Number of lenses in each subsample. The bins are separated with the M*, as shown in the first column. In the following columns, the parameters of each bin are listed in sequence, the number of lenses of subsample, the average redshift, the average projection cluster-centric physical distance, the average comoving projection cluster-centric physical distance, the average stellar mass, host halo normalization α, subhalo mass, SHMR, and average dark matter strip rate. All the masses are in unit of |${\rm M_{\odot }}\, h^{-1}$| and distance in Mpc h−1.
| lg(M*) range . | Num . | <z> . | <Rpp> . | <Rp> . | lg(<M*>) . | α . | rsub . | lg(Menh) . | Menh/<M*> . | τstrip . |
|---|---|---|---|---|---|---|---|---|---|---|
| 10.0–10.3 | 421 86 | 0.3 | 0.25 | 0.33 | 10.19 | |$1.04_{-0.02}^{+0.01}$| | |$0.05_{-0.02}^{+0.02}$| | |$11.01_{-0.55}^{+0.27}$| | |$6.71_{-4.8}^{+5.78}$| | |$0.76_{-0.21}^{+0.17}$| |
| 10.3–10.5 | 513 29 | 0.31 | 0.26 | 0.34 | 10.41 | |$1.01_{-0.03}^{+0.01}$| | |$0.07_{-0.01}^{+0.02}$| | |$11.38_{-0.18}^{+0.16}$| | |$9.37_{-3.13}^{+4.23}$| | |$0.62_{-0.17}^{+0.13}$| |
| 10.5–10.7 | 517 36 | 0.32 | 0.27 | 0.36 | 10.6 | |$0.98_{-0.02}^{+0.02}$| | |$0.09_{-0.01}^{+0.01}$| | |$11.62_{-0.12}^{+0.11}$| | |$10.41_{-2.53}^{+3.0}$| | |$0.59_{-0.12}^{+0.1}$| |
| 10.7–11.0 | 578 28 | 0.33 | 0.29 | 0.38 | 10.84 | |$0.98_{-0.01}^{+0.01}$| | |$0.09_{-0.01}^{+0.01}$| | |$11.76_{-0.08}^{+0.08}$| | |$8.36_{-1.45}^{+1.66}$| | |$0.77_{-0.05}^{+0.04}$| |
| 11.0–11.5 | 262 41 | 0.34 | 0.3 | 0.39 | 11.17 | |$0.96_{-0.03}^{+0.03}$| | |$0.15_{-0.02}^{+0.02}$| | |$12.24_{-0.09}^{+0.09}$| | |$11.67_{-2.16}^{+2.55}$| | |$0.91_{-0.02}^{+0.02}$| |
| lg(M*) range . | Num . | <z> . | <Rpp> . | <Rp> . | lg(<M*>) . | α . | rsub . | lg(Menh) . | Menh/<M*> . | τstrip . |
|---|---|---|---|---|---|---|---|---|---|---|
| 10.0–10.3 | 421 86 | 0.3 | 0.25 | 0.33 | 10.19 | |$1.04_{-0.02}^{+0.01}$| | |$0.05_{-0.02}^{+0.02}$| | |$11.01_{-0.55}^{+0.27}$| | |$6.71_{-4.8}^{+5.78}$| | |$0.76_{-0.21}^{+0.17}$| |
| 10.3–10.5 | 513 29 | 0.31 | 0.26 | 0.34 | 10.41 | |$1.01_{-0.03}^{+0.01}$| | |$0.07_{-0.01}^{+0.02}$| | |$11.38_{-0.18}^{+0.16}$| | |$9.37_{-3.13}^{+4.23}$| | |$0.62_{-0.17}^{+0.13}$| |
| 10.5–10.7 | 517 36 | 0.32 | 0.27 | 0.36 | 10.6 | |$0.98_{-0.02}^{+0.02}$| | |$0.09_{-0.01}^{+0.01}$| | |$11.62_{-0.12}^{+0.11}$| | |$10.41_{-2.53}^{+3.0}$| | |$0.59_{-0.12}^{+0.1}$| |
| 10.7–11.0 | 578 28 | 0.33 | 0.29 | 0.38 | 10.84 | |$0.98_{-0.01}^{+0.01}$| | |$0.09_{-0.01}^{+0.01}$| | |$11.76_{-0.08}^{+0.08}$| | |$8.36_{-1.45}^{+1.66}$| | |$0.77_{-0.05}^{+0.04}$| |
| 11.0–11.5 | 262 41 | 0.34 | 0.3 | 0.39 | 11.17 | |$0.96_{-0.03}^{+0.03}$| | |$0.15_{-0.02}^{+0.02}$| | |$12.24_{-0.09}^{+0.09}$| | |$11.67_{-2.16}^{+2.55}$| | |$0.91_{-0.02}^{+0.02}$| |
Number of lenses in each subsample. The bins are separated with the M*, as shown in the first column. In the following columns, the parameters of each bin are listed in sequence, the number of lenses of subsample, the average redshift, the average projection cluster-centric physical distance, the average comoving projection cluster-centric physical distance, the average stellar mass, host halo normalization α, subhalo mass, SHMR, and average dark matter strip rate. All the masses are in unit of |${\rm M_{\odot }}\, h^{-1}$| and distance in Mpc h−1.
| lg(M*) range . | Num . | <z> . | <Rpp> . | <Rp> . | lg(<M*>) . | α . | rsub . | lg(Menh) . | Menh/<M*> . | τstrip . |
|---|---|---|---|---|---|---|---|---|---|---|
| 10.0–10.3 | 421 86 | 0.3 | 0.25 | 0.33 | 10.19 | |$1.04_{-0.02}^{+0.01}$| | |$0.05_{-0.02}^{+0.02}$| | |$11.01_{-0.55}^{+0.27}$| | |$6.71_{-4.8}^{+5.78}$| | |$0.76_{-0.21}^{+0.17}$| |
| 10.3–10.5 | 513 29 | 0.31 | 0.26 | 0.34 | 10.41 | |$1.01_{-0.03}^{+0.01}$| | |$0.07_{-0.01}^{+0.02}$| | |$11.38_{-0.18}^{+0.16}$| | |$9.37_{-3.13}^{+4.23}$| | |$0.62_{-0.17}^{+0.13}$| |
| 10.5–10.7 | 517 36 | 0.32 | 0.27 | 0.36 | 10.6 | |$0.98_{-0.02}^{+0.02}$| | |$0.09_{-0.01}^{+0.01}$| | |$11.62_{-0.12}^{+0.11}$| | |$10.41_{-2.53}^{+3.0}$| | |$0.59_{-0.12}^{+0.1}$| |
| 10.7–11.0 | 578 28 | 0.33 | 0.29 | 0.38 | 10.84 | |$0.98_{-0.01}^{+0.01}$| | |$0.09_{-0.01}^{+0.01}$| | |$11.76_{-0.08}^{+0.08}$| | |$8.36_{-1.45}^{+1.66}$| | |$0.77_{-0.05}^{+0.04}$| |
| 11.0–11.5 | 262 41 | 0.34 | 0.3 | 0.39 | 11.17 | |$0.96_{-0.03}^{+0.03}$| | |$0.15_{-0.02}^{+0.02}$| | |$12.24_{-0.09}^{+0.09}$| | |$11.67_{-2.16}^{+2.55}$| | |$0.91_{-0.02}^{+0.02}$| |
| lg(M*) range . | Num . | <z> . | <Rpp> . | <Rp> . | lg(<M*>) . | α . | rsub . | lg(Menh) . | Menh/<M*> . | τstrip . |
|---|---|---|---|---|---|---|---|---|---|---|
| 10.0–10.3 | 421 86 | 0.3 | 0.25 | 0.33 | 10.19 | |$1.04_{-0.02}^{+0.01}$| | |$0.05_{-0.02}^{+0.02}$| | |$11.01_{-0.55}^{+0.27}$| | |$6.71_{-4.8}^{+5.78}$| | |$0.76_{-0.21}^{+0.17}$| |
| 10.3–10.5 | 513 29 | 0.31 | 0.26 | 0.34 | 10.41 | |$1.01_{-0.03}^{+0.01}$| | |$0.07_{-0.01}^{+0.02}$| | |$11.38_{-0.18}^{+0.16}$| | |$9.37_{-3.13}^{+4.23}$| | |$0.62_{-0.17}^{+0.13}$| |
| 10.5–10.7 | 517 36 | 0.32 | 0.27 | 0.36 | 10.6 | |$0.98_{-0.02}^{+0.02}$| | |$0.09_{-0.01}^{+0.01}$| | |$11.62_{-0.12}^{+0.11}$| | |$10.41_{-2.53}^{+3.0}$| | |$0.59_{-0.12}^{+0.1}$| |
| 10.7–11.0 | 578 28 | 0.33 | 0.29 | 0.38 | 10.84 | |$0.98_{-0.01}^{+0.01}$| | |$0.09_{-0.01}^{+0.01}$| | |$11.76_{-0.08}^{+0.08}$| | |$8.36_{-1.45}^{+1.66}$| | |$0.77_{-0.05}^{+0.04}$| |
| 11.0–11.5 | 262 41 | 0.34 | 0.3 | 0.39 | 11.17 | |$0.96_{-0.03}^{+0.03}$| | |$0.15_{-0.02}^{+0.02}$| | |$12.24_{-0.09}^{+0.09}$| | |$11.67_{-2.16}^{+2.55}$| | |$0.91_{-0.02}^{+0.02}$| |
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