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We present multiwavelength light curves and polarimetric data of the FlatSpectrum Radio Quasar 3C 273 over 8 years. The wavelength range of our data setextends from radio to gamma-rays. We found that the optical emission in thissource is dominated by the accretion disk during the entire time-frame ofstudy. We additionally find that in contrast with the observed behaviour inother blazars, 3C 273 does not show a correlation between the gamma-rayspectral index and the gamma-ray luminosity. Finally, we identified ananti-correlation between the 15 GHz and V-band light curves for the time-range$JD_{245} = 4860 - 5760$, which we speculate is the consequence of the innerpart of the accretion disk falling into the black hole, followed by theejection of a component into the jet.

Multiwavelength Analysis of the Variability of the Blazar 3C 273