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 imaging...
Published in: | Publications of the Astronomical Society of the Pacific |
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ftunivportsmpubl:oai:researchportal.port.ac.uk:publications/99525366-3064-48b6-946e-5566c96ee84b 2023-05-15T13:43:58+02:00 Probing dark energy with the Kunlun Dark Universe Survey Telescope Zhao, Gong-Bo Zhan, Hu Wang, Lifan Fan, Zuhui Zhang, Xinmin 2011-05-20 https://doi.org/10.1086/660801 https://researchportal.port.ac.uk/portal/en/publications/probing-dark-energy-with-the-kunlun-dark-universe-survey-telescope(99525366-3064-48b6-946e-5566c96ee84b).html eng eng info:eu-repo/semantics/openAccess Zhao , G-B , Zhan , H , Wang , L , Fan , Z & Zhang , X 2011 , ' Probing dark energy with the Kunlun Dark Universe Survey Telescope ' PASP , vol 123 , no. 904 , pp. 725-734 . DOI:10.1086/660801 astro-ph.CO cosmological parameters distance scale gravitational lensing large-scale structure of universe article 2011 ftunivportsmpubl https://doi.org/10.1086/660801 2017-09-28T19:36:35Z 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 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 yJH 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. Article in Journal/Newspaper Antarc* Antarctica University of Portsmouth: Portsmouth Research Portal Publications of the Astronomical Society of the Pacific 123 904 725 734 |
institution |
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University of Portsmouth: Portsmouth Research Portal |
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ftunivportsmpubl |
language |
English |
topic |
astro-ph.CO cosmological parameters distance scale gravitational lensing large-scale structure of universe |
spellingShingle |
astro-ph.CO cosmological parameters distance scale gravitational lensing large-scale structure of universe Zhao, Gong-Bo Zhan, Hu Wang, Lifan Fan, Zuhui Zhang, Xinmin Probing dark energy with the Kunlun Dark Universe Survey Telescope |
topic_facet |
astro-ph.CO cosmological parameters distance scale gravitational lensing large-scale structure of universe |
description |
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 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 yJH 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. |
format |
Article in Journal/Newspaper |
author |
Zhao, Gong-Bo Zhan, Hu Wang, Lifan Fan, Zuhui Zhang, Xinmin |
author_facet |
Zhao, Gong-Bo Zhan, Hu Wang, Lifan Fan, Zuhui Zhang, Xinmin |
author_sort |
Zhao, Gong-Bo |
title |
Probing dark energy with the Kunlun Dark Universe Survey Telescope |
title_short |
Probing dark energy with the Kunlun Dark Universe Survey Telescope |
title_full |
Probing dark energy with the Kunlun Dark Universe Survey Telescope |
title_fullStr |
Probing dark energy with the Kunlun Dark Universe Survey Telescope |
title_full_unstemmed |
Probing dark energy with the Kunlun Dark Universe Survey Telescope |
title_sort |
probing dark energy with the kunlun dark universe survey telescope |
publishDate |
2011 |
url |
https://doi.org/10.1086/660801 https://researchportal.port.ac.uk/portal/en/publications/probing-dark-energy-with-the-kunlun-dark-universe-survey-telescope(99525366-3064-48b6-946e-5566c96ee84b).html |
genre |
Antarc* Antarctica |
genre_facet |
Antarc* Antarctica |
op_source |
Zhao , G-B , Zhan , H , Wang , L , Fan , Z & Zhang , X 2011 , ' Probing dark energy with the Kunlun Dark Universe Survey Telescope ' PASP , vol 123 , no. 904 , pp. 725-734 . DOI:10.1086/660801 |
op_rights |
info:eu-repo/semantics/openAccess |
op_doi |
https://doi.org/10.1086/660801 |
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Publications of the Astronomical Society of the Pacific |
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123 |
container_issue |
904 |
container_start_page |
725 |
op_container_end_page |
734 |
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1766195498360766464 |