Statistical criteria used today in the analysis of radio signals suspected on reasonable extraterrestrial origin, are based on the assumption that all the radio signals of natural origin are described by a Gaussian distribution, which is traditionally understood as the Gauss distribution. Usually the normal (Gauss) distribution is opposed to all the others. However, this is difficult to recognize the reasonable, because in nature there are many different distributions. The article offers a more realistic dichotomy: the Gaussian distributions, obeying the central limiting theorem, dominate in nature, while non-Gaussian ones, obeying the Gnedenko-Doeblin limiting theorem, are generated by intelligent beings. When identifying objects belonging...
We propose a set of new statistics which can be extracted out of the angular distribution of the Fou...
Abstract. The population of compact extragalactic sources contribute to the non-Gaussianity (NG) at ...
As a statistical measure to quantify the topological structure of the large-scale structure in the u...
International audienceComment of the very interesting paper by Hilhorst & Schehr, J. Stat. Mech. P06...
We discuss the requirements of good statistics for quantifying non-Gaussianity in the Cosmic Microwa...
With the widespread explosion of sensing and computing, an increasing number of industrial applicati...
Non-gaussianity represents the statistical signature of physical processes such as turbulence. It c...
The observed abundance of high-redshift galaxies and clusters contains precious information about th...
In the most of all statistical approaches in pattern recognition theories in remote sensing it is as...
We explore the use of different radio galaxy populations as tracers of different mass haloes and the...
International audienceOne of the principle efforts in cosmic microwave background (CMB) research is ...
The data on the angular sizes and flux densities of extragalactic radio sources from the 3CR and the...
We describe a general procedure for using number counts of any object to constrain the probability d...
ABSTRACT Time-series analysis allows for the determination of the Power Spectral Density (PSD) and P...
Non-Gaussian effects are important features in many fields of physics, and the search for non-Gaussi...
We propose a set of new statistics which can be extracted out of the angular distribution of the Fou...
Abstract. The population of compact extragalactic sources contribute to the non-Gaussianity (NG) at ...
As a statistical measure to quantify the topological structure of the large-scale structure in the u...
International audienceComment of the very interesting paper by Hilhorst & Schehr, J. Stat. Mech. P06...
We discuss the requirements of good statistics for quantifying non-Gaussianity in the Cosmic Microwa...
With the widespread explosion of sensing and computing, an increasing number of industrial applicati...
Non-gaussianity represents the statistical signature of physical processes such as turbulence. It c...
The observed abundance of high-redshift galaxies and clusters contains precious information about th...
In the most of all statistical approaches in pattern recognition theories in remote sensing it is as...
We explore the use of different radio galaxy populations as tracers of different mass haloes and the...
International audienceOne of the principle efforts in cosmic microwave background (CMB) research is ...
The data on the angular sizes and flux densities of extragalactic radio sources from the 3CR and the...
We describe a general procedure for using number counts of any object to constrain the probability d...
ABSTRACT Time-series analysis allows for the determination of the Power Spectral Density (PSD) and P...
Non-Gaussian effects are important features in many fields of physics, and the search for non-Gaussi...
We propose a set of new statistics which can be extracted out of the angular distribution of the Fou...
Abstract. The population of compact extragalactic sources contribute to the non-Gaussianity (NG) at ...
As a statistical measure to quantify the topological structure of the large-scale structure in the u...