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Cosmic Microwave Background Spectrum Measurements

Published online by Cambridge University Press:  30 March 2016

George F. Smoot
George F. Smoot*
Affiliation:
Space Sciences Laboratory & Lawrence Berkeley Laboratory, University of California, Berkeley, California, 94720, USA

Abstract

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This paper reviews the three major cosmic microwave background radiation (CMBR) spectrum measurement programs conducted and published since the last (XVII) IAU General Assembly. The results are consistent with a Planckian spectrum with temperature 2.72 ± 0.03 K spanning a wavelength range of 0.1 to 12 cm. Limits on possible distortions and implications are outlined. Ongoing and future measurements are discussed.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 7: Highlights of Astronomy. As presented at the XIXth General Assembly of the IAU, 1985 , 1986 , pp. 297 - 305
Copyright
Copyright © Reidel 1986

References

Chan, K. L., and Jones, B. J. T. 1976, Ap. J., 200, 461.CrossRefGoogle Scholar
De Amici, G., Witebsky, C., Smoot, G. F., and Friedman, S. D. 1984, Phys. Rev. D, 29, 2673.CrossRefGoogle Scholar
De Amici, G., Smoot, G. F., Friedman, S. D., and Witebsky, C. 1985, Ap. J., 298, 710–731.CrossRefGoogle Scholar
Dolgov, A. D., and Zel’dovich, Ya. B. 1981, Rev. Mod. Phys., 53, 1.CrossRefGoogle Scholar
Friedman, S. D., Smoot, G. F., De Amici, G., and Witebsky, C. 1984, Phys. Rev. D, 29, 2677.Google Scholar
Georgi, H., Ginsparg, P., and Glashow, S.L., 1983, Nature, 306, 765.CrossRefGoogle Scholar
Gush, G.P. 1984, Proceedings of Conference on Space Helium Dewars, Huntsville Google Scholar
Illarionov, A. F., and Sunyaev, R. A. 1974, Astron. Zh., 51, 1162 (1975, Soviet Astron., 18, 691).Google Scholar
Lubyarsky, Y.E., and Sunyaev, R.A., 1983, Astron. Astrophys., 123, 171.Google Scholar
Mandolesi, N., Calzolari, P., Cortiglioni, S., and Morigi, G. 1984, Phys. Rev. D, 29, 2680.CrossRefGoogle Scholar
Mather, J.C. 1982, Optical Eng., 21, 769.CrossRefGoogle Scholar
Meyer, D.M., and Jura, M. 1984, Ap J. 276, L1–L3.CrossRefGoogle Scholar
Meyer, D.M., and Jura, M. 1985, ApJ., 297, 119.CrossRefGoogle Scholar
Partridge, R. B., et al. 1984, Phys. Rev. D, 29, 2683.Google Scholar
Peterson, J.B., Richards, P.L., and Timusk, T. 1985, Phys Rev Lett, 55, 232.Google Scholar
Silk, J. and Stebbins, A., 1983, Ap J., 269, 1.CrossRefGoogle Scholar
Sironi, G., Inzani, P., and Ferrari, A. Phys. Rev. D, 1984, 29, 2686.Google Scholar
Smoot, G. et al. 1983, Phys. Rev. Letters, 51, 1099.Google Scholar
Smoot, G. et al. 1985a, Ap. J. (Letters), 291, L23–L27.CrossRefGoogle Scholar
Smoot, G. et al. 1985e, Societa Italiana di Fisica Conference Proceedings, 1, 27.Google Scholar
Stecker, F. D., and Puget, J. L. 1972, Ap. J., 178, 57.CrossRefGoogle Scholar
Sunyaev, R. A., and Zel’dovich, Ya. B. 1970, Ap. Space Sci., 7, 20.CrossRefGoogle Scholar
Sunyaev, R. A., and Zel’dovich, Ya. B. 1980, Ann. Rev. Astr. Ap., 18, 537.CrossRefGoogle Scholar
Woody, D.P. and Richards, P.L. 1981. Astrophys. J. Letters 248, 18 CrossRefGoogle Scholar