Testing the accuracy of reflection-based supermassive black hole spin measurements in AGN

Author: Kammoun E. S.   Nardini E.   Risaliti G.  

Publisher: Edp Sciences

E-ISSN: 1432-0746|614|issue|A44-A44

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.614, Iss.issue, 2018-06, pp. : A44-A44

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

Previous Menu Next

Abstract

Context. X-ray reflection is a very powerful method to assess the spin of supermassive black holes (SMBHs) in active galactic nuclei (AGN), yet this technique is not universally accepted. Indeed, complex reprocessing (absorption, scattering) of the intrinsic spectra along the line of sight can mimic the relativistic effects on which the spin measure is based.