Abstract

Lightcurve period and amplitude results are reported for fifteen asteroids observed at Carbuncle Hill Observatory during June 2004 - March 2005. The following synodic periods and amplitudes were determined: 106 Dione, 16.26±0.02h, 0.08±0.02m; 752 Sulamitis, 27.367±0.005h, 0.20±0.03m; 847 Agnia, 14.827±0.001h, 0.45±0.03m; 1057 Wanda, 28.49±0.03h, 0.14±0.02m; 1630 Milet, 32.55±0.03h, 0.37± 0.03m; 1670 Minnaert, 3.528±0.001h, 0.23±0.02m; 1927 Suvanto, 8.163±0.003h, 0.60±0.03m; 1936 Lugano, 19.651±0.015h, 0.31±0.04m; 2426 Simonov, 5.811±0.002h, 0.40±0.03m; 2612 Kathryn, 7.700±0.002h, 0.43±0.02m; 2647 Sova, 9.37±0.01h, 0.30±0.02m; 4087 Part, 16.47±0.02h, 0.59±0.03m; 5635 Cole, 5.792±0.001h, 0.33±0.04m; 5692 Shirao, 2.886±0.002h, 0.12±0.03m; (6235) 1987VB, 15.515±0.002h, 0.60±0.04m.