tokens: ACKNOWLEDGEMENTS We greatly appreciate valuable comments from Christopher M. Hirata and Patrick Mcdonald. We also thank Tim Eifler for providing the source galaxy redshift information for the PWL-Stage III and IV surveys adopted in this work. ZD, DC, and H-JS are supported by the U.S. Department of Energy, Office of Science,Office of High Energy Physics under Award Number DE-SC0014329. SS was supported in part by JSPS KAKENHI Grant Number JP15H05896 and by World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan. This research used the DESI allocation resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231.
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