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Proceedings Paper

Sensitivity model for the wide-field infrared explorer mission
Author(s): John C. Kemp; Roy W. Esplin; Perry B. Hacking
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Paper Abstract

The wide-field infrared explorer (WIRE) is a cryogenically cooled infrared telescope being prepared to study the evolution of starburst galaxies. The WIRE instrument will measure the infrared energy in two broad bands. Two 128- by 128-pixel arsenic-doped silicon focal plane arrays detect the galactic emissions. We provide a sensitivity analysis for the long wavelength band, 21 to 27 micrometers , including NEP for a single element. Ultimate flux sensitivity is limited by imaging resolution which includes the effects of diffraction, spacecraft jitter, and sampling of the point spread fuction. Observation times to obtain these confusion limited measurements are provided. Ground characterization and on-orbit calibration measurements are outlined, as is the simulation plan.

Paper Details

Date Published: 29 September 1995
PDF: 12 pages
Proc. SPIE 2553, Infrared Spaceborne Remote Sensing III, (29 September 1995); doi: 10.1117/12.221359
Show Author Affiliations
John C. Kemp, Utah State Univ. (United States)
Roy W. Esplin, Utah State Univ. (United States)
Perry B. Hacking, Jamieson Science and Engineering (United States)

Published in SPIE Proceedings Vol. 2553:
Infrared Spaceborne Remote Sensing III
Marija Strojnik; Bjorn F. Andresen, Editor(s)

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