Fig. 5.
Comparison between the backward NFW model and estimates of the mass from X-ray scaling relations (YX from Vikhlinin et al. 2009 – label on X-axis: 
– and fgas from Mantz et al. 2010 – 
), Planck PSZ2 catalog (Planck Collaboration XXIV 2016; 
), dynamical analysis for the HIFLUGCS sample (Zhang et al. 2017; 
), lensing (Herbonnet et al., in prep.; 
and 
), caustics (Rines et al. 2016; 
). The number of objects in common is shown. Shaded regions indicate the < 10% (darkest) and < 30% differences.
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