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Song Huang edited figures/cosSer_CmodMag_4/caption.md
over 9 years ago
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Replace this text Fig. 30: The same with
your caption Fig. 28. Points are color-coded with the input Sersic index. Since the input catalog is based on real galaxies, the distribution of Sersic index is not flat. Instead, it strongly skews toward the lower value. It appears that the bright models with Sersic index between 1.5-2.0 tend to have overestimated total magnitude. The bright models with either n~1 or n~4 behave in a similar way with the Exp/Dev models, which tend to have slightly underestimated total magnitude.
