Image Details
 
                    Caption: Figure 7.
Five-halo mass estimation in the same format used in Figure 6. The mass centers were set to the convergence peaks. In some cases, where the distance between the two neighboring substructures is relatively small, the degeneracy is relatively high (the Pearson correlation coefficients are ρ = −0.535 for the NWE−NWW pair and ρ = −0.685 for the SEN−SES pair).
© 2024. The Author(s). Published by the American Astronomical Society.