Lightcurve analysis of asteroids 106, 752, 847, 1057, 1630, 1670, 1927 1936, 2426, 2612, 2647, 4087, 5635, 5692, and 6235

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.