Fig. C.1.
Two-dimensional view of the star formation history in FCC 170. Stellar populations are mapped according to their age. Each map corresponds to a specific age bin: 11.5–14 Gyr in the top panel, 9–11 Gyr in the middle panel and 0–8.5 Gyr in the bottom panel. The color scale shows the mass density corresponding to the populations in the specific age bin. The total mass in the age bin is indicated on bottom-left of each map. The position of the two MUSE pointings is plotted in gray. A scale bar on bottom-right of each map indicates the correspondence with physical units.
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