[1] The goal was to obtain brightness maps of the universe at ten frequency bands ranging from the near to far infrared (1.25 to 240 micrometer).
[1] During the mission, the instrument could sample half the celestial sphere each day.
The spacecraft contained liquid helium that cooled the DIRBE instrument to below 2K to allow it to image in the infrared wavelengths.
After that date only observations in the 1.25 to 4.9 micrometer bands could be carried out, at about 20% of original sensitivity.
[2] The DIRBE instrument was an absolute radiometer with an off-axis folded-Gregorian reflecting telescope, with 19 cm diameter aperture.