Physics
Scientific paper
Sep 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3..155v&link_type=abstract
Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 155
Physics
Scientific paper
The algorithm to recognize an abundance zone in galaxy distribution is proposed. The method used is the 3--D wavelet analysis which allows to constructa ``tree" of wavelet coefficients keeping information about the distribution of galaxies in zones surrounding an abundance zone. These coefficients are to be used for prediction of galaxy distribution in an abundance zone.
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