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Table 1

Properties of member and field RRLs with previously uncertain status.

ID RA Dec J KS Pa Type db Memb.
(J2000) (J2000) (mag) (mag) (days) (arcmin) (%) (%) status

V19 13:27:30.12 47:28:05.74 13.852 13.631 0.299551 RRc 7.27 100 100 m
V21 13:26:11.15 47:25:59.30 13.538 13.362 0.380812 RRc 6.71 100 99 m
V52 13:26:35.15 47:28:04.33 12.831 12.634 0.660386 RRab 2.16 53 45 m
V56 13:25:55.44 47:37:44.44 13.612 13.301 0.568023 RRab 12.53 98 100 m
V68 13:26:12.79 47:19:36.12 13.168 12.897 0.534696 RRc/ACEP? 10.87 100 100 m?
V80c 13:28:54.96 47:30:16.42 13.568 13.360 0.37718 RRc 21.62 out out m
V84 13:24:47.47 47:49:56.18 13.031 12.712 0.579873 RRab/ACEP? 29.24 0 out m?
V143 13:26:42.59 47:27:28.98 12.783 12.510 0.820734 RRab 1.51 90 99 m
V151 13:28:25.31 47:16:00.01 13.455 13.211 0.407756 RRc 20.94 out out m
V168 13:25:52.74 47:32:03.19 14.164 13.916 0.321299 RRc 9.78 0 0 f
V172d 13:27:55.04 47:04:38.50 13.220 12.927 0.7380 RRab 26.72 out out m
V173 13:29:43.13 47:16:53.80 13.624 13.360 0.3590 RRc 32.05 out out m
V177e 13:29:04.15 47:36:21.42 13.690 13.479 0.31469 RRc 24.31 out out m
V180 13:28:15.22 47:40:32.02 13.201 12.839 0.39006 W UMa 18.93 0 out f
V181 13:30:00.35 47:48:44.96 14.823 14.535 0.5884 RRab 38.17 out out f
V183 13:29:39.50 47:30:18.36 14.690 14.449 0.29603 RRc 29.13 out out f
V268 13:26:35.11 47:26:11.15 13.156 12.827 0.812922 RRab 3.30 70 99 m
V283 13:27:36.53 47:46:40.44 16.947 16.682 0.517233 RRab 19.73 out out f
V411f 13:26:40.77 47:28:17.00 13.123 12.796 0.8449 RRab 1.20 100 99 m
V433g 13:29:03.59 47:48:58.25 14.737 14.151 0.6681 ? 30.58 out out f
ID91 13:26:14.03 47:53:08.20 15.782 15.430 0.637238 RRab? 25.00 out out f
ID99 13:24:40.44 47:45:22.54 15.777 15.275 0.670361 ? 27.07 out out f

Notes.

(a)

Periods are from Kaluzny et al. (2004), except for V80, V172, V173, V177, V180, V181, V183, and V411, which were derived by us.

(b)

Distance to the cluster center was calculated using the center of ω Cen as reported by SIMBAD: RA = 13:26:47.28, Dec = 47:28:46.1, both in J2000.

(f)

V411 has the same coordinates and periods as first reported by Navarrete et al. (2013). Mean magnitudes differ from that paper because the values presented in this paper, but not in Navarrete et al. (2013), are intensity-averaged mean magnitudes.

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