Diffuse Background Radiation

Published 1999 March 25 © 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Richard C. Henry 1999 ApJ 516 L49 DOI 10.1086/312003

1538-4357/516/2/L49

Abstract

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 Lyα recombination radiation is explored. Also, a new standard of units for the display of spectra is advocated.

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10.1086/312003