Table D.1
Inference on models free parameters for the cored mock.
Component | Parameter | Prior | Median | 1σ | 3σ | Actual |
---|---|---|---|---|---|---|
MP | log JMP | [0.3, 2.5] | 0.94 | [0.64, 1.09] | [0.31, 1.20] | 0.8 |
hz, MP | [0, 1.5] | 0.11 | [0.01, 0.26] | [0.00, 0.89] | 0.05 | |
gz, MP | [0, 1.5] | 1.07 | [0.93, 1.19] | [0.58, 1.29] | 1.2 | |
ΓMP | [0, 3] | 1.04 | [0.79, 1.27] | [0.56, 1.52] | 1.0 | |
BMP | [3, 25] | 17.72 | [11.24, 21.82] | [7.22, 24.86] | 14 | |
![]() |
[−2.1, −1.7] | −2.00 | [−2.01, −1.98] | [−2.03, −1.95] | −2 | |
σM, MP [dex] | [0.15, 0.45] | 0.32 | [0.31, 0.33] | [0.29, 0.35] | 0.3 | |
fMP | [0.5, 0.75] | 0.59 | [0.56, 0.61] | [0.53, 0.64] | 0.6 | |
MR | log JMR | [0.3, 2.5] | 1.52 | [1.34, 1.67] | [1.15, 1.87] | 1.5 |
hz, MR | [0, 1.5] | 0.38 | [0.13, 0.86] | [0.00, 1.48] | 0.6 | |
gz, MR | [0, 1.5] | 0.45 | [0.38, 0.51] | [0.28, 0.72] | 0.4 | |
ΓMR | [0, 3] | 0.39 | [0.11, 0.74] | [0.01, 1.23] | 0.4 | |
BMR | [3, 25] | 18.78 | [13.74, 23.31] | [10.34, 24.85] | 20 | |
![]() |
[−1.65, −1.3] | −1.42 | [−1.44, −1.40] | [−1.47, −1.37] | −1.4 | |
σM, MR [dex] | [0.15, 0.45] | 0.32 | [0.31, 0.33] | [0.28, 0.36] | 0.3 | |
fMR | [0.25, 0.5] | 0.41 | [0.39, 0.44] | [0.36, 0.47] | 0.4 | |
DM | log MDM[M⊙] | [7, 11] | 8.41 | [8.26, 8.61] | [8.18, 8.92] | 8.5 |
log rs[kpc] | [−3, 1] | −0.36 | [−0.43, −0.29] | [−0.51, −0.18] | −0.5 | |
α | [0, 7] | 4.65 | [2.82, 6.37] | [1.51, 6.97] | 4.0 | |
η | [2, 7] | 3.49 | [3.00, 4.17] | [2.58, 4.82] | 3.0 | |
γ | [0, 1.9] | 0.17 | [0.04, 0.34] | [0.00, 0.56] | 0.0 |
Notes. The table is divided into three parts showing the parameters of the MP and MR stellar populations and the DM component. Column 1 indicates the components the parameters are referred to; Col. 2 lists the parameters; Col. 3 shows the range of uniform priors we used in the EMCEE runs; Cols. 4, 5, and 6 list the median values, 1σ and 3σ confidence intervals; and finally Col. 7 shows the real value used to produce the mock. Details on the MCMC procedure and on how the 1σ and 3σ confidence intervals are computed are given in App. A
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