On the largeangle anomalies of the microwave sky
Abstract
We apply the multipole vector framework to fullsky maps derived from the firstyear Wilkinson Microwave Anisotropy Probe (WMAP) data. We significantly extend our earlier work showing that the two lowest cosmologically interesting multipoles, l= 2 and 3, are not statistically isotropic. These results are compared to the findings obtained using related methods. In particular, we show that the planes of the quadrupole and the octopole are unexpectedly aligned. Moreover, the combined quadrupole plus octopole is surprisingly aligned with the geometry and direction of motion of the Solar system: the plane they define is perpendicular to the ecliptic plane and to the plane defined by the dipole direction, and the ecliptic plane carefully separates stronger from weaker extrema, running within a couple of degrees of the nullcontour between a maximum and a minimum over more than 120° of the sky. Even given the alignment of the quadrupole and octopole with each other, we find that their alignment with the ecliptic is unlikely at >98 per cent confidence level (CL), and argue that it is in fact unlikely at >99.9 per cent CL. Most of the l= 2 and 3 multipole vectors of the known Galactic foregrounds are located far from those of the observed sky, strongly suggesting that residual contamination by such foregrounds is unlikely to be the cause of the observed correlations. Multipole vectors, like individual a_{lm}, are very sensitive to sky cuts, and we demonstrate that analyses using cut skies induce relatively large errors, thus weakening the observed correlations but preserving their consistency with the fullsky results. Similarly, the analysis of COBE cutsky maps shows increased errors but is consistent with WMAP fullsky results. We briefly extend these explorations to higher multipoles, noting again anomalous deviations from statistical isotropy and comparing with ecliptic asymmetry manifested in the WMAP team's own analysis. If the correlations we observe are indeed a signal of noncosmic origin, then the lack of lowl power will very likely be exacerbated, with important consequences for our understanding of cosmology on large scales.
 Publication:

Monthly Notices of the Royal Astronomical Society
 Pub Date:
 March 2006
 DOI:
 10.1111/j.13652966.2005.09980.x
 arXiv:
 arXiv:astroph/0508047
 Bibcode:
 2006MNRAS.367...79C
 Keywords:

 cosmic microwave background;
 Astrophysics;
 General Relativity and Quantum Cosmology
 EPrint:
 26 pages, 7 figures. High resolution figures, multipole vector code and other information can be found at http://www.phys.cwru.edu/projects/mpvectors/