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Article Contents

ABSTRACT

1.THE LYMAN-BREAK TECHNIQUE AND THE HDF: HOW DID THEY COME TO BE?

2.LYMAN-BREAK GALAXIES

3.THE SPECTRA OF THE LYMAN-BREAK GALAXIES

3.1.The rest-frame UV spectra

3.2.The rest-frame optical spectroscopy

4.THE LYMAN-BREAK GALAXY POPULATION

5.MORPHOLOGY

6.CLUSTERING

6.1.Large structures at high redshifts

6.2.The clustering of Lyman-break galaxies

6.3.Spatial clustering and its "evolution"

7.SUMMARY

REFERENCES