Back to the article index

Article Contents

ABSTRACT

1.INTRODUCTION

2.HOW THE HDF CAME TO BE

3.THE HIGHLIGHTS

3.1.The flattening of the count slope N(m)

3.2.The small angular sizes of the faintest galaxies

3.3.The increasing fraction of irregular and multiple component systems

3.4.The location of high redshift galaxies with modest star formation rates

3.5.Constraints on the redshift distribution of the faintest systems

4.THE UPSHOT

5.WHERE NEXT?

6.CONCLUSIONS

REFERENCES