Indirect rotational spectroscopy of HCO+.


Spectroscopy of the ν1 band of the astrophysically relevant ion HCO(+) is performed with an optical parametric oscillator calibrated with an optical frequency comb. The sub-MHz accuracy of this technique was confirmed by performing a combination differences analysis with the acquired rovibrational data and comparing the results to known ground-state… (More)
DOI: 10.1021/jp400570m


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@article{Siller2013IndirectRS, title={Indirect rotational spectroscopy of HCO+.}, author={Brian M. Siller and James N. Hodges and Adam J. Perry and Benjamin J. McCall}, journal={The journal of physical chemistry. A}, year={2013}, volume={117 39}, pages={10034-40} }