Image Details
Caption: Figure 5.
Mass bias (Equation (26)) as a function of galaxies’ number density ngal under three different selection criterion ﹩{\nu }_{\mathrm{threshold}},{\nu }_{\mathrm{threshold}}=3.0﹩ (left), νthreshold = 4.0 (middle), and νthreshold = 5.0 (right). Large red circles show the results for the shear-selected samples, and small black circles show the results for the corresponding control samples that are selected based on noise-free νNFW instead of νobs to demonstrate that the bias is indeed caused by upscattering due to the noise. The positions of the control samples are slightly shifted rightward to avoid overlaps.
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