Table 3:
Stellar contributions to the galactic spectrum in the visible range by Boisson et al. (2004), converted to the near infrared range.
| Spectral type |
5450 Å |
1.6  m |
| O |
0% |
0% |
| B3-4V |
0% |
0% |
| A1-3V |
0% |
0% |
| F2V |
31.3% |
7.5% |
| F8-9V |
0% |
0% |
| rG0IV |
0% |
0% |
| G4V |
6.3% |
2.4% |
| rG5IV |
0% |
0% |
| G9-K0V |
21.0% |
11.4% |
| rK0V |
3.3% |
1.7% |
| rK3V |
0% |
0% |
| K4V |
8.1% |
7.7% |
| rM1V |
2.5% |
7.3% |
| G0-4III |
0% |
0% |
| wG8III |
0% |
0% |
| G9III |
0% |
0% |
| rG9III |
0% |
0% |
| K2III |
0% |
0% |
| rK3III |
21.5% |
30.7% |
| rK4III |
0% |
0% |
| rK5III |
4.6% |
8.5% |
| M0.5III |
0% |
0% |
| M4III |
0% |
0% |
| M5III |
1.4% |
22.8% |
| G0I |
0% |
0% |
| K4I |
0% |
0% |
| M2I |
0% |
0% |
| rG2I |
0% |
0% |
| K0II |
0% |
0% |
| K3I |
0% |
0% |
Source LaTeX |
All tables |
In the text