English

Higher Criticism Statistic: Detecting and Identifying Non-Gaussianity in the WMAP First Year Data

Astrophysics 2008-11-26 v1

Abstract

Higher Criticism is a recently developed statistic for non-Gaussian detection, proposed in Donoho & Jin 2004. We find that Higher Criticism is useful for two purposes. First, Higher Criticism has competitive detection power, and non-Gaussianity is detected at the level 99% in the first year WMAP data. We find that the Higher Criticism value of WMAP is outside the 99% confidence region at a wavelet scale of 5 degrees (99.46% of Higher Criticism values based on simulated maps are below the values for WMAP). Second, Higher Criticism offers a way to locate a small portion of data that accounts for the non-Gaussianity. Using Higher Criticism, we have successfully identified a ring of pixels centered at (l\approx 209 deg, b\approx -57 deg), which seems to account for the observed detection of non-Gaussianity at the wavelet scale of 5 degrees. Note that the detection is achieved in wavelet space first. Second, it is always possible that a fraction of pixels within the ring might deviate from Gaussianity even if they do not appear to be above the 99% confidence level in wavelet space. The location of the ring coincides with the cold spot detected in Vielva et al. 2004 and Cruz et al. 2005.

Cite

@article{arxiv.astro-ph/0507246,
  title  = {Higher Criticism Statistic: Detecting and Identifying Non-Gaussianity in the WMAP First Year Data},
  author = {L. Cayon and J. Jin and A. Treaster},
  journal= {arXiv preprint arXiv:astro-ph/0507246},
  year   = {2008}
}

Comments

submitted to MNRAS

R2 v1 2026-07-22T08:54:16.356Z