Table B.1
Parameters derived from individual windows in the IR spectrum.
| 10 500–10 920 | 11 760–12 600 | 15 110–15 697 | 15 815–16 390 | 16 439–17 140 | 21 017–22 850 | |
|---|---|---|---|---|---|---|
| Teff (K) | 5082 | 5051 | 4909 | 4942 | 4983 | 4981 |
| log g | 4.65 | 4.45 | 4.49 | 4.46 | 4.61 | 4.21 |
| v sin i (km s−1) | 2.59 | 2.59 | 2.59 | 2.59 | 2.59 | 2.59 |
| ξmic (km s−1) | 1.09 | 1.25 | 0.89 | 1.48 | 0.62 | 2.28 |
| ξmac (km s−1) | 2.08 | 2.30 | 3.91 | 4.34 | 3.84 | 4.81 |
| metallicity | −0.10 | −0.03 | −0.05 | −0.12 | −0.07 | −0.14 |
| B = 1700 G, f = 0.141 | ||||||
| Teff (K) | 5066 | 5081 | 4947 | 5048 | 5067 | 5044 |
| log g | 4.60 | 4.51 | 4.50 | 4.65 | 4.62 | 4.55 |
| v sin i (km s−1) | 2.8 | 2.8 | 2.8 | 2.8 | 2.8 | 2.8 |
| ξmic (km s−1) | 0.72 | 0.85 | 0.51 | 0.89 | 0.0 | 0.92 |
| ξmac (km s−1) | 1.90 | 1.28 | 3.19 | 3.46 | 3.55 | 4.01 |
| metallicity | −0.06 | −0.02 | −0.04 | −0.06 | −0.02 | −0.03 |
Notes. For fits using macroturbulence controlling broadening (top portion) with v sin i inferred from rotation period and radius, and no magnetic field. Fits using the magnetic field from the Zeeman broadening analysis (and v sin i from the visible spectrum analysis) are also presented (bottom portion).
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