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Fig. 13.

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Uncertainties, expressed in percent, of star cluster structural parameters versus cluster core radius, rc. Left column – the median of uncertainties arising due to stochastic IMF sampling and the spatial distribution of cluster stars, δGEN; right column – due to cluster projection effects, δROT. Top row – the median of uncertainties of R50; middle row – R30/R50; bottom row – R50/R80. Results are shown for clusters with log(M/M) = 3.0 and log(t/yr) = 8.0, and three γ values (see legend). Structural parameters are measured using FGCs in the F475W passband. Blue and red markers and corresponding lines are slightly shifted along the X-axis around the original input value for visual clarity. Square root scaling is applied for the X-axis.

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