Fourier domain excision of periodic radio frequency interference

TL;DR

This paper presents a Fourier-domain method for excising periodic radio frequency interference from radio telescope data, significantly improving the detection of weak astrophysical signals like pulsars and FRBs.

Contribution

The paper introduces a novel Fourier-domain RFI excision technique that enhances sensitivity to cosmic signals without affecting pulsar pulse shapes.

Findings

Increases signal-to-noise ratio of pulsar and FRB signals

Detects single pulses that would otherwise be hidden in noise

Enhances timing accuracy and overall sensitivity

Abstract

The discovery and study of pulsars and Fast Radio Bursts (FRBs) in time-domain radio data is often hampered by radio frequency interference (RFI). Some of this terrestrial RFI is impulsive and bright, and relatively easy to identify and remove. Other anthropogenic signals, however, are weaker yet periodic, and their persistence can drown out astrophysical signals. Here we show that Fourier-domain excision of periodic RFI is an effective and powerful step in detecting weak cosmic signals. We find that applying the method significantly increases the signal-to-noise ratio of transient as well as periodic pulsar signals. In live studies, we detected single pulses from pulsars and FRBs that would otherwise have remained buried in background noise. We show the method has no negative effects on pulsar pulse shape and that it enhances timing campaigns. We demonstrate the method on real-life data from a number of large radio telescopes, and conclude that Fourier-domain RFI excision increases the effective sensitivity to astrophysical sources by a significant fraction which can be even larger than an order of magnitude in case of strong RFI. An accelerated implementation of the method runs on standard time-domain radio data formats and is publicly available.