3. These measurements have been made with IDL tools that permit user interaction in the measurements. Each spectrum is displayed and a cursor is used to set limits around each line for integrating the flux above the background for each feature. Since most of the line profiles are distinctly non-Gaussian, the fluxes derived in this way are simply integrated flux above background, not the equivalent flux for a Gaussian fit. These measurements are only lower limits to the actual fluxes since unknown but potentially significant amounts of emission are apparently absorbed by foreground ISM. (See discussion below.) The full-width-zero-intensity (FWZI) values listed in Table 3 indicate the full range over which the integration was made. The values listed in Table 3 are all significantly above the value expected for a filled LWRS aperture, indicating that intrinsic line broadening is detected in all cases. The central velocities listed are not the centroid of measured flux, but rather the center of the FWZI velocity range used. Two things are immediately obvious from inspection of Table 3. For all objects with both O VI and C III lines, the central velocities for C III are more redshifted than for O VI, and the 