Radio astronomy research in Malaysia: Past, present and future

Z. Abidin, Zainol Abidin Ibrahim
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引用次数: 5

Abstract

This paper will report on the progress in the research field of radio astronomy in Malaysia and also in South-East Asia. Radio astronomy research can be said to have only started being done actively in Malaysia in 2005. Fundamental setup and some basic research were done in the early parts. Jupiter radio bursts as well as radio meteor counting were the first few projects. Currently a medium-sized radio telescope which was recently purchased is being used to undergo more advanced research such as observing spectrum of galaxy clusters in order to study Dark Matter. This paper will also report on the latest results on the survey of Radio Frequency Interference (RFI), which is currently done on chosen candidate sites in Malaysia in order to setup on it a large radio telescope in the future. The best site with the lowest averaged RFI level is found at Langkawi (−100.33 dBm or 4.4 × 106 Jy). The author is the chair for the Radio Astronomy Working Group for the South-East Asia Astronomy Network (SEAAN) and the Malaysian team is very much an important part of this group. This group will eventually be a research hub for the global projects of the Global-Very Long Baseline Interferometer (Global-VLBI) and the Square Kilometre Array (SKA).
马来西亚射电天文学研究:过去、现在和未来
本文将报告马来西亚和东南亚射电天文学研究领域的进展。射电天文学的研究可以说是在2005年才开始在马来西亚活跃起来的。本文在前期进行了基础设置和一些基础研究。木星射电爆发和射电流星计数是最初的几个项目。最近购买的中型射电望远镜正在进行更先进的研究,如观测星系团的光谱,以研究暗物质。本文还将报告无线电频率干扰(RFI)调查的最新结果,该调查目前在马来西亚选定的候选地点进行,以便将来在其上建立一个大型射电望远镜。平均RFI水平最低的最佳地点是浮罗交怡(- 100.33 dBm或4.4 × 106 Jy)。作者是东南亚天文网络(SEAAN)射电天文学工作组的主席,马来西亚团队是该工作组的重要组成部分。该小组最终将成为全球甚长基线干涉仪(global - vlbi)和平方公里阵列(SKA)全球项目的研究中心。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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