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Fig. 3.
CAMD MG vs. G − GRP of the 1387 stars of Psc-Eri (cyan dots) and of the 1245 stars of the Pleiades (red dots). The Pleiades sequence is shifted by −5 mag along the MG-axis for better visualisation. The black curves are PARSEC (version 1.2S) isochrones (Chen et al. 2014) with Z = 0.02 and log t = 8.1.
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