Optical/UV Quasar Continuum Variability: Time Lag, Luminosity, Wavelength, Redshift, Radio, X-Ray, and BAL Dependence

Details Optical/UV Quasar Continuum Variability: Time Lag, Luminosity, Wavelength, Redshift, Radio, X-Ray, and BAL Dependence Optical/UV Quasar Continuum Variability: Time Lag, Luminosity, Wavelength, Redshift, Radio, X-Ray, and BAL Dependence

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..311..385w&link_type=abstract

AGN Physics with the Sloan Digital Sky Survey, Proceedings of a conference held in Princeton, NJ, USA, 27-31 July 2003, Edited b

Physics

Scientific paper

Using a sample of over 25,000 spectroscopically confirmed quasars from
the Sloan Digital Sky Survey, we show how quasar variability in the
optical/UV regime depends upon rest-frame time lag, luminosity, rest
wavelength, redshift, the presence of radio and X-ray emission, and the
presence of broad absorption line systems.

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