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The galaxies in a high-galactic latitude field are analysed for clustering using angular correlation analysis. Our sample is unique in that, with a total of 10h of exposure time in V, R and I distributed equally between filters, the seeing for the summed frames is $\sim0.7$ arcsec. Data of this quality allows us to measure the galaxy correlation function to very small angular separations. A preliminary analysis of the ellipticity distribution of the observed galaxies is also presented.
