Abstract
The determination of TCBR at 1.3 mm is particularly interesting because it lies just at the peak of the Black-Body spectrum, where deviations can be most likely (Matsumoto et al., 1988). However, measurements at this wavelength are extremely difficult from the ground.
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References
Crane, P, and Hegyi, D.J., 1988, Astrophys. J.CLettersJ, L35, 326.
Crane, P., Hegyi, D.J., Mandolesi, N., and Danks, A.C.D., 1986, Astrophys. J., 309, 822.
Matsumoto, T., Hayakawa, S., Matsuo, H., Murakami, H., Sata, S., Lange, A.E., and Richards, P.L., 1988, Astrophys. J., 329, 567.
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© 1989 Kluwer Academic Publisher
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Palazzi, E., Mandolesi, N., Crane, P., Hegyi, D.J., Blades, J.C. (1989). Measurements of Tcbr at 1. 3 MM. In: Caffo, M., Fanti, R., Giacomelli, G., Renzini, A. (eds) Astronomy, Cosmology and Fundamental Physics. Astrophysics and Space Science Library, vol 155. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0965-6_43
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DOI: https://doi.org/10.1007/978-94-009-0965-6_43
Publisher Name: Springer, Dordrecht
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