Geometric albedo of WASP-12 b and WASP-76 b in the CHEOPS and TESS bandpasses (Corrigendum)

Open Access

Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/202348502]
[https://doi.org/10.1051/0004-6361/202348270]

Table 1.

WASP-76b’s A_g estimates.

			Datasets
Bandpass	Optical species	D1^a:HST	D2^b:HST + Spitzer	D3^c:HST + Spitzer
	With TiO/VO	< 0.107	0.079 ± 0.014	0.118 ± 0.014
CHEOPS	Without TiO	0.072 ± 0.021	0.079 ± 0.014	0.119 ± 0.014
	Without TiO/VO	0.073 ± 0.021	0.078 ± 0.013	0.119 ± 0.014
	With TiO/VO	<0.13	0.093 ± 0.017	0.172 ± 0.018
TESS	Without TiO	0.082 ± 0.033	0.093 ± 0.018	0.173 ± 0.019
	Without TiO/VO	0.085 ± 0.032	0.092 ± 0.017	0.172 ± 0.018

Notes. Shown values and uncertainties correspond to the posterior distributions’ median and 16th-to-84th percentile span, respectively. Upper limits corresponds to the 99.7th percentile of the posterior distribution. ^(a) HST (Hubble Space Telescope) eclipse depths from Edwards et al. (2020). ^(b) HST eclipse depths from Edwards et al. (2020), Spitzer eclipse depths from Demangeon et al. (2024). ^(c) HST and Spitzer eclipse depths from Fu et al. (2021).

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