Fig. 1: The light curve of WASP-107b observed by JWST-NIRSpec G395H.
From: A warm Neptune’s methane reveals core mass and vigorous atmospheric mixing
a, The normalized wavelength-integrated white-light curves for the two detectors are shown, with the NRS1 (2.70–3.71 μm) and NRS2 (3.83–5.16 μm) detectors offset for clarity. A best-fit limb-darkened transit model is overplotted (blue). See Extended Data Fig. 2 for further details. b, The model residuals that achieve near-photon limited precisions.
