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Table 4

Statistical results of the atmospheric retrieval analysis and the stellar contamination modelling on TRAPPIST-1h HST WFC3 G141 data.

Model χ2 log(E) Δlog(E)
Flat-line 64.95 3.61 110.55 N/A
Atmosphere primary 65.20 3.62 109.92 –0.63
Atmosphere secondary 65.25 3.62 110.18 –0.37
Stellar Zhang et al. (2018) 54.02 3.00 N/A N/A
Stellar Wakeford et al. (2019) 60.70 3.37 N/A N/A
Stellar Morris et al. (2018) 63.91 3.55 N/A N/A

Corrected by Zhang et al. (2018)
Flat-line 54.94 3.05 115.48 N/A
Atmosphere primary 50.54 2.81 115.02 –0.46
Atmosphere secondary 54.77 3.04 115.20 –0.28

Corrected by Wakeford et al. (2019)
Flat-line 61.41 3.41 112.13 N/A
Atmosphere primary 61.91 3.44 111.51 –0.62
Atmosphere secondary 61.80 3.43 112.01 –0.12

Corrected by Morris et al. (2018)
Flat-line 65.11 3.62 110.39 N/A
Atmosphere primary 65.28 3.63 109.79 –0.60
Atmosphere secondary 65.23 3.62 110.12 –0.27

Notes. Chi-squared (χ2) and reduced chi-squared (2) were computed using the result of the retrieval best-fit model and the stellar contamination models. Bayesian logarithm evidence (log(E)) and the Bayes factor (Δlog(E)) were computed when applicable, i.e. only for the atmospheric retrieval analysis.

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