Magnitude differences between total model magnitude r and petrosian magnitude r

Kcorrections r as a function of (gr) for SHELS using the model fits (left) and the analytic prescription of CMZ10 (right)

Kcorrections r as a function of D_{n}4000 for SHELS using the model fits

Comparison of the kcorrections derived from our models and the prescription given by CMZ10 for r as a function of (gr) (left) and D_{n}4000 (right)

Assessment of the accuracy of the analytic approximations for the kcorrections for r as function of (gr) (left) and D_{n}4000 (right)

(gr) as a function of D_{n}4000 color coded by redshift

