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