BVR_cI_c quasi-bolometric light curve of SN 2012aa and other stripped-envelope CCSNe and SLSNe along with the luminous event SN 2010jl. The long dashed vertical line shows the epoch of V-band maximum light. The K-correction and cosmological time dilation effects have been taken into account. For the first two data points, we have only CRTS V-band data, while for the last four points there is incomplete coverage/detection in some bands. For these six epochs we have calculated the BVR_cI_c quasi-bolometric light curves after measuring the temporal evolution of (M_BVRcIc−M_V) as shown in the inset.