Submillimeter polarization and variability of quasar PKS 1830-211
  Polarization from active galactic nuclei is interpreted as a signpost of the
role of magnetic fields in the launch and collimation of their relativistic
radio jets. Here, we report the detection of a clear polarization signal from
ALMA observations of the gravitationally lensed quasar PKS 1830-211 at
submillimeter wavelengths (Band 9, 650 GHz). Applying a
differential-polarimetry technique to the two compact lensed images of the
quasar, we estimate a fractional polarization of ~5% for one lensed image,
while the other appears nearly unpolarized, which implies that the polarization
activity varies on a timescale of a few weeks. With additional ALMA Band 7 and
8 (between 300-500 GHz) concomitant data, we constrain a Faraday rotation of a
few $10^5$ rad m$^{-2}$. We also observe flux-density variability of ~10%
within one hour in Band 9. This work illustrates that a differential analysis
can extract high-accuracy information (flux-density ratio and polarimetry) free
of calibration issues from resolved sources in the submillimeter domain.
