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Table 1

Stellar characteristics of the analysed planet-host candidates (the first three stars are presented here for the first time).

NGC 3680 No. 41 NGC 2345 No. 50 NGC 3532 No. 670 IC4651 No. 9122 NGC 2423 No. 3 NGC 4349 No. 127
Teff K 4612 ± 12 3962 ± 10 4347 ± 11 4582 ± 12 4534 ± 12 4417 ± 12
log ɡ (cm s−2) 2.45 ± 0.04 0.87 ± 0.07 1.75 ± 0.05 2.43 ± 0.04 2.23 ± 0.04 1.78 ± 0.05
[Fe/H] −0.16 ± 0.02 −0.25 ± 0.02 −0.11 ± 0.02 −0.03 ± 0.01 −0.08 ± 0.01 −0.17 ± 0.02
v sin i (km s−1) 5.27 4.64 0.68 2.19 4.81
M M 1.64 ± 0.06 5.84 ± 0.61 3.05 ± 0.23 1.79 ± 0.09 2.03 ± 0.14 3.01 ± 0.24
R R 11.44 ± 0.57 152.28 ± 17.78 40.95 ± 2.37 13.36 ± 0.72 17.71 ± 1.04 37.97 ± 2.56
log(L) L 1.85 3.86 2.73 1.94 2.12 2.76
Age Ga 1.78 0.07 0.35 1.58 1.02 0.32

Distance 938 2251 486 888 766 2176
V mag 10.88 10.40 6.98 10.91 10.04 ± 0.04 10.82 ± 0.08
α 11:25:48.5 07:08:27.0 11:07:57.3 17:24:50.1 07:37:09.2 12:24:35.5
δ −43:09:52.5 −13:12:32.9 –58:17:26.3 −49:56:56.1 –13:54:24.0 –61:49:11.7

Notes. Stellar parameters (above the horizontal line) were derived by Tsantaki et al. (2023). Distances and magnitudes are extracted from WEBDA and SIMBAD, respectively.

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