Extracting Information about EMRIs using Time-Frequency Methods
Linqing Wen (MPI/AEI), Yanbei Chen (MPI/AEI), Jonathan Gair, (University of Cambridge)

TL;DR
This paper discusses a time-frequency analysis approach for detecting and extracting information about EMRIs in LISA data, offering a computationally feasible alternative to matched filtering and introducing a data decomposition method for improved detection and source characterization.
Contribution
The paper extends previous work by evaluating the time-frequency detection method, introducing a data decomposition technique for directional sensitivity, and outlining parameter estimation strategies.
Findings
EMRI detection possible up to 1-3 Gpc distance
Decomposition method improves detection efficiency
Potential for source waveform extraction and parameter estimation
Abstract
The inspirals of stellar-mass compact objects into supermassive black holes are some of the most exciting sources of gravitational waves for LISA. Detection of these sources using fully coherent matched filtering is computationally intractable, so alternative approaches are required. In Wen & Gair (2005), we proposed a detection method based on searching for significant deviation of power density from noise in a time-frequency spectrogram of the LISA data. The performance of the algorithm was assessed in Gair & Wen (2005) using Monte-Carlo simulations on several trial waveforms and approximations to the noise statistics. We found that typical extreme mass ratio inspirals (EMRIs) could be detected at distances of up to 1-3 Gpc, depending on the source parameters. In this paper, we first give an overview of our previous work in Wen & Gair (2005) and Gair & Wen (2005), and discuss the…
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