Figure 1 from Simulating the M–R Relation from APF Follow-up of TESS Targets: Survey Design and Strategies for Overcoming Mass Biases

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Simulating the M–R Relation from APF Follow-up of TESS Targets: Survey Design and Strategies for Overcoming Mass Biases

Authors: Jennifer Burt, Brad Holden, Angie Wolfgang, and L. G. Bouma

2018 The Astronomical Journal 156 255.

Provider: AAS Journals

Caption: Figure 1.

Top: Comparisons of the confirmed Kepler planets from Q1 to Q16 (Mullally et al. 2015) in blue and the simulated planets from our instance of the predicted TESS planet yield in red. Bottom: Kepler magnitudes of the detected Kepler host stars (blue) and simulated detected TESS planet host stars (red).

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