Publications


Performance of a full scale prototype detector at the BR2 reactor for the SoLid experiment

JOURNAL OF INSTRUMENTATION 13 (2018) ARTN P05005

Y Abreu, Y Amhis, L Arnold, G Ban, W Beaumont, M Bongrand, D Boursette, BC Castle, K Clark, B Coupe, D Cussans, A De Roeck, J D'Hondt, D Durand, M Fallot, L Ghys, L Giot, B Guillon, S Ihantola, X Janssen, S Kalcheva, LN Kalousis, E Koonen, M Labare, G Lehaut, L Manzanillas, J Mermans, I Michiels, C Moortgat, D Newbold, J Park, V Pestel, K Petridis, I Pinera, G Pommery, L Popescu, G Pronost, J Rademacker, D Ryckbosch, N Ryder, D Saunders, M-H Schune, L Simard, A Vacheret, S Van Dyck, P Van Mulders, N van Remortel, S Vercaemer, M Verstraeten, A Weber, F Yermia, S Collaboration


Ionization electron signal processing in single phase LArTPCs. Part II. Data/simulation comparison and performance in MicroBooNE

JOURNAL OF INSTRUMENTATION 13 (2018) ARTN P07007

C Adams, R An, J Anthony, J Asaadi, M Auger, S Balasubramanian, B Baller, C Barnes, G Barr, M Bass, F Bay, A Bhat, K Bhattacharya, M Bishai, A Blake, T Bolto, L Camilleri, D Caratelli, IC Terrazas, R Carr, RC Fernandez, F Cavanna, G Cerati, H Chen, Y Chen, E Church, D Cianci, E Cohen, GH Collin, JM Conrad, M Convery, L Cooper-Troendler, I Crespo-Anadon, M Del Tutto, D Devitt, A Diaz, M Dolce, S Dytman, B Eberly, A Ereditato, LE Sanchez, J Esquivel, JJ Evans, AA Fadeeva, BT Fleming, W Foreman, AP Furmanski, D Garcia-Gamez, GT Garvey, V Genty, D Goeldi, S Gollapinni, E Gramellini, H Greenlee, R Grosso, R Guenette, P Guzowski, A Hackenburg, P Hamilton, O Hen, J Hewes, C Hill, J Ho, GA Horton-Smith, A Hourlier, E-C Huang, C James, JJ de Vries, L Jiang, RA Johnson, J Joshi, H Jostlein, Y-J Jwa, D Kaleko, G Karagiorgi, W Ketchum, B Kirby, M Kirby, T Kobilarcik, I Kreslo, Y Li, A Lister, BR Littlejohn, S Lockwitz, D Lorca, WC Louis, M Luethi, B Lundberg, X Luo, A Marchionni, S Marcocci, C Mariani, J Marshall, DAM Caicedo, A Mastbaum, V Meddage, T Mettler, T Miceli, GB Mills, A Mogan, J Moon, M Mooney, CD Moore, J Mousseau, M Murphy, R Murrells, D Naples, P Nienaber, J Nowak, O Palamara, V Pandey, V Paolone, A Papadopoulou, V Papavassiliou, SF Pate, Z Pavlovic, E Piasetzky, D Porzio, G Pulliam, X Qian, JL Raaf, V Radek, A Rafique, L Rochester, M Ross-Lonergan, CR von Rohr, B Russell, DW Schmitz, A Schukraft, W Seligman, MH Shaevitz, J Sinclair, A Smith, EL Snider, M Soderberg, S Soldner-Rembold, SR Soleti, P Spentzouris, J Spitz, J St John, T Strauss, K Sutton, S Sword-Fehlberg, AM Szelc, N Tagg, W Tang, K Terao, M Thomson, M Toups, Y-T Tsai, S Tufanli, T Usher, W Van De Pontseele, RG Van de Water, B Viren, M Weber, H Wei, DA Wickremasinghe, K Wierman, Z Williams, S Wolbers, T Wongjirad, K Woodruff, T Yang, G Yarbrough, LE Yates, B Yu, GP Zeller, J Zennamo, C Zhang, M Collaboration


Photon detector system timing performance in the DUNE 35-ton prototype liquid argon time projection chamber

JOURNAL OF INSTRUMENTATION 13 (2018) ARTN P06022

DL Adams, T Alion, JT Anderson, L Bagby, M Baird, G Barr, N Barros, K Biery, A Blake, E Blaufuss, T Boone, A Booth, D Brailsford, N Buchanan, A Chatterjee, M Convery, J Davies, T Dealtry, P DeLurgio, G Deuerling, R Dharmapala, Z Djurcic, G Drake, B Eberly, J Freeman, S Glavin, RA Gomes, MC Goodman, M Graham, A Hahn, JT Haigh, J Hartnell, A Higuera, A Himmel, J Insler, J Jacobsen, T Junk, B Kirby, J Klein, VA Kudryavtsev, T Kutter, Y Li, X Li, S Lin, J Martin-Albo, N McConkey, CA Moura, S Mufson, TC Nicholls, J Nowak, M Oberling, J Paley, X Qian, JL Raaf, D Rivera, G Santucci, G Sinev, NJC Spooner, M Stancari, I Stancu, D Stefan, J Stewart, J Stock, T Strauss, R Sulej, Y Sun, M Thiesse, LF Thompson, YT Tsai, M Wallbank, TK Warburton, D Warner, D Whittington, RJ Wilson, M Worcester, E Worcester, T Yang, C Zhang


Ionization electron signal processing in single phase LArTPCs. Part I. Algorithm Description and quantitative evaluation with MicroBooNE simulation

JOURNAL OF INSTRUMENTATION 13 (2018) ARTN P07006

C Adams, R An, J Anthony, J Asaadi, M Auger, L Bagby, S Balasubramanian, B Baller, C Barnes, G Barr, M Bass, F Bay, A Bhat, K Bhattacharya, M Bishai, A Blake, T Bolton, L Camilleri, D Caratelli, RC Fernandez, F Cavanna, G Cerati, H Chen, Y Chen, E Church, D Cianci, E Cohen, GH Collin, JM Conrad, M Convery, L Cooper-Troendle, JI Crespo-Anadon, M Del Tutto, D Devitt, A Diaz, S Dytman, B Eberly, A Ereditato, LE Sanchez, J Esquivel, JJ Evans, AA Fadeeva, BT Fleming, W Foreman, AP Furmanski, D Garcia-Gamez, GT Garvey, V Genty, D Goeldi, S Gollapinni, E Gramellini, H Greenlee, R Grosso, R Guenette, P Guzowski, A Hackenburg, P Hamilton, O Hen, J Hewes, C Hill, J Ho, GA Horton-Smith, A Hourlier, E-C Huang, C James, JJ de Vries, L Jiang, RA Johnson, J Joshi, H Jostlein, Y-J Jwa, D Kaleko, G Karagiorgi, W Ketchum, B Kirby, M Kirby, T Kobilarcik, I Kreslo, Y Li, A Lister, BR Littlejohn, S Lockwitz, D Lorca, WC Louis, M Luethi, B Lundberg, X Luo, A Marchionni, S Marcocci, C Mariani, J Marshall, DAM Caicedo, A Mastbaum, V Meddage, T Miceli, GB Mills, A Mogan, J Moon, M Mooney, CD Moore, J Mousseau, M Murphy, R Murrells, D Naples, P Nienaber, J Nowak, O Palamara, V Pandey, V Paolone, A Papadopoulou, V Papavassiliou, SF Pate, Z Pavlovic, E Piasetzky, D Porzio, G Pulliam, X Qian, JL Raaf, V Radeka, A Rafique, L Rochester, M Ross-Lonergan, CR von Rohr, B Russell, DW Schmitz, A Schukraft, W Seligman, MH Shaevitz, J Sinclair, A Smith, EL Snider, M Soderberg, S Soldner-Rembold, SR Soleti, P Spentzouris, J Spitz, J St John, T Strauss, K Sutton, S Sword-Fehlberg, AM Szelc, N Tagg, W Tang, K Terao, M Thomson, C Thorn, M Toups, Y-T Tsai, S Tufanli, T Usher, W Van De Pontseele, RG Van de Water, B Viren, M Weber, H Wei, D Wickremasinghe, K Wierman, Z Williams, S Wolbers, T Wongjirad, K Woodruff, T Yang, G Yarbrough, LE Yates, B Yu, GP Zeller, J Zennamo, C Zhang, M Collaboration


Search for Boosted Dark Matter Interacting with Electrons in Super-Kamiokande.

Physical review letters 120 (2018) 221301-

C Kachulis, K Abe, C Bronner, Y Hayato, M Ikeda, K Iyogi, J Kameda, Y Kato, Y Kishimoto, L Marti, M Miura, S Moriyama, M Nakahata, Y Nakano, S Nakayama, Y Okajima, A Orii, G Pronost, H Sekiya, M Shiozawa, Y Sonoda, A Takeda, A Takenaka, H Tanaka, S Tasaka, T Tomura, R Akutsu, T Kajita, K Kaneyuki, Y Nishimura, K Okumura, KM Tsui, L Labarga, P Fernandez, FDM Blaszczyk, J Gustafson, E Kearns, JL Raaf, JL Stone, LR Sulak, S Berkman, S Tobayama, M Goldhaber, M Elnimr, WR Kropp, S Mine, S Locke, P Weatherly, MB Smy, HW Sobel, V Takhistov, KS Ganezer, J Hill, JY Kim, IT Lim, RG Park, A Himmel, Z Li, E O'Sullivan, K Scholberg, CW Walter, T Ishizuka, T Nakamura, JS Jang, K Choi, JG Learned, S Matsuno, SN Smith, J Amey, RP Litchfield, WY Ma, Y Uchida, MO Wascko, S Cao, M Friend, T Hasegawa, T Ishida, T Ishii, T Kobayashi, T Nakadaira, K Nakamura, Y Oyama, K Sakashita, T Sekiguchi, T Tsukamoto, KE Abe, M Hasegawa, AT Suzuki, Y Takeuchi, T Yano, T Hayashino, T Hiraki, S Hirota, K Huang, M Jiang, KE Nakamura, T Nakaya, B Quilain, ND Patel, RA Wendell, LHV Anthony, N McCauley, A Pritchard, Y Fukuda, Y Itow, M Murase, F Muto, P Mijakowski, K Frankiewicz, CK Jung, X Li, JL Palomino, G Santucci, C Vilela, MJ Wilking, C Yanagisawa, S Ito, D Fukuda, H Ishino, A Kibayashi, Y Koshio, H Nagata, M Sakuda, C Xu, Y Kuno, D Wark, F Di Lodovico, B Richards, R Tacik, SB Kim, A Cole, L Thompson, H Okazawa, Y Choi, K Ito, K Nishijima, M Koshiba, Y Totsuka, Y Suda, M Yokoyama, RG Calland, M Hartz, K Martens, C Simpson, Y Suzuki, MR Vagins, D Hamabe, M Kuze, T Yoshida, M Ishitsuka, JF Martin, CM Nantais, HA Tanaka, A Konaka, S Chen, L Wan, Y Zhang, RJ Wilkes, A Minamino, Super-Kamiokande Collaboration

A search for boosted dark matter using 161.9 kt yr of Super-Kamiokande IV data is presented. We search for an excess of elastically scattered electrons above the atmospheric neutrino background, with a visible energy between 100 MeV and 1 TeV, pointing back to the Galactic center or the Sun. No such excess is observed. Limits on boosted dark matter event rates in multiple angular cones around the Galactic center and Sun are calculated. Limits are also calculated for a baseline model of boosted dark matter produced from cold dark matter annihilation or decay. This is the first experimental search for boosted dark matter from the Galactic center or the Sun interacting in a terrestrial detector.


First Results from the DEAP-3600 Dark Matter Search with Argon at SNOLAB.

Physical review letters 121 (2018) 071801-

P-A Amaudruz, M Baldwin, M Batygov, B Beltran, CE Bina, D Bishop, J Bonatt, G Boorman, MG Boulay, B Broerman, T Bromwich, JF Bueno, PM Burghardt, A Butcher, B Cai, S Chan, M Chen, R Chouinard, BT Cleveland, D Cranshaw, K Dering, J DiGioseffo, S Dittmeier, FA Duncan, M Dunford, A Erlandson, N Fatemighomi, S Florian, A Flower, RJ Ford, R Gagnon, P Giampa, VV Golovko, P Gorel, R Gornea, E Grace, K Graham, E Gulyev, R Hakobyan, A Hall, AL Hallin, M Hamstra, PJ Harvey, C Hearns, CJ Jillings, O Kamaev, A Kemp, M Kuźniak, S Langrock, F La Zia, B Lehnert, JJ Lidgard, C Lim, T Lindner, Y Linn, S Liu, P Majewski, R Mathew, AB McDonald, T McElroy, T McGinn, JB McLaughlin, S Mead, R Mehdiyev, C Mielnichuk, J Monroe, A Muir, P Nadeau, C Nantais, C Ng, AJ Noble, E O'Dwyer, C Ohlmann, K Olchanski, KS Olsen, C Ouellet, P Pasuthip, SJM Peeters, TR Pollmann, ET Rand, W Rau, C Rethmeier, F Retière, N Seeburn, B Shaw, K Singhrao, P Skensved, B Smith, NJT Smith, T Sonley, J Soukup, R Stainforth, C Stone, V Strickland, B Sur, J Tang, J Taylor, L Veloce, E Vázquez-Jáuregui, J Walding, M Ward, S Westerdale, E Woolsey, J Zielinski, DEAP-3600 Collaboration

This Letter reports the first results of a direct dark matter search with the DEAP-3600 single-phase liquid argon (LAr) detector. The experiment was performed 2 km underground at SNOLAB (Sudbury, Canada) utilizing a large target mass, with the LAr target contained in a spherical acrylic vessel of 3600 kg capacity. The LAr is viewed by an array of PMTs, which would register scintillation light produced by rare nuclear recoil signals induced by dark matter particle scattering. An analysis of 4.44 live days (fiducial exposure of 9.87 ton day) of data taken during the initial filling phase demonstrates the best electronic recoil rejection using pulse-shape discrimination in argon, with leakage <1.2×10^{-7} (90% C.L.) between 15 and 31  keV_{ee}. No candidate signal events are observed, which results in the leading limit on weakly interacting massive particle (WIMP)-nucleon spin-independent cross section on argon, <1.2×10^{-44}  cm^{2} for a 100  GeV/c^{2} WIMP mass (90% C.L.).


Atmospheric neutrino oscillation analysis with external constraints in Super-Kamiokande I-IV

PHYSICAL REVIEW D 97 (2018) ARTN 072001

K Abe, C Bronner, Y Haga, Y Hayato, M Ikeda, K Iyogi, J Kameda, Y Kato, Y Kishimoto, L Marti, M Miura, S Moriyama, M Nakahata, T Nakajima, Y Nakano, S Nakayama, Y Okajima, A Orii, G Pronost, H Sekiya, M Shiozawa, Y Sonoda, A Takeda, A Takenaka, H Tanaka, S Tasaka, T Tomura, R Akutsu, T Irvine, T Kajita, I Kametani, K Kaneyuki, Y Nishimura, K Okumura, E Richard, KM Tsui, L Labarga, P Fernandez, FDM Blaszczyk, J Gustafson, C Kachulis, E Kearns, JL Raaf, JL Stone, LR Sulak, S Berkman, S Tobayama, M Goldhaber, G Carminati, M Elnimr, WR Kropp, S Mine, S Locke, A Renshaw, MB Smy, HW Sobel, V Takhistov, P Weatherly, KS Ganezer, BL Hartfiel, J Hill, N Hong, JY Kim, IT Lim, RG Park, T Akiri, A Himmel, Z Li, E O'Sullivan, K Scholberg, CW Walter, T Wongjirad, T Ishizuka, T Nakamura, JS Jang, K Choi, JG Learned, S Matsuno, SN Smith, J Amey, RP Litchfield, WY Ma, Y Uchida, MO Wascko, S Cao, M Friend, T Hasegawa, T Ishida, T Ishii, T Kobayashi, T Nakadaira, K Nakamura, Y Oyama, K Sakashita, T Sekiguchi, T Tsukamoto, KE Abe, M Hasegawa, AT Suzuki, Y Takeuchi, T Yano, T Hayashino, S Hirota, K Huang, K Ieki, M Jiang, T Kikawa, KE Nakamura, T Nakaya, ND Patel, K Suzuki, S Takahashi, RA Wendell, LHV Anthony, N McCauley, A Pritchard, Y Fukuda, Y Itow, G Mitsuka, M Murase, F Muto, T Suzuki, P Mijakowski, K Frankiewicz, J Hignight, J Imber, CK Jung, X Li, JL Palomino, G Santucci, C Vilela, MJ Wilking, C Yanagisawa, S Ito, D Fukuda, H Ishino, T Kayano, A Kibayashi, Y Koshio, T Mori, H Nagata, M Sakuda, C Xu, Y Kuno, D Wark, F Di Lodovico, B Richards, R Tacik, SB Kim, A Cole, L Thompson, H Okazawa, Y Choi, K Ito, K Nishijima, M Koshiba, Y Totsuka, Y Suda, M Yokoyama, RG Calland, M Hartz, K Martens, B Quilain, C Simpson, Y Suzuki, MR Vagins, D Hamabe, M Kuze, T Yoshida, M Ishitsuka, JF Martin, CM Nantais, P de Perio, HA Tanaka, A Konaka, S Chen, L Wan, Y Zhang, RJ Wilkes, A Minamino, SK Collaboration


Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger

ASTROPHYSICAL JOURNAL LETTERS 857 (2018) ARTN L4

K Abe, C Bronner, Y Hayato, M Ikeda, K Iyogi, J Kameda, Y Kato, Y Kishimoto, L Marti, M Miura, S Moriyama, M Nakahata, Y Nakajima, Y Nakano, S Nakayama, A Orii, G Pronost, H Sekiya, M Shiozawa, Y Sonoda, A Takeda, A Takenaka, H Tanaka, S Tasaka, T Yano, R Akutsu, T Kajita, Y Nishimura, K Okumura, KM Tsui, L Labarga, P Fernandez, FDM Blaszczyk, C Kachulis, E Kearns, JL Raaf, JL Stone, LR Sulak, S Berkman, S Tobayama, J Bian, M Elnimr, WR Kropp, S Locke, S Mine, P Weatherly, MB Smy, HW Sobel, V Takhistov, KS Ganezer, J Hill, JY Kim, IT Lim, RG Park, Z Li, E O'Sullivan, K Scholberg, CW Walter, M Gonin, J Imber, TA Mueller, T Ishizuka, T Nakamura, JS Jang, K Choi, JG Learned, S Matsuno, J Amey, RP Litchfield, WY Ma, Y Uchida, MO Wascko, MG Catanesi, RA Intonti, E Radicioni, G De Rosa, A Ali, G Collazuol, L Ludovici, S Cao, M Friend, T Hasegawa, T Ishida, T Ishii, T Kobayashi, T Nakadaira, K Nakamura, Y Oyama, K Sakashita, T Sekiguchi, T Tsukamoto, K Abe, M Hasegawa, AT Suzuki, Y Takeuchi, T Hayashino, S Hirota, M Jiang, M Mori, K Nakamura, T Nakaya, RA Wendell, LHV Anthony, N McCauley, A Pritchard, Y Fukuda, Y Itow, M Murase, F Muto, P Mijakowski, K Frankiewicz, CK Jung, X Li, JL Palomino, G Santucci, C Viela, MJ Wilking, C Yanagisawa, D Fukuda, H Ishino, S Ito, A Kibayashi, Y Koshio, H Nagata, M Sakuda, C Xu, Y Kuno, D Wark, F Di Lodovico, B Richards, SM Sedgwick, R Tacik, SB Kim, A Cole, L Thompson, H Okazawa, Y Choi, K Ito, K Nishijima, M Koshiba, Y Suda, M Yokoyama, RG Calland, M Hartz, K Martens, M Murdoch, B Quilain, C Simpson, Y Suzuki, MR Vagins, D Hamabe, M Kuze, Y Okajima, T Yoshida, M Ishitsuka, JF Martin, CM Nantais, HA Tanaka, T Towstego, A Konaka, S Chen, L Wan, A Minamino, S-K Collaboration


First measurement of the nu(mu) charged-current cross section on a water target without pions in the final state

PHYSICAL REVIEW D 97 (2018) ARTN 012001

K Abe, J Amey, C Andreopoulos, M Antonova, S Aoki, A Ariga, Y Ashida, S Ban, M Barbi, GJ Barker, G Barr, C Barry, M Batkiewicz, V Berardi, S Berkman, S Bhadra, S Bienstock, A Blondel, S Bolognesi, S Bordoni, SB Boyd, D Brailsford, A Bravar, C Bronner, MB Avanzini, RG Calland, T Campbell, S Cao, SL Cartwright, MG Catanesi, A Cervera, A Chappell, C Checchia, D Cherdack, N Chikuma, G Christodoulou, J Coleman, G Collazuol, D Coplowe, A Cudd, A Dabrowska, G De Rosa, T Dealtry, PF Denner, SR Dennis, C Densham, F Di Lodovico, S Dolan, O Drapier, KE Duffy, J Dumarchez, P Dunne, S Emery-Schrenk, A Ereditato, T Feusels, AJ Finch, GA Fiorentini, M Friend, Y Fujii, D Fukuda, Y Fukuda, A Garcia, C Giganti, F Gizzarelli, T Golan, M Gonin, DR Hadley, L Haegel, JT Haigh, D Hansen, J Harada, M Hartz, T Hasegawa, NC Hastings, T Hayashino, Y Hayato, A Hillairet, T Hiraki, A Hiramoto, S Hirota, M Hogan, J Holeczek, F Hosomi, K Huang, AK Ichikawa, M Ikeda, J Imber, J Insler, RA Intonti, T Ishida, T Ishii, E Iwai, K Iwamoto, A Izmaylov, B Jamieson, M Jiang, S Johnson, P Jonsson, CK Jung, M Kabirnezhad, AC Kaboth, T Kajita, H Kakuno, J Kameda, D Karlen, T Katori, E Kearns, M Khabibullin, A Khotjantsev, H Kim, J Kim, S King, J Kisiel, A Knight, A Knox, T Kobayashi, L Koch, T Koga, PP Koller, A Konaka, LL Kormos, Y Koshio, K Kowalik, Y Kudenko, R Kurjata, T Kutter, J Lagoda, I Lamont, M Lamoureux, P Lasorak, M Laveder, M Lawe, M Licciardi, T Lindner, ZJ Liptak, RP Litchfield, X Li, A Longhin, JP Lopez, T Lou, L Ludovici, X Lu, L Magaletti, K Mahn, M Malek, S Manly, L Maret, AD Marino, JF Martin, P Martins, S Martynenko, T Maruyama, V Matveev, K Mavrokoridis, WY Ma, E Mazzucato, M McCarthy, N McCauley, KS McFarland, C McGrew, A Mefodiev, C Metelko, M Mezzetto, A Minamino, O Mineev, S Mine, A Missert, M Miura, S Moriyama, J Morrison, TA Mueller, T Nakadaira, M Nakahata, KG Nakamura, K Nakamura, KD Nakamura, Y Nakanishi, S Nakayama, T Nakaya, K Nakayoshi, C Nantais, C Nielsen, K Nishikawa, Y Nishimura, P Novella, J Nowak, HM O'Keeffe, K Okumura, T Okusawa, W Oryszczak, SM Oser, T Ovsyannikova, RA Owen, Y Oyama, V Palladino, JL Palomino, V Paolone, ND Patel, P Paudyal, M Pavin, D Payne, Y Petrov, L Pickering, ESP Guerra, C Pistillo, B Popov, M Posiadala-Zezula, J-M Poutissou, A Pritchard, P Przewlocki, B Quilain, T Radermacher, E Radicioni, PN Ratoff, MA Rayner, E Reinherz-Aronis, C Riccio, E Rondio, B Rossi, S Roth, AC Ruggeri, A Rychter, K Sakashita, F Sanchez, E Scantamburlo, K Scholberg, J Schwehr, M Scott, Y Seiya, T Sekiguchi, H Sekiya, D Sgalaberna, R Shah, A Shaikhiev, F Shaker, D Shaw, M Shiozawa, T Shirahige, M Smy, JT Sobczyk, H Sobel, J Steinmann, T Stewart, P Stowell, Y Suda, S Suvorov, A Suzuki, SY Suzuki, Y Suzuki, R Tacik, M Tada, A Takeda, Y Takeuchi, R Tamura, HK Tanaka, HA Tanaka, T Thakore, LF Thompson, S Tobayama, W Toki, T Tomura, T Tsukamoto, M Tzanov, M Vagins, Z Vallari, G Vasseur, C Vilela, T Vladisavljevic, T Wachala, CW Walter, D Wark, MO Wascko, A Weber, R Wendell, MJ Wilking, C Wilkinson, JR Wilson, RJ Wilson, C Wret, Y Yamada, K Yamamoto, C Yanagisawa, T Yano, S Yen, N Yershov, M Yokoyama, T Yuan, M Yu, A Zalewska, J Zalipska, L Zambelli, K Zaremba, M Ziembicki, ED Zimmerman, M Zito, T Collaboration


Design and performance of wide-band corrugated walls for the BICEP Array detector modules at 30/40 GHz

Proceedings of SPIE - The International Society for Optical Engineering 10708 (2018)

A Soliman, PAR Ade, Z Ahmed, RW Aikin, KD Alexander, D Barkats, SJ Benton, CA Bischoff, JJ Bock, R Bowens-Rubin, JA Brevik, I Buder, E Bullock, V Buza, J Connors, J Cornelison, BP Crill, M Crumrine, M Dierickx, L Duband, C Dvorkin, JP Filippini, S Fliescher, JA Grayson, G Hall, M Halpern, S Harrison, SR Hildebrandt, GC Hilton, H Hui, KD Irwin, JH Kang, KS Karkare, E Karpel, JP Kaufman, BG Keating, S Kefeli, SA Kernasovskiy, JM Kovac, CL Kuo, K Lau, NA Larsen, EM Leitch, M Lueker, KG Megerian, L Moncelsi, T Namikawa, CB Netterfield, HT Nguyen, RO Brient, RW Ogburn, S Palladino, C Pryke, B Racine, S Richter, R Schwarz, A Schillaci, CD Sheehy, T St Germaine, ZK Staniszewski, B Steinbach, R Sudiwala, GP Teply, KL Thompson, JE Tolan, C Tucker, AD Turner, C Umiltà, J Van Zyl, AG Vieregg, A Wandui, AC Weber, DV Wiebe, J Willmert, CL Wong, WLK Wu, E Yang, KW Yoon, C Zhang

© 2018 SPIE. BICEP Array is a degree-scale Cosmic Microwave Background (CMB) experiment that will search for primordial B-mode polarization while constraining Galactic foregrounds. BICEP Array will be comprised of four receivers to cover a broad frequency range with channels at 30/40, 95, 150 and 220/270 GHz. The first low-frequency receiver will map synchrotron emission at 30 and 40 GHz and will deploy to the South Pole at the end of 2019. In this paper, we give an overview of the BICEP Array science and instrument, with a focus on the detector module. We designed corrugations in the metal frame of the module to suppress unwanted interactions with the antenna-coupled detectors that would otherwise deform the beams of edge pixels. This design reduces the residual beam systematics and temperature-to-polarization leakage due to beam steering and shape mismatch between polarized beam pairs. We report on the simulated performance of single-and wide-band corrugations designed to minimize these effects. Our optimized design alleviates beam differential ellipticity caused by the metal frame to about 7% over 57% bandwidth (25 to 45 GHz), which is close to the level due the bare antenna itself without a metal frame. Initial laboratory measurements are also presented.


Measurement of inclusive double-differential nu(mu) charged-current cross section with improved acceptance in the T2K off-axis near detector

PHYSICAL REVIEW D 98 (2018) ARTN 012004

K Abe, J Amey, C Andreopoulos, L Anthony, M Antonova, S Aoki, A Ariga, Y Ashida, Y Azuma, S Ban, M Barbi, GJ Barker, G Barr, C Barry, M Batkiewicz, V Berardi, S Berkman, RM Berner, S Bhadra, S Bienstock, A Blondel, S Bolognesi, S Bordoni, B Bourguille, SB Boyd, D Brailsford, A Bravar, C Bronner, MB Avanzini, J Calcutt, T Campbell, S Cao, SL Cartwright, MG Catanesi, A Cervera, A Chappell, C Checchia, D Cherdack, N Chikuma, G Christodoulou, J Coleman, G Collazuol, D Coplowe, A Cudd, A Dabrowska, G De Rosa, T Dealtry, PF Denner, SR Dennis, C Densham, F Di Lodovico, S Dolan, O Drapier, KE Duffy, J Dumarchez, P Dunne, S Emery-Schrenk, A Ereditato, T Feusels, AJ Finch, GA Fiorentini, G Fiorillo, C Francois, M Friend, Y Fujii, D Fukuda, Y Fukuda, A Garcia, C Giganti, F Gizzarelli, T Golan, M Gonin, DR Hadley, L Haegel, JT Haigh, P Hamacher-Baumann, D Hansen, J Harada, M Hartz, T Hasegawa, NC Hastings, T Hayashino, Y Hayato, T Hiraki, A Hiramoto, S Hirota, M Hogan, J Holeczek, F Hosomi, AK Ichikawa, M Ikeda, J Imber, T Inoue, RA Intonti, T Ishida, T Ishii, K Iwamoto, A Izmaylov, B Jamieson, M Jiang, S Johnson, P Jonsson, CK Jung, M Kabirnezhad, AC Kaboth, T Kajita, H Kakuno, J Kameda, D Karlen, T Katori, E Kearns, M Khabibullin, A Khotjantsev, H Kim, J Kim, S King, J Kisiel, A Knight, A Knox, T Kobayashi, L Koch, T Koga, PP Koller, A Konaka, LL Kormos, Y Koshio, K Kowalik, Y Kudenko, R Kurjata, T Kutter, L Labarga, J Lagoda, I Lamont, M Lamoureux, P Lasorak, M Laveder, M Lawe, M Licciardi, T Lindner, ZJ Liptak, RP Litchfield, X Li, A Longhin, JP Lopez, T Lou, L Ludovici, X Lu, L Magaletti, K Mahn, M Malek, S Manly, L Maret, AD Marino, JF Martin, P Martins, S Martynenko, T Maruyama, V Matveev, K Mavrokoridis, WY Ma, E Mazzucato, M McCarthy, N McCauley, KS McFarland, C McGrew, A Mefodiev, C Metelko, M Mezzetto, A Minamino, O Mineev, S Mine, A Missert, M Miura, S Moriyama, J Morrison, TA Mueller, Y Nagai, T Nakadaira, M Nakahata, KG Nakamura, K Nakamura, KD Nakamura, Y Nakanishi, S Nakayama, T Nakaya, K Nakayoshi, C Nantais, C Nielsen, K Niewczas, K Nishikawa, Y Nishimura, P Novella, J Nowak, HM O'Keeffe, K Okumura, T Okusawa, W Oryszczak, SM Oser, T Ovsyannikova, RA Owen, Y Oyama, V Palladino, JL Palomino, V Paolone, P Paudyal, M Pavin, D Payne, Y Petrov, L Pickering, ESP Guerra, C Pistillo, B Popov, M Posiadala-Zezula, A Pritchard, P Przewlocki, B Quilain, T Radermacher, E Radicioni, PN Ratoff, MA Rayner, E Reinherz-Aronis, C Riccio, E Rondio, B Rossi, S Roth, AC Ruggeri, A Rychter, K Sakashita, F Sanchez, S Sasaki, E Scantamburlo, K Scholberg, J Schwehr, M Scott, Y Seiya, T Sekiguchi, H Sekiya, D Sgalaberna, R Shah, A Shaikhiev, F Shaker, D Shaw, M Shiozawa, A Smirnov, M Smy, JT Sobczyk, H Sobel, J Steinmann, T Stewart, P Stowell, Y Suda, S Suvorov, A Suzuki, SY Suzuki, Y Suzuki, R Tacik, M Tada, A Takeda, Y Takeuchi, R Tamura, HK Tanaka, HA Tanaka, T Thakore, LF Thompson, S Tobayama, W Toki, T Tsukamoto, M Tzanov, W Uno, M Vagins, Z Vallari, G Vasseur, C Vilela, T Vladisavljevic, T Wachala, J Walker, CW Walter, Y Wang, D Wark, MO Wascko, A Weber, R Wendell, MJ Wilking, C Wilkinson, JR Wilson, RJ Wilson, C Wret, Y Yamada, K Yamamoto, S Yamasu, C Yanagisawa, T Yano, S Yen, N Yershov, M Yokoyama, M Yu, A Zalewska, J Zalipska, L Zambelli, K Zaremba, M Ziembicki, ED Zimmerman, M Zito, A Zykova, T Collaboration


BICEP Array: A multi-frequency degree-scale CMB polarimeter

Proceedings of SPIE - The International Society for Optical Engineering 10708 (2018)

H Hui, PAR Ade, Z Ahmed, RW Aikin, KD Alexander, D Barkats, SJ Benton, CA Bischoff, JJ Bock, R Bowens-Rubin, JA Brevik, I Buder, E Bullock, V Buza, J Connors, J Cornelison, BP Crill, M Crumrine, M Dierickx, L Duband, C Dvorkin, JP Filippini, S Fliescher, J Grayson, G Hall, M Halpern, S Harrison, SR Hildebrandt, GC Hilton, KD Irwin, J Kang, KS Karkare, E Karpel, JP Kaufman, BG Keating, S Kefeli, SA Kernasovskiy, JM Kovac, CL Kuo, K Lau, NA Larsen, EM Leitch, M Lueker, KG Megerian, L Moncelsi, T Namikawa, CB Netterfield, HT Nguyen, R O'Brient, RW Ogburn, S Palladino, C Pryke, B Racine, S Richter, R Schwarz, A Schillaci, CD Sheehy, A Soliman, T St Germaine, ZK Staniszewski, B Steinbach, RV Sudiwala, GP Teply, KL Thompson, JE Tolan, C Tucker, AD Turner, C Umiltà, AG Vieregg, A Wandui, AC Weber, DV Wiebe, J Willmert, CL Wong, WLK Wu, E Yang, KW Yoon, C Zhang

© 2018 SPIE. Bicep Array is the newest multi-frequency instrument in the Bicep/Keck Array program. It is comprised of four 550mm aperture refractive telescopes observing the polarization of the cosmic microwave background (CMB) at 30/40, 95, 150 and 220/270 GHz with over 30,000 detectors. We present an overview of the receiver, detailing the optics, thermal, mechanical, and magnetic shielding design. Bicep Array follows Bicep3's modular focal plane concept, and upgrades to 6» wafer to reduce fabrication with higher detector count per module. The first receiver at 30/40GHz is expected to start observing at the South Pole during the 2019-20 season. By the end of the planned Bicep Array program, we project 0.002σ(r)0.006, assuming current modeling of polarized Galactic foreground and depending on the level of delensing that can be achieved with higher resolution maps from the South Pole Telescope.


2017 upgrade and performance of BICEP3: A 95GHz refracting telescope for degree-scale CMB polarization

Proceedings of SPIE - The International Society for Optical Engineering 10708 (2018)

JH Kang, PAR Ade, Z Ahmed, RW Aikin, KD Alexander, D Barkats, SJ Benton, CA Bischoff, JJ Bock, H Boenish, R Bowens-Rubin, JA Brevik, I Buder, E Bullock, V Buza, J Connors, J Cornelison, BP Crill, M Crumrine, M Dierickx, L Duband, C Dvorkin, JP Filippini, S Fliescher, JA Grayson, G Hall, M Halpern, S Harrison, SR Hildebrandt, GC Hilton, H Hui, KD Irwin, KS Karkare, E Karpel, JP Kaufman, BG Keating, S Kefeli, SA Kernasovskiy, JM Kovac, CL Kuo, NA Larsen, K Lau, EM Leitch, M Lueker, KG Megerian, L Moncelsi, T Namikawa, B Netterfield, HT Nguyen, R O'Brient, RW Ogburn, S Palladino, C Pryke, B Racine, S Richter, A Schillaci, R Schwarz, CD Sheehy, A Soliman, T St Germaine, ZK Staniszewski, B Steinbach, RV Sudiwala, GP Teply, KL Thompson, JE Tolan, C Tucker, AD Turner, C Umiltà, AG Vieregg, A Wandui, AC Weber, DV Wiebe, J Willmert, CL Wong, WLK Wu, H Yang, KW Yoon, C Zhang

© 2018 SPIE. BICEP3 is a 520mm aperture on-axis refracting telescope observing the polarization of the cosmic microwave background (CMB) at 95GHz in search of the B-mode signal originating from in ationary gravitational waves. BICEP3's focal plane is populated with modularized tiles of antenna-coupled transition edge sensor (TES) bolometers. BICEP3 was deployed to the South Pole during 2014-15 austral summer and has been operational since. During the 2016-17 austral summer, we implemented changes to optical elements that lead to better noise performance. We discuss this upgrade and show the performance of BICEP3 at its full mapping speed from the 2017 and 2018 observing seasons. BICEP3 achieves an order-of-magnitude improvement in mapping speed compared to a Keck 95GHz receiver. We demonstrate 6.6μK√s noise performance of the BICEP3 receiver.


Ultra-thin large-aperture vacuum windows for millimeter wavelengths receivers

Proceedings of SPIE - The International Society for Optical Engineering 10708 (2018)

D Barkats, MI Dierickx, JM Kovac, C Pentacoff, PAR Ade, Z Ahmed, RW Aikin, KD Alexander, SJ Benton, CA Bischoff, JJ Bock, R Bowens-Rubin, JA Brevik, I Buder, E Bullock, V Buza, J Connors, J Cornelison, BP Crill, M Crumrine, L Duband, C Dvorkin, JP Filippini, S Fliescher, JA Grayson, G Hall, M Halpern, SA Harrison, SR Hildebrandt, GC Hilton, H Hui, KD Irwin, J Kang, KS Karkare, E Karpel, JP Kaufman, BG Keating, S Kefeli, SA Kernasovskiy, CL Kuo, K Lau, NA Larsen, EM Leitch, M Lueker, KG Megerian, L Moncelsi, T Namikawa, HT Nguyen, R O'Brient, RW Ogburn, S Palladino, C Pryke, B Racine, S Richter, R Schwarz, A Schillaci, CD Sheehy, A Soliman, T St Germaine, ZK Staniszewski, B Steinbach, RV Sudiwala, GP Teply, KL Thompson, JE Tolan, C Tucker, AD Turner, C Umiltà, AG Vieregg, A Wandui, AC Weber, DV Wiebe, J Willmert, CL Wong, WLK Wu, H Yang, KW Yoon, C Zhang

© 2018 SPIE. Targeting faint polarization patterns arising from Primordial Gravitational Waves in the Cosmic Microwave Background requires excellent observational sensitivity. Optical elements in small aperture experiments such as Bicep3 and Keck Array are designed to optimize throughput and minimize losses from transmission, reflection and scattering at millimeter wavelengths. As aperture size increases, cryostat vacuum windows must withstand larger forces from atmospheric pressure and the solution has often led to a thicker window at the expense of larger transmission loss. We have identified a new candidate material for the fabrication of vacuum windows: with a tensile strength two orders of magnitude larger than previously used materials, woven high-modulus polyethylene could allow for dramatically thinner windows, and therefore significantly reduced losses and higher sensitivity. In these proceedings we investigate the suitability of high-modulus polyethylene windows for ground-based CMB experiments, such as current and future receivers in the Bicep/Keck Array program. This includes characterizing their optical transmission as well as their mechanical behavior under atmospheric pressure. We find that such ultra-thin materials are promising candidates to improve the performance of large-aperture instruments at millimeter wavelengths, and outline a plan for further tests ahead of a possible upcoming field deployment of such a science-grade window.


BICEP Array cryostat and mount design

Proceedings of SPIE - The International Society for Optical Engineering 10708 (2018)

M Crumrine, PAR Ade, Z Ahmed, RW Aikin, KD Alexander, D Barkats, SJ Benton, CA Bischoff, JJ Bock, R Bowens-Rubin, JA Brevik, I Buder, E Bullock, V Buza, J Connors, J Cornelison, BP Crill, M Dierickx, L Duband, C Dvorkin, JP Filippini, S Fliescher, JA Grayson, G Hall, M Halpern, SA Harrison, SR Hildebrandt, GC Hilton, H Hui, KD Irwin, JH Kang, KS Karkare, E Karpel, JP Kaufman, BG Keating, S Kefeli, SA Kernasovskiy, JM Kovac, CL Kuo, NA Larsen, K Lau, EM Leitch, MV Lueker, KG Megerian, L Moncelsi, T Namikawa, CB Netterfield, HT Nguyen, R O'Brient, RW Ogburn, S Palladino, C Pryke, B Racine, S Richter, R Schwarz, A Schillaci, CD Sheehy, A Soliman, T St Germaine, ZK Staniszewski, B Steinbach, RV Sudiwala, GP Teply, KL Thompson, JE Tolan, CE Tucker, AD Turner, C Umiltà, AG Vieregg, A Wandui, AC Weber, DV Wiebe, J Willmert, CL Wong, WLK Wu, E Yang, KW Yoon, C Zhang

© 2018 SPIE. Bicep Array is a cosmic microwave background (CMB) polarization experiment that will begin observing at the South Pole in early 2019. This experiment replaces the five Bicep2 style receivers that compose the Keck Array with four larger Bicep3 style receivers observing at six frequencies from 30 to 270GHz. The 95GHz and 150GHz receivers will continue to push the already deep Bicep/Keck CMB maps while the 30/40GHz and 220/270GHz receivers will constrain the synchrotron and galactic dust foregrounds respectively. Here we report on the design and performance of the Bicep Array instruments focusing on the mount and cryostat systems.


The Pandora multi-algorithm approach to automated pattern recognition of cosmic-ray muon and neutrino events in the MicroBooNE detector

EUROPEAN PHYSICAL JOURNAL C 78 (2018) ARTN 82

R Acciarri, C Adams, R An, J Anthony, J Asaadi, M Auger, L Bagby, S Balasubramanian, B Baller, C Barnes, G Barr, M Bass, F Bay, M Bishai, A Blake, T Bolton, L Camilleri, D Caratelli, B Carls, RC Fernandez, F Cavanna, H Chen, E Church, D Cianci, E Cohen, GH Collin, JM Conrad, M Convery, JI Crespo-Anadon, M Del Tutto, D Devitt, S Dytman, B Eberly, A Ereditato, LE Sanchez, J Esquivel, AA Fadeeva, BT Fleming, W Foreman, AP Furmanski, D Garcia-Gamez, GT Garvey, V Genty, D Goeldi, S Gollapinni, N Graf, E Gramellini, H Greenlee, R Grosso, R Guenette, A Hackenburg, P Hamilton, O Hen, J Hewes, C Hill, J Ho, G Horton-Smith, A Hourlier, E-C Huang, C James, JJ de Vries, C-M Jen, L Jiang, RA Johnson, J Joshi, H Jostlein, D Kaleko, G Karagiorgi, W Ketchum, B Kirby, M Kirby, T Kobilarcik, I Kreslo, A Laube, Y Li, A Lister, BR Littlejohn, S Lockwitz, D Lorca, WC Louis, M Luethi, B Lundberg, X Luo, A Marchionni, C Mariani, J Marshall, DAM Caicedo, V Meddage, T Miceli, GB Mills, J Moon, M Mooney, CD Moore, J Mousseau, R Murrells, D Naples, P Nienaber, J Nowak, O Palamara, V Paolone, V Papavassiliou, SF Pate, Z Pavlovic, E Piasetzky, D Porzio, G Pulliam, X Qian, JL Raaf, A Rafique, L Rochester, R von Rohr, B Russell, DW Schmitz, A Schukraft, W Seligman, MH Shaevitz, J Sinclair, A Smith, EL Snider, M Soderberg, S Soldner-Rembold, SR Soleti, P Spentzouris, J Spitz, J St John, T Strauss, AM Szelc, N Tagg, K Terao, M Thomson, M Toups, Y-T Tsai, S Tufanli, T Usher, W Van De Pontseele, RG Van de Water, B Viren, M Weber, DA Wickremasinghe, S Wolbers, T Wongjirad, K Woodruff, T Yang, L Yates, GP Zeller, J Zennamo, C Zhang


Measurement of Final-State Correlations in Neutrino Muon-Proton Mesonless Production on Hydrocarbon at < E-v >=3 GeV

PHYSICAL REVIEW LETTERS 121 (2018) ARTN 022504

X-G Lu, M Betancourt, T Walton, F Akbar, L Aliaga, O Altinok, DA Andrade, M Ascencio, L Bellantoni, A Bercellie, A Bodek, A Bravar, H Budd, T Cai, MF Carneiro, J Chaves, D Coplowe, H da Motta, SA Dytman, GA Diaz, J Felix, L Fields, R Fine, AM Gago, R Galindo, H Gallagher, A Ghosh, R Gran, DA Harris, S Henry, S Jena, D Jena, J Kleykamp, M Kordosky, T Le, E Maher, S Manly, WA Mann, CM Marshall, KS McFarland, AM McGowan, B Messerly, J Miller, A Mislivec, JG Morfin, J Mousseau, D Naples, JK Nelson, C Nguyen, A Norrick, Nuruzzaman, A Olivier, V Paolone, CE Patrick, GN Perdue, MA Ramirez, RD Ransome, L Ren, D Rimal, PA Rodrigues, D Ruterbories, H Schellman, JT Sobczyk, CJ Solano Salinas, H Su, M Sultana, E Valencia, D Wark, A Weber, J Wolcott, M Wospakrik, B Yaeggy, M Collaboration


Physics potentials with the second Hyper-Kamiokande detector in Korea

PROGRESS OF THEORETICAL AND EXPERIMENTAL PHYSICS (2018) ARTN 063C01

K Abe, K Abe, SH Ahn, H Aihara, A Aimi, R Akutsu, C Andreopoulos, I Anghel, LHV Anthony, M Antonova, Y Ashida, V Aushev, M Barbi, GJ Barker, G Barr, P Beltrame, V Berardi, M Bergevin, S Berkman, L Berns, T Berry, S Bhadra, FDM Blaszczyk, A Blondel, S Bolognesi, SB Boyd, A Bravar, C Bronner, MB Avanzini, FS Cafagna, R Calland, S Cao, SL Cartwright, MG Catanesi, C Checchia, Z Chen-Wishart, BG Cheon, MK Cheoun, K Cho, JH Choi, K Choi, KY Choi, EJ Chun, A Cole, J Coleman, G Collazuol, G Cowan, L Cremonesi, T Dealtry, G De Rosa, C Densham, D Dewhurst, E Drakopoulou, F Di Lodovico, O Drapier, J Dumarchez, P Dunne, M Dziewiecki, S Emery, A Esmaili, A Evangelisti, E Fernandez-Martinez, T Feusels, A Finch, GA Fiorentini, G Fiorillo, M Fitton, K Frankiewicz, M Friend, Y Fujii, Y Fukuda, D Fukuda, K Ganezer, M Ghosh, C Giganti, M Gonin, N Grant, P Gumplinger, DR Hadley, B Hartfiel, M Hartz, Y Hayato, K Hayrapetyan, J Hill, S Hirota, S Horiuchi, AK Ichikawa, T Iijima, M Ikeda, J Imber, K Inoue, J Insler, RA Intonti, A Ioannisian, T Ishida, H Ishino, M Ishitsuka, Y Itow, K Iwamoto, A Izmaylov, B Jamieson, HI Jang, JS Jang, SH Jeon, KS Jeong, M Jiang, P Jonsson, KK Joo, A Kaboth, C Kachulis, T Kajita, SK Kang, J Kameda, Y Kataoka, T Katori, K Kayrapetyan, E Kearns, M Khabibullin, A Khotjantsev, CS Kim, HB Kim, HJ Kim, JH Kim, J-S Kim, JY Kim, SB Kim, SC Kim, S-W Kim, SY Kim, TJ Kim, W Kim, S King, Y Kishimoto, P Ko, T Kobayashi, M Koga, A Konaka, LL Kormos, Y Koshio, A Korzenev, KL Kowalik, WR Kropp, Y Kudenko, R Kurjata, T Kutter, M Kuze, K Kwak, EH Kwon, L Labarga, J Lagoda, PJJ Lasorak, M Laveder, M Lawe, JG Learned, CH Lee, SJ Lee, WJ Lee, IT Lim, T Lindner, RP Litchfield, A Longhin, P Loverre, T Lou, L Ludovici, W Ma, L Magaletti, K Mahn, M Malek, L Maret, C Mariani, K Martens, L Marti, JF Martin, J Marzec, S Matsuno, E Mazzucato, M McCarthy, N McCauley, KS McFarland, C McGrew, A Mefodiev, P Mermod, C Metelko, M Mezzetto, J Migenda, P Mijakowski, H Minakata, A Minamino, S Mine, O Mineev, A Mitra, M Miura, T Mochizuki, J Monroe, CS Moon, DH Moon, S Moriyama, T Mueller, F Muheim, K Murase, F Muto, M Nakahata, Y Nakajima, K Nakamura, T Nakaya, S Nakayama, C Nantais, M Needham, T Nicholls, Y Nishimura, E Noah, F Nova, J Nowak, H Nunokawa, Y Obayashi, YD Oh, Y Oh, HM O'Keeffe, Y Okajima, K Okumura, Y Onishchuk, E O'Sullivan, L O'Sullivan, T Ovsiannikova, RA Owen, Y Oyama, J Perez, MY Pac, V Palladino, JL Palomino, V Paolone, HS Park, JC Park, MG Park, SC Park, W Parker, S Parsa, D Payne, JD Perkin, C Pidcott, EP Guerra, S Playfer, B Popov, M Posiadala-Zezula, J-M Poutissou, A Pritchard, NW Prouse, G Pronost, P Przewlocki, B Quilain, M Quinto, E Radicioni, PN Ratoff, F Retiere, C Riccio, B Richards, E Rondio, HJ Rose, C Rott, SD Rountree, AC Ruggeri, A Rychter, D Ryu, R Sacco, M Sakuda, MC Sanchez, E Scantamburlo, M Scott, SM Sedgwick, Y Seiya, T Sekiguchi, H Sekiya, H Seo, SH Seo, D Sgalaberna, R Shah, A Shaikhiev, I Shimizu, M Shiozawa, Y Shitov, S Short, C Simpson, G Sinnis, MB Smy, S Snow, J Sobczyk, HW Sobel, DC Son, Y Sonoda, R Spina, T Stewart, JL Stone, Y Suda, Y Suwa, Y Suzuki, AT Suzuki, R Svoboda, M Taani, R Tacik, A Takeda, A Takenaka, A Taketa, Y Takeuchi, V Takhistov, HA Tanaka, HKM Tanaka, H Tanaka, R Terri, M Thiesse, LF Thompson, M Thorpe, S Tobayama, C Touramanis, T Towstego, T Tsukamoto, KM Tsui, M Tzanov, Y Uchida, MR Vagins, G Vasseur, C Vilela, RB Vogelaar, J Walding, J Walker, M Ward, D Wark, MO Wascko, A Weber, R Wendell, RJ Wilkes, MJ Wilking, JR Wilson, E Won, T Xin, K Yamamoto, C Yanagisawa, T Yano, O Yasuda, S Yen, N Yershov, DN Yeum, M Yokoyama, HD Yoo, J Yoo, SC Yoon, TS Yoon, T Yoshida, I Yu, M Yu, J Zalipska, K Zaremba, M Ziembicki, M Zito, S Zsoldos


Characterization of nuclear effects in muon-neutrino scattering on hydrocarbon with a measurement of final-state kinematics and correlations in charged-current pionless interactions at T2K

PHYSICAL REVIEW D 98 (2018) ARTN 032003

K Abe, J Amey, C Andreopoulos, L Anthony, M Antonova, S Aoki, A Ariga, Y Ashida, Y Azuma, S Ban, M Barbi, GJ Barker, G Barr, C Barry, M Batkiewicz, V Berardi, S Berkman, RM Berner, L Berns, S Bhadra, S Bienstock, A Blondel, S Bolognesi, S Bordoni, B Bourguille, SB Boyd, D Brailsford, A Bravar, C Bronner, MB Avanzini, J Calcutt, T Campbell, S Cao, SL Cartwright, MG Catanesi, A Cervera, A Chappell, C Checchia, D Cherdack, N Chikuma, G Christodoulou, J Coleman, G Collazuol, D Coplowe, A Cudd, A Dabrowska, G De Rosa, T Dealtry, PF Denner, SR Dennis, C Densham, F Di Lodovico, S Dolan, O Drapier, KE Duffy, J Dumarchez, P Dunne, S Emery-Schrenk, A Ereditato, T Feusels, AJ Finch, GA Fiorentini, G Fiorillo, C Francois, M Friend, Y Fujii, D Fukuda, Y Fukuda, A Garcia, C Giganti, F Gizzarelli, T Golan, M Gonin, DR Hadley, L Haegel, JT Haigh, P Hamacher-Baumann, D Hansen, J Harada, M Hartz, T Hasegawa, NC Hastings, T Hayashino, Y Hayato, T Hiraki, A Hiramoto, S Hirota, M Hogan, J Holeczek, F Hosomi, AK Ichikawa, M Ikeda, J Imber, T Inoue, RA Intonti, T Ishida, T Ishii, K Iwamoto, A Izmaylov, B Jamieson, M Jiang, S Johnson, P Jonsson, CK Jung, M Kabirnezhad, AC Kaboth, T Kajita, H Kakuno, J Kameda, D Karlen, T Katori, E Kearns, M Khabibullin, A Khotjantsev, H Kim, J Kim, S King, J Kisiel, A Knight, A Knox, T Kobayashi, L Koch, T Koga, PP Koller, A Konaka, LL Kormos, Y Koshio, K Kowalik, Y Kudenko, R Kurjata, T Kutter, L Labarga, J Lagoda, I Lamont, M Lamoureux, P Lasorak, M Laveder, M Lawe, M Licciardi, T Lindner, ZJ Liptak, RP Litchfield, X Li, A Longhin, JP Lopez, T Lou, L Ludovici, X Lu, L Magaletti, K Mahn, M Malek, S Manly, L Maret, AD Marino, JF Martin, P Martins, S Martynenko, T Maruyama, V Matveev, K Mavrokoridis, WY Ma, E Mazzucato, M McCarthy, N McCauley, KS McFarland, C McGrew, A Mefodiev, C Metelko, M Mezzetto, A Minamino, O Mineev, S Mine, A Missert, M Miura, S Moriyama, J Morrison, TA Mueller, Y Nagai, T Nakadaira, M Nakahata, KG Nakamura, K Nakamura, KD Nakamura, Y Nakanishi, S Nakayama, T Nakaya, K Nakayoshi, C Nantais, C Nielsen, K Niewczas, K Nishikawa, Y Nishimura, P Novella, J Nowak, HM O'Keeffe, K Okumura, T Okusawa, W Oryszczak, SM Oser, T Ovsyannikova, RA Owen, Y Oyama, V Palladino, JL Palomino, V Paolone, P Paudyal, M Pavin, D Payne, Y Petrov, L Pickering, ESP Guerra, C Pistillo, B Popov, M Posiadala-Zezula, A Pritchard, P Przewlocki, B Quilain, T Radermacher, E Radicioni, PN Ratoff, MA Rayner, E Reinherz-Aronis, C Riccio, E Rondio, B Rossi, S Roth, A Ruggeri, A Rychter, K Sakashita, F Sanchez, S Sasaki, E Scantamburlo, K Scholberg, J Schwehr, M Scott, Y Seiya, T Sekiguchi, H Sekiya, D Sgalaberna, R Shah, A Shaikhiev, F Shaker, D Shaw, M Shiozawa, A Smirnov, M Smy, JT Sobczyk, H Sobel, J Steinmann, T Stewart, P Stowell, Y Suda, S Suvorov, A Suzuki, SY Suzuki, Y Suzuki, R Tacik, M Tada, A Takeda, Y Takeuchi, R Tamura, HK Tanaka, HA Tanaka, T Thakore, LF Thompson, W Toki, T Tsukamoto, M Tzanov, W Uno, M Vagins, Z Vallari, G Vasseur, C Vilela, T Vladisavljevic, T Wachala, J Walker, CW Walter, Y Wang, D Wark, MO Wascko, A Weber, R Wendell, MJ Wilking, C Wilkinson, JR Wilson, RJ Wilson, C Wret, Y Yamada, K Yamamoto, S Yamasu, C Yanagisawa, T Yano, S Yen, N Yershov, M Yokoyama, M Yu, A Zalewska, J Zalipska, L Zambelli, K Zaremba, M Ziembicki, ED Zimmerman, M Zito, S Zsoldos, A Zykova, T Collaboration


Measurement of the single pi(0) production rate in neutral current neutrino interactions on water

PHYSICAL REVIEW D 97 (2018) ARTN 032002

K Abe, J Amey, C Andreopoulos, M Antonova, S Aoki, A Ariga, Y Ashida, S Assylbekov, D Autiero, S Ban, M Barbi, GJ Barker, G Barr, C Barry, P Bartet-Friburg, M Batkiewicz, V Berardi, S Berkman, S Bhadra, S Bienstock, A Blondel, S Bolognesi, S Bordoni, SB Boyd, D Brailsford, A Bravar, C Bronner, MB Avanzini, RG Calland, T Campbell, S Cao, SL Cartwright, R Castillo, MG Catanesi, A Cervera, A Chappell, C Checchia, D Cherdack, N Chikuma, G Christodoulou, A Clifton, J Coleman, G Collazuol, D Coplowe, L Cremonesi, A Cudd, A Dabrowska, G De Rosa, T Dealtry, PF Denner, SR Dennis, C Densham, D Dewhurst, F Di Lodovico, S Di Luise, S Dolan, O Drapier, KE Duffy, J Dumarchez, M Dunkman, P Dunne, M Dziewiecki, S Emery-Schrenk, A Ereditato, T Feusels, AJ Finch, GA Fiorentini, M Friend, Y Fujii, D Fukuda, Y Fukuda, AP Furmanski, V Galymov, A Garcia, SG Giffin, C Giganti, K Gilje, F Gizzarelli, T Golan, M Gonin, N Grant, DR Hadley, L Haegel, JT Haigh, P Hamilton, D Hansen, J Harada, T Hara, M Hartz, T Hasegawa, NC Hastings, T Hayashino, Y Hayato, RL Helmer, M Hierholzer, A Hillairet, A Himmel, T Hiraki, A Hiramoto, S Hirota, M Hogan, J Holeczek, F Hosomi, K Huang, AK Ichikawa, K Ieki, M Ikeda, J Imber, J Insler, RA Intonti, TJ Irvine, T Ishida, T Ishii, E Iwai, K Iwamoto, A Izmaylov, A Jacob, B Jamieson, M Jiang, S Johnson, JH Jo, P Jonsson, CK Jung, M Kabirnezhad, AC Kaboth, T Kajita, H Kakuno, J Kameda, D Karlen, I Karpikov, T Katori, E Kearns, M Khabibullin, A Khotjantsev, D Kielczewska, T Kikawa, H Kim, J Kim, S King, J Kisiel, A Knight, A Knox, T Kobayashi, L Koch, T Koga, PP Koller, A Konaka, K Kondo, A Kopylov, LL Kormos, A Korzenev, Y Koshio, K Kowalik, W Kropp, Y Kudenko, R Kurjata, T Kutter, J Lagoda, I Lamont, M Lamoureux, E Larkin, P Lasorak, M Laveder, M Lawe, M Lazos, M Licciardi, T Lindner, ZJ Liptak, RP Litchfield, X Li, A Longhin, JP Lopez, T Lou, L Ludovici, X Lu, L Magaletti, K Mahn, M Malek, S Manly, L Maret, AD Marino, J Marteau, JF Martin, P Martins, S Martynenko, T Maruyama, V Matveev, K Mavrokoridis, WY Ma, E Mazzucato, M McCarthy, N McCauley, KS McFarland, C McGrew, A Mefodiev, C Metelko, M Mezzetto, P Mijakowski, A Minamino, O Mineev, S Mine, A Missert, M Miura, S Moriyama, J Morrison, TA Mueller, S Murphy, J Myslik, T Nakadaira, M Nakahata, KG Nakamura, K Nakamura, KD Nakamura, Y Nakanishi, S Nakayama, T Nakaya, K Nakayoshi, C Nantais, C Nielsen, M Nirkko, K Nishikawa, Y Nishimura, P Novella, J Nowak, HM O'Keeffe, R Ohta, K Okumura, T Okusawa, W Oryszczak, SM Oser, T Ovsyannikova, RA Owen, Y Oyama, V Palladino, JL Palomino, V Paolone, ND Patel, P Paudyal, M Pavin, D Payne, JD Perkin, Y Petrov, L Pickard, L Pickering, ESP Guerra, C Pistillo, B Popov, M Posiadala-Zezula, J-M Poutissou, R Poutissou, A Pritchard, P Przewlocki, B Quilain, T Radermacher, E Radicioni, PN Ratoff, M Ravonel, MA Rayner, A Redij, E Reinherz-Aronis, C Riccio, P Rojas, E Rondio, B Rossi, S Roth, A Rubbia, AC Ruggeri, A Rychter, R Sacco, K Sakashita, F Sanchez, F Sato, E Scantamburlo, K Scholberg, J Schwehr, M Scott, Y Seiya, T Sekiguchi, H Sekiya, D Sgalaberna, R Shah, A Shaikhiev, F Shaker, D Shaw, M Shiozawa, T Shirahige, S Short, M Smy, JT Sobczyk, H Sobel, M Sorel, L Southwell, P Stamoulis, J Steinmann, T Stewart, P Stowell, Y Suda, S Suvorov, A Suzuki, K Suzuki, SY Suzuki, Y Suzuki, R Tacik, M Tada, S Takahashi, A Takeda, Y Takeuchi, R Tamura, HK Tanaka, HA Tanaka, D Terhorst, R Terri, T Thakore, LF Thompson, S Tobayama, W Toki, T Tomura, C Touramanis, T Tsukamoto, M Tzanov, Y Uchida, A Vacheret, M Vagins, Z Vallari, G Vasseur, C Vilela, T Vladisavljevic, T Wachala, K Wakamatsu, CW Walter, D Wark, W Warzycha, MO Wascko, A Weber, R Wendell, RJ Wilkes, MJ Wilking, C Wilkinson, JR Wilson, RJ Wilson, C Wret, Y Yamada, K Yamamoto, M Yamamoto, C Yanagisawa, T Yano, S Yen, N Yershov, M Yokoyama, J Yoo, K Yoshida, T Yuan, M Yu, A Zalewska, J Zalipska, L Zambelli, K Zaremba, M Ziembicki, ED Zimmerman, M Zito, J Zmuda, T Collaboration

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