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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 10.

GP-only component of the model shown in Figure 9 for NRS1 and NRS2. Despite having similar amplitudes and variability timescales, the correlated noise properties in NRS1 are different from those of NRS2.

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