The findings of a nine-orbit calibration plan carried out during HST Cycle 15, to fully determine the NICMOS camera 2 (2.0 !m) polarization calibration to high accuracy, are reported. Recently Ueta et al. and Batcheldor et al. have suggested that NICMOS possesses a residual instrumental polarization at a level of 1.2%–1.5%. This would completely inhibit the data reduction in a number of GO programs, and hamper the ability of the instrument to perform high-accuracy polarimetry. We obtained polarimetric calibration observations of three polarimetric standards at three spacecraft roll angles separated by !60°. Combined with archival data, these observations were used to characterize the residual instrumental polarization in order for NICMOS to reach its full potential of accurate imaging polarimetry at p " 1%. Using these data, we place an 0.6% upper limit on the instrumental polarization and calculate values of the parallel transmission coefficients that reproduce the ground-based results for the polarimetric standards. The uncertainties associated with the parallel transmission coefficients, a result of the photometric repeatability of the observations, are seen to dominate the accuracy of p and ". However, the updated coefficients do allow imaging polarimetry of targets with p " 1:0% at an accuracy of !0:6% and !15°. This work enables a new caliber of science with HST.
Department, Program, or Center
Chester F. Carlson Center for Imaging Science (COS)
Astronomical Society of the Pacific. 121:153-166, 2009 February
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