scholarly journals THE RED-SEQUENCE LUMINOSITY FUNCTION IN MASSIVE INTERMEDIATE-REDSHIFT GALAXY CLUSTERS

2008 ◽  
Vol 690 (2) ◽  
pp. 1158-1180 ◽  
Author(s):  
S. M. Crawford ◽  
M. A. Bershady ◽  
J. G. Hoessel
2010 ◽  
Vol 720 (1) ◽  
pp. 87-98 ◽  
Author(s):  
Rose A. Finn ◽  
Vandana Desai ◽  
Gregory Rudnick ◽  
Bianca Poggianti ◽  
Eric F. Bell ◽  
...  

2009 ◽  
Vol 700 (2) ◽  
pp. 1161-1172 ◽  
Author(s):  
Liyi Gu ◽  
Haiguang Xu ◽  
Junhua Gu ◽  
Yu Wang ◽  
Zhongli Zhang ◽  
...  

2014 ◽  
Vol 786 (1) ◽  
pp. 30 ◽  
Author(s):  
Steven M. Crawford ◽  
Gregory D. Wirth ◽  
Matthew A. Bershady

2004 ◽  
Vol 2004 (IAUC195) ◽  
Author(s):  
R. Pérez-Martínez ◽  
L. Metcalfe ◽  
D. Coia ◽  
A. Biviano ◽  
B. McBreen ◽  
...  

2008 ◽  
Vol 673 (2) ◽  
pp. 742-751 ◽  
Author(s):  
David G. Gilbank ◽  
H. K. C. Yee ◽  
E. Ellingson ◽  
M. D. Gladders ◽  
Y.‐S. Loh ◽  
...  

2015 ◽  
Vol 11 (S319) ◽  
pp. 62-62
Author(s):  
Rachel Paterno-Mahler ◽  
Elizabeth L. Blanton ◽  
Joshua Wing ◽  
M.L.N. Ashby ◽  
Mark Brodwin ◽  
...  

AbstractThe number of confirmed, high-redshift galaxy clusters is very low compared to the number of well-studied clusters nearby. Bent, double-lobed radio sources are frequently found in galaxy clusters, and thus can be used as tracers for efficiently locating high-redshift clusters. Using our Spitzer Snapshot Survey, we have identified approximately 300 potential new clusters with redshifts 0.7 < z < 3. These objects make up the high-redshift portion of the Cluster Occupied by Bent Radio AGN (COBRA) survey. We have created color-magnitude diagrams using infrared and optical data. Using the colors of the radio source host and the red sequence we can estimate redshifts for our clusters, as well as examine the evolution of the cluster galaxies over a large range of cosmic time.


2015 ◽  
Vol 11 (S319) ◽  
pp. 5-5
Author(s):  
Wayne A. Barkhouse ◽  
Haylee Archer ◽  
Jaford Burgad ◽  
Gregory Foote ◽  
Cody Rude ◽  
...  

AbstractWe investigate the alignment effect of red-sequence dwarf galaxies using a sample of 121 low-redshift galaxy clusters and cluster galaxies selected from the HST Frontier Fields.


2000 ◽  
Vol 544 (1) ◽  
pp. 109-116 ◽  
Author(s):  
Joseph J. Mohr ◽  
Erik D. Reese ◽  
E. Ellingson ◽  
Aaron D. Lewis ◽  
August E. Evrard

2016 ◽  
Vol 457 (2) ◽  
pp. 2209-2235 ◽  
Author(s):  
P. Cerulo ◽  
W. J. Couch ◽  
C. Lidman ◽  
R. Demarco ◽  
M. Huertas-Company ◽  
...  

2005 ◽  
Vol 201 ◽  
pp. 459-460
Author(s):  
Michael D. Gladders ◽  
H. K. C. Yee

The Red-Sequence Cluster Survey (RCS) is a 100 deg2 optical survey for high-redshift galaxy clusters. One of the goals of the survey is a measurement of Ωm and σ8 via the evolution of the mass spectrum of galaxy clusters. Herein we briefly describe how this will initially be done, and also demonstrate the eventual power of the RCS for this type of measurement by a qualitative analysis of the first 1/10th of the survey data.


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