Adamson, P.Anghel, I.Aurisano, A.Barr, G.Bishai, M.Blake, A.Bock, G. J.Bogert, D.Cao, S. V.Castromonte, C. M.Cherdack, D.Childress, S.Coelho, J. A. B.Corwin, L.Cronin-Hennessy, D.de Jong, J. K.Devan, A. V.Devenish, N. E.Diwan, M. V.Escobar, C. O.Evans, J. J.Falk, E.Feldman, GaryFrohne, M. V.Gallagher, H. R.Gomes, R. A.Goodman, M. C.Gouffon, P.Graf, N.Gran, R.Grzelak, K.Habig, A.Hahn, S. R.Hartnell, J.Hatcher, R.Himmel, A.Holin, A.Huang, J.Hylen, J.Irwin, G. M.Isvan, Z.James, C.Jensen, D.Kafka, T.Kasahara, S. M. S.Koizumi, G.Kordosky, M.Kreymer, A.Lang, K.Ling, J.Litchfield, P. J.Lucas, P.Mann, W. A.Marshak, M. L.Mayer, N.McGivern, C.Medeiros, M. M.Mehdiyev, R.Meier, J. R.Messier, M. D.Michael, D. G.Miller, W. H.Mishra, S. R.Moed Sher, S.Moore, C. D.Mualem, L.Musser, J.Naples, D.Nelson, J. K.Newman, H. B.Nichol, R. J.Nowak, J. A.O’Connor, J.Orchanian, M.Pahlka, R. B.Paley, J.Patterson, R. B.Pawloski, G.Perch, A.Phan-Budd, S.Plunkett, R. K.Poonthottathil, N.Qiu, X.Radovic, A.Rebel, B.Rosenfeld, C.Rubin, H. A.Sanchez, M. C.Schneps, J.Schreckenberger, A.Schreiner, P.Sharma, R.Sousa, A.Tagg, N.Talaga, R. L.Thomas, J.Thomson, M. A.Tian, X.Timmons, A.Tognini, S. C.Toner, RuthTorretta, D.Tzanakos, G.Urheim, J.Vahle, P.Viren, B.Weber, A.Webb, R. C.White, C.Whitehead, L.Whitehead, L. H.Wojcicki, S. G.Zwaska, R.2016-09-132014Adamson, P., I. Anghel, A. Aurisano, G. Barr, M. Bishai, A. Blake, G. J. Bock, et al. 2014. "Combined Analysis of νμ Disappearance and νμ→νe Appearance in MINOS Using Accelerator and Atmospheric Neutrinos.” Physical Review Letters 112 (19) (May 12). doi:10.1103/physrevlett.112.191801.0031-9007http://nrs.harvard.edu/urn-3:HUL.InstRepos:28456692We report on a new analysis of neutrino oscillations in MINOS using the complete set of accelerator and atmospheric data. The analysis combines the νμ disappearance and νe appearance data using the three-flavor formalism. We measure |Δm232|=[2.28–2.46]×10−3  eV2 (68% C.L.) and sin2θ23=0.35–0.65 (90% C.L.) in the normal hierarchy, and |Δm232|=[2.32–2.53]×10−3  eV2 (68% C.L.) and sin2θ23=0.34–0.67 (90% C.L.) in the inverted hierarchy. The data also constrain δCP, the θ23 octant degeneracy and the mass hierarchy; we disfavor 36% (11%) of this three-parameter space at 68% (90%) C.L.en-USeutrino: mass: hierarchyneutrino: atmosphereneutrino: oscillationMINOSneutrino/mu: beamneutrino/mu: fluxneutrino/e: particle identificationflavor: 3neutrino: mass differenceneutrino: mixing angleCP: violationexperimental resultsJournal Article2016-09-1310.1103/PhysRevLett.112.191801