Table 6: Rotational variables belonging to the cluster. V is the mean brightness value. T0 indicates the time of the maximum brightness. The last column shows the membership probability (when available) or our photometric membership. The two uncertain cases (V41 and V14) are also listed (see text).
Star Type $\alpha_{2000}$ $\delta_{2000}$ V $\langle B-V\rangle$ $\langle V-I\rangle$ Ref. T0 Period Ampl. Notes
        [mag] [mag] [mag]   [HJD-2 452 400] [d] [mag]  
04803_9 RO1 19.347698 37.796043 21.81 1.33 1.84 s 61.799 1.1034 0.17 member (B06)
V82 RO1 19.344366 37.793381 19.01 1.00 1.02 k 56.481 1.1568 0.04 likely memb.
06553_9 RO1 19.349134 37.672577 19.26 1.04 1.13 s 61.421 1.3485 0.08 likely memb.
01724_9 RO1 19.344957 37.785362 20.73 1.29 1.69 s 64.410 1.6130 0.17 likely memb.
V38 RO1 19.351021 37.768288 18.82 0.96   k 55.630 1.96 0.13 member (92%)
03079_9 RO1 19.346190 37.754753 19.23 1.14 1.26 k 66.630 2.640 0.07 member (93%)
V14 RO1 19.347687 37.756874 18.58 0.93 1.05 k 55.933 5.45 0.05 non-member (0%)
V48 RO1 19.352076 37.718506 17.51 0.88   k 65.223 5.65 0.09 member (96%)
V17 RO1 19.344135 37.817928 17.92 1.20 1.28 k 63.211 6.523 0.04 member (88%)
V51 RO1 19.353382 37.748795 19.94 1.22 1.21 k 63.624 6.72 0.09 likely memb.
V52 RO1 19.355795 37.771935 17.49 0.88 0.88 k 64.345 7.06 0.03 likely memb.
V53 RO1 19.350233 37.743187 18.72 0.89 0.93 k 69.294 7.47 0.04 member (86%)
00436_3 RO2 19.352205 37.878635 18.92 0.92 1.08 k 60.018 0.26601 0.04 likely memb.
07483_9 RO2 19.349997 37.746311 21.28 1.32 1.70 s 60.465 0.4375 0.17 likely memb.
V41 RO2 19.347492 37.806892 19.09       60.000 0.4798 0.07 member (77%)
V42 RO2 19.350058 37.714867 19.51 1.05 1.16 k 60.323 0.5068 0.10 member (92%)
V16 RO2 19.352108 37.802662 17.79 0.93 1.01 k 67.713 2.182 0.03 member (96%)


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