SFR-M_* diagram for all the sources in our sample (teal circles). Gray contours show the distribution of nearby galaxies from Leroy et al. (2019). Here, contours increase in steps of 20%, with the lowest one including 90% of the local sample. The pink solid line represents the best-fit relation (by Leroy et al. 2019) to local SFGs (selected in the log(M_*/M_⊙) = 9.5 − 11 range), probing the local star-forming main sequence. We also show the extrapolation of such a relation to the lower stellar mass regime covered by our galaxy sample (pink dotted line). Pink dashed lines are the 3σ scatter associated with the relation. Circles highlighted in white represent galaxies from our sample with individual outflow detections.