Table 3
Spectral bands with low contamination from lines.
| Band | λ-range (Å) | Δλ/λ | Line flux1 |
|
|
|||
| C-15167 | 15 153–15 183 | 0.0020 | 0.6 (210; 20.5) |
| C-15215 | 15 195–15 235 | 0.0026 | – |
| C-15265 | 15 245–15 285 | 0.0026 | 1.6 (400; 19.8) |
| C-16000 | 15 980–16 020 | 0.0025 | 1.2 (320; 20.0) |
| C-166502 | 16 620–16 680 | 0.0036 | 2.3 (380; 19.9) |
| C-16784 | 16 770–16 798 | 0.0017 | 0.5 (170; 20.7) |
| C-16822 | 16 808–16 836 | 0.0017 | – |
| C-16934 | 16 918–16 950 | 0.0019 | 1.3 (390; 19.8) |
| C-16976 | 16 962–16 990 | 0.0016 | 1.0 (360; 19.9) |
| C-17152 | 17 134–17 170 | 0.0021 | 0.7 (190; 20.6) |
| C-17580 | 17 555–17 605 | 0.0028 | 2.2 (430; 19.7) |
Notes.
First entry is the lines flux in photons/m2/s/arcsec2. Numbers in brackets are the equivalent continuum flux (i.e., the line flux averaged over the band width) in photons/m2/s/arcsec2/μm and in AB-mag/arcsec2.
Region used by Maihara et al. (1993) to define the sky continuum.
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