GCN Circular 7915
P.A. Milne (U Arizona) reports on behalf of the Super-LOTIS team: The robotic 0.6m Super-LOTIS telescope began R-band observations of the error region of GRB 080701A at 10:14:25 UT, 49 seconds after the trigger. Initial 10 and 20 second exposures reveal no sources other than those present in the relevant DSS image. A stack of 30x60sec images reveals no source at the location of the XRT source (Stroh et al., GCN 7911), down to a 3-sigma limiting magnitude of R~19.5. Comparisons of initial and final images reveals no brightening or fading sources. We used the USNO-B star at RA=03:02:55.5, Dec=+75:28:42 to derive the R2 magnitude upper-limit. This message can be cited.