Augmenting the power of time-delay cosmography in lens galaxy clusters by probing their member galaxies - II. Cosmic chronometers

Open Access

Table 1.

Intervals at the 68% confidence level for the values of the cosmological parameters obtained with the Bayesian method.

		Flat-ΛCDM ^(a)		Open-wCDM
Err. ^(b)D_Δt	Err. ^(b)H(z_d)	H₀^(c)	Ω_m	H₀^(c)	Ω_m	Ω_de	w
5%	10%
5%	20%
10%	10%
10%	20%

Notes.

^(a)

Ω_m + Ω_de = 1 and w = −1.

^(b)

Adopted percentage relative errors.

^(c)

(km s⁻¹ Mpc⁻¹).

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