  3C 111 is an X-ray bright broad-line radio galaxy which is classified as a
Fanaroff-Riley type II source with a double-lobe/single jet morphology, and
reported superluminal motion. It is a well-known X-ray source, and was observed
by every major X-ray observatory since HEAO-1. In this paper we present the
results of the RXTE and INTEGRAL data analysis and compare them with the
results of the previous observations.
