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Influence of Gravitational Microlensing on X‐Ray Radiation from Accretion Disks of Active Galaxies

Gravitational microlensing is a very useful tool for investigating the innermost part of lensed quasars, especially for studying a relativistic accretion disk around a massive black hole (BH) that is supposed to exist in a quasar’s center. Here we present a short overview of our recent investigations in this field.