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• These plots compute the \mu residual by computing the difference between the expected value of \mu (measured from the redshift and Planck cosmological parameters) and the measured value of \mu mu.  In all cases, errors of mean residual is determined by adding individual errors in quadrature and dividing by number of added Sn.  
• Here is a plot of the residuals on the sky, integrated over redshifts. determined by looking at residual of all Sn within 10 degrees (no redshift information considered).  The color scale denotes number of sigma away from 0.0.
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• Here is a plot of the residual in redshift, integrated over the skyvs redshift (no sky directional information considered). The top panel shows all individual Sn.  The bottom panel shows the average residual in twenty bins bins of even redshift size.