Non-Gaussian spectra in cosmic microwave background temperature anisotropies
Gaussian cosmic microwave background skies are fully specified by the power spectrum. The conventional method of characterizing non-Gaussian skies is to evaluate higher order moments, the n -point functions, and their Fourier transforms. We argue that this method is inefficient, due to the redundan...
Main Authors: | Ferreira, P, Magueijo, J |
---|---|
Format: | Journal article |
Published: |
American Physical Society
1997
|
Similar Items
-
Non-Gaussian spectra in cosmic microwave background temperature anisotropies
by: Ferreira, P, et al.
Published: (1997) -
Non-Gaussian Spectra in the Cosmic Microwave Background
by: Ferreira, P
Published: (1997) -
MAXIMA: an experiment to measure temperature anisotropy in the cosmic
microwave background
by: Lee, A, et al.
Published: (1999) -
MAXIMA: an experiment to measure temperature anisotropy in the cosmic microwave background
by: Lee, A, et al.
Published: (1999) -
Asymmetric Beams in Cosmic Microwave Background Anisotropy Experiments
by: Wu, J, et al.
Published: (2000)