Spectral Properties From Lyman-alpha to H-alpha For An Essentially Complete Sample of Quasars I: Data

Details Spectral Properties From Lyman-alpha to H-alpha For An Essentially Complete Sample of Quasars I: Data Spectral Properties From Lyman-alpha to H-alpha For An Essentially Complete Sample of Quasars I: Data

2007-03-27

arxiv.org/abs/astro-ph/0703690v3

Astron.J.134:294-313,2007

Astronomy and Astrophysics

Astrophysics

42 pages, 10 figures, 13 tables. Accepted by AJ. Supplemental figures not included. Full version available at http://physics

Scientific paper

10.1086/518505

We have obtained quasi-simultaneous ultraviolet-optical spectra for 22 out of 23 quasars in the complete PG-X-ray sample with redshift, z<0.4, and M_B<-23. The spectra cover rest-frame wavelengths from at least Lyman-alpha to H-alpha. Here we provide a detailed description of the data, including careful spectrophotometry and redshift determination. We also present direct measurements of the continua, strong emission lines and features, including Lyman-alpha, SiIV+OIV], CIV, CIII], SiIII], MgII, H-beta, [OIII], He5876+NaI5890,5896, H-alpha, and blended iron emission in the UV and optical. The widths, asymmetries and velocity shifts of profiles of strong emission lines show that CIV and Lyman-alpha are very different from H-beta and H-alpha. This suggests that the motion of the broad line region is related to the ionization structure, but the data appears not agree with the radially stratified ionization structure supported by reverberation mapping studies, and therefore suggest that outflows contribute additional velocity components to the broad emission line profiles.

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