Magnitude differences between total model magnitude r and petrosian magnitude r
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K-corrections r as a function of (g-r) for SHELS using the model fits (left) and the analytic prescription of CMZ10 (right)
 
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K-corrections r as a function of Dn4000 for SHELS using the model fits
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Comparison of the k-corrections derived from our models and the prescription given by CMZ10 for r as a function of (g-r) (left) and Dn4000 (right)
 
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Assessment of the accuracy of the analytic approximations for the k-corrections for r as function of (g-r) (left) and Dn4000 (right)
 
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(g-r) as a function of Dn4000 color coded by redshift
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