Thursday.
1808.09516
Magnification bias in the shear-ratio test: a viable mitigation strategy
Unruh, Schneider, Hilbert
Using the same lens galaxies, the ratios of tangential shears for different source galaxy redshifts is equal to the ratios of their corresponding angular-diameter distances. This is the so-called shear-ratio test (SRT) and it is valid when effects induced by the intervening large-scale structure (LSS) an be neglected. The dominant LSS effect is magnification bias which, on the one hand, induces an additional shear, and on the other hand, causes a magnification of the lens population. The objective is to quantify the magnification bias for the SRT and show an easy-to-apply mitigation strategy that does not rely on additional observations. Use ray-tracing data through the Millennium simulations to measure the influence of magnification on the SRT an test the mitigation strategy. Using the SRT as a null-test, find deviations from zero up to 10% for a flux-limited sample of lens galaxies, which is a strong function of lens redshift and the lens-source line-of-sight separation. Using the mitigation strategy can improve the null-test by a factor of ~100.
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