Rs. Miller et al., A SEARCH FOR ASTROPHYSICAL SOURCES OF LOW-ENERGY NEUTRINOS USING THE IMB DETECTOR, The Astrophysical journal, 428(2), 1994, pp. 629-632
The temporal structure of low-energy (20-60 MeV) neutrino interactions
within the IMB-3 detector during 863 days of livetime between 1986 Ma
y and 1991 March has been analyzed. The neutrino data are consistent w
ith expected cosmic-ray-induced neutrino interactions with no bursts e
vident (excluding SN 1987A). When combined with the 327 effective live
days of IMB-1 data, we place a 90% C.L. upper limit of less-than-or-eq
ual-to 0.71 Galactic supernovae yr-1. We have also performed a tempora
l correlation analysis with gamma-ray bursts (GRBs) using a subset of
the low-energy neutrino data. No significant correlations were observe
d for coincidence windows of 1 minute, 1 hour, or 1 day.