Figure 3.
Distribution of the source-frame flare duration T/(1 + z) versus the time asymmetry parameter k. The shape and colour of each point indicate the host blazar, and the point size is proportional to the logarithm of peak flux Fpeak.
Distribution of the source-frame flare duration T/(1 + z) versus the time asymmetry parameter k. The shape and colour of each point indicate the host blazar, and the point size is proportional to the logarithm of peak flux Fpeak.
