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Table 3

Stellar parameters and iron abundances for giants and dwarfs derived according to method M1.

MASH ASPL

HIP T eff log  g ξ logϵFeI N(FeI) logϵFeII N(FeII) T eff log  g ξ logϵFeI N(FeI) logϵFeII N(FeII)

20205 4874 2.61 1.30 7.62 ± 0.10 22 7.62 ± 0.09 11 4884 2.61 1.30 7.59 ± 0.06 20 7.59 ± 0.06 7
20455 4876 2.59 1.30 7.59 ± 0.10 22 7.62 ± 0.09 11 4876 2.59 1.35 7.56 ± 0.07 20 7.56 ± 0.06 7
20889 4817 2.65 1.35 7.70 ± 0.09 18 7.70 ± 0.10 10 4827 2.60 1.35 7.63 ± 0.08 18 7.63 ± 0.06 6

Average 7.64 ± 0.06 7.65 ± 0.05 7.59 ± 0.04 7.59 ± 0.04

HIP T eff log  g ξ logϵFeI N(FeI) logϵFeII N(FeII) T eff log  g ξ logϵFeI N(FeI) logϵFeII N(FeII)

18946 4661 4.54 0.75 7.63 ± 0.09 21 7.63 ± 0.11 6 4691 4.64 0.70 7.56 ± 0.09 17 7.56 ± 0.21 5
13976 5023 4.51 0.85 7.69 ± 0.07 22 7.69 ± 0.11 8 5013 4.61 0.80 7.64 ± 0.08 22 7.64 ± 0.08 5
19098 5178 4.59 0.85 7.62 ± 0.09 22 7.62 ± 0.06 9 5138 4.54 0.80 7.63 ± 0.09 24 7.63 ± 0.06 7
16529 5237 4.51 0.80 7.64 ± 0.10 22 7.64 ± 0.08 10 5207 4.51 0.85 7.62 ± 0.08 22 7.62 ± 0.05 6
19934 5361 4.57 0.90 7.64 ± 0.06 23 7.64 ± 0.06 9 5341 4.57 0.85 7.62 ± 0.08 27 7.62 ± 0.04 6
20130 5531 4.45 0.95 7.66 ± 0.09 28 7.66 ± 0.07 10 5511 4.55 0.90 7.62 ± 0.06 26 7.62 ± 0.07 7
20146 5563 4.33 1.00 7.67 ± 0.08 26 7.67 ± 0.08 10 5553 4.43 0.95 7.62 ± 0.07 28 7.62 ± 0.04 6
19781 5641 4.35 0.85 7.69 ± 0.09 30 7.69 ± 0.08 10 5621 4.40 0.90 7.60 ± 0.06 27 7.60 ± 0.05 7
19793 5831 4.31 1.00 7.73 ± 0.08 29 7.73 ± 0.09 10 5781 4.41 0.95 7.64 ± 0.08 28 7.64 ± 0.05 7
20899 5916 4.31 0.90 7.66 ± 0.06 26 7.66 ± 0.08 10 5886 4.31 0.95 7.61 ± 0.08 27 7.61 ± 0.04 8
19148 6021 4.37 1.00 7.61 ± 0.06 28 7.61 ± 0.09 10 5961 4.37 0.85 7.62 ± 0.08 28 7.62 ± 0.04 7
22422 6074 4.34 1.05 7.66 ± 0.09 32 7.66 ± 0.08 10 6004 4.34 1.00 7.63 ± 0.06 30 7.63 ± 0.01 6
21112 6161 4.36 1.10 7.60 ± 0.09 34 7.63 ± 0.04 8 6161 4.26 1.05 7.60 ± 0.06 29 7.60 ± 0.03 7
22566 6251 4.30 1.10 7.69 ± 0.08 27 7.69 ± 0.09 9 6211 4.30 1.10 7.66 ± 0.08 26 7.66 ± 0.07 6

Average 7.66 ± 0.04 7.66 ± 0.03 7.62 ± 0.02 7.62 ± 0.02

Notes. The left side of the table shows the results obtained with the MASH line list and the right side the results obtained with the ASPL line list.

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