Fig. 6.
Comparison of the observed mass-to-light ratio versus (g − i) colour in ALHAMBRA with MLCRs from the literature. The contours are the same as in Fig. 2. The dashed green line is from the observational study of T11. The other black lines are from theoretical expectations: Zibetti et al. (2009, dotted) and Roediger & Courteau (2015, solid). All the MLCRs have been scaled to a Chabrier (2003) IMF and referred to BC03 models.
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