Figure 1 from Bayesian Methods for Joint Exoplanet Transit Detection and Systematic Noise Characterization

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Bayesian Methods for Joint Exoplanet Transit Detection and Systematic Noise Characterization

Authors: Jamila S. Taaki, Farzad Kamalabadi, and Athol J. Kemball

2020 The Astronomical Journal 159 283.

Provider: AAS Journals

Caption: Figure 1.

A subset of Kepler raw simple aperture photometry (SAP; Jenkins et al. 2010b) light curves drawn from CCD module 8 and observing quarter 2, normalized and median subtracted. The light curves exhibit common trends due to systematic noise.

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