ultraviolet interpolation

Schiminovich came down again and we got a bit more done on the ultraviolet background, working on the distribution of intensity as a function of quasar (source object) redshift. We haven't yet faced the need to K-correct the intensity information we have collected, but we will have to face that soon. We confirm, disturbingly well in some respects, models of the intergalactic ultraviolet intensity as a function of redshift.

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