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Cited by 229

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Transiting planet search in the Kepler pipeline

Jenkins, Jon M., Chandrasekaran, Hema, McCauliff, Sean D., Caldwell, Douglas A., Tenenbaum, Peter, Li, Jie, Klaus, Todd C., Cote, Miles T., Middour, Christopher·2010·SPIE Proceedings

Abstract

The Kepler Mission simultaneously measures the brightness of more than 160,000 stars every 29.4 minutes over a 3.5-year mission to search for transiting planets. Detecting transits is a signal-detection problem where the signal of interest is a periodic pulse train and the predominant noise source is non-white, non-stationary (1/f) type process of stellar variability. Many stars also exhibit coherent or quasi-coherent oscillations. The detection algorithm first identifies and removes strong oscillations followed by an adaptive, wavelet-based matched filter. We discuss how we obtain super-resolution detection statistics and the effectiveness of the algorithm for Kepler flight data.

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Metadata

Authors
Jenkins, J. M., Chandrasekaran, H., McCauliff, S. D., Caldwell, D. A., Tenenbaum, P., Li, J., Klaus, T. C., Cote, M. T., & Middour, C.
Venue
SPIE Proceedings
Publisher
SPIE
Published
2010-07-16
Volume
7740
Pages
77400D
ISSN
0277-786X (ISSN-L)
OpenAlex
W1992188543
Cited by
229
References
1
FWCI
48.22
Type
conference paper
Language
en
Open access
closed

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CoChat. (2026). Citation check: Transiting planet search in the Kepler pipeline. https://app.cochat.ai/papers/10.1117/12.856764
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Jenkins, J. M., Chandrasekaran, H., McCauliff, S. D., Caldwell, D. A., Tenenbaum, P., Li, J., Klaus, T. C., Cote, M. T., & Middour, C. (2010). Transiting planet search in the Kepler pipeline. SPIE Proceedings. https://doi.org/10.1117/12.856764

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