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Table D.2

C34S lines used in this work.

Transition Rest frequency [GHz] Eup [K] Telescope Integrated intensity [Jy km s−1 for ALMA; K km s−1 for others]
15194-5115 15082-4808 07454-7112 AFGL 3068 IRC +10 216
2-1 96.4129495 6.94 ALMA 14.1 6.0 3.7
4-3 192.8184566 23.13 APEX 2.1 1.4 0.8 0.2 14.2
5-4 241.0160892 34.70 APEX 1.9 1.2 0.9 0.5 17.2
6-5 289.2090684 48.58 APEX 2.7
7-6 337.396459 64.77 APEX 2.5
10-9 481.9158105 127.22 HIFI 0.3
11-10 530.0715537 152.66 HIFI 0.1
12-11 578.217069 180.41 HIFI 0.2
14-13 674.4736177 242.84 HIFI 0.1
15-14 722.5828172 277.52 HIFI 0.2
16-15 770.6780547 314.51 HIFI 0.2

Notes. The ALMA and APEX lines reported are from UK24, unless otherwise specified. All HIFI lines listed are from our Herschel/HIFI spectral survey of IRAS 15194-5115 (see Sect. 3.3.3). For the ALMA lines, the integrated intensity values reported are in units of Jy km s−1. For all other SD observations (APEX, HIFI), the integrated intensities are given in units of K km s−1 , in the main beam (TMB) temperature scale. The relevant beam size ranges and main beam efficiencies for the different telescopes are described in Sect. 3.3, and the individual beam sizes at each transition frequency are indicated in Figs. D.7D.11, alongside the corresponding line spectra.

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