Is the low-l microwave background cosmic?

@article{Schwarz2004IsTL,
  title={Is the low-l microwave background cosmic?},
  author={Dominik J. Schwarz and Glenn D Starkman and Dragan Huterer and Craig J Copi},
  journal={Physical review letters},
  year={2004},
  volume={93 22},
  pages={
          221301
        }
}
The large-angle (low-l) correlations of the cosmic microwave background exhibit several statistically significant anomalies compared to the standard inflationary cosmology. We show that the quadrupole plane and the three octopole planes are far more aligned than previously thought (99.9% C.L.). Three of these planes are orthogonal to the ecliptic at 99.1% C.L., and the normals to these planes are aligned at 99.6% C.L. with the direction of the cosmological dipole and with the equinoxes. The… 

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