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The AARTFAAC All Sky Monitor: System Design and Implementation

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arxiv 1609.04205 v1 pith:GXTVC3BF submitted 2016-09-14 astro-ph.IM

The AARTFAAC All Sky Monitor: System Design and Implementation

classification astro-ph.IM
keywords lofarradioaartfaacdesignfrequencyimagesimplementationlatency
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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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 240 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.

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Cited by 1 Pith paper

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  1. Discovery of a radio-flaring M dwarf in a commensal transient search of the LADUMA field

    astro-ph.SR 2026-07 accept novelty 6.0

    MeerKAT LADUMA monitoring reveals a radio-flaring M3.5 dwarf, LP 888-63, with 13 detections in 41 epochs at 816 MHz.