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Fig. 13.
Projected numbers of galaxies in the overdensity as a function of their distance to AGS24 (black circles) and the black dashed line is the linear fitting to the profile. The red line shows the best-fit projected NFW profile (Navarro et al. 1996) of a galaxy cluster at z = 2.506, CL J1001+0220 (Wang et al. 2016).
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