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2. Sectm1a Suppresses IL-17a Production of Gamma-delta T Cells and Influences Bacterial Clearance During Pneumococcal Pneumonia

Author

Tanaka, H., primary, Kamata, H., additional, Ishii, M., additional, Asakura, T., additional, Namkoong, H., additional, Morita, A., additional, Kusumoto, T., additional, Azekawa, S., additional, Nakagawara, K., additional, Kaji, M., additional, Nagao, G., additional, Asakura, K., additional, Nishimura, T., additional, Hasegawa, N., additional, and Fukunaga, K., additional

Published
2024
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3. Search for double-beta decay of 136Xe to excited states of 136Ba with the KamLAND-Zen experiment

Author

Collaboration, KamLAND-Zen, Asakura, K., Gando, A., Gando, Y., Hachiya, T., Hayashida, S., Ikeda, H., Inoue, K., Ishidoshiro, K., Ishikawa, T., Ishio, S., Koga, M., Matsuda, S., Mitsui, T., Motoki, D., Nakamura, K., Obara, S., Otani, M., Oura, T., Shimizu, I., Shirahata, Y., Shirai, J., Suzuki, A., Tachibana, H., Tamae, K., Ueshima, K., Watanabe, H., Xu, B. D., Yoshida, H., Kozlov, A., Takemoto, Y., Yoshida, S., Fushimi, K., Banks, T. I., Berger, B. E., Fujikawa, B. K., O'Donnell, T., Winslow, L. A., Efremenko, Y., Karwowski, H. J., Markoff, D. M., Tornow, W., Detwiler, J. A., Enomoto, S., and Decowski, M. P.

Subjects
High Energy Physics - Experiment, Physics - Instrumentation and Detectors
Abstract

A search for double-beta decays of 136Xe to excited states of 136Ba has been performed with the first phase data set of the KamLAND-Zen experiment. The 0+1, 2+1 and 2+2 transitions of 0{\nu}\{beta}\{beta} decay were evaluated in an exposure of 89.5kg-yr of 136Xe, while the same transitions of 2{\nu}\{beta}\{beta} decay were evaluated in an exposure of 61.8kg-yr. No excess over background was found for all decay modes. The lower half-life limits of the 2+1 state transitions of 0{\nu}\{beta}\{beta} and 2{\nu}\{beta}\{beta} decay were improved to T(0{\nu}, 0+ \rightarrow 2+) > 2.6\times10^25 yr and T(2{\nu}, 0+ \rightarrow 2+) > 4.6\times10^23 yr (90% C.L.), respectively. We report on the first experimental lower half-life limits for the transitions to the 0+1 state of 136Xe for 0{\nu}\{beta}\{beta} and 2{\nu}\{beta}\{beta} decay. They are T (0{\nu}, 0+ \rightarrow 0+) > 2.4\times10^25 yr and T(2{\nu}, 0+ \rightarrow 0+) > 8.3\times10^23 yr (90% C.L.). The transitions to the 2+2 states are also evaluated for the first time to be T(0{\nu}, 0+ \rightarrow 2+) > 2.6\times10^25 yr and T(2{\nu}, 0+ \rightarrow 2+) > 9.0\times10^23 yr (90% C.L.). These results are compared to recent theoretical predictions., Comment: 16 pages, 4 figures. Published in Nuclear Physics A

Published
2015
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4. KamLAND Sensitivity to Neutrinos from Pre-Supernova Stars

Author

Asakura, K., Gando, A., Gando, Y., Hachiya, T., Hayashida, S., Ikeda, H., Inoue, K., Ishidoshiro, K., Ishikawa, T., Ishio, S., Koga, M., Matsuda, S., Mitsui, T., Motoki, D., Nakamura, K., Obara, S., Oura, T., Shimizu, I., Shirahata, Y., Shirai, J., Suzuki, A., Tachibana, H., Tamae, K., Ueshima, K., Watanabe, H., Xu, B. D., Kozlov, A., Takemoto, Y., Yoshida, S., Fushimi, K., Piepke, A., Banks, T. I., Berger, B. E., Fujikawa, B. K., O'Donnell, T., Learned, J. G., Maricic, J., Matsuno, S., Sakai, M., Winslow, L. A., Efremenko, Y., Karwowski, H. J., Markoff, D. M., Tornow, W., Detwiler, J. A., Enomoto, S., and Decowski, M. P.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment, Physics - Instrumentation and Detectors
Abstract

In the late stages of nuclear burning for massive stars ($M>8~M_{\sun}$), the production of neutrino-antineutrino pairs through various processes becomes the dominant stellar cooling mechanism. As the star evolves, the energy of these neutrinos increases and in the days preceding the supernova a significant fraction of emitted electron anti-neutrinos exceeds the energy threshold for inverse beta decay on free hydrogen. This is the golden channel for liquid scintillator detectors because the coincidence signature allows for significant reductions in background signals. We find that the kiloton-scale liquid scintillator detector KamLAND can detect these pre-supernova neutrinos from a star with a mass of $25~M_{\sun}$ at a distance less than 690~pc with 3$\sigma$ significance before the supernova. This limit is dependent on the neutrino mass ordering and background levels. KamLAND takes data continuously and can provide a supernova alert to the community., Comment: 19 pages, 6 figures, 1 table

Published
2015
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5. Study of electron anti-neutrinos associated with gamma-ray bursts using KamLAND

Author

Asakura, K., Gando, A., Gando, Y., Hachiya, T., Hayashida, S., Ikeda, H., Inoue, K., Ishidoshiro, K., Ishikawa, T., Ishio, S., Koga, M., Matsuda, S., Mitsui, T., Motoki, D., Nakamura, K., Obara, S., Oki, Y., Oura, T., Shimizu, I., Shirahata, Y., Shirai, J., Suzuki, A., Tachibana, H., Tamae, K., Ueshima, K., Watanabe, H., Xu, B. D., Yoshida, H., Kozlov, A., Takemoto, Y., Yoshida, S., Fushimi, K., Piepke, A., Banks, T. I., Berger, B. E., O'Donnell, T., Fujikawa, B. K., Maricic, J., Learned, J. G., Sakai, M., Winslow, L. A., Efremenko, Y., Karwowski, H. J., Markoff, D. M., Tornow, W., Detwiler, J. A., Enomoto, S., and Decowski, M. P.

Subjects
Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment
Abstract

We search for electron anti-neutrinos ($\overline{\nu}_e$) from long and short-duration gamma-ray bursts~(GRBs) using data taken by the KamLAND detector from August 2002 to June 2013. No statistically significant excess over the background level is found. We place the tightest upper limits on $\overline{\nu}_e$ fluence from GRBs below 7 MeV and place first constraints on the relation between $\overline{\nu}_e$ luminosity and effective temperature., Comment: 16 pages and 5 figures

Published
2015
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6. KamLAND SENSITIVITY TO NEUTRINOS FROM PRE-SUPERNOVA STARS

Author

Asakura, K, Gando, A, Gando, Y, Hachiya, T, Hayashida, S, Ikeda, H, Inoue, K, Ishidoshiro, K, Ishikawa, T, Ishio, S, Koga, M, Matsuda, S, Mitsui, T, Motoki, D, Nakamura, K, Obara, S, Oura, T, Shimizu, I, Shirahata, Y, Shirai, J, Suzuki, A, Tachibana, H, Tamae, K, Ueshima, K, Watanabe, H, Xu, BD, Kozlov, A, Takemoto, Y, Yoshida, S, Fushimi, K, Piepke, A, Banks, TI, Berger, BE, Fujikawa, BK, O’Donnell, T, Learned, JG, Maricic, J, Matsuno, S, Sakai, M, Winslow, LA, Efremenko, Y, Karwowski, HJ, Markoff, DM, Tornow, W, Detwiler, JA, Enomoto, S, and Decowski, MP

Subjects
neutrinos, supernovae: general, astro-ph.HE, hep-ex, physics.ins-det, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics
Abstract

In the late stages of nuclear burning for massive stars (M > 8 Mȯ), the production of neutrino-antineutrino pairs through various processes becomes the dominant stellar cooling mechanism. As the star evolves, the energy of these neutrinos increases and in the days preceding the supernova a significant fraction of emitted electron anti-neutrinos exceeds the energy threshold for inverse beta decay on free hydrogen. This is the golden channel for liquid scintillator detectors because the coincidence signature allows for significant reductions in background signals. We find that the kiloton-scale liquid scintillator detector KamLAND can detect these pre-supernova neutrinos from a star with a mass of 25 Mȯ at a distance less than 690 pc with 3σ significance before the supernova. This limit is dependent on the neutrino mass ordering and background levels. KamLAND takes data continuously and can provide a supernova alert to the community.

Published
2016

7. KamLAND SENSITIVITY TO NEUTRINOS FROM PRE-SUPERNOVA STARS

Author

The KamLAND Collaboration, Asakura, K, Gando, A, Gando, Y, Hachiya, T, Hayashida, S, Ikeda, H, Inoue, K, Ishidoshiro, K, Ishikawa, T, Ishio, S, Koga, M, Matsuda, S, Mitsui, T, Motoki, D, Nakamura, K, Obara, S, Oura, T, Shimizu, I, Shirahata, Y, Shirai, J, Suzuki, A, Tachibana, H, Tamae, K, Ueshima, K, Watanabe, H, Xu, BD, Kozlov, A, Takemoto, Y, Yoshida, S, Fushimi, K, Piepke, A, Banks, TI, Berger, BE, Fujikawa, BK, O'Donnell, T, Learned, JG, Maricic, J, Matsuno, S, Sakai, M, Winslow, LA, Efremenko, Y, Karwowski, HJ, Markoff, DM, Tornow, W, Detwiler, JA, Enomoto, S, and Decowski, MP

Subjects
neutrinos, supernovae: general, astro-ph.HE, hep-ex, physics.ins-det, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Physical Chemistry (incl. Structural), Astronomy & Astrophysics
Abstract

In the late stages of nuclear burning for massive stars (M > 8 Mȯ), the production of neutrino-antineutrino pairs through various processes becomes the dominant stellar cooling mechanism. As the star evolves, the energy of these neutrinos increases and in the days preceding the supernova a significant fraction of emitted electron anti-neutrinos exceeds the energy threshold for inverse beta decay on free hydrogen. This is the golden channel for liquid scintillator detectors because the coincidence signature allows for significant reductions in background signals. We find that the kiloton-scale liquid scintillator detector KamLAND can detect these pre-supernova neutrinos from a star with a mass of 25 Mȯ at a distance less than 690 pc with 3σ significance before the supernova. This limit is dependent on the neutrino mass ordering and background levels. KamLAND takes data continuously and can provide a supernova alert to the community.

Published
2016

8. Search for double-beta decay of 136Xe to excited states of 136Ba with the KamLAND-Zen experiment

Author

Asakura, K, Gando, A, Gando, Y, Hachiya, T, Hayashida, S, Ikeda, H, Inoue, K, Ishidoshiro, K, Ishikawa, T, Ishio, S, Koga, M, Matsuda, S, Mitsui, T, Motoki, D, Nakamura, K, Obara, S, Otani, M, Oura, T, Shimizu, I, Shirahata, Y, Shirai, J, Suzuki, A, Tachibana, H, Tamae, K, Ueshima, K, Watanabe, H, Xu, BD, Yoshida, H, Kozlov, A, Takemoto, Y, Yoshida, S, Fushimi, K, Banks, TI, Berger, BE, Fujikawa, BK, O'Donnell, T, Winslow, LA, Efremenko, Y, Karwowski, HJ, Markoff, DM, Tornow, W, Detwiler, JA, Enomoto, S, and Decowski, MP

Subjects
Nuclear and Plasma Physics, Particle and High Energy Physics, Physical Sciences, Clinical Research, Double-beta decay, Xe-136, Excited state, hep-ex, physics.ins-det, Astronomical and Space Sciences, Atomic, Molecular, Nuclear, Particle and Plasma Physics, Quantum Physics, Nuclear & Particles Physics, Astronomical sciences, Nuclear and plasma physics, Particle and high energy physics
Abstract

A search for double-beta decays of 136Xe to excited states of 136Ba has been performed with the first phase data set of the KamLAND-Zen experiment. The 01+, 21+ and 22+ transitions of 0νββ decay were evaluated in an exposure of 89.5 kg⋅yr of 136Xe, while the same transitions of 2νββ decay were evaluated in an exposure of 61.8 kg⋅yr. No excess over background was found for all decay modes. The lower half-life limits of the 21+ state transitions of 0νββ and 2νββ decay were improved to T1/20ν(0+→21+)>2.6×1025 yr and T1/22ν(0+→21+)>4.6×1023 yr (90% C.L.), respectively. We report on the first experimental lower half-life limits for the transitions to the 01+ state of 136Xe for 0νββ and 2νββ decay. They are T1/20ν(0+→01+)>2.4×1025 yr and T1/22ν(0+→01+)>8.3×1023 yr (90% C.L.). The transitions to the 22+ states are also evaluated for the first time to be T1/20ν(0+→22+)>2.6×1025 yr and T1/22ν(0+→22+)>9.0×1023 yr (90% C.L.). These results are compared to recent theoretical predictions.

Published
2016

9. Search for double-beta decay of 136Xe to excited states of 136Ba with the KamLAND-Zen experiment

Author

Asakura, K., Gando, A., Gando, Y., Hachiya, T., Hayashida, S., Ikeda, H., Inoue, K., Ishidoshiro, K., Ishikawa, T., Ishio, S., Koga, M., Matsuda, S., Mitsui, T., Motoki, D., Nakamura, K., Obara, S., Otani, M., Oura, T., Shimizu, I., Shirahata, Y., Shirai, J., Suzuki, A., Tachibana, H., Tamae, K., Ueshima, K., Watanabe, H., Xu, B.D., Yoshida, H., Kozlov, A., Takemoto, Y., Yoshida, S., Fushimi, K., Banks, T.I., Berger, B.E., Fujikawa, B.K., O'Donnell, T., Winslow, L.A., Efremenko, Y., Karwowski, H.J., Markoff, D.M., Tornow, W., Detwiler, J.A., Enomoto, S., and Decowski, M.P.

Published
2016

10. Search for the proton decay mode with KamLAND

Author

Asakura, K., Gando, A., Gando, Y., Hachiya, T., Hayashida, S., Ikeda, H., Inoue, K., Ishidoshiro, K., Ishikawa, T., Ishio, S., Koga, M., Matsuda, R., Matsuda, S., Mitsui, T., Motoki, D., Nakamura, K., Obara, S., Oki, Y., Oura, T., Shimizu, I., Shirahata, Y., Shirai, J., Suzuki, A., Tachibana, H., Tamae, K., Ueshima, K., Watanabe, H., Xu, B. D., Yamauchi, Y., Yoshida, H., Kozlov, A., Takemoto, Y., Yoshida, S., Fushimi, K., Grant, C., Piepke, A., Banks, T. I., Berger, B. E., Freedman, S. J., Fujikawa, B. K., O’Donnell, T., Learned, J. G., Maricic, J., Sakai, M., Dazeley, S., Svoboda, R., Winslow, L. A., Efremenko, Y., Karwowski, H. J., Markoff, D. M., Tornow, W., Detwiler, J. A., Enomoto, S., and Decowski, M. P.

Published
2015

12. EP08.02-10 Clinicopathological Analyses for Predicting Survival After Salvage Surgery for Initially Unresectable Lung Cancer

Author

Oka, N., primary, Hishida, T., additional, Kaseda, K., additional, Oshiro, Y., additional, Sakurada, A., additional, Sugino, K., additional, Aoki, H., additional, Ishiguro, Y., additional, Imoto, T., additional, Okubo, Y., additional, Masai, K., additional, Asakura, K., additional, Emoto, K., additional, and Asamura, H., additional

Published
2023
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22. The influence of season and air temperature on water intake by food groups in a sample of free-living Japanese adults

Author

Tani, Y., Asakura, K., Sasaki, S., Hirota, N., Notsu, A., Todoriki, H., Miura, A., Fukui, M., and Date, C.

Subjects
Water consumption -- Environmental aspects -- Health aspects -- Japan, Atmospheric temperature -- Health aspects, Food/cooking/nutrition, Health
Abstract

BACKGROUND/OBJECTIVES: To examine the influence of season and climate (air temperature and humidity) on water intake by the food group in a sample of free-living Japanese adults. SUBJECTS/METHODS: Four-nonconsecutive-day, semi-weighed dietary records were collected from each of the four seasons in a single 12-month period (16 days in total). The influence of season and climate on individual water intake by the food group was analyzed using a mixed linear model. Participants were 242 healthy adults (121 women aged 30-69 years and 121 men aged 30-76 years) from four areas in Japan. RESULTS: For women and men together, the mean total water intake was 2230g/day (highest in summer: 2331 g/day; lowest in winter: 2134g/day). Fifty-one percent of water was derived from foods and the rest from beverages. In a mixed linear model adjusted for sex, age and body mass index, intake of water from foods decreased by 3.1 g/day and that from beverages increased by 8.4g/day, with an increase in the mean outdoor air temperature on the survey day of 1[degrees]C (both P < 0.0001). The influence of humidity was nonsignificant. CONCLUSIONS: In contrast to previous findings in Western countries, half of water intake in Japanese adults was derived from foods. Water intake from beverages was positively associated with air temperature, whereas that from foods was inversely associated with air temperature. European Journal of Clinical Nutrition (2015) 69, 907-913; doi: 10.1038/ejcn.2014.290; published online 28 January 2015, INTRODUCTION Intake of water sufficient to balance losses and assure adequate hydration of body tissues is essential to health and life. (1,2) Adequate water intake is also important during emergency, [...]

Published
2015
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23. Active Phase Structure of the SiO2-supported Nickel Phosphide Catalysts for Non-oxidative Coupling of Methane (NOCM) Reactions

Author

Al Rashid, M. H., Dipu, A., Nishikawa, Y., Ogihara, H., Inami, Y., Obuchi, S., Yamanaka, I., Nagamatsu, S., Kido, D., and Asakura, K.

Subjects
EXAFS, Non-oxidative coupling of methane, Ni2P, Nickel phosphide
Abstract

SiO2-supported NiP binary catalysts show high activity for the non-oxidative coupling of methane (NOCM) reactions, one of the most difficult but important catalytic reactions. We have studied the SiO2-supported NiP binary catalysts by extended X-ray absorption fine structure (EXAFS) with different Ni : P ratios. NiP binary catalyst with the composition of Ni : P = 1 : 1 was the most active among the three different compositions. EXAFS showed that the NiP catalyst with Ni : P = 1 : 1 had a Ni2P structure. The structure was stable after the high temperature (1173 K) NOCM reaction conditions for 12 h. It is interesting that Ni2P shows high catalytic activities in many other reactions such as hydrodesulfurization, hydrogen evolution reaction, and so on. It may be due to the appropriate electronic and geometrical modification of a Ni active site by P.

Published
2020

25. Abstracts

Author

Beniac, D. R., Ridsdale, R. A., Luckevich, M. D., Tompkins, T. A., Harauz, G., Sedzik, J., Hjertén, S., Brekkan, E., Lundahl, P., Tropak, Michael B., Roder, John C., Giordano, F., Chang, B., La Ronde, A. M., Al-Sabbagh, A., Kretschmer, M., Asipu, A., Blair, G. E., Mak, B., Moscarello, M. A., Doucette, R., Gratto, K., Verge, V., Yeung, J., Nazarali, A., Murphy, P., Topilko, P., Schneider-Maunoury, S., Seitanidou, T., Evercooren, A. Baron-Van, Charnay, P., Lee, M. J., Brennan, A., Tabernero, A., Dong, Z., Blanchard, A., Zoidl, G., Jessen, K. R., Mirsky, R., Couve, E., Cabello, F., Krsulovic, J., Roncagliolo, M., Li, J., Hertzberg, E. L., Nagy, J. I., Neuberg, Dirk H.-H., Anzini, Patrizia, Nelles, Eric, Willecke, Klaus, Schachner, Melitta, Martini, Rudolf, Suter, Ueli, Ankerhold, R., Stuermer, C. A. O., Chandross, Karen J., Norton, W. T., Hudson, L. D., Cohen, R. I., Asakura, K., Hunter, S. F., Rodriguez, M., Bansal, Rashmi, Winkler, Susan, Pfeiffer, S. E., Oh., Y. S., Yong, V. W., Juurlink, B. H. J., Griebel, R. W., Devon, R. M., Khorchid, A., Almazan, G., Liu, H.-N., Konat, G. W., Jin, Gu, Wiggins, R. C., Thorburne, S. K., Bartnik, B. L., Marrif, H., Hertz, L., Jelinski, S. E., Yager, J. Y., Del Bigio, M. R., Kanfer, J. N., Weiner, H. L., Nelson, P. A., Dyer, J. K., Bourque, J., Steeves, J. D., Labes, Monika, Roach, Arthur, Andersen, Parker L., Schreyer, David J., Vanderluit, J. L., Peterson, A., Tetzlaff, W., Hanemann, C. O., Gabreëls-Festen, A., Mueller, H. W., Karchewski, L. A., Verge, V. M. K., Foldvari, M., Jaafari, M. R., Fedoroff, Sergey, editor, Burkholder, Gary D., editor, Juurlink, Bernhard H. J., editor, Devon, Richard M., editor, Doucette, J. Ronald, editor, Nazarali, Adil J., editor, Schreyer, David J., editor, and Verge, Valerie M. K., editor

Published
1997
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34. Transfer hydrogenolysis of aromatic ethers promoted by the bimetallic Pd/Co catalyst

Author

Mauriello, F., 1000090570911, Ariga-Miwa, H., Paone, E., Pietropaolo, R., 1000030359484, Takakusagi, S., 1000060175164, Asakura, K., Mauriello, F., 1000090570911, Ariga-Miwa, H., Paone, E., Pietropaolo, R., 1000030359484, Takakusagi, S., 1000060175164, and Asakura, K.

Abstract

The transfer hydrogenolysis of lignin derived aromatic ethers (benzyl phenyl ether, phenethyl phenyl ether and diphenyl ethers) have been investigated by using the coprecipitated Pd/Co as heterogeneous catalyst and 2propanol as H-donor/solvent. A quantitative conversion of benzyl phenyl ether into toluene and cyclohexanol was obtained after 180 min at 240 degrees C. The bimetallic Pd/Co catalyst is, by far, more efficient if compared to commercial Pd/C and Co-based catalytic systems showing, at the same time, a good reusability. The enhanced ability in the CeO bond cleavage in aromatic ethers is related to the formation of bimetallic Pd-Co ensembles, arisen from the preparation procedure adopted, as confirmed by a complete physico-chemical characterization that includes XRD, SEM, TEM, H-2-TPR, XPS and EXAFS analysis.

Published
2020

47. In situ studies of molecular transfer between microparticles by second-harmonic generation

Author

Yan Liu, Yan, Elsa C. Y., Eisenthal, K.B., Seman, M., Kondo, J.N., Domen, K., Ohminami, Y., and Asakura, K.

Subjects
Sulfates -- Chemical properties, Polystyrene -- Chemical properties, Chemicals, plastics and rubber industries
Abstract

The applicability of the second-harmonic generation (SHG) method in studying the kinetics of molecular transfer between microparticles suspended in aqueous solution is demonstrated. The demonstration founded that the transfer of malachite green (MG) from the polystyrene sulfate (PSS) particles to clay particles can be monitored in real time by measuring the surface population of MG remaining on the polystyrene (PSS) particles.

Published
2001

48. Variability in the structure of supported MoO3 catalysts: studies using Raman and X-ray absorption spectroscopy with ab initio calculations

Author

Radhakrishnana, R., Reed, C., Oyama, S.T., Seman, M., Kondo, J.N., Domen, K., Ohminami, Y., and Asakura, K.

Subjects
Raman spectroscopy -- Usage, Molybdenum oxides -- Chemical properties, X-ray spectroscopy -- Usage, Chemicals, plastics and rubber industries
Abstract

The structure of Mo centers in supported molybdenum oxide catalysts are characterized by using Raman, extended X-ray absorption fine structure spectroscopy (EXAFS), and near-edge X-ray absorption fine structure (NEXAFS) spectroscopies. The structure of a series of silica-, alumina-, and titania-supported catalysis by a variety of techniques is studied and the results are compared to predictions from theoretical calculations.

Published
2001

49. Neck Location on the Outer Convexity is a Predictor of Incomplete Occlusion in Treatment with the Pipeline Embolization Device: Clinical and Angiographic Outcomes

Author

Sunohara, T., primary, Imamura, H., additional, Goto, M., additional, Fukumitsu, R., additional, Matsumoto, S., additional, Fukui, N., additional, Oomura, Y., additional, Akiyama, T., additional, Fukuda, T., additional, Go, K., additional, Kajiura, S., additional, Shigeyasu, M., additional, Asakura, K., additional, Horii, R., additional, Sakai, C., additional, and Sakai, N., additional

Published
2020
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