Same as Fig. 1, but for filtered initial power spectrum. The halos here are the same as in Fig. 1, except that ﹩r_{f}=0.1﹩ Mpc has been applied to ﹩P( k) ﹩. The masses of the three halos are similar to those of the corresponding halos in Fig. 1. For comparison, we show the three halos from Fig. 1 as thin lines in the top left panel; the NFW profile has been omitted in this panel. See § 4.6 for details.