Polarization observations of the radio cores of AGN — I. A sample of quasars

We present total‐intensity and linear‐polarization observations at a single epoch for a sample of 11 quasars and one BL Lac object. The data were taken with the VLA A array at λλ 20, 18, 6 and 2 cm. We examine the variation of the degree of polarization, p , and polarization position angle, PA, with wavelength, and attempt to determine the rotation measure, RM, of the cores in these sources. The degree of polarization does not exhibit any systematic variation with wavelength, the median values ranging from 2.3 to 3.5 per cent at the different wavelengths. The variation of PA with λ 2 is not linear over the entire wavelength range. However, for most sources the λλ 20‐, 18‐ and 6‐cm PAs do follow such a linear relationship, yielding a median |RM| of about 15 rad m −2 . In contrast, the λλ 6‐ and 2‐cm observations give a median |RM| of about 129 rad m −2 . The long‐wavelength emission is likely to originate from a spatially different part of the milliarcsec‐scale jet from the λ 2‐cm emission, which could turn over at a higher frequency and is likely to be more compact and located closer to the quasar nucleus. We have attempted to obtain linear fits over the entire wavelength range allowing for n  π ambiguities in the PAs, but the fits are not statistically significant. The low values of RM for these core‐dominated sources suggest that either the radio emission from the jet intercepts few of the emission‐line clouds and their confining medium, or the clouds have a small filling factor and are possibly magnetically confined.