Comparison of morphology between the surface mass density map derived from two dark halo components and other wavelength images. Top left: white contours of the surface mass density map are overlaid on the X-ray surface brightness image. The contours indicate levels of 2.0, 3.0, 4.0, …, 9.0, 10.0 × 10¹⁵ h ﹩{M}_{\odot }﹩ Mpc⁻². This X-ray image is the same as in the left panel of Figure 1. The mass peak of the main cluster coincides with the X-ray centroid, while no X-ray counterparts are found at the mass peak of the subcluster. Top right: same as top left, but for the SZE image. This SZE image is the same as in the right panel of Figure 1. No SZE counterparts are found at the mass peak of the subcluster. Bottom left: same as top left, but for the X-ray residual image. This X-ray residual image is the same as in the left panel of Figure 2. The clear offset between the mass peak of the subcluster and the X-ray substructure is found. Bottom right: same as top left, but for the SZE residual image. This SZE residual image is the same as in the right panel of Figure 2. As shown in the top right panel, the offset between the SZE substructure and the mass peak of the subcluster is found.