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We report multiband observations of the Optical Transient (OT) associatedwith GRB000301c carried out between 2--4 March 2000 using the 2.34-m VainuBappu Telescope (VBT) at Kavalur, India. When combined with other reporteddata, the initial decline in the R-band magnitude with log ($t-t_0$), the timesince the burst is fit with a slope $\alpha_{1}$ = -0.70 $\pm$ 0.07 whichsteepens after about 6.0 days to a slope of $\alpha_{2}$ = -2.44 $\pm$ 0.29.This change in slope does not occur smoothly but there is an indication for abimodal distribution. The available measurements of the evolution of (B--R)color do not show any discernible evolution in the first 12 days.Comment: 14 pages, 2 postscript figures, Accepted for Publication in ApJ  Letter

Early Observations of the Afterglow of GRB 000301[CLC]c[/CLC]