The Multiband Imaging Photometer for Spitzer (MIPS) provides long-wavelength capability for the mission in imaging bands at 24, 70, and 160 µm and measurements of spectral energy distributions between 52 and 100 µm at a spectral resolution of about 7%. By using true detector arrays in each band, it provides both critical sampling of the Spitzer point-spread function and relatively large imaging fields of view, allowing for substantial advances in sensitivity, angular resolution, and efficiency of areal coverage compared with previous space far-infrared capabilities. The 24 µm array has excellent photometric properties, and measurements with rms relative errors of about 1% can be obtained. The two longer-wavelength arrays use detectors with poor photometric stability, but a system of onboard stimulators used for relative calibration, combined with a unique data pipeline, produce good photometry with rms relative errors of less than 10%.
ADS Citation Query
# citations = 824
average # citations/year = 117.71
(# years = 7)
# citations vs. year [year=citations]
[2010=129]
[2009=185]
[2008=149]
[2007=137]
[2006=130]
[2005=48]
[2004=43]
[determined from ADS on 10 Sep 2010]
Copyright © 2001-2006
Karl D. Gordon
All Rights Reserved