A Next Generation Deep 2-μm Survey: Reconnoitering the Dark Ages

Abstract The next generation 2-μm sky survey should target nascent galaxies in the epoch of reionization for spectroscopic followup on large telescopes. A 2.5-m telescope at a site on the Antarctic plateau has advantages for this purpose and for southern hemisphere infrared surveys in general.

Bibliographic Details
Published in:Publications of the Astronomical Society of Australia
Main Author: Mould, Jeremy
Format: Article in Journal/Newspaper
Language:English
Published: Cambridge University Press (CUP) 2011
Subjects:
Online Access:http://dx.doi.org/10.1071/as11036
https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1323358000000862
Description
Summary:Abstract The next generation 2-μm sky survey should target nascent galaxies in the epoch of reionization for spectroscopic followup on large telescopes. A 2.5-m telescope at a site on the Antarctic plateau has advantages for this purpose and for southern hemisphere infrared surveys in general.