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Using New Submillimetre Surveys to Identify the Evolutionary Status of High-z Galaxies

D. H. Hughes·J. S. Dunlop
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Abstract

This paper describes a key submillimetre survey which we are currently conducting to address some of the outstanding questions in cosmology - how, at what epoch and over what period of time did massive galaxies form at high redshift? A summary of the technical feasibility of future submillimetre observations with new ground-based, airborne and satellite telescopes is also presented.

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D. H. Hughes, J. S. Dunlop. 1997-07-23. Using New Submillimetre Surveys to Identify the Evolutionary Status of High-z Galaxies. https://doi.org/10.1007/978-94-011-5238-9_46

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