Fig. A.2
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Galaxy density map from HSC-SSP survey data at the locations and redshifts of the 19 supercluster candidates. They are obtained by integrating the full probability function of the MIZUKI (Tanaka 2015) photometric redshifts (P(z)) of each galaxy (the S19A catalog; Nishizawa et al. 2020) with a width of the redshift slice of 
, in a similar way as Okabe et al. (2021). The galaxies are brighter than 23 ABmag. The smoothing scale is FWHM= 3 arcmin.
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