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20032007
most citedOn the variability of quasars: a link between Eddington ratio and optical variability?

140 citations · 406 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph2007140 cited

On the variability of quasars: a link between Eddington ratio and optical variability?

B. C. Wilhite, R. J. Brunner, C. J. Grier +2

Repeat scans by the Sloan Digital Sky Survey (SDSS) of a 278 square degree stripe along the Celestial equator have yielded an average of over 10 observations each for nearly 8,000…

astro-ph200718 cited

The Effect of Variability on the Estimation of Quasar Black Hole Masses

B. C. Wilhite, R. J. Brunner, D. P. Schneider +1

We investigate the time-dependent variations of ultraviolet (UV) black hole mass estimates of quasars in the Sloan Digital Sky Survey (SDSS). From SDSS spectra of 615 high-redshift…

astro-ph2006108 cited

Broad Absorption Line Variability in Repeat Quasar Observations from the Sloan Digital Sky Survey

Britt F. Lundgren, Brian C. Wilhite, Robert J. Brunner +5

We present a time-variability analysis of 29 broad absorption line quasars (BALQSOs) observed in two epochs by the Sloan Digital Sky Survey (SDSS). These spectra are selected from…

astro-ph2005

A Synoptic, Multiwavelength Analysis of a Large Quasar Sample

Adam W. Rengstorf, Robert J. Brunner, Brian C. Wilhite

We present variability and multi-wavelength photometric information for the 933 known quasars in the QUEST Variability Survey. These quasars are grouped into variable and non-varia…

astro-ph2005

Spectral Variability of Quasars in the Sloan Digital Sky Survey. II: The C IV Line

B. C. Wilhite, D. E. Vanden Berk, R. J. Brunner +1

We examine the variability of the high-ionizaton C IV line in a sample of 105 quasars observed at multiple epochs by the Sloan Digital Sky Survey. We find a strong correlation betw…

astro-ph2005

Characteristic QSO Accretion Disk Temperatures from Spectroscopic Continuum Variability

Nicolas A. Pereyra, Daniel E. Vanden Berk, David A. Turnshek +5

Using Sloan Digital Sky Survey (SDSS) quasar spectra taken at multiple epochs, we find that the composite flux density differences in the rest frame wavelength range 1300-6000 AA c…