Table D.1
Averaged photoabsorption cross sections and absorption rates (over the [10–11] eV range) of relevant species in this work.
| Species |  [Mbarn] |
 [10−3 s−1 ] |
Species |  [Mbarn] |
 [10−3s−1] |
|---|---|---|---|---|---|
| Pyr+ | 83 ± 28 | 1.17 | Cor+ | 72 ± 41 | 1.02 |
| [Pyr-H]+ | 82 ± 15 | 1.16 | Cor+* | 103 ± 38 | 1.46 |
| [Pyr-2H]+ | 76 ± 26 | 1.08 | [Cor-H]+ | 92 ± 37 | 1.31 |
| [Cor-2H]+ | 93 ± 36 | 1.32 | |||
| 1-MePyr+ | 88 ± 6 | 1.25 | |||
| 1-CH2Pyr+ | 90 ± 11 | 1.27 | MeCor+ | 88 ± 16 | 1.25 |
(1) C15H |
94 ± 24 | 1.33 | C25H |
97 ± 24 | 1.37 |
C23H |
84 ± 40 | 1.19 | |||
| 4-EtPyr+ | 91 ± 9 | 1.29 | |||
| 4-CH2Pyr+ | 81 ± 17 | 1.14 | EtCor+ | 103 ± 17 | 1.46 |
(2) C15H |
89 ± 23 | 1.27 | C25H |
97 ± 24 | 1.37 |
C23H |
84 ± 40 | 1.19 | |||
| H6-Pyr+ | 109 ± 36 | 1.54 |
Notes. The error (standard deviation) on 
quantifies the variability of the cross sections over the considered energy range. No error bar is provided for
since most of the uncertainty would come from the experimental error on the VUV photon flux, which is globally included in the
γ
correction factor as explained in Sect. 4.1.
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