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Table D.1

Summary of the observed properties of the selected TOP100 sources.

(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12)
Source-ID Class d⊙ Lbol Mclump Td log10[Nobs(X/cm−2)]
kpc 102 L⊙ 102 M⊙ K H2CO CH3CCH (CH3CN)cold (CH3CN)hot (CH3OH)cold (CH3OH)hot
G13.18+0.06 70w 2.40 83.18 3.68 24.24 13.66 14.62 13.41 <12.89 16.02 <14.22
G14.49-0.14 70w 3.87 7.50 19.16 12.39 <12.68 14.52 13.22 <12.89 15.85 <14.22
G30.89+0.14 70w 4.90 4.96 19.18 11.44 <12.68 14.16 13.08 <12.93 15.29 <14.17
G351.57+0.77 70w 1.34 4.33 1.64 17.04 <12.68 14.15 <14.53 <12.72 <15.42 <14.20
G353.42-0.08 70w 6.06 45.08 17.91 17.12 <12.68 <15.73 12.74 <12.74 <15.42 <14.20
G354.95-0.54 70w 1.91 4.84 1.47 19.13 <12.68 <15.73 12.71 <12.70 <15.42 <14.20
G08.68-0.37 IRw 4.78 275.00 14.81 24.18 13.72 15.11 13.58 <12.85 15.22 <14.41
G08.71-0.41 IRw 4.78 5.04 16.62 11.81 <12.80 14.46 12.99 <12.84 15.19 <14.36
G10.45-0.02 IRw 8.55 113.14 16.06 20.70 <12.80 14.36 13.34 <12.91 14.96 <14.53
G14.11-0.57 IRw 2.57 31.77 3.53 22.35 13.46 14.63 13.14 <12.87 15.37 <14.40
G14.63-0.58 IRw 1.83 27.78 2.54 22.54 13.54 14.67 13.22 <12.83 15.82 <14.41
G24.63+0.17 IRw 7.72 50.36 15.28 18.12 13.20 14.08 13.21 <12.89 15.03 <14.35
G28.56-0.24 IRw 5.45 17.67 54.14 11.73 <12.80 14.58 12.96 <12.84 14.97 <14.32
G305.19-0.01 IRw 3.80 125.29 5.18 26.07 13.52 <15.30 13.33 <12.85 <14.86 <14.40
G317.87-0.15 IRw 2.95 16.41 3.62 19.26 13.76 14.82 13.51 <12.84 15.88 <14.40
G318.78-0.14 IRw 2.78 64.00 3.59 24.92 13.26 14.22 13.28 <12.92 15.26 <14.39
G326.99-0.03 IRw 3.95 11.44 4.44 17.95 13.84 14.88 13.57 <12.89 15.65 <14.39
G331.71+0.60 IRw 10.53 373.43 51.12 21.00 13.86 14.74 13.48 <12.93 16.00 <14.42
G336.96-0.23 IRw 10.91 36.25 24.22 15.77 13.36 14.71 13.21 <12.89 15.54 <14.40
G337.26-0.10 IRw 11.00 300.11 31.87 21.73 13.35 14.40 13.27 <12.93 15.34 <14.43
G342.48+0.18 IRw 12.55 641.50 49.13 23.61 13.47 14.44 13.18 <12.81 15.15 <14.39
G353.07+0.45 IRw 0.86 0.57 0.18 17.79 <12.80 14.55 <13.48 <12.70 15.11 <14.46
G34.41+0.23 IRb 1.56 48.39 2.14 26.13 14.01 15.20 14.78 14.72 16.15 15.92
G35.20-0.74 IRb 2.19 235.80 4.63 29.54 14.03 14.94 14.26 <14.14 16.33 15.19
G59.78+0.07 IRb 2.16 97.71 2.55 28.19 <12.88 14.36 13.26 <13.11 15.21 <14.59
G305.56+0.01 IRb 3.80 517.18 4.06 33.41 <13.72 <15.00 13.02 <12.96 15.37 <14.55
G310.01+0.39 IRb 3.61 496.33 4.15 32.20 13.46 14.43 13.23 <12.94 14.91 <14.53
G313.58+0.32 IRb 3.78 94.14 1.83 29.17 <12.88 <15.00 <13.30 <12.78 14.88 <14.88
G316.64-0.09 IRb 1.19 9.94 0.18 30.63 <12.88 14.67 13.60 13.57 15.20 15.12
G333.31+0.11 IRb 3.60 107.33 4.27 25.85 13.73 14.73 13.52 <13.01 15.63 <14.58
G339.62-0.12 IRb 3.01 149.96 3.20 28.66 13.65 14.69 13.51 <12.94 14.94 <14.57
G340.75-1.00 IRb 2.76 76.82 2.13 27.07 13.64 14.35 13.19 <12.97 15.75 <14.49
G341.22-0.21 IRb 3.67 162.23 4.90 27.03 13.74 14.33 13.62 <12.91 15.56 <14.59
G345.51+0.35 IRb 2.25 432.67 4.24 32.70 14.04 14.85 13.66 <12.94 16.10 16.05
G345.72+0.82 IRb 1.56 18.73 2.01 22.05 13.28 14.79 13.09 <12.89 15.21 <14.53
G351.77-0.54 IRb 1.00 164.69 2.64 31.79 14.82 15.92 15.68 15.63 16.73 16.68
G353.41-0.36 IRb 3.44 1272.01 34.83 28.26 13.98 15.03 13.59 <12.91 15.88 <14.68
G10.62-0.38 HII 4.95 4227.57 37.87 34.45 14.68 15.43 13.98 13.34 15.95 15.21
G12.81-0.20 HII 2.40 2468.69 18.80 35.15 14.19 15.36 13.64 <13.23 15.32 <14.54
G31.41+0.31 HII 4.90 689.42 30.63 26.32 14.14 15.34 15.45 15.43 16.41 16.38
G34.40+0.23 HII 1.56 29.91 2.76 22.82 13.93 14.85 13.75 <13.09 16.04 <14.54
G301.14-0.23 HII 4.40 2137.40 19.41 34.56 <13.02 15.13 14.01 13.76 15.91 15.78
G330.88-0.37 HII 4.16 1545.88 15.87 33.44 14.26 15.19 14.61 14.49 16.11 16.01
G330.95-0.18 HII 9.32 13 064.99 173.06 33.04 14.45 15.42 14.58 14.44 16.21 16.07
G332.83-0.55 HII 3.60 2419.56 19.36 35.67 14.25 15.30 14.22 14.08 16.03 15.90
G333.28-0.39 HII 3.60 1291.69 20.77 30.37 13.80 14.95 13.47 <13.28 15.76 <14.56
G333.60-0.21 HII 3.60 12 416.71 34.61 41.12 14.23 15.47 13.75 <13.53 14.80 <14.59
G351.42+0.65 HII 1.34 398.57 4.63 33.38 <13.02 15.27 14.85 <14.72 16.88 16.85

Notes. Column 1: TOP100 sources considered in this work; Cols. from (2) to (6): physical properties of each source (König et al. 2017); Cols. from (7) to (12): final beam- and LOS-average column densities, obtained by applying the procedure described in Appendix D to the values reported in Giannetti et al. (2017) and Tang et al. (2018). Upper limits are marked with ‘ <’.

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