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arXiv · 1611.06909

The Future of X-ray Reverberation from AGN

A. C. Fabian·W. N. Alston·E. M. Cackett·E. Kara·P. Uttley·D. R. Wilkins
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Abstract

XMM-Newton is capable of making a transformational advance in our understanding of how luminous accreting black holes work, by dedicating about 10 per cent of future observing time to long observations, of order Megaseconds, to X-ray variable Active Galactic Nuclei (AGN) research. This would enable reverberation studies, already a commonplace feature of AGN, to proceed to the next level and follow the behaviour of the powerful dynamic corona. Such a dedicated legacy programme can only be carried out with XMM-Newton.

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A. C. Fabian, W. N. Alston, E. M. Cackett, E. Kara, P. Uttley, D. R. Wilkins. 2016-11-21. The Future of X-ray Reverberation from AGN. https://doi.org/10.1002/asna.201713341

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