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The MAP Satellite Mission to Map the CMB Anisotropy

Published online by Cambridge University Press:  26 May 2016

Lyman. Page
Lyman. Page*
Affiliation:
Princeton University, Dept. of Physics, Jadwin Hall, Washington Road, Princeton, NJ 08544, USA

Abstract

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The Microwave Anisotropy Probe (MAP) satellite is scheduled to launch in mid-2001. MAP's goal is to produce a map of the anisotropy in the cosmic microwave background of unprecedented accuracy and precision. The guiding design principle has been the minimization of systematic effects. The instrument design and mapping strategy work in concert to take advantage of the unique opportunities afforded by deep space. We give an overview of the mission and compare the projected MAP error bars to recent measurements.

Information

Type
Part III: Primordial CMB Observations: Balloon and Satellite based
Information
Symposium - International Astronomical Union , Volume 201: New Cosmological Data and the Values of the Fundamental Parameters , 2005 , pp. 75 - 85
Copyright
Copyright © Astronomical Society of the Pacific 2005 

References

Bennett, C. L. et al. 1996, ApJ, 464, L1.Google Scholar
Bond, J. R., Jaffe, A. H. & Knox, L. 2000, ApJ, 533, 19.CrossRefGoogle Scholar
de Bernardis, P. et al. 2000, Nature, 404, 955.CrossRefGoogle Scholar
de Oliveira-Costa, A. et al. 1998, ApJ, 509, L77.Google Scholar
Devlin, M. J. et al. 1998, ApJ, 509, L69.Google Scholar
Dodelson, S. & Knox, L. 2000, Phys.Rev.Lett, 84, 3523.CrossRefGoogle Scholar
Ganga, K. et al. 1993, ApJ, 410, L57.Google Scholar
Hanany, S. et al. 2000, astro-ph/0005123.Google Scholar
Herbig, T. et al. 1998, ApJ, 509, L73.CrossRefGoogle Scholar
Hinshaw, G. 2000, astro-ph/0011555.Google Scholar
Hu, W. 2000, astro-ph/0002520.Google Scholar
Jaffe, A. et al. 2000, astro-ph/0007333.Google Scholar
Jarosik, N. 2000, “The Use of Cryogenic HEMT Amplifiers in Wide Band Radiometers.” Proceedings of the European Gallium Arsenide Application Symposium, Paris, France (GAAS2000).Google Scholar
Knox, L. & Page, L. 2000, Phys.Rev.Lett, 85, 1366.Google Scholar
Lineweaver, C. et al. 1994, ApJ, 436, 452.Google Scholar
Mauskopf, P. 2000, ApJ, 536, L59.Google Scholar
Meyer, S. S., Cheng, E. S. & Page, L. A. 1991, ApJ, 371, L7.CrossRefGoogle Scholar
Miller, A. D. et al. 1999, ApJ, 524, L1.Google Scholar
Partridge, B. 1995, 3K: The Cosmic Microwave Background Radiation, Cambridge University Press, New York.Google Scholar
Pospieszalski, M. W. 1992, Proc. IEEE Microwave Theory Tech., MTT-3, 1369 and Pospieszalski, M. W. et al. 1994, Proc. IEEE Microwave Theory Tech., MTT-3, 1345.Google Scholar
Pospieszalski, M. W. & Wollack, E. 2000, “Ultra-Low-Noise, InP Field Effect Transistors Amplifiers for Radio Astronomy Receivers,” Proceedings of the European Gallium Arsenide Application Symposium, Paris, Prance (GAAS2000).Google Scholar
Smoot, G. et al. 1992, ApJ, 153, L1.Google Scholar
Tegmark, M. 1997, Phys.Rev.D, 56.Google Scholar
Tegmark, M. et al. 2000, ApJ, 530, 133.Google Scholar
Toffolatti, L. et al. 1998, MNRAS, 297, 117.Google Scholar
Torbet, E. et al. 1999, ApJ, 521, L79.Google Scholar
Wright, E. L. 1996, astro-ph/9612006.Google Scholar
Weiss, R. 1980, ARA&A, 18, 489–535.Google Scholar