The radial dependence of temperature and iron abundance - Galaxy clusters from z = 0.14 to z = 0.89

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Table 7:

The eight subsets of the sample used to calculate average temperature and iron abundance profiles.
Classification of Subsets
subset #	redshift	temperature	cooling	number
1	z<0.4	<6.8 keV	Yes	6/6
2	z<0.4	$\geq$ 6.8 keV	Yes	4/4
3	z<0.4	<6.8 keV	No	3/3
4	z<0.4	$\geq$ 6.8 keV	No	4/4
5	z>0.4	<6.8 keV	Yes	2/2
6	z>0.4	$\geq$ 6.8 keV	Yes	2/2
7	z>0.4	<6.8 keV	No	5/3
8	z>0.4	$\geq$ 6.8 keV	No	9/7

The two values in the number column represent the number of observations
and the number of unique clusters in that sample, respectively.

Source LaTeX | All tables | In the text

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