Table 5
Detected Fe II lines in the atmosphere of KELT-9b.
Line | h [%] | FWHM [km s−1] | Kp [km s−1] | vsys + vwind [km s−1 ] | vsys [km s−1] | Rλ [Rp] | νmic [km s−1] | νmac [km s−1] | Reff [Rp] |
---|---|---|---|---|---|---|---|---|---|
λ4173.45 | -0.22 ± 0.3 | ![]() |
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![]() |
0.91 ± 0.3 | ![]() |
![]() |
1.15 ± 0.02 |
λ4233.16 | -0.30 ± 0.03 | ![]() |
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![]() |
![]() |
0.88 ± 0.03 | ![]() |
![]() |
1.20 ± 0.02 |
λ4351.76 | -0.21 ± 0.03 | ![]() |
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![]() |
![]() |
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![]() |
![]() |
![]() |
λ4385.37 | ![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
![]() |
1.10 ± 0.03 |
λ4489.17 | ![]() |
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![]() |
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![]() |
![]() |
![]() |
1.06 ± 0.04 |
λ4508.28 | -0.13 ± 0.03 | ![]() |
![]() |
![]() |
![]() |
0.31 ± 0.04 | *![]() |
![]() |
1.09 ± 0.02 |
λ4515.76 | -0.15 ± 0.03 | ![]() |
![]() |
![]() |
![]() |
0.92 ± 0.04 | ![]() |
![]() |
1.11 ± 0.02 |
λ4520.21 | ![]() |
![]() |
![]() |
![]() |
![]() |
1.11 ± 0.03 | *![]() |
![]() |
1.11 ± 0.04 |
λ4522.63 | -0.18 ± 0.03 | ![]() |
![]() |
![]() |
![]() |
1.08 ± 0.03 | ![]() |
![]() |
1.13 ± 0.02 |
λ4555.89 | -0.19 ± 0.03 | ![]() |
![]() |
![]() |
![]() |
0.97 ± 0.03 | ![]() |
![]() |
1.13 ± 0.02 |
λ4583.83 | -0.30 ± 0.02 | ![]() |
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![]() |
![]() |
0.92 ± 0.03 | ![]() |
![]() |
1.20 ± 0.01 |
λ4620.51 | -0.08 ± 0.03 | ![]() |
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![]() |
0.93 ± 0.05 | ![]() |
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1.05 ± 0.02 |
λ4629.33 | -0.17 ± 0.03 | ![]() |
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![]() |
![]() |
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1.12 ± 0.02 |
λ4923.93 | ![]() |
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![]() |
![]() |
![]() |
1.12± 0.03 | ![]() |
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1.27 ± 0.01 |
λ5018.43 | -0.38 ± 0.02 | ![]() |
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![]() |
1.14 ±0.03 | ![]() |
![]() |
1.25 ± 0.01 |
λ5169.03 | -0.48 ± 0.02 | ![]() |
![]() |
![]() |
![]() |
1.25±0.02 | ![]() |
![]() |
1.31 ± 0.01 |
λ5197.57 | -0.16 ± 0.02 | ![]() |
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![]() |
![]() |
![]() |
![]() |
![]() |
1.11 ± 0.01 |
λ5234.62 | -0.16 ± 0.02 | ![]() |
![]() |
![]() |
![]() |
1.23±0.04 | ![]() |
![]() |
1.11 ±0.01 |
λ5275.99 | -0.23 ± 0.02 | ![]() |
![]() |
![]() |
![]() |
1.12±0.04 | ![]() |
*![]() |
1.16 ± 0.02 |
λ5316.6 | -0.29 ± 0.02 | ![]() |
![]() |
![]() |
![]() |
1.26±0.03 | ![]() |
*![]() |
1.19 ± 0.01 |
λ5362.86 | -0.12 ± 0.02 | ![]() |
![]() |
![]() |
![]() |
1.31 ± 0.05 | ![]() |
![]() |
1.08 ± 0.01 |
Notes. The list includes the parameters fitted in the MCMC analysis to detect the planetary signal, as well as the MCMC analysis to fit the micro- and macroturbulence velocity to the observed transmission spectrum based on the NLTE synthetic transmission spectra. The values marked with an asterisk “*” are consistent with 0 km s−1.
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