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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 2.

EAZY output for a line-of-sight object in the field of AGEL2303, with fitted redshift z_phot = 0.80. Left: ﹩{\mathrm{log}}_{10}﹩ flux versus ﹩{\mathrm{log}}_{10}﹩ observed wavelength. The black squares are the observed fluxes in six bands, and the magenta circles are the modeled flux measurements; the green distribution is the SED fit. The posterior SED shows continuum features, consistent with an early-type galaxy. Right: the posterior redshift probability distribution, P(z), against z.

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