Magnitude differences between total model magnitude i and petrosian magnitude i
![Difference between magnitude from model fits and SDSS petroMag](chicomp.028.png)
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K-corrections i as a function of (g-i) for SHELS using the model fits (left) and the analytic prescription of CMZ10 (right)
![K-corrections from SHELS as function of color](chicomp.029.png) ![K-corrections from CMZ10 as function of color](chicomp.030.png)
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K-corrections i as a function of Dn4000 for SHELS using the model fits
![K-corrections SHELS from models](chicomp.031.png) ![K-corrections SHELS from models with predicted k-corrections overlaid](appendixb.046.png)
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Comparison of the k-corrections derived from our models and the prescription given by CMZ10 for i as a function of (g-i) (left) and Dn4000 (right)
![Difference k-corrections SHELS and CMZ10 as function of color](chicomp.032.png) ![Difference k-corrections SHELS and CMZ10 as function of D4000](chicomp.033.png)
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Assessment of the accuracy of the analytic approximations for the k-corrections for i as function of (g-i) (left) and Dn4000 (right)
![Residuals as function of color and redshift](chicomp.034.png) ![Residuals as function of D4000 and redshift](chicomp.035.png)
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(g-i) as a function of Dn4000 color coded by redshift
![Color vs D4000](chicomp.036.png)
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