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Published online by Cambridge University Press: 04 August 2017
The results discussed here are based on observations at λ 1 mm of 36 optically selected quasars (Sherwood et al., 1982; in preparation) and of 24 flat spectrum radio sources with Sν (5 GHz) ≥ 1 Jy (Kühr et al., 1979, 1981). H = 50 km/(s Mpc) and qo = 0 are used.