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B. Aharmim,5 S.N. Ahmed,11 A.E. Anthony,13 E.W. Beier,10 A. Bellerive,3 M. Bergevin,4 S.D. Biller,9 J. Boger,2, a M.G. Boulay,7 M.G. Bowler,9 T.V. Bullard,15 Y.D. Chan,6 M. Chen,11 X. Chen,6, b B.T. Cleveland,9 G.A. Cox,15 C.A. Currat,6 X. Dai,3, 9 F. Dalnoki-Veress,3 H. Deng,10 P.J. Doe,15 R.S. Dosanjh,3 G. Doucas,9 C.A. Duba,15 F.A. Duncan,11 M.(More)
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)
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)
N. Ackerman,* B. Aharmim, M. Auger, D. J. Auty, P. S. Barbeau, K. Barry, L. Bartoszek, E. Beauchamp, V. Belov, C. Benitez-Medina, M. Breidenbach, A. Burenkov, B. Cleveland, R. Conley, E. Conti, J. Cook, S. Cook, A. Coppens, I. Counts, W. Craddock, T. Daniels, M.V. Danilov, C. G. Davis, J. Davis, R. deVoe, Z. Djurcic, A. Dobi, A.G. Dolgolenko, M. J.(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 existing hydrous titanium oxide (HTiO) technique for the measurement of Ra and Ra in the water at the Sudbury Neutrino Observatory (SNO) has been changed to make it faster and less sensitive to trace impurities in the HTiO eluate. Using HTiO-loaded filters followed by cation exchange adsorption and HTiO co-precipitation, Ra isotopes from 200-450 tonnes(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)