The Multiband Imaging Photometer for Spitzer (MIPS)
Author(s) -
G. H. Rieke,
Erick T. Young,
C. W. Engelbracht,
Douglas Kelly,
F. J. Low,
E. E. Haller,
Jeffrey W. Beeman,
Karl D. Gordon,
J. A. Stansberry,
K. A. Misselt,
James Cadien,
Jane Morrison,
G. Rivlis,
William B. Latter,
A. NoriegaCrespo,
Deborah Padgett,
Karl R. Stapelfeldt,
Dean C. Hines,
Eiichi Egami,
James Muzerolle,
A. AlonsoHerrero,
Myra Blaylock,
H. Dole,
J. L. Hinz,
E. Le Floc’h,
Casey Papovich,
Pablo G. PérezGonzález,
Paul S. Smith,
K. Y. L. Su,
Lee Bennett,
D. T. Frayer,
David Henderson,
N. Lu,
Frank J. Masci,
Meyer Z. Pesenson,
L. M. Rebull,
Jeonghee Rho,
J. Keene,
S. Stolovy,
Stefanie Wachter,
W. A. Wheaton,
M. W. Werner,
P. L. Richards
Publication year - 2004
Publication title -
the astrophysical journal supplement series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 3.546
H-Index - 277
eISSN - 1538-4365
pISSN - 0067-0049
DOI - 10.1086/422717
Subject(s) - photometer , photometry (optics) , optics , physics , detector , wavelength , calibration , remote sensing , angular resolution (graph drawing) , near infrared spectroscopy , astrophysics , stars , mathematics , geology , quantum mechanics , combinatorics
The Multiband Imaging Photometer for Spitzer (MIPS) provides long-wavelength capability for the mission in imaging bands at 24, 70, and 160 ?m and measurements of spectral energy distributions between 52 and 100 ?m 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 ?m 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%.
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