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Table B.1.

SPIRE bolometers used for the background subtraction of the spectra of the background contaminated sources.

Name SSW SLW
OH 127.8 +0.0 B2, B3, B4 B2, B3
C2, C5 C2, C4
D2, D6 D2, D3
E2, E5
F2, F3
TX Cam B2, B3, B4 B2, B3
C2, C5 C2, C4
D2, D6 D2, D3
E2, E5
F2, F3
II Lup B2, B3, B4 B2, B3
C2, C5 C2, C4
D2, D6 D3
E2, E5
F2, F3
AFGL 5379 B2, B3, B4 B2, B3
C2, C5 C2, C4
D2, D6 D2, D3
E2, E5
F2, F3
OH21.5 +0.5 B2, B3, B4 B2, B3
C2, C5 C2, C4
D2, D6 D2
E2, E5
F2, F3
OH26.6 +0.6 B2, B3, B4 B2, B3
C2, C5 C2, C4
D2, D6 D2, D3
E2, E5
F2, F3
OH30.1 −0.7 B2, B3, B4 B2, B3
C2, C5 C2
D2, D6 D3
E2, E5
F5
IRAS 18488−0107 B2, B3, B4 B2, B3
C2, C5 C2, C4
D2, D6 D2, D3
E2
F2
OH32.8 −0.3 B3, B4 B2, B3
C5 C2
D2, D6 D2
E2, E5
F2, F3
IRAS 19067+0811 B2, B3, B4 B2, B3
C2, C5 C2, C4
D2, D6 D2, D3
E2, E5
F2, F3

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