Fig. 3
Upper panel: y-axis, number of confirmed clusters; x-axis, number of galaxy redshifts sampling the confirmed clusters. Different colours and line styles are from different spectroscopic surveys. Bottom panel: percentage of galaxy redshifts inside the confirmed clusters coming from a given survey and for a given redshift bin. Because of multiple galaxy spectroscopic measurements, the sum of the percentages for a given redshift bin is larger than 100%.
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