In this review, we presented results from parallel and other deep HST
surveys. In Section 2,
we summarized HST's morphological evidence for the evolution of
different galaxy types
for 19 
B
27.5 mag: early types
(E/S0's and Sabc's) evolved the least since z
1, and late types (Sd/Irr's+Mergers) most rapidly. With better restframe
ANN's, these
results can be extended in the HDF and in future deep NICMOS and ACS images for
B 29 or H
25 mag. This will cover
the bulk of galaxies in the range z ~ 1-3. In
Section 2 we summarized the WFPC2 F410M
medium band searches for faint compact
Ly
emitting objects at z 
2.4. The unexpected success of finding these objects provides
an important confirmation of CDM theories, leads us to the question
whether or not all
high z star-forming systems are obscured by dust, and provides
clues as to where the
long sought Ly emitting
primeval galaxies may be hiding - in many small pieces. The
existence of any larger scale structure at z
2-3 clearly begs further
investigation. In
Section 3, the radio galaxy 53W002 provided
important clues as to how a luminous early-type
galaxy seen today may have formed. For this object at least, this may
have started with
jet-induced star-formation (with an aligned cone associated with its
AGN), soon followed
by the formation of an r1/4-like bulge and within a
few Gyr by a massive disk, which may
get destroyed later by subsequent mergers with the surrounding
sub-galactic objects.
We thank Lee Armus, Nick Scoville, and Dave Burstein for helpful discussion, Doug VanOrsow, Harry Ferguson, Ray Lucas, and the ST ScI staff for their continuous help in these projects, and ST ScI for an inspiring HDF Symposium. Spectroscopic observations were obtained at the Multiple Mirror Telescope Observatory, a joint facility of the University of Arizona and the Smithsonian Institution. Kitt Peak National Observatory is operated by the Association of Universities for Research in Astronomy, Inc., under contract with the NSF. From 1994-1997, much of this work was supported by NASA grants GO-5308.0*-93A, GO-5985.0*-94A & GO-6610.0*-95A (to RAW and WCK), GO.2684.03.94A (to RAW), and GO-6609.0*-95A & AR.6385.01.95A (to RAW and SCO) from ST ScI, which is operated by AURA, Inc., under NASA contract NAS5-26555.