F1′,F′ ← F1′′,F′′ | νobsa | νobs − νcalc | LogA21e |
|
||||
0 ← 1 | ||||
1/2,1 ← 1/2,0 | 942036.954(100) | 0.002 | −2.204 | |
1/2,1 ← 1/2,1 | 942070.537(100)b | −0.002 | −2.204 | |
1/2,0 ← 1/2,1 | 942070.537(100)b | −0.002 | −1.726 | |
1/2,1 ← 3/2,1 | 942143.471(100)c | −0.002 | −2.203 | |
1/2,0 ← 3/2,1 | 942143.471(100)c | −0.002 | −1.726 | |
1/2,1 ← 3/2,2 | 942176.923(100) | 0.002 | −2.203 | |
2 ← 1 | ||||
3/2,2 ← 1/2,1 | 970147.73(50)d | −2.387 | ||
5/2,3 ← 3/2,2 | 970152.62(50)d | −2.533 | ||
3/2,1 ← 1/2,0 | 970159.93(50)d | −2.165 | ||
5/2,2 ← 3/2,1 | 970164.82(50)d | −2.387 | ||
3/2,1 ← 1/2,1 | 970193.48(50)d | −2.165 | ||
5/2,2 ← 3/2,2 | 970198.36(50)d | −2.387 | ||
3/2,2 ← 3/2,2 | 970254.16(50)d | −2.387 | ||
3/2,1 ← 3/2,1 | 970266.36(50)d | −2.165 | ||
1 ← 1 | ||||
3/2,1 ← 1/2,0 | 995534.36(90)d | −2.132 | ||
1/2,1 ← 1/2,0 | 995565.57(90)d | −2.132 | ||
1/2,0 ← 1/2,1 | 995571.81(90)d | −1.654 | ||
3/2,2 ← 1/2,1 | 995595.05(90)d | −2.353 | ||
1/2,1 ← 1/2,1 | 995599.11(90)d | −2.132 | ||
3/2,1 ← 3/2,1 | 995640.79(90)d | −2.131 | ||
1/2,0 ← 3/2,1 | 995644.70(90)d | −1.654 | ||
3/2,2 ← 3/2,1 | 995667.94(90)d | −2.353 | ||
1/2,1 ← 3/2,1 | 995671.99(90)d | −2.131 | ||
3/2,1 ← 3/2,2 | 995674.33(90)d | −2.131 | ||
3/2,2 ← 3/2,2 | 995701.48(90)d | −2.353 | ||
1/2,1 ← 3/2,2 | 995705.54(90)d | −2.131 |
Notes.
These values are predicted frequencies since the corresponding transitions were outside the range of the millimetre-wave sources.
References. (1) Scarl & Dalby (1974).
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