Structure of the extended emission in the infrared celestial background

Details Structure of the extended emission in the infrared celestial background Structure of the extended emission in the infrared celestial background

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986spie..685..167p&link_type=abstract

IN: Infrared technology XII; Proceedings of the Meeting, San Diego, CA, Aug. 19, 20, 1986 (A88-12828 02-35). Bellingham, WA, Soc

Astronomy and Astrophysics

Astronomy

Infrared Astronomy Satellite, Interstellar Matter, Thermal Radiation, Zodiacal Light, Cosmic Dust, Cryogenic Equipment, Solar System, Spaceborne Telescopes, Stellar Envelopes

Scientific paper

Extended celestial background IR emission, which encompasses the zodiacal background, the large discrete sources in the galaxy, and the interstellar dust, presents a varied field for a space-based cryogenic, long-wavelength IR telescope system. Dust arcs, comet trails, and asteroids in the solar system constitute moving sources of spurious signals for area surveys. The highly structured and filigreed background due to structure in molecular clouds, H II regions, and IR cirrus could represent a source of scan noise and spurious signals, due to field rotation and scan aspect.

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