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astro-ph200771 cited

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

Zhaohui Shang, Beverley J. Wills, D. Wills +1

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-f…

astro-ph2004

Principal Component Analysis of AGN Spectra

Zhaohui Shang, Beverley J. Wills

We discuss spectral principal component analysis (SPCA) and show examples of its application in analyzing AGN spectra in both small and large samples. It can be used to identify pe…

astro-ph2003

Indicators of Black Hole Mass and Eddington Accretion Ratio from QSO X-ray and UV Spectra

Beverley J. Wills, Zhaohui Shang

The evolution of luminous QSOs is linked to the evolution of massive galaxies. We know this because the relic black-holes found locally have masses dependent on the properties of t…

astro-ph2001

HST Ultraviolet and Ground-based Optical Spectropolarimetry of IRAS QSOs: Dusty Scattering in Luminous AGN

D. C. Hines, G. D. Schmidt, K. D. Gordon +4

We present UV and optical spectropolarimetry of two highly polarized IRAS-selected QSOs, IRAS 13349+2438 and the BALQSO IRAS 14026+4341. The polarization in both objects rises rapi…

astro-ph1999

X-ray Absorption in Radio-Quiet QSOs

W. N. Brandt, S. C. Gallagher, A. Laor +1

Major flows of ionized gas are thought to be present in the nuclei of most luminous QSOs, and absorption by these flows often has a significant effect upon the observed X-ray conti…

astro-ph1999

Introduction to Unified Schemes

Beverley J. Wills

The differences among apparently diverse classes of AGN are mainly the result of viewing the central engine at different orientations, because dust, which absorbs and scatters the…