Fig. 11
SED for the quasars 3C 286 (left) and 3C 273 (right). We consider data from Planck (black dot, Planck Collaboration I 2014); ALMA (black diamond, Fomalont et al. 2014); XPOl (black triangle, Agudo et al. 2012) and NIKA (blue dot, this paper). For the fit, a color correction of 5% and 6% at 260 GHz and 150 GHz, respectively, has been considered for both quasars.
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