Observed richness-weak-lensing mass relation comparison with different literature results. We compute our model considering an observed richness with a minimum stellar mass of M_{star,  min} = 10¹⁰ h⁻¹ M_⊙ and the parameters have been calculated at z = 0.35. All redMaPPer (Rykoff et al. 2014) richness definitions have been rescaled to DES-Y1 by McClintock et al. (2019) (see their Table 5). The two dotted lines referring to KiDS-DR3 clusters from Lesci et al. (2022a) and Bellagamba et al. (2019) have been computed with the AMICO cluster finder algorithm (Maturi et al. 2019).