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Table A.2

Integrated intensity ) for NGC 7538S and IRS1-mmS,) for IRS1-peak, corresponding to the transitions shown in Fig. .

Species Freq. (GHz) MM1 MM2 MM3 JetN JetS IRS1−mmS IRS1−peak
C18O 219.560 120.82± 0.42 24.22± 0.47 5.80± 0.15 20.96± 0.09 27.52± 0.26 ∇∇ 1.26± 0.02
13CO 220.399 144.74± 6.38 47.60± 0.88 ≥ 8.13 36.47± 1.53 55.36± 3.84 ∇∇ 11.82± 0.18
H2CO 218.476 43.20± 1.89 51.35± 0.38 ≤ 1.04 24.68± 0.55 11.89± 0.59 225.81± 12.56 2.16± 0.00
219.908 9.24± 0.13 24.95± 0.31 ≤ 0.81 ≤ 0.54 7.87± 0.02 72.24± 1.31 0.07± 0.00
CH2CO 220.178 5.77± 0.36 22.09± 0.17 ≤ 0.97 1.78± 0.06 ≤ 0.61 117.79± 1.30 ≤ 0.03
CH3OH 218.440 76.22± 0.69 101.27± 0.89 16.25± 0.13 7.59± 0.72 12.87± 0.35 316.60± 10.35 1.84± 0.03
HCOOCH3 220.167 24.08± 0.36 ≤ 0.78 ≤ 0.65 112.05± 20.48 ≤ 0.06
217.191 17.80± 0.07 5.10± 0.51 ≤ 1.14 ≤ 0.94 ≤ 0.93 131.87± 1.37 ∇∇
DCN 217.239 65.97± 0.18 5.40± 0.65 ≤ 0.94 ≤ 0.83 5.73± 0.82 98.58± 6.93 0.92± 0.00
HNCO 218.981 43.66± 0.35 26.13± 0.06 ≤ 0.57 ≤ 0.72 ≤ 0.39 83.03± 3.19 0.62± 0.05
HC3N 218.325 163.85± 0.96 56.58± 0.75 ≤ 0.92 ≤ 0.63 10.42± 0.53 63.66± 1.58 0.46± 0.01
HC3N(v7 = 1) 218.861 54.90± 0.56 7.84± 0.27 ≤ 0.91 ≤ 0.63 ≤ 1.51 10.35± 1.24 0.18± 0.01
CH3CN 220.730 136.57± 1.93 46.87± 1.40 3.97± 0.02 ≤ 0.38 ≤ 1.28 280.88± 3.92 0.91± 0.03
220.621 10.43± 1.00 0.60± 0.03 ≤ 0.29 ≤ 0.22 ≤ 0.21 9.03± 0.66 ≤ 0.04
CH3CH2CN 218.390 21.32± 0.10 ≤ 0.54 ≤ 0.92 ≤ 0.63 ≤ 1.28 10.13± 0.79 ≤ 0.09
NH2CHO 218.460 8.30± 0.89 19.77± 0.28 ≤ 0.54 0.97± 0.41 ≤ 0.69 87.89± 2.66 0.19± 0.01
OCS 218.903 147.54± 0.97 98.99± 0.24 17.04± 0.53 3.49± 0.06 5.28± 0.60 250.85± 3.88 ≤ 0.14
O13CS 218.198 8.72± 0.66 7.48± 2.62 ≤ 0.83 ≤ 1.10 11.78± 6.42 ≤ 0.14
SO2 219.276 98.07± 0.26 ≤ 0.67 ≤ 0.58 ≤ 0.53 ≤ 0.88 30.03± 5.17 0.25± 0.01
34SO2 219.355 102.32± 0.58 ≤ 0.68 ≤ 0.39 ≤ 0.47 ≤ 1.29 12.80± 0.18 0.03± 0.00
SO 219.949 223.73± 2.95 123.71± 4.35 ≤ 1.37 22.98± 0.51 132.20± 3.98 229.06± 0.66 1.90± 0.06
33SO 217.833 26.83± 0.08 2.97± 0.83 ≤ 0.33 ≤ 0.26 ≤ 0.64 5.23± 1.94 ≤ 0.11

Notes. 1). Most species are measured from Gaussian fits, and uncertainties (written in subscript) on the measured intensities are typically ≤10%. 2). For those marked with “§”, integration has been performed down to the noise level due to their non-Gaussian profile. Uncertainties area however derived from the difference with the Gaussian fit. 3). For species which are not detected, an upper limit derived from 3σ rms is given. 4). “∇∇” indicates no meaningful area can be derived because of obvious absorption in IRS1-mmS, or obvious emission in IRS1-peak. 5). A lower limit is given to species which has partly absorption in NGC 7538 S because of the missing short space. 6). “*” indicates the tentative detected species because only one unblended line has been detected, which has not been observed in our source previously.

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