Total projected mass as a function of aperture radius centered at BCG1 (for the simplicity of the comparison with results of Bradač et al. 2006) for different model components. The two large scale clumps, DM1 and DM2, contribute a similar amount to the mass, the X-rays gas mass measured by (Markevitch et al. 2004) is ~ 9 ± 3% to the total mass at 250 kpc radius. The galaxies (including the BCG) contribute 11 ± 5% within a 250 kpc radial aperture.