Shin'ya Yamada, Hideki Uchiyama, Tadayasu Dotani, Masahiro Tsujimoto, Satoru Katsuda, Kazuo Makishima, Hiromitsu Takahashi, Hirofumi Noda, Shunsuke Torii, Soki Sakurai, Teruaki Enoto, Takayuki Yuasa, Shu Koyama, Aya Bamba
We present the result of a systematic study of pileup phenomena seen in the
X-ray Imaging Spectrometer, an X-ray CCD instrument, onboard the Suzaku
observatory. Using a data set of observed sources in a wide range of brightness
and spectral hardness, we characterized the pileup fraction, spectral
hardening, and grade migration as a function of observed count rate in a frame
per pixel. Using the pileup fraction as a measure of the degree of pileup, we
found that the relative spectral hardening (the hardness ratio normalized to
the intrinsic spectral hardness), branching ratio of split events, and that of
detached events increase monotonically as the pileup fraction increases,
despite the variety of brightness and hardness of the sample sources. We
derived the pileup fraction as a function of radius used for event extraction.
Upon practical considerations, we found that events outside of the radius with
a pileup fraction of 1% or 3% are useful for spectral analysis. We present
relevant figures, tables, and software for the convenience of users who wish to
apply our method for their data reduction of piled-up sources.
View original:
http://arxiv.org/abs/1112.1844
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