VizieR Online Data Catalog: Chemical evolution of galaxy clusters (Liu+, 2020)

The amount of mass in iron was measured in a sample of galaxy clusters observed with Chandra. We select 186 morphologically regular clusters in the redshift range of [0.04, 1.07] from deep and medium-deep Chandra archival observations as of February 2019.

The global properties of the clusters, including the X-ray redshift, the global temperature, the value of r500 and M500, where derived. The X-ray redshift is measured by fitting the spectrum of the global emission within the radius maximizing the signal to noise ratio in the 0.5-7keV band image. Among the 186 clusters in the sample, 184 have optical spectroscopic redshifts published in the literature.

(1 data file).