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. 2023 Dec 23;527(4):12120–12139. doi: 10.1093/mnras/stad3973

Table 4.

Abundance sensitivity to stellar parameters. Effects on abundances are shown for the hot and cool ends of our sample, that is, the co-added spectra RGB1 and TOP3 in Table 3.

Species T eff +100 K log g +0.1 dex v mic +0.3 km s−1
TOP RGB TOP RGB TOP RGB
Inline graphic +0.077 +0.115 −0.001 −0.001 −0.004 +0.033
Inline graphic −0.037 −0.130 +0.030 +0.051 −0.013 −0.021
N (CN) … +0.249 … −0.021 … −0.022
Inline graphic −0.057 −0.092 +0.030 +0.034 −0.017 −0.020
Inline graphic +0.039 +0.064 −0.004 −0.011 −0.004 −0.011
Inline graphic +0.051 +0.053 −0.003 −0.003 −0.013 −0.015
Inline graphic +0.034 +0.032 +0.001 +0.005 −0.002 −0.026
Inline graphic +0.072 +0.111 −0.019 −0.024 −0.077 −0.148
Inline graphic +0.042 +0.073 −0.002 −0.009 −0.048 −0.099
Inline graphic +0.043 +0.060 +0.036 +0.025 +0.007 −0.038
Inline graphic +0.073 +0.097 −0.004 +0.000 −0.036 −0.075
Inline graphic +0.015 −0.029 +0.033 +0.017 −0.012 −0.038
Inline graphic +0.061 +0.092 +0.001 +0.008 −0.011 −0.070
Inline graphic +0.082 +0.079 +0.018 +0.010 −0.132 −0.242