Figure 3.
The distribution of the axis ratios for dark matter haloes identified in the mdpl2 simulation. The top row shows the redshift dependency of a sample selected by mass, while the bottom row shows the mass dependency at z = 0.55.
The distribution of the axis ratios for dark matter haloes identified in the mdpl2 simulation. The top row shows the redshift dependency of a sample selected by mass, while the bottom row shows the mass dependency at z = 0.55.
