Table A.1.
Atmospheric and stellar parameters of the program stars.
Notes. The identification numbers in the first column correspond to those in Table 1. The given uncertainties are 1σ confidence intervals.
The atmospheric parameters are based on spectra taken with instruments abbreviated as follows: A (AAOmega, Sharp et al. 2006), E (ESI, Sheinis et al. 2002), FE (FEROS, Kaufer et al. 1999), FI (FIES, Telting et al. 2014), L (LAMOST, Cui et al. 2012), M (MMT, Brown et al. 2014), S (SDSS, Smee et al. 2013), and U (UVES, Dekker et al. 2000). The approximate resolving power of the individual spectra, λ/Δλ or Δλ, is given in brackets.
The references for the atmospheric and stellar parameters are abbreviated as follows: C (current work), H (Huang et al. 2017), I (Irrgang et al. 2019), KO (Koposov et al. 2020), KR (Kreuzer et al. 2020), and T (Tillich et al. 2009).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.