A new H(z=0.542) measurement of 66 with large uncertainties is derived from the age-redshift trend of 38 passive galaxies in three clusters.
We used archivalHubbleSpace Telescope (HST) multi- colour imaging from the Advanced Camera for Surveys (ACS) and the Wide Field Camera 3 (WFC3)
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Cosmic chronometers with galaxy clusters: a new avenue for multi-probe cosmology
A new H(z=0.542) measurement of 66 with large uncertainties is derived from the age-redshift trend of 38 passive galaxies in three clusters.