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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 9.

Box plot of variations in q and ϕq (value at the right side minus that at the left side) in different radial bins with a width of 4 kpc. Left: difference in q; right: difference in ϕq. For each bin, the red line means median, the box spans from Q1 (first quartile) to Q3 (third quartile), and the whiskers extend from the box to the smallest and largest values within 1.5 × interquartile range. The dashed line indicates zero difference.

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