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Table 6:

Contact binaries that may have a low mass-ratio - the lightcurves have shape but not periods suggesting low mass-ratios.

ID
Subset Right ascension Declination Calibrated magnitudes Period Type
    (J2000.0) (J2000.0) R B-R R-I (days)  
V-9 1A 16:20:50.50 -53:24:40.1987 19.05 1.33 2.28 0.5106 EW
V-92 1C 16:20:48.80 -53:19:04.3178 19.24 2.23 0.94 0.4076 EW
V-115 1E 16:20:53.66 -53:17:11.7310 19.14 2.55 0.67 0.5553 EW
V-467 3E 16:18:59.97 -53:16:25.5253 19.25 2.83 0.52 0.4095 EW
V-482 3E 16:18:56.66 -53:15:05.8831 17.15 1.95 0.53 0.4277 EW
V-493 3F 16:18:36.50 -53:17:09.0202 16.23 1.87 1.75 0.2725 EW
V-523 3F 16:18:30.89 -53:15:11.5286 16.49 2.38   0.9037 EW
V-984 6A 16:18:47.74 -53:41:03.6335 17.74 2.84 0.61 0.6118 EW
V-1091 6F 16:18:38.73 -53:31:56.7975 17.24 2.20 1.08 0.5765 EW
V-1232 7E 16:19:39.57 -53:32:12.9626 18.13 1.65 0.90 0.4570 EW
V-1272 7G 16:19:38.92 -53:27:04.6993 18.47 2.33 0.82 0.2853 EW
V-1312 8A 16:20:38.43 -53:38:56.5849 17.00 1.24 4.28 0.5868 EW
V-1354 8C 16:20:48.55 -53:36:20.9116 18.64 1.86 0.80 0.4498 EW
V-1422 8F 16:20:09.11 -53:32:17.6392 18.48 1.92 0.75 0.4381 EW


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