Preliminary results from the third flight of the Millimeter Anisotropy Experiment (MAX)

M. Devlin; D. Alsop; A. Clapp; D. Cottingham; M. Fischer; J. Gundersen; W. Holmes; A. Lange; P. Lubin; P. Meinhold; P. Richards; G. Smoot

doi:10.1073/pnas.90.11.4774

Preliminary results from the third flight of the Millimeter Anisotropy Experiment (MAX)

M. Devlin, D. Alsop, A. Clapp, D. Cottingham, M. Fischer, J. Gundersen, W. Holmes, A. Lange, P. Lubin, P. Meinhold, P. Richards, G. Smoot

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Abstract

Preliminary results from the June 1991 flight of MAX are presented. Simultaneous observations were made in bands centered at 6, 9, and 12 cm^-1 with a bolometric receiver operating at 300 mK. The experimental sensitivities are the highest reported at angular scales of 0.3° to 1.0°. Interstellar dust is observed to have an emissivity ∝ ν^1.4±0.3 and to correlate with the Infrared Astronomical Satellite (IRAS) 100-μ map. After removal of emission from interstellar dust, 1.3 hr of integration on a 6° scan yields an upper limit of temperature difference ΔT/T < 2.6 × 10^-5 at a Gaussian autocorrelation function centered at 0.5°. The experiment and data analysis are described.

Original language	English (US)
Pages (from-to)	4774-4776
Number of pages	3
Journal	Proceedings of the National Academy of Sciences of the United States of America
Volume	90
Issue number	11
DOIs	https://doi.org/10.1073/pnas.90.11.4774
State	Published - Jun 1 1993
Externally published	Yes

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Devlin, M., Alsop, D., Clapp, A., Cottingham, D., Fischer, M., Gundersen, J., Holmes, W., Lange, A., Lubin, P., Meinhold, P., Richards, P., & Smoot, G. (1993). Preliminary results from the third flight of the Millimeter Anisotropy Experiment (MAX). Proceedings of the National Academy of Sciences of the United States of America, 90(11), 4774-4776. https://doi.org/10.1073/pnas.90.11.4774

Preliminary results from the third flight of the Millimeter Anisotropy Experiment (MAX). / Devlin, M.; Alsop, D.; Clapp, A.; Cottingham, D.; Fischer, M.; Gundersen, J.; Holmes, W.; Lange, A.; Lubin, P.; Meinhold, P.; Richards, P.; Smoot, G.

In: Proceedings of the National Academy of Sciences of the United States of America, Vol. 90, No. 11, 01.06.1993, p. 4774-4776.

Research output: Contribution to journal › Article › peer-review

Devlin, M, Alsop, D, Clapp, A, Cottingham, D, Fischer, M, Gundersen, J, Holmes, W, Lange, A, Lubin, P, Meinhold, P, Richards, P & Smoot, G 1993, 'Preliminary results from the third flight of the Millimeter Anisotropy Experiment (MAX)', Proceedings of the National Academy of Sciences of the United States of America, vol. 90, no. 11, pp. 4774-4776. https://doi.org/10.1073/pnas.90.11.4774

Devlin, M. ; Alsop, D. ; Clapp, A. ; Cottingham, D. ; Fischer, M. ; Gundersen, J. ; Holmes, W. ; Lange, A. ; Lubin, P. ; Meinhold, P. ; Richards, P. ; Smoot, G. / Preliminary results from the third flight of the Millimeter Anisotropy Experiment (MAX). In: Proceedings of the National Academy of Sciences of the United States of America. 1993 ; Vol. 90, No. 11. pp. 4774-4776.

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abstract = "Preliminary results from the June 1991 flight of MAX are presented. Simultaneous observations were made in bands centered at 6, 9, and 12 cm-1 with a bolometric receiver operating at 300 mK. The experimental sensitivities are the highest reported at angular scales of 0.3° to 1.0°. Interstellar dust is observed to have an emissivity ∝ ν1.4±0.3 and to correlate with the Infrared Astronomical Satellite (IRAS) 100-μ map. After removal of emission from interstellar dust, 1.3 hr of integration on a 6° scan yields an upper limit of temperature difference ΔT/T < 2.6 × 10-5 at a Gaussian autocorrelation function centered at 0.5°. The experiment and data analysis are described.",

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AU - Gundersen, J.

AU - Holmes, W.

AU - Lange, A.

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AU - Richards, P.

AU - Smoot, G.

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AB - Preliminary results from the June 1991 flight of MAX are presented. Simultaneous observations were made in bands centered at 6, 9, and 12 cm-1 with a bolometric receiver operating at 300 mK. The experimental sensitivities are the highest reported at angular scales of 0.3° to 1.0°. Interstellar dust is observed to have an emissivity ∝ ν1.4±0.3 and to correlate with the Infrared Astronomical Satellite (IRAS) 100-μ map. After removal of emission from interstellar dust, 1.3 hr of integration on a 6° scan yields an upper limit of temperature difference ΔT/T < 2.6 × 10-5 at a Gaussian autocorrelation function centered at 0.5°. The experiment and data analysis are described.

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Preliminary results from the third flight of the Millimeter Anisotropy Experiment (MAX)

Abstract

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