Image Details

Choose export citation format:

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 4.

Difference in axis ratio q and position angle ϕq between mass and light. Left: principal values of axis ratio q for mass and light maps of our galaxy sample, with both histograms added in the panel to the right. The magenta dashed line means y = x. Right: difference of averaged ϕq and q (within two annuli) between mass and light maps for our sample. Dashed lines indicate 16%, 50%, and 84% quartiles.

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse