Table B.1
SD CO integrated intensities used to constrain RT models
| Line | Telescope | Beam size ["] |  [K km s−] |
||||
|---|---|---|---|---|---|---|---|
| 15194-5115 | 15082-4808 | 07454-7112 | AFGL 3068 | IRC +10 216 | |||
| 1-0 | IRAM | 21.4 | − | − | − | 101.414 | 411.944 |
| 1-0 | OSO | 33 | − | − | − | 26.974; 488 | 3868 |
| 1-0 | SEST | 45 | 611 | 42.410; 36.7111 | 25.5711 | − | − |
| 1-0 | NRAO | 55 | − | − | − | − | 222.7912 |
| 2-1 | IRAM | 10.7 | − | − | − | 118.994 | 830.584 |
| 2-1 | JCMT | 21 | − | − | − | 728 | 6898 |
| 2-1 | SEST | 23 | 1511 | 69.411 | 5011 | − | 491.834 |
| 2-1 | APEX | 27 | 116.322; 128.123 | 81.912 | 55.832; 56.53 | 59.692 | 608.122 |
| 3-2 | JCMT | 14 | − | − | − | 728 | 10708; 852.2412 |
| 3-2 | SEST | 15 | 129.31 | − | − | − | 854.84 |
| 3-2 | APEX | 18 | 126.961, 122.713, 144.44; 1635 | 90.342 | 57.412 | 65.822; 76.164 | 752.922 |
| 3-2 | CSO | 20 | − | − | − | 40.239 | 672.099 |
| 4-3 | JCMT | 12 | − | − | − | 938 | 12308 |
| 4-3 | APEX | 14 | 134.052; 155.94; 128.44 | 85.672 | 53.632 | 72.322; 87.584 | 711.922 |
| 4-3 | CSO | 15.5 | − | − | − | 22.49 | 639.179 |
| 5-4 | HIFI | 36.1 | 16.86 | − | 6.876 | − | − |
| 6-5 | JCMT | 8 | − | − | − | 558 | − |
| 6-5 | CSO | 10.3 | − | − | − | 22.49 | 1130.619 |
| 6-5 | HIFI | 30.4 | 20.26 | − | − | − | − |
| 7-6 | APEX | 7.7 | 82.14; 153.434 | − | − | 152.694 | − |
| 9-8 | HIFI | 20.1 | 17.66 | − | 8.126 | − | − |
| 10-9 | HIFI | 18.2 | 19.47 | − | − | − | − |
| 14-13 | HIFI | 12.9 | − | − | 7.626 | − | − |
| 16-15 | HIFI | 11.5 | 17.27 | − | − | − | − |
Notes. 1Ryde et al. (1999), 2APEX pointing catalogue,3APEX Archivea, 4De Beck et al. (2010), 5Ramstedt & Olofsson (2014), 6 Danilovich et al. (2015), 7HIFIArchiveb, 8Ramstedt et al. (2008), 9Teyssier et al. (2006), 10Nyman et al. (1992), 11Woods et al. (2003), 12De Beck et al. (2012). The integrated intensities reported are in the main-beam temperature (TMB) scale.
ahttps://archive.eso.org/wdb/wdb/eso/apex/form
bhttps://archives.esac.esa.int/hsa/whsa/
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