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Table 3
Observation-model coherency check: Eg characterisation as a function of the λ-dependent extinction and emission features.
| property↓ Eg [eV] = | 0–0.25 | 0.25–0.5 | 0.5–2.7 | |
|
|
||||
| FUV extinction | • | • | • | |
| UV bump | • | |||
| vis extinction | • | • | ||
| E(λ − V)E(B − V) | • | • | ||
| NIR extinction variations | • | • | • | |
| 3.4 μm abs. | • | |||
| IR emission bands | • | |||
| MIR emission | • | |||
| FIR emission (1.6) | • | |||
| mm emission (1.6) | • | |||
| FIR emission (1.8) | • | |||
| mm emission (1.8) | • | |||
| WMAP emission | • | |||
Notes. The bullets indicate consistency between observation and model.
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