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Table 1.
Summary of the maps used for the radiative transfer model and their properties, as well as the observed images that have used to produce each map.
| Component | Images used | Pixel scale | FWHM |
|---|---|---|---|
| [arcsec] | [arcsec] | ||
| Old stellar disc | IRAC 3.6μm | 0.75 | 1.9 |
| Young non-ionising disc | GALEX FUV, IRAC 3.6 μm, SDSS r, MIPS 24 μm, PACS 70 μm, PACS 160μm | 4.0 | 11.2 |
| Young ionising disc | MIPS 24μm, IRAC 3.6 μm, Hα | 2.03 | 6.43 |
| Dust | SDDS r, GALEX FUV, MIPS 24 μm, PACS 70 μm, PACS 160μm | 4.0 | 11.2 |
Notes. The image with the lowest resolution, thus determining the resolution of the map, is indicated in bold.
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