We present a new EROS-2 measurement of the microlensing optical depth toward the Galactic Bulge. Light curves of 5.6x10^6^ clump-giant stars distributed over 66deg^2^ of the Bulge were monitored during seven Bulge seasons. 120 events were found with apparent amplifications greater than 1.6 and Einstein radius crossing times in the range 5d<t_E_<400d. This is the largest existing sample of clump-giant events and the first to include northern Galactic fields.

Cone search capability for table J/A+A/454/185/table3 (The 120 events used for the measurement of the optical depth)