Extended Data Table 2 All results from transit light-curve fits

From: Helium in the eroding atmosphere of an exoplanet

  1. Modified results from a previous study9 are included. RMS denotes the root mean square of the model residuals in parts per million (PPM). The second-to-last column is the RMS divided by the expected photon noise. The last column is the correction factor that we applied to account for stellar variability.
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