The axis of evil revisited

被引:114
作者
Land, Kate
Magueijo, Joao
机构
[1] Univ Oxford, Oxford OX1 3RH, England
[2] Perimeter Inst Theoret Phys, Waterloo, ON N2L 2Y5, Canada
[3] Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada
[4] Imperial Coll, Theoret Phys Grp, London SW7 2BZ, England
关键词
cosmic microwave background;
D O I
10.1111/j.1365-2966.2007.11749.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In light of the three-year data release from the Wilkinson Microwave Anisotropy Probe, we re-examine the evidence for the 'Axis of Evil' (AoE). We discover that previous statistics are not robust with respect to the data sets available and different treatments of the Galactic plane. We identify the cause of the instability and implement an alternative 'model selection' approach. A comparison to Gaussian isotropic simulations finds the features significant at the 94-98 per cent level, depending on the particular AoE model. The Bayesian evidence finds lower significance, ranging from 'substantial' at Delta(ln E) similar to 1.4 to no vidence for the most general AoE model.
引用
收藏
页码:153 / 158
页数:6
相关论文
共 34 条
[1]   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
[2]   On the cosmic microwave background large-scale angular correlations [J].
Bernui, A. ;
Villela, T. ;
Wuensche, C. A. ;
Leonardi, R. ;
Ferreira, I. .
ASTRONOMY & ASTROPHYSICS, 2006, 454 (02) :409-414
[3]   Multimodel inference - understanding AIC and BIC in model selection [J].
Burnham, KP ;
Anderson, DR .
SOCIOLOGICAL METHODS & RESEARCH, 2004, 33 (02) :261-304
[4]   On the large-angle anomalies of the microwave sky [J].
Copi, CJ ;
Huterer, D ;
Schwarz, DJ ;
Starkman, GD .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 367 (01) :79-102
[5]   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
[6]   Can the lack of symmetry in the COBE DMR maps constrain the topology of the universe? [J].
deOliveiraCosta, A ;
Smoot, GF ;
Starobinsky, AA .
ASTROPHYSICAL JOURNAL, 1996, 468 (02) :457-&
[7]   Isotropy of the early universe from CMB anisotropies [J].
Donoghue, EP ;
Donoghue, JF .
PHYSICAL REVIEW D, 2005, 71 (04) :043002-1
[8]   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
[9]   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
[10]   Asymmetries in the cosmic microwave background anisotropy field [J].
Eriksen, HK ;
Hansen, FK ;
Banday, AJ ;
Górski, KM ;
Lilje, PB .
ASTROPHYSICAL JOURNAL, 2004, 605 (01) :14-20