Using New Submillimetre Surveys to Identify the Evolutionary Status of High-z Galaxies
Astrophysics
2016-01-27 v1
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.
Keywords
Cite
@article{arxiv.astro-ph/9707255,
title = {Using New Submillimetre Surveys to Identify the Evolutionary Status of High-z Galaxies},
author = {D. H. Hughes and J. S. Dunlop},
journal= {arXiv preprint arXiv:astro-ph/9707255},
year = {2016}
}
Comments
6 pages, 3 postscript figures, LaTex uses Kluwer book style file crckapb10.sty, to appear in "Observational Cosmology with the New Radio Surveys", 13-15 January 1997, Puerto de la Cruz, Tenerife, M.Bremer, N.Jackson, I.Perez-Fournon (eds.), Kluwer