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PKS 2155-304 is a well known GeV and TeV emitter and one of the brightestblazars in the Fermi sky. We present the results of one year of data takingwith Fermi, producing the longest lightcurve on this object. Together with along duration X-ray monitoring program with RXTE, these data give a betterpicture of the emission mechanisms for PKS 2155-304 on long time scales.

Monitoring the synchrotron and Compton emission of PKS 2155-304: one year of observations with RXTE and Fermi