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Table E.2
Intrinsic spectral luminosity densities of the old and young stellar populations, as defined in Sect. 2.3, for old = 1 and SFR = 1 M⊙ yr-1, respectively, and tabulated at the sampling wavelengths of the radiation fields.
| old = 1 | SFR = 1 M⊙ yr-1 | |
|
|
||
| λ |
|
|
| Å | W/Hz | W/Hz |
|
|
||
| 912. | ... | 0.344 × 1021 |
| 1350. | ... | 0.905 × 1021 |
| 1500. | ... | 0.844 × 1021 |
| 1650. | ... | 0.863 × 1021 |
| 2000. | ... | 0.908 × 1021 |
| 2200. | ... | 0.926 × 1021 |
| 2500. | ... | 0.843 × 1021 |
| 2800. | ... | 0.910 × 1021 |
| 3650. | ... | 1.842 × 1021 |
| 4430. | 4.771 × 1021 | 2.271 × 1021 |
| 5640. | 9.382 × 1021 | 3.837 × 1021 |
| 8090. | 19.54 × 1021 | 5.734 × 1021 |
| 12 590. | 72.20 × 1021 | 0.931 × 1021 |
| 22 000. | 64.97 × 1021 | 0.728 × 1021 |
| 50 000. | 12.58 × 1021 | 0.141 × 1021 |
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