Magnitude differences between total model magnitude u and petrosian magnitude u


Note that the galaxies shown here have an uncertainty in the petrosian magnitude less than 1 mag. The deviation of the high D4000 galaxies at higher redshifts is likely due to the asinh magnitude system.


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

Kcorrections u 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 u as a function of (ur) (left) and D_{n}4000 (right)

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

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

