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We study the environments of 49 WISE/NVSS-selected dusty, hyper-luminous, z~2quasars using the Atacama Large Millimeter/Sub-millimeter Array (ALMA) 345GHzimages. We find that 17 of the 49 WISE/NVSS sources show additional sub-mmgalaxies within the ALMA primary beam, probing scales within ~150 kpc. We finda total of 23 additional sub-mm sources, four of which in the field of a singleWISE/NVSS source. The measured 870 um source counts are ~10 times expectationsfor unbiased regions, suggesting such hyper-luminous dusty quasars areexcellent at probing high-density peaks.

ALMA detected overdensity of sub-mm sources around WISE/NVSS-selected z~2 dusty quasars