Fig. A.1.
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Concentration distributions at z = 0.5 for the three cosmologies. Thick solid lines: host haloes; thin solid lines: subhaloes. Top row: 8.2 < log M/M⊙ < 9; bottom row: 9 < log M/M⊙ < 10. Host–subhost slopes are nearly parallel in every model; CDM displays the smallest separation albeit potentially suffering the greater fragility of its low concentration objects.
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