Fig. 13
Mg b map of FCC 167 with the r-band isophotes (black lines) and B-band isophote (grey line) shown in Fig. 4. The orange and red circles indicate the location of two selected apertures where the Hβ, Mg b, Fe5270, Fe5335, and Fe5406 line-strength indices were measured and fitted in order to constrain the stellar population properties, as shown in Fig. 14.
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