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Table A.2.
Summary of the images used to produce the component maps in our radiative transfer model of M 51, as well as the simulation output images used to derive the local physical parameters.
| Component map | Observed images used |
|---|---|
| Old stellar disc | IRAC 3.6 μm |
| Young non-ionising disc | GALEX FUV, IRAC 3.6 μm, SDSS r, MIPS 24 μm, PACS 70 μm, PACS 160 μm |
| Young ionising disc | MIPS 24 μm, IRAC 3.6 μm, Hα |
| Dust disc | GALEX FUV, SDDS r, MIPS 24 μm, PACS 70 μm, PACS 160 μm |
| Physical map | Model images used |
| SFR | GALEX FUV, MIPS 24 μm, PACS 70 μm, PACS 160 μm |
| Mstar | IRAC 3.6 μm |
Notes. Indicated in bold are the image with the lowest resolution, determining the resolution of each map.
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