The Q/U Imaging Experiment: Polarization Measurements of Radio Sources
  at 43 and 95 GHz
  We present polarization measurements of extragalactic radio sources observed
during the Cosmic Microwave Background polarization survey of the Q/U Imaging
Experiment (QUIET), operating at 43 GHz (Q-band) and 95 GHz (W-band). We
examine sources selected at 20 GHz from the public, $>$40 mJy catalog of the
Australia Telescope (AT20G) survey. There are $\sim$480 such sources within
QUIET's four low-foreground survey patches, including the nearby radio galaxies
Centaurus A and Pictor A. The median error on our polarized flux density
measurements is 30--40 mJy per Stokes parameter. At S/N $> 3$ significance, we
detect linear polarization for seven sources in Q-band and six in W-band; only
$1.3 \pm 1.1$ detections per frequency band are expected by chance. For sources
without a detection of polarized emission, we find that half of the sources
have polarization amplitudes below 90 mJy (Q-band) and 106 mJy (W-band), at 95%
confidence. Finally, we compare our polarization measurements to intensity and
polarization measurements of the same sources from the literature. For the four
sources with WMAP and Planck intensity measurements $>1$ Jy, the polarization
fraction are above 1% in both QUIET bands. At high significance, we compute
polarization fractions as much as 10--20% for some sources, but the effects of
source variability may cut that level in half for contemporaneous comparisons.
Our results indicate that simple models---ones that scale a fixed polarization
fraction with frequency---are inadequate to model the behavior of these sources
and their contributions to polarization maps.
