Massive galaxy clusters contain 2000-7000 faint dwarfs with stellar mass above 100 solar masses whose overall distribution follows the dark matter profile, but detection thresholds make the visible population appear more extended by excluding centrally stripped objects.
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The abundance and radial distribution of faint and ultra-faint dwarfs in galaxy clusters
Massive galaxy clusters contain 2000-7000 faint dwarfs with stellar mass above 100 solar masses whose overall distribution follows the dark matter profile, but detection thresholds make the visible population appear more extended by excluding centrally stripped objects.