James C. Loach

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B. Aharmim,6 S. N. Ahmed,14 A. E. Anthony,17,* N. Barros,8 E. W. Beier,13 A. Bellerive,4 B. Beltran,1 M. Bergevin,5,7 S. D. Biller,12 K. Boudjemline,4 M. G. Boulay,14 T. H. Burritt,19 B. Cai,14 Y. D. Chan,7 D. Chauhan,6 M. Chen,14 B. T. Cleveland,12 G. A. Cox,19 X. Dai,4,12,14 H. Deng,13 J. Detwiler,7 M. DiMarco,14 P. J. Doe,19 G. Doucas,12 P.-L. Drouin,4(More)
An array of Neutral-Current Detectors (NCDs) has been built in order to make a unique measurement of the total active flux of solar neutrinos in the Sudbury Neutrino Observatory (SNO). Data in the third phase of the SNO experiment were collected between November 2004 and November 2006, after the NCD array was added to improve the neutral-current sensitivity(More)
B. Aharmim, S. N. Ahmed, J. F. Amsbaugh, A. E. Anthony, J. Banar, N. Barros, E.W. Beier, A. Bellerive, B. Beltran, M. Bergevin, S. D. Biller, K. Boudjemline, M.G. Boulay, T. J. Bowles, M. C. Browne, T. V. Bullard, T. H. Burritt, B. Cai, Y.D. Chan, D. Chauhan, M. Chen, B. T. Cleveland, G.A. Cox-Mobrand, C. A. Currat, X. Dai, H. Deng, J. Detwiler, M. DiMarco,(More)
B. Aharmim, S. N. Ahmed, A. E. Anthony, a N. Barros, b E. W. Beier, A. Bellerive, B. Beltran, M. Bergevin, 5, c S. D. Biller, K. Boudjemline, 14 M. G. Boulay, B. Cai, Y. D. Chan, D. Chauhan, M. Chen, B. T. Cleveland, G. A. Cox, d X. Dai, 12, 4 H. Deng, J. A. Detwiler, M. DiMarco, P. J. Doe, G. Doucas, P.-L. Drouin, F. A. Duncan, 14 M. Dunford, e E. D.(More)
B. Aharmim, S. N. Ahmed, T. C. Andersen, A. E. Anthony, N. Barros, E.W. Beier, A. Bellerive, B. Beltran, M. Bergevin, S. D. Biller, K. Boudjemline, M.G. Boulay, T. H. Burritt, B. Cai, Y. D. Chan, M. Chen, M.C. Chon, B. T. Cleveland, G.A. Cox-Mobrand, C. A. Currat, X. Dai, F. Dalnoki-Veress, H. Deng, J. Detwiler, P. J. Doe, R. S. Dosanjh, G. Doucas, P.-L.(More)
A search has been made for neutrinos from the hep reaction in the Sun and from the diffuse supernova neutrino background (DSNB) using data collected during the first operational phase of the Sudbury Neutrino Observatory, with an exposure of 0.65 ktons yr. For the hep neutrino search, two events are observed in the effective electron energy range of 14:3 MeV(More)
The Sudbury Neutrino Observatory (SNO) used an array of 3He proportional counters to measure the rate of neutral-current interactions in heavy water and precisely determined the total active (nu_x) 8B solar neutrino flux. This technique is independent of previous methods employed by SNO. The total flux is found to be(More)
The Sudbury Neutrino Observatory (SNO) has confirmed the standard solar model and neutrino oscillations through the observation of neutrinos from the solar core. In this paper we present a search for neutrinos associated with sources other than the solar core, such as gammaray bursters and solar flares. We present a new method for looking for temporal(More)
We present a novel algorithm for optimizing the order in which Chinese characters are learned, one that incorporates the benefits of learning them in order of usage frequency and in order of their hierarchal structural relationships. We show that our work outperforms previously published orders and algorithms. Our algorithm is applicable to any scheduling(More)
B. Aharmim,7 Q. R. Ahmad,22 S. N. Ahmed,17 R. C. Allen,4 T. C. Andersen,6 J. D. Anglin,13 G. Bühler,4 J. C. Barton,14,* E. W. Beier,15 M. Bercovitch,13 M. Bergevin,6,8 J. Bigu,7 S. D. Biller,14 R. A. Black,14 I. Blevis,5 R. J. Boardman,14 J. Boger,3,† E. Bonvin,17 M. G. Boulay,10,17 M. G. Bowler,14 T. J. Bowles,10 S. J. Brice,10,14,‡ M. C. Browne,10,22 T.(More)