Large-Scale Distribution of Galaxies with Different Luminosities
1987 ◽
Vol 124
◽
pp. 363-366
Keyword(s):
Analyses for complete samples of galaxies and clusters of galaxies showed that the two-point correlation function of galaxy-galaxy and cluster-cluster have form of power law with power indices about −1.8 (Peebles, 1980; Bahcall and Soneira, 1983). Because the completeness of a sample means that we have observed completely the objects brighter than a given apparent magnitude in certain sky region. But, we know that a complete sample will be lack of faint objects at distant region. If we attempt to avoid the influences of any non-intrinsic properties on the analysis, we have to use the samples which are complete in certain interval of absolute magnitude.
1983 ◽
Vol 104
◽
pp. 175-175
2005 ◽
Vol 216
◽
pp. 196-202
Keyword(s):
2017 ◽
Vol 469
(2)
◽
pp. 2059-2076
◽
2011 ◽
Vol 737
(2)
◽
pp. 97
◽
Keyword(s):
1998 ◽
Vol 296
(1)
◽
pp. 173-190
◽
2014 ◽
Vol 11
(S308)
◽
pp. 215-216