Probing Dark Energy with the Kunlun Dark Universe Survey Telescope

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 imagin...

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Bibliographic Details
Main Authors: Zhao, Gong-Bo, Zhan, Hu, Wang, Lifan, Fan, Zuhui, Zhang, Xinmin
Other Authors: Zhao, GB (reprint author), Chinese Acad Sci, Inst High Energy Phys, Div Theoret Phys, POB 918-4, Beijing 100049, Peoples R China., Chinese Acad Sci, Inst High Energy Phys, Div Theoret Phys, Beijing 100049, Peoples R China., Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England., Chinese Acad Sci, Natl Astron Observ, Key Lab Opt Astron, Beijing 100012, Peoples R China., Texas A&M Univ, Dept Phys, College Stn, TX 77843 USA., Purple Mt Observ, Nanjing 210008, Peoples R China., Peking Univ, Sch Phys, Dept Astron, Beijing 100871, Peoples R China., Chinese Acad Sci, Ctr Theoret Phys, Sci Facil, Beijing 100864, Peoples R China., Chinese Acad Sci, Inst High Energy Phys, Div Theoret Phys, POB 918-4, Beijing 100049, Peoples R China.
Format: Journal/Newspaper
Language:English
Published: publications of the astronomical society of the pacific 2011
Subjects:
MEASURING COSMOLOGICAL PARAMETERS
WEAK-LENSING MEASUREMENTS
PHOTOMETRIC REDSHIFT
POWER SPECTRUM
IA SUPERNOVAE
CONSTRAINTS
TOMOGRAPHY
SPACE
SHEAR
REQUIREMENTS
Antarc*
Antarctica
Online Access:https://hdl.handle.net/20.500.11897/394753
Description
Summary: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. Astronomy & Astrophysics SCI(E) 0 ARTICLE 904 725-734 123

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