Fig. 19.
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Relation between stellar mass and ξion for the sample of EELGs and control sample (same as in Fig. 16). The gray shaded region is the canonical ξion value given by a simple stellar population at constant SFR over 100 Myr (Robertson et al. 2013), assuming an escape fraction of 0.20. The horizontal dashed lines are the canonical ξion values for an escape fraction of 0.10 and 0.05, respectively.
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