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Table 2

Comparison between the Herschel and ALMA integrated line fluxes.

Molecule Transition Herschel Herschel Herschel Herschel ALMA Comments Comments
rms S/N Fν dν Fν dν Herschel ALMA
(K) (mK) (Jy MHz) (Jy MHz) data data

29SiO 15–14 0.065 9 7 (1408) (834) blend “U”
Si33S 36–35 0.047 8.9 5 210 271 low S/N
SiC2 26, 4, 22–25, 4, 21 0.054 5.5 10 1168 816
SiS v = 2 36–35 0.018 3.3 5 191 159 low S/N
SiC2 27, 6, 22–26, 6, 21 4.5 blend SiO v = 1 blend SiO v = 1
SiO v = 1 15–14 2.9 blend SiC2 blend SiC2
30SiS 37–36 0.055 4.9 11 1035 950
13CS 14–13 0.093 4.7 20 2012 1397 weak blend “U”
29Si34S 38–37 7 blend SiC2 blend SiC2
SiC2 31, 0, 31–30, 0, 30 5.1 blend 29Si34S blend 29Si34S
SiC2 30, 2, 29–29, 2, 28 0.061 8.4 7 1297 883
29SiS 37–36 0.075 6.2 12 1452 1059
AlF 20–19 6.4 blend C18O blend C18O
C18O 6–5 9 blend AlF blend AlF
SiC2 29, 2, 27–28, 2, 26 0.055 5.6 10 1281 735
13CO 6–5 1.235 7 176 32 525 1366 weak blend Si33S J = 37–36 blend Si33S J = 37–36

Notes. Columns 1 and 2 list the molecule and its transition; Cols. 3–5 give the Herschel antenna peak temperature, rms and S/N; the Herschel and ALMA integrated line fluxes are tabulated in Col. 6; comments on blends as seen in the Herschel and ALMA data sets are given in the last two columns. The integrated line fluxes plagued by weak line blends are given within parentheses. A “” indicates the cases of strong line blending where only detailed modelling can reveal the contribution of the individual components. The Herschel point-source sensitivity of 466 Jy/K (Roelfsema et al. 2012) has been used for all lines. For 13CO J = 6–5, the estimated source size of 10′′ (Crosas & Menten 1997) was taken into account.

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