Photometric masking methods and predicted performances for the CoRoT exoplanetary mission

摘要

CoRoT mission for year 2006 is a small space telescope that will measure continuously for 6 months the light flux of 12000 star in a mission of 2(1/2) years. The aim is to detect small droops in the light curves revealing planets transiting in front of their star. For this, 12 000 logical Regions Of Interest (ROI) are denned on the CCD to optimise each star Signal to Noise Ratio (s/n). Unfortunatly only less than 256 different shapes are permitted for all ROIs, forseeing a loss in global S/N. We found a method wich reduces the 12000 ROIs to a small set of 250 shapes in a lossless way. Overall performances are discussed.