Open superclusters - I. The most populated primordial groups of open clusters in the third quadrant of the Galactic disk

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Fig. 4.

Color–magnitude diagram and the fitted isochrone of the new OC Casado-Hendy 4. The continuous lines are the PARSEC isochrone fitted to our data, while dashed ones represent the same isochrone but vertically shifted by −0.75 mag (the locus of unresolved binaries of equal-mass components).

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