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We present a correlation between two intrinsic parameters of GRB opticalafterglows. These are the isotropic luminosity at the maximum of the lightcurve (Lpeak) and the time-integrated isotropic energy (Eiso) radiated afterthe observed maximum. We test the correlation between the logarithms of (Eiso)and (Lpeak) and finally we value the effect of the different samples of GRBs inaccording with the first optical observation reduced to proper time.Comment: To be published in the proceedings of the conference "SWIFT and GRBs:  Unveiling the Relativistic Universe", Venice, June 5-9, 200

GRBs with optical afterglow and known redshift: a statistical study