|作者：||S. Okamura, M. Doi, M. Fukugita, N. Kashikawa, M. Sekiguchi, K. Shimasaku, N. Yasuda|
11 Department of Astronomy, School of Science, University of Tokyo, Tokyo 113, Japan
2 2 Department of Astrophysical Sciences, Princeton University, Princeton, U.S.A.
3 3 Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606, Japan
4 4 National Astronomical Observatory, Mitaka, Tokyo 181, Japan
|刊名：||Symposium - International Astronomical Union, 2016, Vol.161 , pp.243-247|
|来源数据库：||Cambridge University Press Journal|
|原始语种摘要：||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.|