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tokens: B.V.L. was supported by a Stanford University undergraduate research grant. Y.Y.M. was supported by the Weiland Family Stanford Graduate Fellowship. This work received partial support from the U.S. Department of Energy under contract number DE-AC02-76SF00515. We thank Harry Desmond and Andrew Hearin for useful discussions. We thank Rachel Reddick for providing the measurement of observed galaxy statistics used in this work. This research made use of the Dark Sky Simulations, which were produced using an INCITE 2014 allocation on the Oak Ridge Leadership Computing Facility at Oak Ridge National Laboratory. We thank Mike Warren, Matt Turk, and our other Dark Sky collaborators for their efforts in creating these simulations and for providing access to them. We thank Peter Behroozi for providing the halo catalogs and merger trees for the Bolshoi , BolshoiP , and MDPL simulations, which were run by the MultiDark Collaboration. Additional simulations and computations were performed using computational resources at SLAC and at NERSC. We thank the SLAC computational team for their consistent support.