Table 2:

Species and number of detected lines in the 555-636 GHz.
Species $E_{\rm up}$ (K) (1) (2) (3) (4) (5)
H2O 27-680 1 2 1 1 2
HDO 97 0 1 0 0 1
D2O 29 0 1 0 0 0
CO 83 1 1 1 1 1
C17O 83 0 1 1 1 1
HCO+ 119 1 1 1 1 1
H13CO+ 119 0 1 0 0 1
HCN 119 1 1 1 1 1
H13CN 119 0 1 1 0 1
DCN 119 0 1 0 0 1
HNC 119 0 1 1 0 1
CN 82 0 0 2 2 2
N2H+ 95 0 1 1 0 1
NH3 28 1 1 1 1 1
HCl 27 0 1 1 1 1
H37Cl 27 0 1 1 0 1
CCH 117 0 0 2 0 2
H2CO 120-530 4 8 8 0 8
CH3OH 39-1050 17 35 47 3 345
13CH3OH 39-240 0 0 0 0 41
CH3OCH3 115-290 0 0 1 0 30
H2S 160-415 0 2 0 0 4
CS 186 1 1 1 1 1
C34S 175-200 0 2 0 0 2
SO 190-225 0 6 0 2 6
SO2 80-210 0 10 0 0 15
othersc   0 0 0 0 62
Total   27 86 71 16 558

Notes. Second column gives the upper level energy range of the detected transitions. Columns (1) to (5) refer to L1157-B1, IRAS 16293, OMC2-FIR4, AFGL 2591 and NGC 6334I respectively. In L1157-B1 the number refers to the list of lines reported in Codella et al. (2010).


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