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Table C.22.
Output parameters of the dustatt_modified_starburst module.
| Parameter | Unit | Description |
|---|---|---|
| dust.luminosity | W | Luminosity absorbed by the dust |
| attenuation.[filters] | – | Attenuation in filters |
| attenuation.E_BV_lines | mag | E(B − V)l, the colour excess of the nebular lines light for both the |
| young and old population | ||
| attenuation.E_BVs | mag | E(B − V)s, the colour excess of the stellar light for both the young and old population |
| attenuation.E_BV_factor | – | Reduction factor to apply on E_BV_lines to compute E(B − V)s the stellar continuum |
| attenuation | ||
| attenuation.uv_bump_wavelength | nm | Central wavelength of the UV bump |
| attenuation.uv_bump_width | nm | Width (FWHM) of the UV bump |
| attenuation.uv_bump_amplitude | – | Amplitude of the UV bump. For the Milky Way: 3 |
| attenuation.powerlaw_slope | – | Slope delta of the power law modifying the attenuation curve |
| attenuation.filters | – | Filters for which the attenuation will be computed and added to |
| the SED information dictionary |
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