Curvelet analysis of asteroseismic data I: Method description and application to simulated sun-like stars

@article{Lambert2006CurveletAO,
  title={Curvelet analysis of asteroseismic data I: Method description and application to simulated sun-like stars},
  author={P. Lambert and Sandrine Pires and Jérôme Ballot and R. A. Garc{\'i}a and J-L. Starck and S. Turck-chi{\`e}ze},
  journal={Astronomy and Astrophysics},
  year={2006},
  volume={454},
  pages={1021-1027}
}
Context. The detection and identification of oscillation modes (in terms of their � , m, and successive n) is a great challenge for present and future asteroseismic space missions. “Peak tagging" is an important step in the analysis of these data to provide estimations of stellar oscillation mode parameters, i.e., frequencies, rotation rates, and further studies on the stellar structure. Aims. Our goal is to increase the signal-to-noise ratio of the asteroseismic spectra computed from the time… 

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