Fig. 6.
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Distribution of stars on the [Fe/H] – [Mg/Fe] chemical composition plane for galaxies in NEWCLUSTER at z = 0.8. The grey 2D histogram in the background indicates the distribution of all stars. Contours indicate stars which are members of galaxies with different stellar masses drawn by contours that contain 68.2% (solid lines) and 95.5% (dashed lines) of their distribution.
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