Dome Fuji in Antarctica as a Site for Infrared and Terahertz Astronomy
Abstract Dome Fuji on the Antarctic high plateau may be a good site for terahertz astronomy because of its high altitude of 3,810 m and low average temperature of −54°C. We have demonstrated that the opacity at 220 GHz from Dome Fuji in summer is very good and stable; τ = 0.045 ± 0.007. We have deve...
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crcambridgeupr:10.1017/s1743921312016961 2023-05-15T14:11:53+02:00 Dome Fuji in Antarctica as a Site for Infrared and Terahertz Astronomy Seta, Masumichi Nakai, Naomasa Ishii, Shun Nagai, Makoto Miyamoto, Yusuke Ichikawa, Takashi Takato, Naruhisa Motoyama, Hideaki 2012 http://dx.doi.org/10.1017/s1743921312016961 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921312016961 en eng Cambridge University Press (CUP) https://www.cambridge.org/core/terms Proceedings of the International Astronomical Union volume 8, issue S288, page 251-255 ISSN 1743-9213 1743-9221 Astronomy and Astrophysics Space and Planetary Science journal-article 2012 crcambridgeupr https://doi.org/10.1017/s1743921312016961 2022-04-07T08:06:36Z Abstract Dome Fuji on the Antarctic high plateau may be a good site for terahertz astronomy because of its high altitude of 3,810 m and low average temperature of −54°C. We have demonstrated that the opacity at 220 GHz from Dome Fuji in summer is very good and stable; τ = 0.045 ± 0.007. We have developed a transportable 30 cm telescope to map the Milky Way in the CO ( J =4–3) and the [CI] ( 3 P 1 – 3 P 0 ) lines at Dome Fuji from 2014. It has a 9′ beam. Physical conditions such as density and temperature of molecular clouds could be derived from a direct comparison of CO ( J =4–3) and [CI] ( 3 P 1 – 3 P 0 ) with CO ( J =1–0) taken by the Columbia–CfA survey. We are also developing a 1.2 m sub-millimeter telescope. It will be equipped with a dual superconducting device (SIS) receiver for 500/800 GHz. The 1.2 m telescope produces a 2.2′ beam at 492 GHz and could map a molecular cloud entirely. It could also observe nearby galaxies in the CO ( J =4–3), CO ( J =7–6), [CI] ( 3 P 1 – 3 P 0 ), [CI] ( 3 P 2 – 3 P 1 ) and in continuum emission between 460–810 GHz. Article in Journal/Newspaper Antarc* Antarctic Antarctica Cambridge University Press (via Crossref) Antarctic Dome Fuji ENVELOPE(39.700,39.700,-77.317,-77.317) Milky Way ENVELOPE(-68.705,-68.705,-71.251,-71.251) The Antarctic Proceedings of the International Astronomical Union 8 S288 251 255 |
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Cambridge University Press (via Crossref) |
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English |
topic |
Astronomy and Astrophysics Space and Planetary Science |
spellingShingle |
Astronomy and Astrophysics Space and Planetary Science Seta, Masumichi Nakai, Naomasa Ishii, Shun Nagai, Makoto Miyamoto, Yusuke Ichikawa, Takashi Takato, Naruhisa Motoyama, Hideaki Dome Fuji in Antarctica as a Site for Infrared and Terahertz Astronomy |
topic_facet |
Astronomy and Astrophysics Space and Planetary Science |
description |
Abstract Dome Fuji on the Antarctic high plateau may be a good site for terahertz astronomy because of its high altitude of 3,810 m and low average temperature of −54°C. We have demonstrated that the opacity at 220 GHz from Dome Fuji in summer is very good and stable; τ = 0.045 ± 0.007. We have developed a transportable 30 cm telescope to map the Milky Way in the CO ( J =4–3) and the [CI] ( 3 P 1 – 3 P 0 ) lines at Dome Fuji from 2014. It has a 9′ beam. Physical conditions such as density and temperature of molecular clouds could be derived from a direct comparison of CO ( J =4–3) and [CI] ( 3 P 1 – 3 P 0 ) with CO ( J =1–0) taken by the Columbia–CfA survey. We are also developing a 1.2 m sub-millimeter telescope. It will be equipped with a dual superconducting device (SIS) receiver for 500/800 GHz. The 1.2 m telescope produces a 2.2′ beam at 492 GHz and could map a molecular cloud entirely. It could also observe nearby galaxies in the CO ( J =4–3), CO ( J =7–6), [CI] ( 3 P 1 – 3 P 0 ), [CI] ( 3 P 2 – 3 P 1 ) and in continuum emission between 460–810 GHz. |
format |
Article in Journal/Newspaper |
author |
Seta, Masumichi Nakai, Naomasa Ishii, Shun Nagai, Makoto Miyamoto, Yusuke Ichikawa, Takashi Takato, Naruhisa Motoyama, Hideaki |
author_facet |
Seta, Masumichi Nakai, Naomasa Ishii, Shun Nagai, Makoto Miyamoto, Yusuke Ichikawa, Takashi Takato, Naruhisa Motoyama, Hideaki |
author_sort |
Seta, Masumichi |
title |
Dome Fuji in Antarctica as a Site for Infrared and Terahertz Astronomy |
title_short |
Dome Fuji in Antarctica as a Site for Infrared and Terahertz Astronomy |
title_full |
Dome Fuji in Antarctica as a Site for Infrared and Terahertz Astronomy |
title_fullStr |
Dome Fuji in Antarctica as a Site for Infrared and Terahertz Astronomy |
title_full_unstemmed |
Dome Fuji in Antarctica as a Site for Infrared and Terahertz Astronomy |
title_sort |
dome fuji in antarctica as a site for infrared and terahertz astronomy |
publisher |
Cambridge University Press (CUP) |
publishDate |
2012 |
url |
http://dx.doi.org/10.1017/s1743921312016961 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/S1743921312016961 |
long_lat |
ENVELOPE(39.700,39.700,-77.317,-77.317) ENVELOPE(-68.705,-68.705,-71.251,-71.251) |
geographic |
Antarctic Dome Fuji Milky Way The Antarctic |
geographic_facet |
Antarctic Dome Fuji Milky Way The Antarctic |
genre |
Antarc* Antarctic Antarctica |
genre_facet |
Antarc* Antarctic Antarctica |
op_source |
Proceedings of the International Astronomical Union volume 8, issue S288, page 251-255 ISSN 1743-9213 1743-9221 |
op_rights |
https://www.cambridge.org/core/terms |
op_doi |
https://doi.org/10.1017/s1743921312016961 |
container_title |
Proceedings of the International Astronomical Union |
container_volume |
8 |
container_issue |
S288 |
container_start_page |
251 |
op_container_end_page |
255 |
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1766284115936542720 |