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Fig. 4

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Illustration of preselected SExtractor detections considered as possible members (red circles) and artifacts/background sources (yellow circles). Left: many objects are rejected since they are detected in the refraction halo of a foreground star and in the shadows along instrument suspension. Right: a field not affected by artifacts where detections close to spikes of foreground stars were rejected. Only a few objects remain and are considered as possible group members (red circles).

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