The targets selected for this project are Magellanic Clouds And the galactic nucleus ball in the Milky Way, because there are many stars in the middle, it can be used as a gravity lens when the star obscures the target. Many observations were made at the Las Campanas Observatory in Chile, and Princeton University And Carnegie College. The plan is divided into three stages, including OGLE-I, OGLE-II and OGLE-III.
OGLE 2003-BLG-235Lb (MOA 2003-BLG-53b)
OGLE-2005-BLG-071Lb
OGLE-2005-BLG-169Lb
OGLE-2005-BLG-390Lb
OGLE-2006-BLG-109Lb
OGLE-2006-BLG-109Lc
OGLE-TR-10 b
OGLE-TR-56b
OGLE-TR-111b
OGLE-TR-113b
OGLE-TR-132b