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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.1A.3.

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