22 May 2015 Inferential statistics for transient signal detection in radio astronomy phased arrays
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In this paper we develop two statistical rules for the purpose of detecting pulsars and transients using signals from phased array feeds installed on a radio telescope in place of a traditional horn receiver. We assume a known response of the antenna arrays and known coupling among array elements. We briefly summarize a set of pre-processing steps applied to raw array data prior to signal detection and then derive two detection statistics assuming two models for the unknown radio source astronomical signal: (1) the signal is deterministic and (2) the signal is a random process. The performance of both detectors is analyzed using both real and simulated data.
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Natalia A. Schmid, Natalia A. Schmid, Richard M. Prestage, Richard M. Prestage, Marwan Alkhweldi, Marwan Alkhweldi, } "Inferential statistics for transient signal detection in radio astronomy phased arrays", Proc. SPIE 9476, Automatic Target Recognition XXV, 94760S (22 May 2015); doi: 10.1117/12.2184101; https://doi.org/10.1117/12.2184101

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