Table 3
Possible emission lines measured from the summed spectrum of the CAL 83 nebula.
| λ obs | f(λ) | F(λ) | I(λ) | No. spaxels | I(λ)spaxel × 10-3 |
| (Å) | (#) | ||||
|
|
|||||
| 4400–4454∗ | 1.106 | 457.5 | 720.6 | 1213 | 594.1 |
| 4659.4∗ | 1.050 | 61.9 ± 17.4 | 95.3 ± 26.8 | 1213 | 78.6 ± 22.1 |
| 4663.9∗ | 1.048 | 14.8 ± 15.2 | 22.8 ± 23.4 | 1213 | 18.8 ± 19.3 |
| 6462.6 | 0.694 | 70.6 ± 10.6 | 93.9 ± 14.0 | 1233 | 76.2 ± 11.4 |
| 6495.3 | 0.689 | 55.5 ± 10.6 | 73.7 ± 14.1 | 1233 | 59.7 ± 11.4 |
| 6532.7 | 0.684 | 38.5 ± 10.6 | 51.0 ± 14.0 | 1233 | 41.4 ± 11.3 |
| 6634.7 | 0.670 | 61.7 ± 10.6 | 81.3 ± 13.9 | 1233 | 65.9 ± 11.3 |
| 6683.8 | 0.663 | 29.1 ± 8.2 | 38.3 ± 10.7 | 1233 | 31.0 ± 8.7 |
Notes. Absolute observed reddened (F(λ)) and dereddened fluxes (I(λ)) are given with their corresponding errors, in units of 10-16 erg cm-2 s-1. The adopted redding curve, f(λ) and the average flux per spaxel I(λ)spaxel are also given (0.67′′). Lines marked with ∗ are blends. The value of c(Hβ) is 0.18.
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