Table 1
Constraints on lens parameters for different models of mock cluster lensing mass distribution 2.
Parameters | Input | MP-full | SP | MP-constML | SP-constML | MP-s | SP-s | MP-sm |
---|---|---|---|---|---|---|---|---|
θE, fd1 ![]() |
2.00 | ![]() |
− | ![]() |
− | ![]() |
− | ![]() |
θE, fd2 ![]() |
2.00 | ![]() |
− | ![]() |
− | ![]() |
− | ![]() |
xhalo ![]() |
0.00 | ![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
yhalo ![]() |
0.00 | ![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
0.80 | ![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
θhalo [rad] | 0.000 | ![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
θE, halo ![]() |
10.00 | ![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
rc, halo ![]() |
2.00 | ![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
γhalo | 0.40 | ![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
θE, mg ![]() |
0.17 | ![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
rt, mg ![]() |
1.93 | ![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
θE, bd ![]() |
2.00 | ![]() |
− | ![]() |
− | ![]() |
− | ![]() |
rmsbest-fit ![]() |
4 × 10−5 | 0.549 | 0.126 | 0.511 | 0.069 | 0.547 | 0.083 | |
![]() |
7 × 10−6 | 1284 | 66 | 1085 | 20 | 1255 | 29 |
Notes.The first column refers to the values used to simulate, the other columns refer to different models, in order, the full multi-plane, the single cluster-plane, the full multi-plane and the single cluster-plane with constant mass-to-light ratio, the multi-plane and the single cluster-plane with spherical galaxies, and finally the full multi-plane with spherical cluster members only. The values are the medians of the posterior probability distributions of the lens parameters together with their 1σ uncertainties. The subscripts mg refers to the cluster member with the median luminosity among the members (F160W magnitude of 21.47). The orientation is measured counter clockwise from positive x-axis.
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