Design of a multibeam spectrometer for the Green Bank Telescope

J. Ford, M. Bloss, P. Brandt, Hong Chen, J. Chennamangalam, J. Cobb, R. Creager, P. Demorest, G. Jones, R. McCullough, J. Ray, D. Roshi, S. Scott, A. Siemion, M. Wagner, G. Watts, D. Werthimer, M. Whitehead
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Abstract

A new multi-beam spectrometer for the Green Bank Telescope (GBT) is being designed and built by a partnership between the National Radio Astronomy Observatory (NRAO) and the University of California at Berkeley, and partially funded by a National Science Foundation Advanced Technology Instrumentation grant. The spectrometer is a heterogeneous computing device based on a Field Programmable Gate Array (FPGA) front-end and a heterogeneous compute server backend, comprised of Graphical Processing Units (GPUs) and x86 CPUs. Working together, the hardware in this system provides processing power to analyse up to 8 dual-polarization or 16 single-polarization inputs, at bandwidths of up to 1.25 GHz per input. An aggregate of up to 10 GHz of bandwidth, dual polarization, may be processed with the spectrometer.
格林班克望远镜多波束光谱仪的设计
美国国家射电天文台(NRAO)和加州大学伯克利分校正在合作设计和建造一种用于绿岸望远镜(GBT)的新型多波束光谱仪,部分资金由美国国家科学基金会先进技术仪器基金提供。该光谱仪是一种基于FPGA (Field Programmable Gate Array)前端和异构计算服务器后端的异构计算设备,由gpu (Graphical Processing Units)和x86 cpu组成。协同工作,该系统中的硬件提供处理能力,可以分析多达8个双偏振或16个单偏振输入,每个输入的带宽高达1.25 GHz。该分光计可处理高达10ghz带宽的双极化。
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