Hot Exoplanet Atmospheres Resolved with Transit Spectroscopy (HEARTS) - VII. Detection of sodium on the long-transiting inflated sub-Saturn KELT-11 b

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Table 4

Comparison of the different models.

Model	ln Z	ln B₀₁	Strength of evidence^(a)
isothermal	555.74 ± 0.24	–	–
ver_cosθ	558.00 ± 0.25	2.26	Weak – moderate
srot_cosθ	559.81 ± 0.35	4.07	Moderate
dtn_cosθ	562.87 ± 0.33	7.13	Strong

Notes. ^(a)The base model to calculate ln B₀₁ is the isothermal model without added wind patterns. The comparison stems from the Jeffrey scale.

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