  We present the results of the optical, X-ray and gamma-ray analysis of some
recent GRBs. The data were obtained by the automated P60 telescope and the
Swift telescope (UVOT, XRT and BAT). We present some example fits for the
lightcurves. The data reduction and the investigations were made by the Konkoly
Observatory HEART group (http://www.konkoly.hu/HEART/index.html).
