Detection of a Supervoid Aligned with the Cold Spot of the Cosmic Microwave Background
arXiv:1405.1566 · doi:10.1093/mnras/stv488
Abstract
We use the WISE-2MASS infrared galaxy catalog matched with Pan-STARRS1 (PS1) galaxies to search for a supervoid in the direction of the Cosmic Microwave Background Cold Spot. Our imaging catalog has median redshift , and we obtain photometric redshifts from PS1 optical colours to create a tomographic map of the galaxy distribution. The radial profile centred on the Cold Spot shows a large low density region, extending over 10's of degrees. Motivated by previous Cosmic Microwave Background results, we test for underdensities within two angular radii, , and . The counts in photometric redshift bins show significantly low densities at high detection significance, and , respectively, for the two fiducial radii. The line-of-sight position of the deepest region of the void is . Our data, combined with an earlier measurement by Granett et al. 2010, are consistent with a large supervoid with centered at . Such a supervoid, constituting at least a fluctuation in a Gaussian distribution of the model, is a plausible cause for the Cold Spot.
8 pages, 6 figures, accepted for publication by MNRAS
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