Table 3: Fitted parameters of the white dwarfs and supplementary data from literature. The three objects with positive detections of magnetic fields are labelled in bold face.
\begin{displaymath}{\begin{tabular}[c]{l\vert rlcrr\vert r@{.}ll\vert cc} \hline... ...& & \\ &&&&&& 8&67 & 8.83$^{11}$ &&\\ \hline \end{tabular}} \end{displaymath}
References: 1Bergeron et al. (1989); 2Bergeron et al. (1992); 3Bergeron et al. (2001); 4Bragaglia et al. (1995); 5Finley et al. (1997); 6Kawka et al. (2000); 7Kepler & Nelan (1993); 8Kidder et al. (1992); 9Koester & Allard (1993); 10Koester et al. (1998); 11Koester et al. (2001); 12Napiwotzki et al. (1999); 13Pilachowski & Milkey (1984); 14Saffer et al. (1988); 15van Altena et al. (1995); 16Vauclair et al. (1997); 17Vennes (1999); 18Vennes et al. (1997).
* Gravity fixed at a value which reproduced the absolute brightness computed from the parallax.

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