Extended Data Fig. 2: Best-fit orbital parameters for WASP-39b (a-e) and the radial velocity measurements (f).
From: A benchmark JWST near-infrared spectrum for the exoplanet WASP-39 b
The measured transit depth varies between instrumental modes as they each span a different wavelength range. The best-fitting model to the radial velocity data (solid line) alongside its 1, 2, and 3σ contours (shaded regions) are also indicated.
