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Simulating the MR 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 8.

Power-law fits to the decrease in σK as a function of the number of RV data points (modeled as ﹩{\sigma }_{{\rm{K}}}=1/{N}_{\mathrm{obs}}^{b}﹩, where b is the shown power-law index), sampled in 3-month intervals. The four schemes are not well differentiated, which implies that no single scheme reaches higher K/σK values faster than the others. In all four cases, the mean power-law fit is marginally steeper than the −0.5 value expected for the mean of a Gaussian distribution, which is probably due to fitting a small number of RV points in the early data epochs.

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