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Table 1

Spectroscopic and photometric values of Teff and log g for stars without detectable interstellar NaD lines.

ID Teff(spec) log g(spec) [Fe/H] [α/Fe] Teff(b − y) Teff(V − K) log g(HIP) Comment
[K] [cgs] [K] [K] [cgs]
BD−21 3420 5808 4.26  −1.13 0.31 5855 5884 4.09  ± 0.18
CD−33 3337 5979 3.86  −1.36 0.30 6005 5924 4.08  ± 0.08
CD−45 3283 5597 4.55  −0.91 0.12 5646 5616 4.71  ± 0.13
CD−57 1633 5873 4.28  −0.90 0.07 5964 5874 4.26  ± 0.08
G13-38 5263 4.54  −0.88 0.32 5241 5279 4.45  ± 0.12
G18-28 5372 4.41  −0.83 0.31 5376 5320 4.58  ± 0.08 SB1 (1)
G46-31 5901 4.23  −0.83 0.15 5918 5811 4.15  ± 0.40 SB1 (1)
G56-30 5830 4.26  −0.89 0.11 5871 5824
G82-05 5277 4.45  −0.75 0.09 5312 5293 4.73  ± 0.14
G85-13 5628 4.38  −0.59 0.28 5631 5681 4.31  ± 0.20
G94-49 5373 4.50  −0.80 0.31 5346 5363
G99-21 5487 4.39  −0.67 0.29 5528 5536 4.31  ± 0.27
G119-64 6181 4.18  −1.48 0.28 6129 6165 4.07  ± 0.15
G121-12 5928 4.23  −0.93 0.10 5913 5919 4.17  ± 0.24
G159-50 5624 4.37  −0.93 0.31 5622 5660 4.29  ± 0.08
G172-61 5225 4.47  −1.00 0.19 5282 5242 SB1 (1)
G176-53 5523 4.48  −1.34 0.18 5522 5595 4.36  ± 0.10
G180-24 6004 4.21  −1.39 0.33 5958 5986 4.18  ± 0.11
G232-18 5559 4.48  −0.93 0.32 5505 5546
HD3567 6051 4.02  −1.16 0.21 6027 6014 4.12  ± 0.10
HD17820 5773 4.22  −0.67 0.29 5736 5787 4.20  ± 0.06
HD22879 5759 4.25  −0.85 0.31 5763 5754 4.25  ± 0.03
HD25704 5868 4.26  −0.85 0.24 5752 5659 4.20  ± 0.04 (2)
HD51754 5767 4.29  −0.58 0.26 5769 5814 4.24  ± 0.08
HD59392 6012 3.91  −1.60 0.32 5992 5976 3.99  ± 0.15
HD76932 5877 4.13  −0.87 0.29 5883 5871 4.13  ± 0.03
HD97320 6008 4.19  −1.17 0.28 5979 5992 4.22  ± 0.04
HD106516 6196 4.42  −0.68 0.29 6202 6169 4.36  ± 0.03 SB1 (3)
HD114762A 5856 4.21  −0.70 0.24 5815 5748 4.19  ± 0.04
HD120559 5412 4.50  −0.89 0.30 5361 5352 4.56  ± 0.04
HD121004 5669 4.37  −0.70 0.32 5596 5601 4.36  ± 0.07
HD126681 5507 4.45  −1.17 0.35 5506 5497 4.61  ± 0.06
HD148816 5823 4.13  −0.73 0.27 5809 5803 4.10  ± 0.04
HD159482 5737 4.31  −0.73 0.30 5687 5614 4.36  ± 0.06 (2)
HD175179 5713 4.33  −0.65 0.29 5687 5719 4.31  ± 0.08
HD177095 5349 4.39  −0.74 0.31 5321 5375 4.45  ± 0.08
HD189558 5617 3.80  −1.12 0.33 5612 5652 3.82  ± 0.05
HD193901 5656 4.36  −1.09 0.16 5636 5743 4.47  ± 0.05
HD194598 5942 4.33  −1.09 0.18 5936 6000 4.22  ± 0.05
HD199289 5810 4.28  −1.04 0.30 5754 5849 4.23  ± 0.05
HD205650 5698 4.32  −1.17 0.30 5691 5808 4.44  ± 0.06
HD219617 5862 4.28  −1.45 0.28 5887 5967 4.26  ± 0.11 (2)
HD222766 5334 4.27  −0.67 0.30 5380 5380 4.14  ± 0.19
HD230409 5318 4.54  −0.85 0.27 5258 5336 4.49  ± 0.11
HD233511 6006 4.23  −1.55 0.34 5932 5985 4.28  ± 0.14
HD237822 5603 4.33  −0.45 0.29 5621 5611 4.49  ± 0.13
HD241253 5831 4.31  −1.10 0.29 5834 5897 4.15  ± 0.18
HD250792A 5489 4.47  −1.01 0.24 5511 5363 4.37  ± 0.11 (2)

References. (1) Latham et al. (2002). (2) ESA (1997). (3) Ducati et al. (2011).

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