We establish weak convergence of the empirical process on the spherical harmonics of a Gaussian random field in the presence of an unknown angular power spectrum. This result suggests various Gaussianity tests with an asymptotic justification. The issue of testing for Gaussianity on isotropic spherical random fields has recently received strong empirical attention in the cosmological literature, in connection with the statistical analysis of cosmic microwave background radiation
We present a new, model-independent approach for measuring non-Gaussianity of the Cosmic Microwave B...
We study the weak convergence (in the high-frequency limit) of the parameter estimators of power spe...
We study the weak convergence (in the high-frequency limit) of the parameter estimators of power spe...
We establish weak convergence of the empirical process on the spherical harmonics of a Gaussian rand...
We establish weak convergence of the empirical process on the spherical harmonics of a Gaussian rand...
In this paper we study the asymptotic behavior of the angular bispectrum of spherical random field...
We present a new, model-independent approach for measuring non-Gaussianity of the cosmic microwave b...
In this paper we provide some simple characterizations for the spherical harmonics coefficients of a...
In this paper we provide some simple characterizations for the spher-ical harmonics coefficients of ...
The defect of a function f : M -> R is defined as the difference between the measure of the posit...
We present a new, model-independent approach for measuring non-Gaussianity of the Cosmic Microwave B...
We study the weak convergence (in the high-frequency limit) of the parameter estimators of power spe...
We study the weak convergence (in the high-frequency limit) of the parameter estimators of power spe...
We establish weak convergence of the empirical process on the spherical harmonics of a Gaussian rand...
We establish weak convergence of the empirical process on the spherical harmonics of a Gaussian rand...
In this paper we study the asymptotic behavior of the angular bispectrum of spherical random field...
We present a new, model-independent approach for measuring non-Gaussianity of the cosmic microwave b...
In this paper we provide some simple characterizations for the spherical harmonics coefficients of a...
In this paper we provide some simple characterizations for the spher-ical harmonics coefficients of ...
The defect of a function f : M -> R is defined as the difference between the measure of the posit...
We present a new, model-independent approach for measuring non-Gaussianity of the Cosmic Microwave B...
We study the weak convergence (in the high-frequency limit) of the parameter estimators of power spe...
We study the weak convergence (in the high-frequency limit) of the parameter estimators of power spe...