Fig. 4.

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NFW+SIS fits (black line) to the cross-correlation data (black points) for bins 1 to 5 (from left to right, top to bottom) and the general case (bottom right). The corresponding SIS (blue lines) and NFW (green lines) fits are also separately shown. As discussed in more detail in Sects. 5.1.1 and 5.3, the best fits are always below the data for angular separations of between 5 and 10 arcsec and there is a potential lack of power at ∼10 and ∼25 arcsec. Grey points are considered outliers and are not taken into account for the analysis. The dashed lines for bin 5 indicates that the values were chosen by hand in order to produce a reasonable fit because the fitting algorithm does not converge (see text for more details).
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