Science goals for an Antarctic large infrared telescope

Over the past few years, site-testing at the South Pole has revealed conditions that are uniquely favorable for IR astronomy. In particular, the exceptionally low sky brightness throughout the near- and mid-IR leads to the possibility of a modest-sized telescope achieving comparable sensitivity to t...

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Bibliographic Details
Main Authors: Burton, Michael, Storey, John, Ashley, Michael
Format: Conference Object
Language:English
Published: 2000
Subjects:
Online Access:http://hdl.handle.net/1959.4/38602
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spelling ftunswworks:oai:unsworks.library.unsw.edu.au:1959.4/38602 2023-05-15T13:52:09+02:00 Science goals for an Antarctic large infrared telescope Burton, Michael Storey, John Ashley, Michael 2000 http://hdl.handle.net/1959.4/38602 EN eng http://hdl.handle.net/1959.4/38602 metadata only access http://purl.org/coar/access_right/c_14cb CC BY-NC-ND 3.0 https://creativecommons.org/licenses/by-nc-nd/3.0/au/ © 2003 COPYRIGHT SPIE--The International Society for Optical Engineering. CC-BY-NC-ND Discoveries and Research Prospects from 8- to 10-Meter-Class Telescopes, Munich, Germany conference paper http://purl.org/coar/resource_type/c_5794 2000 ftunswworks 2022-08-09T07:40:53Z Over the past few years, site-testing at the South Pole has revealed conditions that are uniquely favorable for IR astronomy. In particular, the exceptionally low sky brightness throughout the near- and mid-IR leads to the possibility of a modest-sized telescope achieving comparable sensitivity to that of existing 8-10 meter class telescopes. An 8m Antarctic telescope, if constructed, would yield performance that would be unrivaled until the advent of the NGST. In this paper we review the scientific potential of IR telescopes in Antarctica, and discuss their complementarity with existing 8-10m class telescopes. Conference Object Antarc* Antarctic Antarctica South pole South pole UNSW Sydney (The University of New South Wales): UNSWorks Antarctic South Pole
institution Open Polar
collection UNSW Sydney (The University of New South Wales): UNSWorks
op_collection_id ftunswworks
language English
description Over the past few years, site-testing at the South Pole has revealed conditions that are uniquely favorable for IR astronomy. In particular, the exceptionally low sky brightness throughout the near- and mid-IR leads to the possibility of a modest-sized telescope achieving comparable sensitivity to that of existing 8-10 meter class telescopes. An 8m Antarctic telescope, if constructed, would yield performance that would be unrivaled until the advent of the NGST. In this paper we review the scientific potential of IR telescopes in Antarctica, and discuss their complementarity with existing 8-10m class telescopes.
format Conference Object
author Burton, Michael
Storey, John
Ashley, Michael
spellingShingle Burton, Michael
Storey, John
Ashley, Michael
Science goals for an Antarctic large infrared telescope
author_facet Burton, Michael
Storey, John
Ashley, Michael
author_sort Burton, Michael
title Science goals for an Antarctic large infrared telescope
title_short Science goals for an Antarctic large infrared telescope
title_full Science goals for an Antarctic large infrared telescope
title_fullStr Science goals for an Antarctic large infrared telescope
title_full_unstemmed Science goals for an Antarctic large infrared telescope
title_sort science goals for an antarctic large infrared telescope
publishDate 2000
url http://hdl.handle.net/1959.4/38602
geographic Antarctic
South Pole
geographic_facet Antarctic
South Pole
genre Antarc*
Antarctic
Antarctica
South pole
South pole
genre_facet Antarc*
Antarctic
Antarctica
South pole
South pole
op_source Discoveries and Research Prospects from 8- to 10-Meter-Class Telescopes, Munich, Germany
op_relation http://hdl.handle.net/1959.4/38602
op_rights metadata only access
http://purl.org/coar/access_right/c_14cb
CC BY-NC-ND 3.0
https://creativecommons.org/licenses/by-nc-nd/3.0/au/
© 2003 COPYRIGHT SPIE--The International Society for Optical Engineering.
op_rightsnorm CC-BY-NC-ND
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