No Higher criticism of the bianchi-corrected Wilkinson microwave anisotropy probe data

被引:19
作者
Cayon, L.
Banday, A. J.
Jaffe, T.
Eriksen, H. K.
Hansen, F. K.
Gorski, K. M.
Jin, J.
机构
[1] Purdue Univ, Dept Phys, W Lafayette, IN 47907 USA
[2] Max Planck Inst Astrophys, D-85741 Garching, Germany
[3] Univ Oslo, Inst Theoret Astrophys, N-0315 Oslo, Norway
[4] Univ Oslo, Dept Math Appl, N-0315 Oslo, Norway
[5] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[6] CALTECH, Pasadena, CA 91125 USA
[7] Purdue Univ, Dept Stat, W Lafayette, IN 47907 USA
关键词
methods : statistical; cosmic microwave background; cosmology : miscellaneous;
D O I
10.1111/j.1365-2966.2006.10381.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Higher Criticism (HC) has been proposed by Donoho & Jin as an effective statistic to detect deviations from Gaussianity. Motivated by the success of the Bianchi VIIh model in addressing many of the anomalies observed in the Wilkinson Microwave Anisotropy Probe (WMAP) data (Jaffe et al.), we present calculations in real and in wavelet space of the HC statistic of the Bianchi-corrected WMAP first-year data. At the wavelet scale of 5 degrees, the HC of the WMAP map drops from a value above the 99 per cent confidence level (c.l.) to a value below the 68 per cent CL when corrected by the Bianchi template. An important property of the HC statistic is its ability to locate the pixels that account for the deviation from Gaussianity. The analysis of the uncorrected WMAP data pointed to a cold spot in the Southern hemisphere, centred at l similar to 209 degrees, b similar to -57 degrees. The HC of the Bianchi-corrected map indicates that this spot remains prominent, albeit at a level completely consistent with Gaussian statistics. Consequently, it is debatable how much emphasis should be placed on this residual feature, but we consider the effect of modestly increasing the scaling of the template. A factor of only 1.2 renders the spot indistinguishable from the background level, with no noticeable impact on the results published in Jaffe et al. for the low-l anomalies, large-scale power asymmetry or wavelet kurtosis. A trivial interpretation would be that the Bianchi template may require a small enhancement of power on scales corresponding to the wavelet scale of 5 degrees.
引用
收藏
页码:598 / 602
页数:5
相关论文
共 32 条
[1]   UNIVERSAL ROTATION - HOW LARGE CAN IT BE [J].
BARROW, JD ;
JUSZKIEWICZ, R ;
SONODA, DH .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1985, 213 (04) :917-943
[2]   First-year Wilkinson Microwave Anisotropy Probe (WMAP) observations:: Preliminary maps and basic results [J].
Bennett, CL ;
Halpern, M ;
Hinshaw, G ;
Jarosik, N ;
Kogut, A ;
Limon, M ;
Meyer, SS ;
Page, L ;
Spergel, DN ;
Tucker, GS ;
Wollack, E ;
Wright, EL ;
Barnes, C ;
Greason, MR ;
Hill, RS ;
Komatsu, E ;
Nolta, MR ;
Odegard, N ;
Peiris, HV ;
Verde, L ;
Weiland, JL .
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2003, 148 (01) :1-27
[3]   Multipole vector anomalies in the first-year WMAP data:: A cut-sky analysis [J].
Bielewicz, P ;
Eriksen, HK ;
Banday, AJ ;
Górski, KM ;
Lilje, PB .
ASTROPHYSICAL JOURNAL, 2005, 635 (02) :750-760
[4]   Higher criticism statistic:: detecting and identifying non-Gaussianity in the WMAP first-year data [J].
Cayón, L ;
Jin, J ;
Treaster, A .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2005, 362 (03) :826-832
[5]   Detection of a non-Gaussian spot in WMAP [J].
Cruz, M ;
Martínez-González, E ;
Vielva, P ;
Cayón, L .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2005, 356 (01) :29-40
[6]   Significance of the largest scale CMB fluctuations in WMAP [J].
de Oliveira-Costa, A ;
Tegmark, M ;
Zaldarriaga, M ;
Hamilton, A .
PHYSICAL REVIEW D, 2004, 69 (06) :12
[7]   Isotropy of the early universe from CMB anisotropies [J].
Donoghue, EP ;
Donoghue, JF .
PHYSICAL REVIEW D, 2005, 71 (04) :043002-1
[8]   Higher criticism for detecting sparse heterogeneous mixtures [J].
Donoho, D ;
Jin, JS .
ANNALS OF STATISTICS, 2004, 32 (03) :962-994
[9]   Testing for non-gaussianity in the Wilkinson Microwave Anisotropy Probe data:: Minkowski functionals and the length of the skeleton [J].
Eriksen, HK ;
Novikov, DI ;
Lilje, PB ;
Banday, AJ ;
Górski, KM .
ASTROPHYSICAL JOURNAL, 2004, 612 (01) :64-80
[10]   On foreground removal from the Wilkinson Microwave Anisotropy Probe data by an internal linear combination method:: Limitations and implications [J].
Eriksen, HK ;
Banday, AJ ;
Górski, KM ;
Lilje, PB .
ASTROPHYSICAL JOURNAL, 2004, 612 (02) :633-646