Gattini 2010: Cutting Edge Science at the Bottom of the World
The high altitude Antarctic sites of Dome A and the South Pole offer intriguing locations for future large scale optical astronomical Observatories. The Gattini project was created to measure the optical sky brightness, large area cloud cover and aurora of the winter-time sky above such high altitud...
Published in: | SPIE Proceedings, Ground-based and Airborne Telescopes III |
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Online Access: | https://doi.org/10.1117/12.858187 |
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ftcaltechauth:oai:authors.library.caltech.edu:x0j8q-46843 2024-09-15T17:42:28+00:00 Gattini 2010: Cutting Edge Science at the Bottom of the World Moore, Anna M. Ahmed, Sara Ashley, Michael C. B. Barreto, Max K. Cui, Xiangqun Delacroix, Alex Feng, LongLong Gong, Xuefei Lawrence, Jon Luong-van, Daniel M. Martin, D. Christopher Riddle, Reed Rowley, Nicole Shang, Zhaohui Storey, John W. V. Tothill, Nick F. H. Travouillon, Tony Wang, Lifan Yang, Huigen Yang, Ji Zhou, Xu Zhu, Zhengxi Stepp, Larry M. Gilmozzi, Roberto Hall, Helen J. 2010 https://doi.org/10.1117/12.858187 unknown Society of Photo-optical Instrumentation Engineers (SPIE) https://doi.org/10.1117/12.858187 oai:authors.library.caltech.edu:x0j8q-46843 eprintid:22891 resolverid:CaltechAUTHORS:20110315-091730089 info:eu-repo/semantics/openAccess Other Conference on Ground-Based and Airborne Telescopes III, San Diego, CA, June 27-July 2, 2010 Gattini Dome A PLATO observatory Antarctic wide field surveys cosmic web site testing cloud cover aurora night sky brightness info:eu-repo/semantics/bookPart 2010 ftcaltechauth https://doi.org/10.1117/12.858187 2024-08-06T15:35:00Z The high altitude Antarctic sites of Dome A and the South Pole offer intriguing locations for future large scale optical astronomical Observatories. The Gattini project was created to measure the optical sky brightness, large area cloud cover and aurora of the winter-time sky above such high altitude Antarctic sites. The Gattini-DomeA camera was installed on the PLATO instrument module as part of the Chinese-led traverse to the highest point on the Antarctic plateau in January 2008. This single automated wide field camera contains a suite of Bessel photometric filters (B, V, R) and a long-pass red filter for the detection and monitoring of OH emission. We have in hand one complete winter-time dataset (2009) from the camera that was recently returned in April 2010. The Gattini-South Pole UV camera is a wide-field optical camera that in 2011 will measure for the first time the UV properties of the winter-time sky above the South Pole dark sector. This unique dataset will consist of frequent images taken in both broadband U and B filters in addition to high resolution (R similar to 5000) long slit spectroscopy over a narrow bandwidth of the central field. The camera is a proof of concept for the 2m-class Antarctic Cosmic Web Imager telescope, a dedicated experiment to directly detect and map the redshifted lyman alpha fluorescence or Cosmic Web emission we believe possible due to the unique geographical qualities of the site. We present the current status of both projects. © 2010 SPIE. This research is supported by the Chinese PANDA International Polar Year project and the Polar Research Institute of China. The authors wish to thank all the members of the 20081200912010 PRIC Dome A expeditions for their heroic efforts in reaching the site and for providing invaluable assistance to the expedition astronomers in setting up the PLATO observatory and its associated instrument suite. This research is financially supported by the US National Science Foundation and the United States Antarctic Program. The operation of ... Book Part Antarc* Antarctic International Polar Year Polar Research Institute of China South pole South pole United States Antarctic Program Caltech Authors (California Institute of Technology) SPIE Proceedings, Ground-based and Airborne Telescopes III 7733 77331S |
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Open Polar |
collection |
Caltech Authors (California Institute of Technology) |
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language |
unknown |
topic |
Gattini Dome A PLATO observatory Antarctic wide field surveys cosmic web site testing cloud cover aurora night sky brightness |
spellingShingle |
Gattini Dome A PLATO observatory Antarctic wide field surveys cosmic web site testing cloud cover aurora night sky brightness Moore, Anna M. Ahmed, Sara Ashley, Michael C. B. Barreto, Max K. Cui, Xiangqun Delacroix, Alex Feng, LongLong Gong, Xuefei Lawrence, Jon Luong-van, Daniel M. Martin, D. Christopher Riddle, Reed Rowley, Nicole Shang, Zhaohui Storey, John W. V. Tothill, Nick F. H. Travouillon, Tony Wang, Lifan Yang, Huigen Yang, Ji Zhou, Xu Zhu, Zhengxi Gattini 2010: Cutting Edge Science at the Bottom of the World |
topic_facet |
Gattini Dome A PLATO observatory Antarctic wide field surveys cosmic web site testing cloud cover aurora night sky brightness |
description |
The high altitude Antarctic sites of Dome A and the South Pole offer intriguing locations for future large scale optical astronomical Observatories. The Gattini project was created to measure the optical sky brightness, large area cloud cover and aurora of the winter-time sky above such high altitude Antarctic sites. The Gattini-DomeA camera was installed on the PLATO instrument module as part of the Chinese-led traverse to the highest point on the Antarctic plateau in January 2008. This single automated wide field camera contains a suite of Bessel photometric filters (B, V, R) and a long-pass red filter for the detection and monitoring of OH emission. We have in hand one complete winter-time dataset (2009) from the camera that was recently returned in April 2010. The Gattini-South Pole UV camera is a wide-field optical camera that in 2011 will measure for the first time the UV properties of the winter-time sky above the South Pole dark sector. This unique dataset will consist of frequent images taken in both broadband U and B filters in addition to high resolution (R similar to 5000) long slit spectroscopy over a narrow bandwidth of the central field. The camera is a proof of concept for the 2m-class Antarctic Cosmic Web Imager telescope, a dedicated experiment to directly detect and map the redshifted lyman alpha fluorescence or Cosmic Web emission we believe possible due to the unique geographical qualities of the site. We present the current status of both projects. © 2010 SPIE. This research is supported by the Chinese PANDA International Polar Year project and the Polar Research Institute of China. The authors wish to thank all the members of the 20081200912010 PRIC Dome A expeditions for their heroic efforts in reaching the site and for providing invaluable assistance to the expedition astronomers in setting up the PLATO observatory and its associated instrument suite. This research is financially supported by the US National Science Foundation and the United States Antarctic Program. The operation of ... |
author2 |
Stepp, Larry M. Gilmozzi, Roberto Hall, Helen J. |
format |
Book Part |
author |
Moore, Anna M. Ahmed, Sara Ashley, Michael C. B. Barreto, Max K. Cui, Xiangqun Delacroix, Alex Feng, LongLong Gong, Xuefei Lawrence, Jon Luong-van, Daniel M. Martin, D. Christopher Riddle, Reed Rowley, Nicole Shang, Zhaohui Storey, John W. V. Tothill, Nick F. H. Travouillon, Tony Wang, Lifan Yang, Huigen Yang, Ji Zhou, Xu Zhu, Zhengxi |
author_facet |
Moore, Anna M. Ahmed, Sara Ashley, Michael C. B. Barreto, Max K. Cui, Xiangqun Delacroix, Alex Feng, LongLong Gong, Xuefei Lawrence, Jon Luong-van, Daniel M. Martin, D. Christopher Riddle, Reed Rowley, Nicole Shang, Zhaohui Storey, John W. V. Tothill, Nick F. H. Travouillon, Tony Wang, Lifan Yang, Huigen Yang, Ji Zhou, Xu Zhu, Zhengxi |
author_sort |
Moore, Anna M. |
title |
Gattini 2010: Cutting Edge Science at the Bottom of the World |
title_short |
Gattini 2010: Cutting Edge Science at the Bottom of the World |
title_full |
Gattini 2010: Cutting Edge Science at the Bottom of the World |
title_fullStr |
Gattini 2010: Cutting Edge Science at the Bottom of the World |
title_full_unstemmed |
Gattini 2010: Cutting Edge Science at the Bottom of the World |
title_sort |
gattini 2010: cutting edge science at the bottom of the world |
publisher |
Society of Photo-optical Instrumentation Engineers (SPIE) |
publishDate |
2010 |
url |
https://doi.org/10.1117/12.858187 |
genre |
Antarc* Antarctic International Polar Year Polar Research Institute of China South pole South pole United States Antarctic Program |
genre_facet |
Antarc* Antarctic International Polar Year Polar Research Institute of China South pole South pole United States Antarctic Program |
op_source |
Conference on Ground-Based and Airborne Telescopes III, San Diego, CA, June 27-July 2, 2010 |
op_relation |
https://doi.org/10.1117/12.858187 oai:authors.library.caltech.edu:x0j8q-46843 eprintid:22891 resolverid:CaltechAUTHORS:20110315-091730089 |
op_rights |
info:eu-repo/semantics/openAccess Other |
op_doi |
https://doi.org/10.1117/12.858187 |
container_title |
SPIE Proceedings, Ground-based and Airborne Telescopes III |
container_volume |
7733 |
container_start_page |
77331S |
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1810489046270476288 |