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To explore the correlation in the GeV band (i.e. the inverse-Comptoncomponent) with the optical band (i.e. the synchrotron component) of blazarsthat are bright in high energies, the light curves of a number of blazarsmonitored with the Fermi Gamma-ray Space Telescope (FGST), were compared to thecorresponding light curves recorded with the Automatic Telescope for OpticalMonitoring (ATOM). The results are presented.

Correlation between the synchrotron and the inverse-Compton components, in the longterm light curve of GeV blazars