.:Analysis:.

-Comparison Cluster SFRs over z-

After the mass normalizations of the average SFRs of each cluster was obtained, they were correlated against the mass-normalized SFRs of low and high redshift cluster, as presented in Finn et al 2005. Trends in average SFR of cluster were identified as the age of the universe increased.

Progression of SFR (Msol/yr/1e14 Msol) with z

Redshift

Low z

Mid z

High z

Sum SFR/Mcl/1e14 Msol in Clusters

6.97

182.66

52.18

0.80

50.78

12.97

1.78

181.17

19.33

72.01

 

71.60

Average

20.39

138.21

39.02

Text Box: As shown in the data table, there is a large spike in SFR at the intermediate redshift range