  This paper joins a series compiling consistent emission line measurements of
large AGN spectral databases, useful for reliable statistical studies of
emission line properties. It is preceded by emission line measurements of 993
spectra from the Large Bright Quasar Survey (Forster et al. 2001) and 174
spectra of AGN obtained from the Faint Object Spectrograph (FOS) on HST prior
to the installation of COSTAR (Kuraszkiewicz et al. 2002). This time we
concentrate on 220 spectra obtained with the FOS after the installation of
COSTAR, completing the emission line analysis of all FOS archival spectra. We
use the same automated technique as in previous papers, which accounts for
Galactic extinction, models blended optical and UV iron emission, includes
Galactic and intrinsic absorption lines and models emission lines using
multiple Gaussians. We present UV and optical emission line parameters
(equivalent widths, fluxes, FWHM, line positions) for a large number (28) of
emission lines including upper limits for undetected lines. Further scientific
analyses will be presented in subsequent papers.
