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Spectral Variability of Quasars in the Sloan Digital Sky Survey. I. Wavelength Dependence

  • Authors: Brian C. Wilhite, Daniel E. Vanden Berk, Richard G. Kron, Donald P. Schneider, Nicholas Pereyra, Robert J. Brunner, Gordon T. Richards, and Jonathan V. Brinkmann

Wilhite et al. 2005 The Astrophysical Journal 633 638.

  • Provider: AAS Journals

Caption: Fig. 12.

Top: Bright‐ (black line) and faint‐phase (gray line) arithmetic mean composite spectra for the 315 objects in the final variable quasar sample. As both composites were created from quasar spectra scaled to a value of 1 at 3060 Å, only relative color changes are meaningful. Both spectra are boxcar smoothed with a smoothing length of 20 pixels. Bottom: Ratio of bright‐phase composite to faint‐phase composite as a function of wavelength.

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