Table 1
Median values of the average ray crossing length distribution for the Milky Way models with the optical depth scaled by the factors 0.5, 1 and 2.
| 0.5τ0 | τ 0 | 2τ0 | |||||||
|
|
|||||||||
| UV | opt | NIR | UV | opt | NIR | UV | opt | NIR | |
| DIRECT | 0.45 | 0.47 | 0.51 | 0.44 | 0.47 | 0.50 | 0.42 | 0.45 | 0.49 |
| SCA IT 1 | 0.38 | 0.38 | 0.24 | 0.39 | 0.39 | 0.27 | 0.39 | 0.40 | 0.30 |
| SCA IT 2 | 0.30 | 0.29 | 0.02 | 0.34 | 0.33 | 0.03 | 0.36 | 0.36 | 0.07 |
| SCA IT 3 | 0.20 | 0.17 | 0.28 | 0.26 | 0.32 | 0.31 | |||
| SCA IT 4 | 0.04 | 0.05 | 0.18 | 0.18 | 0.27 | 0.27 | |||
| SCA IT 5 | 0.05 | 0.19 | 0.22 | ||||||
| SCA IT 6 | 0.10 | ||||||||
| SCA IT 7 | 0.03 | ||||||||
Notes. For each model the median values are given for the UV, optical and NIR wavelengths and for the direct light processing phase as well as each scattering iteration. The values are in units of the model linear size.
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