TL;DR
This paper presents a matched filtering technique for detecting weak spectral lines in interferometric data, demonstrating significant SNR improvements and providing an open-source implementation for practical use.
Contribution
It introduces an approximate matched filter method constructed from prior observations or models, optimized for the Fourier domain, enhancing weak line detection in radio interferometry.
Findings
Achieved ~53% SNR boost on ALMA data
Method improves detection sensitivity over traditional aperture extraction
Open-source Python implementation available for community use
Abstract
Modern radio interferometers enable observations of spectral lines with unprecedented spatial resolution and sensitivity. In spite of these technical advances, many lines of interest are still at best weakly detected and therefore necessitate detection and analysis techniques specialized for the low signal-to-noise ratio (SNR) regime. Matched filters can leverage knowledge of the source structure and kinematics to increase sensitivity of spectral line observations. Application of the filter in the native Fourier domain improves SNR while simultaneously avoiding the computational cost and ambiguities associated with imaging, making matched filtering a fast and robust method for weak spectral line detection. We demonstrate how an approximate matched filter can be constructed from a previously observed line or from a model of the source, and we show how this filter can be used to robustly…
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