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Table A.1

Herschel OBSID’s of the observed transitions analysed in this paper.

Source Species Frequency Band LO-settinga Date OBSID
(GHz)

W49N NHb 946.476 3b A 2010-04-13 1342194700
B 1342194701
C 1342194702
NH 974.478 4a A 2010-04-18 1342195004
B 1342195005
C 1342195006
o-NH2 952.578 3b A 2010-04-13 1342194706
B 1342194707
C 1342194708
o-NH3 572.498 1b A 2010-04-11 1342194517
B 1342194518
C 1342194519
p-NH 1215.246 5a A 2010-04-18 1342195067
B 1342195068
C 1342195069
NH+ 1012.540 4a A 2010-04-18 1342194998
B 1342194999
C 1342195000
G10.6-0.4 NHb 946.476 3b A 2010-03-18 1342192316
B 1342192317
C 1342192318
NH 974.478 4a A 2010-03-03 1342191620
B 1342191621
C 1342191622
o-NH2 952.578 3b A 2010-03-18 1342192319
B 1342192320
C 1342192321
o-NH3 572.498 1b A 2010-03-02 1342191578
B 1342191579
C 1342191580
p-NH 1215.246 5a A 2010-03-05 1342191697
B 1342191698
C 1342191699
NH+ 1012.540 4a A 2010-03-03 1342191623
B 1342191624
C 1342191625

Notes. 

(a)

Three different frequency settings of the LO were performed, with approximately 15 km s-1 between each setting in order to determine the sideband origin of the signals.

(b)

Observed in the same setting as CH2 at 946 GHz.

(c)

The ortho-NH3 20–10 transition at 1214.859 GHz is observed in the same setting as para-NH3 21–11 at 1215.246 GHz.

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