The AARTFAAC All-Sky Monitor: System Design and Implementation

被引:32
|
作者
Prasad, Peeyush [1 ]
Huizinga, Folkert [1 ]
Kooistra, Eric [2 ]
van der Schuur, Daniel [2 ]
Gunst, Andre [2 ]
Romein, John [2 ]
Kuiack, Mark [1 ]
Molenaar, Gijs [1 ]
Rowlinson, Antonia [1 ,2 ]
Swinbank, John D. [3 ]
Wijers, Ralph A. M. J. [1 ]
机构
[1] Univ Amsterdam, Anton Pannekoek Inst, Postbus 94249, NL-1090 GE Amsterdam, Netherlands
[2] ASTRON, NL-7991 PD Oude Hoogeveensedijk, Netherlands
[3] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA
关键词
Radio telescopes; interferometry; calibration; imaging; radio transients; correlators;
D O I
10.1142/S2251171716410087
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Amsterdam-ASTRON Radio Transients Facility And Analysis Center (AARTFAAC) all sky monitor is a sensitive, real time transient detector based on the Low Frequency Array (LOFAR). It generates images of the low frequency radio sky with spatial resolution of 10s of arcmin, MHz bandwidths, and a time cadence of a few seconds, while simultaneously but independently observing with LOFAR. The image timeseries is then monitored for short and bright radio transients. On detection of a transient, a low latency trigger will be generated for LOFAR, which can interrupt its schedule to carry out follow-up observations of the trigger location at high sensitivity and resolutions. In this paper, we describe our heterogeneous, hierarchical design to manage the 259 Gbps raw data rate, and large scale computing to produce real-time images with minimum latency. We discuss the implementation of the instrumentation, its performance, and scalability.
引用
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页数:17
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