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Fig. 2


Bias map under a wide range of cosmological parameters. For these two panels, the KS inversion is applied. The dark energy equation of state is . The S/N bin is ν = [4.0, 4.5]. The filter size is 1.2 arcmin for the left panel and 2.4 arcmin for the right panel. Contours of parameters sharing the same bias level can be clearly observed. However, they are not necessarily centered on the same parameters when the filter changes. The bias levels are not similar either. These contours vary even more when we examine other choices of bins.

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