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Fig. 14

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ALMA and CONCERTO measurements for quasars. The ALMA fluxes in LF and HF are deduced from ALMA band 3 and 7 measurements (See Sect. 8.3 for details). CONCERTO and ALMA fluxes are colour corrected to a fixed effective frequency, which is derived using Uranus SED (veffUranus )$\left( {v_{{\rm{eff}}}^{{\rm{Uranus}}}} \right)$. The first-order polynomial fitting (dashed lines) gives Jy-to-Hz calibration factors of 24.7±0.4 Hz (Jybeam–1)–1 and 18.8±0.4 Hz (Jybeam–1)–1, for LF and HF, respectively.

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