Table 1
Demonstration of the coverage of our sample.
| Luminosity (R magnitude) | Stellar mass | Color B − R | ||||||||||||
| Bins | faint | → | → | bright | low | → | → | high | blue | → | → | red | ||
|
|
||||||||||||||
| Members | 21% | 37% | 32% | 10% | 15% | 41% | 29% | 16% | 13% | 47% | 25% | 15% | ||
| Zgals | 12% | 39% | 41% | 8% | 11% | 39% | 42% | 8% | 11% | 55% | 24% | 11% | ||
| Fraction | 16% | 30% | 36% | 22% | 20% | 27% | 42% | 14% | 22% | 33% | 27% | 20% | ||
Notes. First row: percentage of spectroscopic members of MAC0416 representative of the blue cloud in the given bins in luminosity, mass, and color. Second row: selected Zgals objects for this metallicity study in the given bins in luminosity, mass, and color. Third row: the fractions of Zgals objects in different luminosity/mass/color bins with respect to the parent sample of blue cluster members (numbers shown in Fig. 1).
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