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.
Published in: | Publications of the Astronomical Society of Australia |
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Format: | Article in Journal/Newspaper |
Language: | English |
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Cambridge University Press (CUP)
2011
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Online Access: | http://dx.doi.org/10.1071/as11036 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1323358000000862 |
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. |
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