Wavelet Denoising of Radio Observations of Rotating Radio Transients (RRATs): Improved Timing Parameters for Eight RRATs
Min Jiang, Bingyi Cui, Natalia Schmid, Maura McLaughlin, Zhicheng Cao

TL;DR
This paper introduces a wavelet-based denoising method for radio observations of RRATs, significantly improving pulse detection and timing accuracy, which aids in understanding their physical nature and relation to other neutron stars.
Contribution
The paper presents a novel wavelet denoising technique tailored for RRAT signals, enhancing pulse detection and timing precision over conventional methods.
Findings
Increased number of detected TOAs by 12% to 69%.
Reduced parameter estimation errors by 16% to 90%.
Wavelet denoising effectively improves RRAT signal analysis.
Abstract
Rotating radio transients (RRATs) are sporadically emitting pulsars detectable only through searches for single pulses. While over 100 RRATs have been detected, only a small fraction (roughly 20\%) have phase-connected timing solutions, which are critical for determining how they relate to other neutron star populations. Detecting more pulses in order to achieve solutions is a key to understanding their physical nature. Astronomical signals collected by radio telescopes contain noise from many sources, making the detection of weak pulses difficult. Applying a denoising method to raw time series prior to performing a single-pulse search typically leads to a more accurate estimation of their times of arrival (TOAs). Taking into account some features of RRAT pulses and noise, we present a denoising method based on wavelet data analysis, an image-processing technique. Assuming that the spin…
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