Image Details
 
                    Caption: Figure 6.
Posterior distributions from three-halo simultaneous mass estimation in our MCMC analysis. The mass centers were set to the first moments of the local convergence values. The black and gray filled contours represent approximately 68% and 95% confidence limits, respectively. The low Pearson correlation coefficients ρ suggest that the degeneracies among the masses of the three halos are low.
© 2024. The Author(s). Published by the American Astronomical Society.