Table 3
Fluxes and equivalent widths for the contaminated V = 12.7 hot star.
| Exp. | Sat. | S/N | He I (667.8 nm) | Proportions | ||||
|---|---|---|---|---|---|---|---|---|
| t. | Eff. | Cont. | Line | Eq.w. | Cont. | Line | Eq.w. | |
| (s) | Mag. | ×10−18 | ×10−19 | (mÅ) | ||||
| Contaminated | ||||||||
| 20 | 16.0 | 16.3 | 2.37 | −1.26 | 181.0 | 1.13 | 1.01 | 0.90 |
| 75 | 17.4 | 35.4 | 2.17 | −1.24 | 195.5 | 1.04 | 1.00 | 0.97 |
| 300 | 18.9 | 78.3 | 2.13 | −1.24 | 199.9 | 1.01 | 1.00 | 0.99 |
| Not contaminated | ||||||||
| 300 | – | 90.0 | 2.09 | −1.24 | 201.6 | 1 | 1 | 1 |
Notes. Exp.t is the exposure time in seconds; Sat.Eff.Mag. the satellite effective magnitude (for a contaminating satellite with V = 6 moving at 25° min−1); S/N is the measured signal-to-noise ratio; continuum and line are the fluxes (in erg cm−2 s−1 Å−1) measure for the wavelength range 666.047-669.453 nm); proportion lists the ratio of the quantities relative to the non-contaminated spectrum.
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