Table 4: The variables in the NOT01 field. The first column contains the variable name, where the new variables are printed with italics ( V79-V100). Columns 2-4 contain ID, right ascension, and declination from Stetson et al. (2003). Columns 5 and 6 are the periods and amplitudes (in the V filter) we have determined. The last column gives the variable star type. The positions of the variables in the colour-magnitude diagram are given in Figs. 3 and 5 while the phased light curves of some of the stars are shown in Figs. 6, 7, and 8.
Name ID $\alpha_{2000.0}$ $\delta_{2000.0}$ P [days] A [mag] Var. type
V1 6271 19$^{\rm h}$20$^{\rm m}$47 $.\!\!^{\rm s}$61 +37$^\circ$44 ${}^{\prime}$32 $.\!\!^{\prime\prime}$0 0.2676766 0.194 EB, close
V4 8576 19$^{\rm h}$20$^{\rm m}$54 $.\!\!^{\rm s}$22 +37$^\circ$48 ${}^{\prime}$23 $.\!\!^{\prime\prime}$8 0.325667 0.046 EB, close
V5 5883 19$^{\rm h}$20$^{\rm m}$46 $.\!\!^{\rm s}$53 +37$^\circ$48 ${}^{\prime}$47 $.\!\!^{\prime\prime}$9 0.312666 0.017 EB, close
V6 11376 19$^{\rm h}$21$^{\rm m}$02 $.\!\!^{\rm s}$72 +37$^\circ$48 ${}^{\prime}$49 $.\!\!^{\prime\prime}$1 0.279062 0.042 EB, close
V9 6371 19$^{\rm h}$20$^{\rm m}$47 $.\!\!^{\rm s}$88 +37$^\circ$46 ${}^{\prime}$37 $.\!\!^{\prime\prime}$4 3.19174 0.040a EB, close
V16 12695 19$^{\rm h}$21$^{\rm m}$07 $.\!\!^{\rm s}$59 +37$^\circ$48 ${}^{\prime}$09 $.\!\!^{\prime\prime}$6 4.53 0.026 EB, close
V31 11307 19$^{\rm h}$21$^{\rm m}$02 $.\!\!^{\rm s}$47 +37$^\circ$47 ${}^{\prime}$09 $.\!\!^{\prime\prime}$3 3.34154 0.015 EB, close
V33 3886 19$^{\rm h}$20$^{\rm m}$39 $.\!\!^{\rm s}$81 +37$^\circ$43 ${}^{\prime}$54 $.\!\!^{\prime\prime}$4 2.35944 0.040 EB, close
V38 11652 19$^{\rm h}$21$^{\rm m}$03 $.\!\!^{\rm s}$69 +37$^\circ$46 ${}^{\prime}$05 $.\!\!^{\prime\prime}$9 3.845 0.023 EB, close
V20 8600 19$^{\rm h}$20$^{\rm m}$54 $.\!\!^{\rm s}$30 +37$^\circ$45 ${}^{\prime}$34 $.\!\!^{\prime\prime}$7 14.4698 0.3a EB, detached
V60 10746 19$^{\rm h}$21$^{\rm m}$00 $.\!\!^{\rm s}$70 +37$^\circ$45 ${}^{\prime}$45 $.\!\!^{\prime\prime}$1 7.510/7.1b 0.4/0.015b EB, detached
V79 8943 19$^{\rm h}$20$^{\rm m}$55 $.\!\!^{\rm s}$21 +37$^\circ$46 ${}^{\prime}$39 $.\!\!^{\prime\prime}$7 $\sim$9.0038 0.15a EB, detached
V80c 12390 19$^{\rm h}$21$^{\rm m}$06 $.\!\!^{\rm s}$48 +37$^\circ$47 ${}^{\prime}$27 $.\!\!^{\prime\prime}$8 4.447 0.014 EB?
V14 7637 19$^{\rm h}$20$^{\rm m}$51 $.\!\!^{\rm s}$67 +37$^\circ$45 ${}^{\prime}$24 $.\!\!^{\prime\prime}$8 5.4-5.8 0.028 Periodic Var.
V17 3626 19$^{\rm h}$20$^{\rm m}$38 $.\!\!^{\rm s}$88 +37$^\circ$49 ${}^{\prime}$04 $.\!\!^{\prime\prime}$6 6.42566 0.036 Periodic Var.
V41 7397 19$^{\rm h}$20$^{\rm m}$50 $.\!\!^{\rm s}$97 +37$^\circ$48 ${}^{\prime}$24 $.\!\!^{\prime\prime}$8 0.4807278 0.039 Periodic Var.
V53 10798 19$^{\rm h}$21$^{\rm m}$00 $.\!\!^{\rm s}$84 +37$^\circ$44 ${}^{\prime}$35 $.\!\!^{\prime\prime}$4 7.815 0.039 Periodic Var.
V81 3268 19$^{\rm h}$20$^{\rm m}$49 $.\!\!^{\rm s}$65 +37$^\circ$48 ${}^{\prime}$08 $.\!\!^{\prime\prime}$7 7.58 0.008 Periodic Var.
V82 3857 19$^{\rm h}$20$^{\rm m}$39 $.\!\!^{\rm s}$71 +37$^\circ$47 ${}^{\prime}$36 $.\!\!^{\prime\prime}$1 7.58886 0.010 Periodic Var.
V83 5848 19$^{\rm h}$20$^{\rm m}$46 $.\!\!^{\rm s}$40 +37$^\circ$44 ${}^{\prime}$14 $.\!\!^{\prime\prime}$1 7.014 0.037 Periodic Var.
V84 6305 19$^{\rm h}$20$^{\rm m}$47 $.\!\!^{\rm s}$71 +37$^\circ$44 ${}^{\prime}$58 $.\!\!^{\prime\prime}$2 1.6333 0.03 Periodic Var.
V85 7011 19$^{\rm h}$20$^{\rm m}$49 $.\!\!^{\rm s}$86 +37$^\circ$45 ${}^{\prime}$50 $.\!\!^{\prime\prime}$9 4.100 0.007 Periodic Var., EB?
V86 7099 19$^{\rm h}$20$^{\rm m}$50 $.\!\!^{\rm s}$13 +37$^\circ$48 ${}^{\prime}$31 $.\!\!^{\prime\prime}$7 7.39 0.011 Periodic Var.
V87 8033 19$^{\rm h}$20$^{\rm m}$52 $.\!\!^{\rm s}$78 +37$^\circ$44 ${}^{\prime}$58 $.\!\!^{\prime\prime}$8 6.971 0.006 Periodic Var.
V88 8088 19$^{\rm h}$20$^{\rm m}$52 $.\!\!^{\rm s}$91 +37$^\circ$46 ${}^{\prime}$36 $.\!\!^{\prime\prime}$9 6.91 0.008 Periodic Var.
V89 9432 19$^{\rm h}$20$^{\rm m}$56 $.\!\!^{\rm s}$64 +37$^\circ$46 ${}^{\prime}$36 $.\!\!^{\prime\prime}$2 5.7617 0.028 Periodic Var.
V90 10169 19$^{\rm h}$20$^{\rm m}$58 $.\!\!^{\rm s}$86 +37$^\circ$44 ${}^{\prime}$47 $.\!\!^{\prime\prime}$2 5.71 0.008 Periodic Var.
V91 10699 19$^{\rm h}$21$^{\rm m}$00 $.\!\!^{\rm s}$54 +37$^\circ$48 ${}^{\prime}$40 $.\!\!^{\prime\prime}$7 5.13 0.011 Periodic Var.
V92 11380 19$^{\rm h}$21$^{\rm m}$02 $.\!\!^{\rm s}$73 +37$^\circ$46 ${}^{\prime}$00 $.\!\!^{\prime\prime}$8 7.24 0.008 Periodic Var.
V93 12049 19$^{\rm h}$21$^{\rm m}$05 $.\!\!^{\rm s}$23 +37$^\circ$47 ${}^{\prime}$08 $.\!\!^{\prime\prime}$5 0.94928 0.007 Periodic Var.
B7 12652 19$^{\rm h}$21$^{\rm m}$07 $.\!\!^{\rm s}$40 +37$^\circ$47 ${}^{\prime}$56 $.\!\!^{\prime\prime}$5 $\sim$13.3 0.15 Long period
V62 11475 19$^{\rm h}$21$^{\rm m}$03 $.\!\!^{\rm s}$06 +37$^\circ$43 ${}^{\prime}$51 $.\!\!^{\prime\prime}$8 $\sim$17 0.027 Long period
V65 7920 19$^{\rm h}$20$^{\rm m}$52 $.\!\!^{\rm s}$47 +37$^\circ$47 ${}^{\prime}$30 $.\!\!^{\prime\prime}$5 8.613 0.008 Long period
V67 11645 19$^{\rm h}$21$^{\rm m}$03 $.\!\!^{\rm s}$67 +37$^\circ$48 ${}^{\prime}$03 $.\!\!^{\prime\prime}$7 $\sim$10 0.05 Long period
V73 8108 19$^{\rm h}$20$^{\rm m}$52 $.\!\!^{\rm s}$97 +37$^\circ$46 ${}^{\prime}$52 $.\!\!^{\prime\prime}$5 $\sim$20.9 0.02 Long Period
V94 4640 19$^{\rm h}$20$^{\rm m}$42 $.\!\!^{\rm s}$50 +37$^\circ$44 ${}^{\prime}$36 $.\!\!^{\prime\prime}$9 $\sim$15.57 0.01 Long period
V95 4805 19$^{\rm h}$20$^{\rm m}$43 $.\!\!^{\rm s}$05 +37$^\circ$47 ${}^{\prime}$32 $.\!\!^{\prime\prime}$5 9.477 0.012 Long period
V96 5485 19$^{\rm h}$20$^{\rm m}$45 $.\!\!^{\rm s}$26 +37$^\circ$45 ${}^{\prime}$48 $.\!\!^{\prime\prime}$8 9.307 0.012 Long Period
V97 6777 19$^{\rm h}$20$^{\rm m}$49 $.\!\!^{\rm s}$17 +37$^\circ$49 ${}^{\prime}$14 $.\!\!^{\prime\prime}$8 9.563 0.013 Long period
V98 9353 19$^{\rm h}$20$^{\rm m}$56 $.\!\!^{\rm s}$42 +37$^\circ$45 ${}^{\prime}$38 $.\!\!^{\prime\prime}$4 $\sim$8.99 0.01 Long period
V99 9568 19$^{\rm h}$20$^{\rm m}$57 $.\!\!^{\rm s}$06 +37$^\circ$48 ${}^{\prime}$12 $.\!\!^{\prime\prime}$2 $\sim$10 0.003 Long period
V100 11111 19$^{\rm h}$21$^{\rm m}$01 $.\!\!^{\rm s}$81 +37$^\circ$45 ${}^{\prime}$42 $.\!\!^{\prime\prime}$0 12.5215 0.01 Long period
a For the eclipsing binaries V9, V20, and V79 the depth of the primary eclipse in the V filter is given.
b V60 is variable with a low amplitude and a period of $P\sim7.1$ days while the period estimated from the
secondary and primary eclipses is $7.510\pm0.005$ days. The primary eclipse depth is 0.4 mag in V.
c V80 was detected in our search for transit-like events and is also given the name T9 (cf Fig. 4).
Furthermore, V80 is variable with a low amplitude.


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