A semi-analytic galaxy formation model predicts that the star formation rate surface density main sequence peaks in slope near redshift 3 and flattens by today, with massive galaxies driving the change.
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Evolution of the star formation rate surface density main sequence. Insights from a semi-analytic simulation since $z = 12$
A semi-analytic galaxy formation model predicts that the star formation rate surface density main sequence peaks in slope near redshift 3 and flattens by today, with massive galaxies driving the change.