The Robert Stobie Spectrograph (RSS) is an imaging spectrograph designed to occupy the Prime Focus Instrument Package of the Southern African Large Telescope (SALT). Grating spectropolarimetry, 3200 - 9000 ˚A, with resolution R up to 10 000, is always available, using rotating half and quarter waveplates near the telescope focal plane and a calcite mosaic beamsplitter in the collimated space. This paper describes improvements made to the polarimetric calibration to correct for an unexpected time-dependent position angle ‘ripple’ vs wavelength which has been seen in high-precision RSS observations, and which appears to be due to variations in illumination of the pupil during an observation. A new calibration technique, which explicitly models the pupil dependence of the polarimetric sensitivity, has been developed. The net spectral polarization sensitivity vs field of view position X, Y , and wavelength λ is computed as the polarization pupil dependence, weighted by the pupil intensity illumination of the observation. We find that the polarization pupil dependence, degree P and position angle θ are adequately represented by a polynomial function of position in the pupil. A pupil intensity illumination model for SALT has been devised, calibrated by twilight observations through a pinhole slitmask grid, observed out of focus. The polarization pupil dependence model has been calibrated using observations of the full Moon through a similar mask, plus a polaroid. The final calibration has been checked using repeated observations of known highly polarized standard stars.
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