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Fig. 14


Relation between stellar mass (M) and specific SFR (sSFR) for positions A, B, and C (red points) from LSQ14mo system compared to a selection of local dwarf galaxies (z < 0.3). The contours represent the star-forming sample of Yates et al. (2012), showing the 68th, 95th, and 99.5th percentiles of the distribution. All three LSQ14mo systems have SFRs (and sSFRs) slightly higher than most galaxies of their mass.

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