paper

Continuum Variability of Active Galactic Nuclei in the Optical-UV Range

arXiv:astro-ph/0012408 · doi:10.1086/320055

Abstract

The variability of the continuum spectral energy distribution has been analyzed for a complete magnitude-limited sample of quasars in Selected Area 57, observed at two epochs in the photographic , , and bands with the Mayall 4m telescope at Kitt Peak. Changes of the spectral slope appear correlated with brightness variations indicating an average hardening of the spectrum in the bright phases. This confirms that the correlation of variability with redshift, found in a single observing band, is due to intrinsic spectral changes. The average observed relation is consistent with the spectral change due to temperature variation of a black body of about .

30 pages, 6 figures, to appear in ApJ (2001)

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