  A new determination of the upper limit to the cosmic diffuse background
radiation, at ~110 nm, of 300 photons s-1 cm-2 sr-1 nm-1, is placed in the
context of diffuse background measurements across the entire electromagnetic
spectrum, including new optical, infrared, visible, and gamma-ray background
measurements. The possibility that observed excess diffuse visible radiation is
due to redshifted cosmological Lyman alpha recomination radiation is explored.
Also, a new standard of units for the display of spectra is advocated.
