the data are maintained as a photon list: the intermediate data file - IDF. Bad photons are flagged but not discarded, so the user can examine and combined data without re-running CalFUSE. For each target, we combined the individual exposures (using the IDF files) and channels to create a time-averaged spectrum weighted in the flux in each output datum by the exposure time and sensitivity of the input exposure and channel of origin. The details are given here. The spectral regions covered by the spectral channels overlap, and these overlap regions are then used to renormalize the spectra in the SiC1, LiF2, and SiC2 channels to the flux in the LiF1 channel. We then produce a final spectrum that covers almost the full [*[FUSE]{}*]{} wavelength range $905-1182$Å. The low sensitivity portions of each channel are discarded. In most channels there exists a narrow dark stripe of decreased flux in the spectra running in the dispersion direction. This stripe has been affectionately known as the ”worm” and it can attenuate as much as 50% of the incident light in the affected portions of the spectrum. The worm has been observed to move as much as 2000 pixels during a single orbit 