An upgrade of the IF polarimeter [16] is now available, where the cross correlation between the IF signals from a pair of orthogonally polarized receivers is made digitally in VESPA. The new observing procedure XPOL generates simultaneous spectra of all 4 Stokes parameters. The following combinations of spectral resolution (KHz) and bandwidth (MHz) are available: 40/120, 80/240, 320/480, and 1250/640.
Although successful XPOL observations were made at several frequencies, experience is still limited, particularly with respect to long integrations and observations of extended sources. Data reduction software using CLASS enhanced with a graphical user interface is available (H. Wiesemeyer). A short guide (at ./IRAMFR/PV/veleta.html) describes XPOL observations. Polarimetry proposals will be considered with the restriction that the target sources be not larger than the main beam.