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Fig. 8
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Specific radio luminosity, Lν,R, as a function of bolometric luminosity, Lbol, for the SMGPS-RASS, eRASS1 sources. The solid and dashed lines, and markers are the same as in Fig. 7. The blue and red lines in both panels are the power-law fit for RASS and eRASS1, respectively.
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