Abstract Traditionally, fast radio transient searches are conducted on dedispersed time series using thresholding techniques. However, peaks in dedispersed time series do not directly provide information on the nature of the source. In the DM–time domain, the S/N variation of real, dispersed astrophysical signals forms a characteristic bow tie shape, whereas radio frequency interference (RFI) can take multiple different forms. We have developed a method that bypasses the thresholding step of traditional single-pulse searches in favour of a direct DM–time domain image analysis. We further generalise the expected S/N degradation of a single pulse as a function of dispersion measure to define physically motivated DM and time ranges for constructing optimal search windows. We also propose a modified version of the traditional dedispersion plan optimised for this method. The backbone of our pipeline is a Mask R-CNN, a deep learning model designed for object detection, enabling it to identify the bow tie signature and distinguish real sources from RFI. We have trained the model on simulated bursts injected on top of real MeerKAT noise observations. We tested the model on MeerKAT follow-up observations of the repeater FRB20240114A and we were able to recover all bursts with a signal-to-noise above the traditional threshold, while detecting two bursts that were fainter. Notably, the pipeline can identify multiple bursts within the same search window. Our new approach considerably reduces the number of candidates above a nominal threshold while being capable of running in real time for typical surveys.
Díaz et al. (Mon,) studied this question.