Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

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 10.

PSDs of the RVs taken on each of the two long-observation nights. The light orange and light blue lines represent the original PSDs, while the darker lines are the smoothed. The green solid lines represent the PSDs of the best-fit GP model (same model as in Figures 8 and 9), while the dashed lines are for the model components (granulation, oscillation, and white noise). The PSDs validate the goodness of-fit for the GP models in the frequency domain since the GP regression was only done in the time domain (Figure 9). See Section 4.4 for more details.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article

Show More

Copyright and Terms & Conditions

Additional terms of reuse