Table 1.
Summary of the H0 values (Col. 2) reported in Wong et al. (2020) and Shajib et al. (2020).
| H0 | σv | ξ | ξPL | ξcomposite | Aperture | θeff | θE | θaperture | |
|---|---|---|---|---|---|---|---|---|---|
| [km s−1 Mpc−1] | [km s−1] | (All models) | (power-law) | (composite) | |||||
| B1608+656 |
 |
260 ± 15 | 0.27 ± 0.01 | 0.27 ± 0.01 | – |
 |
 |
 |
 |
| RX J1131−1231 |
 |
323 ± 20 | 0.02 ± 0.01 | 0.04 ± 0.01 | 0.01 ± 0.01 |
 |
 |
 |
 |
| HE 0435−1223 |
 |
222 ± 15 | 0.08 ± 0.01 | 0.03 ± 0.01 | 0.13 ± 0.01 |
 |
 |
 |
 |
| SDSS J1206+4332 |
 |
290 ± 30 | 0.42 ± 0.01 | 0.51 ± 0.06 | 0.25 ± 0.01 |
 |
 |
 |
 |
| WFI 2033−4723 |
 |
250 ± 19 | 0.17 ± 0.02 | 0.09 ± 0.01 | 0.35 ± 0.06 |
 |
 |
 |
 |
| PG 1115+080 |
 |
281 ± 25 | −0.04 ± 0.01 | 0.08 ± 0.01 | −0.02 ± 0.01 |
 |
 |
 |
 |
| DES J0408−5354 |
 |
227 ± 9 | −0.01 ± 0.01 | −0.01 ± 0.01 | −0.01 ± 0.01 |
 |
 |
 |
 |
| All | – | – | 0.07 ± 0.02 | 0.07 ± 0.01 | 0.06 ± 0.02 | – | – | – |
Notes. Column 3 gives the aperture velocity dispersion used for their analysis along with 1σ error bars. Columns 4–6 give the sensitivity, ξ, of the inferred H0 value to the lens galaxy velocity dispersion. When the information is available, we make a distinction between composite and power-law model and the combination of these. Columns 7–9 list the size of the aperture used for the velocity dispersion measurement, the effective radius θeff of the lens and the Einstein radius of each lens. Column 10 give the aperture radius θaperture, computed by taking half of the average length of the slit side.
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