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Article Contents
- ABSTRACT
- 1.INTRODUCTION
- 2.DETECTION OF MOLECULAR GAS AT HIGH
REDSHIFT
- 2.1.Emission lines
- 2.2.Absorption lines
- 3.DETECTION OF DUST AT HIGH REDSHIFT
- 3.1.Submm continuum surveys
- 3.2.Extremely red objects, EROs
- 3.3.AGN or Starbursts
- 3.4.Star Formation Rate
- 4.PERSPECTIVES WITH FUTURE MM INSTRUMENTS
- 4.1.Predicted Line and Continuum
Fluxes
- 4.2.Source Counts
- 5.CONCLUSION
- REFERENCES