... T h e C o s m ic M ic r o w a v e B a c k g r o u n d Maxima DASI WMAP U n iv e r s e a t z > 1 1 0 0 is h o t, m a tte r d o m in a te d , b u t s till fu ll o f p h o to n s . ...
... Emission from these cosmic rays explains the WMAP Haze observed at microwave wavelengths around the Galactic centre as well as the Bubbles wider-scale radio polarization and gamma-ray emission. ...
... For the third year WMAP parameters (Spergel et al. 2006), C decreases to 1.61. ... et al. (2004), and the results of the 3 year WMAP-only fit from Spergel et al ... The WMAP three year results (Spergel et al. 2006) noticeably lower the predicted ...
... Testing the CMB Data for systematic effects . Griffiths, L., Lineweaver C.H. , 2003, astro-ph/0301490 (Pre-WMAP data only) . ... Grether, D., Lineweaver C.H. , 2003, IAU presentation . Is the pre-WMAP CMB data self-consistent? ...
... to recent results reported using the WMAP satellite, also in combination with the ... very similar to recent results reported using the WMAP satellite: 20 TONRY ET AL ...
... for vacuum energy and neutrino masses in the light of WMAP-3', Journal of Cosmology and Astro-Particle Physics 1, 25 ... Wright, E. L. (2006), `Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology', astro-ph ...
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Ссылки http://www.mso.anu.edu.au/~charley/papers/LineweaverEgan2007.pdf -- 484.1 Кб -- 30.04.2007 Похожие документы