Unveiling the internal structure and formation history of the three planets transiting HIP 29442 (TOI-469) with CHEOPS

Open Access

Table B.2

Time needed to calculate the transit radii of 100 randomly sampled planetary structures from the posteriors of the internal structure models for HIP 29442 b, c, and d, both with the trained DNNs and the full planetary structure model from BICEPS.

Model	HIP 29442 b			HIP 29442 c			HIP 29442 d
Model	t_BICEPS [s]	t_DNN [s]	Speed-up	t_BICEPS [s]	t_DNN [s]	Speed-up	t_BICEPS [s]	t_DNN [s]	Speed-up
A1	1363	0.034	40088×	1462	0.038	38474×	1454	0.034	42706×
A2	1209	0.031	39000×	1415	0.036	39306×	1402	0.036	38944×
A3	1350	0.032	42188×	1372	0.035	39200×	1341	0.035	38314×

B1	2414	0.036	67056×	2405	0.035	68714×	2403	0.038	63237×
B2	2070	0.035	59143×	2085	0.036	57917×	2079	0.038	54711×
B3	2329	0.036	64694×	2295	0.035	65571×	2295	0.034	67500×

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