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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 5.

Emission spectrum of TOI-1685 b using NIRSpec/G395H. Different data reductions follow the same color convention as Figure 4. Different symbols show different parts of the time series used in the fit as described in Section 3.2. Black circles represent the final emission spectrum from the prayer-bead analysis carried out in Section 3.3.3. The different data sets are offset slightly in wavelength to improve visualization.

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