Notes. For each light curve, labelled as ID 1–30, the date of the beginning of the observing night is given as well as the heliocentric (R_h) and geocentric (Δ) distances measured in AU, the solar phase angle (α), and the observed ecliptic longitude (λ_O), and latitude (β_O) of the target. In some cases (light curves 1, 2, 4, 5, and 28) a single light curve has been composed of segments gathered over a few nights. The designation of instrument used is listed in the “Telescope” column. For each light curve segment a total time span of the light curve in hours, and imaging filter used are listed in columns “Total” and “Filter”, respectively. Where applicable, a reference to the already published work is given in the “Ref.” column. Telescope key (with MPC site code): (MtL, I52) NASA-UA Mt. Lemmon 60 in, Arizona, USA; (S90, 695), Steward Observatory 90 in Bok Telescope, Arizona, USA; (Kh, 121), Kharkiv Astronomical Observatory 0.7 m Telescope, Ukraine; (ESO1, 809), European Southern Observatory (ESO) 1 m Telescope, La Silla, Chile; (ESOD, 809), Danish 1.54 m Telescope, La Silla, Chile; (SAS, A12), Stazione Astronomica di Sozzago 0.4 m Telescope, Italy; (NTT, 809), European Southern Observatory 3.5 m New Technology Telescope, Chile; (TMO, 673), Table Mountain Observatory, California, USA; (ESO22, 809), ESO/Max Planck Institute 2.2 m Telescope, La Silla, Chile; (PAL, 675), Palomar Observatory 5 m Hale Telescope, California, USA.

References.(1) Wisniewski et al. (1997); (2) Velichko et al. (1989); (3) Hoffmann et al. (1993); (4) Erikson et al. (2000); (5) Beherend & Manzini (priv. comm.).