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Magellan/PFS Radial Velocities of GJ 9827, a Late K dwarf at 30 pc with Three Transiting Super-Earths

  • Authors: Johanna K. Teske, Sharon Wang, Angie Wolfgang, Fei Dai, Stephen A. Shectman, R. Paul Butler, Jeffrey D. Crane, and Ian B. Thompson

2018 The Astronomical Journal 155 148.

  • Provider: AAS Journals

Caption: Figure 8.

The radial velocity measurements of GJ 9827 from PFS. The colored dashed lines are circular Keplerian models of the three planets. The blue dotted line shows the Gaussian Process model of correlated stellar noise, with priors inferred from the K2 light curve. The red solid line is the combined signal. The Gaussian Process model is poorly constrained (notice the spiky features) when the data have poor temporal sampling.

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