Yuichi Higuchi, Masamune Oguri, Takashi Hamana
We study the prospects for measuring the dark matter distribution of voids with stacked weak lensing. We select voids from a large set of N-body simulations, and explore their lensing signals with the full ray-tracing simulations including the effect of the large-scale structure along the line-of-sight. The lensing signals are compared with simple void model predictions to reconstruct the three-dimensional mass distribution of voids. We show that the stacked weak lensing signals are detected at significant level (S/N \geq 5) for a 5000 degree^2 survey area, for a wide range of void radii up to \sim 50 Mpc. The error from the shape noise little affects lensing signals at large scale. It is also found that dense ridges around voids have a great impact on the weak lensing signals, suggesting that proper modeling of the void density profile including surrounding ridges is essential for extracting the average total mass of voids.
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http://arxiv.org/abs/1211.5966
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