Clustering properties of X ray sources from the analysis of the GINGA P(D) distribution

Details Clustering properties of X ray sources from the analysis of the GINGA P(D) distribution Clustering properties of X ray sources from the analysis of the GINGA P(D) distribution

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992xrea.conf..358t&link_type=abstract

In MPI für Extraterrestrische Physik, X Ray Emission from Active Galactic Nuclei and the Cosmic X Ray Background p 358-361 (SEE

Mathematics

Probability

Background Radiation, Data Processing, Galactic Clusters, Probability Distribution Functions, X Ray Sources, Ginga Satellite, Variations

Scientific paper

A P(D) analysis, the probability function of the fluctuations measured in integrated backgrounds using data from 132 independent samples measured at galactic latitudes in regions of the sky devoid of sources was performed. A figure illustrating the chi squared contours in the parameter space adopting a Euclidean slope for the N(greater than S) relation is given. The 1, 2, and 3 sigma probability levels and the star minimum fit are shown on the figure. A further similar figure is given, but the slope gamma = 1.6 for N(greater than S) relation is adopted.

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