RATAN-600 new zenith field survey and CMB problems

Simple item page
dc.creatorParijskij, Yu. N.
dc.creatorBursov, N. N.
dc.creatorBerlin, A. B.
dc.creatorBalanovskij, A. A.
dc.creatorKhaikin, V. B.
dc.creatorMajorova, E. K.
dc.creatorMingaliev, M. G.
dc.creatorNizhelskij, N. A.
dc.creatorPylypenko, O. M.
dc.creatorTsibulev, P. A.
dc.creatorVerkhodanov, O. V.
dc.creatorZhekanis, G. V.
dc.creatorZverev, Yu. K.
dc.date2005-08-02
dc.date.accessioned2026-07-25T19:48:03Z
dc.descriptionWe 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<l<2000) should be well visible even at ~10 GHz. The polarized noise from relic gravitational waves (l~80) may be confused with B-mode of synchrotron Galaxy polarized noise at the frequencies below 100 GHz, but there are no problems at HFI-band.
dc.description6 pages, 11 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0508065
dc.identifierhttp://arxiv.org/abs/astro-ph/0508065
dc.identifierGrav.Cosmol. 10 (2004) 1-10
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/67268
dc.subjectAstrophysics
dc.titleRATAN-600 new zenith field survey and CMB problems
dc.typetext

Files

Collections

Artificial intelligence