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Fig. 3.

image

Number of targets per square arcminute in a KMOS OB as a function of radial distance in arcminutes from the field center. The overall target numbers are divided by 24 to show the typical target density per KMOS field. Fields 1 and 5 are the most extreme fields in terms of target density: field 1 is at the higher density limit and field 5 is at the lower density limit and also has fewer observed stars because one subset was not successfully observed. The downward-facing arrows mark bins in which no star was observed.

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