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In this part we will be doing the same routine as in 1C but with Kuiper's test rather than Kolmogorov-Smirnov. This involves dividing the domain on which the two cumulated distribution functions lie and computing the maximum separation $D_{\pm}$ on each half. The statistic of interest is then $V = D_{+} + D_{-}$ and the significance level equation is slightly adjusted from that in 1C. The results from my Kuiper test and that found in \texttt{astropy} do not compare well for small $N_{numbers}$ but that is an issue with the test itself ($D_{\pm}$ are computed from samples of size $N_{numbers}/2$).