1. Small scale I, U, Q galaxy noise at cm. waves.
- Author
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Parijskij, Yu. N., Berlin, A. B., Bogdantsov, A., Bursov, N. N., Nizhelskij, N. A., Tsibulev, P., Novikov, I. D., and Naselskij, P. D.
- Subjects
COSMIC background radiation ,ANISOTROPY ,POLARIZATION (Nuclear physics) - Abstract
It is shown that the “spinning dust” component does not prevent observation of the CMB anysotropy at high l, values, as well as observation of the CMB polarization at scales which are the most interesting (l=1000). These results were obtained with the 600-meter reflector RATAN-600, equipped with a multi-frequency feed array with an angular resolution up to 0.1×1 arcmin and with a temperature resolution below 100 μK. © 2002 American Institute of Physics. [ABSTRACT FROM AUTHOR]
- Published
- 2002