E. Miyata

Publication List Details

Period

1998 - 2008

Number

22

Co-Authors

Suzaku Observations of Tycho's Supernova Remnant (2008)

Tamagawa, T., Hayato, A., Nakamura, S., Terada, Y., Bamba, A., Hiraga, J. S., ...

Tycho's supernova remnant was observed by the XIS and HXD instruments onboard the Suzaku satellite on 2006 June 26-29 for 92 ks. The spectrum up to 30 keV was well fitted with a two-component model,...

Asymmetric Ejecta Distribution of the Cygnus Loop revealed with Suzaku (2008)

Katsuda, S., Tsunemi, H., Miyata, E., Mori, K., Namiki, M., Nemes, N., ...

We observed a linearly sliced area of the Cygnus Loop from the north-east to the south-west with Suzaku in seven pointings. After dividing the entire fields of view (FOV) into 119 cells, we extracted...

Abundance Inhomogeneity in the Northeastern Rim of the Cygnus Loop Revealed by Suzaku Observatory (2008)

Katsuda, S., Tsunemi, H., Uchida, H., Miyata, E., Nemes, N., Miller, E. D., ...

We present the results of a spatially resolved spectral analysis from four Suzaku observations covering the northeastern rim of the Cygnus Loop. A two-kT_e non-ionization equilibrium (NEI) model...

Wide band X-ray Imager (WXI) and Soft Gamma-ray Detector (SGD) for the NeXT Mission (2004)

Takahashi, T., Awaki, A., Dotani, T., Fukazawa, Y., Hayashida, K., Kamae, T., ...

The NeXT mission has been proposed to study high-energy non-thermal phenomena in the universe. The high-energy response of the super mirror will enable us to perform the first sensitive imaging...

Novel Photon-Counting Detector for 0.1-100 keV X-ray Imaging Possessing High Spatial Resolution (2003)

Miyata, E., Tamura, K.

We report on a new photon-counting detector possessing unprecedented spatial resolution, moderate spectral resolution and high background-rejection capability for 0.1-100 keV X-rays. It consists of...

Proton Irradiation Experiment for the X-ray Charge-Coupled Devices of the Monitor of All-sky X-ray Image mission onboard the International Space Station: I. Experimental Setup and Measurement of the Charge Transfer Inefficiency (2002)

Miyata, E., Kamazuka, T., Kouno, H., Mihara, M. Fukuda M., Matsuta, K., Tsunemi, H., ...

We have investigated the radiation damage effects on a CCD to be employed in the Japanese X-ray astronomy mission including the Monitor of All-sky X-ray Image (MAXI) onboard the International Space...

Application of the Mesh Experiment for the Back-Illuminated CCD: I. Experiment and the Charge Cloud Shape (2002)

Miyata, E., Miki, M., Hiraga, J., Kouno, H., Yasui, K., Tsunemi, H., ...

We have employed a mesh experiment for back-illuminated (BI) CCDs. BI CCDs possess the same structure to those of FI CCDs. Since X-ray photons enter from the back surface of the CCD, a primary charge...

Direct X-ray Imaging of $\mu$m precision using Back-Illuminated CCD (2002)

Miyata, E., Miki, M., Tsunemi, H., Hiraga, J., Kouno, H., Miyaguchi, K.

A charge-coupled device (CCD) is a standard imager in optical region in which the image quality is limited by its pixel size. CCDs also function in X-ray region but with substantial differences in...

SSC of MAXI experiment (2001)

Sakano, M., Tomida, H., Matsuoka, M., Ueno, S., Komatsu, S., Shirasaki, Y., ...

Monitor of All-sky X-ray Image (MAXI) on the International Space Station (ISS) has two kinds of X-ray detectors: the Gas Slit Camera (GSC) and the Solid-state Slit Camera (SSC). SSC is an X-ray CCD...

Nonthermal X-Ray Emission from G266.2-1.2 (RX J0852.0-4622) (2001)

Slane, P., Hughes, J. P., Edgar, R. J., Plucinsky, P. P., Miyata, E., Aschenbach, B.

The newly discovered supernova remnant G266.2-1.2 (RX J0852.0-4622), along the line of sight to the Vela SNR, was observed with ASCA for 120 ks. We find that the X-ray spectrum is featureless, and...

Preparation of new lipases derivatives with high activity- stability in anhydrous media: adsorption on hydrophobic supports plus hydrophilization with polyethylenimine (2001)

Guisan, J. M., Sabuquillo, P., Fernandez-Lafuente, R., Fernandez-Lorente, G., Mateo, C., Halling, P. J., ...

A novel method to prepare immobilized lipases derivatives is hereby proposed. Lipases are firstly adsorbed on supports having large internal surfaces covered by hydrophobic groups (e.g. polyacrylic...

Preparation of new lipases derivatives with high activity- stability in anhydrous media: adsorption on hydrophobic supports plus hydrophilization with polyethylenimine (2001)

Guisan, J.M., Sabuquillo, P., Fernandez-Lafuente, R., Fernandez-Lorente, G., Mateo, C., Halling, P.J., ...

A novel method to prepare immobilized lipases derivatives is hereby proposed. Lipases are firstly adsorbed on supports having large internal surfaces covered by hydrophobic groups (e.g. polyacrylic...

Preparation of new lipases derivatives with high activity- stability in anhydrous media: adsorption on hydrophobic supports plus hydrophilization with polyethylenimine (2001)

Guisan, J.M., Sabuquillo, P., Fernandez-Lafuente, R., Fernandez-Lorente, G., Mateo, C., Halling, P.J., ...

A novel method to prepare immobilized lipases derivatives is hereby proposed. Lipases are firstly adsorbed on supports having large internal surfaces covered by hydrophobic groups (e.g. polyacrylic...

Subpixel Spatial Resolution of the X-Ray Charge-Coupled Device Based on the Charge Cloud Shape (2001)

Hiraga, J., Tsunemi, H., Miyata, E.

When an X-ray photon lands into a pixel (event pixel), the primary charge is mainly collected into the event pixel. If the X-ray landing position is sufficiently close to the pixel boundary, the...

Spectroscopic Study of the Vela-Shrapnel (1999)

Tsunemi, H., Miyata, E., Aschenbach, B.

Several shrapnels have been detected in the vicinity of Vela SNR by the ROSAT all-sky survey. We present here the spectral properties of shrapnel `A' observed with the ASCA satellite. A prominent...

The X-ray CCD camera of the MAXI Experiment on the ISS/JEM (1999)

Miyata, E., Tsunemi, H., Ogata, H., Akutsu, D., Yoshita, K., Hashimoto, Y., ...

MAXI, Monitor of All-sky X-ray Image, is the X-ray observatory on the Japanese experimental module (JEM) Exposed Facility (EF) on the International Space Station (ISS). MAXI is a slit scanning camera...

ASCA observation of the Cygnus Loop Supernova Remnant (1999)

Miyata, E., Tsunemi, H., Koyama, K., Ishisaki, Y.

We present here the results of the mapping observation of the Cygnus Loop with the Gas Imaging Spectrometer (GIS) onboard the ASCA observatory. The data covered the entire region of the Cygnus Loop....

Discovery of the compact X-ray source inside the Cygnus Loop (1998)

Miyata, E., Tsunemi, H., Torii, K., Hashimotodani, K., Tsuru, T. G., Koyama, K., ...

We detected an X-ray compact source inside the Cygnus Loop during the observation project of the whole Cygnus Loop with the ASCA GIS. The source intensity is 0.11 c s$^{-1}$ for GIS and 0.15 c...

Immune response to gangliosides in a case of Guillain-Barré syndrome after varicella

Yoshikawa, T., Suzuki, K., Suga, S., Miyata, E., Yamamoto, H., Hosokawa, T., ...

An 8 year old girl was admitted to hospital with the typical clinical features of Guillain-Barré syndrome (GBS) after recovering from varicella. Onset of the disease was just two weeks after the...