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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 7.

Our θE measurements compared to 4 HST photometry mass-modeled lenses in N. Sahu et al. (2024) and 11 in L. Iwamoto et al. (2026, in preparation; obtained via private correspondence). We find ﹩\frac{{\rm{\Delta }}{\theta }_{\rm{E}\,}}{{\theta }_{\,\rm{E}}}=0.15,0.11,0.15﹩, for the line (blue circles), circle (green squares), and blended line (orange stars) models, respectively. The error bars correspond to half the primary image arc width measured from DECaLS imaging. We incorporate this scatter into uncertainty for the rest of our θE measurements.

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