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
The power spectrum has long been the workhorse summary statistics for large-scale structure cosmolog...
The current paradigm of a 6 parameter ΛCDM cosmology with single field slow-roll inflation predicts ...
We develop the formalism necessary to study four-point functions of the cosmic microwave background ...
We propose an estimator for the trispectrum of a scalar random field on a sphere, discuss its geomet...
The trispectrum of the cosmic microwave background can be used to assess the level of non-Gaussianit...
We introduce and study the distribution of an estimator for the normalized bispectrum of the Cosmic ...
We extend a previous bispectrum analysis of the Cosmic Microwave Background temperature anisotropy, ...
We calculate the two-, three- and (for the first time) four-point correlation functions of the COBE-...
We compute the three-point temperature correlation function of the {\it COBE} Differential Microwave...
We derive an optimal linear filter to suppress the noise from the COBE DMR sky maps for a given powe...
We review our recent claim that there is evidence of non-Gaussianity in the 4 Year COBE DMR data. We...
I review our recent claim that there is evidence of non-Gaussianity in the 4 Year COBE DMR data. I d...
We measure the angular bispectrum of the cosmic microwave background (CMB) radiation anisotropy from...
Cosmic microwave background studies of non-Gaussianity involving higher order multispectra can disti...
Considerable recent attention has focussed on the prospects to use the cosmic microwave background (...
The power spectrum has long been the workhorse summary statistics for large-scale structure cosmolog...
The current paradigm of a 6 parameter ΛCDM cosmology with single field slow-roll inflation predicts ...
We develop the formalism necessary to study four-point functions of the cosmic microwave background ...
We propose an estimator for the trispectrum of a scalar random field on a sphere, discuss its geomet...
The trispectrum of the cosmic microwave background can be used to assess the level of non-Gaussianit...
We introduce and study the distribution of an estimator for the normalized bispectrum of the Cosmic ...
We extend a previous bispectrum analysis of the Cosmic Microwave Background temperature anisotropy, ...
We calculate the two-, three- and (for the first time) four-point correlation functions of the COBE-...
We compute the three-point temperature correlation function of the {\it COBE} Differential Microwave...
We derive an optimal linear filter to suppress the noise from the COBE DMR sky maps for a given powe...
We review our recent claim that there is evidence of non-Gaussianity in the 4 Year COBE DMR data. We...
I review our recent claim that there is evidence of non-Gaussianity in the 4 Year COBE DMR data. I d...
We measure the angular bispectrum of the cosmic microwave background (CMB) radiation anisotropy from...
Cosmic microwave background studies of non-Gaussianity involving higher order multispectra can disti...
Considerable recent attention has focussed on the prospects to use the cosmic microwave background (...
The power spectrum has long been the workhorse summary statistics for large-scale structure cosmolog...
The current paradigm of a 6 parameter ΛCDM cosmology with single field slow-roll inflation predicts ...
We develop the formalism necessary to study four-point functions of the cosmic microwave background ...