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Most Strong Lensing Deflectors in the AGEL Survey Are in Group and Cluster Environments

  • Authors: William J. Gottemoller, Nandini Sahu, Rodrigo Cordova Rosado, Leena Iwamoto, Courtney B. Watson, Kim-Vy H. Tran, A. Makai Baker, Tania M. Barone, Duncan J. Bowden, Karl Glazebrook, Anishya Harshan, Tucker Jones, Glenn G. Kacprzak, Camryn M. Neches

William J. Gottemoller et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 10.

Σ5(z) versus measured Einstein mass (﹩{{\mathrm{log}}}_{10}\frac{M(\lt {\theta }_{\,\rm{E}\,})}{{M}_{\odot }}﹩). The downward-facing triangles are systems for which we estimate the upper limit Σ5(z), the circles are systems with measured Σ5(z), and the star is the system AGEL0424 (see Figure 11). The color scheme is based on zdefl. We find a Spearman correlation of 0.38, suggesting only a weak correlation between Einstein mass and halo mass.

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