Abstract
Cross correlating gamma-ray maps with locations of galaxies in the low-redshift Universe vastly increases sensitivity to signatures of annihilation of dark matter particles. Low-redshift galaxies are ideal targets, as the largest contribution to anisotropy in the gamma-ray sky from annihilation comes from $z\ensuremath{\lesssim}0.1$, where we expect minimal contributions from astrophysical sources such as blazars. Cross correlating the five-year data of Fermi-LAT with the redshift catalog of the 2MASS survey can detect gamma rays from annihilation if dark matter has the canonical annihilation cross section and its mass is smaller than $\ensuremath{\sim}100\text{ }\text{ }\mathrm{GeV}$.
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