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We aim to observe 7 targets in M33 with COS. Unfortunately, M33 has a large amount of diffuse structure, especially at the 5'' beam of GALEX, and so it is difficult to use the standard GALEX AIS to clear these targets. We wish to use the existing data, consisting of FUSE spectra of each target, and deep NGS GALEX imaging to a) clear the targets from dangerously bright objects and b) get the best guess as to the flux from these targets to use for flux estimation for buffer timing and SNR estimation.