Classification of cosmic sources - A statistical approach

Details Classification of cosmic sources - A statistical approach Classification of cosmic sources - A statistical approach

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....95..138g&link_type=abstract

Astronomy and Astrophysics, vol. 95, no. 1, Feb. 1981, p. 138-142.

Mathematics

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9

Dwarf Stars, Novae, Statistical Analysis, Taxonomy, X Ray Sources, Astronomical Catalogs, Classifications, Data Acquisition, Probability Theory

Scientific paper

A fast statistical classification method is presented which makes it possible to (1) recognize homogeneous classes of objects without any a priori knowledge of the taxonomical units; (2) identify class boundaries; and (3) assign a new object of unidentified nature to a given class with a definite probability. In case of X-ray sources and dwarf novae, good agreement is found between the proposed G-mode classification technique and the classification of Brandt et al. (1978).

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