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TESS Investigation—Demographics of Young Exoplanets (TI-DYE). III. An Inner Super-Earth in TOI 2076

  • Authors: Madyson G. Barber, Andrew W. Mann, Andrew Vanderburg, Andrew W. Boyle, Ana Isabel Lopez Murillo

Madyson G. Barber et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 2.

(Left) TESS light curve binned to 10 minutes intervals and phase-folded (gray points) with the full (unbinned) TESS light curve phase folded and binned to 15 minutes intervals for clarity (purple points). The best-fit transit model is shown as the bright, opaque red line with 25 model fits pulled from the posterior shown as the dark, translucent red lines. The best-fit GP stellar variability model has been removed from the data and transit model. (Right) Representative section of the TESS light curve (gray points) with the best-fit GP model (red line). Transits of TOI 2076 e are highlighted in purple, and transits of TOI 2076 b, c, and d are highlighted in pink, green, and blue, respectively.

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