A Search For Large-Scale Structure at High Redshift
Abstract
We present new and exciting results on our search for large-scale structure at high redshift. Specifically, we have just completed a detailed analysis of the area surrounding the cluster CL0016+16 (z=0.546) and have the most compelling evidence yet that this cluster resides in the middle of a supercluster. From the distribution of galaxies and clusters we find that the supercluster appears to be a sheet of galaxies, viewed almost edge-on, with a radial extent of 31 Mpc, transverse dimension of 12 Mpc, and a thickness of ~4 Mpc. The surface density and velocity dispersion of this coherent structure are consistent with the properties of the ``Great Wall'' in the CfA redshift survey.
Cite
@article{arxiv.astro-ph/9702025,
title = {A Search For Large-Scale Structure at High Redshift},
author = {A. J. Connolly and A. S. Szalay and A. K. Romer and R. C. Nichol and B. Holden and D. Koo and T. Miyaji},
journal= {arXiv preprint arXiv:astro-ph/9702025},
year = {2007}
}
Comments
3 pages, Latex file, includes 3 postscript figures (uses sprocl.sty and psfig). To appear in: Proceedings of the 18th Texas Symposium in Relativistic Astrophysics, Chicago, 15-20th December 1996. See also http://tarkus.pha.jhu.edu/~ajc/papers/supercluster/sc.html