A stellar census in globular clusters with MUSE - Extending the CaT-metallicity relation below the horizontal branch and applying it to multiple populations

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Fig. 1.

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Upper panel: chromosome map of NGC 1851 with the three identified populations marked in different colors (see text in Sect. 3 for explanation). The same color-coding is used for the color-magnitude diagram in the lower panel, where the populations can also easily be distinguished.

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