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Fig. 5.

image

Comparison between X-ray and caustic masses for the 25 clusters in common with Sohn et al. (2020). Relaxed (R) and disturbed (D) clusters are plotted with blue and red circles, respectively. Filled and empty circles represent the clusters with N200 >  100 and N200 <  100, respectively. The dotted magenta line represents the average MHE/Mc ratio. The dashed green line represents the average MHE/Mc ratio obtained after removing the clusters with less than 100 galaxies within R200.

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