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Validation of TOI-1221 b: A Warm Sub-Neptune Exhibiting Transit Timing Variations around a Sun-like Star

  • Authors: Christopher Mann, David Lafreniére, Diana Dragomir, Samuel N. Quinn, Thiam-Guan Tan, Karen A. Collins, Steve B. Howell, Carl Ziegler, Andrew W. Mann, Keivan G. Stassun, Martti H. Kristiansen, Hugh Osborn, Tabetha Boyajian, Nora Eisner, Coel Hellier, George R. Ricker, Roland Vanderspek, David W. Latham, S. Seager, Joshua N. Winn, Jon M. Jenkins, Jesus Noel Villaseñor, Brian McLean, Pamela Rowden, Guillermo Torres, Douglas A. Caldwell, Kevin I. Collins, Richard P. Schwarz

Christopher Mann et al 2023 The Astronomical Journal 165 .

  • Provider: AAS Journals

Caption: Figure 1.

First row: sector-by-sector PDCSAP flux, normalized to within-sector median. Purple bars indicate where transits were detected, orange bars indicate where expected transits fell in observing gaps. Rows 2 and 3: zoomed plot of each of the six caught transits. The TESS data were taken at a cadence of 2 minutes and are shown binned to 60 minute intervals with cyan points. The displayed transit model is described in Sections 3 and 4. Orange vertical lines show the predicted midpoints given a fixed-period ephemeris. Dashed black lines indicate the fitted midpoints, showing TTVs described in Section 3.4.

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