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Fig. 11

image

Upper two panels: same data and relations as in Fig. 10. Here we have shifted each redshift slice to remove the effect of redshift evolution. In the left column we have applied shifts to bring the blue and green solid lines on top of the red (i.e. applied redshift corrections as reported in Karim et al. 2011), in the right we did the same but used the dashed lines. Lower panels: best fit of broken MS relations. It is seen that under both assumptions, the relation steepens towards lower stellar masses.

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