Fig. 10
Comparison between Spitzer/IRAC 3.6 μm-detected (red; brighter than m3.6 ~ 25 mag) and IRAC-undetected (blue; fainter than m3.6 ~ 25 mag) galaxies as function of stellar mass and SFR for SFGN, SFGL, and LAEs. The fraction of galaxies detected/un-detected in IRAC are shown in the legend. The solid curve is the KDE of the distribution. The statistical significance based on the KS test is shown to confirm the observed correlation.
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