Left-hand panel: whisker plot showing the average galaxy ellipticity as a function of field position for the CFHTLenS fail fields. Middle/right-hand panel: the correlation function with and without recalibration. The middle row shows the weighted mean of and its 68% confidence intervals, determined using all radial bins up to the one of interest. The bottom row shows the p-values of the null hypothesis, with the solid black (red-dashed) line for (). The remaining trends are worse than those observed in the fields that passed the Heymans et al. (2012) star-galaxy cross-correlation selection (shown in Fig. 3; note the different scaling of the y-axis).