A Self-Learning Neural Network Approach for RFI Detection and Removal in Radio Astronomy

TL;DR

This paper introduces a self-learning neural network method for detecting and removing RFI in radio astronomy signals without requiring training data, leveraging the Gaussian nature of true astronomical signals for effective cleaning.

Contribution

The novel approach uses a variational encoder/decoder network that does not need a training set, exploiting the Gaussian property of astronomical signals for RFI removal.

Findings

Effective RFI cleaning on simulated data

RFI residuals are within 10% in contaminated channels

Method shows promise for real-time implementation in radio telescopes

Abstract

We present a novel neural network (NN) method for the detection and removal of Radio Frequency Interference (RFI) from the raw digitized signal in the signal processing chain of a typical radio astronomy experiment. The main advantage of our method is that it does not require a training set. Instead, our method relies on the fact that the true signal of interest coming from astronomical sources is thermal and therefore described as a Gaussian random process, which cannot be compressed. We employ a variational encoder/decoder network to find the compressible information in the datastream that can explain the most variance with the fewest degrees of freedom. We demonstrate it on a set of toy problems and stored ringbuffers from the Baryon Mapping eXperiment (BMX) prototype. We find that the RFI subtraction is effective at cleaning simulated timestreams: while we find that the power spectra of the RFI-cleaned timestreams output by the NN suffer from extra signal consistent with additive noise, we find that it is generally around percent level across the band and sub 10 percent in contaminated spectral channels even when RFI power is an order of magnitude larger than the signal. We discuss advantages and limitations of this method and possible implementation in the front-end of future radio experiments.