Motivations for Imaging Spectroscopy at Dome C
Antarctica offers unique conditions for ground-based observations, such as low sky background in the infrared, improved seeing, and low turbulence and scintillation noise. These properties are particularly beneficial to imaging, precision photometry, and infrared observations. It may be less clear i...
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ftdatacite:10.48550/arxiv.0812.3726 2023-05-15T14:03:03+02:00 Motivations for Imaging Spectroscopy at Dome C Kelz, Andreas 2008 https://dx.doi.org/10.48550/arxiv.0812.3726 https://arxiv.org/abs/0812.3726 unknown arXiv https://dx.doi.org/10.1051/eas:0833033 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Astrophysics astro-ph FOS Physical sciences article-journal Article ScholarlyArticle Text 2008 ftdatacite https://doi.org/10.48550/arxiv.0812.3726 https://doi.org/10.1051/eas:0833033 2022-04-01T14:54:32Z Antarctica offers unique conditions for ground-based observations, such as low sky background in the infrared, improved seeing, and low turbulence and scintillation noise. These properties are particularly beneficial to imaging, precision photometry, and infrared observations. It may be less clear if Antarctica offers equally compelling advantages for spectroscopy, in particular in the optical domain. However, scientific programmes that make use of imaging (or 3D) spectroscopy for selected follow-up studies of IR surveys, long-term monitoring of extended targets and resolved stellar population studies in crowded fields, also benefit from the site conditions at Dome C. : 4 pages, in: 2nd ARENA Conference: The Astrophysical Science Case at Dome C, H. Zinnecker, N. Epchtein & H. Rauer (eds) Text Antarc* Antarctica DataCite Metadata Store (German National Library of Science and Technology) |
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DataCite Metadata Store (German National Library of Science and Technology) |
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Astrophysics astro-ph FOS Physical sciences |
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Astrophysics astro-ph FOS Physical sciences Kelz, Andreas Motivations for Imaging Spectroscopy at Dome C |
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Astrophysics astro-ph FOS Physical sciences |
description |
Antarctica offers unique conditions for ground-based observations, such as low sky background in the infrared, improved seeing, and low turbulence and scintillation noise. These properties are particularly beneficial to imaging, precision photometry, and infrared observations. It may be less clear if Antarctica offers equally compelling advantages for spectroscopy, in particular in the optical domain. However, scientific programmes that make use of imaging (or 3D) spectroscopy for selected follow-up studies of IR surveys, long-term monitoring of extended targets and resolved stellar population studies in crowded fields, also benefit from the site conditions at Dome C. : 4 pages, in: 2nd ARENA Conference: The Astrophysical Science Case at Dome C, H. Zinnecker, N. Epchtein & H. Rauer (eds) |
format |
Text |
author |
Kelz, Andreas |
author_facet |
Kelz, Andreas |
author_sort |
Kelz, Andreas |
title |
Motivations for Imaging Spectroscopy at Dome C |
title_short |
Motivations for Imaging Spectroscopy at Dome C |
title_full |
Motivations for Imaging Spectroscopy at Dome C |
title_fullStr |
Motivations for Imaging Spectroscopy at Dome C |
title_full_unstemmed |
Motivations for Imaging Spectroscopy at Dome C |
title_sort |
motivations for imaging spectroscopy at dome c |
publisher |
arXiv |
publishDate |
2008 |
url |
https://dx.doi.org/10.48550/arxiv.0812.3726 https://arxiv.org/abs/0812.3726 |
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Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_relation |
https://dx.doi.org/10.1051/eas:0833033 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.0812.3726 https://doi.org/10.1051/eas:0833033 |
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1766273546438311936 |