Investigating the relation between the environment and internal structure of massive elliptical galaxies using strong lensing

Open Access

Fig. 5.

Left: Distribution of the local galaxy density, Σ₁₀, vs. the Einstein radius, θ_E. Right: Distribution of the local galaxy density, Σ₁₀, vs. the residual shear magnitude, γ_shear (right-hand panel). The correlation is very weak for both the Einstein radius and the residual shear magnitude.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.