-91405, Orsay Cedex, France June 30, 2004 Abstract Currently, it appears that the best method for non-Gaussianity detection in the Cosmic Microwave Background ( CMB ) consists in calculating the kurtosis of the wavelet coefficients ... Max (Mn ). ... It has been shown [44] that it is also possible to separate the nonGaussian signatures associated with cosmic strings from those due to SZ effect by combining the excess kurtosis derived from these both the curvelet and the wavelet transform. ...
[
Текст
]
Ссылки http://hea-www.harvard.edu/AstroStat/Stat310_fMMV/EURASIP-Paper.pdf -- 1245.1 Кб -- 22.09.2005 Похожие документы
... We quote the 2 per degree of freedom of the best fitting line and the significance of the fit for each regression in Table 4. ... 43 Table 2--Continued Exp eriment Ref. eff m in max T obs ± obs eff a c Publication Date (yrs) 2001.2 2001.2 2001.2 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 2002.4 ...
. Johnson: . Johnson: Space Center home page" shape=RECT alt="Return to Johnson: Space Center home page" coords=184,24,254,48 href="http://www.nasa.gov/centers/ Johnson: Johnson: Space Center home page" shape=RECT alt="Return to Johnson: Space Center home page" coords=-1,24,152,48 href="http://www.nasa.gov/centers/ Johnson: . Wright: Today is June 23, 1999. This oral history with C. Frederick Matthews is being conducted in Lexington, Massachusetts, for the Johnson Space Center Oral History Project.