Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apj...428..629m&link_type=abstract
The Astrophysical Journal, vol. 428, no. 2, pt. 1, p. 629-632
Astronomy and Astrophysics
Astrophysics
5
Cosmic Rays, Gamma Ray Bursts, Neutrinos, Radiation Sources, Supernovae, Ginga Satellite, Monte Carlo Method, Photomultiplier Tubes, Solar Maximum Mission, Temporal Resolution
Scientific paper
The temporal structure of low-energy (20 to 60 MeV) neutrino interactions within the Irvine-Michigan-Brookhaven-3 (IMB-3) detector during 863 days of livetime between 1986 May and 1991 March has been analyzed. The neutrino data are consistent with expected cosmic-ray-induced neutrino interactions with no bursts evident (excluding SN 1987A). When combined with the 327 effective livedays of IMB-1 data, we place a 90% C.L. upper limit of less than or equal to 0.71 Galactic supernovae/yr. We have also performed a temporal correlation analysis with gamma-ray bursts (GRBs) using a subset of the low-energy neutrino data. No significant correlations were observed for coincidence windows of 1 minute, 1 hour, or 1 day.
Becker-Szendy R.
Bratton C. B.
Breault J.
Casper D.
Dye Stephen T.
No associations
LandOfFree
A search for astrophysical sources of low-energy neutrinos using the IMB detector does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A search for astrophysical sources of low-energy neutrinos using the IMB detector, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A search for astrophysical sources of low-energy neutrinos using the IMB detector will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1862934