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Table 5.

Cosmological models, probes, and strong lensing datasets considered in extensions of the ΛCDM model.

ΛCDM extensions
Model ID Cosmological model Experiments/datasets Cosmological priors

H0 ∼ 𝒰 (0, 150) km s−1 Mpc−1
UoΛCDM Open ΛCDM TDCOSMO Ωm ∼𝒰 (0.05, 0.5)
oΛCDM Open ΛCDM TDCOSMO + Planck Ωk ∼𝒰 (−0.5, 0.5)
ΩΛ = 1 − Ωm − Ωk > 0

UwCDM Flat wCDM TDCOSMO
wCDM1 Flat wCDM TDCOSMO + Planck H0 ∼ 𝒰 (0, 150) km s−1 Mpc−1
wCDM2 Flat wCDM TDCOSMO + DESI BAO Ωm ∼ 𝒰 (0.05, 0.5)
wCDM3 Flat wCDM TDCOSMO + Pantheon+ w0 ∼𝒰 (−1.5, 0.5)

Uw0waCDM Flat w0waCDM TDCOSMO H0 ∼ 𝒰 (0, 150) km s−1 Mpc−1
w0waCDM1 Flat w0waCDM TDCOSMO + Planck Ωm ∼𝒰 (0.05, 0.5)
w0waCDM2 Flat w0waCDM TDCOSMO + DESI BAO w0 ∼𝒰 (−1.5, 0.5)
w0waCDM3 Flat w0waCDM TDCOSMO + Pantheon+ wa ∼ 𝒰 (−10, 10)
w0waCDM4 Flat w0waCDM TDCOSMO + DESI BAO + Pantheon+

UwϕCDM Flat wϕCDM TDCOSMO H0 ∼ 𝒰 (0, 150) km s−1 Mpc−1
wϕCDM1 Flat wϕCDM TDCOSMO + DESI BAO Ωm ∼𝒰 (0.05, 0.5)
wϕCDM2 Flat wϕCDM TDCOSMO + Pantheon+ w0 ∼𝒰 (−1.5, 0.5)
α ∼ 𝒰 (1.35, 1.55)

Notes. All cases in this table include the external lensing datasets from the SLACS and SL2S. The group of parameter priors within each row block is used for all cosmological models within that row block.

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