Calibration of radii and masses of open clusters with a simulation

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Fig. 8

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Histogram of the fraction on the sky per bin in M_t/M_cl corresponding to the T₄ = 1.31 Gyr parameter surface from Fig. 7. M_t and M_cl are the “tidal masses” calculated with Eq. (9) from r_t and r_J, respectively.

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