Tied-array beam flatfielding
Dirk Kuiper, Cees Bassa, Ziggy Pleunis, Jason Hessels

TL;DR
This paper introduces a simple, computationally inexpensive method called beam flatfielding that uses multi-beam spatial information to stabilize bandpasses, reduce false positives, and improve the detection of genuine astrophysical signals in phased-array radio telescopes.
Contribution
It presents a novel post-beamforming technique that significantly reduces false triggers in pulsar and transient detection pipelines by leveraging multi-beam data for bandpass stabilization.
Findings
Reduces false positives by a factor of ~200 in LOTAAS data.
Improves pulse signal-to-noise ratios with beam flatfielding.
Produces flatter dynamic spectra and more Gaussian noise statistics.
Abstract
Context. Multi-element phased-array radio telescopes use digital beamforming to widen their field-of-view with numerous tied-array beams (TABs). These beams share bandpass variations and radio frequency interference (RFI). Yet, most pulsar and transient pipelines process each beam independently, ignoring shared spatial information. This leads to many RFI-dominated false positives that require extensive later sifting. Aims. We exploit multi-beam spatial information to stabilize bandpasses, suppress red noise and broad-band RFI, and drastically reduce false positives without degrading genuine astrophysical signals. Methods. We derive tied-array gain against residual phase dispersion, showing off-beam sources converge to the incoherent limit. Using chi-squared statistics, we analyze dividing a TAB by a beam-averaged reference and quantify the necessary smoothing. We test these predictions…
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Taxonomy
TopicsRadio Astronomy Observations and Technology · Astrophysics and Cosmic Phenomena · Antenna Design and Optimization
