CIV λ1549 as an eigenvector 1 parameter for active galactic nuclei

We are exploring a spectroscopic unification for all types of broad-line emitting AGNs. The four-dimensional Eigenvector 1 (4DE1) parameter space organizes quasar diversity in a sequence primarily governed by Eddington ratio. This paper considers the role of C iv lambda 1549 measures as 4DE1 diagnostics. We use HST archival spectra for 130 sources with S/N high enough to permit reliable C iv lambda 1549 broad-componentmeasures. We find a C iv lambda 1549(BC) profile blueshift that is strongly concentrated among ( largely radio-quiet [RQ]) sources with FWHM( H beta(BC)) less than or similar to 4000 km s(-1) ( which we call Population A). Narrow-line Seyfert 1 (NLSy1; with FWHM H beta <= 2000 km s(-1)) sources belong to this population but do not emerge as a distinct class. The systematic blueshift, widely interpreted as arising in a disk wind/outflow, is not observed in broader line AGNs (including most radio-loud [RL] sources), which we call Population B. We find new correlations involving FWHM( C iv lambda 1549(BC)), C iv lambda 1549 line shift, and equivalent width only among Population A sources. Sulentic et al. suggested C iv lambda 1549 measures enhance an apparent dichotomy between sources with FWHM(H beta(BC)) less and greater than 4000 km s-1, suggesting that it has more significance in the context of broad-line region structure than the more commonly discussed RL versus RQ dichotomy. Black hole masses computed from FWHM C iv lambda 1549(BC) for about 80 AGNs indicate that the C iv lambda 1549 width is a poor virial estimator. Comparison of mass estimates derived from H beta(BC) and C iv lambda 1549 reveals that the latter show different and nonlinear offsets for Population A and B sources. A significant number of sources also show narrow-line C iv lambda 1549 emission that must be removed before C iv lambda 1549(BC) measures can be made and interpreted effectively. We present a recipe for C iv lambda 1549 narrow-component extraction.