Table 6
Theoretical residual flux for the Lyman series (Lyβ to Ly6) of a galaxy with a clumpy dust geometry.
| H I lines | EB-V | |||
|---|---|---|---|---|
| 0.0 | 0.1 | 0.2 | 0.3 | |
| Lyβ | 0.100 | 0.245 | 0.489 | 0.737 |
| Lyγ | 0.100 | 0.254 | 0.512 | 0.764 |
| Lyδ | 0.100 | 0.259 | 0.523 | 0.775 |
| Ly5 | 0.100 | 0.261 | 0.530 | 0.782 |
| Ly6 | 0.100 | 0.262 | 0.533 | 0.785 |
Notes. Theoretical measurements of the residual flux of a saturated absorption line for five Lyman series lines. These values are calculated assuming fesc = 0.10, a clumpy dust geometry, saturated Lyman lines, and the Reddy et al. (2016a) dust attenuation law. The differences found between various Lyman lines for a given EB-V are small and accurate residual flux measurements are required to distinguish the geometries.
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