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This article has an erratum: [https://doi.org/10.1051/0004-6361/202556143e]


Table 2

Best-fit posterior estimates.

Parameter Value
R [R] 0.372290.00896+0.00921$\[0.37229_{-0.00896}^{+0.00921}\]$
M [M] 0.35300.0082+0.0080$\[0.3530_{-0.0082}^{+0.0080}\]$
T0 [BJD] 2458765.676810.00092+0.00089$\[2458 ~765.67681_{-0.00092}^{+0.00089}\]$
P [days] 1.880516090.00000143+0.00000146$\[1.88051609_{-0.00000143}^{+0.00000146}\]$
b 0.4600.052+0.050$\[0.460_{-0.052}^{+0.050}\]$
Rp/R 0.03450.00099+0.00099$\[0.0345_{-0.00099}^{+0.00099}\]$
fp / fs, joint, [ppm] 31130+31$\[311_{-30}^{+31}\]$
fp / fs, 1 [ppm] 23953+50$\[239_{-53}^{+50}\]$
fp / fs, 2 [ppm] 34153+52$\[341_{-53}^{+52}\]$
fp / fs, 3 [ppm] 35752+52$\[357_{-52}^{+52}\]$
log(s) 7.1720.012+0.012$\[-7.172_{-0.012}^{+0.012}\]$

Notes. The number in the subscript in the occultation depth parameter fp/ fs refers to the corresponding visit, and joint means that the orbital parameters of the three light curves are shared, but the systematics parameters were still allowed to vary individually. log(s) is the natural logarithm of the flux uncertainty for each measurement.

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