Open Access

Table A.1

Comparison of white-light and photometric occultation depths from different methods

Visit stark Eureka! Eureka! HANSOLO transitspectroscopy SPARTA
(ppm) R1 (ppm) R2 (ppm) (ppm) (ppm) (ppm)
White-light occultation depths
Visit 1 (Nov 18, 2022) 7.08.8+8.8$7.0_{ - 8.8}^{ + 8.8}$ 49.212.3+12.4$49.2_{ - 12.3}^{ + 12.4}$ 2.62.6+14.1$2.6_{ - 2.6}^{ + 14.1}$ 15.911.4+11.6$15.9_{ - 11.4}^{ + 11.6}$ 52.110.3+11.1$52.1_{ - 10.3}^{ + 11.1}$
Visit 2 (Nov 20, 2022) 65.242.2+22.3$65.2_{ - 42.2}^{ + 22.3}$ 85.19.8+9.6$85.1_{ - 9.8}^{ + 9.6}$ 6.46.1+31.0$6.4_{ - 6.1}^{ + 31.0}$ 52.211.5+11.5$52.2_{ - 11.5}^{ + 11.5}$ 79.09.5+10.0$79.0_{ - 9.5}^{ + 10.0}$
Visit 3 (Nov 23, 2022) 101.432.4+17.1$101.4_{ - 32.4}^{ + 17.1}$ 130.911.3+10.3$130.9_{ - 11.3}^{ + 10.3}$ 112.131.9+28.4$112.1_{ - 31.9}^{ + 28.4}$ 141.912.0+11.5$141.9_{ - 12.0}^{ + 11.5}$ 119.110.3+10.8$119.1_{ - 10.3}^{ + 10.8}$
Visit 4 (Nov 24, 2022) 119.219.0+34.0$119.2_{ - 19.0}^{ + 34.0}$ 134.19.5+9.6$134.1_{ - 9.5}^{ + 9.6}$ 37.824.1+28.8$37.8_{ - 24.1}^{ + 28.8}$ 115.58.9+8.9$115.5_{ - 8.9}^{ + 8.9}$ 82.918.3+18.0$82.9_{ - 18.3}^{ + 18.0}$
Visit 5 (Apr 24, 2023) 95.416.8+13.5$95.4_{ - 16.8}^{ + 13.5}$ 106.711.7+9.2$106.7_{ - 11.7}^{ + 9.2}$ 73.521.4+21.3$73.5_{ - 21.4}^{ + 21.3}$ 98.610.8+11.0$98.6_{ - 10.8}^{ + 11.0}$ 95.910.1+11.3$95.9_{ - 10.1}^{ + 11.3}$

Photometric occultation depths

Visit 1 (Nov 18, 2022) 47.415.5+21.0${47.4_{ - 15.5}^{ + 21.0}}$ 42.84.7+4.9${42.8_{ - 4.7}^{ + 4.9}}$
Visit 2 (Nov 20, 2022) 5.16.0+5.5${ - 5.1_{ - 6.0}^{ + 5.5}}$ 9.86.0+5.6${ - 9.8_{ - 6.0}^{ + 5.6}}$
Visit 3 (Nov 23, 2022) 37.34.6+4.7${37.3_{ - 4.6}^{ + 4.7}}$ 28.25.6+5.5${28.2_{ - 5.6}^{ + 5.5}}$
Visit 4 (Nov 24, 2022) 36.832.9+27.7${36.8_{ - 32.9}^{ + 27.7}}$ 39.55.6+6.0${39.5_{ - 5.6}^{ + 6.0}}$
Visit 5 (Apr 24, 2023) 95.97.9+8.1${95.9_{ - 7.9}^{ + 8.1}}$ 92.45.5+5.9${92.4_{ - 5.5}^{ + 5.9}}$

Notes. The uncertainties are 68 percentile of the corresponding posterior distribution. Visit 4 is the archival observation from Hu et al. (2024).

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