Nonlinear Noise Reduction: Extending the Transit Method to Multi-Planet Systems?

Details Nonlinear Noise Reduction: Extending the Transit Method to Multi-Planet Systems? Nonlinear Noise Reduction: Extending the Transit Method to Multi-Planet Systems?

Sep 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008dps....40.1118j&link_type=abstract

American Astronomical Society, DPS meeting #40, #11.18; Bulletin of the American Astronomical Society, Vol. 40, p.404

Astronomy and Astrophysics

Astronomy

Scientific paper

Nonlinear local projective noise reduction is a powerful tool for lowering noise in cases where a fundamental and a harmonic are present in the power spectrum of a light curve. Thus, it is particularly useful for resonances. The method however, is limited to continuous light curves (WET, etc). With Kepler scheduled to launch in February 2009, transit data amenable to nonlinear noise reduction will shortly become available. To date, no multiple planet systems have been detected using the transit method. We explore the potential of nonlinear noise reduction to yield information on multiple planet systems with resonance using simulated light curves.

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