Any merger effects will be traced. Searchs for other structures, especially any which may funnel the gas to the nucleus, will be made. Observations 03 and 04 had a few saturated pixels in the core of the target. There was also a loss of lock during observation 03 which reduced the exposure time by 6.5 seconds, and there was one 7 second recentering during observation 07. The stability of the FOS Blue side wavelength scale and spectral locations will be measured.
All observations are internals.
This is a WFPC snapshot survey of 100 radio galaxies and QSOs in the 3CR catalog. Most of the exposures will use the Linear Ramp Filter. The purpose is to study the morphology of the radio galaxies. The first two sets of observations each show a weak object off-center in WF2 and WF4, respectively, which were the targeted chips. It is unclear if these are the intended targets 3C93.0 and 3C289.0.