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We model the chameleon effect on cosmological statistics for the modified gravity f(R) model of cosmic acceleration.
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This corrects a 3% absolute error in the initial amplitude reported in Oyaizu et al. 2008 but does not change results relative to Λ \Lambda CDM significantly
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G.-B. Zhao, B. Li, and K. Koyama, Phys.Rev. D83
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