Table 4.
Results obtained from the cross-correlation data with flat priors (FPA FPC; second column) on astrophysical and cosmological parameters.
| Param | Priors | FPA FPC | FPA FPC shifted | ||||
|---|---|---|---|---|---|---|---|
| F[a,b] | μ | σ | Peak | μ | σ | Peak | |
| ±68 CL | 68 CL | ±68 CL | 68 CL | ||||
| log(Mmin/M⊙) | F[11.6,13.6] |
 |
0.27 | 12.61 |
 |
0.22 | 12.53 |
| log(M1/M⊙) | F[13,14.5] | – | – | 14.39 |
 |
0.40 | 13.69 |
| α | F[0.5,1.37] | – | – | 0.50 |
 |
0.24 | 0.50 |
| Ωm | F[0.1,0.8] |
 |
0.16 | 0.67 |
 |
0.17 | 0.59 |
| σ8 | F[0.6,1.2] |
 |
0.11 | 0.74 |
 |
0.12 | 0.77 |
| h | F[0.5,1.0] |
 |
0.14 | 1.00 | – | – | 0.85 |
Notes. From left to right, the columns are the parameters, the priors, and the results (the mean μ with the upper and lower limit at the 68% CL, the σ, and the peak of the posterior distribution) for the default and shifted binning, respectively. Parameters without a σ value indicate that there is no constraint at 68% CL, i.e. they are unconstrained.
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