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Low-multiplicity burst search at the Sudbury Neutrino Observatory

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Low-multiplicity burst search at the Sudbury Neutrino Observatory. / SNO Collaboration.
In: The Astrophysical Journal, Vol. 728, No. 2, 83, 20.02.2011.

Research output: Contribution to Journal/Magazine › Journal article › peer-review

Harvard

SNO Collaboration 2011, 'Low-multiplicity burst search at the Sudbury Neutrino Observatory', The Astrophysical Journal, vol. 728, no. 2, 83. https://doi.org/10.1088/0004-637X/728/2/83

APA

SNO Collaboration (2011). Low-multiplicity burst search at the Sudbury Neutrino Observatory. The Astrophysical Journal, 728(2), Article 83. https://doi.org/10.1088/0004-637X/728/2/83

Vancouver

SNO Collaboration. Low-multiplicity burst search at the Sudbury Neutrino Observatory. The Astrophysical Journal. 2011 Feb 20;728(2):83. doi: 10.1088/0004-637X/728/2/83

Author

SNO Collaboration. / Low-multiplicity burst search at the Sudbury Neutrino Observatory. In: The Astrophysical Journal. 2011 ; Vol. 728, No. 2.

Bibtex

@article{5e161525e1524bbba0e39d98a41a068a,
title = "Low-multiplicity burst search at the Sudbury Neutrino Observatory",
abstract = "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.",
keywords = "neutrinos, supernovae , general",
author = "B. Aharmim and Ahmed, {S. N.} and Anthony, {A. E.} and N. Barros and Beier, {E. W.} and A. Bellerive and B. Beltran and M. Bergevin and Biller, {S. D.} and K. Boudjemline and Boulay, {M. G.} and B. Cai and Chan, {Y. D.} and D. Chauhan and M. Chen and Cleveland, {B. T.} and X. Dai and H. Deng and J. Detwiler and G. Doucas and P.-l. Drouin and Duncan, {F. A.} and M. Dunford and Earle, {E. D.} and Elliott, {S. R.} and Evans, {H. C.} and Ewan, {G. T.} and J. Farine and H. Fergani and F. Fleurot and Ford, {R. J.} and Formaggio, {J. A.} and N. Gagnon and Goon, {J. T. M.} and K. Graham and E. Guillian and S. Habib and Hahn, {R. L.} and Hallin, {A. L.} and Hallman, {E. D.} and Harvey, {P. J.} and R. Hazama and Heintzelman, {W. J.} and J. Heise and Helmer, {R. L.} and A. Hime and C. Howard and M. Huang and B. Jamieson and O'keeffe, {H. M.} and {SNO Collaboration}",
year = "2011",
month = feb,
day = "20",
doi = "10.1088/0004-637X/728/2/83",
language = "English",
volume = "728",
journal = "The Astrophysical Journal",
issn = "0004-637X",
publisher = "Institute of Physics Publishing",
number = "2",

}

RIS

TY - JOUR

T1 - Low-multiplicity burst search at the Sudbury Neutrino Observatory

AU - Aharmim, B.

AU - Ahmed, S. N.

AU - Anthony, A. E.

AU - Barros, N.

AU - Beier, E. W.

AU - Bellerive, A.

AU - Beltran, B.

AU - Bergevin, M.

AU - Biller, S. D.

AU - Boudjemline, K.

AU - Boulay, M. G.

AU - Cai, B.

AU - Chan, Y. D.

AU - Chauhan, D.

AU - Chen, M.

AU - Cleveland, B. T.

AU - Dai, X.

AU - Deng, H.

AU - Detwiler, J.

AU - Doucas, G.

AU - Drouin, P.-l.

AU - Duncan, F. A.

AU - Dunford, M.

AU - Earle, E. D.

AU - Elliott, S. R.

AU - Evans, H. C.

AU - Ewan, G. T.

AU - Farine, J.

AU - Fergani, H.

AU - Fleurot, F.

AU - Ford, R. J.

AU - Formaggio, J. A.

AU - Gagnon, N.

AU - Goon, J. T. M.

AU - Graham, K.

AU - Guillian, E.

AU - Habib, S.

AU - Hahn, R. L.

AU - Hallin, A. L.

AU - Hallman, E. D.

AU - Harvey, P. J.

AU - Hazama, R.

AU - Heintzelman, W. J.

AU - Heise, J.

AU - Helmer, R. L.

AU - Hime, A.

AU - Howard, C.

AU - Huang, M.

AU - Jamieson, B.

AU - O'keeffe, H. M.

AU - SNO Collaboration

PY - 2011/2/20

Y1 - 2011/2/20

N2 - 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.

AB - 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.

KW - neutrinos

KW - supernovae

KW - general

U2 - 10.1088/0004-637X/728/2/83

DO - 10.1088/0004-637X/728/2/83

M3 - Journal article

VL - 728

JO - The Astrophysical Journal

JF - The Astrophysical Journal

SN - 0004-637X

IS - 2

M1 - 83

ER -