Normalized covariance matrix (i.e., the correlation coefficient) used in this work. There is a strong anti-correlation that exists between the lensing-galaxy correlation w^Gg and the IA-galaxy correlation w^Ig (including the contamination from w^Gκgal), as we found in our previous work. The covariance of the 12 data points is calculated from Jackknife resampling with 200 regions. We note the IA information is passed from 1 < θ < 20 [arcmin] for w^Ig to 20 < θ < 300 [arcmin] for w^γκ with the scale-independent A_IA assumption.