Quick Search:
Prog. Theor. Phys. Supplement No.169 (2007) pp. 282-285
Hard X-Ray Variability of AGN Observed with Suzaku
Yasushi Fukazawa,1
Mahito Sasada,1
Hirohisa Shirai,1
Hideyo Kunieda,2
Tomokazu Nakamura,2
HXD background Team and
the Suzaku Team
1Department of Physical Sciences, Hiroshima University,
Higashi-Hiroshima 739-8536, Japan
2Department of Physics, Nagoya University, Nagoya 464-8602, Japan
Abstract:
Stydy of time variable spectra is independept tool to decompose the
spectral components in the AGN (Active Galactic Nucleus); direct nuclear
emission and relfection component.
Since the difference between these two components becomes clear by
comparing the behavior below and above 10 keV, hard X-ray study of time
variability of AGNs is very important.
Here we report the initial results of studies of hard X-ray variability
of AGNs (MCG-6-30-15, MCG-5-23-16, NGC 4388, NGC 3516) observed with
Suzaku.
RMS spectra and flux-flux correlation above 10 keV is derived and discussed.
URL :
http://ptp.ipap.jp/link?PTPS/169/282/
DOI : 10.1143/PTPS.169.282
References:
-
S. Deluit and T. J.-L. Courvoisier, Astron. Astrophys. 399 (2003), 77[CrossRef].
- Y. Fukazawa et al., Suzaku-Memo 2007-02 (2007),
http://www.astro.isas.jaxa.jp/suzaku/doc/suzakumemo/suzakumemo-2007-02.pdf
- A. C. Fabian and S. Vaughan, Mon. Not. R. Astron. Soc. 340 (2003), L28.
-
A. Malizia et al., Astrophys. J. 589 (2003), L17[IoP STACKS].
- G. Miniutti et al., Publ. Astron. Soc. Jpn. 59 (2007), S315.
- T. Mizuno et al., Suzaku-Memo 2006-42 (2006),
http://www.astro.isas.jaxa.jp/suzaku/doc/suzakumemo/suzakumemo-2006-42.pdf
- T. Nakamura et al., Proc. Suzaku conference, Kyoto (2007).
- J. N. Reeves et al., Publ. Astron. Soc. Jpn. 59 (2007), S301.
- G. Risaliti, Astron. Astrophys. 386 (2002), 379.
- H. Takahashi et al., Suzaku-Memo 2006-43 (2007),
http://www.astro.isas.jaxa.jp/suzaku/doc/suzakumemo/suzakumemo-2006-43.pdf
-
A. A. Zdziarski et al., Astrophys. J. 438 (1995), L63[CrossRef].
