Astronomy and Astrophysics – Astrophysics
Scientific paper
Oct 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aps..tsf.b3005d&link_type=abstract
American Physical Society, Texas Section Fall, October 23-25, 2003, Texas Tech Campus, Lubbock Texas, MEETING ID: TSF03, abstrac
Astronomy and Astrophysics
Astrophysics
Scientific paper
Using morphology classifications for galaxies provides a direct approach to view galaxy populations back to an early stage in their lifetime, and hence to study many astrophysical problems such as large-scale structure, galaxy formation and evolution. In the past, most of morphology classification was done visually. In recent years the vast amount of data produced by large surveys (such as SDSS, NED and 2MASS) has made visual inspection a daunting task. One potential solution to this problem is to automate galaxy classification using a neural network trained to distinguish patterns and relationships using various photometric indexes. We will present preliminary galaxy classification results using this method.
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