  We have made spectroscopic identifications of 39 additional quasar candidates
from the Deep Multicolor Survey (DMS) of Hall et al. (1996, ApJ, 462, 614,
astro-ph/9512052). We have identified 9 new quasars with 0.3 < z < 2.8 and 16.8
< B < 21.6, all from the group of candidates with ultraviolet excess (UVX). No
new quasars with z > 3 were found among the observed candidates selected due to
their red (B-R) and (V-R) colors. As a result, there are now 55 confirmed
quasars in the survey: 42 with 0.3 < z < 2, nine with 2 < z < 3, three with 3 <
z < 4, and 1 at z = 4.3. One new quasar, DMS 0059-0055, is very bright with
B=16.8 and z=0.3, making its detection by our survey very unexpected. Including
this new spectroscopy, the results of the DMS are converging with the predicted
space densities of other surveys. In particular, we no longer find an excess of
quasars with z < 2.3 and B < 21 in the survey over predictions based on models
by Koo & Kron. Also, the excess in the number of quasars seen at z > 3 over
predictions based on models by Warren, Hewett, & Osmer is less than previously
suggested. We also demonstrate the success of our quasar color modeling which
is important in assessing the completeness of our survey.
