Table A.1.
Total error in the abundance of zinc determined from the Zn I lines in the atmosphere of the Sun, σ(A)tot.
| Element | λ nm | σ(Teff) ±10 K, | σ(log g) ±0.02 | σ(ξt) ±0.06 km s−1 | σ(cont) | σ(fit) | σ(A)tot |
|---|---|---|---|---|---|---|---|
| Sun | |||||||
| Zn I | 472.21 | ±0.005 | ∓0.001 | ∓0.023 | ±0.015 | ±0.017 | 0.032 |
| Zn I | 481.05 | ±0.011 | ∓0.005 | ∓0.032 | ±0.016 | ±0.019 | 0.042 |
Notes. The sign ± or ∓ reflects the change in the elemental abundance that occurs due to the increase (top sign) or decrease (bottom sign) in the uncertainty from a given error source (as indicated in column header; see Paper II for details).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.