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Submillimeter and Far-infrared Spectroscopy of Monodeuterated Amidogen Radical (NHD): Improved Rest Frequencies for Astrophysical Observations

  • Authors: Luca Bizzocchi, Mattia Melosso, Barbara Michela Giuliano, Luca Dore, Filippo Tamassia, Marie-Aline Martin-Drumel, Olivier Pirali, Laurent Margulès, and Paola Caselli

2020 The Astrophysical Journal Supplement Series 247 59.

  • Provider: AAS Journals

Caption: Figure 2.

Recording (black trace) of the ﹩{N}_{{K}_{a},{K}_{c}}={4}_{\mathrm{1,3}}\leftarrow {4}_{\mathrm{0,4}},J=9/2\leftarrow 9/2﹩ fine-structure transitions showing six resolvable components. Integration time: 390 s; RC = 3 ms; scanning rate: 1.3 MHz s−1; modulation depth: 850 kHz. The blue trace plots the modeled spectrum computed with proFFiT using a modulated Voigt profile (see the text). The red sticks indicate the position and relative intensity of the 18 hyperfine components. Note that the F2 and F quantum numbers are not shown in the plot.

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