Open Access

Table A.1

Stellar parameters and correlations

Name B-V TS Teff FeH Number Time logI Global Nb. of LT Nb. of ST
(K) of nights span (nights) Correlation seasons Correlation subsets Correlation
HD132052 0.32 F0V 69275 -0.015 16 1955 -4.39 -0.59 -0.02± 0.10 1 - 0 -
HD218396 0.26 F0V 76566 -0.477 15 3667 -4.19 -0.74 0.67± 0.03 1 - 0 -
HD109085 0.38 F2V 68264 -0.074 18 1957 -4.52 -0.82 0.59± 0.10 1 - 0 -
HD164259 0.36 F2V 66275 -0.195 14 2608 -4.49 -0.76 0.08± 0.15 1 - 0 -
HD49933 0.35 F3V 65353 -0.403 26 2589 -4.49 -0.94 0.964±0.004 3 - 2 0.93± 0.01
HD4247 0.30 F3V 69454 -0.374 17 2163 -4.32 -0.78 0.61± 0.08 1 - 1 0.17± 0.20

Notes. The full table is available at the CDS. Only a few lines are shown here to illustrate the content. B, V, and spectral type are from the CDS. Luminosity classes are from the CDS, except for HD163441 (Lorenzo-Oliveira et al. 2018), HD78534 (dos Santos et al. 2016), and HD141943 (Grandjean et al. 2020). Teff values have been shifted depending on the reference to produce a data set that is as homogeneous as possible following the temperatures provided in Sousa et al. (2008), as in Meunier et al. (2017). The number of seasons refers to those with at least five nights. References for Teff and metallicities, indicated as exponents, are the following: (1) Sousa et al. (2008), (2) Ramírez et al. (2014), Teff shifted by +5 K, (3) Marsden et al. (2014), Teff shifted by +13 K (4) Gray et al. (2006), Teff shifted by +42 K, (5) Holmberg et al. (2009), Teff shifted by -71 K (6) Ammons et al. (2006), Teff shifted by +61 K, (7) Gáspár et al. (2016), (8) Mortier et al. (2013), (9) Soubiran et al. (2016), and Teff shifted by +16 K.

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