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|a Chen, Min
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|a Massachusetts Institute of Technology. Department of Physics
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|a Massachusetts Institute of Technology. Laboratory for Nuclear Science
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|a Chen, Min
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|a Chen, Min
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|a Formaggio, Joseph A.
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|a Miller, M. L.
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|a Monreal, Benjamin
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|a Monroe, Jocelyn
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|a Solomon-Oblath, Noah
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|a Ott, Richard A.
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|a Sonley, T. J.
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|a Formaggio, Joseph A.
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|a Miller, M. L.
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|a Monreal, Benjamin
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|a Monroe, Jocelyn
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|a Solomon-Oblath, Noah
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|a Ott, Richard A.
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|a Sonley, T. J.
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|a Low-multiplicity Burst Search at the Sudbury Neutrino Observatory
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|b Institute of Physics Publishing,
|c 2012-04-13T15:42:48Z.
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|z Get fulltext
|u http://hdl.handle.net/1721.1/70015
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|a Results are reported from a search for low-multiplicity neutrino bursts in the Sudbury Neutrino Observatory. Such bursts could indicate the detection of a nearby core-collapse supernova explosion. The data were taken from Phase I (1999 November-2001 May), when the detector was filled with heavy water, and Phase II (2001 July-2003 August), when NaCl was added to the target. The search was a blind analysis in which the potential backgrounds were estimated and analysis cuts were developed to eliminate such backgrounds with 90% confidence before the data were examined. The search maintained a greater than 50% detection probability for standard supernovae occurring at a distance of up to 60 kpc for Phase I and up to 70 kpc for Phase II. No low-multiplicity bursts were observed during the data-taking period.
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|a United States. Dept. of Energy
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|a Alfred P. Sloan Foundation
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|a en_US
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|a Article
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|t Astrophysical Journal
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