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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 6.

Difference between the white light curves from each data reduction. Each panel shows the MAD of the data. Apart from the presence of a small linear trend (−34 ppm day−1 in NRS1 and 64 ppm day−1 in NRS2), the differences follow a Gaussian distribution, indicating that the presence and properties of correlated noise are pipeline-independent.

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