WE PROPOSE TO ANALYZE LAT DATA TO SEARCH FOR EMISSION FROM CATACLYSMIC VARIABLES.THE PREVIOUS DETECTION/UPPER LIMIT SEARCH CONDUCTED IN 1995 USED EGRET DATA. THAT RESULT WAS NULLIFIED BY SMALL-SCALE STRUCTURE UNCOVERED IN THE EGRET BACKGROUND IN 2008. CONSEQUENTLY A NEW SEARCH MUST BE UNDERTAKEN TO PROVIDE RELIABLE DETECTIONS OR UPPER LIMITS ON THE GAMMA-RAY EMISSION OF CVS SO THAT PROGRESS MAY BE MADE TO UNDERSTAND THE EMISSION MECHANISMS.