Table 2.
Covered emission lines in each frequency setup with their rest frequency.
Covered emission lines | Rest frequency (GHz) (1) | Setup ID (2) |
---|---|---|
CO(7 − 6) | 806.652 | A |
[CI]369 μm | 809.342 | |
CO(10 − 9) | 1151.985 | B |
H2O 312 − 221 | 1153.127 | |
H2O 321 − 312 | 1162.912 | |
[NII]205 μm | 1461.131 | C |
H2O 303 − 212 | 1716.770 | D |
CO(15 − 14) | 1726.603 | |
OH 2Π1/2,![]() |
1834.744 | |
OH 2Π1/2,![]() |
1837.800 | |
CO(16 − 15) | 1841.346 |
Notes. (1)Rest frequency of the lines are taken from the “Splatalogue database for astronomical spectroscopy” available at https://www.cv.nrao.edu/php/splat, see references therein. (2)Setup IDs are listed in Table 1. ( ⋆ )The Λ-doubling transitions of the hydroxyl molecule listed here are two triplets produced by the hyperfine structure splitting of the upper and lower level that is not spectrally resolved in the observations. We report the average rest frequency of the triplets. The six transitions are OH 2Π1/2,,1 − 1; OH 2Π1/2,
,2 − 1; OH 2Π1/2,
,1 − 0 and OH 2Π1/2,
,1 − 1; OH 2Π1/2,
,2 − 1; and OH 2Π1/2,
,1 − 0.
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