Optimized Trigger for Ultra-High-Energy Cosmic-Ray and Neutrino Observations with the Low Frequency Radio Array
DOI: 10.1016/j.nima.2011.10.041 (http) or 10.1016/j.nima.2011.10.041 (doi)
ADS bibcode 2012NIMPA.664..171S
arXiv:1108.5745
K. Singh et al. (including O. Wucknitz)
Abstract
When an ultra-high energy neutrino or cosmic ray strikes the Lunar surface a radio-frequency pulse is emitted. We plan to use the LOFAR radio telescope to detect these pulses. In this work we propose an e?cient trigger implementation for LOFAR optimized for the observation of short radio pulses.
Nuclear Instruments and Methods in Physics Research Section A 664 (2012) 171 (link to online journal)
DOI (Digital Object Identifier): 10.1016/j.nima.2011.10.041 (http) or 10.1016/j.nima.2011.10.041 (doi)
ADS bibcode 2012NIMPA.664..171S (link to ADS entry)
arXiv:1108.5745 (link to e-print archive)
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15 pages, NIMA version
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