Automatic Morphological Classification of Galaxies
Sadanori Okamura, Mamoru Doi, M. Fukugita, Nobunari Kashikawa, M. Sekiguchi, Kazuhiro Shimasaku, Naoki Yasuda · Symposium - International Astronomical Union · 1994
We study the performance and limitations of the morphological classification method based on luminosity concentration and mean surface brightness. In particular, the effects of the different colour bands and of a finite seeing are investigated.