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Fig. 8.

image

Cosmological constraints in flat ΛCDM from the mock sample of 20 lensed SN Ia systems with good time-delay measurements. Grey contours/histograms show the marginalised constraints from having only DΔt measurements, orange are those from only Dd measurements, and blue are the results based on both DΔt and Dd measurements. The dashed contours indicate the 68%, 95%, and 99.7% credible regions, whereas the vertical dashed lines in the histograms indicate the 68% credible intervals. The input values are denoted in black and are recovered within the marginalised 68% credible intervals in 1D (or within the 95% credible regions in the 2D H0 − Ωm plane). In flat ΛCDM, even a modest sample of 20 lensed SNe Ia could constrain H0 and Ωm with precisions of 1.3% and 19%, respectively.

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