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Table 3

Flux deviations from HD 97658 reference Lyman-α spectra.

Visit Orbit Spectral range Amplitude S / N p-value

1 0 N/D
1 [264; 238] 33.6 ± 17.6% 2.0 71%
2 [251; 67 ] 10.5 ± 3.7% 2.9 12%
3 N/D
4 [185; 27] 10.3 ± 4.0% 2.6 26%
[264; 211] 48.6 ± 22.2% 2.2 49%

0 [157; 236] 18.9 ± 9.4% 2.0 63%
1 [78; 118] 12.0 ± 5.8% 2.1 59%
2 N/D
3 [131; 184] 20.0 ± 7.8% 2.6 25%
4 [65; 118] 13.4 ± 5.8% 2.3 39%

2 0 [184; 39] 11.9 ± 4.5% 2.6 20%
1 N/D
2 N/D
3 [197; 158] 28.6 ± 10.4% 2.8 15%
4 [66; 26.] 14.6 ± 7.0% 2.1 55%

0 [40; 184] 20.9 ± 5.5% 3.8 0.6%
1 N/D
2 N/D
3 [40; 171] 14.4 ± 4.4% 3.3 3.7%
4 N/D

3 0 N/D
1 N/D
2 [113; 34] 11.4 ± 4.5% 2.5 26%
[245; 179] 24.7 ± 11.1% 2.2 47%
3 N/D
4 N/D

0 [150; 282] 18.3 ± 8.5% 2.2 52%
1 N/D
2 N/D
3 [203; 242] 49.1 ± 24.5% 2.0 64%
4 N/D

Notes. In each visit, the upper subpanel corresponds to the blue wing of the line, the lower subpanel to the red wing. N/D indicates that no variations were found above 2σ from the reference spectrum of the visit. Spectral ranges are given as velocities in the star rest frame (km s-1), and flux variations are in erg s-1 cm-2 Å-1.

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