Fig. B.1.
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Comparison between the stellar masses inferred by PPXF and BEAGLE. The orange line indicates the 1:1 line. The green solid line show the best-fit relation between the two mass-estimated. The dashed green lines show the 1-sigma error on the best-fit. The masses show a strong correlation, with an RMS-scatter of 0.2 dex, but an offset of 0.2 dex at the low-mass end.
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