Fig. 1

Predicted (in red) and observed (in blue) rotational spectrum of 13C methylamine between 882 and 908 GHz dominated by cQ-type series of transitions with Ka = 6 ← 5. A slight inconsistency between predicted and observed spectrum, which may be visible for some strong lines, is due to source power and detector sensitivity variations. Weak unassigned lines are due to higher excited vibrational states.
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