The trispectrum of the 4 year COBE DMR data

被引:46
作者
Kunz, M
Banday, AJ
Castro, PG
Ferreira, PG
Górski, KM
机构
[1] Univ Oxford, Dept Astrophys, Oxford OX1 3RH, England
[2] Max Planck Inst Astrophys, D-85741 Garching, Germany
[3] European So Observ, D-8046 Garching, Germany
[4] Univ Warsaw Observ, PL-00478 Warsaw, Poland
关键词
cosmic microwave background; cosmology : observations;
D O I
10.1086/338602
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We propose an estimator for the trispectrum of a scalar random field on a sphere, discuss its geometrical and statistical properties, and outline its implementation. By estimating the trispectrum of the 4 yr COBE Differential Microwave Radiometer experiment data (in HEALPix pixelization), we find new evidence of a non-Gaussian signal associated with a known systematic effect. We find that by removing data from the sky maps for those periods of time perturbed by this effect, the amplitudes of the trispectrum coefficients become completely consistent with predictions for a Gaussian sky. These results reinforce the importance of statistical methods based in harmonic space for quantifying non-Gaussianity.
引用
收藏
页码:L99 / L102
页数:4
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