Band-pass corrections derived from two red galaxy templates (dotted dashed red lines; see Fig. 7 for details). The p_LRG derived from the DIRBE/IRAS dust map are shown by the black dots with the plotted values corresponding to bpc_LRG = p_B5/p_LRG where the optimal p_B5 = 0.0225. For a direct comparison of this analysis with the Schlegel calibration work, the band-pass corrections derived from local (z < 0.05) elliptical galaxy templates from the COSMOS template library (seven templates; see Fig. 3) are reproduced here (red solid lines). The average band-pass correction derived from these models is bpc_SFD98 = 0.927.