Image Details
Caption: Fig. 15.
Difference in detection times vs. the cosine of the angular separation between MACRO upward‐going muon events and BATSE gamma‐ray bursts. Panels a and b have different timescales. The BATSE GRB of 1995 September 22 (4B 950922) was detected 39.4 s before one MACRO event at an angular distance of 17﹩\fdg﹩6 and the BATSE (4B 940527) GRB of 1994 May 27 280 s after another very horizontal MACRO event at 14﹩\fdg﹩9. In a they are indicated with the name of the bursts.
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