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Table 1.
Summary of the cosmological probes and parameters present in the different cases considered.
| Case | Cosmological probes | Cosmological parameters | Nuisance parameters |
|---|---|---|---|
| SNIa | SNIa | hi | α, β, M, ΔM |
| SNIa+BAO free H0rd | SNIa+BAO | hi, H0rd | α, β, M, ΔM |
| SNIa+ev+BAO free H0rd | SNIa+BAO | hi, H0rd | α, β, M, ΔM, ϵ, δ |
| SNIa+BAO prior rd | SNIa+BAO | hi, H0, rd | α, β, M, ΔM |
| SNIa+ev+BAO prior rd | SNIa+BAO | hi, H0, rd | α, β, M, ΔM, ϵ, δ |
| SNIa+BAO free rd+CMB | SNIa+BAO+CMB | hi, H0, rd, Ωm, ωb | α, β, M, ΔM, zCMB |
| SNIa+ev+BAO free rd+CMB | SNIa+BAO+CMB | hi, H0, rd, Ωm, ωb | α, β, M, ΔM, zCMB, ϵ, δ |
| SNIa+BAO prior rd+CMB | SNIa+BAO+CMB | hi, H0, rd, Ωm, ωb | α, β, M, ΔM, zCMB |
| SNIa+ev+BAO prior rd+CMB | SNIa+BAO+CMB | hi, H0, rd, Ωm, ωb | α, β, M, ΔM, zCMB, ϵ, δ |
| SNIa+BAO compute rd+CMB | SNIa+BAO+CMB | hi, H0, Ωm, ωb | α, β, M, ΔM, zCMB, zdrag |
| SNIa+ev+BAO compute rd+CMB | SNIa+BAO+CMB | hi, H0, Ωm, ωb | α, β, M, ΔM, zCMB, zdragϵ, δ |
Notes. The i-index on hi goes from 1 to 5 for SNIa data alone, while it goes up to 6 when BAO data are included. When working with coasting reconstructions we only consider the last two knots hi.
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