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Table 4.
Combinations of cosmological probes and strong lensing datasets considered in this work, assuming a flat ΛCDM cosmology.
| Baseline flat-ΛCDM cosmology | ||||
|---|---|---|---|---|
| Model ID | Cosmological model | Experiments/datasets | External lenses | Cosmological priors |
| UΛCDM1 | Flat ΛCDM | TDCOSMO | – | |
| UΛCDM2 | Flat ΛCDM | TDCOSMO | SLACS | H0 ∼ 𝒰 (0, 150) km s−1 Mpc−1 |
| UΛCDM3 | Flat ΛCDM | TDCOSMO | SL2S | Ωm ∼ 𝒰 (0.05, 0.5) |
| UΛCDM4 | Flat ΛCDM | TDCOSMO | SLACS + SL2S | |
| ΛCDM1a | Flat ΛCDM | TDCOSMO + Pantheon+ | – | |
| ΛCDM1b | Flat ΛCDM | TDCOSMO + Pantheon+ | SLACS | |
| ΛCDM1c | Flat ΛCDM | TDCOSMO + Pantheon+ | SL2S | |
| ΛCDM1d | Flat ΛCDM | TDCOSMO + Pantheon+ | SLACS + SL2S | H0 ∼ 𝒰 (0, 150) km s−1 Mpc−1 |
| ΛCDM2a | Flat ΛCDM | TDCOSMO + DES-SN5YR | – | Ωm ∼ 𝒰 (0.05, 0.5) |
| ΛCDM2b | Flat ΛCDM | TDCOSMO + DES-SN5YR | SLACS + SL2S | |
| ΛCDM3a | Flat ΛCDM | TDCOSMO + DESI BAO | – | |
| ΛCDM3b | Flat ΛCDM | TDCOSMO + DESI BAO | SLACS + SL2S | |
Notes. The group of parameter priors within each row block is used for all cosmological models within that row block.
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