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2009

Measuring the Spin of GRS 1915+105 with Relativistic Disk Reflection

Blum, J. L., Miller, J. M., Fabian, A. C. et al.

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GRS 1915+105 harbors one of the most massive known stellar black holes in the Galaxy.

In May 2007, we observed GRS 1915+105 for 117 ksec in the low/hard state using Suzaku.
We collected and analyzed the data with the HXD/PIN and XIS cameras spanning the energy range from 2.3-55 keV.
Fits to the spectra with simple models reveal strong disk reflection through an Fe K emission line and a Compton back-scattering hump.

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