Small-scale galactic emission fluctuation observations with RATAN-600 radio telescope

Details Small-scale galactic emission fluctuation observations with RATAN-600 radio telescope Small-scale galactic emission fluctuation observations with RATAN-600 radio telescope

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012astbu..67...29s&link_type=abstract

Astrophysical Bulletin, Volume 67, Issue 1, pp.29-43

Mathematics

Logic

Galaxy: Foregrounds, Galaxy: Diffuse Emission

Scientific paper

We present the estimates of Galactic synchrotron and free-free emission power at intermediate and small scales (500 < l < 1000, 20' < θ < 40'), based on the RATAN-600 radio telescope observations (SAO RAS). The observations were conducted in the frequency range of 2.3-11.2 GHz using the transit scan mode, in the declination range of 40.7° s δ < 42.3°. The power spectrum estimates of synchrotron and free-free components were obtained. They can be further used in the data processing stage of the high-resolution cosmological experiments like Planck.

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