Fig. 7.
Top: comparison of the metallicity, dust attenuation, age, and δ derived from the Withline and Noline runs. Bottom: comparison of the metallicity, dust attenuation, age, and δ derived from the Withline and Nonebular runs. Orange dots are galaxies in Sample-A. Blue circles are galaxies in Sample-B. Sample-A has a better data quality than Sample-B, as defined in Sect. 3.3. The dotted line are the 1:1 line.
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