Abstract
The digital record of the voltage in a radio telescope receiver, after frequency conversion and sampling at a finite rate, is not a perfect representation of the original analog signal. To detect and characterise a transient event with a duration comparable to the inverse bandwidth it is necessary to compensate for these effects, altering the statistical properties of the signal and making it difficult to determine the significance of a potential detection. We present an analysis of these modified statistics and demonstrate them with experimental results from Bedlam, a new digital backend for the Parkes radio telescope.
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Acknowledgements
The Parkes radio telescope is part of the Australia Telescope which is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO. This research was supported by the Australian Research Council’s Discovery Project funding scheme (project number DP0881006).
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Bray, J.D., Ekers, R.D. & Roberts, P. Noise statistics in a fast digital radio receiver: the Bedlam backend for the Parkes radio telescope. Exp Astron 36, 155–174 (2013). https://doi.org/10.1007/s10686-012-9327-9
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DOI: https://doi.org/10.1007/s10686-012-9327-9