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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 5.

Radial velocity time series (top panel) and phase-folded plots of the planetary signals (TOI-6695b, bottom left; TOI-6695c, bottom right). In addition to the RVs from HARPS, CHIRON, PFS, and CORALIE, FEROS data are overlayed as grayed-out diamonds, to show their general agreement with our model, but also their overall poor quality.

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