Fig. 1.
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Properties of the complete galaxy sample as presented in Appendix A. (a) Distribution of galaxy type; (b) SFR as a function of total mass enclosed within the radius of the star-forming disc; and (c) specific SFR (sSFR; per total mass) as a function of the optical galaxy diameter (projected apparent diameter D25). The galaxies are grouped according to the respective subsample to which they belong (Sect. 2.1).
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