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What is Quasar 3C298: Nanodiamond Emission Study about?

This document discusses the potential detection of meteoritic nanodiamonds in the quasar 3C298 based on their expected infrared emission signatures. The authors calculate the expected dust emission at 3.43 and 3.53 microns if hydrogenated nanodiamonds are responsible for the observed far-ultraviolet break in quasars. Using Spitzer Observatory data of 3C298, they do not find evidence for these emission bands. They conclude that while pure nanodiamonds may still explain the far-UV break, hydrogenated nanodiam

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