Small scale I, U, Q galaxy noise at cm. waves

Details Small scale I, U, Q galaxy noise at cm. waves Small scale I, U, Q galaxy noise at cm. waves

Mar 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..609...51p&link_type=abstract

ASTROPHYSICAL POLARIZED BACKGROUNDS: Workshop on Astrophysical Polarized Backgrounds, held 9-12 October, 2001 in Bologna Italy.

Physics

3

Background Radiations, Radiation Mechanisms, Polarization, Interstellar Dust Grains, Diffuse Emission, Infrared Cirrus, Radio, Microwave

Scientific paper

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 (=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. .

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