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• W3103046941 abstract "We report on the results of spectral fits made to data obtained from a 168 ksec Suzaku observation of the Seyfert-1 galaxy Fairall 9. The source is clearly detected out to 30 keV. The observed spectrum is fairly simple; it is well-described by a power-law with a soft excess and disk reflection. A broad iron line is detected, and easily separated from distinct narrow components owing to the resolution of the CCDs in the X-ray Imaging Spectrometer (XIS). The broad line is revealed to be asymmetric, consistent with a disk origin. We fit the XIS and Hard X-ray Detector (HXD) spectra with relativistically-blurred disk reflection models. With the assumption that the inner disk extends to the innermost stable circular orbit, the best-fit model implies a black hole spin parameter of a = 0.60(7) and excludes extremal values at a high level of confidence. We discuss this result in the context of Seyfert observations and models of the cosmic distribution of black hole spin." @default.
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• W3103046941 date "2009-09-17" @default.
• W3103046941 modified "2023-10-14" @default.
• W3103046941 title "CONSTRAINING THE SPIN OF THE BLACK HOLE IN FAIRALL 9 WITH<i>SUZAKU</i>" @default.
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• W3103046941 doi "https://doi.org/10.1088/0004-637x/703/2/2171" @default.
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