most citedXSPEC model for testing the Kerr black hole hypothesis using the continuum-fitting method

31 citations · 86 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.HE202017 cited

Impact of the reflection model on the estimate of the properties of accreting black holes

Ashutosh Tripathi, Honghui Liu, Cosimo Bambi

Relativistic reflection features in the X-ray spectra of black hole binaries and AGNs originate from illumination of the inner part of the accretion disk by a hot corona. In the pr…

gr-qc20209 cited

Reflection features in the X-ray spectrum of Fairall 9 and implications for tests of general relativity

Honghui Liu, Haiyang Wang, Askar B. Abdikamalov +2

X-ray reflection spectroscopy is potentially a powerful tool to probe the spacetime geometry around astrophysical black holes and test general relativity in the strong field regime…

gr-qc2020

Testing general relativity with the stellar-mass black hole in LMC X-1 using the continuum-fitting method

Ashutosh Tripathi, Menglei Zhou, Askar B. Abdikamalov +6

The iron line and the continuum-fitting methods are currently the two leading techniques for measuring black hole spins with electromagnetic radiation. They can be naturally extend…

gr-qc201929 cited

Testing the Kerr hypothesis using X-ray reflection spectroscopy with NuSTAR data of Cygnus X-1 in the soft state

Honghui Liu, Askar B. Abdikamalov, Dimitry Ayzenberg +4

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…

gr-qc201931 cited

XSPEC model for testing the Kerr black hole hypothesis using the continuum-fitting method

Menglei Zhou, Askar B. Abdikamalov, Dimitry Ayzenberg +3

We present NKBB, an XSPEC model for the thermal spectrum of thin accretion disks in parametric black hole spacetimes. We employ the Novikov-Thorne model for the description of the…