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The Multiband Imaging Photometer for Spitzer (MIPS)

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Rieke, G. H., Young, E. T., Engelbracht, C. W., Kelly, D. M., Low, F. J., Haller, E. E., Beeman, J. W., Gordon, K. D., Stansberry, J. A., Misselt, K. A., Cadien, J., Morrison, J. E., Rivlis, G., Latter, W. B., Noriega‐Crespo, A., Padgett, D. L., Stapelfeldt, K. R., Hines, D. C., Egami, E., Muzerolle, J., Alonso‐Herrero, A., Blaylock, M., Dole, H., Hinz, J. L., Le Floc’h, E., Papovich, C., Perez‐Gonzalez, P. G., Smith, P. S., Su, K. Y. L., Bennett, L., Frayer, D. T., Henderson, D., Lu, N., Masci, F., Pesenson, M., Rebull, L., Rho, J., Keene, J., Stolovy, S., Wachter, S., Wheaton, W., Werner, M. W., Richards, P. L.·2004·The Astrophysical Journal Supplement Series

Abstract

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%.

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Authors
Rieke, G. H., Young, E. T., Engelbracht, C. W., Kelly, D. M., Low, F. J., Haller, E. E., Beeman, J. W., Gordon, K. D., Stansberry, J. A., Misselt, K. A., Cadien, J., Morrison, J. E., Rivlis, G., Latter, W. B., Noriega‐Crespo, A., Padgett, D. L., Stapelfeldt, K. R., Hines, D. C., Egami, E., Muzerolle, J., Alonso‐Herrero, A., Blaylock, M., Dole, H., Hinz, J. L., Le Floc’h, E., Papovich, C., Perez‐Gonzalez, P. G., Smith, P. S., Su, K. Y. L., Bennett, L., Frayer, D. T., Henderson, D., Lu, N., Masci, F., Pesenson, M., Rebull, L., Rho, J., Keene, J., Stolovy, S., Wachter, S., Wheaton, W., Werner, M. W., & Richards, P. L.
Venue
The Astrophysical Journal Supplement Series
Published
2004-09
Volume
154
Issue
1
Pages
25-29
ISSN
  • 0067-0049 (ISSN-L)
  • 1538-4365
OpenAlex
W2044669640
Cited by
2,044
References
0
FWCI
155.43
Type
journal article
Language
en
Open access
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CoChat. (2026). Citation check: The Multiband Imaging Photometer for Spitzer (MIPS). https://app.cochat.ai/papers/10.1086/422717
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Rieke, G. H., Young, E. T., Engelbracht, C. W., Kelly, D. M., Low, F. J., Haller, E. E., Beeman, J. W., Gordon, K. D., Stansberry, J. A., Misselt, K. A., Cadien, J., Morrison, J. E., Rivlis, G., Latter, W. B., Noriega‐Crespo, A., Padgett, D. L., Stapelfeldt, K. R., Hines, D. C., Egami, E., . . . Richards, P. L. (2004). The Multiband Imaging Photometer for Spitzer (MIPS). The Astrophysical Journal Supplement Series. https://doi.org/10.1086/422717

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

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