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Table A.1.

Atmospheric parameters, abundances, radial velocity, pulsation period and class of HD 331986, DO Hya and BPS CS 30317-056. All abundances are in NLTE with model atoms retrieved from the following sources: iron (Bergemann et al. 2012b; Semenova et al. 2020), calcium (Mashonkina et al. 2017; Semenova et al. 2020), titanium (Bergemann 2011), manganese (Bergemann et al. 2019), aluminium (Ezzeddine et al. 2018), magnesium (Bergemann et al. 2017), and strontium come from (Bergemann et al. 2012a; Gerber et al. 2023). The line list is available upon request.

star Teff logg Vmic [Fe/H] [Al/Fe] [Mg/Fe] [Ca/Fe] [Ti/Fe] [Mn/Fe] [Sr/Fe] RV Period class
(K) (dex) (km s−1) (km s−1) (days)
HD331986 6450±80 2.90±0.10 3.5±0.5 −3.40 ± 0.05 < 0 0.50±0.05 0.21±0.10 —- <  − 1.00 < −0.5 −97.2 ± 2.9 0.3711815 RRc
DO Hya 5835±80 2.50±0.10 3.1±0.5 −3.28 ± 0.02 −0.07 ± 0.10 0.55±0.03 0.22±0.10 0.61±0.02 −0.06±0.10 0.31±0.10 272.5 ± 6.8 0.7133254 RRab
BPS 6025±80 2.50±0.15 3.0±0.5 −2.77±0.05 −0.25±0.10 0.34±0.05 0.24±0.10 0.56±0.05 −0.37 ± 0.12 −0.02±0.08 −58.9 ± 4.6 0.7484904 RRab
CS 30317-056

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