Absolute calibration and characterization of the multiband imaging photometer for Spitzer. III. An asteroid-based calibration of MIPS at 160 μm

J. A. Stansberry, K. D. Gordon, B. Bhattacharya, C. W. Engelbracht, George H. Rieke, F. R. Marleau, D. Fadda, D. T. Frayer, A. Noriega-Crespo, S. Wachter, E. T. Young, T. G. Müller, D. M. Kelly, M. Blaylock, D. Henderson, G. Neugebauer, J. W. Beeman, E. E. Haller

Research output: Contribution to journalArticle

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Abstract

We describe the absolute calibration of the Multiband Imaging Photometer for Spitzer (MIPS) 160 μm channel. After the on-orbit discovery of a near-IR ghost image that dominates the signal for sources hotter than about 2000 K, we adopted a strategy utilizing asteroids to transfer the absolute calibrations of the MIPS 24 and 70 μm channels to the 160 μm channel. Near-simultaneous observations at all three wavelengths are taken, and photometry at the two shorter wavelengths is fit using the standard thermal model. The 160 μm flux density is predicted from those fits and compared with the observed 160 μm signal to derive the conversion from instrumental units to surface brightness. The calibration factor we derive is 41.7 MJy sr -1 MIPS160 -1 (MIPS 160 being the instrumental units). The scatter in the individual measurements of the calibration factor, as well as an assessment of the external uncertainties inherent in the calibration, lead us to adopt an uncertainty of 5.0 MJy sr -1 MIPS160 -1 (12%) for the absolute uncertainty on the 160 μm flux density of a particular source as determined from a single measurement. For sources brighter than about 2 Jy, nonlinearity in the response of the 160 μm detectors produces an underestimate of the flux density: for objects as bright as 4 Jy, measured flux densities are likely to be ≲ 20% too low. This calibration has been checked against that of the ISO (using ULIRGs) and IRAS (using IRAS-derived diameters), and is consistent with those at the 5% level.

Original languageEnglish (US)
Pages (from-to)1038-1051
Number of pages14
JournalPublications of the Astronomical Society of the Pacific
Volume119
Issue number859
DOIs
StatePublished - 2007

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photometer
asteroids
asteroid
photometers
flux density
calibration
Infrared Astronomy Satellite
ghosts
wavelengths
wavelength
photometry
brightness
nonlinearity
orbits
detectors

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Absolute calibration and characterization of the multiband imaging photometer for Spitzer. III. An asteroid-based calibration of MIPS at 160 μm. / Stansberry, J. A.; Gordon, K. D.; Bhattacharya, B.; Engelbracht, C. W.; Rieke, George H.; Marleau, F. R.; Fadda, D.; Frayer, D. T.; Noriega-Crespo, A.; Wachter, S.; Young, E. T.; Müller, T. G.; Kelly, D. M.; Blaylock, M.; Henderson, D.; Neugebauer, G.; Beeman, J. W.; Haller, E. E.

In: Publications of the Astronomical Society of the Pacific, Vol. 119, No. 859, 2007, p. 1038-1051.

Research output: Contribution to journalArticle

Stansberry, JA, Gordon, KD, Bhattacharya, B, Engelbracht, CW, Rieke, GH, Marleau, FR, Fadda, D, Frayer, DT, Noriega-Crespo, A, Wachter, S, Young, ET, Müller, TG, Kelly, DM, Blaylock, M, Henderson, D, Neugebauer, G, Beeman, JW & Haller, EE 2007, 'Absolute calibration and characterization of the multiband imaging photometer for Spitzer. III. An asteroid-based calibration of MIPS at 160 μm', Publications of the Astronomical Society of the Pacific, vol. 119, no. 859, pp. 1038-1051. https://doi.org/10.1086/521880
Stansberry, J. A. ; Gordon, K. D. ; Bhattacharya, B. ; Engelbracht, C. W. ; Rieke, George H. ; Marleau, F. R. ; Fadda, D. ; Frayer, D. T. ; Noriega-Crespo, A. ; Wachter, S. ; Young, E. T. ; Müller, T. G. ; Kelly, D. M. ; Blaylock, M. ; Henderson, D. ; Neugebauer, G. ; Beeman, J. W. ; Haller, E. E. / Absolute calibration and characterization of the multiband imaging photometer for Spitzer. III. An asteroid-based calibration of MIPS at 160 μm. In: Publications of the Astronomical Society of the Pacific. 2007 ; Vol. 119, No. 859. pp. 1038-1051.
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abstract = "We describe the absolute calibration of the Multiband Imaging Photometer for Spitzer (MIPS) 160 μm channel. After the on-orbit discovery of a near-IR ghost image that dominates the signal for sources hotter than about 2000 K, we adopted a strategy utilizing asteroids to transfer the absolute calibrations of the MIPS 24 and 70 μm channels to the 160 μm channel. Near-simultaneous observations at all three wavelengths are taken, and photometry at the two shorter wavelengths is fit using the standard thermal model. The 160 μm flux density is predicted from those fits and compared with the observed 160 μm signal to derive the conversion from instrumental units to surface brightness. The calibration factor we derive is 41.7 MJy sr -1 MIPS160 -1 (MIPS 160 being the instrumental units). The scatter in the individual measurements of the calibration factor, as well as an assessment of the external uncertainties inherent in the calibration, lead us to adopt an uncertainty of 5.0 MJy sr -1 MIPS160 -1 (12{\%}) for the absolute uncertainty on the 160 μm flux density of a particular source as determined from a single measurement. For sources brighter than about 2 Jy, nonlinearity in the response of the 160 μm detectors produces an underestimate of the flux density: for objects as bright as 4 Jy, measured flux densities are likely to be ≲ 20{\%} too low. This calibration has been checked against that of the ISO (using ULIRGs) and IRAS (using IRAS-derived diameters), and is consistent with those at the 5{\%} level.",
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T1 - Absolute calibration and characterization of the multiband imaging photometer for Spitzer. III. An asteroid-based calibration of MIPS at 160 μm

AU - Stansberry, J. A.

AU - Gordon, K. D.

AU - Bhattacharya, B.

AU - Engelbracht, C. W.

AU - Rieke, George H.

AU - Marleau, F. R.

AU - Fadda, D.

AU - Frayer, D. T.

AU - Noriega-Crespo, A.

AU - Wachter, S.

AU - Young, E. T.

AU - Müller, T. G.

AU - Kelly, D. M.

AU - Blaylock, M.

AU - Henderson, D.

AU - Neugebauer, G.

AU - Beeman, J. W.

AU - Haller, E. E.

PY - 2007

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N2 - We describe the absolute calibration of the Multiband Imaging Photometer for Spitzer (MIPS) 160 μm channel. After the on-orbit discovery of a near-IR ghost image that dominates the signal for sources hotter than about 2000 K, we adopted a strategy utilizing asteroids to transfer the absolute calibrations of the MIPS 24 and 70 μm channels to the 160 μm channel. Near-simultaneous observations at all three wavelengths are taken, and photometry at the two shorter wavelengths is fit using the standard thermal model. The 160 μm flux density is predicted from those fits and compared with the observed 160 μm signal to derive the conversion from instrumental units to surface brightness. The calibration factor we derive is 41.7 MJy sr -1 MIPS160 -1 (MIPS 160 being the instrumental units). The scatter in the individual measurements of the calibration factor, as well as an assessment of the external uncertainties inherent in the calibration, lead us to adopt an uncertainty of 5.0 MJy sr -1 MIPS160 -1 (12%) for the absolute uncertainty on the 160 μm flux density of a particular source as determined from a single measurement. For sources brighter than about 2 Jy, nonlinearity in the response of the 160 μm detectors produces an underestimate of the flux density: for objects as bright as 4 Jy, measured flux densities are likely to be ≲ 20% too low. This calibration has been checked against that of the ISO (using ULIRGs) and IRAS (using IRAS-derived diameters), and is consistent with those at the 5% level.

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