Table 5: Eclipsing variables with well defined light curves. EA stands for a $\beta $ Per system, EB for a $\beta $ Lyr one. V is the brightness at maximum and T0 is the time of the primary minimum. Also B4, V60 and 02461_8, whose parameters are reported in the Appendix, are possible cluster members. The last column shows the Cudworth membership probability (when available).
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]  

V119

EB 19.351961 37.916328 18.15 1.13 1.33 k 59.879 0.30197 0.15 member?
V29 EB 19.354796 37.751386 20.00 1.23 1.61 k 69.012 0.43662 0.22 likely memb.
01558_5 EB 19.372697 37.953469 19.15       69.028 0.52910 0.28 likely non-memb.
01393_1 EA 19.329588 37.970392 21.23       59.326 0.58998 0.56 likely non-memb.
00331_3 EB 19.352367 37.864391 19.73 1.20 1.36 k 68.815 0.7347 0.13 member?
V11 EA 19.342575 37.804802 19.38 0.96 1.22 k 67.875 0.8833 0.48 member?
05736_9 EA 19.348484 37.721855 20.20 1.21   k 68.333 1.210 0.29 likely memb.
V12 EB 19.345259 37.849083 17.52 0.96   k 64.103 1.524 0.06 member (96%)
00645_10 EA 19.354692 37.710104 20.60 1.33 1.46 k 60.893 1.451 0.20 likely memb.
V9 EB 19.346634 37.777035 17.15 1.23 1.38 k 63.873: 3.2 >0.2 member (82%)
V107 EA 19.355068 37.761553 17.97 0.93 1.00 k 64.433 3.27 0.24 member?
V109 EA 19.342716 37.793961 20.73 1.46 1.60 k 69.021 3.70 0.86 member?


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