Barred spiral galaxies with stronger boxy/peanut (m=4) and hexapole (m=6) components produce larger cusp flux ratio anomalies in simulations (Spearman r=0.85–0.89).
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Gravitational lensing by a spiral galaxy I: the influence from bar's structure to the flux ratio anomaly
Barred spiral galaxies with stronger boxy/peanut (m=4) and hexapole (m=6) components produce larger cusp flux ratio anomalies in simulations (Spearman r=0.85–0.89).