Fig. 4.
LX–TX relation for a sample of groups and clusters at low and intermediate redshift (z ≲ 0.3) from Kundert et al. (2015, their Fig. 5) and Zou et al. (2016, also their Fig. 5). MKW 4s is shown for comparison. The pink shaded area and the red line correspond to the fit by Zou et al. (2016) and the black dashed line is the fit from Kundert et al. (2015).
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