http://arxiv.org/abs/1904.08027
We continue exploring the constraining capabilities of X-ray reflection spectroscopy to test the Kerr-nature of astrophysical black holes and we present the results of our analysis of two NuSTAR observations of Cygnus X-1 in the soft state. We find that the final measurement can strongly depend on the assumption of the intensity profile. We conclude that Cygnus X-1 is not suitable for tests of general relativity using X-ray reflection spectroscopy and we discuss the desired properties of a source to be a good candidate for our studies.
H. Liu, A. Abdikamalov, D. Ayzenberg, et. al.
Thu, 18 Apr 19
36/75
Comments: 15 pages, 8 figures
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