Searching for Transient Pulses with the ETA Radio Telescope release_pxsrzuu2sjcundedv5o3pxgy54

by Cameron D. Patterson, Steven W. Ellingson, Brian S. Martin, Kshitija Deshpande, John H. Simonetti, Michael Kavic, Sean E. Cutchin

Released as a report .

2008  

Abstract

Array-based, direct-sampling radio telescopes have computational and communication requirements unsuited to conventional computer and cluster architectures. Synchronization must be strictly maintained across a large number of parallel data streams, from A/D conversion, through operations such as beamforming, to dataset recording. FPGAs supporting multi-gigabit serial I/O are ideally suited to this application. We describe a recently-constructed radio telescope called ETA having all-sky observing capability for detecting low frequency pulses from transient events such as gamma ray bursts and primordial black hole explosions. Signals from 24 dipole antennas are processed by a tiered arrangement of 28 commercial FPGA boards and 4 PCs with FPGA-based data acquisition cards, connected with custom I/O adapter boards supporting InfiniBand and LVDS physical links. ETA is designed for unattended operation, allowing configuration and recording to be controlled remotely.
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Type  report
Stage   submitted
Date   2008-12-06
Version   v1
Language   en ?
Number  VPI-IPNAS-08-18
arXiv  0812.1255v1
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