The SPACE Program - I. The featureless spectrum of HD 86226 c challenges sub-Neptune atmosphere trends

Open Access

Table B.1

Transit depths of HD 86226 c derived with Eureka!.

Wavelength μm	Transit Depth ppm	Uncertainty ppm	β
Broadband	460	17	2.3
1.13	636	66	2.1
1.15	464	42	2.5
1.17	404	49	2.6
1.19	414	46	2.8
1.21	526	57	2.6
1.23	378	44	2.8
1.25	465	29	2.3
1.27	412	22	2.0
1.29	518	26	1.9
1.31	433	23	1.5
1.33	422	25	1.7
1.35	439	17	1.5
1.37	467	16	1.4
1.39	501	22	1.5
1.41	410	22	1.5
1.43	440	27	1.9
1.45	465	18	1.4
1.47	483	22	1.4
1.49	459	24	1.5
1.51	427	18	1.4
1.53	437	22	1.6
1.55	477	16	1.3
1.57	371	23	1.8
1.59	467	14	1.3
1.61	416	24	1.5
1.63	438	32	1.9
1.65	413	65	2.8

Notes. This uncertainties in this table correspond to the 1 σ percentiles from the Eureka! output multiplied by the β-factor given in the last column. We did not include the 1.13 μm bin in our analysis.

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