Status of Japanese gravitational wave detectors (2009)
Arai, K., Takahashi, R., Tatsumi, D., Izumi, K., Wakabayashi, Y., Ishizaki, H., ...
The Large-scale Cryogenic Gravitational wave Telescope (LCGT) is planned as a future Japanese project for gravitational wave detection. A 3 km interferometer will be built in an underground mine at...
Experimental and numerical studies of portable PEMFC stack (2009)
Shimpalee, S., Ohashi, M., Zee, J.W. Van, Ziegler, C., Stoeckmann, C., Sadeler, C., ...
The objective of this work is to establish the design principles of a proton exchange membrane (PEM) fuel cell (FC) stack for portable applications. A combination of experiments and numerical...
Current status of the CLIO project (2008)
Yamamoto, K, Uchiyama, T, Miyoki, S, Ohashi, M, Kuroda, K, Ishitsuka, H, ...
CLIO (Cryogenic Laser Interferometer Observatory) is a Japanese gravitational wave detector project. One of the main purposes of CLIO is to demonstrate thermal-noise suppression by cooling mirrors...
Parametric instabilities in the LCGT arm cavity (2008)
Yamamoto, K, Uchiyama, T, Miyoki, S, Ohashi, M, Kuroda, K, Numata, K
We evaluated the parametric instabilities of LCGT (Japanese interferometric gravitational wave detector project) arm cavity. The number of unstable modes of LCGT is 10-times smaller than that of...
Ando, M., Kawamura, Seiji, Nakamura, T., Tsubono, K., Tanaka, T., Funaki, I., ...
DECIGO pathfinder (DPF) is a milestone satellite mission for DECIGO (DECi-hertz Interferometer Gravitational wave Observatory) which is a future space gravitational wave antenna. DECIGO is expected...
The Japanese space gravitational wave antenna: DECIGO (2008)
Kawamura, Seiji, Ando, M., Nakamura, T., Tsubono, K., Tanaka, T., Funaki, I., ...
DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. DECIGO is expected to open a new window of observation for gravitational...
The Japanese space gravitational wave antenna - DECIGO (2008)
Kawamura, Seiji, Ando, M., Nakamura, T., Tsubono, K., Tanaka, T., Funaki, I., ...
DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. The goal of DECIGO is to detect gravitational waves from various kinds of...
Control system for the seismic attenuation system (SAS) in TAMA300 (2008)
Agatsuma, K., Takahashi, R., Arai, K., Tatsumi, D., Fukushima, M., Yamazaki, T., ...
A new seismic isolation system, TAMA Seismic Attenuation System (TAMA-SAS), was installed to TAMA300 in order to improve the sensitivity at low frequencies. Inertial damping is one of the...
Fukuda, T, Ohashi, M, Wei, B, Okada, T, Ichikawa, M, Taniguchi, Y
This paper was published in [OPTICS LETTERS] and is made available as an electronic reprint with the permission of OSA. The paper can be found at the following URL on the OSA website:...
Joint LIGO and TAMA300 search for gravitational waves from inspiralling neutron star binaries (2006)
Abbott, B., Abbott, R., Adhikari, R., Ageev, A., Agresti, J., Ajith, P., ...
We search for coincident gravitational wave signals from inspiralling neutron star binaries using LIGO and TAMA300 data taken during early 2003. Using a simple trigger exchange method, we perform an...
Joint LIGO and TAMA300 search for gravitational waves from inspiralling neutron star binaries (2006)
Abbott, B., Abbott, R., Adhikari, R., Ageev, A., Agresti, Juri, Ajith, P., ...
We search for coincident gravitational wave signals from inspiralling neutron star binaries using LIGO and TAMA300 data taken during early 2003. Using a simple trigger exchange method, we perform an...
Akutsu, Tomomi, Akutsu, Tomotadu, Ando, Masaki, Arai, Koji, Araya, Akito, Asada, H., ...
We analyze the data of the TAMA300 detector to search for gravitational waves from inspiraling compact star binaries with masses of the component stars in the range 1M[sun]–3M[sun]. In this...
The Japanese space gravitational wave antenna - DECIGO (2006)
Kawamura, Seiji, Nakamura, T., Ando, M., Seto, N., Tsubono, K., Numata, K., ...
DECi-hertz Interferometer Gravitational wave Observatory (DECIGO) is the future Japanese space gravitational wave antenna. It aims at detecting various kinds of gravitational waves between 1 mHz and...
Upper limits from the LIGO and TAMA detectors on the rate of gravitational-wave bursts (2005)
Abbott, B., Abbott, R., Adhikari, R., Ageev, A., Agresti, Juri, Ajith, P., ...
Ando, M., Arai, K., Aso, Y., Beyersdorf, P. T., Hayama, K., Iida, Y., ...
Upper limits from the LIGO and TAMA detectors on the rate of gravitational-wave bursts (2005)
Abbott, B., Abbott, R., Adhikari, R., Ageev, A., Agresti, J., Ajith, P., ...
Sato, S., Miyoki, S., Telada, S., Tatsumi, D., Araya, A., Ohashi, M., ...
In order to detect the rare astrophysical events that generate gravitational wave (GW) radiation, sufficient stability is required for GW antennas to allow long-term observation. In practice, seismic...
Dynamic Stress Concentration Factor in the Strip Plate with Fillet (1997)
Nakayama, N., Ohashi, M., Sano, T., Horikoshi, S., Takeishi, H.
Dynamic and static stress concentration factors αDmax and αS generated at a fillet part are observed by photoelastic method, and the comparison between two different factors is carried out....
Dynamic Stress Concentration Factor in the Strip Plate with Fillet (1997)
Nakayama, N., Ohashi, M., Sano, T., Horikoshi, S., Takeishi, H.
Dynamic and static stress concentration factors αDmax and αS generated at a fillet part are observed by photoelastic method, and the comparison between two different factors is carried out....
Dynamic Stress Concentration Factor in the Strip Plate with Fillet (1997)
Nakayama, N., Ohashi, M., Sano, T., Horikoshi, S., Takeishi, H.
Dynamic and static stress concentration factors αDmax and αS generated at a fillet part are observed by photoelastic method, and the comparison between two different factors is carried out....
Design for the control and data-acquisition system for the TAMA 300 m laser interferometer (1996)
Kamikubota, N, Kanda, N, Mizuno, E, Ohashi, M, Takahashi, R, Yamazaki, T
A Surface Emitting Laser Amplifier for Parallel Optical Buses (1994)
Ohashi Hamasaki, M. Ohashi, H. Hamasaki, K. Kaminishi, M. Nakamura
h as gain properties, carrier injection, resonant effects, and so on, in order to decide which structure is more effective. Therefore we propose a prototype of a vertical transmission optical...
Direct observation of the decay of beauty particles into charm particles (1990)
Albanese, J P, Alpe, V, Aoki, S, Arnold, R, Baroni, Giustina, Barth, Monique, ...
A hybrid experiment to search for beauty particles (1990)
Aoki, S, Arnold, R, Baroni, Giustina, Barth, Monique, Bartley, J H, Bertrand, D, ...
Some properties of charmed particles produced in pi-.nucleus interactions (1990)
Aoki, S, Arnold, R, Baroni, Giustina, Barth, Monique, Bertrand-Coremans, G H, Bisi, V, ...
An attempt to observe directly beauty particles in nuclear emulsions (1990)
Albanese, J P, Allasia, D, Armenise, N, Arnold, R, Baroni, Giustina, Barth, Monique, ...
MAGNETIC TRANSITIONS IN CrAs1-xSbx (x ≥ 0.6) (1988)
Ohashi, M., Suzuki, T., Ido, H., Yamaguchi, Y.
Four magnetic phases were found by neutron diffraction measurements in CrAs0.4Sb0.6. The low temperature phase is the CrSb type antiferromagnet with the magnetic moment of 2.06±0.07 µB / Cr being...
MAGNETIC TRANSITIONS IN CrAs1-xSbx (x ≥ 0.6) (1988)
Ohashi, M., Suzuki, T., Ido, H., Yamaguchi, Y.
Four magnetic phases were found by neutron diffraction measurements in CrAs0.4Sb0.6. The low temperature phase is the CrSb type antiferromagnet with the magnetic moment of 2.06±0.07 µB / Cr being...
MAGNETIC TRANSITIONS IN CrAs1-xSbx (x ≥ 0.6) (1988)
Ohashi, M., Suzuki, T., Ido, H., Yamaguchi, Y.
Four magnetic phases were found by neutron diffraction measurements in CrAs0.4Sb0.6. The low temperature phase is the CrSb type antiferromagnet with the magnetic moment of 2.06±0.07 µB / Cr being...
MAGNETIC PROPERTIES OF DyAu2 AND DyAg2 (1971)
Miura, S., Kaneko, T., Ohashi, M., Kamigaki, K.
The magnetization of compounds DyAu2 and DyAg2 was measured at temperatures between 4.2° to 300 °K and under the magnetic field up to 100 kOe. Both compounds were found to be antiferromagnetic. In...
MAGNETIC PROPERTIES OF DyAu2 AND DyAg2 (1971)
Miura, S., Kaneko, T., Ohashi, M., Kamigaki, K.
The magnetization of compounds DyAu2 and DyAg2 was measured at temperatures between 4.2° to 300 °K and under the magnetic field up to 100 kOe. Both compounds were found to be antiferromagnetic. In...
MAGNETIC PROPERTIES OF DyAu2 AND DyAg2 (1971)
Miura, S., Kaneko, T., Ohashi, M., Kamigaki, K.
The magnetization of compounds DyAu2 and DyAg2 was measured at temperatures between 4.2° to 300 °K and under the magnetic field up to 100 kOe. Both compounds were found to be antiferromagnetic. In...
Etoh, S., Ohashi, M., Baba, A., Iwata, H.
1. The effects of a novel anti-asthmatic drug, 3-isobutyryl-2-isopropylpyrazolo [1,5-a]pyridine (ibudilast, KC-404) on leukotriene D4 (LTD4)-induced formation of inositol phosphates were studied in...
Clinical features of anti-chromo antibodies associated with anti-centromere antibodies
IWAI, T, MURO, Y, SUGIMOTO, K, MATSUMOTO, Y, OHASHI, M
Anti-chromo antibodies (AChA) are autoantibodies accompanying anti-centromere antibodies (ACA). We determined the frequency and clinical significance of AChA in autoimmune rheumatic diseases. Serum...
貫, 文三郞, 大橋, 正, 和田, 國三郞, Nuki, B., Ohashi, M., Wada, K.
Verf. haben den Blutdruck des normalen und nicht narkotisierten Kaninchens blutig unter dem Gebrauch des Hg-Manometers an der Karotis und unblutig mittles Fukuda-Kawaguchis Verfahren an der...
Die Versuche wurden am normalen Kaninchen ausgefuhrt. Der Blutdruck wurde mittels Fukuda-Kawaguchis Verfahren an der Ohrarterie unblutig und durch Hg-Manometer an der Karotis blutig bestimmt. Um die...
Ohashi, M, Yoshida, K, Kushida, M, Miura, Y, Ohnami, S, Ikarashi, Y, ...
We previously demonstrated a characteristically high sensitivity of pancreatic cancer cells to interferon alpha (IFN-α) gene transfer, which induced a more prominent growth suppression and cell...