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Table 2.

STELLA observing log and results.

Name Time range NSpec texp S/N RV Teff log g v sin i [M/H]
(ddmmyy) (s) range (km s−1) (K) (cgs) (km s−1) (solar)
α Aur1 Ongoing ... 8 220–700 SB2 5150 1.7 4.5 −0.55
β Aur2 260516-020417 127 60 120–510 SB2 ... ... 29.3 ± 1.3 ...
ε Aur Ongoing ... 120 100–360 −3 var 7600 ± 110 0.0 ± 0.3 32 ± 4 0.0 ± 0.4
η Aur 110416-010417 109 60 80–270 10.2 var ... ... 66 ± 14 ...
θ Aur 040916-300317 163 250 110–680 30.5 var ... ... 54.6 ± 1.0 ...
ν Aur 130916-020417 103 60 80–220 13.0 var 4610 ± 50 2.2 ± 0.1 2.7 ± 0.2 −0.12 ± 0.03
ι Aur 080416-010417 104 60 100–400 18.1 var 4130 ± 60 1.25 ± 0.3 5.5 ± 1.0 −0.20 ± 0.03
κ1 Cet 091216-180217 28 1800 200–670 18.95 ± 0.03 5664 ± 13 4.46 ± 0.02 4.6 ± 0.2 −0.12 ± 0.03
V711 Tau1 091216-030417 116 1800 100–480 SB2 4420 var 2.5 ± 0.7 45.0 ± 1.0 −0.66 ± 0.33

Notes.RV⟩ are mean values. Time range is in standard UT time. “Ongoing” means that the target is continued to be observed whenever possible. The notation var indicates that the value is systematically changing. Error bars are rms. S/N is given per pixel; (1)for the primary; (2)same value for both components.

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