A next generation deep 2-mu m Survey: reconnoitering the dark ages

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
Other Authors: Swinburne University of Technology
Format: Article in Journal/Newspaper
Language:unknown
Published: CSIRO Publishing 2011
Subjects:
Antarctic
The Antarctic
Antarc*
Online Access:http://hdl.handle.net/1959.3/206379
https://doi.org/10.1071/as11036
id ftswinburne:tle:c2629586-ced8-4c5e-a9cb-e499e1f1e684:28f49f06-0da8-44be-9edc-ad1dd0a9c582:1
record_format openpolar
spelling ftswinburne:tle:c2629586-ced8-4c5e-a9cb-e499e1f1e684:28f49f06-0da8-44be-9edc-ad1dd0a9c582:1 2023-05-15T13:57:59+02:00 A next generation deep 2-mu m Survey: reconnoitering the dark ages Mould, Jeremy Swinburne University of Technology 2011 http://hdl.handle.net/1959.3/206379 https://doi.org/10.1071/as11036 unknown CSIRO Publishing http://purl.org/au-research/grants/arc/CE11E0090 http://hdl.handle.net/1959.3/206379 https://doi.org/10.1071/as11036 Copyright © 2011 Astronomical Society of Australia. The accepted manuscript is reproduced in accordance with the copyright policy of the publisher. Publications of the Astronomical Society of Australia, Vol. 28, no. 3 (2011), pp. 266-270 Journal article 2011 ftswinburne https://doi.org/10.1071/as11036 2019-09-07T21:44:36Z 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. Article in Journal/Newspaper Antarc* Antarctic Swinburne University of Technology: Swinburne Research Bank Antarctic The Antarctic Publications of the Astronomical Society of Australia 28 3 266 270
institution Open Polar
collection Swinburne University of Technology: Swinburne Research Bank
op_collection_id ftswinburne
language unknown
description 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.
author2 Swinburne University of Technology
format Article in Journal/Newspaper
author Mould, Jeremy
spellingShingle Mould, Jeremy
A next generation deep 2-mu m Survey: reconnoitering the dark ages
author_facet Mould, Jeremy
author_sort Mould, Jeremy
title A next generation deep 2-mu m Survey: reconnoitering the dark ages
title_short A next generation deep 2-mu m Survey: reconnoitering the dark ages
title_full A next generation deep 2-mu m Survey: reconnoitering the dark ages
title_fullStr A next generation deep 2-mu m Survey: reconnoitering the dark ages
title_full_unstemmed A next generation deep 2-mu m Survey: reconnoitering the dark ages
title_sort next generation deep 2-mu m survey: reconnoitering the dark ages
publisher CSIRO Publishing
publishDate 2011
url http://hdl.handle.net/1959.3/206379
https://doi.org/10.1071/as11036
geographic Antarctic
The Antarctic
geographic_facet Antarctic
The Antarctic
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_source Publications of the Astronomical Society of Australia, Vol. 28, no. 3 (2011), pp. 266-270
op_relation http://purl.org/au-research/grants/arc/CE11E0090
http://hdl.handle.net/1959.3/206379
https://doi.org/10.1071/as11036
op_rights Copyright © 2011 Astronomical Society of Australia. The accepted manuscript is reproduced in accordance with the copyright policy of the publisher.
op_doi https://doi.org/10.1071/as11036
container_title Publications of the Astronomical Society of Australia
container_volume 28
container_issue 3
container_start_page 266
op_container_end_page 270
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