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Table 1

Photometric and spectroscopic data for the program stars with VT ≤ 8.0.

HD V Tycho (B − V)Johnson (B − V)Tycho (b − y) m 1 S C T eff phot [Fe/H]phot σ () λ6145 λ6563 FEROS UV
1835 6.5 0.659 0.758 0.422 0.225 4.03 5686 −0.10 4.90 0.05 – – –
4308 6.6 0.655 0.723 0.402 0.198 2.24 5743 −0.17 4.93 0.04 280 180 – √
9986 6.8 0.648 0.720 0.408 0.217 0.22 5785 −0.01 4.79 0.06 – – 220
11131 6.8 0.654 0.711 0.403 0.188 4.85 5711 −0.31 4.98 0.23 – – –
13724 8.0 0.667 0.746 0.414 0.228 1.69 5753 +0.04 4.78 0.10 70 140 – √
18757 6.7 0.634 0.729 0.417 0.191 5.40 5639 −0.45 4.92 0.05 – – –
19518 7.9 0.642 0.731 0.399 0.203 2.10 5784 −0.08 4.84 0.11 120 – 450 √
24293 7.9 0.658 0.727 0.412 0.211 0.58 5724 −0.14 4.79 0.10 60 90 – √
25680 6.0 0.620 0.720 0.397 0.212 3.45 5854 +0.05 4.85 0.05 – – –
25874 6.8 0.667 0.747 0.410 0.227 1.06 5774 +0.08 4.77 0.04 170 170 –
28471 8.0 0.650 0.717 0.399 0.210 1.38 5812 +0.00 4.79 0.08 – – –
28701 7.9 0.650 0.710 0.402 0.186 5.64 5714 −0.32 4.76 0.08 – – –
28821 7.7 0.683 0.747 0.422 0.205 5.31 5597 −0.35 4.85 0.10 80 170 – √
30495 5.6 0.632 0.710 0.399 0.213 2.18 5844 +0.04 4.94 0.04 260 380 –
32963 7.7 0.664 0.743 0.403 0.237 2.46 5858 +0.29 4.92 0.10 – – 410 √
35041 7.7 0.636 0.731 0.395 0.213 2.58 5847 +0.08 4.89 0.10 – – 250 √
37773 7.8 0.692 0.746 0.429 0.236 10.90 5656 −0.08 4.90 0.11 – – 610 √
64184 7.6 0.675 0.755 0.420 0.218 3.45 5661 −0.16 4.95 0.07 – – –
66653 7.6 0.655 0.726 0.400 0.222 0.85 5839 +0.14 4.80 0.06 130 – 560 √
68168 7.4 0.667 0.729 0.419 0.224 2.52 5717 −0.07 4.79 0.09 – – 630 √
70516 7.8 0.652 0.725 0.415 0.222 1.08 5753 −0.04 4.93 0.19 – – –
71334 7.9 0.643 0.746 0.408 0.220 0.39 5782 +0.02 4.92 0.09 – 220 660 √
73350 6.8 0.655 0.731 0.405 0.224 0.31 5815 +0.11 4.95 0.07 180 210 700
76151 6.1 0.661 0.752 0.410 0.239 2.93 5820 +0.23 4.91 0.04 – – –
77006 8.0 0.651 0.707 0.384 0.202 9.07 5867 +0.05 4.82 0.11 – – –
86226 8.0 0.647 0.719 0.381 0.204 10.48 5883 +0.10 4.85 0.10 – – –
88072 7.6 0.647 0.753 0.404 0.221 0.63 5801 +0.08 4.74 0.10 – – 250
88084 7.6 0.649 0.712 0.399 0.215 1.33 5835 +0.06 4.87 0.08 – – –
98618 7.7 0.642 0.713 0.404 0.208 1.10 5787 −0.07 4.78 0.09 – – –
108575 8.0 0.68 0.745 0.417 0.234 3.37 5745 +0.07 4.90 0.34 – – –
112257 7.9 0.665 0.758 0.417 0.223 2.30 5707 −0.05 4.76 0.11 – – –
114174 6.9 0.667 0.757 0.418 0.233 3.72 5737 +0.05 4.76 0.07 – – –
117939 7.4 0.669 0.738 0.409 0.208 0.83 5714 −0.13 4.96 0.07 140 120 –
134664 7.8 0.662 0.739 0.404 0.207 0.76 5746 −0.08 4.83 0.12 100 180 –
138573 7.3 0.656 0.745 0.413 0.228 1.24 5770 +0.05 4.85 0.07 130 120 –
139777 6.7 0.665 0.723 0.413 0.211 0.95 5715 −0.15 4.94 0.04 – – –
142072 7.9 0.670 0.749 0.420 0.210 3.21 5640 −0.26 4.83 0.11 120 170 –
145825 6.6 0.646 0.727 0.395 0.228 2.74 5895 +0.27 4.93 0.06 180 230 –
146233 5.6 0.652 0.736 0.400 0.221 0.78 5831 +0.13 4.83 0.04 340 230 380 √
150248 7.1 0.653 0.740 0.412 0.212 0.52 5723 −0.12 4.83 0.08 180 200 –
155114 7.6 0.637 0.720 0.396 0.197 4.27 5791 −0.12 4.85 0.09 140 120 – √
158222 7.9 0.667 0.727 0.414 0.219 0.99 5733 −0.06 4.83 0.08 – – –
164595 7.1 0.635 0.722 0.404 0.209 1.11 5790 −0.06 4.84 0.06 190 160 –
187237 7.0 0.660 0.718 0.402 0.215 0.62 5804 +0.03 4.88 0.05 – – 100
189567 6.1 0.648 0.718 0.399 0.199 2.76 5774 −0.13 4.90 0.04 – – –
189625 7.4 0.654 0.729 0.406 0.232 1.15 5840 +0.20 4.74 0.09 150 110 – √
190771 6.3 0.654 0.732 0.406 0.231 1.00 5834 +0.18 4.89 0.04 290 150 – √
202628 6.8 0.637 0.710 0.396 0.210 2.83 5845 +0.03 4.95 0.06 – – –
207043 7.7 0.660 0.737 0.410 0.228 0.80 5791 +0.09 5.01 0.08 130 160 –
214385 8.0 0.640 0.723 0.403 0.195 3.03 5740 −0.22 4.97 0.11 120 – – √
218739 7.2 0.658 0.716 0.398 0.212 1.53 5819 +0.04 4.86 0.16 – – –
222143 6.7 0.665 0.724 0.402 0.220 0.65 5814 +0.09 4.85 0.05 – – –

Notes. The second to sixth columns provide VTycho, (B − V)Johnson, (B − V)Tycho, (b − y), and m1, respectively. The seventh column gives the photometric similarity index with respect to the solar colors (see text). Columns 8 and 9 list the photometrically derived effective temperature Teff and metallicity. Columns 10 and 11 list the visual absolute magnitude from the Tycho VT band and its corresponding uncertainty, respectively. Columns 12–14 list the S/Ns of the spectroscopic observations as follows: λ6145 and λ6563 ranges from the OPD coudé spectrograph; FEROS spectrograph. The last column merely notes if low-resolution UV spectra from the Boller-Chivens Cassegrain spectrograph of the ESO 1.52 m telescope have been obtained.

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