Author: "Kanbe T" - Searchworks@Jio Institute Digital Library Search Results

Your search keyword '"Kanbe T"' showing total 482 results

Start Over Author "Kanbe T"

482 results on '"Kanbe T"'

1. Application of eDNA methods to evaluate abundance and reproduction of winter-breeding freshwater mussels (Buldowskia iwakawai) in the Ishikari River floodplain

Author: Wu, J., Negishi, J. N., Izumi, H., Kanbe, T., Mizumoto, H., and Araki, H.
Published: 2024
Full Text: View/download PDF

2. Search for correlations of the arrival directions of ultra-high energy cosmic ray with extragalactic objects as observed by the telescope array experiment

Author: Abu-Zayyad, T., Aida, R., Allen, M., Anderson, R., Azuma, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Cady, R., Cheon, B. G., Chiba, J., Chikawa, M., Cho, E. J., Cho, W. R., Fujii, H., Fujii, T., Fukuda, T., Fukushima, M., Hanlon, W., Hayashi, K., Hayashi, Y., Hayashida, N., Hibino, K., Hiyama, K., Honda, K., Iguchi, T., Ikeda, D., Ikuta, K., Inoue, N., Ishii, T., Ishimori, R., Ito, H., Ivanov, D., Iwamoto, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kanbe, T., Kasahara, K., Kawai, H., Kawakami, S., Kawana, S., Kido, E., Kim, H. B., Kim, H. K., Kim, J. H., Kitamoto, K., Kitamura, S., Kitamura, Y., Kobayashi, K., Kobayashi, Y., Kondo, Y., Kuramoto, K., Kuzmin, V., Kwon, Y. J., Lan, J., Lim, S. I., Lundquist, J. P., Machida, S., Martens, K., Matsuda, T., Matsuura, T., Matsuyama, T., Matthews, J. N., Minamino, M., Miyata, K., Murano, Y., Myers, I., Nagasawa, K., Nagataki, S., Nakamura, T., Nam, S. W., Nonaka, T., Ogio, S., Ohnishi, M., Ohoka, H., Oki, K., Oku, D., Okuda, T., Ono, M., Oshima, A., Ozawa, S., Park, I. H., Pshirkov, M. S., Rodriguez, D. C., Roh, S. Y., Rubtsov, G., Ryu, D., Sagawa, H., Sakurai, N., Sampson, A. L., Scott, L. M., Shah, P. D., Shibata, F., Shibata, T., Shimodaira, H., Shin, B. K., Shin, J. I., Shirahama, T., Smith, J. D., Sokolsky, P., Springer, R. W., Stokes, B. T., Stratton, S. R., Stroman, T., Suzuki, S., Takahashi, Y., Takeda, M., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsunesada, Y., Tsutsumi, K., Tsuyuguchi, Y., Uchihori, Y., Udo, S., Ukai, H., Urban, F., Vasiloff, G., Wada, Y., Wong, T., Yamakawa, Y., Yamane, R., Yamaoka, H., Yamazaki, K., Yang, J., Yoneda, Y., Yoshida, S., Yoshii, H., Zhou, X., Zollinger, R., and Zundel, Z.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We search for correlations between positions of extragalactic objects and arrival directions of Ultra-High Energy Cosmic Rays (UHECRs) with primary energy $E \ge 40$ EeV as observed by the surface detector array of the Telescope Array (TA) experiment during the first 40 months of operation. We examined several public astronomical object catalogs, including the Veron-Cetty and Veron catalog of active galactic nuclei. We counted the number of TA events correlated with objects in each catalog as a function of three parameters: the maximum angular separation between a TA event and an object, the minimum energy of the events, and the maximum redshift of the objects. We determine combinations of these parameters which maximize the correlations, and calculate the chance probabilities of having the same levels of correlations from an isotropic distribution of UHECR arrival directions. No statistically significant correlations are found when penalties for scanning over the above parameters and for searching in several catalogs are taken into account.
Published: 2013
Full Text: View/download PDF

3. Energy Spectrum of Ultra-High Energy Cosmic Rays Observed with the Telescope Array Using a Hybrid Technique

Author: Abu-Zayyad, T., Aida, R., Allen, M., Anderson, R., Azuma, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Cady, R., Cheon, B. G., Chiba, J., Chikawa, M., Cho, E. J., Cho, W. R., Fujii, H., Fujii, T., Fukuda, T., Fukushima, M., Hanlon, W., Hayashi, K., Hayashi, Y., Hayashida, N., Hibino, K., Hiyama, K., Honda, K., Iguchi, T., Ikeda, D., Ikuta, K., Inoue, N., Ishii, T., Ishimori, R., Ito, H., Ivanov, D., Iwamoto, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kanbe, T., Kasahara, K., Kawai, H., Kawakami, S., Kawana, S., Kido, E., Kim, H. B., Kim, H. K., Kim, J. H., Kitamoto, K., Kitamura, S., Kitamura, Y., Kobayashi, K., Kobayashi, Y., Kondo, Y., Kuramoto, K., Kuzmin, V., Kwon, Y. J., Lan, J., Lim, S. I., Lundquist, J. P., Machida, S., Martens, K., Matsuda, T., Matsuura, T., Matsuyama, T., Matthews, J. N., Minamino, M., Miyata, K., Murano, Y., Myers, I., Nagasawa, K., Nagataki, S., Nakamura, T., Nam, S. W., Nonaka, T., Ogio, S., Ohnishi, M., Ohoka, H., Oki, K., Oku, D., Okuda, T., Ono, M., Oshima, A., Ozawa, S., Park, I. H., Pshirkov, M. S., Rodriguez, D. C., Roh, S. Y., Rubtsov, G., Ryu, D., Sagawa, H., Sakurai, N., Sampson, A. L., Scott, L. M., Shah, P. D., Shibata, F., Shibata, T., Shimodaira, H., Shin, B. K., Shin, J. I., Shirahama, T., Smith, J. D., Sokolsky, P., Springer, R. W., Stokes, B. T., Stratton, S. R., Stroman, T., Suzuki, S., Takahashi, Y., Takeda, M., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsunesada, Y., Tsutsumi, K., Tsuyuguchi, Y., Uchihori, Y., Udo, S., Ukai, H., Urban, F., Vasiloff, G., Wada, Y., Wong, T., Yamakawa, Y., Yamane, R., Yamaoka, H., Yamazaki, K., Yang, J., Yoneda, Y., Yoshida, S., Yoshii, H., Zhou, X., Zollinger, R., and Zundel, Z.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We measure the spectrum of cosmic rays with energies greater than $10^{18.2}$ eV with the Fluorescence Detectors (FDs) and the Surface Detectors (SDs) of the Telescope Array Experiment using the data taken in our first 2.3-year observation from May 27 2008 to September 7 2010. A hybrid air shower reconstruction technique is employed to improve accuracies in determination of arrival directions and primary energies of cosmic rays using both FD and SD data. The energy spectrum presented here is in agreement with our previously published spectra and the HiRes results., Comment: 28 pages, 12 figures, submitted to Astroparticle Physics
Published: 2013

4. The Energy Spectrum of Ultra-High-Energy Cosmic Rays Measured by the Telescope Array FADC Fluorescence Detectors in Monocular Mode

Author: The Telescope Array Collaboration, Abu-Zayyad, T., Aida, R., Allen, M., Anderson, R., Azuma, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Cady, R., Cheon, B. G., Chiba, J., Chikawa, M., Cho, E. J., Cho, W. R., Fujii, H., Fujii, T., Fukuda, T., Fukushima, M., Hanlon, W., Hayashi, K., Hayashi, Y., Hayashida, N., Hibino, K., Hiyama, K., Honda, K., Iguchi, T., Ikeda, D., Ikuta, K., Inoue, N., Ishii, T., Ishimori, R., Ito, H., Ivanov, D., Iwamoto, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kanbe, T., Kasahara, K., Kawai, H., Kawakami, S., Kawana, S., Kido, E., Kim, H. B., Kim, H. K., Kim, J. H., Kitamoto, K., Kitamura, S., Kitamura, Y., Kobayashi, K., Kobayashi, Y., Kondo, Y., Kuramoto, K., Kuzmin, V., Kwon, Y. J., Lan, J., Lim, S. I., Lundquist, J. P., Machida, S., Martens, K., Matsuda, T., Matsuura, T., Matsuyama, T., Matthews, J. N., Myers, I., Minamino, M., Miyata, K., Murano, Y., Nagataki, S., Nakamura, T., Nam, S. W., Nonaka, T., Ogio, S., Ogura, J., Ohnishi, M., Ohoka, H., Oki, K., Oku, D., Okuda, T., Ono, M., Oshima, A., Ozawa, S., Park, I. H., Pshirkov, M. S., Rodriguez, D. C., Roh, S. Y., Rubtsov, G., Ryu, D., Sagawa, H., Sakurai, N., Sampson, A. L., Scott, L. M., Shah, P. D., Shibata, F., Shibata, T., Shimodaira, H., Shin, B. K., Shin, J. I., Shirahama, T., Smith, J. D., Sokolsky, P., Sonley, T. J., Springer, R. W., Stokes, B. T., Stratton, S. R., Stroman, T. A., Suzuki, S., Takahashi, Y., Takeda, M., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsunesada, Y., Tsutsumi, K., Tsuyuguchi, Y., Uchihori, Y., Udo, S., Ukai, H., Vasiloff, G., Wada, Y., Wong, T., Yamakawa, Y., Yamane, R., Yamaoka, H., Yamazaki, K., Yang, J., Yoneda, Y., Yoshida, S., Yoshii, H., Zollinger, R., and Zundel, Z.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: We present a measurement of the energy spectrum of ultra-high-energy cosmic rays performed by the Telescope Array experiment using monocular observations from its two new FADC-based fluorescence detectors. After a short description of the experiment, we describe the data analysis and event reconstruction procedures. Since the aperture of the experiment must be calculated by Monte Carlo simulation, we describe this calculation and the comparisons of simulated and real data used to verify the validity of the aperture calculation. Finally, we present the energy spectrum calculated from the merged monocular data sets of the two FADC-based detectors, and also the combination of this merged spectrum with an independent, previously published monocular spectrum measurement performed by Telescope Array's third fluorescence detector (Abu-Zayyad {\it et al.}, {Astropart. Phys.} 39 (2012), 109). This combined spectrum corroborates the recently published Telescope Array surface detector spectrum (Abu-Zayyad {\it et al.}, {Astrophys. Journ.} 768 (2013), L1) with independent systematic uncertainties., Comment: 10 pages, 10 figures, submitted to Astroparticle Physics
Published: 2013

5. Upper limit on the flux of photons with energies above 10^19 eV using the Telescope Array surface detector

Author: Abu-Zayyad, T., Aida, R., Allen, M., Anderson, R., Azuma, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Cady, R., Cheon, B. G., Chiba, J., Chikawa, M., Cho, E. J., Cho, W. R., Fujii, H., Fujii, T., Fukuda, T., Fukushima, M., Gorbunov, D., Hanlon, W., Hayashi, K., Hayashi, Y., Hayashida, N., Hibino, K., Hiyama, K., Honda, K., Iguchi, T., Ikeda, D., Ikuta, K., Inoue, N., Ishii, T., Ishimori, R., Ivanov, D., Iwamoto, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kanbe, T., Kasahara, K., Kawai, H., Kawakami, S., Kawana, S., Kido, E., Kim, H. B., Kim, H. K., Kim, J. H., Kitamoto, K., Kitamura, S., Kitamura, Y., Kobayashi, K., Kobayashi, Y., Kondo, Y., Kuramoto, K., Kuzmin, V., Kwon, Y. J., Lan, J., Lim, S. I., Machida, S., Martens, K., Matsuda, T., Matsuura, T., Matsuyama, T., Matthews, J. N., Minamino, M., Miyata, K., Murano, Y., Myers, I., Nagasawa, K., Nagataki, S., Nakamura, T., Nam, S. W., Nonaka, T., Ogio, S., Ohnishi, M., Ohoka, H., Oki, K., Oku, D., Okuda, T., Oshima, A., Ozawa, S., Park, I. H., Pshirkov, M. S., Rodriguez, D. C., Roh, S. Y., Rubtsov, G. I., Ryu, D., Sagawa, H., Sakurai, N., Sampson, A. L., Scott, L. M., Shah, P. D., Shibata, F., Shibata, T., Shimodaira, H., Shin, B. K., Shin, J. I., Shirahama, T., Smith, J. D., Sokolsky, P., Stokes, B. T., Stratton, S. R., Stroman, T., Suzuki, S., Takahashi, Y., Takeda, M., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsunesada, Y., Tsutsumi, K., Tsuyuguchi, Y., Uchihori, Y., Udo, S., Ukai, H., Vasiloff, G., Wada, Y., Wong, T., Wood, M., Yamakawa, Y., Yamane, R., Yamaoka, H., Yamazaki, K., Yang, J., Yoneda, Y., Yoshida, S., Yoshii, H., Zhou, X., Zollinger, R., and Zundel, Z.
Subjects: Astrophysics - High Energy Astrophysical Phenomena, High Energy Physics - Experiment, High Energy Physics - Phenomenology
Abstract: We search for ultra-high energy photons by analyzing geometrical properties of shower fronts of events registered by the Telescope Array surface detector. By making use of an event-by-event statistical method, we derive upper limits on the absolute flux of primary photons with energies above 10^19, 10^19.5 and 10^20 eV based on the first three years of data taken., Comment: 7 pages, 5 figures
Published: 2013
Full Text: View/download PDF

6. Search for Anisotropy of Ultra-High Energy Cosmic Rays with the Telescope Array Experiment

Author: Abu-Zayyad, T., Aida, R., Allen, M., Anderson, R., Azuma, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Cady, R., Cheon, B. G., Chiba, J., Chikawa, M., Cho, E. J., Cho, W. R., Fujii, H., Fujii, T., Fukuda, T., Fukushima, M., Hanlon, W., Hayashi, K., Hayashi, Y., Hayashida, N., Hibino, K., Hiyama, K., Honda, K., Iguchi, T., Ikeda, D., Ikuta, K., Inoue, N., Ishii, T., Ishimori, R., Ivanov, D., Iwamoto, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kanbe, T., Kasahara, K., Kawai, H., Kawakami, S., Kawana, S., Kido, E., Kim, H. B., Kim, H. K., Kim, J. H., Kitamoto, K., Kitamura, S., Kitamura, Y., Kobayashi, K., Kobayashi, Y., Kondo, Y., Kuramoto, K., Kuzmin, V., Kwon, Y. J., Lim, S. I., Machida, S., Martens, K., Martineau, J., Matsuda, T., Matsuura, T., Matsuyama, T., Matthews, J. N., Minamino, M., Miyata, K., Murano, Y., Myers, I., Nagasawa, K., Nagataki, S., Nakamura, T., Nam, S. W., Nonaka, T., Ogio, S., Ohnishi, M., Ohoka, H., Oki, K., Oku, D., Okuda, T., Oshima, A., Ozawa, S., Park, I. H., Pshirkov, M. S., Rodriguez, D. C., Roh, S. Y., Rubtsov, G., Ryu, D., Sagawa, H., Sakurai, N., Sampson, A. L., Scott, L. M., Shah, P. D., Shibata, F., Shibata, T., Shimodaira, H., Shin, B. K., Shin, J. I., Shirahama, T., Smith, J. D., Sokolsky, P., Sonley, T. J., Springer, R. W., Stokes, B. T., Stratton, S. R., Stroman, T., Suzuki, S., Takahashi, Y., Takeda, M., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsunesada, Y., Tsutsumi, K., Tsuyuguchi, Y., Uchihori, Y., Udo, S., Ukai, H., Vasiloff, G., Wada, Y., Wong, T., Wood, M., Yamakawa, Y., Yamane, R., Yamaoka, H., Yamazaki, K., Yang, J., Yoneda, Y., Yoshida, S., Yoshii, H., Zhou, X., Zollinger, R., and Zundel, Z.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: We study the anisotropy of Ultra-High Energy Cosmic Ray (UHECR) events collected by the Telescope Array (TA) detector in the first 40 months of operation. Following earlier studies, we examine event sets with energy thresholds of 10 EeV, 40 EeV, and 57 EeV. We find that the distributions of the events in right ascension and declination are compatible with an isotropic distribution in all three sets. We then compare with previously reported clustering of the UHECR events at small angular scales. No significant clustering is found in the TA data. We then check the events with E>57 EeV for correlations with nearby active galactic nuclei. No significant correlation is found. Finally, we examine all three sets for correlations with the large-scale structure of the Universe. We find that the two higher-energy sets are compatible with both an isotropic distribution and the hypothesis that UHECR sources follow the matter distribution of the Universe (the LSS hypothesis), while the event set with E>10 EeV is compatible with isotropy and is not compatible with the LSS hypothesis at 95% CL unless large deflection angles are also assumed. We show that accounting for UHECR deflections in a realistic model of the Galactic magnetic field can make this set compatible with the LSS hypothesis., Comment: 10 pages, 9 figures
Published: 2012
Full Text: View/download PDF

7. The Cosmic Ray Energy Spectrum Observed with the Surface Detector of the Telescope Array Experiment

Author: Abu-Zayyad, T., Aida, R., Allen, M., Anderson, R., Azuma, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Cady, R., Cheon, B. G., Chiba, J., Chikawa, M., Cho, E. J., Cho, W. R., Fujii, H., Fujii, T., Fukuda, T., Fukushima, M., Hanlon, W., Hayashi, K., Hayashi, Y., Hayashida, N., Hibino, K., Hiyama, K., Honda, K., Iguchi, T., Ikeda, D., Ikuta, K., Inoue, N., Ishii, T., Ishimori, R., Ivanov, D., Iwamoto, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kanbe, T., Kasahara, K., Kawai, H., Kawakami, S., Kawana, S., Kido, E., Kim, H. B., Kim, H. K., Kim, J. H., Kitamoto, K., Kitamura, S., Kitamura, Y., Kobayashi, K., Kobayashi, Y., Kondo, Y., Kuramoto, K., Kuzmin, V., Kwon, Y. J., Lan, J., Lim, S. I., Machida, S., Martens, K., Matsuda, T., Matsuura, T., Matsuyama, T., Matthews, J. N., Minamino, M., Miyata, K., Murano, Y., Myers, I., Nagasawa, K., Nagataki, S., Nakamura, T., Nam, S. W., Nonaka, T., Ogio, S., Ohnishi, M., Ohoka, H., Oki, K., Oku, D., Okuda, T., Oshima, A., Ozawa, S., Park, I. H., Pshirkov, M. S., Rodriguez, D. C., Roh, S. Y., Rubtsov, G., Ryu, D., Sagawa, H., Sakurai, N., Sampson, A. L., Scott, L. M., Shah, P. D., Shibata, F., Shibata, T., Shimodaira, H., Shin, B. K., Shin, J. I., Shirahama, T., Smith, J. D., Sokolsky, P., Stokes, B. T., Stratton, S. R., Stroman, T. A., Suzuki, S., Takahashi, Y., Takeda, M., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsunesada, Y., Tsutsumi, K., Tsuyuguchi, Y., Uchihori, Y., Udo, S., Ukai, H., Vasiloff, G., Wada, Y., Wong, T., Wood, M., Yamakawa, Y., Yamane, R., Yamaoka, H., Yamazaki, K., Yang, J., Yoneda, Y., Yoshida, S., Yoshii, H., Zhou, X., Zollinger, R., and Zundel, Z.
Subjects: Astrophysics - High Energy Astrophysical Phenomena
Abstract: The Telescope Array (TA) collaboration has measured the energy spectrum of ultra-high energy cosmic rays with primary energies above 1.6 x 10^(18) eV. This measurement is based upon four years of observation by the surface detector component of TA. The spectrum shows a dip at an energy of 4.6 x 10^(18) eV and a steepening at 5.4 x 10^(19) eV which is consistent with the expectation from the GZK cutoff. We present the results of a technique, new to the analysis of ultra-high energy cosmic ray surface detector data, that involves generating a complete simulation of ultra-high energy cosmic rays striking the TA surface detector. The procedure starts with shower simulations using the CORSIKA Monte Carlo program where we have solved the problems caused by use of the "thinning" approximation. This simulation method allows us to make an accurate calculation of the acceptance of the detector for the energies concerned., Comment: Accepted for publication by Astrophysical Journal Letters
Published: 2012
Full Text: View/download PDF

8. The Energy Spectrum of Telescope Array's Middle Drum Detector and the Direct Comparison to the High Resolution Fly's Eye Experiment

Author: Abu-Zayyad, T., Aida, R., Allen, M., Anderson, R., Azuma, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Cady, R., Cheon, B. G., Chiba, J., Chikawa, M., Cho, E. J., Cho, W. R., Fujii, H., Fujii, T., Fukuda, T., Fukushima, M., Gorbunov, D., Hanlon, W., Hayashi, K., Hayashi, Y., Hayashida, N., Hibino, K., Hiyama, K., Honda, K., Iguchi, T., Ikeda, D., Ikuta, K., Inoue, N., Ishii, T., Ishimori, R., Ivanov, D., Iwamoto, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kanbe, T., Kasahara, K., Kawai, H., Kawakami, S., Kawana, S., Kido, E., Kim, H. B., Kim, H. K., Kim, J. H., Kitamoto, K., Kitamura, S., Kitamura, Y., Kobayashi, K., Kobayashi, Y., Kondo, Y., Kuramoto, K., Kuzmin, V., Kwon, Y. J., Lim, S. I., Machida, S., Martens, K., Martineau, J., Matsuda, T., Matsuura, T., Matsuyama, T., Matthews, J. N., Minamino, M., Miyata, K., Murano, Y., Nagataki, S., Nakamura, T., Nam, S. W., Nonaka, T., Ogio, S., Ohnishi, M., Ohoka, H., Oki, K., Oku, D., Okuda, T., Oshima, A., Ozawa, S., Park, I. H., Pshirkov, M. S., Rodriguez, D. C., Roh, S. Y., Rubtsov, G., Ryu, D., Sagawa, H., Sakurai, N., Sampson, A. L., Scott, L. M., Shah, P. D., Shibata, F., Shibata, T., Shimodaira, H., Shin, B. K., Shin, J. I., Shirahama, T., Smith, J. D., Sokolsky, P., Sonley, T. J., Springer, R. W., Stokes, B. T., Stratton, S. R., Stroman, T., Suzuki, S., Takahashi, Y., Takeda, M., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsunesada, Y., Tsutsumi, K., Tsuyuguchi, Y., Uchihori, Y., Udo, S., Ukai, H., Vasiloff, G., Wada, Y., Wong, T., Wood, M., Yamakawa, Y., Yamane, R., Yamaoka, H., Yamazaki, K., Yang, J., Yoneda, Y., Yoshida, S., Yoshii, H., Zollinger, R., and Zundel, Z.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The Telescope Array's Middle Drum fluorescence detector was instrumented with telescopes refurbished from the High Resolution Fly's Eye's HiRes-1 site. The data observed by Middle Drum in monocular mode was analyzed via the HiRes-1 profile-constrained geometry reconstruction technique and utilized the same calibration techniques enabling a direct comparison of the energy spectra and energy scales between the two experiments. The spectrum measured using the Middle Drum telescopes is based on a three-year exposure collected between December 16, 2007 and December 16, 2010. The calculated difference between the spectrum of the Middle Drum observations and the published spectrum obtained by the data collected by the HiRes-1 site allows the HiRes-1 energy scale to be transferred to Middle Drum. The HiRes energy scale is applied to the entire Telescope Array by making a comparison between Middle Drum monocular events and hybrid events that triggered both Middle Drum and the Telescope Array's scintillator Ground Array., Comment: 27 pages, 21 figures
Published: 2012
Full Text: View/download PDF

9. The surface detector array of the Telescope Array experiment

Author: Abu-Zayyad, T., Aida, R., Allen, M., Anderson, R., Azuma, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Cady, R., Cheon, B. G., Chiba, J., Chikawa, M., Cho, E. J., Cho, W. R., Fujii, H., Fujii, T., Fukuda, T., Fukushima, M., Gorbunov, D., Hanlon, W., Hayashi, K., Hayashi, Y., Hayashida, N., Hibino, K., Hiyama, K., Honda, K., Iguchi, T., Ikeda, D., Ikuta, K., Inoue, N., Ishii, T., Ishimori, R., Ivanov, D., Iwamoto, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kanbe, T., Kasahara, K., Kawai, H., Kawakami, S., Kawana, S., Kido, E., Kim, H. B., Kim, H. K., Kim, J. H., Kitamoto, K., Kobayashi, K., Kobayashi, Y., Kondo, Y., Kuramoto, K., Kuzmin, V., Kwon, Y. J., Lim, S. I., Machida, S., Martens, K., Martineau, J., Matsuda, T., Matsuura, T., Matsuyama, T., Matthews, J. N., Myers, I., Minamino, M., Miyata, K., Miyauchi, H., Murano, Y., Nakamura, T., Nam, S. W., Nonaka, T., Ogio, S., Ohnishi, M., Ohoka, H., Oki, K., Oku, D., Okuda, T., Oshima, A., Ozawa, S., Park, I. H., Pshirkov, M. S., Rodriguez, D., Roh, S. Y., Rubtsov, G., Ryu, D., Sagawa, H., Sakurai, N., Sampson, A. L., Scott, L. M., Shah, P. D., Shibata, F., Shibata, T., Shimodaira, H., Shin, B. K., Shin, J. I., Shirahama, T., Smith, J. D., Sokolsky, P., Sonley, T. J., Springer, R. W., Stokes, B. T., Stratton, S. R., Stroman, T. A., Suzuki, S., Takahashi, Y., Takeda, M., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Thomas, S. B., Thomson, G. B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsunesada, Y., Tsutsumi, K., Tsuyuguchi, Y., Uchihori, Y., Udo, S., Ukai, H., Vasiloff, G., Wada, Y., Wong, T., Wood, M., Yamakawa, Y., Yamaoka, H., Yamazaki, K., Yang, J., Yoshida, S., Yoshii, H., Zollinger, R., and Zundel, Z.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics
Abstract: The Telescope Array (TA) experiment, located in the western desert of Utah,USA, is designed for observation of extensive air showers from extremely high energy cosmic rays. The experiment has a surface detector array surrounded by three fluorescence detectors to enable simultaneous detection of shower particles at ground level and fluorescence photons along the shower track. The TA surface detectors and fluorescence detectors started full hybrid observation in March, 2008. In this article we describe the design and technical features of the TA surface detector., Comment: 32 pages, 17 figures
Published: 2012
Full Text: View/download PDF

10. New air fluorescence detectors employed in the Telescope Array experiment

Author: Tokuno, H., Tameda, Y., Takeda, M., Kadota, K., Ikeda, D., Chikawa, M., Fujii, T., Fukushima, M., Honda, K., Inoue, N., Kakimoto, F., Kawana, S., Kido, E., Matthews, J. N., Nonaka, T., Ogio, S., Okuda, T., Ozawa, S., Sagawa, H., Sakurai, N., Shibata, T., Taketa, A., Thomas, S. B., Tomida, T., Tsunesada, Y., Udo, S., Abu-zayyad, T., Aida, R., Allen, M., Anderson, R., Azuma, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Cady, R., Cheon, B. G., Chiba, J., Cho, E. J., Cho, W. R., Fujii, H., Fukuda, T., Gorbunov, D., Hanlon, W., Hayashi, K., Hayashi, Y., Hayashida, N., Hibino, K., Hiyama, K., Iguchi, T., Ikuta, K., Ishii, T., Ishimori, R., Ivanov, D., Iwamoto, S., Jui, C. C. H., Kalashev, O., Kanbe, T., Kasahara, K., Kawai, H., Kawakami, S., Kim, H. B., Kim, H. K., Kim, J. H., Kitamoto, K., Kobayashi, K., Kobayashi, Y., Kondo, Y., Kuramoto, K., Kuzmin, V., Kwon, Y. J., Lim, S. I., Machida, S., Martens, K., Martineau, J., Matsuda, T., Matsuura, T., Matsuyama, T., Myers, I., Minamino, M., Miyata, K., Miyauchi, H., Murano, Y., Nakamura, T., Nam, S. W., Ohnishi, M., Ohoka, H., Oki, K., Oku, D., Oshima, A., Park, I. H., Pshirkov, M. S., Rodriguez, D., Roh, S. Y., Rubtsov, G., Ryu, D., Sampson, A. L., Scott, L. M., Shah, P. D., Shibata, F., Shimodaira, H., Shin, B. K., Shin, J. I., Shirahama, T., Smith, J. D., Sokolsky, P., Sonley, T. J., Springer, R. W., Stokes, B. T., Stratton, S. R., Stroman, T., Suzuki, S., Takahashi, Y., Takita, M., Tanaka, H., Tanaka, K., Tanaka, M., Thomson, G. B., Tinyakov, P., Tkachev, I., Troitsky, S., Tsutsumi, K., Tsuyuguchi, Y., Uchihori, Y., Ukai, H., Vasiloff, G., Wada, Y., Wong, T., Wood, M., Yamakawa, Y., Yamaoka, H., Yamazaki, K., Yang, J., Yoshida, S., Yoshii, H., Zollinger, R., and Zundel, Z.
Subjects: Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Since 2007, the Telescope Array (TA) experiment, based in Utah, USA, has been observing ultra high energy cosmic rays to understand their origins. The experiment involves a surface detector (SD) array and three fluorescence detector (FD) stations. FD stations, installed surrounding the SD array, measure the air fluorescence light emitted from extensive air showers (EASs) for precise determination of their energies and species. The detectors employed at one of the three FD stations were relocated from the High Resolution Fly's Eye experiment. At the other two stations, newly designed detectors were constructed for the TA experiment. An FD consists of a primary mirror and a camera equipped with photomultiplier tubes. To obtain the EAS parameters with high accuracies, understanding the FD optical characteristics is important. In this paper, we report the characteristics and installation of new FDs and the performances of the FD components. The results of the monitored mirror reflectance during the observation time are also described in this report., Comment: 44 pages, 23 figures, submitted to NIM-A
Published: 2011
Full Text: View/download PDF

11. Application of eDNA methods to evaluate abundance and reproduction of winter-breeding freshwater mussels (Buldowskia iwakawai) in the Ishikari River floodplain

Author: Wu, J., primary, Negishi, J. N., additional, Izumi, H., additional, Kanbe, T., additional, Mizumoto, H., additional, and Araki, H., additional
Published: 2023
Full Text: View/download PDF

12. Morphological Variation in a Toroid Generated from a Single Polymer Chain

Author: Takenaka, Y., Yoshikawa, Y., Koyama, Y., Kanbe, T., and Yoshikawa, K.
Subjects: Physics - Biological Physics
Abstract: A single semiflexible polymer chain folds into a toroidal object under poor solvent conditions. In this study, we examined the morphological change in such a toroidal state as a function of the width and stiffness of the chain together with the surface energy, which characterizes the segmental interaction parameter. Changes in the thickness and outer/inner radius are interpreted in terms of these parameters. Our theoretical expectation corresponds to the actual morphological changes in a single giant DNA molecule as observed by electron microscopy., Comment: 14 pages, 3 figures
Published: 2005
Full Text: View/download PDF

13. Soft X-ray Magnetic Circular Dichroism of c(2x2) CuMn Ordered Surface Alloy

Author: Kimura, A., Kanbe, T., Xie, T., Taniguchi, M., Qiao, S., Muro, T., Imada, S., and Suga, S.
Subjects: Condensed Matter - Materials Science
Abstract: Mn 2p soft X-ray absorption (XAS) spectroscopy excited with circularly polarized synchrotron radiation has been applied to a new class of material, c(2x2)CuMn/Cu(001) two-dimensional ordered surface alloy. A significant X-ray magnetic circular dichroism (XMCD) signal has been clearly observed at T=25K, indicating the existence of the ferromagnetic state under the external magnetic field of 1.4 Tesla. The lineshape analyses of the XAS and XMCD spectra clearly show that the Mn 3d state is rather localized and has a high spin magnetic moment due to its half-filled character., Comment: REVTeX, 3pages, 3figures. To appear in Jpn. J. Appl. Phys. Vol.42 (2003)
Published: 2003
Full Text: View/download PDF

14. Energy spectrum of ultra-high energy cosmic rays observed with the Telescope Array using a hybrid technique

Author: Abu-Zayyad, T., Aida, R., Allen, M., Anderson, R., Azuma, R., Barcikowski, E., Belz, J.W., Bergman, D.R., Blake, S.A., Cady, R., Cheon, B.G., Chiba, J., Chikawa, M., Cho, E.J., Cho, W.R., Fujii, H., Fujii, T., Fukuda, T., Fukushima, M., Hanlon, W., Hayashi, K., Hayashi, Y., Hayashida, N., Hibino, K., Hiyama, K., Honda, K., Iguchi, T., Ikeda, D., Ikuta, K., Inoue, N., Ishii, T., Ishimori, R., Ito, H., Ivanov, D., Iwamoto, S., Jui, C.C.H., Kadota, K., Kakimoto, F., Kalashev, O., Kanbe, T., Kasahara, K., Kawai, H., Kawakami, S., Kawana, S., Kido, E., Kim, H.B., Kim, H.K., Kim, J.H., Kitamoto, K., Kitamura, S., Kitamura, Y., Kobayashi, K., Kobayashi, Y., Kondo, Y., Kuramoto, K., Kuzmin, V., Kwon, Y.J., Lan, J., Lim, S.I., Lundquist, J.P., Machida, S., Martens, K., Matsuda, T., Matsuura, T., Matsuyama, T., Matthews, J.N., Minamino, M., Miyata, K., Murano, Y., Myers, I., Nagasawa, K., Nagataki, S., Nakamura, T., Nam, S.W., Nonaka, T., Ogio, S., Ohnishi, M., Ohoka, H., Oki, K., Oku, D., Okuda, T., Ono, M., Oshima, A., Ozawa, S., Park, I.H., Pshirkov, M.S., Rodriguez, D.C., Roh, S.Y., Rubtsov, G., Ryu, D., Sagawa, H., Sakurai, N., Sampson, A.L., Scott, L.M., Shah, P.D., Shibata, F., Shibata, T., Shimodaira, H., Shin, B.K., Shin, J.I., Shirahama, T., Smith, J.D., Sokolsky, P., Springer, R.W., Stokes, B.T., Stratton, S.R., Stroman, T., Suzuki, S., Takahashi, Y., Takeda, M., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Thomas, S.B., Thomson, G.B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsunesada, Y., Tsutsumi, K., Tsuyuguchi, Y., Uchihori, Y., Udo, S., Ukai, H., Urban, F., Vasiloff, G., Wada, Y., Wong, T., Yamakawa, Y., Yamane, R., Yamaoka, H., Yamazaki, K., Yang, J., Yoneda, Y., Yoshida, S., Yoshii, H., Zhou, X., Zollinger, R., and Zundel, Z.
Published: 2015
Full Text: View/download PDF

15. Gain monitoring of telescope array photomultiplier cameras for the first 4 years of operation

Author: Shin, B.K., Tokuno, H., Tsunesada, Y., Abu-Zayyad, T., Aida, R., Allen, M., Anderson, R., Azuma, R., Barcikowski, E., Belz, J.W., Bergman, D.R., Blake, S.A., Cady, R., Cheon, B.G., Chiba, J., Chikawa, M., Cho, E.J., Cho, W.R., Fujii, H., Fujii, T., Fukuda, T., Fukushima, M., Hanlon, W., Hayashi, K., Hayashi, Y., Hayashida, N., Hibino, K., Hiyama, K., Honda, K., Iguchi, T., Ikeda, D., Ikuta, K., Inoue, N., Ishii, T., Ishimori, R., Ivanov, D., Iwamoto, S., Jui, C.C.H., Kadota, K., Kakimoto, F., Kalashev, O., Kanbe, T., Kasahara, K., Kawai, H., Kawakami, S., Kawana, S., Kido, E., Kim, H.B., Kim, H.K., Kim, J.H., Kitamoto, K., Kitamura, S., Kitamura, Y., Kobayashi, K., Kobayashi, Y., Kondo, Y., Kuramoto, K., Kuzmin, V., Kwon, Y.J., Lim, S.I., Machida, S., Martens, K., Martineau, J., Matsuda, T., Matsuura, T., Matsuyama, T., Matthews, J.N., Myers, I., Minamino, M., Miyata, K., Murano, Y., Nagasawa, K., Nagataki, S., Nakamura, T., Nam, S.W., Nonaka, T., Ogio, S., Ohnishi, M., Ohoka, H., Oki, K., Oku, D., Okuda, T., Oshima, A., Ozawa, S., Park, I.H., Pshirkov, M.S., Rodriguez, D.C., Roh, S.Y., Rubtsov, G., Ryu, D., Sagawa, H., Sakurai, N., Sampson, A.L., Scott, L.M., Shah, P.D., Shibata, F., Shibata, T., Shimodaira, H., Shin, J.I., Shirahama, T., Smith, J.D., Sokolsky, P., Sonley, T.J., Springer, R.W., Stokes, B.T., Stratton, S.R., Stroman, T., Suzuki, S., Takahashi, Y., Takeda, M., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Thomas, S.B., Thomson, G.B., Tinyakov, P., Tkachev, I., Tomida, T., Troitsky, S., Tsutsumi, K., Tsuyuguchi, Y., Uchihori, Y., Udo, S., Ukai, H., Vasiloff, G., Wada, Y., Wong, T., Wood, M., Yamakawa, Y., Yamane, R., Yamaoka, H., Yamazaki, K., Yang, J., Yoneda, Y., Yoshida, S., Yoshii, H., Zhou, X., Zollinger, R., and Zundel, Z.
Published: 2014
Full Text: View/download PDF

16. The energy spectrum of ultra-high-energy cosmic rays measured by the Telescope Array FADC fluorescence detectors in monocular mode

Author: Abu-Zayyad, T., Aida, R., Allen, M., Anderson, R., Azuma, R., Barcikowski, E., Belz, J.W., Bergman, D.R., Blake, S.A., Cady, R., Cheon, B.G., Chiba, J., Chikawa, M., Cho, E.J., Cho, W.R., Fujii, H., Fujii, T., Fukuda, T., Fukushima, M., Hanlon, W., Hayashi, K., Hayashi, Y., Hayashida, N., Hibino, K., Hiyama, K., Honda, K., Iguchi, T., Ikeda, D., Ikuta, K., Inoue, N., Ishii, T., Ishimori, R., Ito, H., Ivanov, D., Iwamoto, S., Jui, C.C.H., Kadota, K., Kakimoto, F., Kalashev, O., Kanbe, T., Kasahara, K., Kawai, H., Kawakami, S., Kawana, S., Kido, E., Kim, H.B., Kim, H.K., Kim, J.H., Kitamoto, K., Kitamura, S., Kitamura, Y., Kobayashi, K., Kobayashi, Y., Kondo, Y., Kuramoto, K., Kuzmin, V., Kwon, Y.J., Lan, J., Lim, S.I., Lundquist, J.P., Machida, S., Martens, K., Matsuda, T., Matsuura, T., Matsuyama, T., Matthews, J.N., Myers, I., Minamino, M., Miyata, K., Murano, Y., Nagataki, S., Nakamura, T., Nam, S.W., Nonaka, T., Ogio, S., Ogura, J., Ohnishi, M., Ohoka, H., Oki, K., Oku, D., Okuda, T., Ono, M., Oshima, A., Ozawa, S., Park, I.H., Pshirkov, M.S., Rodriguez, D.C., Roh, S.Y., Rubtsov, G., Ryu, D., Sagawa, H., Sakurai, N., Sampson, A.L., Scott, L.M., Shah, P.D., Shibata, F., Shibata, T., Shimodaira, H., Shin, B.K., Shin, J.I., Shirahama, T., Smith, J.D., Sokolsky, P., Sonley, T.J., Springer, R.W., Stokes, B.T., Stratton, S.R., Stroman, T.A., Suzuki, S., Takahashi, Y., Takeda, M., Taketa, A., Takita, M., Tameda, Y., Tanaka, H., Tanaka, K., Tanaka, M., Thomas, S.B., Thomson, G.B., Tinyakov, P., Tkachev, I., Tokuno, H., Tomida, T., Troitsky, S., Tsunesada, Y., Tsutsumi, K., Tsuyuguchi, Y., Uchihori, Y., Udo, S., Ukai, H., Vasiloff, G., Wada, Y., Wong, T., Yamakawa, Y., Yamane, R., Yamaoka, H., Yamazaki, K., Yang, J., Yoneda, Y., Yoshida, S., Yoshii, H., Zollinger, R., and Zundel, Z.
Published: 2013
Full Text: View/download PDF

17. Telescope Array Experiment

Author: Kawai, H., Yoshida, S., Yoshii, H., Tanaka, K., Cohen, F., Fukushima, M., Hayashida, N., Hiyama, K., Ikeda, D., Kido, E., Kondo, Y., Nonaka, T., Ohnishi, M., Ohoka, H., Ozawa, S., Sagawa, H., Sakurai, N., Shibata, T., Shimodaira, H., Takeda, M., Taketa, A., Takita, M., Tokuno, H., Torii, R., Udo, S., Yamakawa, Y., Fujii, H., Matsuda, T., Tanaka, M., Yamaoka, H., Hibino, K., Benno, T., Doura, K., Chikawa, M., Nakamura, T., Teshima, M., Kadota, K., Uchihori, Y., Hayashi, K., Hayashi, Y., Kawakami, S., Matsuyama, T., Minamino, M., Ogio, S., Ohshima, A., Okuda, T., Shimizu, N., Tanaka, H., Bergman, D.R., Hughes, G., Stratton, S., Thomson, G.B., Endo, A., Inoue, N., Kawana, S., Wada, Y., Kasahara, K., Azuma, R., Iguchi, T., Kakimoto, F., Machida, S., Misumi, K., Murano, Y., Tameda, Y., Tsunesada, Y., Chiba, J., Miyata, K., Abu-Zayyad, T., Belz, J.W., Cady, R., Cao, Z., Huentemeyer, P., Jui, C.C.H., Martens, K., Matthews, J.N., Mostofa, M., Smith, J.D., Sokolsky, P., Springer, R.W., Thomas, J.R., Thomas, S.B., Wiencke, L.R., Doyle, T., Taylor, M.J., Wickwar, V.B., Wilkerson, T.D., Hashimoto, K., Honda, K., Ikuta, K., Ishii, T., Kanbe, T., and Tomida, T.
Published: 2008
Full Text: View/download PDF

18. Effect of rectal administration of rebamipide on dextran sulfate sodium-induced colitis: Role of hepatocyte growth factor

Author: Murai, R., Kanbe, T., Mukoyama, T., Shimomura, T., Hashiguchi, K., Yoshida, Y., Tsuchiya, H., Hoshikawa, Y., Kurimasa, A., and Shiota, G.
Published: 2007
Full Text: View/download PDF

19. Identification of a single nuclear localization signal in the C-terminal domain of an Aspergillus DNA topoisomerase II

Author: Kim, K.-H., Kanbe, T., Akashi, T., Mizuguchi, I., and Kikuchi, A.
Published: 2002
Full Text: View/download PDF

20. Localized accumulation of cell wall mannoproteins and endomembranes induced by brefeldin A in hyphal cells of the dimorphic yeastCandida albicans

Author: Akashi, T., Kanbe, T., and Tanaka, K.
Published: 1997
Full Text: View/download PDF

21. Effect of cytochalasin A on actin distribution in the fission yeastSchizosaccharomyces pombe studied by fluorescent and electron microscopy

Author: Kanbe, T., Akashi, T., and Tanaka, K.
Published: 1993
Full Text: View/download PDF

22. Preparation of ultra-thin carbon overcoat for magnetic recording medium by filtered cathodic vacuum arc technology

Author: Fujimaki, S., Yatsue, T., Kokaku, Y., Ohno, T., and Kanbe, T.
Published: 2004
Full Text: View/download PDF

23. Serum levels of soluble stem cell factor and soluble KIT are elevated in patients with atopic dermatitis and correlate with the disease severity

Author: Kanbe, T., Soma, Y., Kawa, Y., Kashima, M., and Mizoguchi, M.
Published: 2001

24. A crossreactivity at the immunoglobulin E level of the cell wall mannoproteins of Candida albicans with other pathogenic Candida and airborne yeast species

Author: KANBE, T., UTSUNOMIYA, K., and ISHIGURO, A.
Published: 1997

25. Phase ordering and its effect on magnetic and structural properties of FeRh ultrathin films.

Author: Yap, Q. J., Qiu, J. J., Luo, P., Ying, J. F., Han, G. C., Laughlin, D. E., Zhu, J.-G., Kanbe, T., and Shige, T.
Subjects: IRON compounds spectra, ANTIFERROMAGNETIC materials, ANTIFERROMAGNETISM, FERROMAGNETISM, SPUTTERING (Physics), MAGNETIC transitions
Abstract: Applications using FeRh for controllable exchange coupling of two magnetic layers with in-plane and out-of-plane anisotropies require ultrathin (~10 nm) films with pure antiferromagnetic (AF) FeRh α" phase at room temperature (RT). However, it is also well known that the antiferromagnetic-ferromagnetic (AF-FM) transition of FeRh is sensitive to composition and deteriorates at low thicknesses. Hence, in this work, we study the composition-dependent phase ordering of co-sputtered FeRh thin films at ultrathin thicknesses of ~10 nm. As the ultrathin films get richer in Rh, the appearance of α" phase is typically characterized magnetically by a sudden drop in RT moment, and structurally by a slight decrease in degree of B2 chemical ordering with a sharp decrease in c-axis lattice constant. These observations are consistent with the FeRh phase diagram where FeRh abruptly enters the AF α" phase once it becomes slightly disordered. Dependences of magnetic transition parameters on composition were also described. Moreover, higher sputtering powers possibly allow the formation of purer α" phase with less γ-face centered cubic phase impurities. Consequently, a composition optimized 10 nm film shows a relatively low residual moment (13.5 emu/cc), thus suggesting good AF phase formation. In addition, correlation of the magnetic transition parameters with the crystal structural parameters reveal that the maximum rate of AF-FM transition (Rmax,h) and the corresponding total change in magnetization (ΔMh) interestingly shows linear dependence on the c-axis lattice constant, but would depart from this linearity under certain conditions, i.e., when grain sizes were large, crystallinity was improved and Fe content was high. [ABSTRACT FROM AUTHOR]
Published: 2014
Full Text: View/download PDF

26. Effects of bottom layer on recording performance and thermal stability for AFC media

Author: Kanbe, T., Yahisa, Y., Kashiwase, H., and Kataoka H.
Subjects: Electromagnetism -- Research, Storage media -- Research, Magnetic recorders and recording -- Research, Business, Electronics, Electronics and electrical industries
Abstract: Recording performance and thermal stability of the antiferromagnetically coupled (AFC) media that utilize CoCrPt alloy as the bottom layer were investigated. The dependence of media noise on the bottom layer thickness ([t.sub.B]) is sensitive to the magnetization of the bottom layer ([Ms.sub.B]). A strong dependence of media noise on [t.sub.B] is observed for the media with high [Ms.sub.B](> 0.7 T). Contrary, the media noise is almost constant in the range of [t.sub.B] = 2-5 nm for low M [s.sub.B](< 0.7 T). The relationship between Ku V/kT and [t.sub.B] is sensitive to anisotropy field of the bottom layer (H [k.sub.B]). Thermal stability can be improved by increasing H [k.sub.B], which is noticeable for the media with thicker [t.sub.B]. Index Terms--Antiferromagnetically coupled media, recording performance, thermal stability.
Published: 2003

27. Low noise antiferromagnetically coupled media with CrTiB underlayer

Author: Kanbe, T., Yahisa, Y., Suzuki, H., Kataoka, H., Takahashi, Y., and Hirayama, Y.
Subjects: Oxides -- Magnetic properties, Titanium compounds -- Magnetic properties, Chromium compounds -- Magnetic properties, Storage media -- Research, Physics
Abstract: The effects of the addition of 1.5 - 3 at. percent B to the CrTi20 underlayer of the antiferromagnetically coupled (AFC) media composed of CoCrPtB/Ru/CoCrPt magnetic layers were examined. The addition of 3 at. percent B led to a decline in the average grain size from 16.1 to 11.9 nm and the grain-size distribution of the magnetic layer reduced by 12 percent.
Published: 2002

28. Role of active oxygen species in diethyldithiocarbamate-induced gastric ulcer in the rat

Author: Oka, S., Ogino, K., Hobara, T., Yoshimura, S., Yanai, H., Okazaki, Y., Takemoto, T., Ishiyama, H., Imaizumi, T., Yamasaki, K., and Kanbe, T.
Published: 1990
Full Text: View/download PDF

29. Effects of CoCrZr seed layer on noise properties and microstructure of CoCrPt media

Author: Kanbe, T., Tamai, I., Takahashi, Y., Tanahashi, K., Ishikawa, A., and Hosoe, Y.
Subjects: Magnetism -- Research, Magnetic recorders and recording -- Research, Thin films -- Magnetic properties, Physics
Abstract: A study was conducted to analyze the influence of CoCrZr seed layer on the noise characteristics and microstructure of CoCrPT media. The films were deposited on chemically enforced soda-lime glass substrates by direct current magnetron sputtering. Experimental results indicated that the microstructure is very sensitive to the zirconium content and affects the microstructure of the magnetic layer.
Published: 1999

30. Suppression of low-temperature ferromagnetic phase in ultrathin FeRh films.

Author: Han, G. C., Qiu, J. J., Yap, Q. J., Luo, P., Kanbe, T., Shige, T., Laughlin, D. E., and Zhu, J.-G.
Subjects: ANTIFERROMAGNETIC materials, THIN films, SEMICONDUCTORS, SILICON, MAGNETIZATION
Abstract: Highly ordered B2 FeRh films with sharp magnetic transitions from the antiferromagnetic (AF) to ferromagnetic (FM) states were prepared on thermally oxidized Si wafers with thicknesses as low as 10 nm. It is found that the transition temperature increases as the thickness decreases from 80 nm to 15 nm, and then decreases from 15 nm to 10 nm. While the ratio of the residual magnetization to the maximum magnetization keeps nearly unchanged for the film thickness of 15 nm and larger, it increases significantly when the thickness is reduced to 10 nm. This residual magnetization was suppressed by slightly increasing the Rh atomic content in 10 nm thick FeRh films. Low-pressure deposition is found to play an important role in the stabilization of the AF phase. By depositing FeRh films at an extremely low pressure of 0.057 Pa, a residual magnetization as small as 13.5 emu/cc at 100 K was observed for a film with a nominal thickness of 10 nm deposited on Si wafer. This value was further reduced to 6 emu/cc when the film is deposited on MgO substrates due to much improved FeRh crystallinity. These results are in close agreement with theoretical predictions on defect and interface induced FM stabilization. [ABSTRACT FROM AUTHOR]
Published: 2013
Full Text: View/download PDF

31. Experimental study of thermal decay in high-density magnetic recording media

Author: Hosoe, Y., Tamai, I., Tanahashi, K., Takahashi, Y., Yamamoto, T., Kanbe, T., and Yajima, Y.
Subjects: Thin films -- Evaluation, Business, Electronics, Electronics and electrical industries
Abstract: The thermal decay of written bits in CoCrPt/CrTi thin film media for high density longitudinal magnetic recording is examined using a magnetoresistive head at room temperature. A decay in signal output over time is observed for the media with a thin magnetic layer less than about 14 nm thick and the media noise increases. The thermal stability factor Ku [center dot] V/k [center dot] T of these media is estimated to be less than about 100. The signal decay and noise increase are more serious at higher linear recording densities. These results are consistent with the results of a micromagnetic simulation taking into account the thermal aftereffects. These characteristics suggest that media with a large magnetic anisotropy constant Ku will be required to realize high storage densities of over 10 Gb/[in.sup.2].
Published: 1997

32. Effects of boron addition to underlayer for CoCrPt media on magnetic characteristics and microstructure

Author: Kanbe, T., Tamai, I., Takahashi, Y., Tanahashi, K., Hosoe, Y., Ishikawa, A., and Kataoka, H.
Subjects: Boron -- Analysis, Thin films -- Magnetic properties, Microstructure -- Analysis, Business, Electronics, Electronics and electrical industries
Abstract: Magnetic and recording characteristics of CoCrPt media with a CrTiB underlayer was investigated. Higher coercivity Hc and coercive squareness [S.sup.*] were obtained compared with the media that had a CrTi underlayer. The overwrite property of the media was also improved by adding boron, while the change in media noise was very small. Transmission electron microscopy analysis showed that the crystal grain-size dispersion in the magnetic layer was reduced by about 15% when boron was added to the underlayer, and the average grain size was almost the same as when the CrTi underlayer was used. The higher [S.sup.*] and improved overwrite property that resulted when using a CrTiB underlayer should be attributed to the reduction in the grain size dispersion, which provides a narrower switching field distribution.
Published: 1997

33. Gene disruption to improve 1,3-propanediol production in Citrobacter braakii strain TB-96

Author: Matsumoto, M., primary, Kiyoshi, K., additional, Nonaka, D., additional, Morita, T., additional, and Nakajima-Kanbe, T., additional
Published: 2018
Full Text: View/download PDF

34. Effects of Surface Oxidization of Amorphous Ni-Based Alloy Seed Layers on Noise in CoCrPt/CrTi Media

Author: Matsuda, Y., Sakamoto, K., Takahashi, Y., Tanahashi, K., Kanbe, T., Katou, A., and Hosoe, Y.
Subjects: Magnetism -- Research, Noise reduction systems (Electronics) -- Research, Business, Electronics, Electronics and electrical industries
Abstract: New amorphous seed layers of NiCrZr and NiTa have been developed to reduce the noise of CoCrPt/CrTi thin film media on a glass substrate. By exposing the surfaces of the Ni-based amorphous seed layers to low pressure oxygen of the order of [10.sup.-3] Pa, the crystal orientation of the CoCrPt magnetic layer is changed from random-like to (11.0), and the magnetic crystal grain size is reduced as in the case of Co-based amorphous seed layer of CoCrZr. These changes in microstructure result in higher coercivities and lower media noises in both cases for the NiCrZr and NiTa seed layers. The grain size distribution of the magnetic layer is also reduced by the surface oxidization of the seed layer. This also contributes to improvements in read/write performance of the media. Index Terms--CoCrPt/CrTi, media noise, NiCrZr, NiTa, seed layer, surface oxidization.
Published: 2001

35. Effects of Surface Oxidization of Amorphous Ni-Based Alloy Seed Layers on Noise in CoCrPt/CrTi Media

Author: Matsuda, Y., Sakamoto, K., Takahashi, Y., Tanahashi, K., Kanbe, T., Katou, A., and Hosoe, Y.
Subjects: Amorphous substances -- Magnetic properties, Thin films -- Magnetic properties, Nickel alloys -- Testing, Surface chemistry -- Influence, Business, Electronics, Electronics and electrical industries
Abstract: New amorphous seed layers of NiCrZr and NiTa have been developed to reduce the noise of CoCrPt/CrTi thin film media on a glass substrate. By exposing the surfaces of the Ni-based amorphous seed layers to low pressure oxygen of the order of [10.sup.-3] Pa, the crystal orientation of the CoCrPt magnetic layer is changed from random-like to (11.0), and the magnetic crystal grain size is reduced as in the case of Co-based amorphous seed layer of CoCrZr. These changes in microstructure result in higher coercivities and lower media noises in both cases for the NiCrZr and NiTa seed layers. The grain size distribution of the magnetic layer is also reduced by the surface oxidization of the seed layer. This also contributes to improvements in read/write performance of the media. Index Terms--CoCrPt/CrTi, media noise, NiCrZr, NiTa, seed layer, surface oxidization.
Published: 2000

36. Effects of underlayer grain size on the microstructure of the magnetic layer in CoCrPt media

Author: Kanbe, T., Takahashi, Y., Tanahashi, K., Ishikawa, A., and Hosoe, Y.
Subjects: Magnetism -- Research, Thin films -- Magnetic properties, Microstructure -- Research, Business, Electronics, Electronics and electrical industries
Abstract: The average grain size of the CrTi or CrTiB underlayer was reduced from 16 to 7 nm and structural changes of the CoCrPt magnetic layer deposited on them were investigated. Reduction of the underlayer grain size tends to suppress the formation of bi-crystal clusters, though the magnetic layer has a CoCrPt (11.0) crystallographic texture. The average grain size of the magnetic layer showed a minimum when that of the underlayer was 9 nm. Further reduction of the underlayer grain size to 7 nm increased the average magnetic grain size about 15 %. On the other hand, when the average underlayer grain size was less than 11 nm, the normalized standard deviation of the magnetic layer remained the same upon further reduction in the normalized standard deviation of the underlayer. Index terms--thin film media, microstructure, bi-crystal, grain size HRTEM.
Published: 1999

37. The author list of the Telescope Array Collaboration

Author: Yoneda Y., Yoshida S., Yang J., Yamaoka H., Yamazaki K., Yamane R., Yamakawa Y., Wood M., Wong T., Vasiloff G., Wada Y., Ukai H., Udo S., Uchihori Y., Tsuyuguchi Y., Tsutsumi K., Tsunesada Y., Tomida T., Troitsky S., Tokuno H., Tinyakov P., Tkachev I., Thomson G.B., Thomas S.B., Tanaka M., Tanaka H., Tanaka K., Tameda Y., Takita M., Taketa A., Takahashi Y., Takeda M., Suzuki S., Stroman T., Stratton S.R., Stokes B.T., Springer R.W., Sonley T.J., Sokolsky P., Shirahama T., Smith J.D., Shin J.I., Shimodaira H., Shin B.K., Shibata T., Shibata F., Shah P.D., Scott L.M., Sampson A.L., Sakurai N., Sagawa H., Rubtsov G., Ryu D., Roh S.Y., Rodriguez D.C., Park I.H., Pshirkov M.S., Ozawa S., Oshima A., Okuda T., Oku D., Oki K., Ohnishi, Ohoka H., Nonaka T., Ogio S., Nam S.W., Nagataki S., Nakamura T., Nagasawa K., Myers I., Murano Y., Minamino M., Miyata K., Matthews J.N., Matsuyama T., Matsuura T., Matsuda T., Martineau J., Martens K., Machida S., Lim S.I., Kwon Y.J., Kuramoto K., Kuzmin V., Kondo Y., Kobayashi Y., Kobayashi K., Kitamura Y., Kitamoto K., Kitamura S., Kim J.H., Kim H.K., Kim H.B., Kawana S., Kido E., Kawakami S., Kawai H., Kanbe T., Kasahara K., Kalashev O., Kakimoto F., Kadota K., Jui C.C.H., Ivanov D., Iwamoto S., Ishimori R., Inoue N., Ishii T., Ikuta K., Ikeda D., Iguchi T., Honda K., Hiyama K., Hayashida N., Hibino K., Hayashi Y., Hayashi K., Hanlon W., Fukushima M., Fukuda T., Fujii T., Fujii H., Cho W.R., Cho E.J., Chikawa M., Chiba J., Cheon B.G., Cady R., Blake S.A., Bergman D.R., Belz J.W., Barcikowski E., Azuma R., Anderson R., Allen M., Aida R., Abu-Zayyad T., Yoshii H., Zhou X., Zollinger R., and Zundel Z.
Subjects: lcsh:Physics, lcsh:QC1-999
Published: 2013

38. Mitosis in the dermatophyteMicrosporum canis as revealed by freeze substitution electron microscopy

Author: Kanbe, T. and Tanaka, K.
Published: 1985
Full Text: View/download PDF

39. Effects of an intermediate layer on the magnetic and recording characteristics of CoCrPtTa media.

Author: Tanahashi, K., Tamai, I., Matsunuma, S., Kanbe, T., Ishikawa, A., Matsuda, Y., Yahisa, Y., and Hosoe, Y.
Subjects: MAGNETIC recorders & recording, ELECTRONIC noise
Abstract: Effects of bcc and hcp intermediate layers between a bcc–Cr[sub 80]Ti[sub 20] underlayer and a hcp–CoCrPtTa magnetic layer on magnetic and recording characteristics were investigated. The medium without an intermediate layer has a low coercivity H[sub c] of 0.27 kOe due to the perpendicular orientation of the c axis of the CoCrPtTa layer. By introducing a 5-nm-thick intermediate layer of bcc–Cr[sub 60]Mo[sub 40] or hcp–Co[sub 70]Cr[sub 30], the c axis of the CoCrPtTa layer can be effectively in-plane oriented, resulting in a high H[sub c] of 2.71–2.87 kOe and a coercive squareness S[sup *] of 0.72–0.81. The medium with the Cr[sub 60]Mo[sub 40] layer has lower media noise than the medium with the Co[sub 70]Cr[sub 30] layer. This lower noise is considered to be caused by the small grain size of 10.4 nm. The addition of the thin Cr[sub 60]Mo[sub 40] intermediate layer is therefore effective to obtain both high H[sub c] and low noise in the CoCrPtTa media with the CrTi underlayer. © 2000 American Institute of Physics. [ABSTRACT FROM AUTHOR]
Published: 2000
Full Text: View/download PDF

40. Juvenile hormone titre and related gene expression during the change of reproductive modes in the pea aphid

Author: Ishikawa, A., Ogawa, K., Gotoh, H., Walsh, T. K., Tagu, Denis, Brisson, J. A., Rispe, Claude, Jaubert-Possamai, S., Kanbe, T., Tsubota, T., Shiotsuki, T., Miura, T., Hokkaido University [Sapporo, Japan], Commonwealth Scientific and Industrial Research Organisation [Canberra] (CSIRO), Institut de Génétique, Environnement et Protection des Plantes (IGEPP), Université de Rennes 1 (UR1), Université de Rennes (UNIV-RENNES)-Université de Rennes (UNIV-RENNES)-AGROCAMPUS OUEST, Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro)-Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro)-Institut National de Recherche pour l’Agriculture, l’Alimentation et l’Environnement (INRAE), University of Nebraska, Partenaires INRAE, Institut National de la Recherche Agronomique (INRA)-Université de Rennes 1 (UR1), Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro)-Institut national d'enseignement supérieur pour l'agriculture, l'alimentation et l'environnement (Institut Agro), National Institute of Agrobiological Sciences, Ministry of Education, Culture, Sports, Science and Technology of Japan [18370007, 20033002, 20657004, 21677001], Inamori Foundation, France by ANR, CSIRO OCE, and Institut National de la Recherche Agronomique (INRA)-Université de Rennes (UR)-AGROCAMPUS OUEST
Subjects: cyclical parthenogenesis, MYZUS-PERSICAE, PARTHENOGENESIS, juvenile hormone, Polyphenism, [SDV]Life Sciences [q-bio], food and beverages, PHOTOPERIODICALLY CONTROLLED POLYMORPHISM, MASS-SPECTROMETRY, KINOPRENE, EVOLUTIONARY GENETICS, SOCIAL-INSECT, SEXUAL FORMS, ACYRTHOSIPHON-PISUM, juvenile hormone esterase, MEGOURA-VICIAE BUCKTON
Abstract: Publication Inra prise en compte dans l'analyse bibliométrique des publications scientifiques mondiales sur les Fruits, les Légumes et la Pomme de terre. Période 2000-2012. http://prodinra.inra.fr/record/256699; International audience; Most aphids show reproductive polyphenism, i.e. they alternate their reproductive modes from parthenogenesis to sexual reproduction in response to short photoperiods. Although juvenile hormone (JH) has been considered a likely candidate for regulating the transition from asexual to sexual reproduction after photoperiod sensing, there are few studies investigating the direct relationship between JH titres and the reproductive-mode change. In addition, the sequencing of the pea aphid genome has allowed identification of the genes involved in the JH pathway, which in turn allows us to examine their expression levels in relation to the reproductive-mode change. Using liquid chromatography-mass spectrometry in the pea aphid, JHIII titre was shown to be lower in aphids producing sexual morphs under short-day conditions than in aphids producing parthenogenetic morphs under long-day conditions. The expression levels of genes upstream and downstream of JH action were quantified by real-time quantitative reverse-transcription-PCR across the reproductive-mode change. The expression level of JH esterase, which is responsible for JH degradation, was significantly higher in aphids reared under short-day conditions. This suggests that the upregulation of the JH degradation pathway may be responsible for the lower JHIII titre in aphids exposed to short-days, leading to the production of sexual morphs.
Published: 2012

41. SELECTIVE INHIBITION OF CYCLIC AMP PHOSPHODIESTERASE BY OPC-3689 AN ANTITHROMBOTIC AGENT

Author: Kohri, H., primary, Kimura, Y., additional, Watanabe, K., additional, Kanbe, T., additional, Nishi, T., additional, Nakagawa, K., additional, Hayashi, H., additional, and Hidaka, H., additional
Published: 1978
Full Text: View/download PDF

42. A ring structure around the dividing plane of theCyanidium caldarium chloroplast

Author: Mita, T., Kanbe, T., Tanaka, K., and Kuroiwa, T.
Published: 1986
Full Text: View/download PDF

43. Upper limit on the flux of photons with energies above1019eVusing the Telescope Array surface detector

Author: Abu-Zayyad, T., primary, Aida, R., additional, Allen, M., additional, Anderson, R., additional, Azuma, R., additional, Barcikowski, E., additional, Belz, J. W., additional, Bergman, D. R., additional, Blake, S. A., additional, Cady, R., additional, Cheon, B. G., additional, Chiba, J., additional, Chikawa, M., additional, Cho, E. J., additional, Cho, W. R., additional, Fujii, H., additional, Fujii, T., additional, Fukuda, T., additional, Fukushima, M., additional, Gorbunov, D., additional, Hanlon, W., additional, Hayashi, K., additional, Hayashi, Y., additional, Hayashida, N., additional, Hibino, K., additional, Hiyama, K., additional, Honda, K., additional, Iguchi, T., additional, Ikeda, D., additional, Ikuta, K., additional, Inoue, N., additional, Ishii, T., additional, Ishimori, R., additional, Ivanov, D., additional, Iwamoto, S., additional, Jui, C. C. H., additional, Kadota, K., additional, Kakimoto, F., additional, Kalashev, O., additional, Kanbe, T., additional, Kasahara, K., additional, Kawai, H., additional, Kawakami, S., additional, Kawana, S., additional, Kido, E., additional, Kim, H. B., additional, Kim, H. K., additional, Kim, J. H., additional, Kitamoto, K., additional, Kitamura, S., additional, Kitamura, Y., additional, Kobayashi, K., additional, Kobayashi, Y., additional, Kondo, Y., additional, Kuramoto, K., additional, Kuzmin, V., additional, Kwon, Y. J., additional, Lan, J., additional, Lim, S. I., additional, Machida, S., additional, Martens, K., additional, Matsuda, T., additional, Matsuura, T., additional, Matsuyama, T., additional, Matthews, J. N., additional, Minamino, M., additional, Miyata, K., additional, Murano, Y., additional, Myers, I., additional, Nagasawa, K., additional, Nagataki, S., additional, Nakamura, T., additional, Nam, S. W., additional, Nonaka, T., additional, Ogio, S., additional, Ohnishi, M., additional, Ohoka, H., additional, Oki, K., additional, Oku, D., additional, Okuda, T., additional, Oshima, A., additional, Ozawa, S., additional, Park, I. H., additional, Pshirkov, M. S., additional, Rodriguez, D. C., additional, Roh, S. Y., additional, Rubtsov, G. I., additional, Ryu, D., additional, Sagawa, H., additional, Sakurai, N., additional, Sampson, A. L., additional, Scott, L. M., additional, Shah, P. D., additional, Shibata, F., additional, Shibata, T., additional, Shimodaira, H., additional, Shin, B. K., additional, Shin, J. I., additional, Shirahama, T., additional, Smith, J. D., additional, Sokolsky, P., additional, Stokes, B. T., additional, Stratton, S. R., additional, Stroman, T., additional, Suzuki, S., additional, Takahashi, Y., additional, Takeda, M., additional, Taketa, A., additional, Takita, M., additional, Tameda, Y., additional, Tanaka, H., additional, Tanaka, K., additional, Tanaka, M., additional, Thomas, S. B., additional, Thomson, G. B., additional, Tinyakov, P., additional, Tkachev, I., additional, Tokuno, H., additional, Tomida, T., additional, Troitsky, S., additional, Tsunesada, Y., additional, Tsutsumi, K., additional, Tsuyuguchi, Y., additional, Uchihori, Y., additional, Udo, S., additional, Ukai, H., additional, Vasiloff, G., additional, Wada, Y., additional, Wong, T., additional, Wood, M., additional, Yamakawa, Y., additional, Yamane, R., additional, Yamaoka, H., additional, Yamazaki, K., additional, Yang, J., additional, Yoneda, Y., additional, Yoshida, S., additional, Yoshii, H., additional, Zhou, X., additional, Zollinger, R., additional, and Zundel, Z., additional
Published: 2013
Full Text: View/download PDF

44. CORRELATIONS OF THE ARRIVAL DIRECTIONS OF ULTRA-HIGH ENERGY COSMIC RAYS WITH EXTRAGALACTIC OBJECTS AS OBSERVED BY THE TELESCOPE ARRAY EXPERIMENT

Author: Abu-Zayyad, T., primary, Aida, R., additional, Allen, M., additional, Anderson, R., additional, Azuma, R., additional, Barcikowski, E., additional, Belz, J. W., additional, Bergman, D. R., additional, Blake, S. A., additional, Cady, R., additional, Cheon, B. G., additional, Chiba, J., additional, Chikawa, M., additional, Cho, E. J., additional, Cho, W. R., additional, Fujii, H., additional, Fujii, T., additional, Fukuda, T., additional, Fukushima, M., additional, Hanlon, W., additional, Hayashi, K., additional, Hayashi, Y., additional, Hayashida, N., additional, Hibino, K., additional, Hiyama, K., additional, Honda, K., additional, Iguchi, T., additional, Ikeda, D., additional, Ikuta, K., additional, Inoue, N., additional, Ishii, T., additional, Ishimori, R., additional, Ito, H., additional, Ivanov, D., additional, Iwamoto, S., additional, Jui, C. C. H., additional, Kadota, K., additional, Kakimoto, F., additional, Kalashev, O., additional, Kanbe, T., additional, Kasahara, K., additional, Kawai, H., additional, Kawakami, S., additional, Kawana, S., additional, Kawata, K., additional, Kido, E., additional, Kim, H. B., additional, Kim, H. K., additional, Kim, J. H., additional, Kitamoto, K., additional, Kitamura, S., additional, Kitamura, Y., additional, Kobayashi, K., additional, Kobayashi, Y., additional, Kondo, Y., additional, Kuramoto, K., additional, Kuzmin, V., additional, Kwon, Y. J., additional, Lan, J., additional, Lim, S. I., additional, Lundquist, J. P., additional, Machida, S., additional, Martens, K., additional, Matsuda, T., additional, Matsuura, T., additional, Matsuyama, T., additional, Matthews, J. N., additional, Minamino, M., additional, Miyata, K., additional, Murano, Y., additional, Myers, I., additional, Nagasawa, K., additional, Nagataki, S., additional, Nakamura, T., additional, Nam, S. W., additional, Nonaka, T., additional, Ogio, S., additional, Ohnishi, M., additional, Ohoka, H., additional, Oki, K., additional, Oku, D., additional, Okuda, T., additional, Ono, M., additional, Oshima, A., additional, Ozawa, S., additional, Park, I. H., additional, Pshirkov, M. S., additional, Rodriguez, D. C., additional, Roh, S. Y., additional, Rubtsov, G., additional, Ryu, D., additional, Sagawa, H., additional, Sakurai, N., additional, Sampson, A. L., additional, Scott, L. M., additional, Shah, P. D., additional, Shibata, F., additional, Shibata, T., additional, Shimodaira, H., additional, Shin, B. K., additional, Shin, J. I., additional, Shirahama, T., additional, Smith, J. D., additional, Sokolsky, P., additional, Springer, R. W., additional, Stokes, B. T., additional, Stratton, S. R., additional, Stroman, T., additional, Suzuki, S., additional, Takahashi, Y., additional, Takeda, M., additional, Taketa, A., additional, Takita, M., additional, Tameda, Y., additional, Tanaka, H., additional, Tanaka, K., additional, Tanaka, M., additional, Thomas, S. B., additional, Thomson, G. B., additional, Tinyakov, P., additional, Tkachev, I., additional, Tokuno, H., additional, Tomida, T., additional, Troitsky, S., additional, Tsunesada, Y., additional, Tsutsumi, K., additional, Tsuyuguchi, Y., additional, Uchihori, Y., additional, Udo, S., additional, Ukai, H., additional, Urban, F., additional, Vasiloff, G., additional, Wada, Y., additional, Wong, T., additional, Yamakawa, Y., additional, Yamane, R., additional, Yamaoka, H., additional, Yamazaki, K., additional, Yang, J., additional, Yoneda, Y., additional, Yoshida, S., additional, Yoshii, H., additional, Zhou, X., additional, Zollinger, R., additional, and Zundel, Z., additional
Published: 2013
Full Text: View/download PDF

45. Magnetic stability of ultrathin FeRh films

Author: Han, G. C., primary, Qiu, J. J., additional, Yap, Q. J., additional, Luo, P., additional, Laughlin, D. E., additional, Zhu, J. G., additional, Kanbe, T., additional, and Shige, T., additional
Published: 2013
Full Text: View/download PDF

46. THE COSMIC-RAY ENERGY SPECTRUM OBSERVED WITH THE SURFACE DETECTOR OF THE TELESCOPE ARRAY EXPERIMENT

Author: Abu-Zayyad, T., primary, Aida, R., additional, Allen, M., additional, Anderson, R., additional, Azuma, R., additional, Barcikowski, E., additional, Belz, J. W., additional, Bergman, D. R., additional, Blake, S. A., additional, Cady, R., additional, Cheon, B. G., additional, Chiba, J., additional, Chikawa, M., additional, Cho, E. J., additional, Cho, W. R., additional, Fujii, H., additional, Fujii, T., additional, Fukuda, T., additional, Fukushima, M., additional, Hanlon, W., additional, Hayashi, K., additional, Hayashi, Y., additional, Hayashida, N., additional, Hibino, K., additional, Hiyama, K., additional, Honda, K., additional, Iguchi, T., additional, Ikeda, D., additional, Ikuta, K., additional, Inoue, N., additional, Ishii, T., additional, Ishimori, R., additional, Ivanov, D., additional, Iwamoto, S., additional, Jui, C. C. H., additional, Kadota, K., additional, Kakimoto, F., additional, Kalashev, O., additional, Kanbe, T., additional, Kasahara, K., additional, Kawai, H., additional, Kawakami, S., additional, Kawana, S., additional, Kido, E., additional, Kim, H. B., additional, Kim, H. K., additional, Kim, J. H., additional, Kitamoto, K., additional, Kitamura, S., additional, Kitamura, Y., additional, Kobayashi, K., additional, Kobayashi, Y., additional, Kondo, Y., additional, Kuramoto, K., additional, Kuzmin, V., additional, Kwon, Y. J., additional, Lan, J., additional, Lim, S. I., additional, Machida, S., additional, Martens, K., additional, Matsuda, T., additional, Matsuura, T., additional, Matsuyama, T., additional, Matthews, J. N., additional, Minamino, M., additional, Miyata, K., additional, Murano, Y., additional, Myers, I., additional, Nagasawa, K., additional, Nagataki, S., additional, Nakamura, T., additional, Nam, S. W., additional, Nonaka, T., additional, Ogio, S., additional, Ohnishi, M., additional, Ohoka, H., additional, Oki, K., additional, Oku, D., additional, Okuda, T., additional, Oshima, A., additional, Ozawa, S., additional, Park, I. H., additional, Pshirkov, M. S., additional, Rodriguez, D. C., additional, Roh, S. Y., additional, Rubtsov, G., additional, Ryu, D., additional, Sagawa, H., additional, Sakurai, N., additional, Sampson, A. L., additional, Scott, L. M., additional, Shah, P. D., additional, Shibata, F., additional, Shibata, T., additional, Shimodaira, H., additional, Shin, B. K., additional, Shin, J. I., additional, Shirahama, T., additional, Smith, J. D., additional, Sokolsky, P., additional, Stokes, B. T., additional, Stratton, S. R., additional, Stroman, T., additional, Suzuki, S., additional, Takahashi, Y., additional, Takeda, M., additional, Taketa, A., additional, Takita, M., additional, Tameda, Y., additional, Tanaka, H., additional, Tanaka, K., additional, Tanaka, M., additional, Thomas, S. B., additional, Thomson, G. B., additional, Tinyakov, P., additional, Tkachev, I., additional, Tokuno, H., additional, Tomida, T., additional, Troitsky, S., additional, Tsunesada, Y., additional, Tsutsumi, K., additional, Tsuyuguchi, Y., additional, Uchihori, Y., additional, Udo, S., additional, Ukai, H., additional, Vasiloff, G., additional, Wada, Y., additional, Wong, T., additional, Wood, M., additional, Yamakawa, Y., additional, Yamane, R., additional, Yamaoka, H., additional, Yamazaki, K., additional, Yang, J., additional, Yoneda, Y., additional, Yoshida, S., additional, Yoshii, H., additional, Zhou, X., additional, Zollinger, R., additional, and Zundel, Z., additional
Published: 2013
Full Text: View/download PDF

47. The energy spectrum of Telescope Array’s Middle Drum detector and the direct comparison to the High Resolution Fly’s Eye experiment

Author: Abu-Zayyad, T., primary, Aida, R., additional, Allen, M., additional, Anderson, R., additional, Azuma, R., additional, Barcikowski, E., additional, Belz, J.W., additional, Bergman, D.R., additional, Blake, S.A., additional, Cady, R., additional, Cheon, B.G., additional, Chiba, J., additional, Chikawa, M., additional, Cho, E.J., additional, Cho, W.R., additional, Fujii, H., additional, Fujii, T., additional, Fukuda, T., additional, Fukushima, M., additional, Gorbunov, D., additional, Hanlon, W., additional, Hayashi, K., additional, Hayashi, Y., additional, Hayashida, N., additional, Hibino, K., additional, Hiyama, K., additional, Honda, K., additional, Iguchi, T., additional, Ikeda, D., additional, Ikuta, K., additional, Inoue, N., additional, Ishii, T., additional, Ishimori, R., additional, Ivanov, D., additional, Iwamoto, S., additional, Jui, C.C.H., additional, Kadota, K., additional, Kakimoto, F., additional, Kalashev, O., additional, Kanbe, T., additional, Kasahara, K., additional, Kawai, H., additional, Kawakami, S., additional, Kawana, S., additional, Kido, E., additional, Kim, H.B., additional, Kim, H.K., additional, Kim, J.H., additional, Kitamoto, K., additional, Kitamura, S., additional, Kitamura, Y., additional, Kobayashi, K., additional, Kobayashi, Y., additional, Kondo, Y., additional, Kuramoto, K., additional, Kuzmin, V., additional, Kwon, Y.J., additional, Lim, S.I., additional, Machida, S., additional, Martens, K., additional, Martineau, J., additional, Matsuda, T., additional, Matsuura, T., additional, Matsuyama, T., additional, Matthews, J.N., additional, Myers, I., additional, Minamino, M., additional, Miyata, K., additional, Murano, Y., additional, Nagataki, S., additional, Nakamura, T., additional, Nam, S.W., additional, Nonaka, T., additional, Ogio, S., additional, Ohnishi, M., additional, Ohoka, H., additional, Oki, K., additional, Oku, D., additional, Okuda, T., additional, Oshima, A., additional, Ozawa, S., additional, Park, I.H., additional, Pshirkov, M.S., additional, Rodriguez, D.C., additional, Roh, S.Y., additional, Rubtsov, G., additional, Ryu, D., additional, Sagawa, H., additional, Sakurai, N., additional, Sampson, A.L., additional, Scott, L.M., additional, Shah, P.D., additional, Shibata, F., additional, Shibata, T., additional, Shimodaira, H., additional, Shin, B.K., additional, Shin, J.I., additional, Shirahama, T., additional, Smith, J.D., additional, Sokolsky, P., additional, Sonley, T.J., additional, Springer, R.W., additional, Stokes, B.T., additional, Stratton, S.R., additional, Stroman, T.A., additional, Suzuki, S., additional, Takahashi, Y., additional, Takeda, M., additional, Taketa, A., additional, Takita, M., additional, Tameda, Y., additional, Tanaka, H., additional, Tanaka, K., additional, Tanaka, M., additional, Thomas, S.B., additional, Thomson, G.B., additional, Tinyakov, P., additional, Tkachev, I., additional, Tokuno, H., additional, Tomida, T., additional, Troitsky, S., additional, Tsunesada, Y., additional, Tsutsumi, K., additional, Tsuyuguchi, Y., additional, Uchihori, Y., additional, Udo, S., additional, Ukai, H., additional, Vasiloff, G., additional, Wada, Y., additional, Wong, T., additional, Wood, M., additional, Yamakawa, Y., additional, Yamane, R., additional, Yamaoka, H., additional, Yamazaki, K., additional, Yang, J., additional, Yoneda, Y., additional, Yoshida, S., additional, Yoshii, H., additional, Zollinger, R., additional, and Zundel, Z., additional
Published: 2012
Full Text: View/download PDF

48. The surface detector array of the Telescope Array experiment

Author: Abu-Zayyad, T., primary, Aida, R., additional, Allen, M., additional, Anderson, R., additional, Azuma, R., additional, Barcikowski, E., additional, Belz, J.W., additional, Bergman, D.R., additional, Blake, S.A., additional, Cady, R., additional, Cheon, B.G., additional, Chiba, J., additional, Chikawa, M., additional, Cho, E.J., additional, Cho, W.R., additional, Fujii, H., additional, Fujii, T., additional, Fukuda, T., additional, Fukushima, M., additional, Gorbunov, D., additional, Hanlon, W., additional, Hayashi, K., additional, Hayashi, Y., additional, Hayashida, N., additional, Hibino, K., additional, Hiyama, K., additional, Honda, K., additional, Iguchi, T., additional, Ikeda, D., additional, Ikuta, K., additional, Inoue, N., additional, Ishii, T., additional, Ishimori, R., additional, Ivanov, D., additional, Iwamoto, S., additional, Jui, C.C.H., additional, Kadota, K., additional, Kakimoto, F., additional, Kalashev, O., additional, Kanbe, T., additional, Kasahara, K., additional, Kawai, H., additional, Kawakami, S., additional, Kawana, S., additional, Kido, E., additional, Kim, H.B., additional, Kim, H.K., additional, Kim, J.H., additional, Kitamoto, K., additional, Kobayashi, K., additional, Kobayashi, Y., additional, Kondo, Y., additional, Kuramoto, K., additional, Kuzmin, V., additional, Kwon, Y.J., additional, Lim, S.I., additional, Machida, S., additional, Martens, K., additional, Martineau, J., additional, Matsuda, T., additional, Matsuura, T., additional, Matsuyama, T., additional, Matthews, J.N., additional, Myers, I., additional, Minamino, M., additional, Miyata, K., additional, Miyauchi, H., additional, Murano, Y., additional, Nakamura, T., additional, Nam, S.W., additional, Nonaka, T., additional, Ogio, S., additional, Ohnishi, M., additional, Ohoka, H., additional, Oki, K., additional, Oku, D., additional, Okuda, T., additional, Oshima, A., additional, Ozawa, S., additional, Park, I.H., additional, Pshirkov, M.S., additional, Rodriguez, D., additional, Roh, S.Y., additional, Rubtsov, G., additional, Ryu, D., additional, Sagawa, H., additional, Sakurai, N., additional, Sampson, A.L., additional, Scott, L.M., additional, Shah, P.D., additional, Shibata, F., additional, Shibata, T., additional, Shimodaira, H., additional, Shin, B.K., additional, Shin, J.I., additional, Shirahama, T., additional, Smith, J.D., additional, Sokolsky, P., additional, Sonley, T.J., additional, Springer, R.W., additional, Stokes, B.T., additional, Stratton, S.R., additional, Stroman, T.A., additional, Suzuki, S., additional, Takahashi, Y., additional, Takeda, M., additional, Taketa, A., additional, Takita, M., additional, Tameda, Y., additional, Tanaka, H., additional, Tanaka, K., additional, Tanaka, M., additional, Thomas, S.B., additional, Thomson, G.B., additional, Tinyakov, P., additional, Tkachev, I., additional, Tokuno, H., additional, Tomida, T., additional, Troitsky, S., additional, Tsunesada, Y., additional, Tsutsumi, K., additional, Tsuyuguchi, Y., additional, Uchihori, Y., additional, Udo, S., additional, Ukai, H., additional, Vasiloff, G., additional, Wada, Y., additional, Wong, T., additional, Wood, M., additional, Yamakawa, Y., additional, Yamaoka, H., additional, Yamazaki, K., additional, Yang, J., additional, Yoshida, S., additional, Yoshii, H., additional, Zollinger, R., additional, and Zundel, Z., additional
Published: 2012
Full Text: View/download PDF

49. SEARCH FOR ANISOTROPY OF ULTRAHIGH ENERGY COSMIC RAYS WITH THE TELESCOPE ARRAY EXPERIMENT

Author: Abu-Zayyad, T., primary, Aida, R., additional, Allen, M., additional, Anderson, R., additional, Azuma, R., additional, Barcikowski, E., additional, Belz, J. W., additional, Bergman, D. R., additional, Blake, S. A., additional, Cady, R., additional, Cheon, B. G., additional, Chiba, J., additional, Chikawa, M., additional, Cho, E. J., additional, Cho, W. R., additional, Fujii, H., additional, Fujii, T., additional, Fukuda, T., additional, Fukushima, M., additional, Hanlon, W., additional, Hayashi, K., additional, Hayashi, Y., additional, Hayashida, N., additional, Hibino, K., additional, Hiyama, K., additional, Honda, K., additional, Iguchi, T., additional, Ikeda, D., additional, Ikuta, K., additional, Inoue, N., additional, Ishii, T., additional, Ishimori, R., additional, Ivanov, D., additional, Iwamoto, S., additional, Jui, C. C. H., additional, Kadota, K., additional, Kakimoto, F., additional, Kalashev, O., additional, Kanbe, T., additional, Kasahara, K., additional, Kawai, H., additional, Kawakami, S., additional, Kawana, S., additional, Kido, E., additional, Kim, H. B., additional, Kim, H. K., additional, Kim, J. H., additional, Kitamoto, K., additional, Kitamura, S., additional, Kitamura, Y., additional, Kobayashi, K., additional, Kobayashi, Y., additional, Kondo, Y., additional, Kuramoto, K., additional, Kuzmin, V., additional, Kwon, Y. J., additional, Lim, S. I., additional, Machida, S., additional, Martens, K., additional, Martineau, J., additional, Matsuda, T., additional, Matsuura, T., additional, Matsuyama, T., additional, Matthews, J. N., additional, Minamino, M., additional, Miyata, K., additional, Murano, Y., additional, Myers, I., additional, Nagasawa, K., additional, Nagataki, S., additional, Nakamura, T., additional, Nam, S. W., additional, Nonaka, T., additional, Ogio, S., additional, Ohnishi, M., additional, Ohoka, H., additional, Oki, K., additional, Oku, D., additional, Okuda, T., additional, Oshima, A., additional, Ozawa, S., additional, Park, I. H., additional, Pshirkov, M. S., additional, Rodriguez, D. C., additional, Roh, S. Y., additional, Rubtsov, G., additional, Ryu, D., additional, Sagawa, H., additional, Sakurai, N., additional, Sampson, A. L., additional, Scott, L. M., additional, Shah, P. D., additional, Shibata, F., additional, Shibata, T., additional, Shimodaira, H., additional, Shin, B. K., additional, Shin, J. I., additional, Shirahama, T., additional, Smith, J. D., additional, Sokolsky, P., additional, Sonley, T. J., additional, Springer, R. W., additional, Stokes, B. T., additional, Stratton, S. R., additional, Stroman, T., additional, Suzuki, S., additional, Takahashi, Y., additional, Takeda, M., additional, Taketa, A., additional, Takita, M., additional, Tameda, Y., additional, Tanaka, H., additional, Tanaka, K., additional, Tanaka, M., additional, Thomas, S. B., additional, Thomson, G. B., additional, Tinyakov, P., additional, Tkachev, I., additional, Tokuno, H., additional, Tomida, T., additional, Troitsky, S., additional, Tsunesada, Y., additional, Tsutsumi, K., additional, Tsuyuguchi, Y., additional, Uchihori, Y., additional, Udo, S., additional, Ukai, H., additional, Vasiloff, G., additional, Wada, Y., additional, Wong, T., additional, Wood, M., additional, Yamakawa, Y., additional, Yamane, R., additional, Yamaoka, H., additional, Yamazaki, K., additional, Yang, J., additional, Yoneda, Y., additional, Yoshida, S., additional, Yoshii, H., additional, Zhou, X., additional, Zollinger, R., additional, and Zundel, Z., additional
Published: 2012
Full Text: View/download PDF

50. New air fluorescence detectors employed in the Telescope Array experiment

Author: Tokuno, H., primary, Tameda, Y., additional, Takeda, M., additional, Kadota, K., additional, Ikeda, D., additional, Chikawa, M., additional, Fujii, T., additional, Fukushima, M., additional, Honda, K., additional, Inoue, N., additional, Kakimoto, F., additional, Kawana, S., additional, Kido, E., additional, Matthews, J.N., additional, Nonaka, T., additional, Ogio, S., additional, Okuda, S., additional, Ozawa, S., additional, Sagawa, H., additional, Sakurai, N., additional, Shibata, T., additional, Taketa, A., additional, Thomas, S.B., additional, Tomida, T., additional, Tsunesada, Y., additional, Udo, S., additional, Abu-zayyad, T., additional, Aida, R., additional, Allen, M., additional, Anderson, R., additional, Azuma, R., additional, Barcikowski, E., additional, Belz, J.W., additional, Bergman, D.R., additional, Blake, S.A., additional, Cady, R., additional, Cheon, B.G., additional, Chiba, J., additional, Cho, E.J., additional, Cho, W.R., additional, Fujii, H., additional, Fukuda, T., additional, Gorbunov, D., additional, Hanlon, W., additional, Hayashi, K., additional, Hayashi, Y., additional, Hayashida, N., additional, Hibino, K., additional, Hiyama, K., additional, Iguchi, T., additional, Ikuta, K., additional, Ishii, T., additional, Ishimori, R., additional, Ivanov, D., additional, Iwamoto, S., additional, Jui, C.C.H., additional, Kalashev, O., additional, Kanbe, T., additional, Kasahara, K., additional, Kawai, H., additional, Kawakami, S., additional, Kim, H.B., additional, Kim, H.K., additional, Kim, J.H., additional, Kitamoto, K., additional, Kobayashi, K., additional, Kobayashi, Y., additional, Kondo, Y., additional, Kuramoto, K., additional, Kuzmin, V., additional, Kwon, Y.J., additional, Lim, S.I., additional, Machida, S., additional, Martens, K., additional, Martineau, J., additional, Matsuda, T., additional, Matsuura, T., additional, Matsuyama, T., additional, Myers, I., additional, Minamino, M., additional, Miyata, K., additional, Miyauchi, H., additional, Murano, Y., additional, Nakamura, T., additional, Nam, S.W., additional, Ohnishi, M., additional, Ohoka, H., additional, Oki, K., additional, Oku, D., additional, Oshima, A., additional, Park, I.H., additional, Pshirkov, M.S., additional, Rodriguez, D., additional, Roh, S.Y., additional, Rubtsov, G., additional, Ryu, D., additional, Sampson, A.L., additional, Scott, L.M., additional, Shah, P.D., additional, Shibata, F., additional, Shimodaira, H., additional, Shin, B.K., additional, Shin, J.I., additional, Shirahama, T., additional, Smith, J.D., additional, Sokolsky, P., additional, Sonley, T.J., additional, Springer, R.W., additional, Stokes, B.T., additional, Stratton, S.R., additional, Stroman, T., additional, Suzuki, S., additional, Takahashi, Y., additional, Takita, M., additional, Tanaka, H., additional, Tanaka, K., additional, Tanaka, M., additional, Thomson, G.B., additional, Tinyakov, P., additional, Tkachev, I., additional, Troitsky, S., additional, Tsutsumi, K., additional, Tsuyuguchi, Y., additional, Uchihori, Y., additional, Ukai, H., additional, Vasiloff, G., additional, Wada, Y., additional, Wong, T., additional, Wood, M., additional, Yamakawa, Y., additional, Yamaoka, H., additional, Yamazaki, K., additional, Yang, J., additional, Yoshida, S., additional, Yoshii, H., additional, Zollinger, R., additional, and Zundel, Z., additional
Published: 2012
Full Text: View/download PDF

Catalog

Books, media, physical & digital resources

See catalog results

Searchworks

Select search scope, currently: Articles Catalog books, media & more in Jio Institute collections Articles journal articles & other e-resources

Search

Search Constraints

Refine your results

Search Limiters

Topic

Publication Year Range

Language

Publication Type

Journal

Region

Database

Publisher

482 results on '"Kanbe T"'

Search Results

Catalog

Select search scope, currently: Articles

Catalog

books, media & more in Jio Institute collections

Articles

journal articles & other e-resources