NOAO is operated by the Association of Universities for research in Astronomy, Inc., under contract with the National Science Foundation.

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Tables 2 and 3 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/391/1039

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...1995)

Their $T_{\rm eff}$ are very similar to those given by SF00.

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... 25 pc)

HIP 39780, 40843, 50384, 57629, 57757, 60098, 71284, 72567, 73996, 75971, 76568 & 86032.

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...T

The $T_{\rm eff}$ derived from each colour was given a weight that is proportional to the inverse square of its error (in K); these errors in $T_{\rm eff}$ were determined from the error in the colour using the $T_{\rm eff}$ vs. colour relation in Table 2.

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... 55 pc

Excluding stars where the error in their percentage polarization exceeds $30\times10^{-5}$ and five stars with intrinsic percentage polarizations that exceed $125\times10^{-5}$ .

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