INTERPRETING THE DISTANCE CORRELATION RESULTS FOR THE COMBO-17 SURVEY
INTERPRETING THE DISTANCE CORRELATION RESULTS FOR THE COMBO-17 SURVEY
The accurate classification of galaxies in large-sample astrophysical databases of galaxy clusters depends sensitively on the ability to distinguish between morphological types, especially at higher redshifts. This capability can be enhanced through a new statistical measure of association and correlation, called the {\it distance correlation coefficient}, which has more statistical …