Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.0714f&link_type=abstract
American Astronomical Society, HEAD meeting #9, #7.14; Bulletin of the American Astronomical Society, Vol. 38, p.351
Astronomy and Astrophysics
Astronomy
Scientific paper
Suzaku observed several Seyfert galaxies and BLAZARs in the PV phase in the energy band 0.3-600 keV with a combination of the X-ray Imaging Spectrometer (XIS) and the Hard X-ray Detector (HXD). Hard X-ray continuum above 10 keV and clear iron-K line were detected with good S/N. Accurate measurement of the continuum shape in the broad X-ray band enables us to constrain the broard iron line and reflection component. Short-term time variability was detected from most objects,and thus we can strongly consrain the constant reflection component. Accurate energy scale of the XIS enables us to mesaure the center energy of iron-K line to give the constraint of the ionization degrees and Doppler shift, and high S/N of the XIS spectra help us to detect weak iron-K line features such as absorption line and Kbeta line. This talk will review the first results of Suzaku AGN observations.
Fukazawa Yasushi
Suzaku Team
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