Modeling uncertainties in X-ray reflection spectroscopy measurements I: Impact of higher order disk images
arXiv:1910.12494 · doi:10.1103/PhysRevD.101.043010
Abstract
There are many simplifications in current relativistic reflection models and this introduces systematic uncertainties in the measurement of the properties of the source. In this paper, we study the impact of the radiation crossing the equatorial plane between the black hole and the inner edge of the accretion disk; that is, the radiation produced by the other side of the disk or circling the black hole one or more times (higher order disk images). For slow-rotating black holes with a larger plunging region, the effect is not very sensitive to the exact inclination angle of the disk. For fast-rotating black holes with a smaller plunging region, the effect is very weak for low inclination angles and becomes more important as the angle increases. We simulate some observations without and with higher order disk images and fit the data with the reflection model RELXILL_NK to check its capability of recovering the correct input parameters. Our results suggest that the effect of higher order disk images can be safely ignored for observations with present and near future X-ray missions, even for tests of the Kerr hypothesis.
9 pages, 5 figures. v2: refereed version
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- Impact of the reflection model on the estimate of the properties of accreting black holes
- Testing relativistic reflection models with GRMHD simulations of accreting black holes
- Testing the Keplerian disk hypothesis using X-ray reflection spectroscopy
- Impact of the returning radiation in current tests of the Kerr black hole hypothesis using X-ray reflection spectroscopy
- Exploring higher order images with Fe K_α-lines from relativistic disks: black hole spin determination and bias
- Impact of ionization and electron density gradients in X-ray reflection spectroscopy measurements
- Impact of the returning radiation on X-ray reflection spectroscopy measurements: the case of Galactic black holes
- Measuring black hole spins with x-ray reflection spectroscopy: A GRMHD outlook
- Tests of General Relativity using black hole X-ray data