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The Elvis 1994 AGN template has been phenomenally successful at matching the SEDs of the vast majority of Type-1 quasars from the local Universe to z~6. Nonetheless, a population of hot-dust-poor or hot-dust-free quasars has been found both at intermediate and high-z. Estimates of the numbers of these anomalous quasars vary widely, along with speculations on their place in quasar evolution, e.g., whether they are related to the early growth of the black holes. To answer some of these questions,doi:10.5281/zenodo.60529 fatcat:3vdkubpmcfbyhntjmsdzcvlfrq