Incidence of outflows as a function of host galaxy properties. The bottom panels from left to right report the detection rate as a function of stellar mass, star formation rate estimated over the last 10 Myr, and specific star formation rate. The binomial uncertainties are reported as error bars for each bin. The uncertainties on the galaxy properties are smaller than the bin sizes. The top panels illustrate the number of targets in each bin. Incidence values are not reported for bins with fewer than five targets.