Smith et al. 2004), and a handful of objects where optical longslit echelle data from CTIO (Danforth 2003) indicated high velocity emission in H$\alpha$ but for which no previous SNR identification had been suggested. Such objects may represent SNRs ‘buried’ in H II regions that have not heretofore called attention to themselves, similar to the SMC SNR 0057-7226 mentioned earlier. We culled this list by removing objects previously observed with $\fuse$ (see Table 1) and a small subset for which optical extinction measurements or X-ray derived neutral hydrogen column densities indicated severe attenuation of any potential FUV emission. Finally, a selection of six SNRs newly identified in the Magellanic Cloud Emission Line Survey (MCELS) team (Smith et al. 2004) were added in the second year of the survey. Our final list contained 39 objects in the LMC and 11 objects in the SMC. The observations reported below took place over two observing cycles, using $\fuse$ program identifiers D904 (44 LMC and SMC remnants) and E900 (six new MCELS objects in the LMC).

The $\fuse$ instrument covers the wavelength range 905 – 1187 Å, with a nominal point source resolution R = $\lambda/\Delta\lambda ~ \ge$ 20,000. For diffuse sources of interest 