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Table D.1

Species abundances, relative to CH3OH, at the end of the collapse phase for all the runs.

Runs Species abundance (relative to CH3OH)

/ Obs. CH3 CCH C3 H6 C3 H8 C3 O HCCCHO C2H3CHO C2H5CHO C3H7OH(a)
PILS 1.1 × 10−3 4.2 × 10−3 8.0 × 10−3 2.0 × 10−6 5.0 × 10−5 3.4 × 10−5 2.2 × 10−4 6.0 × 10−4
A1 9.5 × 10−3 2.8 × 10−3 1.5 × 10−3 1.4 × 10−5 5.8 × 10−4 2.7 × 10−4 4.0 × 10−4 1.5 × 10−3
B1 9.5 × 10−3 2.8 × 10−3 1.5 × 10−3 1.5 × 10−5 5.8 × 10−4 2.7 × 10−4 4.0 × 10−4 1.6 × 10−3
C1 1.0 × 10−2 7.6 × 10−3 1.1 × 10−2 2.1 × 10−7 3.4 × 10−4 3.1 × 10−4 7.6 × 10−4 2.3 × 10−3
D1 9.7 × 10−3 2.9 × 10−3 1.6 × 10−3 1.5 × 10−5 5.9 × 10−4 1.6 × 10−4 2.3 × 10−4 1.6 × 10−3
E1 9.3 × 10−3 3.0 × 10−3 1.6 × 10−3 2.2 × 10−5 5.4 × 10−4 2.6 × 10−4 4.0 × 10−4 1.5 × 10−3
A2 1.2 × 10−2 9.0 × 10−3 1.4 × 10−2 1.8 × 10−5 8.8 × 10−4 1.8 × 10−3 3.6 × 10−3 1.5 × 10−2
B2 1.2 × 10−2 9.0 × 10−3 1.4 × 10−2 1.9 × 10−5 8.8 × 10−4 1.8 × 10−3 3.6 × 10−3 1.5 × 10−2
C2 1.0 × 10−2 8.7 × 10−3 1.5 × 10−2 2.1 × 10−7 3.5 × 10−4 3.1 × 10−4 1.1 × 10−3 1.6 × 10−2
D2 1.2 × 10−2 9.3 × 10−3 1.4 × 10−2 1.8 × 10−5 8.9 × 10−4 1.6 × 10−3 2.9 × 10−3 1.5 × 10−2
E2 1.2 × 10−2 8.7 × 10−3 1.4 × 10−2 2.7 × 10−5 7.8 × 10−4 1.6 × 10−3 3.3 × 10−3 1.4 × 10−2

C2 H5 OH C2 H5 OCH3 CH3 COCH3 CH3 OCHO CH3OCH2OH HC(O)CHO CH2(OH)CHO (CH2OH)2

PILS 2.3 × 10−2 1.8 × 10−3 1.7 × 10−3 2.6 × 10−2 1.4 × 10−2 5.0 × 105 6.8 × 10−3 2.0 × 10−3
A1 1.6 × 10−2 1.6 × 10−3 1.4 × 10−4 5.8 × 10−2 3.9 × 10−4 9.5 × 10−3 2.1 × 10−2 1.8 × 10−4
B1 1.6 × 10−2 1.6 × 10−3 1.5 × 10−4 4.6 × 10−2 1.2 × 10−3 7.0 × 10−3 1.7 × 10−2 7.7 × 10−4
C1 3.1 × 10−2 3.2 × 10−3 1.8 × 10−4 2.1 × 10−2 2.0 × 10−3 2.1 × 10−3 1.7 × 10−2 2.1 × 10−3
D1 1.6 × 10−2 1.6 × 10−3 1.5 × 10−4 5.9 × 10−2 3.9 × 10−4 9.7 × 10−3 4.3 × 10−2 1.8 × 10−4
E1 1.3 × 10−2 1.9 × 10−3 1.9 × 10−4 4.8 × 10−2 1.2 × 10−3 6.8 × 10−3 1.3 × 10−2 6.4 × 10−4
A2 1.7 × 10−2 1.6 × 10−3 4.5 × 10−4 5.7 × 10−2 3.5 × 10−4 9.2 × 10−3 2.1 × 10−2 1.6 × 10−4
B2 1.7 × 10−2 1.6 × 10−3 4.6 × 10−4 4.4 × 10−2 1.2 × 10−3 6.7 × 10−3 1.7 × 10−2 7.8 × 10−4
C2 3.2 × 10−2 3.3 × 10−3 2.1 × 10−4 2.0 × 10−2 1.9 × 10−3 2.0 × 10−3 1.7 × 10−2 2.0 × 10−3
D2 1.7 × 10−2 1.7 × 10−3 4.6 × 10−4 5.9 × 10−2 3.3 × 10−4 9.4 × 10−3 4.3 × 10−2 1.5 × 10−4
E2 1.5 × 10−2 1.9 × 10−3 4.6 × 10−4 4.7 × 10−2 1.2 × 10−3 6.6 × 10−3 1.3 × 10−2 6.4 × 10−4

Notes. (a) C3H7OH abundance for the PILS observations is the sum of the abundance of all the isomers.

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