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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 7.

Relation between m₄ strength a₄/a and axis ratio q. Blue points and histograms: our sample; red points and histograms: C. N. Hao et al. (2006a); gray points and shaded histograms: random sample generated by prior in M. S. H. Oh et al. (2026). See also Figure 6 in S. Hou et al. (2026).

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