New CTI Correction Method for Spaced-Row Charge Injection of the Suzaku X-Ray Imaging Spectrometer

The charge transfer inefficiency (CTI) of the X-ray CCDs aboard the Suzaku satellite (X-ray Imaging Spectrometers: XIS) has increased since the launch due to radiation damage, and the energy resolution has been degraded. To improve the CTI, we have applied a spaced-row charge injection (SCI) techniq...

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Veröffentlicht in:Publications of the Astronomical Society of Japan 2009-01, Vol.61 (sp1), p.S9-S15
Hauptverfasser: Uchiyama, Hideki, Ozawa, Midori, Matsumoto, Hironori, Tsuru, Takeshi Go, Koyama, Katsuji, Kimura, Masashi, Uchida, Hiroyuki, Nakajima, Hiroshi, Hayashida, Kiyoshi, Tsunemi, Hiroshi, Mori, Hideyuki, Bamba, Aya, Ozaki, Masanobu, Dotani, Tadayasu, Takei, Dai, Murakami, Hiroshi, Mori, Koji, Ishisaki, Yoshitaka, Kohmura, Takayoshi, Prigozhin, Gregory, Kissel, Steve, Miller, Eric D., LaMarr, Beverly, Bautz, Marshall
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Sprache:eng
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Zusammenfassung:The charge transfer inefficiency (CTI) of the X-ray CCDs aboard the Suzaku satellite (X-ray Imaging Spectrometers: XIS) has increased since the launch due to radiation damage, and the energy resolution has been degraded. To improve the CTI, we have applied a spaced-row charge injection (SCI) technique to the XIS in orbit; by injecting charges into CCD rows periodically, the CTI is actively decreased. The CTI in the SCI mode depends on the distance between a signal charge and a preceding injected row, and the pulse height shows periodic positional variations. Using in-flight data of onboard calibration sources and of the strong iron line from the Perseus cluster of galaxies, we studied the variation in detail. We developed a new method to correct the variation. By applying the new method, the energy resolution (FWHM) at 5.9 keV in 2008 March is $\sim$ 155 eV for the front-illuminated CCDs and $\sim$ 175 eV for the back-illuminated CCD.
ISSN:0004-6264
2053-051X
DOI:10.1093/pasj/61.sp1.S9