The far-UV diffuse background revisited

Details The far-UV diffuse background revisited The far-UV diffuse background revisited

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...246..243p&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 246, no. 1, June 1991, p. 243-248.

Astronomy and Astrophysics

Astronomy

10

Background Radiation, Diffuse Radiation, Far Ultraviolet Radiation, Sky Surveys (Astronomy), Spaceborne Astronomy, Cosmic Dust, Interstellar Gas, Ionized Gases, Ultraviolet Spectrophotometers

Scientific paper

A new reduction is presented of the high-galactic latitude whole-sky survey obtained with the D2B-AURA satellite at 1690 A. This reduction differs in several ways from the previously published one (Joubert et al., 1983), especially by a correction for gain variations with time which had remained unnoticed in the first reduction. The existence of a correlation between the UV sky background and gas and dust is confirmed. There are no clear local excesses at large scale of UV radiation with respect to the mean relations UV versus gas or dust column densities.

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