Table 3.
H0 distributions from Fig. 9.
| Hao’s ditribution |
50/50 distribution |
|||||
|---|---|---|---|---|---|---|
| H0 | σmultipole | σno multipole | H0 | σmultipole | σno multipole | |
| [km s−1 Mpc−1] | [%H0] | [%H0] | [km s−1 Mpc−1] | [%H0] | [%H0] | |
| 5400 s very bright |
 |
1.7% | 3.0% |
 |
2.0% | 2.9% |
| 3000 s bright |
 |
4.7% | 3.4% |
 |
5.6% | 3.4% |
| 3000 s faint |
 |
4.9% | 3.8% |
 |
5.4% | 3.9% |
Notes. H0 distributions for the different S/Ns and the two different fractions of boxy and discy galaxies. Left: 36% boxy, 64% discy, following Hao et al. (2006); right: 50% boxy, 50% discy. For each distribution, the median H0 and its 68% credible interval are given in km s−1 Mpc−1 on the left, the specific contribution from the multipole to the error budget calculated as in (5) expressed as a percentage of the median H0 is displayed in the middle, and that from multipole-free lensing galaxies is displayed on the right. More specifically, the σmultipole and σno multipole are the mean values of the two sides of the 68% credible intervals.
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