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Article Contents

ABSTRACT

1.INTRODUCTION

1.1.Faint galaxy classifications with HST

1.2.Clues to galaxy formation with HST

1.3.Where and why are the primeval galaxies hiding?

1.4.Confrontation of recent HST results with CDM models

1.5.How much clustering is allowed at high redshifts and on what scales?

1.6.Clues from the formation of a weak radio galaxy

2.AUTOMATED MORPHOLOGICAL CLASSIFICATION IN DEEP HST FIELDS

2.1.WFPC2 observations, reduction, and ANN classifications

2.2.WFPC2 B-band results and discussion

3.SUBGALACTIC CLUMPS AT Z 2.4 & IMPLICATIONS FOR GALAXY FORMATION

3.1.Deep F410M surveys for faint Ly emitting candidates at z 2.4

3.2.Details of the WFPC2 F410M search for Ly emitting z 2.4 candidates

3.3.Faint blue sub-galactic clumps

3.4.Discussion of surveys for faint Ly emitting candidates at z 2.4

3.5.Future prospect for space-based Ly surveys

4.DEEP PC IMAGING OF A COMPACT RADIO GALAXY AT Z = 2.390

4.1.WFPC2 observations and astrometry

4.2.Structure of the PC images of 53W002

4.3.Discussion and conclusions

5.SUMMARY

REFERENCES