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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 21.

Results of the PCA for NRS1 (left three panels) and NRS2 (right three panels). We created 20 independent eigenvectors using the PCA functionality in scikit-learn. We show the results for a single spectroscopic channel (λcen = 4.143 ± 0.017). Top: black is the reduced spectroscopic light curve. Red is the light curve after it has been correlated against the four “best” eigenvectors, shown in the middle panel. Bottom: results of the Lomb–Scargle periodogram on the four eigenvectors in the middle plot.

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