|Name||Spectral type||Teff||log g||[Fe/H]||Reference|
|HD 15316||A2Iab||8770||1.7||–||Verdugo et al. (1999)|
|HD 13784||F0II2||7080||2.1||0.0||Luck (2014)|
|HD 40457 (CO Aur)||∼F5Ib (Classical Cepheid)||6620||2.5||−0.1||Luck (2014)|
|HD 187921 (SV Vul)||∼F8Ia (Classical Cepheid)||4900−6330||0.29−1.28||0.0||Luck (2018)|
|HD 12650||G2II||5325||2.7||–||Hohle et al. (2010)|
|HD 14346||K0II||4585||2.2||–||Hohle et al. (2010)|
Notes. The effective temperatures of the Cepheids depend on the phase at which the spectrum was collected. The same holds for the spectral type.
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