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DETERMINING THE MASS OF KEPLER-78b WITH NONPARAMETRIC GAUSSIAN PROCESS ESTIMATION

  • Authors: Samuel K. Grunblatt, Andrew W. Howard, and Raphaëlle D. Haywood

2015 The Astrophysical Journal 808 127.

  • Provider: AAS Journals

Caption: Figure 3.

Residuals of the HIRES and HARPS-N data after the quasi-periodic GP regression to the data with the Keplerian signal subtracted is removed, phase-folded at the known orbital period of the planet. HIRES data is shown in blue, and HARPS-N data is shown in red. The planetary signal model is shown by the dotted black line, and binned data are shown by black points.

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