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Table 1

Basic data and atmospheric parameters of weak G-band stars derived from the Hipparcos catalogue for HIP stars (Col. 2).

HD No. HIP No. m v B − V π σ(π) σ(%) log(L/L) σ T eff σ log g σ Ref.

18474 13965 5.47 0.869 6.390 0.350 5.4 2.192 0.088 5140 110 2.59 0.20 H
18636 13865 7.63 0.897 3.480 0.570 16.3 1.864 0.184 5080 110 2.90 0.29 H
21018 15807 6.37 0.851 2.680 0.740 27.6 2.628 0.28 5300 80 2.21 0.39 H
26575 19509 6.43 1.070 3.800 0.390 10.2 2.332 0.128 4690 110 2.29 0.24 H
28932 21250 7.94 0.996 1.940 0.730 37.6 2.276 0.368 4880 90 2.42 0.48 H
31274 22620 7.13 0.958 3.730 0.380 10.1 2.072 0.128 5040 80 2.68 0.24 H
31869 9.27 0.92
36552 8.08 0.84 5250 1.5
40402 28184 8.55 0.930 1.870 1.390 74.3 2.044 0.688 5010 120 2.70 0.80 H
49960 32734 8.34 1.020 1.030 0.760 73.7 2.676 0.68 4830 80 2.00 0.79 H
56438 35016 8.10 1.033 1.820 0.640 35.1 2.284 0.344 4790 110 2.38 0.45 H
67728 39867 7.54 1.106 2.160 0.670 31.0 2.384 0.308 4660 90 2.23 0.42 H
78146 44636 8.57 1.160 0.840 0.990 117.8 2.824 1.064 4530 90 1.74 1.17 H
82595 8.20 1.00 4910 1.5
91805 51816 6.09 0.940 2.870 0.430 14.9 2.736 0.172 5350 80 2.11 0.28 H
94956 53561 8.45 0.960 2.580 0.790 30.6 1.816 0.308 4950 110 2.90 0.41 H
102851 57724 8.78 1.053 1.400 1.220 87.1 2.244 0.796 4760 110 2.40 0.91 H
119256 66975 7.29 1.123 4.160 1.110 26.6 2.000 0.272 4870 400 2.69 0.38 H
120213 68009 5.95 1.411 4.070 0.330 8.1 2.644 0.112 4120 100 1.76 0.22 A
120170 9.03 0.93 5265 2.70
124721 9.48 0.93
146116 79604 7.68 1.070 1.160 0.710 61.2 2.856 0.572 4720 80 1.78 0.68 H
165462 88671 6.32 1.014 4.650 0.480 10.3 2.172 0.128 4840 110 2.50 0.24 H
165634 88839 4.55 0.938 9.620 0.260 2.7 2.276 0.064 5060 260 2.48 0.17 H
166208 88788 5.00 0.913 7.960 0.620 7.7 2.200 0.108 5050 110 2.55 0.22 H
188328 97922 7.02 0.584 12.110 1.670 13.7 0.932 0.16 6040 90 4.13 0.27 H
204046 105901 9.00 1.037 1.390 1.270 91.3 2.160 0.836 4790 110 2.50 0.94 H
207774 107885 8.92 0.969 2.320 1.300 56.0 1.720 0.528 4940 80 2.99 0.64 H

Notes. Last column (H or A) means that the atmospheric parameters were derived according to the Houdashelt tabular data or the photometric calibration of Alonso respectively (see text).

References. H = Houdashelt (2000). A = Alonso et al. (1999).

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