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arXiv · 1005.3810

Probing Dark Energy with the Kunlun Dark Universe Survey Telescope

Gong-Bo Zhao·Hu Zhan·Lifan Wang·Zuhui Fan·Xinmin Zhang
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Abstract

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 square degrees in \emph{ugrizyJH} bands can provide competitive constraints on dark energy equation of state parameters using type Ia 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 \emph{yJH} bands over 5000--10,000 deg$^2$ and the Large Synoptic Survey Telescope in \emph{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.

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Gong-Bo Zhao, Hu Zhan, Lifan Wang, Zuhui Fan, Xinmin Zhang. 2010-05-24. Probing Dark Energy with the Kunlun Dark Universe Survey Telescope. https://doi.org/10.1086/660801

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