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Table B.1

Coefficients found for the photometric baselines models fitted jointly with the physical light curve model.

Occultations

Date 19 March 2020 27 March 2020
A0
     
A1
     
A2
     
D1

Date 30 March 2020 07 April 2020

A0
     
A1 0.000189 ± 0.000019
     
A2 0
     
D1 2.29 ± 0.16

Transits

Date 15 June 2020 18 June 2020

Flux shift (ppm) − 61 ± 7
c1 (ppm) − 76 ± 14 − 30 ± 14
c2 (ppm) + 74 ± 11 − 5 ± 10
c3 (ppm) + 78 ± 16 + 23 ± 17
c4 (ppm) + 18 ± 9 + 6 ± 9
s1 (ppm) − 40 ± 14 + 90 ± 11
s2 (ppm) − 74 ± 19 + 17 ± 21
s3 (ppm) + 3 ± 11 − 13 ± 11
s4 (ppm) + 26 ± 9 − 16 ± 10

Notes. For the occultations, Ai refer to the coefficients of second-order polynomials in time, with A0 denoting the normalisation constant. D1 is the coefficient of a linear trend with contamination. For the transits, c stand for the cosine, and s for the sine terms of the Fourier-series.

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