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The Properties of Isolated Main Galaxies in Sloan Digital Sky Survey Data Release 3 (SDSS DR3)
Xinfa
Deng A B,
Xinsheng
Ma A,
Chenghong
Luo A,
Qun
Zhang A,
Qing-Hua
Liao A,
Ji-zhou
He A
A
Mathematics and Physics College, Nanchang University, Jiangxi 330047, China
B
Corresponding author. E-mail: xinfadeng@163.com
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Publications of the Astronomical Society of Australia 23(2) 76–81 http://dx.doi.org/10.1071/AS05019
Submitted: 22 June 2005
Accepted: 7 October 2005
Published online: 25 July 2006
Abstract
We have constructed a Main galaxy subsample of 67777 galaxies with redshifts in the range 0.08 ≤ z ≤ 0.12 from the Sloan Digital Sky Survey Data Release 3. Using cluster analysis, two isolated Main galaxy samples were extracted from this subsample. The two isolated Main galaxy samples identified at different radii have the same properties. Additionally, we find fewer early-type galaxies in isolated Main galaxy samples than in a close double galaxy sample.
Keywords:
cosmology,
galaxy,
cluster analysis
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