Fig. A.1.
Distribution of kinetic luminosities of all RL AGN in XXL-S using different scaling relations. The relations from Godfrey & Shabala (2013) for FRI and FRII sources are similar to the relation from Cavagnolo et al. (2010) (which is similar to Merloni & Heinz 2007 and O’Sullivan et al. 2011), but this apparent agreement is due to the similar distance dependence of jet-power measurement techniques used for FRI and FRII radio galaxies in these samples.
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