Magnitude differences between total model magnitude i and petrosian magnitude i

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

Kcorrections i 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 i as a function of (gi) (left) and D_{n}4000 (right)

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

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

