  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.
