All Tables

Table 1: Fluxes and other parameters of the quasar sample. The total submm fluxes are from Willott et al. (2002), observed between March 1999 and April 2001. Column 7 lists the thermal contribution at 1.25 mm derived from a dust model fitted to the submm data, as explained in Sect. 3.1.1 and shown in Fig. 2. Column 8 lists the synchrotron contribution at 1.25 mm, as total minus thermal contribution (Cols. 3-7) and Col. 9 lists the synchrotron fraction in percent. The spectral indices $\alpha$ $_{\rm cm-mm}$ are determined for most sources between 6 cm and 1.25 mm with an accuracy of better than 5%; more details are given in Sect. 3.1.2. These spectral indices are used to extrapolate from longer wavelength data the 450 and 850 $\mu$ m synchrotron fluxes listed in Cols. 11 and 12.
Table 2: Parameters of the comparison radio galaxy sample of Willott et al. (2002): Spectral indices, $\alpha$ $_{\rm cm}$ , fitted to the total cm wavelengh data with an accuracy of about 5%. Via $F_\nu \propto \nu ^{\alpha }$ the 850 $\mu$ m synchrotron fluxes are extrapolated from the cm fluxes with a formal uncertainty of about 30-40%.