Fig. 11.
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Comparison of the AMR derived in this work with the one provided by Graczyk et al. (2018). Metallicity values obtained from spectroscopy (blue) and isochrones (red) from Graczyk et al. (2018), and this work (black and open squares; open circles). Green points in the zoom panel mark average metallicites of star clusters from non-bar regions calculated in age bins of 0.3 Gyr in the age range between 0.6 to 2 Gyr.
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