Metallicity of the globular cluster NGC 6388 based on high-resolution spectra of more than 160 giant stars

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Fig. 12.

m_F336W − m_F814W versusm_F336W for NGC 6388 (selecting only stars with a valid sharpness parameter (for details, see text)). Stars in our spectroscopic sample are indicated by larger black dots, while stars selected on the redder part of the RGB are shown as red circles.

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