We have observed the error box of GRB030913 (Suzuki et al., GCNC 2383) with MASTER system (http://observ.pereplet.ru) equipped with new AP16E CCD during the first night after the GRB. 25 frames, obtained during first 4 hours after the burst, were combined to achieve the better magnitude limit. No new sources were detected up to 17.5 unfiltered instrumental magnitude with S/N ratio of 3. The part of processed frame is available at http://__/_. North is up, east is left. Position of possible OT, reported by Guziy et al. (GCN 2391) is marked on the image. No source brighter than 17.5 is seen there. This message is citable.