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How Many Transiting Giant Planets Can JWST Search for Moons and Rotational Oblateness?

  • Authors: Le-Chris Wang, 乐 王, Joshua N. Winn, 乔书 温

Le-Chris Wang et al 2026 The Astrophysical Journal Letters 1006 .

  • Provider: AAS Journals

Caption: Figure 1.

JWST photometric precision per minute, based on bandpass-summed time series data and plotted vs. apparent K magnitude. (a) Empirically measured scatter reported in the literature (points), compared with ETC predictions from PandExo for three instruments/modes (curves). The dashed curve is a fitting function for the lower envelope of the ETC predictions (Equation (1)); in this fit, NIRISS/SOSS is favored for K < 11.2 and NIRSpec/PRISM at fainter magnitudes. (b) Same, but with curves fitted to empirical scatter rather than ETC predictions (Equation (2)); in this model, NIRSpec/G395H is favored for K < 9.5 and NIRSpec/PRISM at fainter magnitudes.

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