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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 3.

TLS power spectrum periodogram of TOI-6695. The top panel shows the results of the detrended and normalized TESS and OMES light curves. The bottom panel shows the residual TLS power after subtracting the full photodynamical model. The dashed blue line represents the orbital period of the transiting planet candidate, whereas dashed horizontal lines indicate the TLS signal detection efficiency (M. Hippke et al. 2019) power levels of 5.7, 7.0, and 8.3, which correspond to false-alarm-probability (FAP) levels of 10%, 1%, and 0.1%, respectively.

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