Fig. 7.
PCA coefficients for MAGMA log(Mstar) plotted against Mbreak for the division into the two PCAs. Right panel: magnification of the left panel, showing, more effectively, that the range of Mstar coefficients as the Mbreak mass is varied. The lower values of the Mstar coefficient toward higher Mbreak results from the flattening of the MZR at high Mstar.
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