Image Details
Caption: Figure 3.
Geometric dependence of the lensing signal, plotted vs. the distance ratio
x ≡ ω
S
/ω
L
, for a WMAP7 cosmology with Ω
M
= 0.27,
. The solid (red) curve shows the theoretical prediction Γ(
x) = 0 for
x < 1; Γ(
x) = 1 − 1/
x for
x > 1. Note that the data have not been weighted for cosmological sensitivity (as in Section 4.2); a fit to the unweighted
data favors a slightly shorter length scale for
x (i.e., lower value of
) but with very large uncertainties.
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