Fig. 1
The four P i lines are here shown in the case of HD 13555. The observed spectrum (solid black) is compared to the synthetic profile (solid red) with the P abundance derived from the EW measurement. Also shown are the synthetic profiles obtained by changing the P abundance by ± 0.1 dex (solid green). The telluric absorption affecting the 1051 pm line is clearly visible in the upper-left panel.
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