Photometric observations of asteroids 232 Russia, 1117 Reginita and (11200) 1999 CV121

Photometric observations of three main-belt asteroids were obtained from 2018 April-July from Malta in order to determine their synodic rotation periods. We provide lightcurves for 232 Russia and 1117 Reginita that were obtained from the Spin/Shape Modeling Opportunities list by Warner et al. (2018). The asteroid (11200) 1999 CV121 did not have a referenced period in the LCDB database (Warner et al., 2009).
peer-reviewed