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Density-split analyses of the pairwise kinetic Sunyaev-Zeldovich effect
We consider the dependence of the kinetic Sunyaev-Zeldovich (kSZ) effect on the environments of foreground cosmological structures. Standard pairwise kSZ estimators exploit the fact that galaxies below separations of $\sim 200\,h^{-1}{\rm M}_\odot$ fall towards each other on average, yielding a nega
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