Clustering in the Caltech Faint Galaxy Redshift Survey

Abstract

The Caltech Faint Galaxy Redshift Survey has collected $\sim$2000 spectra taken with multi-slit masks using the Low Resolution Imaging Spectrograph at the Keck Observatory (Oke et al 1995) in two widely separated fields on the sky, each $\sim$1 x 1 deg$^2$. Most of these objects are faint field galaxies; about 10% are Galactic stars and about 1% are broad-lined AGNs. I summarize the small scale clustering of this sample as well as the evidence in support of large scale structure.

To appear in proceedings of conference Clustering At High Redshift, ASP Conf. Series, ed. A. Mazuer and O.Le Fevre (Marseilles, July 1999). 7 pages, 4 figures, reformatted from pasptex to aastex