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Table 1.

Cluster binning used for the weak lensing analysis.

z range zeff λ* range Ncl zs,eff
[0.10,  0.30] 0.189 ± 0.001 [0,  15] 10.20 ± 0.09 −0.73 ± 0.07 1246 0.849 ± 0.002
[0.10,  0.30] 0.212 ± 0.002 [15,  25] 18.88 ± 0.12 −0.38 ± 0.07 684 0.867 ± 0.002
[0.10,  0.30] 0.222 ± 0.004 [25,  35] 29.02 ± 0.21 0.05 ± 0.07 209 0.879 ± 0.002
[0.10,  0.30] 0.228 ± 0.007 [35,  45] 39.75 ± 0.32 0.32 ± 0.06 82 0.877 ± 0.005
[0.10,  0.30] 0.222 ± 0.008 [45,  150] 56.59 ± 2.20 0.54 ± 0.06 44 0.890 ± 0.013
[0.30,  0.45] 0.374 ± 0.001 [0,  20] 15.10 ± 0.11 −0.41 ± 0.08 1113 0.948 ± 0.003
[0.30,  0.45] 0.387 ± 0.002 [20,  30] 24.08 ± 0.11 −0.07 ± 0.07 767 0.944 ± 0.004
[0.30,  0.45] 0.389 ± 0.002 [30,  45] 35.91 ± 0.27 0.21 ± 0.06 320 0.941 ± 0.005
[0.30,  0.45] 0.390 ± 0.005 [45,  60] 50.88 ± 0.50 0.41 ± 0.08 87 0.950 ± 0.015
[0.30,  0.45] 0.379 ± 0.006 [60,  150] 73.60 ± 2.09 0.68 ± 0.07 45 0.946 ± 0.012
[0.45,  0.60] 0.498 ± 0.001 [0,  25] 19.71 ± 0.11 −0.33 ± 0.09 1108 0.958 ± 0.001
[0.45,  0.60] 0.514 ± 0.002 [25,  35] 29.23 ± 0.12 −0.07 ± 0.07 761 0.961 ± 0.004
[0.45,  0.60] 0.523 ± 0.003 [35,  45] 39.25 ± 0.18 0.21 ± 0.07 299 0.961 ± 0.006
[0.45,  0.60] 0.513 ± 0.004 [45,  150] 55.12 ± 0.76 0.36 ± 0.07 197 0.960 ± 0.004

Notes. The computation of zeff and and their uncertainties are described in Bellagamba et al. (2019). For the logarithm of the measured mean masses, , we quote the mean and the standard deviation of the posterior probability distribution. We note that Ncl is the number of clusters in the bin. In the last column, zs,eff is the effective redshift of the lensed sources, obtained by following the procedure described in Giocoli et al. (2021). Quoted masses refer to a flat ΛCDM model with Ωm = 0.3 and h = 0.7.

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