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Fig. 12


Probability contours in the fm,0 vs. m plane as a function of the B-band luminosity selection (Table 4). The contours enclose 68.2%, 95.4% and 99.7% of the probability. The crosses mark the most probable values of the parameters, with the larger cross for the more luminous galaxies. The dashed line is from the Eq. (25) fit to the data, fm,0 = 2.84 − m. (Colour version online.)

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