Showing papers by "Tsuyoshi Nakaya published in 2022"
TL;DR: The application of gwpcorMapper is demonstrated by using it to investigate census data to find meaningful relationships that describe the work-life environment in the 23 special wards of Tokyo, Japan.
6 citations
TL;DR: In this paper , a search for cosmic-ray boosted dark matter with hadrons using directional information was conducted using the Super-Kamiokande experiment during the 1996-2018 period (SKI-IV phase).
Abstract: We report a search for cosmic-ray boosted dark matter with protons using the 0.37 megaton×years data collected at Super-Kamiokande experiment during the 1996-2018 period (SKI-IV phase). We searched for an excess of proton recoils above the atmospheric neutrino background from the vicinity of the Galactic Center. No such excess is observed, and limits are calculated for two reference models of dark matter with either a constant interaction cross section or through a scalar mediator. This is the first experimental search for boosted dark matter with hadrons using directional information. The results present the most stringent limits on cosmic-ray boosted dark matter and exclude the dark matter-nucleon elastic scattering cross section between 10^{-33}cm^{2} and 10^{-27}cm^{2} for dark matter mass from 1 MeV/c^{2} to 300 MeV/c^{2}.
4 citations
TL;DR: In this article , the authors focus on detecting more distant supernovae whose event rate may be too small to trigger in real time, but may be identified using an offline approach.
Abstract: Super-Kamiokande has been searching for neutrino bursts characteristic of core-collapse supernovae continuously, in real time, since the start of operations in 1996. The present work focuses on detecting more distant supernovae whose event rate may be too small to trigger in real time, but may be identified using an offline approach. The analysis of data collected from 2008 to 2018 found no evidence of distant supernovae bursts. This establishes an upper limit of 0.29 yr−1 on the rate of core-collapse supernovae out to 100 kpc at 90% C.L. For supernovae that fail to explode and collapse directly to black holes the limit reaches to 300 kpc.
2 citations
22 Mar 2022
TL;DR: In this article , the authors present a survey of the state-of-the-art research work in the area of artificial neural networks and propose a set of guidelines for how to use them.
Abstract: P. Weatherly, K. Abe, 49 C. Bronner, Y. Hayato, 49 K. Hiraide, 49 M. Ikeda, 49 K. Iyogi, J. Kameda, 49 Y. Kanemura, Y. Kataoka, 49 Y. Kato, Y. Kishimoto, 49 S. Miki, M. Miura, 49 S. Moriyama, 49 T. Mochizuki, M. Nakahata, 49 Y. Nakano, S. Nakayama, 49 T. Okada, K. Okamoto, A. Orii, G. Pronost, K. Sato, H. Sekiya, 49 M. Shiozawa, 49 Y. Sonoda, Y. Suzuki, A. Takeda, 49 Y. Takemoto, 49 A. Takenaka, H. Tanaka, 49 S. Tasaka, X. Wang, S. Watanabe, T. Yano, S. Han, T. Kajita, 49 K. Kaneyuki, K. Okumura, 49 T. Tashiro, R. Wang, J. Xia, G. D. Megias, L. Labarga, B. Zaldivar, B. W. Pointon, 53 F. d. M. Blaszczyk, C. Kachulis, E. Kearns, 49 J. L. Raaf, J. L. Stone, 49 L. R. Sulak, S. Sussman, L. Wan, T. Wester, S. Berkman, S. Tobayama, J. Bian, M. Elnimr, N. J. Griskevich, W. R. Kropp, ∗ S. Locke, S. Mine, M. B. Smy, 49 H. W. Sobel, 49 V. Takhistov, 49 A. Yankelevich, K. S. Ganezer, ∗ J. Hill, J. Y. Kim, I. T. Lim, R. G. Park, B. Bodur, Z. Li, K. Scholberg, 49 C. W. Walter, 49 L. Bernard, A. Coffani, O. Drapier, A. Giampaolo, S. El Hedri, J. Imber, Th. A. Mueller, P. Paganini, B. Quilain, 49 A. D. Santos, T. Ishizuka, T. Nakamura, J. S. Jang, J. G. Learned, S. Matsuno, S. Cao, J. Amey, L. H. V. Anthony, R. P. Litchfield, W. Y. Ma, D. Martin, M. Scott, A. A. Sztuc, Y. Uchida, M. O. Wascko, V. Berardi, M. G. Catanesi, R. A. Intonti, E. Radicioni, N. F. Calabria, L. N. Machado, G. De Rosa, G. Collazuol, F. Iacob, M. Lamoureux, M. Mattiazzi, N. Ospina, L. Ludovici, M. Gonin, Y. Maekawa, Y. Nishimura, M. Friend, T. Hasegawa, T. Ishida, M. Jakkapu, T. Kobayashi, T. Matsubara, T. Nakadaira, K. Nakamura, 49 Y. Oyama, K. Sakashita, T. Sekiguchi, T. Tsukamoto, T. Boschi, F. Di Lodovico, J. Gao, T. Katori, J. Migenda, M. Taani, S. Zsoldos, 49 KE. Abe, M. Hasegawa, Y. Isobe, Y. Kotsar, H. Miyabe, H. Ozaki, T. Sugimoto, A. T. Suzuki, Y. Takeuchi, 49 S. Yamamoto, Y. Ashida, J. Feng, T. Hayashino, S. Hirota, M. Jiang, T. Kikawa, M. Mori, T. Nakaya, 49 R. A. Wendell, 49 K. Yasutome, P. Fernandez, N. McCauley, P. Mehta, A. Pritchard, K. M. Tsui, Y. Fukuda, Y. Itow, 32 H. Menjo, M. Murase, K. Frankiewicz, J. Lagoda, S. M. Lakshmi, M. Mandal, P. Mijakowski, Y. S. Prabhu, J. Zalipska, M. Jia, J. Jiang, C. K. Jung, X. Li, J. L. Palomino, G. Santucci, C. Vilela, M. J. Wilking, C. Yanagisawa, † D. Fukuda, K. Hagiwara, M. Harada, H. Ishino, S. Ito, H. Kitagawa, Y. Koshio, 49 W. Ma, S. Sakai, M. Sakuda, Y. Takahira, C. Xu, Y. Kuno, G. Barr, D. Barrow, L. Cook, 49 A. Goldsack, 49 S. Samani, C. Simpson, 49 D. Wark, 43 S. Molina Sedgwick, R. Tacik, 53 F. Nova, J. Y. Yang, S. J. Jenkins, M. Malek, J. M. McElwee, O. Stone, M. D. Thiesse, L. F. Thompson, H. Okazawa, Y. Choi, S. B. Kim, J. W. Seo, I. Yu, A. Ichikawa, K. D. Nakamura, K. Nishijima, M. Koshiba, ∗ K. Iwamoto, K. Nakagiri, Y. Nakajima, 49 Y. Suda, N. Taniuchi, M. Yokoyama, 49 K. Martens, M. Murdoch, M. R. Vagins, 8 D. Hamabe, S. Izumiyama, M. Kuze, Y. Okajima, T. Yoshida, M. Inomoto, M. Ishitsuka, H. Ito, T. Kinoshita, R. Matsumoto, M. Shinoki, T. Suganuma, M. Yonenaga, J. F. Martin, C. M. Nantais, H. A. Tanaka, T. Towstego, R. Akutsu, P. de Perio, V. Gousy-Leblanc, ‡ M. Hartz, A. Konaka, P. de Perio, N. W. Prouse, S. Chen, B. D. Xu, 54 B. Zhang, M. Posiadala-Zezula, D. Hadley, M. Nicholson, M. O’Flaherty, B. Richards, A. Ali, 53 B. Jamieson, P. Giorgio, Ll. Marti, A. Minamino, G. Pintaudi, S. Sano, R. Sasaki, and K. Wada
2 citations
TL;DR: In this paper , the Super-Kamiokande water Cherenkov experiment was used to search for proton decay via p → μ þ K 0 in 0 .37 Mton · years of data collected between 1996 and 2018 from the Super Kamiokane water Chechenkov experiment.
Abstract: We searched for proton decay via p → μ þ K 0 in 0 . 37 Mton · years of data collected between 1996 and 2018 from the Super-Kamiokande water Cherenkov experiment. The selection criteria were defined separately for K 0 S and K 0 L channels. No significant event excess has been observed. As a result of this
2 citations
TL;DR: In this article , a scintillation tracker for the muon track matching in the neutrino-nucleus interaction measurement with nuclear emulsion detectors is presented, which consists of four layers of horizontally and vertically aligned scintillator bars, covering an area of 1m×1m.
Abstract: Precise measurement of neutrino–nucleus interactions with an accelerator neutrino beam is highly important for current and future neutrino oscillation experiments. To measure muon-neutrino charged-current interactions with nuclear-emulsion-based hybrid detector, muon track matching among the detectors are essential. We describe the design and performance of a newly developed scintillation tracker for the muon track matching in the neutrino–nucleus interaction measurement with nuclear emulsion detectors. The muon tracks are reconstructed using the scintillation tracker and another detector called Baby MIND, then, they are matched with the tracks in nuclear emulsion detectors. The scintillation tracker consists of four layers of horizontally and vertically aligned scintillator bars, covering an area of 1m×1m. In the layer, 24 mm-wide plastic scintillator bars are specially arranged with deliberate gaps between each other. By recognizing the hit pattern of the four layers, a precise positional resolution of 2.5 mm is achieved while keeping the number of readout channels as small as 256. The efficiency of the track matching is evaluated to be more than 97% for forward-going muons, and the positional and angular resolutions of the scintillation tracker are 2.5 mm and 20–40 mrad respectively. The results demonstrate the usefulness of the design of the scintillation tracker for the muon track matching in the nuclear-emulsion-based neutrino–nucleus interaction measurements.
2 citations
24 Oct 2022
TL;DR: In this paper , the Super-Kamiokande detector was used to search for neutrinos from solar flares that occurred during solar cycles 23 and 24, including the largest solar neutrino (X28.0) on November 4th, 2003.
Abstract: Neutrinos associated with solar flares (solar-flare neutrinos) provide information on particle acceleration mechanisms during the impulsive phase of solar flares. We searched using the Super-Kamiokande detector for neutrinos from solar flares that occurred during solar cycles 23 and 24, including the largest solar flare (X28.0) on November 4th, 2003. In order to minimize the background rate we searched for neutrino interactions within narrow time windows coincident with γ -rays and soft X-rays recorded by satellites. In addition, we performed the first attempt to search for solar-flare neutrinos from solar flares on the invisible side of the Sun by using the emission time of coronal mass ejections (CMEs). By selecting twenty powerful solar flares above X5.0 on the visible side and eight CMEs whose emission speed exceeds 2000 km s − 1 on the invisible side from 1996 to 2018, we found two (six) neutrino events coincident with solar flares occurring on the visible (invisible) side of the Sun, with a typical background rate of 0 . 10 (0 . 62) events per flare in the MeV–GeV energy range. No significant solar-flare neutrino signal above the estimated background rate was observed. As a result we set the following upper limit on neutrino fluence at the Earth Φ < 1 . 1 × 10 6 cm − 2 at the 90% confidence level for the largest solar flare. The resulting fluence limits allow us to constrain some of the theoretical models for solar-flare neutrino emission.
1 citations
DOI•
TL;DR: In this paper , the degradation of the light yield of the T2K-II and Hyper-Kamiokande era was investigated and it was shown that the reduction in light yield can be attributed to the ageing of the plastic scintillator.
Abstract: The T2K experiment widely uses plastic scintillator as a target for neutrino interactions and an active medium for the measurement of charged particles produced in neutrino interactions at its near detector complex. Over 10 years of operation the measured light yield recorded by the scintillator based subsystems has been observed to degrade by 0.9–2.2% per year. Extrapolation of the degradation rate through to 2040 indicates the recorded light yield should remain above the lower threshold used by the current reconstruction algorithms for all subsystems. This will allow the near detectors to continue contributing to important physics measurements during the T2K-II and Hyper-Kamiokande eras. Additionally, work to disentangle the degradation of the plastic scintillator and wavelength shifting fibres shows that the reduction in light yield can be attributed to the ageing of the plastic scintillator. The long component of the attenuation length of the wavelength shifting fibres was observed to degrade by 1.3–5.4% per year, while the short component of the attenuation length did not show any conclusive degradation.
1 citations
TL;DR: In this article , the cosmogenic neutrino yield was measured using data acquired during the period after the gadolinium loading at the Super-Kamiokande detector, and the yield was found to be $(2.76 \pm 0.02\,\mathrm{(stat.) \ pm 0.19\, \mathm{(syst.)}}) \times 10^{-4}\,\mu^{-1} \mathr{g^{ −1} cm^{2}}$ at 259 GeV of average muon energy at the super-kamikande detector.
Abstract: Cosmic-ray muons that enter the Super-Kamiokande detector cause hadronic showers due to spallation in water, producing neutrons and radioactive isotopes. Those are a major background source for studies of MeV-scale neutrinos and searches for rare events. Since 2020, gadolinium was introduced in the ultra-pure water in the Super-Kamiokande detector to improve the detection efficiency of neutrons. In this study, the cosmogenic neutron yield was measured using data acquired during the period after the gadolinium loading. The yield was found to be $(2.76 \pm 0.02\,\mathrm{(stat.) \pm 0.19\,\mathrm{(syst.)}}) \times 10^{-4}\,\mu^{-1} \mathrm{g^{-1} cm^{2}}$ at 259 GeV of average muon energy at the Super-Kamiokande detector.
DOI•
TL;DR: In this paper , the authors presented the development of Neutrino tagging techniques in Super-Kamiokande IV using a neural network analysis, which was performed on 3,244.4 days of SK-IV atmospheric neutrino data, identifying 18,091 neutrons in 26,473 neutrinos events.
Abstract: We present the development of neutron-tagging techniques in Super-Kamiokande IV using a neural network analysis. The detection efficiency of neutron capture on hydrogen is estimated to be 26%, with a mis-tag rate of 0.016 per neutrino event. The uncertainty of the tagging efficiency is estimated to be 9.0%. Measurement of the tagging efficiency with data from an Americium-Beryllium calibration agrees with this value within 10%. The tagging procedure was performed on 3,244.4 days of SK-IV atmospheric neutrino data, identifying 18,091 neutrons in 26,473 neutrino events. The fitted neutron capture lifetime was measured as 218±9 μs.
TL;DR: This research highlights the need to understand more fully the role of language and culture in the decision-making process and the role that language and language skills play in the development of knowledge and identity.
Abstract: A. Alavi-Harati, I.F. Albuquerque, T. Alexopoulos, M. Arenton, K. Arisaka, S. Averitte, A.R. Barker, L. Bellantoni, A. Bellavance, J. Belz, R. Ben-David, D.R. Bergman, E. Blucher, G.J. Bock, C. Bown, S. Bright, E. Cheu, S. Childress, R. Coleman, M.D. Corcoran, G. Corti, B. Cox, M.B. Crisler, A.R. Erwin, R. Ford, A. Glazov, A. Golossanov, G. Graham, J. Graham, K. Hagan, E. Halkiadakis, K. Hanagaki, M. Hazumi, S. Hidaka, Y.B. Hsiung, V. Jejer, J. Jennings, D.A. Jensen, R. Kessler, H.G.E. Kobrak, J. LaDue, A. Lath, A. Ledovskoy, P.L. McBride, A.P. McManus, P. Mikelsons, E. Monnier, T. Nakaya, U. Nauenberg, K.S. Nelson, H. Nguyen, V. O’Dell, M. Pang, R. Pordes, V. Prasad, C. Qiao, B. Quinn, E.J. Ramberg, R.E. Ray, A. Roodman, M. Sadamoto, S. Schnetzer, K. Senyo, P. Shanahan, P.S. Shawhan, J. Shields, W. Slater, N. Solomey, S.V. Somalwar, R.L. Stone, I. Suzuki, E.C. Swallow, R.A. Swanson, S.A. Taegar, R.J. Tesarek, G.B. Thomson, P.A. Toale, A. Tripathi, R. Tschirhart, Y.W. Wah, J. Wang, H.B. White, J. Whitmore, B. Winstein, R. Winston, J.-Y. Wu, T. Yamanaka and E.D. Zimmerman (KTeV Collaboration)
DOI•
16 Mar 2022
TL;DR: In this paper , a nuclear emulsion detector with a 65 kg iron target was exposed to a neutrino beam corresponding to 4.0 × 10 19 protons on target with a mean neutrinos energy of 1.49 GeV.
Abstract: This study conducted an analysis of muons, protons, and charged pions emitted from ν µ charged-current interactions on iron using a nuclear emulsion detector. The emulsion detector with a 65 kg iron target was exposed to a neutrino beam corresponding to 4.0 × 10 19 protons on target with a mean neutrino energy of 1.49 GeV. The measurements were performed at a momentum threshold of 200 (50) MeV/ c for protons (pions), which are the lowest momentum thresholds attempted up to now. The measured quantities are the multiplicities, emission angles, and momenta of the muons, protons, and charged pions. In addition to these inclusive measurements, exclusive measurements such as the muon-proton emission-angle correlations of specific channels and the opening angle between the protons of CC0 π 2 p events were performed. The data were compared to Monte Carlo (MC) predictions and some significant differences were observed. The results of the study demonstrate the capability of detailed measurements of neutrino-nucleus interactions using a nuclear emulsion detector to improve neutrino interaction models. is shifted. The total uncertainties of these backgrounds
TL;DR: This list of players and coaches from the 2016 Rio Olympics and Paralympic Games in Rio de Janeiro, Brazil has been released.
Abstract: J. Adams, A. Alavi-Harati, I.F. Albuquerque, T. Alexopoulos, M. Arenton, K. Arisaka, S. Averitte, A.R. Barker, L. Bellantoni, A. Bellavance, J. Belz, R. Ben-David, D.R. Bergman, E. Blucher, G.J. Bock, C. Bown, S. Bright, E. Cheu, S. Childress, R. Coleman, M.D. Corcoran, G. Corti, B. Cox, M.B. Crisler, A.R. Erwin, S. Field, R. Ford, G. Graham, J. Graham, K. Hagan, E. Halkiadakis, K. Hanagaki, M. Hazumi, S. Hidaka, V. Jejer, J. Jennings, D.A. Jensen, P.T. Johnson, R. Kessler, H.G.E. Kobrak, J. LaDue, A. Lath, A. Ledovskoy, A.P. McManus, P. Mikelsons, S. Mochida, E. Monnier, T. Nakaya, U. Nauenberg, K.S. Nelson, H. Nguyen, V. O’Dell, M. Pang, R. Pordes, V. Prasad, C. Qiao, B. Quinn, E.J. Ramberg, R.E. Ray, A. Ronzhin, A. Roodman, M. Sadamoto, S. Schnetzer, K. Senyo, P. Shanahan, P.S. Shawhan, W. Slater, N. Solomey, S.V. Somalwar, R.L. Stone, I. Suzuki, E.C. Swallow, R.A. Swanson, S.A. Taegar, R.J. Tesarek, G.B. Thomson, P.A. Toale, A. Tripathi, R. Tschirhart, Y.W. Wah, H.B. White, J. Whitmore, B. Winstein, R. Winston, J.-Y. Wu, T. Yamanaka, E.D. Zimmerman
TL;DR: In this paper , the Super-Kamiokande (SK) experiment moved to a new stage (SK-Gd), in which gadolinium (Gd) sulfate octahydrate was added to the water in the detector, enhancing the efficiency to detect thermal neutrons.
Abstract: In 2020, the Super-Kamiokande (SK) experiment moved to a new stage (SK-Gd) in which gadolinium (Gd) sulfate octahydrate was added to the water in the detector, enhancing the efficiency to detect thermal neutrons and consequently improving the sensitivity to low energy electron anti-neutrinos from inverse beta decay (IBD) interactions. SK-Gd has the potential to provide early alerts of incipient core-collapse supernovae through detection of electron anti-neutrinos from thermal and nuclear processes responsible for the cooling of massive stars before the gravitational collapse of their cores. These pre-supernova neutrinos emitted during the silicon burning phase can exceed the energy threshold for IBD reactions. We present the sensitivity of SK-Gd to pre-supernova stars and the techniques used for the development of a pre-supernova alarm based on the detection of these neutrinos in SK, as well as prospects for future SK-Gd phases with higher concentrations of Gd. For the current SK-Gd phase, high-confidence alerts for Betelgeuse could be issued up to 9 hr in advance of the core collapse itself.
28 Aug 2022
TL;DR: In this article , the Super-Kamiokande water Cherenkov experiment was used to search for proton decay via p → µ + K 0 in 0.37 Mton · years of data collected between 1996 and 2018.
Abstract: We searched for proton decay via p → µ + K 0 in 0.37 Mton · years of data collected between 1996 and 2018 from the Super-Kamiokande water Cherenkov experiment. The selection criteria were defined separately for K 0 S and K 0 L channels. No significant event excess has been observed. As a result of this analysis, which extends the previous search by an additional 0.2 Mton · years of exposure and uses an improved event reconstruction, we set a lower limit of 3 . 6 × 10 33 years on the proton lifetime.
TL;DR: A search for periodic modulations of the solar neutrino was performed using the Super-Kamiokande-I data taken from May 31st, 1996 to July 15th, 2001 as discussed by the authors .
Abstract: A search for periodic modulations of the solar neutrino flux was performed using the Super-Kamiokande-I data taken from May 31st, 1996 to July 15th, 2001. The detector’s capability of measuring the exact time of events, combined with a relatively high yield of solar neutrino events, allows a search for short-time variations in the observed flux. We employed the Lomb test to look for periodic modulations of the observed solar neutrino flux. The obtained periodogram is consistent with statistical fluctuation and no significant periodicity was found.
TL;DR: The KTeV Collaboration A.R. Alavi-Harati, T. Alexopoulos, M.D. Averitte, A.B. Arenton, K.S. Hidaka, Y.W. Hsiung, V.J. Jejer, D.E. Kessler, H.L. McBride, P. Mikelsons, E.T. Stone, I.V. Shawhan, W.Winstein, R.
Abstract: The KTeV Collaboration A. Alavi-Harati, T. Alexopoulos, M. Arenton, K. Arisaka, S. Averitte, A.R. Barker, L. Bellantoni, A. Bellavance, J. Belz, R. Ben-David, D.R. Bergman, E. Blucher, G.J. Bock, C. Bown, S. Bright, E. Cheu, S. Childress, R. Coleman, M.D. Corcoran, G. Corti, B. Cox, M.B. Crisler, A.R. Erwin, R. Ford, P.M. Fordyce, A. Glazov, A. Golossanov, G. Graham, J. Graham, K. Hagan, E. Halkiadakis, K. Hanagaki, S. Hidaka, Y.B. Hsiung, V. Jejer, D.A. Jensen, R. Kessler, H.G.E. Kobrak, J. LaDue, A. Lath, A. Ledovskoy, P.L. McBride, P. Mikelsons, E. Monnier, T. Nakaya, K.S. Nelson, H. Nguyen, V. O’Dell, M. Pang, R. Pordes, V. Prasad, C. Qiao, B. Quinn, E.J. Ramberg, R.E. Ray, A. Roodman, M. Sadamoto, S. Schnetzer, K. Senyo, P. Shanahan, P.S. Shawhan, W. Slater, N. Solomey, S.V. Somalwar, R.L. Stone, I. Suzuki, E.C. Swallow, S.A. Taegar, R.J. Tesarek, G.B. Thomson, P.A. Toale, A. Tripathi, R. Tschirhart, Y.W. Wah, J. Wang, H.B. White, J. Whitmore, B. Winstein, R. Winston, T. Yamanaka, E.D. Zimmerman
TL;DR: In this paper , a new method for momentum reconstruction of charged particles using multiple Coulomb scatterings (MCS) in a nuclear emulsion detector with a lay-ered structure of nuclear materials and target materials is described.
Abstract: This paper describes a new method for momentum reconstruction of charged particles using multiple Coulomb scatterings (MCS) in a nuclear emulsion detector with a lay-ered structure of nuclear emulsion films and target materials. The method utilizes the scattering angles of particles precisely measured in the emulsion films. The method is based on the maximum likelihood to newly include information on the decrease of the energy as the particle travels through the detector. According to the MC simulations, this method can measure momentum with a resolution of 10% for muons of 500 MeV /c passing through the detector perpendicularly. The momentum resolution is evaluated to be 10–20%, depending on the momentum and emission angle of the particle. By accounting for the effect of the energy decrease, the momentum can be reconstructed correctly with less bias, particularly in the low-momentum region. We apply this method to measure the momentum of muon tracks detected in the NINJA experiment where the momentum is also measured independently by using the track range. The two measurements agree well within experimental uncertainties of a 2% difference, verifying the method experimentally. This method will extend the measurable phase space of muons and hadrons in the NINJA experiment.
TL;DR: In this article , the authors present a survey of the state-of-the-art work in the field of computer vision and artificial intelligence, including the following: A.R. Bergman, E.J. Blucher, G.C. Bock, C. Bown, S.B. Cheu, S., E.C., B. Nelson, H.E. Jejer, J.M. Quinton, D.A. Quinn, B.M., A.E., R.R., M.R..
Abstract: A. Alavi-Harati, I.F. Albuquerque, T. Alexopoulos, M. Arenton, K. Arisaka, S. Averitte, A.R. Barker, L. Bellantoni, A. Bellavance, J. Belz, R. Ben-David, D.R. Bergman, E. Blucher, G.J. Bock, C. Bown, S. Bright, E. Cheu, S. Childress, R. Coleman, M.D. Corcoran, G. Corti, B. Cox, M.B. Crisler, A.R. Erwin, R. Ford, A. Glazov, A. Golossanov, G. Graham, J. Graham, K. Hagan, E. Halkiadakis, K. Hanagaki, M. Hazumi, S. Hidaka, Y.B. Hsiung, V. Jejer, J. Jennings, D.A. Jensen, R. Kessler, H.G.E. Kobrak, J. LaDue, A. Lath, A. Ledovskoy, P.L. McBride, A.P. McManus, P. Mikelsons, E. Monnier, T. Nakaya, K.S. Nelson, H. Nguyen, V. O’Dell, M. Pang, R. Pordes, V. Prasad, C. Qiao, B. Quinn, E.J. Ramberg, R.E. Ray, A. Roodman, M. Sadamoto, S. Schnetzer, K. Senyo, P. Shanahan, P.S. Shawhan, W. Slater, N. Solomey, S.V. Somalwar, R.L. Stone, I. Suzuki, E.C. Swallow, R.A. Swanson, S.A. Taegar, R.J. Tesarek, G.B. Thomson, P.A. Toale, A. Tripathi, R. Tschirhart, Y.W. Wah, J. Wang, H.B. White, J. Whitmore, B. Winstein, R. Winston, T. Yamanaka, E.D. Zimmerman