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探测暗能量的新型射电干涉仪CHIME的标定

Calibrating CHIME, A New Radio Interferometer to Probe Dark Energy

Laura B. Newburgh, Graeme E. Addison, Mandana Amiri, Kevin Bandura, J. Richard Bond, Liam Connor, Jean-François Cliche, Greg Davis, Meiling Deng, Nolan Denman, … 展开作者

Laura B. Newburgh, Graeme E. Addison, Mandana Amiri, Kevin Bandura, J. Richard Bond, Liam Connor, Jean-François Cliche, Greg Davis, Meiling Deng, Nolan Denman, Matt Dobbs, Mateus Fandino, Heather Fong, Kenneth Gibbs, Adam Gilbert, Elizabeth Griffin, Mark Halpern, David Hanna, Adam D. Hincks, Gary Hinshaw, Carolin Höfer, Peter Klages, Tom Landecker, Kiyoshi Masui, Juan Mena Parra, Ue-Li Pen, Jeff Peterson, Andre Recnik, J. Richard Shaw, Kris Sigurdson, Michael Sitwell, Graeme Smecher, Rick Smegal, Keith Vanderlinde, Don Wiebe

摘要:

加拿大氢强度测绘实验(英语:Canadian Hydrogen Intensity Mapping Experiment,CHIME)是一个凌日干涉仪,目前正在加拿大不列颠哥伦比亚省彭蒂克顿的自治领射电天体物理观测台(英语:Dominion Radio Astrophysical Observatory,DRAO)建造。我们将用CHIME在400 - 800 MHz频率范围内对半个天空的中性氢进行测图,测量红移在0.8 - 2.5之间的重子声学振荡(BAO),以探测暗能量。我们已经部署了CHIME的探路者版本,它将对BAO功率谱产生约束,并为我们的校准方案提供测试平台。我将讨论CHIME校准要求,并描述我们正在开发的仪器,以满足这些要求。

英文摘要:

The Canadian Hydrogen Intensity Mapping Experiment (CHIME) is a transit interferometer currently being built at the Dominion Radio Astrophysical Observatory (DRAO) in Penticton, BC, Canada. We will use CHIME to map neutral hydrogen in the frequency range 400 -- 800\,MHz over half of the sky, producing a measurement of baryon acoustic oscillations (BAO) at redshifts between 0.8 -- 2.5 to probe dark energy. We have deployed a pathfinder version of CHIME that will yield constraints on the BAO power spectrum and provide a test-bed for our calibration scheme. I will discuss the CHIME calibration requirements and describe instrumentation we are developing to meet these requirements.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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