Top: Log sSFR as a function of stellar mass for AGN (left) and non-AGN (right). The circle points are the median value of the log sSFR in that stellar mass range. The error bars denote the bootstrap errors in each stellar mass interval. Each point has been slightly shifted along the x-axis so that the error bars are visible. Bottom left: Ratio between the log sSFR of Out-V, S, W, and all AGN host galaxies to In-V. Bottom right: Ratio between the log sSFR of Out-V, S, W, and all non-AGN host galaxies to In-V (see Section 2.4 for definitions).