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Fig. 4.

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Star formation main sequence relation for MgII absorber host galaxies. The symbols are colour-coded with a specific SFR. The shaded and hatched regions indicate the 1σ confidence interval. Additionally, the dotted line represents the SFR threshold for wind launching from Murray et al. (2011). Top panel: SFR of Mg II galaxies normalized by the main sequence star-forming galaxy at the respective redshift.

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