RATAN-600 new zenith field survey and CMB problems

Details RATAN-600 new zenith field survey and CMB problems RATAN-600 new zenith field survey and CMB problems

2005-08-02

arxiv.org/abs/astro-ph/0508065v1

Grav.Cosmol. 10 (2004) 1-10

Astronomy and Astrophysics

Astrophysics

6 pages, 11 figures

Scientific paper

We present new RATAN-600 data on the synchrotron Galaxy radiation at the PLANCK Mission and WMAP frequencies at high Galactic latitudes upto l=3000. The difference between the standard synchrotron template (l<50) of the WMAP group and RATAN-600 data was detected with the strong synchrotron ``longitude quadrant asymmetry''. It may change the WMAP estimates of z_{reheating} from low l polarization data. The polarized synchrotron noise for very deep observations (<< 1 microK) at the PLANCK HFI was not detected at l>200 scales. ``Sakharov Oscillations'' in the E-mode (500

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