IHEP OpenIR  > 理论物理室
Probing Dark Energy with the Kunlun Dark Universe Survey Telescope
Zhao GB(赵公博); Zhang XM(张新民); Zhao, GB; Zhan, H; Wang, LF; Fan, ZH; Zhang, XM
2011
发表期刊PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC
卷号123期号:904页码:725-734
通讯作者[Zhao, Gong-Bo ; Zhang, Xinmin] Chinese Acad Sci, Inst High Energy Phys, Div Theoret Phys, Beijing 100049, Peoples R China ; [Zhao, Gong-Bo] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England ; [Zhan, Hu] Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China ; [Wang, Lifan] Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA ; [Wang, Lifan] Purple Mt Observ, Nanjing 210008, Peoples R China ; [Fan, Zuhui] Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China ; [Zhang, Xinmin] Chinese Acad Sci, Ctr Theoret Phys, Sci Facil, Beijing 100864, Peoples R China
文章类型Article
摘要Dark energy is an important science driver of many upcoming large-scale surveys. With small, stable seeing, and low thermal infrared background, Dome A, Antarctica, offers a unique opportunity for shedding light on fundamental questions about the universe. We show that a deep, high-resolution imaging survey of 10, 000 deg(2) in ugrizyJH bands can provide competitive constraints on dark enemy equation-of-state parameters using Type la supernovae, baryon acoustic oscillations, and weak-lensing techniques. Such a survey may be partially achieved with a coordinated effort of the Kunlun Dark Universe Survey Telescope (KDUST) in bands over 5000-10,000 deg(2) and the Large Synoptic Survey Telescope in ugrizy bands over the same area. Moreover, the joint survey can take advantage of the high-resolution imaging at Dome A to further tighten the constraints on dark energy and to measure dark matter properties with strong lensing, as well as galaxy/galaxy weak lensing.
学科领域Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics ; Astronomy & Astrophysics
URL查看原文
语种英语
研究领域[WOS]Astronomy & Astrophysics ; Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
WOS记录号WOS:000292421300007
引用统计
被引频次:6[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ihep.ac.cn/handle/311005/238362
专题理论物理室
作者单位中国科学院高能物理研究所
推荐引用方式
GB/T 7714
Zhao GB,Zhang XM,Zhao, GB,et al. Probing Dark Energy with the Kunlun Dark Universe Survey Telescope[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,2011,123(904):725-734.
APA 赵公博.,张新民.,Zhao, GB.,Zhan, H.,Wang, LF.,...&Zhang, XM.(2011).Probing Dark Energy with the Kunlun Dark Universe Survey Telescope.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC,123(904),725-734.
MLA 赵公博,et al."Probing Dark Energy with the Kunlun Dark Universe Survey Telescope".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC 123.904(2011):725-734.
条目包含的文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
5245.pdf(436KB)期刊论文作者接受稿限制开放CC BY-NC-SA请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[赵公博]的文章
[张新民]的文章
[Zhao, GB]的文章
百度学术
百度学术中相似的文章
[赵公博]的文章
[张新民]的文章
[Zhao, GB]的文章
必应学术
必应学术中相似的文章
[赵公博]的文章
[张新民]的文章
[Zhao, GB]的文章
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。