We have constructed an ultra wide field telescope named WIDGET to observe
possible prompt optical emission associated with GRBs or shock breakout of
SN explosions. Performing the simultaneous observation with GRB satellite
such as HETE-2 and Swift, the telescope should have an ultra-wide FOV. The
WIDGET telescope has 70 degrees FOV in each side which covers almost all of
the FOV of those satellites. WIDGET is located at Akeno Observatory in
Japan where is about 150km away from Tokyo. The telescope is in operation
since June 2004. We will present the status and early results of one and
half year observations in the conference.