Mean SEDs of z<0.75 quasars redden in MIR/NIR/UV with rising Eddington ratio but blue in optical, showing accretion-rate dependence of Type 1 AGN emission.
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The Dependence of the Mean Spectral Energy Distributions on the Accretion Rate for Quasars with $z < 0.75$ from the Sloan Digital Sky Survey
Mean SEDs of z<0.75 quasars redden in MIR/NIR/UV with rising Eddington ratio but blue in optical, showing accretion-rate dependence of Type 1 AGN emission.