Results of using the method of successive frequency synthesis on RT-22 at 18–26 GHz

Abstract

The results of VLBI observations between the RT-22 (Simeiz) and RT-70 (Yevpatoriya) using the method of successive frequency synthesis at 18-26 GHz within the framework of “Radioastron” project are presented. The cross-correlation functions for five active galactic nuclei (BL Lac, 2145+067, 3C454.3, 3C84, 0528+134) and two sources in water vapor line (W3OH and ORION KL) are determined.