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A Dark, Bare Rock for TOI-1685 b from a JWST NIRSpec G395H Phase Curve

  • Authors: Rafael Luque, Brandon Park Coy, Qiao Xue, Adina D. Feinstein, Eva-Maria Ahrer, Quentin Changeat, Michael Zhang, Sarah E. Moran, Jacob L. Bean, Edwin Kite, Megan Weiner Mansfield, Enric Pallé

Rafael Luque et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 9.

Same as Figure 1, but including a GP to the model. The gold dashed line is the same model in Figure 1 without GP, and the brown solid line is the model with GP. The bottom panel shows the difference between those two lines in ppm units. It is clear how the use of a GP is not only degenerate with the phase curve parameters, but also affects both the transit and eclipse depths.

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