A Study of the Correlation between the Amplification of the Fe Kα Line and the X‐Ray Continuum of Quasars due to Microlensing
Luka Č. Popović(Chinese Academy of Sciences), G. Chartas, C. Abajas(Instituto de Astrofísica de Canarias), E. Mediavilla(Instituto de Astrofísica de Canarias), J. A. Muñoz(Universitat de València), P. Jovanović(Isaac Newton Institute), A. F. Zakharov(Astro Space Center)
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