Wavelets with Ridges: A High-Resolution Representation of Cataclysmic Variable Time-Series
Claire Blackman

TL;DR
This paper introduces an enhanced wavelet-based method with ridges for high-resolution analysis of low signal-to-noise quasi-periodic oscillations in variable star data, significantly improving detection rates.
Contribution
The paper develops and validates a wavelet ridge technique that outperforms existing methods for analyzing noisy, low-coherence astronomical time-series data.
Findings
Detected 62 new QPOs in VW Hyi data.
Identified 7 new long-period DNOs.
Improved detection rate for QPOs compared to previous methods.
Abstract
Quasi-periodic oscillations and dwarf nova oscillations occur in dwarf novae and nova-like variables during outburst and occasionally during quiescence, and have analogues in high-mass X-ray binaries and black-hole candidates. The frequent low coherence of quasi-period oscillations and dwarf nova oscillations can make detection with standard time-series tools such as periodograms problematic. This paper develops tools to analyse quasi-periodic brightness oscillations. We review the use of time-frequency representations in the astronomical literature, and show that representations such as the Choi-Williams Distribution and Zhao-Atlas-Marks Representation, which are best suited to high signal-to-noise data, cannot be assumed a priori to be the best techniques for our data, which have a much higher noise level and lower coherence. This leads us to a detailed analysis of the time-frequency…
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