Table 3: We give the name, ID number, $\alpha $, $\delta $, V, V-I, and B-I for the stars with transit-like light curves. All information except the adapted name in the first column is from Stetson et al. (2003). The positions of the stars in the CMD is shown in Fig. 3 and the light curves can be seen in Fig. 4. As discussed in the text, the transits seen for T1-4, T6, and T9 are not likely to be due to transiting giant planets (they are marked by a * symbol).
Name ID $\alpha_{2000.0}$ $\delta_{2000.0}$ V V-I B-I
T1* 4891 19$^{\rm h}$20$^{\rm m}$43 $.\!\!^{\rm s}$37 +37$^\circ$47 ${}^{\prime}$31 $.\!\!^{\prime\prime}$5 17.675 0.928 1.818
T2* 6598 19$^{\rm h}$20$^{\rm m}$48 $.\!\!^{\rm s}$65 +37$^\circ$47 ${}^{\prime}$41 $.\!\!^{\prime\prime}$1 18.175 0.979 1.901
T3* 12616 19$^{\rm h}$21$^{\rm m}$07 $.\!\!^{\rm s}$28 +37$^\circ$47 ${}^{\prime}$39 $.\!\!^{\prime\prime}$9 17.718 0.915 1.809
T4* 9049 19$^{\rm h}$20$^{\rm m}$55 $.\!\!^{\rm s}$47 +37$^\circ$44 ${}^{\prime}$06 $.\!\!^{\prime\prime}$1 17.493 1.005 1.839
T5 3671 19$^{\rm h}$20$^{\rm m}$39 $.\!\!^{\rm s}$07 +37$^\circ$47 ${}^{\prime}$26 $.\!\!^{\prime\prime}$1 17.509 0.901 1.784
T6* 3567 19$^{\rm h}$20$^{\rm m}$38 $.\!\!^{\rm s}$63 +37$^\circ$45 ${}^{\prime}$33 $.\!\!^{\prime\prime}$3 17.635 0.919 1.811
T7 3723 19$^{\rm h}$20$^{\rm m}$39 $.\!\!^{\rm s}$25 +37$^\circ$45 ${}^{\prime}$39 $.\!\!^{\prime\prime}$3 18.002 0.954 1.827
T8 9020 19$^{\rm h}$20$^{\rm m}$55 $.\!\!^{\rm s}$40 +37$^\circ$47 ${}^{\prime}$23 $.\!\!^{\prime\prime}$4 17.029 0.848 1.670
T9* 12390 19$^{\rm h}$21$^{\rm m}$06 $.\!\!^{\rm s}$48 +37$^\circ$47 ${}^{\prime}$27 $.\!\!^{\prime\prime}$8 17.886 1.015 1.947
T10* 8279 19$^{\rm h}$20$^{\rm m}$53 $.\!\!^{\rm s}$42 +37$^\circ$48 ${}^{\prime}$14 $.\!\!^{\prime\prime}$6 18.907 1.079 2.092


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