The Infrared Array Camera (IRAC) for the Spitzer Space Telescope

dc.creatorFazio, G. G.
dc.creatorteam, the IRAC
dc.date2004-05-31
dc.date.accessioned2026-07-07T11:29:24Z
dc.date.available2026-07-07T11:29:24Z
dc.descriptionThe Infrared Array Camera (IRAC) is one of three focal plane instruments in the Spitzer Space Telescope. IRAC is a four-channel camera that obtains simultaneous broad-band images at 3.6, 4.5, 5.8, and 8.0 microns. Two nearly adjacent 5.2x5.2 arcmin fields of view in the focal plane are viewed by the four channels in pairs (3.6 and 5.8 microns; 4.5 and 8 microns). All four detector arrays in the camera are 256x256 pixels in size, with the two shorter wavelength channels using InSb and the two longer wavelength channels using Si:As IBC detectors. IRAC is a powerful survey instrument because of its high sensitivity, large field of view, and four-color imaging. This paper summarizes the in-flight scientific, technical, and operational performance of IRAC.
dc.description7 pages, 3 figures. Accepted for publication in the ApJS. A higher resolution version is at http://cfa-www.harvard.edu/irac/publications
dc.identifierhttps://arxiv.org/abs/astro-ph/0405616
dc.identifierhttp://arxiv.org/abs/astro-ph/0405616
dc.identifierAstrophys.J.Suppl.154:10-17,2004
dc.identifierdoi:10.1086/422843
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/196701
dc.subjectAstrophysics
dc.titleThe Infrared Array Camera (IRAC) for the Spitzer Space Telescope
dc.typetext

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