Is the anti-correlation between the X-ray variability amplitude and black hole mass of AGNs intrinsic?
Yuan Liu, Shuang Nan Zhang

TL;DR
This study investigates whether the observed anti-correlation between X-ray variability amplitude and black hole mass in AGNs is intrinsic, finding that the correlation with luminosity may be the true underlying relationship.
Contribution
The paper clarifies that the intrinsic correlation of X-ray variability with black hole mass is uncertain, emphasizing the importance of sample selection and measurement methods.
Findings
The apparent correlation between variability and black hole mass is influenced by sample selection.
The intrinsic correlation is more likely with X-ray luminosity rather than black hole mass.
Sample analysis shows the anti-correlation with black hole mass may be an artifact.
Abstract
Aims. Both the black hole mass and the X-ray luminosity of AGNs have been found to be anti-correlated with the normalized excess variance () of the X-ray light curves. We investigate which correlation with is the intrinsic one. Methods. We divide a full sample of 33 AGNs (O' Neill et al. 2005) into two sub-samples. The black hole masses of 17 objects in sub-sample 1 were determined by the reverberation mapping or the stellar velocity dispersion. The black hole masses of the remaining 16 objects were estimated from the relationship between broad line region radius and optical luminosity (sub-sample 2). Then partial correlation analysis, ordinary least squares regression and K-S tests are performed on the full sample and the sub-samples, respectively. Results. We find that seems to be intrinsically correlated with the…
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