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TOI-6695: A Pair of Near-resonant Massive Planets Observed with TESS from the WINE Survey

  • Authors: Jan Eberhardt, Trifon Trifonov, Thomas Henning, Marcelo Tala Pinto, Rafael Brahm, Andrés Jordán, Nestor Espinoza, Matías I. Jones, Melissa J. Hobson, Felipe I. Rojas, Martin Schlecker, Lorena Acuña, Remo Burn, Gavin Boyle, Rodrigo Leiva, James McCormac, Nicholas Dunckel, Diana Dragomir, Jeffrey D. Crane, Stephen Shectman, Johanna K. Teske, David Osip, Arvind F. Gupta, Solène Ulmer-Moll, François Bouchy, Monika Lendl, Davide Gandolfi, George R. Ricker, Jon M. Jenkins, Sara Seager, Joshua N. Winn

Jan Eberhardt et al 2025 The Astronomical Journal 169 .

  • Provider: AAS Journals

Caption: Figure 4.

MLP periodograms for RV and stellar activity data of TOI-6695. The top four panels show the periodograms of the raw and residual RVs after subtracting Keplerian models, panels 5–9 show the periodograms of the stellar activity indicators and the bottom panel shows the RV window function. Dashed blue lines indicate the planetary orbital periods, and the red dashed line and shaded region correspond to the assumed stellar rotational period. Dashed horizontal lines correspond to FAP levels of 10%, 1%, and 0.1%.

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