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Next Generation Deep 2μm Survey

Published online by Cambridge University Press:  30 January 2013

Jeremy Mould
Jeremy Mould*
Affiliation:
Centre for Astrophysics and Supercomputing, Swinburne University, Hawthorn 3122, Australia
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Abstract

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There is a major opportunity for the KDUST 2.5 m telescope to carry out the next generation IR survey. A resolution of 0.2 arcsec is obtainable from Dome A over a wide field. This opens a unique discovery space during the 2015–2025 decade.

A next generation 2μm survey will feed JWST with serendipitous targets for spectroscopy, including spectra and images of the first galaxies.

Keywords

infraredsurveygalaxies
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S288: Astrophysics from Antarctica , August 2012 , pp. 239 - 242
Copyright
Copyright © International Astronomical Union 2013

References

Blandford, R. 2009, AAS, 213, 21301Google Scholar
Burton, M.G.et al. 2005, PASA, 22, 199.CrossRefGoogle Scholar
Cui, X. 2010, Highlights of Astronomy, 15, 639Google Scholar
Green, J.et al. 2012, astro-ph 1208.4012Google Scholar
Ilie, C., Freese, K., Valluri, M., Iliev, I. & Shapiro, P. 2012, MNRAS, 422, 2164CrossRefGoogle Scholar
wMcGregor, P., Hart, J., Stevanovic, D., Bloxham, G., Jones, D., VanAAAAHarmelen, J., Griesbach, J., Dawson, M., Young, P. & Jarnyk, M. 2004, SPIE, 5492, 1033Google Scholar
McGregor, P. J., Conroy, P., Bloxham, G. & vanAAAAHarmelen, J. 1999, PASA, 16, 273CrossRefGoogle Scholar
Mould, J. 2011, PASA, 28, 266Google Scholar
Thompson, R.et al. 2007, ApJ, 657, 669Google Scholar
Zhao, G-B., Zhan, H., Wang, L., Fan, Z. & Zhang, X. 2011, PASP, 123, 725Google Scholar