Fig. 6.
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Color grid. Black lines indicate the FASTAR fully sampled predictions for the same age and metallicity ranges as in Fig. 4. Green, red, and blue contours show the distributions of (g − r) and Mgb values for a 10 Gyr and solar metallicity population with a variable number of stars (Nstars = 105.5, 103.5, and 102.5, respectively).
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