Continuum Variability of Active Galactic Nuclei in the Optical-UV Range
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 $U$, $B_J$, $F$ and $N$ bands with the Mayall 4m telescope at Kitt Peak. Changes $δα$ of the spectral slope $α$ appear correlated with brightness variations $δlog f_ν$ 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 $δα- δlog f_ν$ relation is consistent with the spectral change due to temperature variation of a black body of about $2.5 \cdot 10^4 K$.
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