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3,089 results on '"H Kawai"'

1. Design and production of pressure vessel for food processing machine using underwater shock using measurement of particle velocity and results of numerical analysis

Author

K Shimojima, Y Higa, O Higa, A Takemoto, H Iyama, T Watanabe, H Kawai, K Hokamoto, and S Itoh

Subjects
Physics, QC1-999
Abstract

Okinawa National College of Technology has developed a food processing machine using underwater shock waves. Several prototype machines were developed, and experimental results (sterilization, improvement of juice extraction, milling flour, emulsification etc.) were obtained. After deciding food materials to be processed and the desired processing results, we designed and manufactured a pressure vessel for experiments. In this report, the process flow for designing and manufacturing a pressure vessel for softening meat using underwater shock and its concept design are described. The relationships among the number of shock waves, the distance between the shock wave generation point and the meat, the backing material, and the amount of softening ware experimentally compared. We measured the velocity of the shock wave penetrating to the inside of the meat, from which we estimated the particle velocity. We developed computer simulation model using the estimated particle velocity in the meat. Using the results of the analysis obtained from the computer simulation model, we designed and fabricated the pressure vessel.

Published
2019
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2. Laminoplasty for Patients Aged 75 Years or Older with Cervical Myelopathy

Author

M Ishii, E Wada, T Ishii, H Kawai, N Kaneko, and T Fuji

Subjects
Orthopedic surgery, RD701-811
Abstract

Purpose. To assess the neurological and walking status of 56 elderly patients after cervical myelopathy to determine whether the surgery was justified. Methods. Records of 23 men and 33 women aged 75 to 86 (mean, 79) years who underwent laminoplasty for cervical myelopathy were retrospectively reviewed. They had been followed up for a mean of 3.5 (range, 0.2–8.6) years. Walking status was assessed according to long-term care insurance criteria. In 45 patients with more than 2 years of follow-up, neurological status was evaluated according to the Japanese Orthopaedic Association (JOA) score. Neurological recovery rate was classified as excellent, good, fair, poor, and worse. Results. Postoperatively, of the 47 patients still living, 22 could walk independently, 22 required assistance outdoors, 2 were using a wheelchair, and one was bedridden. The mean JOA score was 9.7 preoperatively, 12.2 one year postoperatively, and 11.8 at final assessment (p

Published
2008
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3. Factors Contributing to Historical and Future Trends in Arctic Precipitation

Author

S. Yukimoto, N. Oshima, H. Kawai, M. Deushi, and T. Aizawa

Subjects
Arctic precipitation, atmospheric radiative cooling, meridional heat transport, Geophysics. Cosmic physics, QC801-809
Abstract

Abstract The Arctic is notable as a region where the greatest rate of increase in precipitation associated with global warming is anticipated. The Arctic precipitation simulated by the Coupled Model Intercomparison Project Phase 6 models showed a strong increasing trend since the 1980s. We found that the forcing factor of the trend is a combination of the continued strengthening of greenhouse gas forcing and the leveling off of aerosol forcing dominated in earlier periods. From an energetic perspective, we found that the increased atmospheric radiative cooling and reduced sensible heat transport from lower latitudes contributed equally to the recent increase in Arctic precipitation. The combination of these two energetic factors suggests a doubling of the Arctic amplification factor for precipitation relative to that for temperature. Future Arctic precipitation will change in proportion to the temperature change, and the fractional contributions of the energetic factors will remain stable across various scenarios.

Published
2024
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4. ACTIVATION OF HUMAN FIBROBLASTS BY CHRONIC RADIATION RATHER THAN ACUTE RADIATION

Author

T Shimura, E Zaharieva, M Sasatani, H Kawai, K Kamiya, and A Ushiyama

Subjects
Radiation, Cancer-Associated Fibroblasts, Radiological and Ultrasound Technology, Neoplasms, Tumor Microenvironment, Public Health, Environmental and Occupational Health, Humans, Radiology, Nuclear Medicine and imaging, General Medicine, Fibroblasts, Reactive Oxygen Species
Abstract

Cancer-associated fibroblast (CAF), an activated type of fibroblast, is a major stromal cell that contributes to tumor initiation and development in the tumor microenvironment (TME). We previously reported that fractionated radiation rather than acute radiation causes progressive damage to mitochondria and increases the generation of reactive oxygen species, playing an important role in the fibroblast activation in normal tissue injury. Activated fibroblasts then become CAF by interacting with tumor cells, promoting tumor growth in vivo. We here examined the chronic radiation effect on fibroblast activation. Acute radiation (

Published
2022
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6. Rivaroxaban Monotherapy in Patients With Atrial Fibrillation After Coronary Stenting

Author

Tetsuya Matoba, Satoshi Yasuda, Koichi Kaikita, Masaharu Akao, Junya Ako, Masato Nakamura, Katsumi Miyauchi, Nobuhisa Hagiwara, Kazuo Kimura, Atsushi Hirayama, Kunihiko Matsui, Hisao Ogawa, Yukihiro Koretsune, Takafumi Hiro, Tetsuya Sumiyoshi, Kazumi Kimura, Yoichiro Hashimoto, Teruyuki Hirano, Hiroyuki Daida, Yasushi Okada, Tsutomu Yamazaki, A. Nakamura, E. Tamiya, T. Yamamoto, S. Suetake, T. Noguchi, S. Nakamura, A. Matsumura, J. Kojima, S. Suwa, H. Yamaguchi, K. Kaikita, T. Yasu, A. Nakajima, T. Yamada, H. Arai, Y. Hata, T. Sakanashi, H. Tateishi, T. Nakayama, Y. Nozaki, M. Akao, Y. Okumura, M. Tokue, N. Kuroki, Y. Maruyama, T. Matoba, N. Hagiwara, H. Suzuki, Y. Nishida, M. Ajioka, K. Yumoto, S. Shimizu, T. Aoyama, H. Shimomura, T. Takeda, K. Oshiro, N. Sugishita, Y. Shibata, T. Otonari, H. Kihara, H. Ogawa, A. Ohno, M. Hazama, M. Shimizu, K. Tsukahara, S. Haruta, T. Wakeyama, T. Haruna, M. Ito, K. Fujii, N. Atsuchi, M. Sata, K. Kimura, N. Hasebe, Y. Kobayasi, K. Ohsato, K. Hironaga, Y. Naganuma, K. Anzaki, K. Oiwa, S. Okazaki, Y. Nakagawa, K. Tokuhiro, K. Tanaka, T. Momose, Y. Fukushima, R. Kametani, K. Kawamitsu, Y. Saito, S. Akashi, K. Kumagai, K. Eshima, T. Tobaru, T. Seo, K. Okuhara, K. Kozuma, Y. Ikari, T. Takahashi, I. Michishita, H. Fujikura, S. Momomura, Y. Yamamoto, K. Otomo, T. Matsubara, H. Tashiro, T. Inoue, M. Ishihara, I. Shiojima, E. Tachibana, J. Ako, K. Sumii, N. Yamamoto, N. Ohmura, T. Nakamura, Y. Morita, N. Takahashi, K. Watanabe, H. Fujinaga, M. Maruyama, T. Oka, T. Shirayama, T. Amano, K. Fukui, K. Ando, S. Oshima, S. Kagiyama, H. Teragawa, M. Yuge, S. Ono, T. Koga, K. Fujiu, M. Kuwabara, Y. Ohya, Y. Yumoto, N. Kuji, M. Ikemura, K. Kario, K. Chatani, K. Sato, H. Miyagi, M. Murakami, K. Saito, M. Hoshiga, S. Sato, N. Kubo, Y. Sakamoto, K. Ashida, H. Sakamoto, S. Murasaki, H. Uehara, T. Akasaka, Y. Ooba, S. Nakahara, Y. Hanaoka, T. Nishimiya, R. Tsunoda, Y. Onuma, S. Higuchi, A. Tani, A. Wada, M. Kato, H. Obata, Y. Higuchi, T. Endo, R. Katou, T. Matsunaga, T. Matsuoka, H. Noguchi, M. Usui, T. Hayashi, Y. Otsuji, T. Osaki, H. Zaizen, H. Yoshihara, K. Kadota, T. Hirose, T. Miyazawa, A. Mori, M. Takano, W. Shimizu, M. Wake, S. Oriso, M. Yoshiyama, S. Kakinoki, T. Nishioka, T. Ozaki, K. Nomoto, K. Seki, K. Kawai, Y. Ozaki, S. Miura, M. Kawasaki, R. Funada, K. Dote, T. Nagano, S. Okamoto, T. Kubo, Y. Murozono, T. Owada, T. Doke, T. Matsumura, M. Horiuchi, A. Takaishi, M. Yamamoto, H. Nakashima, M. Munemasa, Y. Sakata, N. Inoue, T. Ota, Y. Hamano, N. Abe, T. Tsubokura, M. Goto, I. Kubota, M. Yano, K. Umetani, T. Date, H. Morimoto, T. Noda, S. Goto, K. Hibi, A. Nakano, S. Hiramitsu, Y. Kihara, M. Sugi, N. Shiba, D. Izumi, T. Sato, S. Tayama, T. Matsui, A. Suzuki, K. Ajiki, M. Oishi, M. Kiryu, T. Ko, H. Ando, S. Miyazaki, T. Kinugawa, H. Otake, H. Kitaoka, Y. Hirata, S. Honda, M. Manita, Y. Ishii, H. Oka, Y. Nanba, M. Nishino, T. Sakamoto, T. Saito, H. Sakai, M. Ichikawa, S. Namiuchi, K. Inoue, N. Komiyama, Y. Akashi, Y. Nakamura, T. Komaru, T. Hosokawa, T. Chikamori, H. Tanaka, O. Arasaki, K. Aonuma, Y. Wakasa, T. Yoshizawa, T. Sugano, N. Yokota, A. Kakutani, T. Suzuki, Y. Abe, T. Kataoka, H. Okayama, H. Yokoi, K. Chin, K. Hasegawa, H. Tomita, H. Honzyo, H. Kawai, K. Yamamoto, Y. Morino, S. Tsujiyama, S. Hamasaki, Y. Niijima, Y. Mizuno, A. Maki, K. Tanabe, T. Murohara, S. Naomi, M. Arikawa, T. Kato, N. Matsumoto, T. Minamino, H. Sairenji, N. Miyamoto, H. Ito, Y. Matsuura, S. Hata, Y. Nakatsu, T. Onodera, M. Yoshimura, H. Amano, E. Tokutake, M. Kasao, M. Moriguchi, M. Tsuji, H. Yamamoto, Y. Yanbe, T. Iwasawa, M. Suzuki, and H. Mori

Subjects
Rivaroxaban, medicine.medical_specialty, business.industry, Unstable angina, medicine.medical_treatment, Percutaneous coronary intervention, Atrial fibrillation, medicine.disease, Thrombosis, Coronary artery disease, Internal medicine, medicine, Cardiology, cardiovascular diseases, Myocardial infarction, Cardiology and Cardiovascular Medicine, business, Stroke, medicine.drug
Abstract

Objectives The aim of this AFIRE (Atrial Fibrillation and Ischemic Events With Rivaroxaban in Patients With Stable Coronary Artery Disease) trial subgroup analysis was to examine rivaroxaban monotherapy benefits and their relation to the time between stenting and enrollment among patients after coronary stenting. Background Of 2,215 patients with atrial fibrillation and stable coronary artery disease in the AFIRE trial, rivaroxaban monotherapy was noninferior to rivaroxaban plus antiplatelet therapy (combination therapy) in terms of efficacy and superior for safety endpoints. However, thrombotic risk after antiplatelet therapy cessation remained a concern among 1,444 patients who had undergone coronary stenting >1 year before enrollment. Methods The benefits of rivaroxaban monotherapy in coronary stenting subgroups were assessed for efficacy (a composite of stroke, systemic embolism, myocardial infarction, unstable angina requiring revascularization, or death of any cause), safety (major bleeding defined according to International Society on Thrombosis and Haemostasis criteria), ischemic endpoints, net adverse clinical event, and time between stenting and enrollment. Results Efficacy and safety endpoints for monotherapy were superior to combination therapy, with HRs of 0.70 for efficacy (95% CI: 0.50-0.98; P = 0.036) and 0.55 for safety (95% CI: 0.33-0.92; P = 0.019). For ischemic endpoints, the HR was 0.82 (95% CI: 0.58-1.15; P = 0.240). The HR became smaller with longer time between stenting and enrollment (efficacy, P for interaction = 0.158; safety, P = 0.097). Conclusions In patients with atrial fibrillation after coronary stenting, the benefits of rivaroxaban monotherapy for efficacy and safety endpoints were consistent with those in the whole AFIRE trial population. The benefits became apparent with longer time between stenting and enrollment. (Atrial Fibrillation and Ischemic Events With Rivaroxaban in Patients With Stable Coronary Artery Disease Study [AFIRE]; UMIN000016612 , NCT02642419 )

Published
2021
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8. ACE values in the diagnosis of sarcoidosis

Author

H Kawai, H Naruse, M Sarai, Y Kato, Y Sato, S Motoyama, J Ishii, S Morimoto, and H Izawa

Subjects
Cardiology and Cardiovascular Medicine
Abstract

Background In clinical practice, we often encounter the patients with sarcoidosis showing relatively high in the normal range of serum angiotensin-converting enzyme (ACE) value. Purpose We aimed to examine the serum ACE value of the patients with sarcoidosis and determine the new cut-off value for detecting the patients with sarcoidosis. Methods and results We retrospectively examined all 3781 subjects (51.1% men, 60.1±17.0 y.o.) in whom ACE was measured for any reasons including suspected sarcoidosis between 2009 and 2020 in our hospital. Of 293 patients with sarcoidosis, 101, 212, 84, and 88 were diagnosed as sarcoidosis in heart, lung, skin, and eyes, respectively. After excluding 477 patients taking ACE inhibitor and/or immunosuppression agent or those with any diseases affecting serum ACE levels, we analyzed 3304 subjects including 215 with sarcoidosis. Serum ACEs were 19.6 IU/L [IQR, 15.1–31.5] in the subjects with sarcoidosis and 10.7 [8.4–16.5] in those without (P Conclusion(s) In the current cut-off value of serum ACE, sensitivity for detecting sarcoidosis was comparatively low, though positive predictive value was low when the new-cut-off value was used in our study. Further examinations may be needed for the patients suspected sarcoidosis with relatively high ACE in the normal range. Funding Acknowledgement Type of funding sources: None.

Published
2022
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9. Effects of antifouling compounds on the growth of macroalgae Undaria pinnatifida

Author

M. Nomura, H. Okamura, Y. Horie, C.K. Yap, C. Emmanouil, S. Uwai, and H. Kawai

Subjects
Environmental Engineering, Biofouling, Health, Toxicology and Mutagenesis, Gametophytes, Public Health, Environmental and Occupational Health, Reproducibility of Results, General Medicine, General Chemistry, Antifoulants, Seaweeds, Undaria, Seaweed, Pollution, Ecotoxicity test, Diuron, Biocides, Environmental Chemistry, Ecosystem
Abstract

Seaweeds are some of the principal primary producers of marine environments, and they are important ecological elements of coastal ecosystems. The effects of harmful chemicals on seaweeds may adversely affect coastal ecosystems, hence we aimed to develop a new phytotoxicity test using the gametophytes of a common temperate kelp species, Undaria pinnatifida (KU-1630), for the widely used antifouling chemical substances Cybutryne, Diuron, Cu

Published
2022

11. LES around a Realistic City Block Designed Based on a Future City Concept

Author

T. Nozu, A. Ono, T. Tamura, and H. Kawai

Abstract

In this study, we discuss the flow field of the realistic city block model planned according to the concept of the future city, in the case of an actual typhoon and a winter monsoon hit. This study applied BCM-LES technique, which enables large scale simulation with high efficient of parallel computing. The fluctuating inflow of the actual typhoon was created by using the method of adding the turbulent component based on WRF-LES. From the computed results, we confirmed that properties of inflow and the location of high-rise buildings affect the flow field and the pressure distribution of target high-rise building.

Published
2022

12. Measurement of structure dependent radiative K+ → e+νγ decays using stopped positive kaons

Author

H. Ito, A. Kobayashi, S. Bianchin, T. Cao, C. Djalali, D.H. Dongwi, T. Gautam, D. Gill, M.D. Hasinoff, K. Horie, Y. Igarashi, J. Imazato, N. Kalantarians, H. Kawai, S. Kimura, S. Kodama, M. Kohl, H. Lu, O. Mineev, P. Monaghan, S. Shimizu, S. Strauch, M. Tabata, R. Tanuma, A. Toyoda, H. Yamazaki, and N. Yershov

Subjects
Nuclear and High Energy Physics, 010308 nuclear & particles physics, Physics, QC1-999, 0103 physical sciences, 010306 general physics, 01 natural sciences
Abstract

The structure dependent radiative K+→e+νγ (Ke2γSD+) decay was investigated with stopped positive kaons. The e+ momentum spectra containing 574±30 Ke2γSD+ events with a K+→μ+ν (Kμ2) background of 28±19 events were measured with and without a photon in coincidence and analyzed with Monte Carlo simulations for acceptance and detector response to extract the ratio of the branching ratio of the Ke2γSD+ decay and the K+→e+ν decay including the internal bremsstrahlung process (Ke2(γ)). A value of Br(Ke2γSD+)/Br(Ke2(γ))=1.12±0.07stat±0.04syst was obtained. This indicates a partial branching ratio, Br(Ke2γSD+,pe>200MeV/c,Eγ>10MeV)/Br(Kμ2)=(1.85±0.11stat±0.07syst)×10−5, which is 25% (∼2.5σ) higher than the previous experimental result.

Published
2022

14. Precise Measurement of Differential Cross Sections of the Σ^{-}p→Λn Reaction in Momentum Range 470-650 MeV/c

Author

K, Miwa, J K, Ahn, Y, Akazawa, T, Aramaki, S, Ashikaga, S, Callier, N, Chiga, S W, Choi, H, Ekawa, P, Evtoukhovitch, N, Fujioka, M, Fujita, T, Gogami, T, Harada, S, Hasegawa, S H, Hayakawa, R, Honda, S, Hoshino, K, Hosomi, M, Ichikawa, Y, Ichikawa, M, Ieiri, M, Ikeda, K, Imai, Y, Ishikawa, S, Ishimoto, W S, Jung, S, Kajikawa, H, Kanauchi, H, Kanda, T, Kitaoka, B M, Kang, H, Kawai, S H, Kim, K, Kobayashi, T, Koike, K, Matsuda, Y, Matsumoto, S, Nagao, R, Nagatomi, Y, Nakada, M, Nakagawa, I, Nakamura, T, Nanamura, M, Naruki, S, Ozawa, L, Raux, T G, Rogers, A, Sakaguchi, T, Sakao, H, Sako, S, Sato, T, Shiozaki, K, Shirotori, K N, Suzuki, S, Suzuki, M, Tabata, C D L, Taille, H, Takahashi, T, Takahashi, T N, Takahashi, H, Tamura, M, Tanaka, K, Tanida, Z, Tsamalaidze, M, Ukai, H, Umetsu, S, Wada, T O, Yamamoto, J, Yoshida, and K, Yoshimura

Abstract

The differential cross sections of the Σ^{-}p→Λn reaction were measured accurately for the Σ^{-} momentum (p_{Σ}) ranging from 470 to 650 MeV/c at the J-PARC Hadron Experimental Facility. Precise angular information about the Σ^{-}p→Λn reaction was obtained for the first time by detecting approximately 100 reaction events at each angular step of Δcosθ=0.1. The obtained differential cross sections show a slightly forward-peaking structure in the measured momentum regions. The cross sections integrated for -0.7≤cosθ≤1.0 were obtained as 22.5±0.68 [statistical error(stat.)] ±0.65 [systematic error(syst.)] mb and 15.8±0.83(stat)±0.52(syst) mb for 470p_{Σ}(MeV/c)550 and 550p_{Σ}(MeV/c)650, respectively. These results show a drastic improvement compared with past measurements of the hyperon-proton scattering experiments. They will play essential roles in updating the theoretical models of the baryon-baryon interactions.

Published
2021

15. Measurement of the differential cross sections of the Σ−p elastic scattering in momentum range 470 to 850 MeV/c

Author

Yudai Ichikawa, Toshiyuki Gogami, C. d. L. Taille, Z. Tsamalaidze, Manami Nakagawa, Mifuyu Ukai, S. H. Kim, S. Ishimoto, J. K. Ahn, Kazuhiro Suzuki, T. Shiozaki, Hitoshi Tamura, L. Raux, Hiroyuki Ekawa, Hitoshi Takahashi, S. Hoshino, S. Nagao, S. Callier, T. Nanamura, K. Miwa, Takeshi Koike, Y. Nakada, T. Harada, Masaharu Ieiri, T. Aramaki, M. Ikeda, H. Kawai, K. Tanida, M. Ichikawa, B. M. Kang, Kotaro Shirotori, Shoichi Hasegawa, R. Nagatomi, Kenichi Imai, Makoto Tabata, Masaaki Tanaka, S. Wada, Ryotaro Honda, Hiroyuki Sako, S. W. Choi, H. Umetsu, K. Matsuda, Petr Evtoukhovitch, Yuya Akazawa, Toshiyuki Takahashi, S. Ozawa, T. G. Rogers, H. Kanda, N. Fujioka, H. Kanauchi, S. Y. Suzuki, T. Kitaoka, Takashi Yamamoto, T. Takahashi, Y. Matsumoto, Junya Yoshida, Megumi Naruki, Atsushi Sakaguchi, Manami Fujita, Koji Yoshimura, T. Sakao, S. Ashikaga, S. H. Hayakawa, Kensuke Kobayashi, Yoshikazu Ishikawa, Nobuyuki Chiga, S. Kajikawa, Susumu Sato, I. Nakamura, Kenji Hosomi, and W. S. Jung

Subjects
Nuclear physics, Elastic scattering, Physics, Range (particle radiation), Momentum (technical analysis), 010308 nuclear & particles physics, 0103 physical sciences, 010306 general physics, 01 natural sciences, Differential (mathematics)
Published
2021
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16. ПОИСК НЕЙТРИНО УЛЬТРАВЫСОКИХ ЭНЕРГИЙ ПО ДАННЫМ НАЗЕМНОЙ РЕШЕТКИ ЭКСПЕРИМЕНТА TELESCOPE ARRAY

Author

Taka Tomida, J. Remington, Kenta Yashiro, Yasunori Saito, M. Abe, O. Kalashev, Jonathan Smith, Takeshi Okuda, Igor Tkachev, N. Inoue, M. Ohnishi, Federico R. Urban, Yuichiro Tameda, H. Oda, Akimichi Taketa, T. Suzawa, Naoaki Hayashida, Shingo Kawana, Yasuhiro H. Takahashi, John N. Matthews, Isaac Myers, Vladim Kuzmin, William Hanlon, Elliott Barcikowski, Seok Ho Jeong, K. Nagasawa, B. G. Cheon, Hidemi Ito, Fumiya Shibata, Zach Zundel, J. Yang, S. Kitamura, Dmitri Ivanov, Keijiro Mukai, R. Sahara, John Belz, Y. J. Kwon, Hideyuki Ohoka, Fumio Kakimoto, Toshiyuki Nonaka, Toshitsugu Fujii, Daisuke Ikeda, R. Ishimori, Yuta Tanoue, D. R. Bergman, S. R. Stratton, G. Furlich, Takaaki Ishii, Tiffany Wong, Hideki Tanaka, K. Kadota, Inkyu Park, Motoki Hayashi, Hisono Tokuno, T. K. Sako, J. P. Lundquist, D. C. Rodriguez, Ben Stokes, Toru Nakamura, K. Yamazaki, Hongsu Kim, S. B. Thomas, Masahiro Fukushima, S. Kawakami, K. Hibino, Pierre Sokolsky, Ryo Nakamura, K. H. Lee, Jihee Kim, T.-A. Shibata, Eiji Kido, M. V. Kuznetsov, Kazuhiro Machida, Hiroshi Yamaoka, Keitaro Fujita, M. Takeda, Shigehiro Nagataki, Yana Zhezher, Y. Uchihori, Kei Nakai, Kohei Yada, Gordon Thomson, Tom Stroman, Robert Cady, Kazuo Saito, Charlie Jui, BayarJon Paul Lubsandorzhiev, Hiroyuki Sagawa, Mayuko Minamino, Michiyuki Chikawa, K. Honda, Yasunori Kitamura, Grigory Rubtsov, Masaaki Tanaka, Kalen Martens, M. Takita, H. Yoshii, Bokkyun Shin, Koichi Sekino, Kiyoshi Tanaka, Maxim Pshirkov, Jyunsei Chiba, P. Tinyakov, Dongsu Ryu, Y. Omura, Mai Takamura, Y. Takagi, Samuel Blake, Shoichi Ogio, Priti Shah, Ryuji Takeishi, J. Ogura, M. Allen, K. Kasahara, Shoichi Kishigami, Akitoshi Oshima, Y. Tsunesada, Hideaki Shimodaira, Hyoming Jeong, Masaomi Ono, K. Tsutsumi, Rasha Abbasi, Tareq Abu-Zayyad, L. M. Scott, Y. Hayashi, K. Kawata, M. Yamamoto, Nobuyuki Sakurai, Ryota Onogi, J. H. Kim, A. Di Matteo, Ryota Fujiwara, R. Mayta, Heungsu Shin, Naoto Sakaki, Shigeharu Udo, R. Azuma, H. Kawai, T. Seki, T. Matsuyama, S. Ozawa, and Sergey Troitsky

Subjects
General Physics and Astronomy
Published
2020
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17. A Prospective Cohort Study to Define the Clinical Features and Outcome of Lung Cancers Harboring HER2 Aberration in Japan (HER2-CS STUDY)

Author

Kiichiro Ninomiya, Tae Hata, Hiroshige Yoshioka, Kadoaki Ohashi, Akihiro Bessho, Shinobu Hosokawa, Nobuhisa Ishikawa, Masahiro Yamasaki, Takuo Shibayama, Keisuke Aoe, Toshiyuki Kozuki, Shingo Harita, Yutaka Ueda, Toshi Murakami, Nobukazu Fujimoto, Hiroyuki Yanai, Shinichi Toyooka, Minoru Takata, Katsuyuki Hotta, Katsuyuki Kiura, K. Gemba, G. Ikeda, M. Yasugi, E. Kurimoto, K. Nakano, T. Moritaka, K. Inoue, S. Miyoshi, N. Hamaguchi, R. Ito, Y. Sano, I. Takata, A. Mitani, T. Nishisaka, H. Shoda, A. Nishida, S. Tamamoto, K. Fujitaka, T. Masuda, S. Miyamoto, N. Hattori, K. Sugimoto, S. Fujii, Y. Ueda, M. Sakugawa, N. Fukamatsu, Y. Ogata, S. Bandoh, N. Kanaji, N. Takigawa, H. Yamane, N. Ochi, Y. Honda, M. Oka, M. Kittaka, T. Kubota, A. Yokoyama, T. Yokoyama, E. Sato, Y. Shiota, N. Horita, T. Kanematsu, Y. Awaya, A. Nakamasu, I. Murakami, S. Kuyama, K. Kudo, T. Tamura, T. Umeno, D. Morichika, K. Fujiwara, K. Sato, D. Harada, N. Nogami, K. Nishii, Y. Fuchimoto, T. Kishimoto, H. Kawai, K. Watanabe, K. Tokumo, T. Isobe, Y. Tsubata, M. Inoue, H. Ichikawa, Y. Nishioka, M. Hanibuchi, H. Goto, T. Sumikawa, M. Kodani, H. Suyama, H. Makino, N. Kinosita, E. Shimizu, H. Obata, H. Ikegami, K. Chikamori, T. Maeda, T. Kishino, H. Kamei, H. Ueoka, Y. Kunihiro, T. Kobayashi, K. Ueda, M. Hayashi, M. Kamiya, J. Murakami, A. Sato, E. Ichihara, T. Kubo, T. Ninomiya, T. Hirata, D. Minami, Y. Kato, H. Higo, G. Makimoto, Y. Toyota, N. Oda, M. Nakanishi, H. Kayatani, S. Senoo, H. Kano, H. Watanabe, T. Ando, T. Nakasuka, N. Hara, J. Itano, H. Nakashima, and M. Tabata

Subjects
Adult, Male, Pulmonary and Respiratory Medicine, Oncology, medicine.medical_specialty, Lung Neoplasms, Anaplastic Lymphoma, Receptor, ErbB-2, Critical Care and Intensive Care Medicine, Cohort Studies, 03 medical and health sciences, 0302 clinical medicine, Asian People, Japan, Epidermal growth factor, Carcinoma, Non-Small-Cell Lung, Internal medicine, medicine, Humans, 030212 general & internal medicine, Epidermal growth factor receptor, skin and connective tissue diseases, Prospective cohort study, neoplasms, Aged, Neoplasm Staging, Aged, 80 and over, Lung, Oncogene, biology, business.industry, Middle Aged, medicine.anatomical_structure, 030228 respiratory system, Mutation, biology.protein, Immunohistochemistry, Female, Cardiology and Cardiovascular Medicine, business, Cohort study
Abstract

Background Human epidermal growth factor 2 (HER2) is a potential driver oncogene. Although HER2-targeted precision therapy has been tested in non-small cell lung cancer (NSCLC), the demographic characteristics of HER2-positive NSCLC have not been systematically defined. Methods Patients with pathologically confirmed stage IIIB/IV or recurrent NSCLC, Eastern Cooperative Oncology Group performance status 0 to 2, were prospectively registered. HER2 immunohistochemistry (IHC) and fluorescence in situ hybridization (FISH) assays were performed to screen patients. HER2 mutations were identified by using direct gene sequencing. The aim of this study was to clarify the frequency, characteristics, and outcome of HER2-positive NSCLC. HER2 was defined as positive if the tumor harbored IHC3+, IHC2+/FISH+, or exon 20 insertion mutations. Results Of the 1,126 tumors screened, 34 (3.0%) were IHC3+, and 34 (3.0%) were IHC2+/FISH+. Among the 724 epidermal growth factor receptor wild-type tumors, 21 (2.9%) were HER2-mutant tumors, including A775-G776insYVMA (n = 15). Interestingly, the IHC3+ tumors and mutant tumors were entirely exclusive. Female patients had HER2-mutant tumors more frequently, whereas both IHC3+ and IHC2+/FISH+ tumors were detected more often in male subjects and smokers. Patients with an HER2-aberrant tumor had a significantly worse prognosis than those with epidermal growth factor receptor-positive and anaplastic lymphoma kinase-positive tumors, possibly due to the low proportion that received HER2-targeted therapies (n = 15 [26%]) and low response rates of 0% and 14% in patients with HER2-overexpressing and HER2-mutant tumors, respectively. Conclusions This prospective large-scale cohort study is the first to show comprehensively the frequency and clinical demographic characteristics of those with HER2-positive advanced lung tumors in detail, providing critical historical data for future drug development against HER2-positive NSCLC. Future treatment strategies would be developed stratified according to the types of HER2 aberrations. Trial Registry UMIN Registration No. 000017003; URL: https://upload.umin.ac.jp/cgi-open-bin/ctr_e/ctr_view.cgi?recptno=R000019691

Published
2019
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18. Observation of Variations in Cosmic Ray Single Count Rates During Thunderstorms and Implications for Large-Scale Electric Field Changes

Author

R. U. Abbasi, T. Abu-Zayyad, M. Allen, Y. Arai, R. Arimura, E. Barcikowski, J. W. Belz, D. R. Bergman, S. A. Blake, I. Buckland, R. Cady, B. G. Cheon, J. Chiba, M. Chikawa, T. Fujii, K. Fujisue, K. Fujita, R. Fujiwara, M. Fukushima, R. Fukushima, G. Furlich, N. Globus, R. Gonzalez, W. Hanlon, M. Hayashi, N. Hayashida, K. Hibino, R. Higuchi, K. Honda, N. Husseini, D. Ikeda, T. Inadomi, N. Inoue, T. Ishii, H. Ito, D. Ivanov, H. Iwakura, A. Iwasaki, H. M. Jeong, S. Jeong, H. Johnson, C. C. H. Jui, K. Kadota, F. Kakimoto, O. Kalashev, K. Kasahara, S. Kasami, H. Kawai, S. Kawakami, S. Kawana, K. Kawata, I. Kharuk, E. Kido, H. B. Kim, J. H. Kim, M. H. Kim, S. W. Kim, Y. Kimura, S. Kishigami, Y. Kubota, S. Kurisu, V. Kuzmin, M. Kuznetsov, Y. J. Kwon, K. H. Lee, R. LeVon, B. Lubsandorzhiev, J. P. Lundquist, K. Machida, H. Matsumiya, T. Matsuyama, J. N. Matthews, R. Mayta, J. Mazich, M. Minamino, K. Mukai, I. Myers, P. Myers, S. Nagataki, K. Nakai, R. Nakamura, T. Nakamura, Y. Nakamura, A. Nakazawa, E. Nishio, T. Nonaka, K. O’Brien, H. Oda, S. Ogio, M. Ohnishi, H. Ohoka, Y. Oku, T. Okuda, Y. Omura, M. Ono, R. Onogi, A. Oshima, S. Ozawa, I. H. Park, M. Potts, M. S. Pshirkov, J. Remington, D. C. Rodriguez, G. I. Rubtsov, D. Ryu, H. Sagawa, R. Sahara, Y. Saito, N. Sakaki, T. Sako, N. Sakurai, K. Sano, K. Sato, T. Seki, K. Sekino, P. D. Shah, Y. Shibasaki, F. Shibata, N. Shibata, T. Shibata, H. Shimodaira, B. K. Shin, H. S. Shin, D. Shinto, J. D. Smith, P. Sokolsky, N. Sone, B. T. Stokes, T. A. Stroman, Y. Takagi, Y. Takahashi, M. Takamura, M. Takeda, R. Takeishi, A. Taketa, M. Takita, Y. Tameda, H. Tanaka, K. Tanaka, M. Tanaka, Y. Tanoue, S. B. Thomas, G. B. Thomson, P. Tinyakov, I. Tkachev, H. Tokuno, T. Tomida, S. Troitsky, R. Tsuda, Y. Tsunesada, Y. Uchihori, S. Udo, T. Uehama, F. Urban, T. Wong, M. Yamamoto, K. Yamazaki, J. Yang, K. Yashiro, F. Yoshida, Y. Yoshioka, Y. Zhezher, and Z. Zundel

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Physics - Atmospheric and Oceanic Physics, High Energy Physics - Experiment (hep-ex), Astrophysics::High Energy Astrophysical Phenomena, Atmospheric and Oceanic Physics (physics.ao-ph), FOS: Physical sciences, Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract

We present the first observation by the Telescope Array Surface Detector (TASD) of the effect of thunderstorms on the development of cosmic ray single count rate intensity over a 700 km$^{2}$ area. Observations of variations in the secondary low-energy cosmic ray counting rate, using the TASD, allow us to study the electric field inside thunderstorms, on a large scale, as it progresses on top of the 700 km$^{2}$ detector, without dealing with the limitation of narrow exposure in time and space using balloons and aircraft detectors. In this work, variations in the cosmic ray intensity (single count rate) using the TASD, were studied and found to be on average at the $\sim(0.5-1)\%$ and up to 2\% level. These observations were found to be both in excess and in deficit. They were also found to be correlated with lightning in addition to thunderstorms. These variations lasted for tens of minutes; their footprint on the ground ranged from 6 to 24 km in diameter and moved in the same direction as the thunderstorm. With the use of simple electric field models inside the cloud and between cloud to ground, the observed variations in the cosmic ray single count rate were recreated using CORSIKA simulations. Depending on the electric field model used and the direction of the electric field in that model, the electric field magnitude that reproduces the observed low-energy cosmic ray single count rate variations was found to be approximately between 0.2-0.4 GV. This in turn allows us to get a reasonable insight on the electric field and its effect on cosmic ray air showers inside thunderstorms.

Published
2021
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19. Observations of the Origin of Downward Terrestrial Gamma‐Ray Flashes

Author

Hideaki Shimodaira, Hyoming Jeong, Hidemi Ito, N. Inoue, Takashi Sako, D. Ikeda, M. Ohnishi, Taichi Inadomi, Tareq Abu-Zayyad, Takayuki Tomida, Toru Nakamura, Federico R. Urban, Yuya Oku, Oleg Kalashev, Fumiya Shibata, Kenichi Kadota, S. Udo, C. C. H. Jui, Pierre Sokolsky, M. Takeda, Zach Zundel, Shigehiro Nagataki, Sergey Troitsky, Toshiyuki Nonaka, M. Byrne, Kengo Sano, R. Sahara, Matt Potts, K. H. Lee, Yasunori Saito, Hiroyuki Sagawa, Ben Stokes, T.-A. Shibata, Heungsu Shin, S. B. Thomas, H. Tokuno, H. Yamaoka, Yuta Tanoue, Motoki Hayashi, J. P. Lundquist, Gordon Thomson, Tom Stroman, Robert Cady, Kiyoshi Tanaka, Michiyuki Chikawa, J. Remington, Y. Hayashi, G. Furlich, Takaaki Ishii, Igor Tkachev, Naohiro Sone, Y. Zhezher, Yoshihiko Nakamura, Akimichi Taketa, J. D. Smith, T. Fujii, Keitaro Fujita, Y. J. Kwon, Hideyuki Ohoka, Vladim Kuzmin, H. Oda, K. Kawata, D. C. Rodriguez, S. Ozawa, BayarJon Paul Lubsandorzhiev, S. Jeong, B. K. Shin, D. Rodeheffer, Naoaki Hayashida, B. G. Cheon, T. Matuyama, Kenta Yashiro, Mayuko Minamino, M. Allen, Tiffany Wong, R. Takeishi, Yuichiro Tameda, Isaac Myers, K. Honda, Ryota Fujiwara, John N. Matthews, John Belz, Elliott Barcikowski, K. Kasahara, Masaki Fukushima, Akitoshi Oshima, Fumio Kakimoto, Dmitri Ivanov, Naoto Sakaki, Paul R. Krehbiel, M. Yamamoto, Y. Takahashi, Keijiro Mukai, Masaomi Ono, Masato Takita, M. Wallace, K. Yamazaki, H. Kawai, Masaaki Tanaka, Nobuyuki Sakurai, S. Kawakami, Hiroyuki Matsumiya, Saori Kasami, A. Di Matteo, T. Seki, Takafumi Uehama, Y. Tsunesada, Maxim Pshirkov, R. Mayta, R. LeVon, Hongsu Kim, Y. Uchihori, Eiji Kido, Kei Nakai, M. V. Kuznetsov, Kazuhiro Machida, K. Sekino, William Hanlon, T. Okuda, Inkyu Park, Grigory Rubtsov, William Rison, D. R. Bergman, R. U. Abbasi, Peter Tinyakov, Samuel Blake, Shoichi Ogio, J. H. Kim, Y. Omura, Dongsu Ryu, Mark A. Stanley, Hirokazu Iwakura, Y. Takagi, Ryo Nakamura, Kazuo Saito, H. Yoshii, M. Yosei, and K. Hibino

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Atmospheric Science, 010504 meteorology & atmospheric sciences, Conjunction (astronomy), Gamma ray, FOS: Physical sciences, Astrophysics, Electron, Radio atmospheric, 01 natural sciences, Lightning, High Energy Physics - Experiment, Physics - Atmospheric and Oceanic Physics, High Energy Physics - Experiment (hep-ex), Geophysics, Space and Planetary Science, Electric field, Atmospheric and Oceanic Physics (physics.ao-ph), Earth and Planetary Sciences (miscellaneous), Atmospheric electricity, Astrophysics - High Energy Astrophysical Phenomena, Cosmic-ray observatory, 0105 earth and related environmental sciences
Abstract

In this paper we report the first close, high-resolution observations of downward-directed terrestrial gamma-ray flashes (TGFs) detected by the large-area Telescope Array cosmic ray observatory, obtained in conjunction with broadband VHF interferometer and fast electric field change measurements of the parent discharge. The results show that the TGFs occur during strong initial breakdown pulses (IBPs) in the first few milliseconds of negative cloud-to-ground and low-altitude intracloud flashes, and that the IBPs are produced by a newly-identified streamer-based discharge process called fast negative breakdown. The observations indicate the relativistic runaway electron avalanches (RREAs) responsible for producing the TGFs are initiated by embedded spark-like transient conducting events (TCEs) within the fast streamer system, and potentially also by individual fast streamers themselves. The TCEs are inferred to be the cause of impulsive sub-pulses that are characteristic features of classic IBP sferics. Additional development of the avalanches would be facilitated by the enhanced electric field ahead of the advancing front of the fast negative breakdown. In addition to showing the nature of IBPs and their enigmatic sub-pulses, the observations also provide a possible explanation for the unsolved question of how the streamer to leader transition occurs during the initial negative breakdown, namely as a result of strong currents flowing in the final stage of successive IBPs, extending backward through both the IBP itself and the negative streamer breakdown preceding the IBP., Comment: Typo fixed and reference added. Manuscript is 36 pages. Supplemental Information is 42 pages. This paper is to be published in the Journal of Geophysical Research: Atmospheres. Online data repository: Open Science Framework DOI: 10.17605/OSF.IO/Z3XDA

Published
2020
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20. Conduction gaps after pulmonary vein isolation due to high contact force ablation in patients with atrial fibrillation

Author

K Takai, K Fujita, M Takada, H Kawai, Satoshi Takahashi, Y Nishibori, T Maruyama, F Yoshikawa, and Takanao Mine

Subjects
medicine.medical_specialty, Isolation (health care), business.industry, medicine.medical_treatment, Atrial fibrillation, Ablation, medicine.disease, Pulmonary vein, Contact force, Internal medicine, medicine, Cardiology, In patient, Cardiology and Cardiovascular Medicine, business
Abstract

Background Catheter ablation for atrial fibrillation (AF) with high contact force (CF) has been reported to lead to the gaps after pulmonary vein isolation (PVI), and the appearance of the gaps depends on the site in the left atrium (LA). Purpose The aim of this study is to clarify the relationship between the gaps appearance and high CF. Methods In the clinical study, 74 consecutive patients (39 males, age 71±9, 46 with paroxysmal AF) underwent conventional PVI with a point-by-point radiofrequency (RF) ablation using a CF sensing catheter (TactiCath SETM). RF energy (J), number of RF point, Lesion index (LSI), force-time integral (FTI), average CF (g), and the degree of LA depression with high CF were evaluated. In the experimental study (figure), the relationship between the ablation area and the degree of depression with high CF using bovine left ventricular wall. Results In the clinical study, the gaps were found in 175 of 1182 sites after first path PVI ablation. The CF in the gap sites was higher than without the gap sites in RPV roof, anterior RSPV and anterior RPV carina (18.9±6.8 vs 15.0±5.7g p=0.0262, 26.4±11.6 vs 19.5±6.0g p=0.0029, 22.7±6.4 vs 19.1±5.5g, p=0.0161). Meanwhile, there were no differences in RF energy, number of RF point, LSI, FTI. High CF (≥30g) showed a depression of 3 mm or more in only RPV roof and anterior RPV (figure). In the experimental study, the ablation range narrowed as the indentation deepened with more than 30g CF (r=0.6417, p=0.0625). Conclusion Catheter ablation for AF with high contact force might lead to the gaps in RPV roof and anterior RPV site by the reduction of the ablation area due to depression caused by the pressure. Extension of each contact force Funding Acknowledgement Type of funding source: None

Published
2020
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21. Performance check of the CsI(Tl) calorimeter for the J-PARC E36 experiment by observing e+ from muon decay

Author

S. Bianchin, S. Kimura, J. Imazato, K. Horie, A. Kobayashi, H. Lu, N. Kalantarians, O. V. Mineev, Makoto Tabata, R. Tanuma, S. Kodama, Y. Igarashi, N. Yershov, D. R. Gill, Michael Kohl, H. Kawai, S. Shimizu, Hiroshi Ito, M. D. Hasinoff, B. Dongwi, and Chaden Djalali

Subjects
Physics, Nuclear and High Energy Physics, Muon, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, New energy, 01 natural sciences, Nuclear physics, 0103 physical sciences, Radiative transfer, High Energy Physics::Experiment, J-PARC, Cosmic muons, 010306 general physics, Instrumentation, Lepton
Abstract

The J-PARC E36 experiment is searching for lepton universality violation with a stopped kaon beam by measuring the ratio of the K + decay widths Γ ( K e 2 ) ∕ Γ ( K μ 2 ) = Γ ( K + → e + ν e ) ∕ Γ ( K + → μ + ν μ ) . Since the radiative K + → e + ν e γ decays are backgrounds to be removed in this measurement, the radiated γ rays were detected in a CsI(Tl) calorimeter . The energy calibration for the 768 CsI(Tl) modules was performed using mono-chromatic μ + s from the K μ 2 decays. The delayed e + signals from the muon decays were required in order to improve the S/N ratio of the K μ 2 peak by suppressing background events. In addition, a new energy calibration method of the CsI(Tl) calorimeter using stopped cosmic muons has been established.

Published
2018
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22. Gamma Ray Showers Observed at Ground Level in Coincidence With Downward Lightning Leaders

Author

Fumiya Shibata, R. W. Springer, Maxim Pshirkov, John Belz, Akitoshi Oshima, Hiroyuki Sagawa, Fumio Kakimoto, D. R. Bergman, Zach Zundel, K. Hibino, Koichi Sekino, K. Kasahara, Y. Tsunesada, Hideaki Shimodaira, Ryo Nakamura, R. LeVon, Hongsu Kim, Kazuo Saito, Shoichi Kishigami, Heungsu Shin, Shunsuke Ozawa, Mayuko Minamino, K. Honda, Hidemi Ito, K. Martens, Toshitsugu Fujii, M. Yamamoto, Y. Yoneda, N. Inoue, G. Vasiloff, Ryuji Takeishi, Masato Takita, Nobuyuki Sakurai, Masaomi Ono, Priti Shah, Hideki Tanaka, Grigory Rubtsov, M. Ohnishi, H. Yoshii, Ryota Onogi, Ben Stokes, Daisuke Ikeda, Elliott Barcikowski, Sergey Troitsky, Masaaki Tanaka, T. Matuyama, Vladim Kuzmin, Jyunsei Chiba, Dongsu Ryu, M. Allen, Helio Takai, Takayuki Tomida, Dmitri Ivanov, Tiffany Wong, B. G. Cheon, Keijiro Mukai, S. Jeong, Masaki Fukushima, B. K. Shin, K. Oki, Federico R. Urban, J. Remington, S. Udo, C. C. H. Jui, Tareq Abu-Zayyad, R. Yamane, Peter Tinyakov, Samuel Blake, Shoichi Ogio, Rasha Abbasi, William Rison, H. Kawai, Michiyuki Chikawa, M. Byrne, Naoaki Hayashida, S. Kawakami, Kiyoshi Tanaka, S. B. Thomas, Akimichi Taketa, Y. Hayashi, Toru Nakamura, K. Kawata, T. Seki, Kenichi Kadota, J. Lan, Igor Tkachev, R. Cady, J. P. Lundquist, G. Furlich, Takaaki Ishii, D. Rodeheffer, Toshiyuki Nonaka, T.-A. Shibata, Gordon Thomson, S. Yoshida, Hiroshi Yamaoka, Tom Stroman, Naoto Sakaki, Kenta Yashiro, D. C. Rodriguez, Isaac Myers, Inkyu Park, Y. Uchihori, H. Tokuno, K. Yamazaki, J. D. Smith, Yuichiro Tameda, John N. Matthews, William Hanlon, T. Okuda, J. H. Kim, J. Yang, Y. J. Kwon, Hideyuki Ohoka, Paul R. Krehbiel, T. Goto, Eiji Kido, Pierre Sokolsky, Kazuhiro Machida, M. Takeda, Shigehiro Nagataki, R. J. Thomas, and O. Kalashev

Subjects
Atmospheric Science, 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, Radiation, 01 natural sciences, High Energy Physics - Experiment, law.invention, Telescope, High Energy Physics - Experiment (hep-ex), Electron avalanche, law, 0103 physical sciences, Earth and Planetary Sciences (miscellaneous), Cosmic-ray observatory, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Lightning detection, Astrophysics::Instrumentation and Methods for Astrophysics, Gamma ray, Lightning, Physics - Atmospheric and Oceanic Physics, Geophysics, 13. Climate action, Space and Planetary Science, Atmospheric and Oceanic Physics (physics.ao-ph), Satellite, Astrophysics - High Energy Astrophysical Phenomena
Abstract

Bursts of gamma ray showers have been observed in coincidence with downward propagating negative leaders in lightning flashes by the Telescope Array Surface Detector (TASD). The TASD is a 700~square kilometer cosmic ray observatory located in southwestern Utah, U.S.A. In data collected between 2014 and 2016, correlated observations showing the structure and temporal development of three shower-producing flashes were obtained with a 3D lightning mapping array, and electric field change measurements were obtained for an additional seven flashes, in both cases co-located with the TASD. National Lightning Detection Network (NLDN) information was also used throughout. The showers arrived in a sequence of 2--5 short-duration ($\le$10~$\mu$s) bursts over time intervals of several hundred microseconds, and originated at an altitude of $\simeq$3--5 kilometers above ground level during the first 1--2 ms of downward negative leader breakdown at the beginning of cloud-to-ground lightning flashes. The shower footprints, associated waveforms and the effect of atmospheric propagation indicate that the showers consist primarily of downward-beamed gamma radiation. This has been supported by GEANT simulation studies, which indicate primary source fluxes of $\simeq$$10^{12}$--$10^{14}$ photons for $16^{\circ}$ half-angle beams. We conclude that the showers are terrestrial gamma-ray flashes (TGFs), similar to those observed by satellites, but that the ground-based observations are more representative of the temporal source activity and are also more sensitive than satellite observations, which detect only the most powerful TGFs.

Published
2018
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23. Recent progress and future prospects of hyperon nucleon scattering experiment

Author

Koji Miwa, Takuya Nanamura, Tamao Sakao, J. K. Ahn, Y. Akazawa, T. Aramaki, S. Ashikaga, S. Callier, N. Chiga, S. W. Choi, H. Ekawa, P. Evtoukhovitch, N. Fujioka, M. Fujita, T. Gogami, T. Harada, S. Hasegawa, S. H. Hayakawa, R. Honda, S. Hoshino, K. Hosomi, M. Ichikawa, Y. Ichikawa, M. Ieiri, M. Ikedai, K. Imai, Y. Ishikawa, S. Ishimoto, W. S. Jung, S. Kajikawa, H. Kanauchi, H. Kanda, T. Kitaoka, B. M. Kang, H. Kawai, S. H. Kim, K. Kobayashi, T. Koike, K. Matsuda, Y. Matsumoto, S. Nagao, R. Nagatomi, Y. Nakada, M. Nakagawa, I. Nakamura, M. Naruki, S. Ozawa, L. Raux, T. G. Rogers, A. Sakaguchi, H. Sako, S. Sato, T. Shiozaki, K. Shirotori, K. N. Suzuki, S. Suzuki, M. Tabata, C. d. L. Taille, H. Takahashi, T. Takahashi, T. N. Takahashi, H. Tamura, M. Tanaka, K. Tanida, Z. Tsamalaidze, M. Ukai, H. Umetsu, S. Wada, T. O. Yamamoto, J. Yoshida, and K. Yoshimura

Abstract

A new hyperon-proton scattering experiment, dubbed J-PARC E40, was performed to measure differential cross sections of the Σ+p, Σ−p elastic scatterings and the Σ−p → Λn scattering by identifying a lot of Σ particles in the momentum ranging from 0.4 to 0.8 GeV/c produced by the π±p → K+Σ± reactions. We successfully measured the differential cross sections of these three channels with a drastically improved accuracy with a fine angular step. These new data will become important experimental constraints to improve the theories of the two-body baryon-baryon interactions. Following this success, we proposed a new experiment to measure the differential cross sections and spin observables by using a highly polarized Λ beam for providing quantitative information on the ΛN interaction. The results of three Σp channels and future prospects of the Λp scattering experiment are described.

Published
2022
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24. Molecular characterization and antibiotic resistance of Streptococcus dysgalactiae subspecies equisimilis isolated from patients with streptococcal toxic shock syndrome

Author

T. Ikebe, R. Okuno, M. Sasaki, Y. Kanda, H. Otsuka, R. Kawahara, H. Ohya, M. Suzuki, K. Uchida, H. Nihonmatsu, M. Ohnishi, Y. Morimoto, Y. Sakamoto, S. Sato, M. Musashi, A. Shirasawa, T. Konno, T. Kobayashi, Y. Watanabe, J. Seto, Y. Kobayashi, K. Sakai, Y. Aihara, R. Kiritani, S. Kataoka, M. Takayama, N. Hamamoto, M. Nakamura, Y. Matsumoto, E. Yuzawa, H. Satoh, Y. Igawa, H. Nagaoka, H. Ehara, Y. Tsuchiya, K. Tomari, K. Takeuchi, Y. Tsunomori, H. Kawai, H. Akita, C. Kuribayashi, J. Uchida, F. Ichihara, K. semba, A. Tokaji, Y. Carle, M. Honda, E. Nakamura, M. Ogata, N. Tsuru, and T. Takara

Subjects
Adult, Male, 0301 basic medicine, Microbiology (medical), Adolescent, Genotyping Techniques, Streptococcus pyogenes, 030106 microbiology, Microbial Sensitivity Tests, Biology, medicine.disease_cause, Microbiology, Group G streptococcus, 03 medical and health sciences, Antibiotic resistance, Japan, Streptococcal Infections, Drug Resistance, Bacterial, Genotype, medicine, Humans, Pharmacology (medical), Typing, Aged, Aged, 80 and over, Antigens, Bacterial, Clindamycin, Broth microdilution, Middle Aged, Shock, Septic, Virology, Anti-Bacterial Agents, Streptococcus dysgalactiae subspecies equisimilis, Infectious Diseases, Streptococcal toxic shock syndrome, Female, Carrier Proteins, Bacterial Outer Membrane Proteins
Abstract

Streptococcal toxic shock syndrome (STSS) is a severe invasive infection characterized by the sudden onset of shock, multiorgan failure, and high mortality. Although STSS is mainly caused by Streptococcus pyogenes, group G streptococcus identified as S. dysgalactiae subsp. equisimilis (SDSE) causing STSS has also been reported; however, no study has analyzed >100 isolates of SDSE causing STSS. Therefore, we characterized the emm genotype of 173 SDSE isolates obtained from STSS patients in Japan during 2014–2016 and performed antimicrobial susceptibility testing using the broth microdilution method and emm gene typing. The predominant emm genotype was found to be stG6792, followed by stG485, stG245, stG10, stG6, and stG2078. These six genotypes constituted more than 75% of the STSS isolates. The proportion of each emm genotype in STSS isolates correlated with that in invasive isolates previously reported. We found that 16.2% of the isolates showed clindamycin resistance. The proportion of clindamycin-resistant SDSE isolates was significantly higher than that of S. pyogenes isolates. Thus, while treating STSS caused by SDSE, it is necessary to consider the possibility of clindamycin resistance and to ensure judicious use of the drug.

Published
2018
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25. Search forCPViolation inτ±→KS0π±ντDecays at Belle

Author

M. Bischofberger, H. Hayashii, K. Adamczyk, H. Aihara, V. Aulchenko, A. M. Bakich, V. Balagura, E. Barberio, K. Belous, A. Bozek, M. Bračko, T. E. Browder, P. Chen, B. G. Cheon, C.-C. Chiang, I.-S. Cho, K. Cho, Y. Choi, M. Danilov, Z. Doležal, A. Drutskoy, S. Eidelman, D. Epifanov, B. Golob, H. Ha, J. Haba, K. Hayasaka, Y. Horii, Y. Hoshi, W.-S. Hou, Y. B. Hsiung, H. J. Hyun, K. Inami, A. Ishikawa, R. Itoh, M. Iwabuchi, Y. Iwasaki, T. Julius, J. H. Kang, H. Kawai, T. Kawasaki, C. Kiesling, H. O. Kim, M. J. Kim, Y. J. Kim, K. Kinoshita, B. R. Ko, P. Kodyš, P. Križan, Y.-J. Kwon, S.-H. Kyeong, J. S. Lange, M. J. Lee, S.-H. Lee, J. Li, Y. Li, C. Liu, R. Louvot, J. MacNaughton, S. McOnie, K. Miyabayashi, H. Miyata, Y. Miyazaki, R. Mizuk, G. B. Mohanty, A. Moll, T. Mori, Y. Nagasaka, E. Nakano, M. Nakao, H. Nakazawa, S. Nishida, K. Nishimura, O. Nitoh, T. Ohshima, S. Okuno, G. Pakhlova, H. Park, H. K. Park, M. Petrič, L. E. Piilonen, M. Röhrken, S. Ryu, H. Sahoo, Y. Sakai, O. Schneider, C. Schwanda, K. Senyo, M. Shapkin, J.-G. Shiu, B. Shwartz, F. Simon, P. Smerkol, Y.-S. Sohn, S. Stanič, M. Starič, T. Sumiyoshi, Y. Teramoto, K. Trabelsi, S. Uehara, T. Uglov, S. Uno, G. Varner, A. Vinokurova, A. Vossen, C. H. Wang, P. Wang, M. Watanabe, Y. Watanabe, E. Won, H. Yamamoto, Y. Yamashita, C. Z. Yuan, P. Zhou, V. Zhulanov, and T. Zivko

Published
2011
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26. Development of slow control system for the Belle II ARICH counter

Author

T. Sumiyoshi, P. Križan, M. Yonenaga, Rok Dolenec, H. Kindo, K. Ogawa, S. Nishida, T. Kumita, K. Hataya, Y. Yusa, R. Kataura, T. Kobayashi, Makoto Tabata, H. Kawai, Luka Santelj, Ichiro Adachi, S. Iori, Hidekazu Kakuno, R. Pestotnik, Samo Korpar, S. Ogawa, Shuichi Iwata, and M. Mrvar

Subjects
Physics, Nuclear and High Energy Physics, Pixel, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, Cherenkov detector, business.industry, Detector, 01 natural sciences, 030218 nuclear medicine & medical imaging, law.invention, 03 medical and health sciences, 0302 clinical medicine, Software, Data acquisition, law, Control system, 0103 physical sciences, Scalability, High Energy Physics::Experiment, business, Instrumentation, Computer hardware, Graphical user interface
Abstract

A slow control system (SCS) for the Aerogel Ring Imaging Cherenkov (ARICH) counter in the Belle II experiment was newly developed and coded in the development frameworks of the Belle II DAQ software. The ARICH is based on 420 Hybrid Avalanche Photo-Detectors (HAPDs). Each HAPD has 144 pixels to be readout and requires 6 power supply (PS) channels, therefore a total number of 2520 PS channels and 60,480 pixels have to be configured and controlled. Graphical User Interfaces (GUIs) with detector oriented view and device oriented view, were also implemented to ease the detector operation. The ARICH SCS is in operation for detector construction and cosmic rays tests. The paper describes the detailed features of the SCS and preliminary results of operation of a reduced set of hardware which confirm the scalability to the full detector.

Published
2017
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27. Test of the HAPD light sensor for the Belle II Aerogel RICH

Author

H. Kawai, K. Hayata, H. Kakuno, K. Ogawa, T. Kumita, Makoto Tabata, Ichiro Adachi, S. Iori, S. Nishida, Samo Korpar, Rok Dolenec, Y. Yusa, R. Kataura, P. Krizan, M. Yonenaga, H. Kindo, T. Sumiyoshi, M. Mrvar, S. Iwata, Luka Santelj, T. Kobayashi, and R. Pestotnik

Subjects
Physics, Nuclear and High Energy Physics, Spectrometer, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, business.industry, Cherenkov detector, Vacuum tube, Photodetector, Avalanche photodiode, 01 natural sciences, law.invention, Electron avalanche, Optics, law, 0103 physical sciences, 010306 general physics, business, Instrumentation, Cherenkov radiation, Dark current
Abstract

The Aerogel Ring-Imaging Cherenkov detector (ARICH) is being installed in the endcap region of Belle II spectrometer to identify particles from B meson decays by detecting the Cherenkov ring image from aerogel radiators. To detect single photons, high-sensitive photon detector which has wide effective area (∼70 mm × 70 mm), a Hybrid Avalanche Photo Detector (HAPD), has been developed in a collaboration with Hamamatsu K.K. The HAPD consists of hybrid structure of a vacuum tube and an avalanche photodiode (APD). It can be operated in 1.5 T magnetic field of the spectrometer and withstands the radiation levels expected in the Belle II experiment. There are two steps of electric pulse amplification: acceleration of photo-electron in electric field in the vacuum tube part and electron avalanche in the APD part resulting in total gain of order 105. For the ARICH, we use 420 HAPDs in total. Before installing them, we performed quality assessment studies such as measurements of dark current, noise level, signal-to-noise ratio and two-dimensional scan with laser illumination. We also measured quantum efficiency of the photocathode. During the HAPD performance tests in the magnetic field, we observed very large signal pulses which cause long dead time of the readout electronics in some of the HAPDs. We have carried out a number of studies to understand this phenomenon, and have found a way to mitigate it and suppress the degradation of the ARICH performance. In this report, we will show a summary of the HAPD performance and quality assessment measurements including validation in the magnetic field for all of the HAPDs manufactured for the ARICH in the Belle II.

Published
2017
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28. Recent developments in software for the Belle II aerogel RICH

Author

T. Sumiyoshi, Iki Adachi, Samo Korpar, Rok Dolenec, K. Hataya, P. Križan, K. Ogawa, Hidekazu Kakuno, Shuichi Iwata, M. Yonenaga, H. Kawai, T. Kobayashi, M. Mrvar, S. Ogawa, H. Kindo, Luka Santelj, S. Iori, R. Pestotnik, S. Nishida, T. Kumita, Makoto Tabata, R. Kataura, and Y. Yusa

Subjects
Physics, Nuclear and High Energy Physics, Spectrometer, Physics::Instrumentation and Detectors, business.industry, Detector, Cosmic ray, Aerogel, Nuclear physics, Pion, Software, Radiator (engine cooling), High Energy Physics::Experiment, Nuclear Experiment, business, Instrumentation, Cherenkov radiation
Abstract

For the Belle II spectrometer a proximity focusing RICH counter with an aerogel radiator (ARICH) will be employed as a PID system in the forward end-cap region of the spectrometer. The detector will provide about 4 σ separation of pions and kaons up to momenta of 3.5 GeV/ c , at the kinematic limits of the experiment. We present the up-to-date status of the ARICH simulation and reconstruction software, focusing on the recent improvements of the reconstruction algorithms and detector description in the Geant4 simulation. In addition, as a demonstration of detector readout software functionality we show the first cosmic ray Cherenkov rings observed in the ARICH.

Published
2017
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29. The aerogel Ring Imaging Cherenkov system at the Belle II spectrometer

Author

S. Ogawa, T. Kobayashi, Hidekazu Kakuno, K. Ogawa, S. Nishida, Luka Santelj, M. Yonenaga, K. Hataya, M. Mrvar, Samo Korpar, H. Kindo, H. Kawai, Shuichi Iwata, R. Pestotnik, Y. Yusa, R. Kataura, Iki Adachi, T. Sumiyoshi, S. Iori, P. Križan, Makoto Tabata, Rok Dolenec, and T. Kumita

Subjects
Physics, Nuclear and High Energy Physics, Photon, Spectrometer, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, business.industry, Cherenkov detector, Detector, Cosmic ray, Solenoid, 01 natural sciences, law.invention, Optics, Data acquisition, law, 0103 physical sciences, High Energy Physics::Experiment, 010306 general physics, business, Instrumentation, Cherenkov radiation
Abstract

In the forward end-cap of the Belle II spectrometer, a proximity focusing Ring Imaging Cherenkov counter with an aerogel radiator will be installed. The detector will occupy a limited space inside solenoid magnet with longitudinal field of 1.5 T. It will consist of a double layer aerogel radiator, an expansion volume and a photon detector. 420 Hamamatsu hybrid avalanche photo sensors with 144 channels each will be used to read out single Cherenkov photons with high efficiency. More than 60,000 analog signals will be digitized and processed in the front end electronics and send to the unified experiment data acquisition system. The detector components have been successfully produced and are now being installed in the spectrometer. Tested before on the bench, they are currently being installed in the mechanical frame. Part of the detector have been commissioned and connected to the acquisition system to register the cosmic ray particles. The first preliminary results are in accordance with previous expectations. We expect an excellent performance of the device which will allow at least a 4 σ separation of pions from kaons in the experiment kinematic region from 0.5 GeV/c to 4 GeV/c.

Published
2017
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30. The bursts of high energy events observed by the telescope array surface detector

Author

Hiroshi Yamaoka, T. Suzawa, Robert M. Anderson, Hideaki Shimodaira, Isaac Myers, M. Abe, Kenta Yashiro, T. Goto, Elliott Barcikowski, Dmitri Ivanov, Keijiro Mukai, Maxim Pshirkov, Sergey Troitsky, A. L. Sampson, Takaaki Ishii, Kanako Yamazaki, Priti Shah, K. Tsutsumi, S. Kitamura, Fumiya Shibata, D. C. Rodriguez, Hidemi Ito, S. Kawakami, J. P. Lundquist, Keiji Saito, Igor Tkachev, R. Ishimori, John Belz, R. W. Springer, Pierre Sokolsky, Naoaki Hayashida, Akimichi Taketa, Ben Stokes, K. Oki, Koichi Sekino, H. Yoshii, Tareq Abu-Zayyad, R. Yamane, Federico R. Urban, Kiyoshi Tanaka, Y. Yoneda, N. Inoue, M. Ohnishi, Michiyuki Chikawa, Hiroyuki Sagawa, R. Zollinger, S. Udo, C. C. H. Jui, Heungsu Shin, M. Takeda, Shigehiro Nagataki, Ryuji Takeishi, Akitoshi Oshima, Y. Uchihori, Y. J. Kwon, Hideyuki Ohoka, K. Nagasawa, S. B. Thomas, Tomohiro Matsuda, H. Kawai, Mai Takamura, T.-A. Shibata, Fumio Kakimoto, Peter Tinyakov, Gordon Thomson, K. Hibino, Samuel Blake, Byung Gu Cheon, Tom Stroman, Robert Cady, Shoichi Ogio, Zach Zundel, Hang Bae Kim, G. Vasiloff, L. M. Scott, J. Ogura, K. Martens, Hideki Tanaka, Jyunsei Chiba, Dongsu Ryu, B. K. Shin, Takayuki Tomida, Masato Takita, Mayuko Minamino, K. Honda, Yasunori Kitamura, Rasha Abbasi, A. Nozato, Y. Hayashi, Yoshiki Tsunesada, Daisuke Ikeda, M. Allen, Inkyu Park, S. R. Stratton, K. Kawata, Masaaki Tanaka, Nobuyuki Sakurai, Tiffany Wong, Masaki Fukushima, Douglas Bergman, Takahiro Fujii, V. Kuzmin, Ryota Onogi, J. H. Kim, S. Yoshida, Naoto Sakaki, O. Kalashev, Toru Nakamura, Eiji Kido, Kazuhiro Machida, Kenichi Kadota, T. Matsuyama, S. Ozawa, Yasunori Saito, K. Kasahara, Shoichi Kishigami, R. Azuma, Yuichiro Tameda, John N. Matthews, Masaomi Ono, G. Rubtsov, Shingo Kawana, William Hanlon, T. Okuda, J. Yang, H. Tokuno, J. D. Smith, J. Lan, and Toshiyuki Nonaka

Subjects
Physics, 010504 meteorology & atmospheric sciences, Gamma ray, General Physics and Astronomy, Astronomy, Cosmic ray, Astrophysics, 01 natural sciences, Lightning, Particle detector, law.invention, Telescope, Air shower, law, 0103 physical sciences, Ultra-high-energy cosmic ray, 010306 general physics, 0105 earth and related environmental sciences, Terrestrial gamma-ray flash
Abstract

The Telescope Array (TA) experiment is designed to detect air showers induced by ultra high energy cosmic rays. The TA ground Surface particle Detector (TASD) observed several short-time bursts of air shower like events. These bursts are not likely due to chance coincidence between single shower events. The expectation of chance coincidence is less than 10 − 4 for five-year's observation. We checked the correlation between these bursts of events and lightning data, and found evidence for correlations in timing and position. Some features of the burst events are similar to those of a normal cosmic ray air shower, and some are not. On this paper, we report the observed bursts of air shower like events and their correlation with lightning.

Published
2017
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31. Search for Large-scale Anisotropy on Arrival Directions of Ultra-high-energy Cosmic Rays Observed with the Telescope Array Experiment

Author

Takashi Sako, Hideaki Shimodaira, Hyoming Jeong, Ryo Higuchi, Inkyu Park, Kenta Yashiro, R. U. Abbasi, Tareq Abu-Zayyad, R. Azuma, Fumiya Shibata, F. Kakimoto, R. Ishimori, Daisuke Ikeda, K. Yamazaki, H. Kawai, Tiffany Wong, R. Takeishi, Masaki Fukushima, Maxim Pshirkov, Hongsu Kim, B. K. Shin, Hideki Tanaka, Toshiyuki Fujii, B. G. Cheon, T. Seki, John Belz, K. Kawata, BayarJon Paul Lubsandorzhiev, Akimichi Taketa, Min Hyo Kim, G. Furlich, Takaaki Ishii, Mayuko Minamino, K. Honda, Takayuki Tomida, Seok Ho Jeong, K. H. Lee, Yuta Tanoue, Masaaki Tanaka, D. C. Rodriguez, T.-A. Shibata, S. Kawakami, Motoki Hayashi, Zach Zundel, Peter Tinyakov, Samuel Blake, Gordon Thomson, Ben Stokes, Tom Stroman, Robert Cady, J. P. Lundquist, Shoichi Ogio, Kozo Fujisue, Hiroyuki Sagawa, M. Yamamoto, M. Yosei, Hidemi Ito, Grigory Rubtsov, Koichi Sekino, Kiyoshi Tanaka, D. R. Bergman, T. Suzawa, Y. Zhezher, Heungsu Shin, Isaac Myers, Katsuaki Kasahara, Y. Takahashi, Mai Takamura, Nobuyuki Sakurai, Yuya Oku, Oleg Kalashev, K. Hibino, Shoichi Kishigami, M. Allen, Sergey Troitsky, Toru Nakamura, Kenichi Kadota, T. Matsuyama, S. Ozawa, Masaomi Ono, Toshiyuki Nonaka, Y. Uchihori, Kei Nakai, Ryota Onogi, A. Di Matteo, J. Remington, Hideyuki Ohoka, R. Mayta, Vladim Kuzmin, Ryota Fujiwara, Keitaro Fujita, Saori Kasami, Shingo Kawana, Naoto Sakaki, Naoaki Hayashida, Yoshihiko Nakamura, William Hanlon, Priti Shah, T. Okuda, J. Yang, Masato Takita, R. Sahara, Pierre Sokolsky, M. Takeda, Shigehiro Nagataki, M. Abe, Akitoshi Oshima, Y. Tsunesada, H. Tokuno, Younghoon Kwon, J. D. Smith, J. H. Kim, Elliott Barcikowski, Dmitri Ivanov, Keijiro Mukai, Jyunsei Chiba, Dongsu Ryu, Hirokazu Iwakura, Y. Takagi, Kohei Yada, Y. Omura, Igor Tkachev, Naohiro Sone, H. Oda, N. Inoue, M. Ohnishi, Taichi Inadomi, Federico R. Urban, S. Udo, C. C. H. Jui, Kengo Sano, S. B. Thomas, Yasunori Saito, Yuichiro Tameda, John N. Matthews, S. W. Kim, Hiroyuki Matsumiya, M. Chikawa, Takafumi Uehama, Eiji Kido, M. V. Kuznetsov, Kazuhiro Machida, and Ryo Nakamura

Subjects
Physics, Pierre Auger Observatory, High Energy Astrophysical Phenomena (astro-ph.HE), 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy and Astrophysics, Cosmic ray, 01 natural sciences, Auger, Computational physics, law.invention, Telescope, Dipole, Amplitude, Space and Planetary Science, law, 0103 physical sciences, Ultra-high-energy cosmic ray, Astrophysics - High Energy Astrophysical Phenomena, Anisotropy, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences
Abstract

Motivated by the detection of a significant dipole structure in the arrival directions of ultrahigh-energy cosmic rays above 8 EeV reported by the Pierre Auger Observatory (Auger), we search for a large-scale anisotropy using data collected with the surface detector array of the Telescope Array Experiment (TA). With 11 years of TA data, a dipole structure in a projection of the right ascension is fitted with an amplitude of 3.3+- 1.9% and a phase of 131 +- 33 degrees. The corresponding 99% confidence-level upper limit on the amplitude is 7.3%. At the current level of statistics, the fitted result is compatible with both an isotropic distribution and the dipole structure reported by Auger., Comment: 6 pages, 3 figures, 1 table, Proofed title. Added journal reference and DOI

Published
2020
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32. Performance evaluation of the aerogel RICH counter for the Belle II spectrometer using early beam collision data

Author

G. Nazaryan, P. Križan, Y. Lai, Hidekazu Kakuno, H. Kitamura, S. Nishida, R. Pestotnik, H. Kawai, Tomoyuki Konno, Makoto Tabata, M. Nishimura, T. Kumita, L. Burmistrov, F. Le Diberder, K. Ogawa, H. Kindo, Takeo Kawasaki, Samo Korpar, Takashi Kohriki, Y. Yusa, Masayoshi Shoji, S. Kakimoto, A. Seljak, L. Santelj, Shuichi Iwata, K. Kuze, S. Ogawa, M. Mrvar, Masakazu Kobayashi, M. Yonenaga, S. Tamechika, G. Karyan, Iki Adachi, T. Sumiyoshi, Toru Iijima, Laboratoire de l'Accélérateur Linéaire (LAL), and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)

Subjects
Photon, Physics - Instrumentation and Detectors, measurement methods, aerogel, General Physics and Astronomy, FOS: Physical sciences, BELLE, 01 natural sciences, Particle identification, 030218 nuclear medicine & medical imaging, High Energy Physics - Experiment, Nuclear physics, K: particle identification, 03 medical and health sciences, High Energy Physics - Experiment (hep-ex), 0302 clinical medicine, Pion, 0103 physical sciences, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], H14 Particle identification, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Nuclear Experiment, RICH, Cherenkov radiation, Physics, Spectrometer, 010308 nuclear & particles physics, Detector, Instrumentation and Detectors (physics.ins-det), detector: alignment, calibration, efficiency, High Energy Physics::Experiment, pi: particle identification, Event (particle physics), Beam (structure), performance
Abstract

The Aerogel Ring Imaging Cherenkov (ARICH) counter serves as a particle identification device in the forward end-cap region of the Belle II spectrometer. It is capable of identifying pions and kaons with momenta up to $4 \, {\rm GeV}/c$ by detecting Cherenkov photons emitted in the silica aerogel radiator. After the detector alignment and calibration of the probability density function, we evaluate the performance of the ARICH counter using early beam collision data. Event samples of $D^{\ast +} \to D^0 \pi^+ (D^0 \to K^-\pi^+)$ were used to determine the $\pi(K)$ efficiency and the $K(\pi)$ misidentification probability. We found that the ARICH counter is capable of separating kaons from pions with an identification efficiency of $93.5 \pm 0.6 \, \%$ at a pion misidentification probability of $10.9 \pm 0.9 \, \%$. This paper describes the identification method of the counter and the evaluation of the performance during its early operation., Comment: To be published in Prog. Theor. Exp. Phys

Published
2020
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33. Performance of the FOREST/BLC Spectrometer for Study of the $$\eta $$-nucleon Interaction via the $$\gamma d \rightarrow p\eta n$$ Reaction

Author

A. O. Tokiyasu, T. Ishikawa, Takuya Ueda, Kanae Aoki, H. Kanda, S. Miyata, Hiroyuki Fujioka, Tomoaki Hotta, Hajime Shimizu, H. Ohnishi, Kazushige Maeda, Yuki Honda, Norihito Muramatsu, Manabu Miyabe, K. Itahashi, Y Matsumura, Kyoichiro Ozawa, Yusuke Tsuchikawa, Makoto Tabata, H. Kawai, and C. Yoshida

Subjects
Nuclear physics, Physics, Photon, Meson, Spectrometer, Nuclear Theory, High Energy Physics::Experiment, Electron, Nuclear Experiment, Nucleon
Abstract

The current experimental information about interactions between the \(\eta \) meson and nucleon (N) is not enough to understand the nature of the \(\eta \) meson in a nucleus. We installed a new spectrometer and started an experiment to determine the \(\eta N\) scattering parameters at the Research Center for Electron Photon Science, Tohoku University. We present the current status of the experiment.

Published
2020
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34. Establishment of a modern experimental technique of a \(\Sigma p\) scattering experiment at J-PARC

Author

Y. Matsumoto, H. Umetsu, K. Tanida, H. Kanauchi, Toshiyuki Gogami, C. d. L. Taille, Atsushi Sakaguchi, Mifuyu Ukai, L. Raux, Megumi Naruki, Kazuhiro Suzuki, Makoto Tabata, S. Hoshino, Manami Fujita, Nobuyuki Chiga, Koji Yoshimura, S. Kajikawa, Masaharu Ieiri, M. Ikeda, S. Callier, Satoshi Sato, T. Shiozaki, Ryotaro Honda, H. Kawai, Kotaro Shirotori, T. G. Rogers, T. Aramaki, T. Harada, S. H. Hayakawa, Hiroyuki Ekawa, Takashi Yamamoto, Yuya Akazawa, Hiroyuki Sako, I. Nakamura, T. Nanamura, Junya Yoshida, R. Nagatomi, Yudai Ichikawa, K. Matsuda, Petr Evtoukhovitch, Kenichi Imai, Shoichi Hasegawa, Kenji Hosomi, S. Ozawa, Y. Nakada, N. Fujioka, M. Ichikawa, B. M. Kang, S. Y. Suzuki, Hitoshi Takahashi, Hitoshi Tamura, S. Ishimoto, Masaaki Tanaka, H. Kanda, T. Sakao, T. Takahashi, S. Ashikaga, Yoshikazu Ishikawa, Kensuke Kobayashi, J. K. Ahn, W. S. Jung, S. H. Kim, Manami Nakagawa, Z. Tsamalaidze, K. Miwa, T. N. Takahashi, Takeshi Koike, S. Nagao, S. W. Choi, Organisation de Micro-Électronique Générale Avancée (OMEGA), and École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)

Subjects
Scattering cross-section, Physics, Particle physics, Scattering, Sigma-: production, J-PARC Lab, p Sigma: scattering, Sigma, differential cross section, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], Production (computer science), J-PARC, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], talk, Analysis method
Abstract

International audience; A part of the experiment was performed in 2018 and 2019 in J-PARC. As a result of analyzing the collected data, the \(\Sigma ^{ - }\) production and the \(\Sigma ^{ - }p\) scattering reaction have been identified. It means that our new measurement and analysis method are successfully working well. Analysis for deriving the differential cross section of the \(\Sigma p\) scattering is on going.

Published
2019
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35. Study of \(\Lambda \) Identification Method by the \(\pi ^{ - }p \to K^{0}\Lambda \) Reaction for a \(\Lambda p\) Scattering Experiment at J-PARC

Author

S. Callier, H. Kawai, Kotaro Shirotori, Yudai Ichikawa, Megumi Naruki, Yuya Akazawa, H. Kanauchi, Y. Nakada, M. Ichikawa, B. M. Kang, Manami Fujita, Koji Yoshimura, T. Nanamura, Masaaki Tanaka, T. Harada, H. Umetsu, Hitoshi Tamura, T. Aramaki, Manami Nakagawa, S. Ishimoto, T. Sakao, K. Matsuda, Petr Evtoukhovitch, Y. Matsumoto, S. Ashikaga, Yoshikazu Ishikawa, Takashi Yamamoto, Z. Tsamalaidze, Junya Yoshida, T. G. Rogers, Shoichi Hasegawa, Toshiyuki Gogami, C. d. L. Taille, R. Nagatomi, Kensuke Kobayashi, K. Tanida, Makoto Tabata, L. Raux, Kenichi Imai, Satoshi Sato, Ryotaro Honda, S. Hoshino, S. W. Choi, W. S. Jung, Atsushi Sakaguchi, Mifuyu Ukai, Kazuhiro Suzuki, K. Miwa, Hitoshi Takahashi, Kenji Hosomi, S. H. Hayakawa, I. Nakamura, S. Kajikawa, S. Nagao, H. Kanda, T. Takahashi, Tadayuki Takahashi, S. H. Kim, J. K. Ahn, Hiroyuki Sako, S. Ozawa, N. Fujioka, S. Y. Suzuki, M. Ikeda, Organisation de Micro-Électronique Générale Avancée (OMEGA), and École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)

Subjects
p Lambda: scattering, momentum: missing-energy, Particle physics, Proton, Hypernuclear Physics, Lambda, Momentum, mass spectrum, p: target, +K0+Lambda%22">pi- p --> K0 Lambda, Pi, [PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex], [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], Spectroscopy, cluster, Particle Physics, Physics, Scattering, J-PARC Lab, Strangeness, K0: decay, magnetic spectrometer, J-PARC, Mass spectrum, missing-mass, talk
Abstract

International audience; The \(\pi ^{ - }p \to K^{0}\Lambda \) reaction is an important elementary process to produce \(\Lambda \) from a proton target and is a key for a \(\Lambda p\) scattering experiment where the momentum of \(\Lambda \) should be tagged from the missing momentum of the \((\pi ^{ - },K^{0})\) reaction. However, the \((\pi ^{ - },K^{0})\) spectroscopy method has not been established yet due to the difficulty of the K^0 detection. Therefore, we have proposed a new K^0 detection method where \(\pi ^{ + }\) and \(i^{ - }\) from the K^0 decay are measured by a forward magnetic spectrometer and a detector cluster surrounding the target, respectively. The feasibility of the K^0 detection method was confirmed by analyzing the J-PARC E40 data taken with such a detector system. In the analysis, \(\Lambda \)’s were successfully identified in the missing mass spectrum of the \(\pi ^{ - }p \to K^{0}X\) reaction.

Published
2019
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38. Search for Ultra-High-Energy Neutrinos with the Telescope Array Surface Detector

Author

Koichi Sekino, Y. Takahashi, Mai Takamura, S. Kitamura, Hidemi Ito, K. Martens, Yuta Tanoue, Motoki Hayashi, J. P. Lundquist, K. Tsutsumi, John Belz, Heungsu Shin, Vladim Kuzmin, Takashi Sako, Toru Nakamura, Inkyu Park, Kenichi Kadota, Yana Zhezher, Hiroyuki Sagawa, D. R. Bergman, Maxim Pshirkov, Charlie Jui, BayarJon Paul Lubsandorzhiev, Mayuko Minamino, K. Yamazaki, M. Abe, K. H. Lee, K. Honda, Daisuke Ikeda, S. R. Stratton, Yasunori Kitamura, T.-A. Shibata, Gordon Thomson, Toshiyuki Fujii, Ryo Nakamura, Tom Stroman, Robert Cady, Masaaki Tanaka, Fumiya Shibata, M. Yamamoto, Nobuyuki Sakurai, Tiffany Wong, R. Takeishi, L. M. Scott, Hongsu Kim, Y. Hayashi, R. Ishimori, Masaki Fukushima, Kazuo Saito, Ben Stokes, N. Inoue, M. Ohnishi, Y. J. Kwon, Akimichi Taketa, Eiji Kido, B. G. Cheon, H. Kawai, K. Kawata, Federico R. Urban, M. V. Kuznetsov, Ryota Onogi, Hideyuki Ohoka, Pierre Sokolsky, A. Di Matteo, H. Yoshii, S. Udo, Kazuhiro Machida, Hideaki Shimodaira, Hyoming Jeong, M. Takeda, Shigehiro Nagataki, R. Mayta, T. Seki, Seok Ho Jeong, S. B. Thomas, Peter Tinyakov, Samuel Blake, Oleg Kalashev, Shoichi Ogio, Priti Shah, Igor Tkachev, Zach Zundel, S. Kawakami, Fumio Kakimoto, Tareq Abu-Zayyad, K. Nagasawa, H. Oda, H. Tokuno, R. Azuma, Toshiyuki Nonaka, K. Hibino, Kenta Yashiro, Akitoshi Oshima, Y. Tsunesada, Keitaro Fujita, B. K. Shin, H. Yamaoka, Michiyuki Chikawa, Masato Takita, J. D. Smith, Sergey Troitsky, Y. Omura, J. Remington, J. H. Kim, Elliott Barcikowski, Dmitri Ivanov, Jyunsei Chiba, Keijiro Mukai, Naoaki Hayashida, Shingo Kawana, Dongsu Ryu, Y. Takagi, Yasunori Saito, William Hanlon, T. Okuda, J. Yang, Yuichiro Tameda, John N. Matthews, Kohei Yada, Hideki Tanaka, Takayuki Tomida, K. Kasahara, Shoichi Kishigami, Kiyoshi Tanaka, Grigory Rubtsov, M. Allen, Masaomi Ono, R. Sahara, Ryota Fujiwara, Naoto Sakaki, Y. Uchihori, Kei Nakai, Rasha Abbasi, T. Matsuyama, S. Ozawa, T. Suzawa, J. Ogura, Isaac Myers, G. Furlich, Takaaki Ishii, and D. C. Rodriguez

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Physics, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Detector, FOS: Physical sciences, General Physics and Astronomy, Flux, Observable, Cosmic ray, 01 natural sciences, law.invention, Telescope, Optics, Distribution function, law, 0103 physical sciences, Alternating decision tree, High Energy Physics::Experiment, Neutrino, 010306 general physics, business, Astrophysics - High Energy Astrophysical Phenomena
Abstract

We present an upper limit on the flux of ultra-high-energy down-going neutrinos for $E > 10^{18}\ \mbox{eV}$ derived with the nine years of data collected by the Telescope Array surface detector (05-11-2008 -- 05-10-2017). The method is based on the multivariate analysis technique, so-called Boosted Decision Trees (BDT). Proton-neutrino classifier is built upon 16 observables related to both the properties of the shower front and the lateral distribution function., 10 pages, 4 figures, accepted to JETP

Published
2019

39. Geographical and seasonal characteristics of APHRODITE and GSMaP in Lao P.D.R

Author

K Noda, M K Zaki, and H Kawai

Subjects
Environmental science
Abstract

Water-related hazards account for 90 percent of all-natural hazards, and their frequency is generally rising, in association with climate change. To combat climate change, real-time and gridded precipitation data is important, especially where no ground observation is operated. Hence, this study aimed to assess the performances of different gridded precipitation datasets, APHRODITE and GSMaP in geographical and climate terms, in Lao P.D.R. For the elevation factor, precipitation at the time of conversion from over to underestimation of GSMaP was found to be dependent on elevation, as the conversions occur with lower precipitation in higher elevation classes. About the climate factor, we also found that the conversion happened at smallest precipitation in the end of rainy season, then beginning of rainy season and then middle of the rainy season.

Published
2021
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40. The Cosmic-Ray Composition between 2 PeV and 2 EeV Observed with the TALE Detector in Monocular Mode

Author

BayarJon Paul Lubsandorzhiev, Mayuko Minamino, K. Honda, Masaaki Tanaka, Ryuji Takeishi, Hiroyuki Sagawa, Yasunori Saito, Pierre Sokolsky, B. K. Shin, M. Takeda, M. Yamamoto, Shigehiro Nagataki, R. Sahara, Toshiyuki Fujii, Shingo Kawana, William Hanlon, T. Okuda, J. Yang, M. Allen, Seok Ho Jeong, Nobuyuki Sakurai, K. H. Lee, T.-A. Shibata, Shoichi Kishigami, Yuichiro Tameda, John N. Matthews, Zach Zundel, T. Suzawa, Fugo Yoshida, Gordon Thomson, Tom Stroman, Fumiya Shibata, Ryota Onogi, Saori Kasami, D. Ikeda, Robert Cady, S. W. Kim, Ryosuke Tsuda, Isaac Myers, Hidemi Ito, R. Mayta, Masaomi Ono, H. Kawai, K. Kawata, N. Inoue, B. G. Cheon, Katsuaki Kasahara, J. H. Kim, Takashi Sako, T. Seki, Kiyoshi Tanaka, Koichi Sekino, M. Ohnishi, Min Hyo Kim, Takayuki Tomida, Grigory Rubtsov, Hideki Tanaka, Peter Tinyakov, Samuel Blake, Toshiyuki Nonaka, Taichi Inadomi, Norimichi Shibata, Y. Omura, Hideaki Shimodaira, Hyoming Jeong, Shoichi Ogio, Younghoon Kwon, Inkyu Park, John Belz, T. Matsuyama, Ryo Higuchi, Ryota Fukushima, S. Ozawa, Katsuya Yamazaki, Y. Nakamura, Federico R. Urban, Heungsu Shin, Kohei Yada, S. Kawakami, Keitaro Fujita, Y. Takahashi, Mai Takamura, Elliott Barcikowski, R. U. Abbasi, Y. Uchihori, Kei Nakai, Maxim Pshirkov, Dmitri Ivanov, S. Udo, C. C. H. Jui, Koki Sato, Tiffany Wong, Yuto Arai, Keijiro Mukai, Hiroyuki Matsumiya, Masaki Fukushima, Yusuke Kimura, Akimichi Taketa, Yuta Tanoue, Ryota Fujiwara, M. Chikawa, Takafumi Uehama, Tareq Abu-Zayyad, Motoki Hayashi, G. Furlich, Takaaki Ishii, J. P. Lundquist, Jyunsei Chiba, Naoto Sakaki, Daiki Shinto, Eiji Kido, M. V. Kuznetsov, Kazuhiro Machida, D. C. Rodriguez, Kozo Fujisue, Kengo Sano, Priti Shah, Dongsu Ryu, S. B. Thomas, Hirokazu Iwakura, Y. Takagi, Igor Tkachev, Naohiro Sone, H. Oda, Kenta Yashiro, Masato Takita, F. Kakimoto, Hongsu Kim, Sergey Troitsky, J. Remington, Naoaki Hayashida, Akitoshi Oshima, Y. Tsunesada, Ben Stokes, Y. Zhezher, Hideyuki Ohoka, Vladim Kuzmin, Toru Nakamura, Kenichi Kadota, M. Abe, Yuya Oku, Oleg Kalashev, Ryo Nakamura, D. R. Bergman, K. Hibino, H. Tokuno, and J. D. Smith

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Astroparticle physics, Physics, Monocular, Astrophysics::High Energy Astrophysical Phenomena, Detector, Mode (statistics), FOS: Physical sciences, Astronomy and Astrophysics, Cosmic ray, Astrophysics, 030226 pharmacology & pharmacy, 01 natural sciences, 03 medical and health sciences, 0302 clinical medicine, Space and Planetary Science, 0103 physical sciences, Astrophysics - High Energy Astrophysical Phenomena, 010303 astronomy & astrophysics
Abstract

We report on a measurement of the cosmic ray composition by the Telescope Array Low-Energy Extension (TALE) air fluorescence detector (FD). By making use of the Cherenkov light signal in addition to air fluorescence light from cosmic ray (CR) induced extensive air showers, the TALE FD can measure the properties of the cosmic rays with energies as low as $\sim 2$ PeV and exceeding 1 EeV. In this paper, we present results on the measurement of $X_{\rm max}$ distributions of showers observed over this energy range. Data collected over a period of $\sim 4$ years was analyzed for this study. The resulting $X_{\rm max}$ distributions are compared to the Monte Carlo (MC) simulated data distributions for primary cosmic rays with varying composition and a 4-component fit is performed. The comparison and fit are performed for energy bins, of width 0.1 or 0.2 in $\log_{10} (E/{\rm eV})$, spanning the full range of the measured energies. We also examine the mean $X_{\rm max}$ value as a function of energy for cosmic rays with energies greater than $10^{15.8}$ eV. Below $10^{17.3}$ eV, the slope of the mean $X_{\rm max}$ as a function of energy (the elongation rate) for the data is significantly smaller than that of all elements in the models, indicating that the composition is becoming heavier with energy in this energy range. This is consistent with a rigidity-dependent cutoff of events from galactic sources. Finally, an increase in the $X_{\rm max}$ elongation rate is observed at energies just above $10^{17}$ eV indicating another change in the cosmic rays composition., 20 pages, 22 figures, accepted for publication in ApJ

Published
2021
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41. Studies of a hybrid avalanche photo-detector in magnetic field

Author

T. Sumiyoshi, Shuichi Iwata, P. Križan, A. Stanovnik, S. Ogawa, K. Nath, Makoto Tabata, H. Kindo, Samo Korpar, Hidekazu Kakuno, E. Tahirović, Luka Santelj, Iki Adachi, Y. Yusa, S. Nishida, R. Pestotnik, S. Iori, H. Kawai, A. Seljak, M. Mrvar, R. Kataura, and K. Hataya

Subjects
Physics, Nuclear and High Energy Physics, Photon, Spectrometer, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, business.industry, Photodetector, Dead time, Radiation, 01 natural sciences, Signal, 010305 fluids & plasmas, Magnetic field, Optics, 0103 physical sciences, Photonics, business, Instrumentation
Abstract

For the Belle II spectrometer a proximity focusing RICH counter with an aerogel radiator (ARICH) will be employed as a PID system in the forward endcap region of the spectrometer. The main challenge was the development of a reliable multichannel sensor for single photons that operates in the high magnetic field of the spectrometer (1.5 T) and withstands the radiation levels expected at the experiment. A 144-channel Hybrid Avalanche Photo-Detector (HAPD) was developed with Hamamatsu Photonics K.K. and the mass production of ∼480 HAPDs was completed recently. While our first tests of HAPD performance in the magnetic field (before mass production) showed no issues, we lately observed a presence of very large signal pulses (∼5000× single photon signal), generated internally within about 20% of HAPDs, while operating in the magnetic field. The rate of these pulses varies from sample to sample. These pulses impact the HAPD performance in two ways: they introduce periods of dead time and, in some cases, damage to the front-end electronics was observed. Here we present conditions under which such large pulses are generated, their properties and impact on HAPD performance, and discuss possible mechanism of their origin.

Published
2017
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42. Low-energy scattering parameters between the eta meson and nucleon from eta photoproduction on the deuteron

Author

Hiroaki Ohnishi, H. Kanda, Hajime Shimizu, Y. Inoue, Makoto Tabata, Hiroyuki Fujioka, T. Nishi, S. Miyata, A. O. Tokiyasu, Norihito Muramatsu, R. Shirai, H. Yamazaki, Yuji Matsumura, K. Maeda, K. Itahashi, K. Aoki, Tomoaki Hotta, Yusuke Tsuchikawa, Manabu Miyabe, Kyoichiro Ozawa, Yuki Honda, Takatsugu Ishikawa, and H. Kawai

Subjects
Physics, Particle physics, Low energy, Deuterium, 010308 nuclear & particles physics, 0103 physical sciences, Eta meson, Scattering parameters, General Physics and Astronomy, 010306 general physics, Nucleon, 01 natural sciences
Published
2017

43. First upper limits on the radar cross section of cosmic-ray induced extensive air showers

Author

John Belz, Eiji Kido, Nobuyuki Sakurai, Fumiya Shibata, Kazuhiro Machida, R. Ishimori, Takahiro Fujii, Helio Takai, M. Abou Bakr Othman, Maxim Pshirkov, J. H. Kim, W. R. Cho, C. Jayanthmurthy, O. Kalashev, R. W. Springer, Peter Tinyakov, Samuel Blake, Shoichi Ogio, Charlie Jui, Mayuko Minamino, K. Honda, Yasunori Kitamura, Masaaki Tanaka, G. Vasiloff, J. P. Lundquist, Toru Nakamura, Jyunsei Chiba, Kenichi Kadota, Akitoshi Oshima, Dongsu Ryu, Ryuji Takeishi, M. J. Chae, S. Kitamura, Hidemi Ito, K. Nagasawa, Y. Uchihori, Hideaki Shimodaira, Hiroyuki Sagawa, Fumio Kakimoto, T. Matsuyama, D. Z. Besson, M. Allen, Y. J. Kwon, Michiyuki Chikawa, Priti Shah, T. Suzawa, Hideyuki Ohoka, Isaac Myers, K. Oki, Y. Yoneda, N. Inoue, S. I. Lim, M. Ohnishi, Tomohiro Matsuda, S. Prohira, Masato Takita, Suresh Venkatesh, K. Yamazaki, J. Ogura, Mai Takamura, Tareq Abu-Zayyad, R. Yamane, Ahmad RezazadehReyhani, Toshiyuki Nonaka, T. Goto, S. Udo, R. Azuma, Rasha Abbasi, Hiroshi Yamaoka, Pierre Sokolsky, Yuichiro Tameda, B. G. Cheon, John N. Matthews, L. M. Scott, Zach Zundel, Behrouz Farhang-Boroujeny, Takaaki Ishii, Bokkyun Shin, A. Nozato, Y. Hayashi, Sergey Troitsky, Hongsu Kim, A. L. Sampson, K. Kawata, D. C. Rodriguez, V. Kuzmin, S. Kawakami, Akimichi Taketa, K. Martens, H. Kawai, S. Yoshida, Hideki Tanaka, M. Takeda, Daisuke Ikeda, M. Byrne, S. B. Thomas, S. R. Stratton, Shigehiro Nagataki, Tiffany Wong, Masaki Fukushima, J. Lan, Douglas Bergman, Ross Anderson, Kiyoshi Tanaka, Kenta Yashiro, K. Tsutsumi, R. Zollinger, Naoaki Hayashida, M. Abe, S. Kunwar, Igor Tkachev, R. Cady, David Schurig, K. Hibino, H. Yoshii, Y. Tsunesada, Shunsuke Ozawa, Ben Stokes, Elliott Barcikowski, Dmitri Ivanov, Keijiro Mukai, Federico R. Urban, T.-A. Shibata, Gordon Thomson, Tom Stroman, Inkyu Park, K. Kasahara, Masaomi Ono, G. Rubtsov, Takayuki Tomida, W.H. Gillman, H. Tokuno, J. D. Smith, Shingo Kawana, William Hanlon, T. Okuda, J. Yang, and J. C. Hanson

Subjects
Physics, Radar cross-section, Physics::Instrumentation and Detectors, Pulse-Doppler radar, business.industry, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astronomy and Astrophysics, 01 natural sciences, law.invention, Continuous-wave radar, Radar engineering details, Optics, Radar astronomy, law, Radar imaging, 0103 physical sciences, Radar, Radar display, Astrophysics - Instrumentation and Methods for Astrophysics, 010306 general physics, business, Instrumentation and Methods for Astrophysics (astro-ph.IM), 010303 astronomy & astrophysics, Remote sensing
Abstract

TARA (Telescope Array Radar) is a cosmic ray radar detection experiment colocated with Telescope Array, the conventional surface scintillation detector (SD) and fluorescence telescope detector (FD) near Delta, Utah, U.S.A. The TARA detector combines a 40 kW, 54.1 MHz VHF transmitter and high-gain transmitting antenna which broadcasts the radar carrier over the SD array and within the FD field of view, towards a 250 MS/s DAQ receiver. TARA has been collecting data since 2013 with the primary goal of observing the radar signatures of extensive air showers (EAS). Simulations indicate that echoes are expected to be short in duration (~10 microseconds) and exhibit rapidly changing frequency, with rates on the order of 1 MHz/microsecond. The EAS radar cross-section (RCS) is currently unknown although it is the subject of over 70 years of speculation. A novel signal search technique is described in which the expected radar echo of a particular air shower is used as a matched filter template and compared to waveforms obtained by triggering the radar DAQ using the Telescope Array fluorescence detector. No evidence for the scattering of radio frequency radiation by EAS is obtained to date. We report the first quantitative RCS upper limits using EAS that triggered the Telescope Array Fluorescence Detector., Comment: 21 pages, 30 figures

Published
2017
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44. Search for EeV protons of galactic origin

Author

R. Ishimori, R. Zollinger, Kenta Yashiro, Yasunori Saito, Yuichiro Tameda, John N. Matthews, K. Nagasawa, J. Yang, Y. J. Kwon, Eiji Kido, Hideyuki Ohoka, Kazuhiro Machida, J. Lan, S. Kitamura, Masato Takita, M. Abe, Byung Gu Cheon, Hidemi Ito, John Belz, Toshiyuki Nonaka, Elliott Barcikowski, Takayuki Tomida, Igor Tkachev, R. Cady, Motoki Hayashi, J. P. Lundquist, Ryuji Takeishi, BayarJon Paul Lubsandorzhiev, K. Hibino, Ben Stokes, Inkyu Park, T. Matsuyama, L. M. Scott, S. Ozawa, Dmitri Ivanov, Keijiro Mukai, Hiroshi Yamaoka, Tomohiro Matsuda, Mayuko Minamino, K. Honda, Y. Yoneda, N. Inoue, Federico R. Urban, A. Nozato, Y. Hayashi, K. Oki, M. Ohnishi, Yasunori Kitamura, T. Goto, S. Udo, C. C. H. Jui, K. Kawata, M. Allen, Douglas Bergman, Yoshiki Tsunesada, Nobuyuki Sakurai, Masaaki Tanaka, Sergey Troitsky, Daisuke Ikeda, Hideaki Shimodaira, Toru Nakamura, Kenichi Kadota, S. R. Stratton, H. Kawai, K. Kasahara, Akitoshi Oshima, S. B. Thomas, O. Kalashev, Shoichi Kishigami, Koichi Sekino, Kanako Yamazaki, Takahiro Fujii, Tiffany Wong, Priti Shah, K. Saito, Masaki Fukushima, Masaomi Ono, Jyunsei Chiba, Dongsu Ryu, B. K. Shin, Grigory Rubtsov, K. Martens, Hideki Tanaka, S. Yoshida, Y. Takahashi, Mai Takamura, Ryota Onogi, J. H. Kim, Vladim Kuzmin, H. Yoshii, Tareq Abu-Zayyad, A. H. Tirone, R. Yamane, Kiyoshi Tanaka, J. Ogura, Naoto Sakaki, Naoaki Hayashida, Peter Tinyakov, Samuel Blake, Maxim Pshirkov, Shoichi Ogio, T.-A. Shibata, Gordon Thomson, Tom Stroman, Zach Zundel, Pierre Sokolsky, Hang Bae Kim, Akimichi Taketa, Heungsu Shin, Rasha Abbasi, M. Takeda, Fumio Kakimoto, Shigehiro Nagataki, Michiyuki Chikawa, K. Tsutsumi, R. Azuma, S. Kawakami, Hiroyuki Sagawa, Y. Uchihori, T. Suzawa, Isaac Myers, Takaaki Ishii, D. C. Rodriguez, Shingo Kawana, William Hanlon, T. Okuda, H. Tokuno, J. D. Smith, and Fumiya Shibata

Subjects
High Energy Astrophysical Phenomena (astro-ph.HE), Physics, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Galactic anticenter, FOS: Physical sciences, Astronomy, Astronomy and Astrophysics, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Galactic plane, 01 natural sciences, Galactic tide, law.invention, Telescope, law, 0103 physical sciences, Galactic corona, Astrophysics - High Energy Astrophysical Phenomena, Anisotropy, Longitude, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics
Abstract

Cosmic rays in the energy range $10^{18.0}$ - $10^{18.5}$ eV are thought to have a light, probably protonic, composition. To study their origin one can search for anisotropy in their arrival directions. Extragalactic cosmic rays should be isotropic, but galactic cosmic rays of this type should be seen mostly along the galactic plane, and there should be a shortage of events coming from directions near the galactic anticenter. This is due to the fact that, under the influence of the galactic magnetic field, the transition from ballistic to diffusive behavior is well advanced, and this qualitative picture persists over the whole energy range. Guided by models of the galactic magnetic field that indicate that the enhancement along the galactic plane should have a standard deviation of about 20$^\circ$ in galactic latitude, and the deficit in the galactic anticenter direction should have a standard deviation of about 50$^\circ$ in galactic longitude, we use the data of the Telescope Array surface detector in $10^{18.0}$ to $10^{18.5}$ eV energy range to search for these effects. The data are isotropic. Neither an enhancement along the galactic plane nor a deficit in the galactic anticenter direction is found. Using these data we place an upper limit on the fraction of EeV cosmic rays of galactic origin at 1.3% at 95% confidence level.

Published
2017
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45. Aligning Potency and Pharmacokinetic Properties for Pyridine-Based NCINIs

Author

Steven R. LaPlante, René Coulombe, Thao Trinh, Dominik Wernic, Rebekah J. Carson, Nathalie Rioux, Bruno Simoneau, Catherine Chabot, Youla S. Tsantrizos, Jianmin Duan, Simon Surprenant, Pierre R. Bonneau, Carl Thibeault, Stephen W. Mason, Serge Landry, Craig Fenwick, François Bilodeau, Araz Jakalian, Murray D. Bailey, Stephen H. Kawai, Clint James, Yves Bousquet, Bounkham Thavonekham, Michel Garneau, Eric Beaulieu, Sébastien Morin, Christiane Yoakim, Ted Halmos, Lee Fader, and Jennifer Tsoung

Subjects
0301 basic medicine, 010405 organic chemistry, Organic Chemistry, Integrase inhibitor, Biology, Pharmacology, 01 natural sciences, Biochemistry, Desymmetrization, Virus, Chemical space, 0104 chemical sciences, Integrase, 03 medical and health sciences, chemistry.chemical_compound, 030104 developmental biology, Pharmacokinetics, chemistry, Drug Discovery, Pyridine, biology.protein, Potency
Abstract

Optimization of pyridine-based noncatalytic site integrase inhibitors (NCINIs) based on compound 2 has led to the discovery of molecules capable of inhibiting virus harboring N124 variants of HIV integrase (IN) while maintaining minimal contribution of enterohepatic recirculation to clearance in rat. Structure-activity relationships at the C6 position established chemical space where the extent of enterohepatic recirculation in the rat is minimized. Desymmetrization of the C4 substituent allowed for potency optimization against virus having the N124 variant of integrase. Combination of these lessons led to the discovery of compound 20, having balanced serum-shifted antiviral potency and minimized excretion in to the biliary tract in rat, potentially representing a clinically viable starting point for a new treatment option for individuals infected with HIV.

Published
2016
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46. Behaviour of Belle II ARICH Hybrid Avalanche Photo-Detector in magnetic field

Author

T. Sumiyoshi, T. Kobayashi, Luka Santelj, Y. Yusa, Rok Dolenec, S. Ogawa, K. Ogawa, R. Pestotnik, Iki Adachi, P. Kriz^an, T. Konno, S. Iori, M. Yonenaga, K. Hataya, S. Korpar, H. Kawai, M. Mrvar, Makoto Tabata, H. Kindo, Hidekazu Kakuno, Shuichi Iwata, R. Kataura, T. Kumita, and S. Nishida

Subjects
Physics, Nuclear and High Energy Physics, APDS, 010308 nuclear & particles physics, business.industry, Cherenkov detector, Detector, Electrical engineering, Photodetector, Biasing, Dead time, 01 natural sciences, Signal, law.invention, Nuclear physics, law, 0103 physical sciences, 010306 general physics, business, Instrumentation, Voltage
Abstract

The proximity-focusing Aerogel Ring-Imaging Cherenkov detector (ARICH) has been designed to separate kaons from pions in the forward end-cap of the Belle II spectrometer. The detector will be placed in 1.5 T magnetic field and must have immunity to it. In ARICH R&D, we solve the problem with new equipment called Hybrid Avalanche Photo-Detector (HAPD) which developed by Hamamatsu Photonics. Recently the production of about 500 HAPDs was completed. We test HAPDs in magnetic field in KEK. We found some HAPDs have significant amount of dead time, which reaches up to 30% in the worst case. The dead time is caused by very large (more than 10,000 times larger than a single photon signal) and frequent (∼5 Hz) signals, which make electronics paralysed. The huge signals are observed in about 30% of HAPDs. To identify the origin and understand the mechanism, we perform some extra test of HAPDs. We find a strange dependence of the huge signals to the APD bias voltage. If we reduce the bias voltage applied to one of the 4 APDs by 10 V, the frequency of the huge signals is much reduced. On the other hand, if we reduce the voltage of all the 4 HAPDs, huge signals do not decrease, or even increase in some case. We also find the huge signals seems to be related to the vacuum inside HAPD. We present about the observation of the huge signals of HAPDs in the magnetic field, and our strategy to manage it.

Published
2017
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47. Study of ∑N interaction from the ∑p scattering experiment at J-PARC

Author

Kenji Hosomi, T. Aramaki, H. Kanauchi, Shoichi Hasegawa, Manami Nakagawa, S. Ozawa, Y. Matsumoto, Hitoshi Takahashi, Makoto Tabata, N. Fujioka, Z. Tsamalaidze, Tadayuki Takahashi, T. Nanamura, S. Y. Suzuki, S. Callier, Satoshi Sato, Ryotaro Honda, R. Nagatomi, T. Shiozaki, T. G. Rogers, L. Raux, H. Kawai, Kotaro Shirotori, Hiroyuki Ekawa, S. H. Kim, Toshiyuki Gogami, C. d. L. Taille, S. Hoshino, S. H. Hayakawa, Yuya Akazawa, Yudai Ichikawa, S. Ishimoto, M. Ichikawa, B. M. Kang, J. K. Ahn, H. Kanda, K. Miwa, Y. Nakada, H. Umetsu, T. Takahashi, T. Harada, Kenichi Imai, W. S. Jung, Masaharu Ieiri, S. W. Choi, M. Ikeda, Takeshi Koike, Hiroyuki Sako, Masaaki Tanaka, T. Sakao, S. Ashikaga, Yoshikazu Ishikawa, Junya Yoshida, Hitoshi Tamura, Mifuyu Ukai, Kazuhiro Suzuki, Takashi Yamamoto, Kensuke Kobayashi, S. Nagao, Manami Fujita, Koji Yoshimura, K. Matsuda, Petr Evtoukhovitch, Megumi Naruki, Nobuyuki Chiga, S. Kajikawa, I. Nakamura, K. Tanida, and Atsushi Sakaguchi

Subjects
Nuclear physics, Physics, History, 010308 nuclear & particles physics, Scattering, 0103 physical sciences, J-PARC, 010306 general physics, 01 natural sciences, Computer Science Applications, Education
Abstract

A high statistics ∑p scattering experiment has been performed at the K1.8 beamline in the J-PARC Hadron Experimental Facility. Data for momentum-tagged ∑− beam running in a liquid hydrogen target were accumulated by detecting the π − p → K + ∑ − reaction with a high intensity π− beam of 20 M/spill. The number of the Σ− beam was about 1.7 × 107 in total. The ∑−ρ elastic scattering and the ∑−p → Λn inelastic scattering events were successfully observed with about 100 times larger statistics than that in past experiments.

Published
2020
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48. Evidence for a Supergalactic Structure of Magnetic Deflection Multiplets of Ultra-high-energy Cosmic Rays

Author

R. U. Abbasi, M. Abe, T. Abu-Zayyad, M. Allen, R. Azuma, E. Barcikowski, J. W. Belz, D. R. Bergman, S. A. Blake, R. Cady, B. G. Cheon, J. Chiba, M. Chikawa, A. di Matteo, T. Fujii, K. Fujisue, K. Fujita, R. Fujiwara, M. Fukushima, G. Furlich, W. Hanlon, M. Hayashi, N. Hayashida, K. Hibino, R. Higuchi, K. Honda, D. Ikeda, T. Inadomi, N. Inoue, T. Ishii, R. Ishimori, H. Ito, D. Ivanov, H. Iwakura, H. M. Jeong, S. Jeong, C. C. H. Jui, K. Kadota, F. Kakimoto, O. Kalashev, K. Kasahara, S. Kasami, H. Kawai, S. Kawakami, S. Kawana, K. Kawata, E. Kido, H. B. Kim, J. H. Kim, M. H. Kim, S. W. Kim, S. Kishigami, V. Kuzmin, M. Kuznetsov, Y. J. Kwon, K. H. Lee, B. Lubsandorzhiev, J. P. Lundquist, K. Machida, H. Matsumiya, T. Matsuyama, J. N. Matthews, R. Mayta, M. Minamino, K. Mukai, I. Myers, S. Nagataki, K. Nakai, R. Nakamura, T. Nakamura, Y. Nakamura, T. Nonaka, H. Oda, S. Ogio, M. Ohnishi, H. Ohoka, Y. Oku, T. Okuda, Y. Omura, M. Ono, R. Onogi, A. Oshima, S. Ozawa, I. H. Park, M. S. Pshirkov, J. Remington, D. C. Rodriguez, G. Rubtsov, D. Ryu, H. Sagawa, R. Sahara, Y. Saito, N. Sakaki, T. Sako, N. Sakurai, K. Sano, T. Seki, K. Sekino, P. D. Shah, F. Shibata, T. Shibata, H. Shimodaira, B. K. Shin, H. S. Shin, J. D. Smith, P. Sokolsky, N. Sone, B. T. Stokes, T. A. Stroman, T. Suzawa, Y. Takagi, Y. Takahashi, M. Takamura, R. Takeishi, A. Taketa, M. Takita, Y. Tameda, H. Tanaka, K. Tanaka, M. Tanaka, Y. Tanoue, S. B. Thomas, G. B. Thomson, P. Tinyakov, I. Tkachev, H. Tokuno, T. Tomida, S. Troitsky, Y. Tsunesada, Y. Uchihori, S. Udo, T. Uehama, F. Urban, T. Wong, K. Yada, M. Yamamoto, K. Yamazaki, J. Yang, K. Yashiro, M. Yosei, Y. Zhezher, and Z. Zundel

Subjects
Physics, 010504 meteorology & atmospheric sciences, High-energy astronomy, Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, Astronomy and Astrophysics, Cosmic ray, Astrophysics, 01 natural sciences, Galaxy, Spectral line, Magnetic field, Space and Planetary Science, Sky, 0103 physical sciences, Ultra-high-energy cosmic ray, Anisotropy, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, media_common
Abstract

Evidence for a large-scale supergalactic cosmic-ray multiplet (arrival directions correlated with energy) structure is reported for ultra-high-energy cosmic-ray (UHECR) energies above 1019 eV using 7 years of data from the Telescope Array (TA) surface detector and updated to 10 years. Previous energy–position correlation studies have made assumptions regarding magnetic field shapes and strength, and UHECR composition. Here the assumption tested is that, because the supergalactic plane is a fit to the average matter density of the local large-scale structure, UHECR sources and intervening extragalactic magnetic fields are correlated with this plane. This supergalactic deflection hypothesis is tested by the entire field-of-view (FOV) behavior of the strength of intermediate-scale energy–angle correlations. These multiplets are measured in spherical cap section bins (wedges) of the FOV to account for coherent and random magnetic fields. The structure found is consistent with supergalactic deflection, the previously published energy spectrum anisotropy results of the TA (the Hotspot and Coldspot), and toy-model simulations of a supergalactic magnetic sheet. The seven year data posttrial significance of this supergalactic structure of multiplets appearing by chance, on an isotropic sky, is found by Monte Carlo simulation to be 4.2σ. The 10 years of data posttrial significance is 4.1σ. Furthermore, the starburst galaxy M82 is shown to be a possible source of the TA Hotspot, and an estimate of the supergalactic magnetic field using UHECR measurements is presented.

Published
2020
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49. Search for point sources of ultra-high energy photons with the Telescope Array surface detector

Author

Yasunori Saito, Yuichiro Tameda, John N. Matthews, G. Furlich, Takaaki Ishii, Takayuki Tomida, Heungsu Shin, D. C. Rodriguez, Fumio Kakimoto, Hideki Tanaka, Hideyuki Ohoka, Pierre Sokolsky, Elliott Barcikowski, M. Takeda, Shigehiro Nagataki, Yana Zhezher, K. Hibino, Dmitri Ivanov, Douglas Bergman, Hideaki Shimodaira, Hyoming Jeong, Keijiro Mukai, Younghoon Kwon, T. Suzawa, K. Martens, Eiji Kido, Kenta Yashiro, M. V. Kuznetsov, K. Tsutsumi, Kazuhiro Machida, K. Yamazaki, Isaac Myers, Sergey Troitsky, K. H. Lee, Grigory Rubtsov, T.-A. Shibata, Hidemi Ito, J. Remington, Gordon Thomson, BayarJon Paul Lubsandorzhiev, K. Kasahara, Tom Stroman, Shoichi Kishigami, Robert Cady, Mayuko Minamino, John Belz, Hiroyuki Sagawa, Kiyoshi Tanaka, Kuzmin, Maxim Pshirkov, K. Honda, J. H. Kim, Toshio Seki, Y. Uchihori, Kei Nakai, Masaaki Tanaka, Naoaki Hayashida, Akitoshi Oshima, Y. Tsunesada, Y. Omura, Fumiya Shibata, Masaomi Ono, Toshiyuki Nonaka, R. Sahara, M. Allen, Takashi Sako, R. Ishimori, Hongsu Kim, Toru Nakamura, Kohei Yada, Igor Tkachev, Kenichi Kadota, Inkyu Park, Shingo Kawana, Jyunsei Chiba, Dongsu Ryu, H. Oda, T. Fujii, Keitaro Fujita, Y. Takagi, Akimichi Taketa, Ben Stokes, Tareq Abu-Zayyad, N. Inoue, B. G. Cheon, H. Kawai, B. K. Shin, M. Ohnishi, Federico R. Urban, S. Udo, C. C. H. Jui, Oleg Kalashev, William Hanlon, S. B. Thomas, S. Kawakami, T. Okuda, Rasha Abbasi, Seok Ho Jeong, J. Yang, L. M. Scott, Y. Hayashi, M. Yamamoto, Priti Shah, K. Kawata, Zach Zundel, Nobuyuki Sakurai, Ryota Onogi, A. Di Matteo, Daisuke Ikeda, Ryota Fujiwara, R. Mayta, S. R. Stratton, Tiffany Wong, Naoto Sakaki, R. Takeishi, Ryo Nakamura, Kazuo Saito, Masaki Fukushima, H. Yoshii, R. Azuma, T. Matsuyama, S. Ozawa, Masato Takita, H. Yamaoka, Michiyuki Chikawa, H. Tokuno, J. D. Smith, Peter Tinyakov, Samuel Blake, Shoichi Ogio, Yuta Tanoue, Motoki Hayashi, J. P. Lundquist, Koichi Sekino, Y. Takahashi, Mai Takamura, and M. Abe

Subjects
Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Photon flux, Library science, FOS: Physical sciences, Astronomy and Astrophysics, 01 natural sciences, Joint research, High energy photon, Science research, Space and Planetary Science, 0103 physical sciences, Research policy, Science policy, Astrophysics - High Energy Astrophysical Phenomena, 010306 general physics, 010303 astronomy & astrophysics, Vice president
Abstract

The surface detector (SD) of the Telescope Array (TA) experiment allows one to indirectly detect photons with energies of order $10^{18}$ eV and higher and to separate photons from the cosmic-ray background. In this paper we present the results of a blind search for point sources of ultra-high energy (UHE) photons in the Northern sky using the TA SD data. The photon-induced extensive air showers (EAS) are separated from the hadron-induced EAS background by means of a multivariate classifier based upon 16 parameters that characterize the air shower events. No significant evidence for the photon point sources is found. The upper limits are set on the flux of photons from each particular direction in the sky within the TA field of view, according to the experiment's angular resolution for photons. Average 95% C.L. upper limits for the point-source flux of photons with energies greater than $10^{18}$, $10^{18.5}$, $10^{19}$, $10^{19.5}$ and $10^{20}$ eV are $0.094$, $0.029$, $0.010$, $0.0073$ and $0.0058$ km$^{-2}$yr$^{-1}$ respectively. For the energies higher than $10^{18.5}$ eV, the photon point-source limits are set for the first time. Numerical results for each given direction in each energy range are provided as a supplement to this paper., Comment: accepted to MNRAS, 11 pages, 4 figures, 2 tables; results in text-file format are supplemented to paper source

Published
2019
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50. The Liquid Argon In A Testbeam (LArIAT) Experiment

Author

M. Soderberg, T. Maruyama, E. Kearns, Z. Williams, M. Reggiani Guzzo, J. Hugon, W. Badgett, A. Falcone, H. Wenzel, J. Esquivel, B. Baller, A. M. Szelc, G. P. Zeller, Makoto Tabata, R. Carey, D. Gratieri, J. I. Cevallos Aleman, B. Rebel, Laura Paulucci, T. Kobilarcik, M. Kordosky, O. Benevides Rodrigues, W. Metcalf, E. Segreto, R. Gran, L. Mendes Santos, J. M. Paley, H. Jostlein, Michael H Kirby, Craig L. Hill, A. Holin, J. Asaadi, T. Ghosh, D. Totani, T. Yang, A. A. Machado, D. Phan, O. Palamara, F. Spagliardi, P. Dedin, R. Castillo Fernandez, J. St. John, A. Marchionni, M. V. Dos Santos, R. A. Johnson, D. Stefan, S. Shahsavarani, R. Sulej, Alec Habig, P. Kryczynski, B. Passarelli Gelli, M. Soares Nunes, M. Ross-Lonergan, P. M. Hamilton, S. Lockwitz, W. Foreman, M. Elkins, Daniel Gastler, J. Ho, R. Acciarri, D. Garcia-Gamez, Irene Nutini, G. Pulliam, Karol Lang, X. Luo, E. Kemp, C. Adams, D. Sessumes, P. Guzowski, W. Flanagan, R. J. Nichol, I. Parmaksiz, M. Tzanov, C. Bromberg, D. A. Jensen, B.T. Fleming, Amir Farbin, M. Stephens, Jong-Sung Yu, H. Kawai, R. Bouabid, J. J. Evans, A. Hahn, D. W. Schmitz, R. Linehan, R. A. Gomes, E. Gramellini, M. Backfish, Junjie Zhu, C. A. Moura, M. Stancari, D. Smith, D. Edmunds, D. Walker, J. L. Raaf, B. Soubasis, G. A. Valdiviesso, A. Olivier, F. Cavanna, E. Iwai, F. d. M. Blaszczyk, Carlos Escobar, D. Shooltz, S. Zhang, Animesh Chatterjee, Acciarri, R, Adams, C, Asaadi, J, Backfish, M, Badgett, W, Baller, B, Benevides Rodrigues, O, Blaszczyk, F, Bouabid, R, Bromberg, C, Carey, R, Castillo Fernandez, R, Cavanna, F, Cevallos Aleman, J, Chatterjee, A, Dedin, P, Dos Santos, M, Edmunds, D, Elkins, M, Escobar, C, Esquivel, J, Evans, J, Falcone, A, Farbin, A, Flanagan, W, Fleming, B, Foreman, W, Garcia-Gamez, D, Gastler, D, Ghosh, T, Gomes, R, Gramellini, E, Gran, R, Gratieri, D, Guzowski, P, Habig, A, Hahn, A, Hamilton, P, Hill, C, Ho, J, Holin, A, Hugon, J, Iwai, E, Jensen, D, Johnson, R, Jostlein, H, Kawai, H, Kearns, E, Kemp, E, Kirby, M, Kobilarcik, T, Kordosky, M, Kryczynski, P, Lang, K, Linehan, R, Lockwitz, S, Luo, X, Machado, A, Marchionni, A, Maruyama, T, Mendes Santos, L, Metcalf, W, Moura, C, Nichol, R, Nutini, I, Olivier, A, Palamara, O, Paley, J, Parmaksiz, I, Passarelli Gelli, B, Paulucci, L, Phan, D, Pulliam, G, Raaf, J, Rebel, B, Reggiani Guzzo, M, Ross-Lonergan, M, Soares Nunes, M, Schmitz, D, Segreto, E, Sessumes, D, Shahsavarani, S, Shooltz, D, Smith, D, Soderberg, M, Soubasis, B, Spagliardi, F, John, J, Stancari, M, Stefan, D, Stephens, M, Sulej, R, Szelc, A, Tabata, M, Totani, D, Tzanov, M, Valdiviesso, G, Walker, D, Wenzel, H, Williams, Z, Yang, T, Yu, J, Zeller, G, Zhang, S, and Zhu, J

Subjects
Physics - Instrumentation and Detectors, Materials science, double-phase), ionization, Noble liquid detectors (scintillation, Particle tracking detectors, Time projection chambers, Physics::Instrumentation and Detectors, Nuclear Theory, chemistry.chemical_element, FOS: Physical sciences, 01 natural sciences, Particle detector, High Energy Physics - Experiment, 030218 nuclear medicine & medical imaging, Nuclear physics, 03 medical and health sciences, High Energy Physics - Experiment (hep-ex), 0302 clinical medicine, 0103 physical sciences, Fermilab, Nuclear Experiment, Instrumentation, Mathematical Physics, Argon, Time projection chamber, 010308 nuclear & particles physics, Detector, Instrumentation and Detectors (physics.ins-det), Charged particle, Particle tracking detector, chemistry, Beamline, Noble liquid detectors (scintillation, ionization), Physics::Accelerator Physics, High Energy Physics::Experiment, Beam (structure)
Abstract

The LArIAT liquid argon time projection chamber, placed in a tertiary beam of charged particles at the Fermilab Test Beam Facility, has collected large samples of pions, muons, electrons, protons, and kaons in the momentum range 0∼30-0140 MeV/c. This paper describes the main aspects of the detector and beamline, and also reports on calibrations performed for the detector and beamline components.

Published
2019
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