The Norris Survey of the Corona Borealis Supercluster

@inproceedings{Small1996TheNS,
  title={The Norris Survey of the Corona Borealis Supercluster},
  author={Todd A. Small and Chung-Pei Ma and Wallace L. W. Sargent and Donald Hamilton},
  year={1996}
}
We present a study of the structure and dynamics of the Corona Borealis supercluster (z ≈ 0.07) based on the redshifts of 528 galaxies in the supercluster. The galaxy distribution within Corona Borealis is clumpy and appears overall to be far from relaxed. Approximately one-third of the supercluster galaxies lie outside of the Abell clusters in the supercluster. A background supercluster at z ≈ 0.11 makes a substantial contribution to the projected surface density of galaxies in the Corona… 
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We measure the field galaxy luminosity function (LF) as a function of color and redshift from z = 0 to z = 0.5 using galaxies from the Norris Survey of the Corona Borealis Supercluster. The data set
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