  We report $R_cI_c$ light curves of 2 novae in the M31 galaxy which were
detected in the four year Nainital Microlensing Survey. One of these novae has
been tracked from the initial increase in flux while other has been observed
during its descending phase of brightness. The photometry of the first nova
during the outburst phase suggests its peak $R_c$ magnitude to be about 17.2
mag with a flux decline rate of 0.11 mag day$^{-1}$ which indicates that it was
a fast nova. A month after its outburst, it shows reddening followed by a
plateau in $I_c$ flux. The second nova exhibits a bump in $R_c$ and $I_c$,
possibly about three weeks after the outburst.
