Group 614 of 02 contains fill data and is useless. Individual groups contain few counts, but the sum of many groups should produce adequate spectra. The count rates suggest that the principal source of UV light was eclipsed during 01 and remained in eclipse throughout 02. Measurements of the instrumental background of both FOS detectors will be made. The proposal will execute 7 times during cycle 6.
All exposures are internals.
All spectra are image mode. These calibration spectra were not displayed. They appear to have been carried out as planned. These data will allow a study of the optical properties of an unbiased sample of AGN host galaxies. The data will provide information on the structure of the inner regions of the AGN nuclei.