Moscow, Moscow, Russian Federation
In terms of program execution on finding and selecting candidates for dual supermassive black holes (DSMBHs) collected data long-term multi-frequency monitoring of active galactic nuclei (AGNs) from the databases of the Crimean Astrophysical Observatory and other world databases. Methods for determining the harmonic components in the data series of multi-frequency monitoring, obtaining cross-correlation functions, and determining the parameters of DSMBHs have been developed. The efficiency of the proposed methods, which will be used to determine the power of the GW coming from the selected DSMCHD, is shown on the example of the AGN AO 0235+164.
gravitational waves, AGN, black holes, radio emission
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