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Table A.6

Continuation of Table A.5 with additional species.

Source C18O OCS(1) H2CO(1) CH3OH(1) H2CO(2) CH3OH(2) OCS(2) C33S H2,29 H2,beam x(e)

IRDC011.1 4.4(15) 1.6(14) 5.5(13) 9.1(13) 8.5(12) 2.7(13) 5.2(14) 4.3(12) 3.7(22) 5.3(22) 8.9(–09)
IRDC028.1 4.6(15) 1.9(14) 1.0(14) 2.0(14) 1.4(13) 4.8(13) 5.0(14) 4.1(12) 3.2(22) 4.3(22) 1.0(–08)
IRDC028.2 9.3(15) 1.7(15) 5.8(14) 1.3(15) 5.6(14) 2.8(15) 3.9(12) 1.1(23) 1.6(23) 4.1(–09)
IRDC048.6 1.2(15) 1.4(14) 1.6(13) 1.7(13) 9.5(11) 2.9(13) 1.2(15) 9.6(12) 8.6(21) 1.3(22) 1.4(–08)
IRDC079.1 7.7(15) 4.4(14) 5.0(13) 5.3(13) 9.3(12) 2.2(13) 8.9(14) 7.3(12) 4.3(22) 5.5(22) 7.1(–09)
IRDC079.3 2.6(15) 4.0(14) 4.5(13) 4.7(13) 3.2(12) 2.2(13) 8.9(14) 7.3(12) 2.7(22) 3.1(22) 1.1(–08)
IRDC18151 7.3(15) 1.6(14) 2.7(14) 4.0(14) 3.0(13) 2.9(14) 5.1(14) 4.2(12) 5.1(22) 1.4(23) 9.0(–09)
IRDC18182 3.3(15) 1.6(14) 1.8(13) 1.9(13) 3.8(12) 1.2(13) 5.0(14) 4.1(12) 1.3(22) 3.4(22) 1.1(–08)
IRDC18223 5.4(15) 1.6(14) 6.2(13) 9.0(13) 8.7(12) 8.2(13) 5.1(14) 4.2(12) 2.0(22) 6.7(22) 2.2(–08)
IRDC18306 3.5(15) 1.5(14) 1.7(13) 1.8(13) 1.0(12) 1.2(13) 5.0(14) 4.1(12) 1.7(22) 3.6(22) 6.8(–09)
IRDC18308 3.8(15) 1.5(14) 4.7(13) 1.1(14) 7.8(12) 2.9(13) 3.7(14) 3.0(12) 2.4(22) 5.1(22) 6.3(–09)
IRDC18310 2.4(15) 1.6(14) 4.2(13) 7.3(13) 7.4(12) 1.3(13) 5.2(14) 4.2(12) 1.6(22) 3.1(22) 1.2(–08)
IRDC18337 2.2(15) 1.2(14) 1.3(14) 2.2(14) 1.5(13) 8.1(13) 3.7(14) 3.0(12) 7.8(21) 2.9(22) 1.9(–08)
IRDC18385 1.8(15) 3.5(14) 4.0(13) 4.1(13) 6.6(12) 1.2(13) 5.1(14) 4.2(12) 7.7(21) 1.8(22) 1.7(–08)
IRDC18437 3.8(15) 3.4(14) 3.8(13) 4.0(13) 1.2(12) 1.3(13) 5.5(14) 4.5(12) 1.0(22) 2.1(22) 7.6(–09)
IRDC18454.1 3.7(15) 3.7(14) 4.2(13) 4.3(13) 1.3(12) 1.3(13) 5.4(14) 4.4(12) 1.4(22) 4.1(22) 8.6(–09)
IRDC18454.3 8.7(15) 3.4(14) 3.9(13) 1.1(14) 1.2(13) 1.3(13) 5.4(14) 4.4(12) 2.0(22) 4.8(22) 2.1(–08)
IRDC19175 2.4(15) 2.6(14) 2.9(13) 3.0(13) 2.9(12) 3.1(13) 1.2(15) 1.0(13) 9.1(21) 2.0(22) 8.6(–09)
IRDC20081 5.9(15) 3.9(14) 4.5(13) 4.7(13) 6.3(12) 2.4(13) 9.8(14) 8.0(12) 2.0(22) 5.7(22) 8.2(–09)
HMPO18089 2.3(16) 1.5(15) 3.7(14) 9.9(14) 1.6(14) 1.2(15) 3.6(13) 8.2(22) 3.6(23) 1.2(–08)
HMPO18102 5.0(15) 2.8(14) 1.4(14) 3.9(14) 3.2(13) 1.0(14) 1.3(14) 3.7(12) 4.2(22) 9.5(22) 1.6(–08)
HMPO18151 1.2(16) 5.4(13) 8.2(13) 1.2(14) 2.5(13) 6.4(13) 1.3(14) 8.9(12) 4.3(22) 1.5(23) 1.7(–08)
HMPO18182 2.4(16) 4.8(14) 2.0(14) 6.7(14) 3.5(13) 2.2(14) 8.4(14) 2.2(13) 5.5(22) 2.2(23) 1.5(–08)
HMPO18247 1.1(16) 5.3(13) 2.8(13) 7.2(13) 9.0(12) 1.9(13) 2.5(14) 3.9(12) 2.8(22) 9.1(22) 1.1(–08)
HMPO18264 1.3(16) 4.5(14) 5.3(14) 1.0(15) 9.6(13) 2.6(14) 5.5(14) 1.3(13) 9.4(22) 3.2(23) 1.2(–08)
HMPO18310 1.2(16) 5.2(13) 2.1(13) 4.1(13) 9.8(12) 9.8(12) 1.3(14) 3.5(12) 2.9(22) 5.5(22) 1.5(–08)
HMPO18488 1.5(16) 7.3(13) 1.5(14) 4.8(14) 3.9(13) 1.3(14) 5.4(14) 1.1(13) 3.2(22) 8.4(22) 1.7(–08)
HMPO18517 1.6(16) 3.7(14) 2.0(14) 4.6(14) 4.4(13) 1.9(14) 5.5(14) 1.1(13) 7.0(22) 1.7(23) 1.5(–08)
HMPO18566 1.0(16) 4.6(14) 1.3(14) 4.4(14) 2.9(13) 1.9(14) 1.5(15) 2.9(13) 2.5(22) 9.4(22) 2.7(–08)
HMPO19217 1.4(16) 5.8(13) 2.3(14) 7.1(14) 4.1(13) 2.7(14) 7.5(14) 8.4(12) 4.2(22) 1.2(23) 1.7(–08)
HMPO19410 8.3(15) 1.7(14) 1.3(14) 2.4(14) 3.0(13) 7.7(13) 1.7(14) 8.9(12) 6.8(22) 1.4(23) 1.0(–08)
HMPO20126 8.8(15) 1.4(14) 2.9(14) 3.6(14) 4.8(13) 1.9(14) 1.6(14) 4.3(12) 5.7(22) 2.0(23) 1.5(–08)
HMPO20216 5.7(15) 1.8(14) 3.5(13) 5.6(13) 8.3(12) 1.8(13) 2.3(14) 6.4(12) 1.3(22) 4.6(22) 2.0(–08)
HMPO20293 7.1(15) 1.4(14) 1.5(14) 3.0(14) 3.5(13) 6.5(13) 2.4(14) 6.6(12) 4.3(22) 8.3(22) 1.4(–08)
HMPO22134 7.8(15) 4.7(13) 4.0(13) 1.5(13) 1.0(13) 1.6(13) 2.1(14) 5.8(12) 2.4(22) 5.1(22) 9.3(–09)
HMPO23033 8.1(15) 4.5(13) 1.1(14) 1.5(14) 3.2(13) 5.5(13) 2.2(14) 6.2(12) 4.0(22) 1.1(23) 1.7(–08)
HMPO23139 9.4(15) 1.8(14) 2.1(14) 3.4(14) 4.6(13) 8.6(13) 2.2(14) 6.2(12) 3.0(22) 8.8(22) 1.1(–08)
HMPO23151 9.7(15) 4.6(13) 6.0(13) 7.4(13) 1.4(13) 1.1(13) 1.4(14) 3.8(12) 2.3(22) 7.2(22) 4.2(–09)
HMPO23545 6.3(15) 4.9(13) 1.8(13) 1.6(13) 5.9(12) 1.7(13) 2.2(14) 6.2(12) 1.5(22) 3.1(22) 1.0(–08)
HMC009.62 5.2(16) 9.9(14) 3.7(14) 1.7(15) 9.9(13) 2.1(14) 3.5(14) 2.2(13) 9.5(22) 1.5(23) 2.4(–08)
HMC010.47 5.7(16) 4.7(15) 1.0(15) 4.7(15) 1.2(15) 6.1(15) 2.0(14) 2.3(23) 4.3(23) 1.2(–08)
HMC029.96 5.0(16) 1.7(15) 5.5(14) 1.3(15) 1.3(14) 3.1(14) 2.1(15) 1.0(14) 9.4(22) 1.6(23) 1.7(–08)
HMC031.41 4.3(16) 3.4(15) 7.5(14) 3.7(15) 8.7(14) 4.2(15) 2.1(14) 1.6(23) 2.8(23) 4.8(–09)
HMC034.26 8.0(16) 5.5(15) 1.6(15) 5.4(15) 2.5(14) 1.5(15) 7.1(15) 3.1(14) 4.1(23) 6.7(23) 9.0(–09)
HMC045.47 2.0(16) 2.0(14) 1.7(14) 5.8(14) 5.5(13) 1.2(14) 2.6(14) 1.3(13) 4.5(22) 6.5(22) 3.6(–08)
HMC075.78 2.9(16) 4.2(14) 2.9(14) 6.7(14) 8.1(13) 2.1(14) 7.5(14) 3.7(13) 6.3(22) 8.7(22) 1.8(–08)
W3H2O 3.2(16) 1.6(15) 5.6(14) 1.6(15) 1.2(14) 8.7(14) 3.7(15) 1.9(14) 7.4(22) 1.1(23) 1.4(–08)
W3IRS5 2.9(16) 6.7(13) 1.5(14) 6.8(13) 4.1(13) 3.4(13) 2.6(14) 1.1(13) 6.0(22) 7.6(22) 7.1(–09)
NGC 7538B 2.1(16) 2.4(14) 2.9(14) 4.1(14) 8.1(13) 1.8(14) 4.1(14) 3.4(13) 1.2(23) 1.7(23) 6.4(–09)
Orion-KL 8.1(16) 3.7(16) 8.2(15) 1.8(16) 1.6(15) 7.3(15) 5.8(16) 6.7(14) 1.3(24) 1.7(24) 6.4(–10)
UCH005.89 5.5(16) 2.1(15) 1.3(15) 2.0(15) 2.7(14) 5.3(14) 2.4(15) 1.2(14) 2.2(23) 3.6(23) 1.8(–08)
UCH010.10 1.1(14) 2.8(13) 6.9(12) 1.4(13) 5.8(11) 1.1(13) 8.3(13) 3.9(12) 6.4(21) 1.3(22) 2.3(–08)
UCH010.30 3.3(16) 3.1(14) 2.3(14) 7.8(14) 8.8(13) 1.5(14) 1.5(14) 2.7(13) 8.1(22) 1.1(23) 2.0(–08)
UCH012.21 3.1(16) 7.2(14) 3.4(14) 1.3(15) 7.6(13) 7.3(14) 2.0(15) 8.4(13) 9.6(22) 1.6(23) 1.2(–08)
UCH013.87 2.9(16) 3.8(13) 7.8(13) 1.6(14) 2.5(13) 3.9(13) 7.3(13) 1.7(13) 5.3(22) 7.6(22) 1.7(–08)
UCH030.54 1.7(16) 3.6(13) 3.7(13) 1.8(13) 1.3(13) 8.0(12) 6.3(13) 3.0(12) 2.1(22) 3.1(22) 1.1(–08)
UCH035.20 2.7(16) 3.6(13) 1.4(14) 9.2(13) 4.1(13) 5.0(12) 3.9(13) 1.8(13) 1.1(23) 1.4(23) 5.7(–09)
UCH045.12 1.4(16) 3.4(13) 7.4(13) 1.7(13) 2.3(13) 2.8(12) 2.2(13) 8.1(12) 7.4(22) 1.1(23) 9.6(–09)
UCH045.45 1.5(16) 3.4(13) 9.9(13) 1.1(14) 2.6(13) 2.8(12) 2.2(13) 1.7(13) 4.2(22) 5.6(22) 7.9(–09)

Notes. Iteration 1 column densities in a(x) = a × 10x cm-2 derived with the mean temperatures from the best-fit models of iteration 0 (see Sect. 4.3 and Tables 36). Non-detections are indicated by and the upper limit derived with the 3σ rms value. A blank entry means that the molecule is detected, but rejected from the analysis due to reasons discussed in Sect. 3.2. The last column gives the lower limit for the ionization degree x(e).

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