Comparison of different clustering measurements in the GAMA area and how they compare with the KiDS-Bright correlations measured with (blue) and without (red) 100A organised randoms. Red and blue data-points are the same in all rows, whilst grey points and shading are the angular clustering measured with uniform randoms for (top) the KiDS-Bright-GAMA cross-matched catalogue, (middle) KiDS-Bright galaxies within the GAMA window, and (bottom) KiDS-Bright galaxies within the GAMA window, and with r < 19.8. Errors are estimated with delete-one jackknifes from 31 sub-regions of KiDS-Bright or 20 sub-regions of the GAMA window. Errors on scales ϑ ≳ 180 arcmin (the approximate scale of each sub-region) are thus likely to be underestimated for the GAMA-area correlations.