THz Astrophysics from Dome A
The THz spectral region includes a number of important transitions which allow us to trace the evolution of the interstellar medium. Because of the opacity of the atmosphere in this spectral range, the best sites for ground-based THz observations are on the Antarctic Plateau; of these sites, Dome A...
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Published in | EAS publications series Vol. 40; pp. 275 - 280 |
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Main Authors | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
Published |
EDP Sciences
2010
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Subjects | |
Online Access | Get full text |
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Summary: | The THz spectral region includes a number of important transitions which allow us to trace the evolution of the interstellar medium. Because of the opacity of the atmosphere in this spectral range, the best sites for ground-based THz observations are on the Antarctic Plateau; of these sites, Dome A is expected to be the best. THz survey science can be carried out with small telescopes, easing logistical constraints. By deploying a submillimetre-wave tipper/ telescope to Dome A, we have trialled several technologies for such an instrument, and we are able to test whether the site quality is sufficient for THz surveys. |
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Bibliography: | publisher-ID:eas1040040 PII:S1633476040000404 other:2010EAS....40..275T ark:/67375/80W-7644FD0J-G istex:B3AD225530A242A72502CE8924A646A42D12DD40 ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 |
ISSN: | 1633-4760 1638-1963 |
DOI: | 10.1051/eas/1040040 |