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Observations were made with the NASA/European Space Agency HST and obtained from the data archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, under NASA contract NAS 5-26S5S. These observations are associated with program GO9733. This work is also based on observations obtained with the Gemini Telescope. We acknowledge the support given by ASTROVIRTEL, a project funded by the European Commission under FP5 contract no. HPRI-CT-1999-00081. J.R.M., M.A.H., and S.J.S. thank Partide Physics and Astronomy Research Council for financial support, and S.M. acknowledges the "Physics of Type la SNe" Research Training Network under contract HPRN-CT-2002-00303. We thank B. Januszewski for help in coordinating and executing the HST observations and P. Meikle and R. Kotak for assistance, advice, and reading of the manuscript.
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