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Fig. 15.

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Distribution of the error in zbest, Δz, for the galaxies in the spectroscopic sample. The tails of the distribution at |Δz| > 0.03 are truncated to emphasise the shape of the central peak. Only sources with odds > 0.61 are shown. Each colour represents the distribution for an individual pointing. The black histogram represents the combined distribution for all four pointings.

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