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%)

**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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