Abstract
Data of six-year observations of very high energy (E > 1011 eV) gamma-ray flux from the active galactic nucleus Mk 501 obtained using the ground-based GT-48 telescope are analyzed and compared with the 2–10 keV X-ray data obtained using the ASM instrument onboard the RXTE satellite. A positive correlation between the average annual X-and gamma-ray fluxes is demonstrated.
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