Table 2
Lightcurve characteristics for asteroids (21) Lutetia, (26) Proserpina, and (585) Bilkis incorporated in the present study.
Asteroid | Class | N | K | Tobs (d) | Tobs (a) |
---|---|---|---|---|---|
(21) Lutetia | M | 4012 | 50 | 17 306.80 | 47.38 |
7 | 1 | 435.65 | 1.19 | ||
4019 | 51 | 19 365.98 | 53.02 | ||
(26) Proserpina | S | 6664 | 29 | 17 609.83 | 48.21 |
563 | 1 | 4847.88 | 13.27 | ||
39 | 1 | 542.78 | 1.49 | ||
7266 | 31 | 18 694.55 | 51.18 | ||
(585) Bilkis | C/D/P | 1844 | 17 | 4926.69 | 13.49 |
32 | 1 | 621.66 | 1.70 | ||
1876 | 18 | 5480.45 | 15.00 |
Notes. “Class” denotes the Tholen taxonomical class, N and K denote the numbers of observations and lightcurves, respectively, and Tobs is the time span of the observations. For Lutetia and Bilkis, the uppermost numbers refer to the ground-based observations, the ones in the middle to the GDR2 observations, and the lowermost ones refer to the combined observations. For Proserpina, the second row describes an additional sparse ground-based lightcurve. For the references to the observations, see Tables A.1–A.3.
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