Table 3.
Cosmological parameters extracted with MontePython MCMC sampling.
| Cosmological model | Ωm | ΩCDM | ΩΛ | ΩDE | Ωk | w0 | wa | H0 |
|---|---|---|---|---|---|---|---|---|
| Lenses only | ||||||||
| Flat ΛCDM |
|
|
|
≡0 | ≡0 | ≡ − 1 | ≡0 |
|
| Flat wCDM |
|
|
≡0 |
|
≡0 |
|
≡0 |
|
| Flat w0waCDM |
|
|
≡0 |
|
≡0 |
|
|
|
| Non-flat ΛCDM |
|
|
|
≡0 |
|
≡ − 1 | ≡0 |
|
| Lenses + SNe Ia | ||||||||
| Flat ΛCDM |
|
|
|
≡0 | ≡0 | ≡ − 1 | ≡0 |
|
| Flat wCDM |
|
|
≡0 |
|
≡0 |
|
≡0 |
|
| Flat w0waCDM |
|
|
≡0 |
|
≡0 |
|
|
|
| Non-flat ΛCDM |
|
|
|
≡0 |
|
≡ − 1 | ≡0 |
|
| Non-flat wCDM |
|
|
≡0 |
|
|
|
≡0 |
|
| Non-flat w0waCDM |
|
|
≡0 |
|
|
|
|
|
Notes. Results for different cosmological models are shown for quasar time delays alone (upper four lines) and for the combination of the time-delay measurements with the JLA SN Ia sample (lower six lines). The quoted numbers are the median values, while the uncertainties correspond to the 16th and 84th percentiles.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.