Fig. B.1
Iron abundance vs. temperature for the 62 clusters. The black line denotes our best power-law fit using the bisector method. The dot-dashed line is the best fit in Balestra et al. (2007) for clusters at higher redshifts (z ≥ 0.3) and in a higher temperature range (3–15 keV). The colors and symbols have the same meaning as those in Fig. 3.
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