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Can Third- and Fourth-order Multipoles plus Radial Variation of Isodensity Ellipses Explain the Observed Flux Ratios in B1422+231? YES, and a Lesson Learned from a TNG100 Lensing Galaxy Sample

  • Authors: Ruizhe Feng, Dandan Xu, Dominique Sluse, Giulia Despali, Anowar J. Shajib, Cai-Na Hao

Ruizhe Feng et al 2026 The Astrophysical Journal 1012 .

  • Provider: AAS Journals

Caption: Figure 5.

Comparison of a4/a between the mass and light distributions for our full galaxy sample (black points and histograms) and a subsample with velocity dispersion σv ≥ 200 km s−1 (blue points and histograms). The magenta dashed line means y = x, and the red histogram is the distribution from C. N. Hao et al. (2006a).

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