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. 11.

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As in Fig. 8, slopes are plotted as function of metallicity, but here for the quadratic fit from Fig. 9 at three different values for V − V_HB. The blue and orange lines show the fitted relations from Fig. 8.

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