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

Published online by Cambridge University Press:  02 January 2013

Jeremy Mould
Jeremy Mould
Affiliation:
Swinburne University, Hawthorn Vic 3122, Australia. Email: [email protected] ARC Centre of Excellence for All-sky Astrophysics (CAASTRO)
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Abstract

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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.

Keywords

infrared: generalgalaxies: high redshifttelescopes
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 28 , Issue 3 , 2011 , pp. 266 - 270
Copyright
Copyright © Astronomical Society of Australia 2011

References

Ashley, M. C. B., Burton, M. G., Storey, J. W. V., Lloyd, J. P., Bally, J., Briggs, J. & Harper, D. A., 1996, PASP, 108, 721CrossRefGoogle Scholar
Burton, M. G., Burgarella, D., Andersen, M., Busso, M., Eiroa, C., Epchtein, N., Maillard, J.-P. & Persi, P., 2010, EAS, 40, 125Google Scholar
Ichikawa, T., 2010, Highlights of Astronomy, 15, 632Google Scholar
Kaiser, N. et al. , 2010, SPIE, 7733, 12Google Scholar
Lawrence, A. et al. , 2007, MNRAS, 379, 1599Google Scholar
Lawrence, J. S., Ashley, M. C. B., Burton, M. G. & Storey, J. W. V. 2002a, in Proc. SPIE, Vol. 4836, Survey and Other Telescope Technologies and Discoveries, eds Tyson, J. Anthony & Wolff, S., 129CrossRefGoogle Scholar
Lawrence, J. S., Ashley, M. C. B., Burton, M. G., Calisse, P. G., Everett, J. R., Pernic, R. J., Phillips, A. & Storey, J. W. V., 2002b, PASA, 19, 328CrossRefGoogle Scholar
Lawrence, J. et al. , 2009, PASA, 26, 415CrossRefGoogle Scholar
Lascaux, F., Masciadri, E. & Hagelin, S., 2011, MNRAS, 411, 693Google Scholar
Leitherer, C., Schaerer, D., Goldader, J. D., González Delgado, R. M., Robert, C., Kune, D. F., de Mello, D. F. & Devost, D., 1999, ApJS, 123, 3CrossRefGoogle Scholar
Matsumoto, T., Matsuura, S. & Noda, M., 1994, PASP, 106, 1217CrossRefGoogle Scholar
Levi, M., Kim, A., Lampton, M. & Sholl, M., 2011, astro-ph 1105.0959Google Scholar
Ota, K. et al. , 2010, ApJ, 722, 803CrossRefGoogle Scholar
Rousselot, P., Lidman, C., Cuby, J.-G., Moreels, G. & Monnet, G., 2000, A&A, 354, 1134Google Scholar
Saunders, W., Gillingham, P., McGrath, A., Haynes, R., Brzeski, J., Storey, J. & Lawrence, J., 2008, SPIE, 7012, 151Google Scholar
Skrutskie, M. et al. , 2006, AJ, 131, 1163CrossRefGoogle Scholar
Sutherland, W., 2008, EAS, 33, 83Google Scholar
Wright, E., 2001, ApJ, 553, 538CrossRefGoogle Scholar
Wright, E., 2006, PASP, 118, 1711CrossRefGoogle Scholar
Zhao, J., Wang, D., Yuan, X. & Wang, J., 2010, SPIE, 7658, 40Google Scholar