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题名: Optimising the K Dark Filter for the Kunlun Infrared Sky Survey
作者: Li, Yushan1; Zheng, Jessica2; Tuthill, Peter1; Freeman, Matthew3; Ashley, Michael3; Burton, Michael3; Lawrence, Jon2; Mould, Jeremy4; Wang LiFan(王力帆)5, 6, 7
刊名: PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA
出版日期: 2016-03-10
卷号: 33
关键词: infrared: general ; stars: protostars ; supernovae: general ; surveys ; techniques: photometric
DOI: 10.1017/pasa.2016.5
文章类型: Article
英文摘要: The Kunlun Infrared Sky Survey will be the first comprehensive exploration of the time varying Universe in the infrared. A key feature in optimising the scientific yield of this ambitious research programme is the choice of the survey passband. In particular, the survey aims to maximally exploit the unique thermal and atmospheric conditions pertaining to the high Antarctic site. By simulating the expected signal-to-noise for varying filter properties within the so-called 'K-DARK' 2.4 mu m window, filter performance can be tuned and best-case designs are given covering a range of conditions.
WOS标题词: Science & Technology ; Physical Sciences
类目[WOS]: Astronomy & Astrophysics
研究领域[WOS]: Astronomy & Astrophysics
关键词[WOS]: SOUTH-POLE ; ANTARCTIC PLATEAU ; DOME-C ; SURFACE-LAYER ; TELESCOPE ; PILOT ; SITE ; BRIGHTNESS ; EMISSION ; UNIVERSE
收录类别: SCI
项目资助者: Australian Research Council LIEF(LE15100024)
语种: 英语
WOS记录号: WOS:000371716900001
Citation statistics:
内容类型: 期刊论文
URI标识: http://libir.pmo.ac.cn/handle/332002/16166
Appears in Collections:南极天文中心_期刊论文

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作者单位: 1.Univ Sydney, Sydney, NSW 2006, Australia
2.Australian Astron Observ, N Ryde, NSW, Australia
3.Univ New S Wales, Sydney, NSW 2052, Australia
4.Swinburne Univ, Melbourne, Vic, Australia
5.Texas A&M Univ, College Stn, TX 77843 USA
6.Chinese Acad Sci, Purple Mt Observ, Nanjing, Jiangsu, Peoples R China
7.Chinese Ctr Antarctic Astron, Nanjing, Jiangsu, Peoples R China
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