Table 7: Long period variable stars that are likely members of NGC 6791 (ordered by increasing right ascension). Column 9 shows the membership probability (when available) or our photometric membership.
Star $\alpha_{2000}$ $\delta_{2000}$ V $\langle B-V\rangle$ $\langle V-I\rangle$ Ref. Ampl. Notes Distance

[mag] [mag] [mag] [mag] arcmin

02138_8 19.341864 37.749653 19.68 1.12 1.18 k 0.06 likely memb. 4.6

02444_8 19.342766 37.810604 18.34 0.93 1.00 k 0.02 member (78%) 4.4

00510_9 19.343704 37.796719 18.67 0.94 0.98 k 0.03 member (83%) 3.4

01610_9 19.344818 37.740486 19.09 1.01 1.05 k 0.02 likely memb. 3.0

V94 19.345139 37.743549 17.54 0.88 0.92 k 0.03 member (90%) 2.7

V95 19.345295 37.792412 19.16 1.03 1.10 k 0.07 member (93%) 2.3

V56(=V96) 19.345908 37.763525 17.01 0.95 0.97 k 0.04 member (98%) 1.6

04392_3 19.345982 37.870571 17.90 0.88 0.92 k 0.02 likely memb. 6.1

V75 19.346651 37.766308 17.38 0.94 0.98 s 0.01 likely memb. 1.0

04133_9 19.347109 37.777020 18.47 0.94 0.98 k 0.04 member (98%) 0.7

V76(=V85) 19.347192 37.764169 18.19 1.03 1.15 k 0.11 member (97%) 0.8

V86 19.347258 37.808815 19.44 1.06 1.14 k 0.03 member (83%) 2.3

V87 19.347996 37.749668 18.12 0.91 0.93 k 0.03 member (98%) 1.3

05740_9 19.348534 37.808022 17.96 0.93 k 0.03 member (95%) 2.2

06725_9 19.349329 37.724495 17.77 0.91 k 0.02 member (91%) 3.0

06796_9 19.349415 37.769268 18.46 0.92 1.04 k 0.03 member (92%) 1.0

V90 19.349686 37.746449 18.11 0.86 0.94 k 0.01 member (94%) 1.9

07680_9 19.350193 37.718224 18.32 0.89 0.97 k 0.03 member (98%) 3.5

V31 19.350683 37.785912 17.12 1.00 1.02 k 0.01 member (97%) 2.1

09376_9 19.351952 37.831886 18.21 1.00 1.02 k 0.01 member (92%) 4.6

09611_9 19.352139 37.773365 17.97 0.85 0.91 k 0.01 member (76%) 2.9

V58 19.354042 37.801240 17.52 0.89 0.94 k 0.05 member (87%) 4.6

02268_10 19.359475 37.731544 18.59 0.95 0.99 k 0.02 likely memb. 8.5

**Table 7:** Long period variable stars that are likely members of NGC 6791 (ordered by increasing right ascension). Column 9 shows the membership probability (when available) or our photometric membership.
Star	$\alpha_{2000}$	$\delta_{2000}$	V	$\langle B-V\rangle$	$\langle V-I\rangle$	Ref.	Ampl.	Notes	Distance
			[mag]	[mag]	[mag]		[mag]		arcmin
02138_8	19.341864	37.749653	19.68	1.12	1.18	k	0.06	likely memb.	4.6
02444_8	19.342766	37.810604	18.34	0.93	1.00	k	0.02	member (78%)	4.4
00510_9	19.343704	37.796719	18.67	0.94	0.98	k	0.03	member (83%)	3.4
01610_9	19.344818	37.740486	19.09	1.01	1.05	k	0.02	likely memb.	3.0
V94	19.345139	37.743549	17.54	0.88	0.92	k	0.03	member (90%)	2.7
V95	19.345295	37.792412	19.16	1.03	1.10	k	0.07	member (93%)	2.3
V56(=V96)	19.345908	37.763525	17.01	0.95	0.97	k	0.04	member (98%)	1.6
04392_3	19.345982	37.870571	17.90	0.88	0.92	k	0.02	likely memb.	6.1
V75	19.346651	37.766308	17.38	0.94	0.98	s	0.01	likely memb.	1.0
04133_9	19.347109	37.777020	18.47	0.94	0.98	k	0.04	member (98%)	0.7
V76(=V85)	19.347192	37.764169	18.19	1.03	1.15	k	0.11	member (97%)	0.8
V86	19.347258	37.808815	19.44	1.06	1.14	k	0.03	member (83%)	2.3
V87	19.347996	37.749668	18.12	0.91	0.93	k	0.03	member (98%)	1.3
05740_9	19.348534	37.808022	17.96	0.93		k	0.03	member (95%)	2.2
06725_9	19.349329	37.724495	17.77	0.91		k	0.02	member (91%)	3.0
06796_9	19.349415	37.769268	18.46	0.92	1.04	k	0.03	member (92%)	1.0
V90	19.349686	37.746449	18.11	0.86	0.94	k	0.01	member (94%)	1.9
07680_9	19.350193	37.718224	18.32	0.89	0.97	k	0.03	member (98%)	3.5
V31	19.350683	37.785912	17.12	1.00	1.02	k	0.01	member (97%)	2.1
09376_9	19.351952	37.831886	18.21	1.00	1.02	k	0.01	member (92%)	4.6
09611_9	19.352139	37.773365	17.97	0.85	0.91	k	0.01	member (76%)	2.9
V58	19.354042	37.801240	17.52	0.89	0.94	k	0.05	member (87%)	4.6
02268_10	19.359475	37.731544	18.59	0.95	0.99	k	0.02	likely memb.	8.5

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