Table 2: Photometric distances and its dispersion (all in pc) as derived from data in Table 1.
STAR D(V-R) $\sigma_{D(V-R)}$ D(V-I) $\sigma_{D(V-I)}$ D $\sigma_{D}$*
WT98 22 3 27 1 26 1
WT110 87 9 90 3 89 3
WT121 32 6 35 3 34 3
WT133 28 2 31 1 31 1
WT135 38 6 47 2 46 2
WT143 388 70 441 37 429 33
WT178 14 1 17 1 17 1
WT233b 227 30 275 11 269 10
WT233f 2140 662 1340 287 1467 263
WT1289 44 8 46 3 46 3
WT1353 37 2 41 1 40 1
WT1356 24 4 29 2 28 2
WT1463 45 9 50 3 50 2
WT1481 164 12 165 3 165 3
WT1515 23 6 27 2 27 2
WT1530 33 8 43 3 41 3
WT1542 20 4 25 2 24 2
WT1759 2459 342 2414 271 2432 212
WT1760b 26 4 33 2 32 1
WT2390 45 6 51 3 50 3
WT2431 58 6 77 2 75 2
WT2451 34 7 36 2 36 2
WT2461 42 5 44 3 44 2
WT2462 21 2 24 1 24 1
WT2463 100 13 116 8 117 7
WT2475 23 1 28 1 27 1
LTT1323 19 1 20 1 20 1
LTT1588 241 11 171 3 175 3
LTT1697 44 1 57 1 50 1
LTT1848 31 3 39 2 38 1
LTT2202 96 17 120 5 118 5
LTT2631 14 1 15 1 15 1
LTT2856 21 1 25 1 24 1
LTT3461 29 1 34 1 33 1
LTT3496 3582 202 3416 166 3483 128
LTT3553 20 1 21 1 21 1
LTT3616 16 1 16 1 16 1
LTT3632 22 2 23 1 23 1
LTT3725 53 3 54 6 53 2
LTT3742 17 1 19 1 19 1
LTT3790 16 1 19 1 18 1
LTT3791 12 1 15 1 14 1
LTT3802 18 1 24 1 21 1
LTT3861 28 1 35 1 33 1
* Note that this error does not include the possible metallicity effects discussed in the text,
  which could increase the error of the derived distance up to 14%.


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