|Sal, BC/Sal, M||Cha, BC/Kro, M|
|Notes: in each aperture, the lower and upper limits of the intervals are chosen as the smallest and the largest values predicted, at 1 confidence level, by the best-fit power-law and pseudo-Jaffe models. These values are given in units of the luminous mass, that is determined by adopting a Salpeter (left) or Chabrier/Kroupa (right) IMF.|
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