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Table 3:

Stellar parameters for the white dwarfs and M-dwarfs in EC 12477-1738, EC 13349-3237 and EC 14329-1625 determined from a spectroscopic decomposition of the CTIO spectra.
  $T_{\rm wd}$ [K] $\log g$ $M_{\rm wd}~[M_\odot]$ $d_{\rm wd}$ [pc] Sp(sec) $d_{\rm sec}$ [pc]

EC 12477-1738
$18330\pm1212$ $8.08\pm0.26$ $0.67\pm0.16$ $111\pm19$ M$3\pm0.5$ $206\pm41$
  $17106\pm1131$ $7.88\pm0.26$ $0.55\pm0.15$ $151\pm24$ M$3\pm0.5$ $247\pm49$
  $\it {17718\pm865}$ $\it {7.98\pm0.14}$ $\it {0.61\pm0.08}$ $\it {131\pm28}$ $\it {M3\pm0.5}$ $\it {226\pm45}$
EC 13349-3237 $37424\pm3880$ $7.73\pm0.54$ $0.54\pm0.28$ $394\pm133$ M$1\pm0.5$ $321\pm63$
  $32595\pm2052$ $7.31\pm0.53$ $0.38\pm0.19$ $572\pm196$ M$1\pm0.5$ $373\pm73$
  $\it {35010\pm3415}$ $\it {7.52\pm0.30}$ $\it {0.46\pm0.11}$ $\it {483\pm126}$ $\it {M1\pm0.5}$ $\it {347\pm68}$
EC 14329-1625 $13904\pm1409$ $7.87\pm0.25$ $0.54\pm0.15$ $71\pm11$ M$3\pm0.5$ $120\pm24$
  $15246\pm1299$ $8.14\pm0.22$ $0.70\pm0.14$ $53\pm8$ M$3\pm0.5$ $106\pm21$
  $\it {14575\pm949}$ $\it {8.01\pm0.19}$ $\it {0.62\pm0.11}$ $\it {62\pm13}$ $\it {M3\pm0.5}$ $\it {113\pm10}$
Note: Three lines are given for each object, with the top (middle) line referring to the parameters determined from the spectra taken on April 3 (5) 2007. The bottom line, in italics, gives the average values and sample variance, except for $d_{\rm sec}$, where the error is the average of the two individual errors.

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