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Fig. 4


Histograms of the stellar mass (top panel), SFR (middle panel), and Δ SFR (bottom panel), where ΔSFR = log(SFR∕SFRMS), normalized for the rotation dominated galaxies compared to other types. We combine our data with SINS (Förster Schreiber et al. 2009), Livermore et al. (2015), MUSE-HDFS (Contini et al. 2016), MUSE-KMOS (Swinbank et al. 2017), KLASS (Mason et al. 2017), and KDS (Turner et al. 2017). KLASS is considered for the mass only, no SFR is available.

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