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RV×TESS. I. Modeling Asteroseismic Signals with Simultaneous Photometry and Radial Velocities

  • Authors: Jiaxin Tang, Sharon X. Wang, Yaguang Li, Timothy R. Bedding, Guang-Yao Xiao, Fabo Feng, Jie Yu, Zun Wang, Jennifer A. Burt, R. Paul Butler, Brad Carter, Jeffrey D. Crane, Matías R. Díaz, Samuel K. Grunblatt, Daniel Huber, Hugh Jones, Stephen R. Kane, Jacob K. Luhn, Stephen A. Shectman, Johanna Teske, Rob Wittenmyer, Jason T. Wright, Jeremy Bailey, Simon J. O'Toole, Chris G. Tinney

Jiaxin Tang et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 11.

Completeness maps for planet searches using RVs of HD 5562 presented in this work before (left panel) and after (right panel) subtracting the best-fit GP model, which represents the stellar RV jitter from the asteroseismic signals. The comparison between the left and right panels illustrates the improved effectiveness of planet detection enabled under an idealized condition, where stellar jitter could be subtracted a priori without affecting any underlying planetary signals, and thus it shows the best-case scenario. The circles are injected planet signals that can (blue) or cannot (red) be recovered. The red contours illustrate the probabilities of recovery, where the solid black line marks the 50% detection probability. The maps were made using RVsearch. See Section 5.2 for more details.

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