Table 5.
Mean values and their corresponding errors, in minutes, for the elapsed time between observations corresponding to contiguous filters.
| Contiguous filters | tcont (min) | Δ Mag. | Rerr (%) (a) |
|---|---|---|---|
| J0378 − u | 20.7 ± 2.4 | 0.08 | 7 |
| J0395 − J0378 | 12.3 ± 2.1 | 0.05 | 5 |
| J0410 − J0395 | 19 ± 3 | 0.08 | 7 |
| J0430 − J0410 | 10.4 ± 1.3 | 0.04 | 4 |
| g − J0430 | 26 ± 3 | 0.10 | 9 |
| J0515 − g | 19 ± 3 | 0.08 | 7 |
| r − J0515 | 6.6 ± 1.2 | 0.03 | 3 |
| J0660 − r | 8.8 ± 2.1 | 0.04 | 4 |
| i − J0660 | 29 ± 4 | 0.12 | 11 |
| J0861 − i | 10.3 ± 1.4 | 0.04 | 4 |
| z − J0861 | 30 ± 4 | 0.12 | 11 |
Notes.
The penultimate column corresponds to the mean magnitude variations estimated using the median values of the light-curve amplitudes and periods in the Asteroid Lightcurve Database (see main text). The final column represents the percentage of error induced in the reflectance by the variations in magnitude.
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