Suzaku observations of AGN and synergy with GLAST

Jun Kataoka*, Tad Takahashi, Greg Madejski

*この研究の対応する著者

研究成果

抄録

In next five years, dramatic progress is anticipated for the AGN studies, as we have two important missions to observe celestial sources in the high energy regime: GLAST and Suzaku. Suzaku is the 5th Japanese X-ray astronomy satellite which was successfully launched in July 2005. It carries four X-ray sensitive imaging CCD cameras (0.2-12 keV) located in the focal planes of X-ray telescope, and a non-imaging, collimated hard X-ray detector, which extends the bandpass of the observatory to include the 10-600 keV range. Simultaneous monitoring observations by the two instruments (GLAST and Suzaku) will be particularly valuable for variable radio-loud AGN, allowing the cross-correlations of time series as well as detailed modeling of the spectral evolution between the X-ray and gamma-ray energy bands. In this paper, we show early highlights from Suzaku observations of radio-loud AGNs, and discuss what we can do with GLAST in forthcoming years.

本文言語English
ホスト出版物のタイトルFirst GLAST Symposium
ページ89-91
ページ数3
DOI
出版ステータスPublished - 2007
外部発表はい
イベント1st Gamma-ray Large Area Space Telescope Symposium, GLAST - Stanford, CA, United States
継続期間: 2007 2 52007 2 8

出版物シリーズ

名前AIP Conference Proceedings
921
ISSN(印刷版)0094-243X
ISSN(電子版)1551-7616

Conference

Conference1st Gamma-ray Large Area Space Telescope Symposium, GLAST
国/地域United States
CityStanford, CA
Period07/2/507/2/8

ASJC Scopus subject areas

  • 物理学および天文学(全般)

フィンガープリント

「Suzaku observations of AGN and synergy with GLAST」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。

引用スタイル