Table 4
Summary of the method used in this work and Paradis et al. (2011a), and the different tests we performed to allow the comparison of these two studies.
| This work | Paradis et al. (2011a) | Test | Results of the tests | |
|---|---|---|---|---|
| Resolution | 1′ | 4′ | 4′, with HI/CO/Hα; |  and  |
| Model: DBP90 | ||||
| Hα phase | Yes | No | 4′, HI/CO (Hα removed) |  and  |
| Model: DBP90 | ||||
| Dark gas phase | No (yes) | Yes | 4′, HI/CO+Dark gas |  and  |
| Model: DBP90 | ||||
| Wavelength range | 3.6–500 μm | 3.6–160 μm | – | – |
| Modeling | AJ13, MC11 | DBP90 | ||
| DL07, DBP90 | ||||
| Comparison of the results |  |
 |
||
 |
 |
|||
Notes.This table does not show all the results of this present analysis, but only results that can be directly comparable with Paradis et al. (2011a). Columns 2 and 3 describe the angular resolution, the presence or not of the ionized and dark gas phases (in addition to the atomic and molecular phases), the wavelength range, the model(s) used, and the results of these two studies in terms of dust temperature and PAH relative abundance in the atomic and molecular phases. Column 4 describes the different tests we applied, indicating the angular resolution, the gas phases we considered in the analysis, and the model we used. Column 5 summarizes the results of the tests.
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