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Table 4

Parameters derived from the reconstruction of the Lyman-α line profiles.

Parameter ISM properties Unit

log10N(H i) 18.18 cm-2
b(H i) 13.1 km s-1
γ(H i)/∗ 8.6 km s-1

Parameter Visit 0 Visit 1 Visit 2 Visit 3 Unit

Fit range [1214.661215.57] [1214.431216.89] [1214.441215.61] [1214.461216.91] Å
[1215.861216.67] [1215.771216.36] Å
[1216.521216.89] Å
χ 2 146.0 39.3 18.4 28.6
d.o.f 132 39 33 39

0.91 0.93 0.95
1.69 0.92 ± 0.08 0.94 1.03± 0.07 STIS pixels
3.8 5.7 ± 1.3 5.8 STIS pixels
fpeak(1 au) 14.2 14.1± 0.6 13.2 13.0 erg cm-2 s-1 Å-1
Δ vD 64.3 69.89 72.7 ± 3.4 71.0 ± 2.5 km s-1
a damp 0.037 0.048 ± 0.003 0.036 ± 0.007 0.044 ± 0.004
γ 2.3 5.4 ± 0.5 4.5 ± 0.6 4.3 ± 0.5 km s-1
FLyα(1 au) 7.6 8.4 ± 0.2 7.8 ± 0.2 7.8 ± 0.2 erg cm-2 s-1
FLyα(Earth) 4.0 4.4 ± 0.1 4.1 ± 0.1 4.1 ± 0.1 ×10-13 erg cm-2 s-1

Notes. FLyα is the flux integrated in the entire Lyman-α line, calculated at Earth distance and at 1 au from the star. ISM properties are derived from the reconstruction of the weighted mean of the Visits 1, 2, and 3 spectra, and from the single Visit 0 spectrum.

(†)

A pixel width is about 0.015 Å  for the E140M mode and 0.053 Å  for the G140M.

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