Table 7: Long period variable stars that are likely members of NGC 6791 (ordered by increasing right ascension). Column 9 shows the membership probability (when available) or our photometric membership.

Star
$\alpha_{2000}$ $\delta_{2000}$ V $\langle B-V\rangle$ $\langle V-I\rangle$ Ref. Ampl. Notes Distance
      [mag] [mag] [mag]   [mag]   arcmin
02138_8 19.341864 37.749653 19.68 1.12 1.18 k 0.06 likely memb. 4.6
02444_8 19.342766 37.810604 18.34 0.93 1.00 k 0.02 member (78%) 4.4
00510_9 19.343704 37.796719 18.67 0.94 0.98 k 0.03 member (83%) 3.4
01610_9 19.344818 37.740486 19.09 1.01 1.05 k 0.02 likely memb. 3.0
V94 19.345139 37.743549 17.54 0.88 0.92 k 0.03 member (90%) 2.7
V95 19.345295 37.792412 19.16 1.03 1.10 k 0.07 member (93%) 2.3
V56(=V96) 19.345908 37.763525 17.01 0.95 0.97 k 0.04 member (98%) 1.6
04392_3 19.345982 37.870571 17.90 0.88 0.92 k 0.02 likely memb. 6.1
V75 19.346651 37.766308 17.38 0.94 0.98 s 0.01 likely memb. 1.0
04133_9 19.347109 37.777020 18.47 0.94 0.98 k 0.04 member (98%) 0.7
V76(=V85) 19.347192 37.764169 18.19 1.03 1.15 k 0.11 member (97%) 0.8
V86 19.347258 37.808815 19.44 1.06 1.14 k 0.03 member (83%) 2.3
V87 19.347996 37.749668 18.12 0.91 0.93 k 0.03 member (98%) 1.3
05740_9 19.348534 37.808022 17.96 0.93   k 0.03 member (95%) 2.2
06725_9 19.349329 37.724495 17.77 0.91   k 0.02 member (91%) 3.0
06796_9 19.349415 37.769268 18.46 0.92 1.04 k 0.03 member (92%) 1.0
V90 19.349686 37.746449 18.11 0.86 0.94 k 0.01 member (94%) 1.9
07680_9 19.350193 37.718224 18.32 0.89 0.97 k 0.03 member (98%) 3.5
V31 19.350683 37.785912 17.12 1.00 1.02 k 0.01 member (97%) 2.1
09376_9 19.351952 37.831886 18.21 1.00 1.02 k 0.01 member (92%) 4.6
09611_9 19.352139 37.773365 17.97 0.85 0.91 k 0.01 member (76%) 2.9
V58 19.354042 37.801240 17.52 0.89 0.94 k 0.05 member (87%) 4.6
02268_10 19.359475 37.731544 18.59 0.95 0.99 k 0.02 likely memb. 8.5


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