e-VLBI observations of GRB 080409 afterglow with an Australasian radio telescope network

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作者
Aquib Moin [1 ,2 ,3 ,4 ]
Philip G.Edwards [4 ]
Steven J.Tingay [3 ,5 ]
Chris J.Phillips [4 ]
Anastasios K.Tzioumis [4 ]
Shaun W.Amy [4 ]
Tao An [2 ,6 ]
Mamoru Sekido [7 ]
Zhong-Xiang Wang [2 ]
机构
[1] Physics Department,United Arab Emirates University
[2] Shanghai Astronomical Observatory,Chinese Academy of Sciences
[3] International Centre for Radio Astronomy Research,Curtin University
[4] CSIRO Astronomy and Space Science
[5] Osservatorio di Radio Astronomia,Istituto Nazionale di Astrofisica
[6] Key Laboratory of Radio Astronomy,Chinese Academy of Sciences
[7] Kashima Space Research Center,National Institute of Information and Communications Technology(NICT)
关键词
techniques:interferometric; galaxies:active; gamma rays:bursts;
D O I
暂无
中图分类号
P111.44 [射电望远镜(无线电望远镜)];
学科分类号
摘要
Transcontinental e-VLBI observations were conducted in June 2008 with telescopes in Australia,China and Japan. Detections were made of the radio-loud quasar PKS B0727-115, which shows superluminal motion, and the intra-day variable quasar PKS B0524+034. The latter source was used as a phase reference calibrator for observations at the position of the gamma-ray burst GRB 080409, for which an upper limit to the radio emission is set. Australia Telescope Compact Array data were also used to derive a limit on the radio flux density of the GRB afterglow. These observations demonstrate the capability to form a large Australasian radio telescope network for e-VLBI, with data transported and processed in realtime over high capacity networks. This campaign represents the first step towards more regular e-VLBI observations in this region.
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页码:3 / 8
页数:6
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