YONETOKU Daisuke
,
TANABE Sachiko
,
MURAKAMI Toshio
,
EMURA Naomi
,
AOYAMA Yuka
,
KIDAMURA Takashi
,
KODAIRA Hironobu
,
KODAMA Yoshiki
,
KOZAKA Ryota
,
NASHIMOTO Takuro
,
OKUNO Shinya
,
YOKOTA Satoshi
,
YOSHINARI Satoru
,
ABE Keiichi
,
ONDA Kaori
,
TASHIRO Makoto S.
,
URATA Yuji
,
NAKAGAWA Yujin E.
,
SUGITA Satoshi
,
YAMAOKA Kazutaka
,
YOSHIDA Atsumasa
,
ISHIMURA Takuto
,
KAWAI Nobuyuki
,
SHIMOKAWABE Takashi
,
KINUGASA Kenzo
,
KOHMURA Takayoshi
,
KUBOTA Kaori
,
SUGIYASU Kei
,
UEDA Yoshihiro
,
MASUI Kensuke
,
NAKAZAWA Kazuhiro
,
TAKAHASHI Tadayuki
,
MAENO Shouta
,
SONODA Eri
,
YAMAUCHI Makoto
,
KUWAHARA Makoto
,
TAMAGAWA Toru
,
MATSUURA Daisuke
,
SUZUKI Motoko
,
BARTHELMY Scott
,
GEHRELS Neil
,
NOUSEK John
… arXiv:0708.3968v1 [astro-ph] http://arxiv.org/abs/0708.3968We observed an X-ray afterglow of GRB 060904A with the Swift and Suzaku satellites. … After that, typical afterglow spectra with F = 2.0 have been continuously and preciously monitored by both Swift/XRT and Suzaku/XIS. … We could successfully trace the temporal history of two characteristic break energies that have a time dependence of (proportional to t(-3)-t(-4), while the following afterglow spectra are quite stable. …
Publications of the Astronomical Society of Japan 60(1), 351, 2008-02-20
IR
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