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Table 3.
ONIR filter effective wavelengths λ, zero-point fluxes F0 (Buxton et al. 2012) and derived extinction.
| Filter | λ | F0 | Aλ |
|---|---|---|---|
| (Å) | (Jy) | (mag) | |
| V | 5450 | 3636 | 3.58 |
| I | 7980 | 2416 | 2.16 (+0.15) |
| J | 12500 | 1670 | 1.00 |
| H | 16500 | 980 | 0.64 |
Notes. Extinction coefficients are calculated using the interstellar extinction laws from Cardelli et al. (1989) and O’Donnell (1994).
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