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This article has been cited by the following article(s):
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Mass Selection and the Evolution of the Morphology‐Density Relation fromz= 0.8 to 0
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Infrared Luminosity Function of the Coma Cluster
Lei Bai, George H. Rieke, Marcia J. Rieke, et al. The Astrophysical Journal 639(2) 827 (2006) https://doi.org/10.1086/499620
The Possible
z
= 0.83 Precursors of
z
= 0,
M
* Early-Type Cluster Galaxies
B. P. Holden, M. Franx, G. D. Illingworth, et al. The Astrophysical Journal 642(2) L123 (2006) https://doi.org/10.1086/504714
Luminosity segregation in three clusters of galaxies (A119, A2443, A2218)
Michael B. Pracy, Simon P. Driver, Roberto De Propris, Warrick J. Couch and Paul E. J. Nulsen Monthly Notices of the Royal Astronomical Society 364(4) 1147 (2005) https://doi.org/10.1111/j.1365-2966.2005.09686.x
The build-up of the Coma cluster by infalling substructures