摘要: Recently, several studies reported a significant discrepancy between the
clustering and lensing of the Baryon Oscillation Spectroscopic Survey (BOSS)
galaxies in the $\textit{Planck}$ cosmology. We construct a simple yet powerful
model based on the linear theory to assess whether this discrepancy points
toward deviations from $\textit{Planck}$. Focusing on scales $10
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