NGC 4414 Table 11a: Secondary Standards WF-2 ID RA(2000) Dec(2000) V sigmaV I sigmaI 5189 12:26:23.37 31:13:23.1 20.95 0.01 20.33 0.01 5940 12:26:21.93 31:13:27.2 22.04 0.01 21.07 0.01 5174 12:26:23.15 31:12:47.5 23.54 0.01 22.55 0.01 6006 12:26:21.60 31:13:35.4 23.44 0.01 22.54 0.01 6031 12:26:21.27 31:13:13.0 24.26 0.01 22.48 0.01 2764 12:26:24.66 31:12:54.1 23.99 0.02 23.29 0.04 5502 12:26:23.18 31:13:40.7 24.08 0.01 23.17 0.03 4607 12:26:23.83 31:13:28.2 24.04 0.03 23.61 0.05 4136 12:26:24.11 31:13:20.9 24.08 0.03 23.76 0.05 5958 12:26:21.76 31:13:14.0 24.60 0.02 24.45 0.05 2977 12:26:24.52 31:12:47.0 24.17 0.03 23.65 0.05 3233 12:26:24.48 31:13:01.5 24.25 0.03 24.28 0.07 5197 12:26:23.19 31:12:56.9 24.35 0.02 23.75 0.05 4595 12:26:23.76 31:13:15.1 24.80 0.03 24.50 0.07 4773 12:26:23.59 31:13:11.1 24.63 0.04 23.78 0.06 5843 12:26:22.49 31:13:38.1 25.18 0.04 24.79 0.06 1890 12:26:25.01 31:12:43.1 24.96 0.04 24.58 0.07 1666 12:26:25.06 31:12:37.0 24.92 0.04 24.64 0.07 4586 12:26:23.80 31:13:20.8 24.97 0.04 24.61 0.07 5876 12:26:22.44 31:13:47.1 25.17 0.04 24.92 0.06 5740 12:26:22.48 31:13:04.5 25.65 0.04 24.85 0.06 3837 12:26:24.10 31:12:51.0 23.40 0.01 21.31 0.04 Magnitudes of secondary standards are based on ALLFRAME photometry. Errors quoted do not include uncertainty in the photometric calibration. Table 11b: Secondary Standards WF-3 ID RA(2000) Dec(2000) V sigmaV I sigmaI 3953 12:26:24.22 31:14:25.5 20.18 0.00 19.41 0.00 4508 12:26:25.44 31:14:23.0 22.95 0.01 21.64 0.01 1560 12:26:22.82 31:14:04.2 23.18 0.01 22.63 0.03 1900 12:26:23.67 31:14:06.1 22.82 0.01 22.41 0.01 3724 12:26:23.77 31:14:23.8 22.88 0.01 22.67 0.03 4095 12:26:25.78 31:14:25.3 22.80 0.01 21.89 0.02 5585 12:26:22.05 31:14:48.1 23.43 0.01 23.38 0.02 2579 12:26:23.19 31:14:13.5 23.30 0.01 22.63 0.01 1742 12:26:21.56 31:14:07.1 23.32 0.01 22.44 0.02 1300 12:26:24.31 31:14:00.0 23.66 0.02 22.90 0.03 3113 12:26:24.44 31:14:17.6 23.70 0.02 22.82 0.03 4431 12:26:24.25 31:14:30.4 23.60 0.01 23.72 0.05 4022 12:26:25.24 31:14:25.0 23.81 0.02 22.97 0.04 4860 12:26:22.57 31:14:36.9 24.27 0.01 23.32 0.02 5110 12:26:23.68 31:14:38.5 24.11 0.01 21.49 0.01 5731 12:26:21.37 31:14:52.2 24.21 0.01 24.11 0.04 4821 12:26:26.15 31:14:32.5 23.75 0.01 23.53 0.05 212 12:26:26.15 31:14:32.5 23.70 0.02 22.59 0.03 6063 12:26:22.71 31:14:58.6 24.36 0.01 24.40 0.05 1361 12:26:24.66 31:14:00.2 23.99 0.02 22.56 0.04 565 12:26:23.92 31:13:53.7 24.55 0.03 23.49 0.04 5767 12:26:26.04 31:14:47.9 24.60 0.03 24.40 0.05 5583 12:26:25.80 31:14:43.8 24.85 0.03 23.99 0.05 5912 12:26:25.78 31:14:52.1 24.90 0.02 25.15 0.08 3995 12:26:24.58 31:14:25.5 23.52 0.03 23.37 0.05 2324 12:26:24.59 31:14:09.4 24.47 0.03 23.21 0.04 6131 12:26:25.67 31:14:56.6 25.03 0.03 24.37 0.05 6079 12:26:23.44 31:14:58.2 24.80 0.03 24.18 0.05 4488 12:26:23.87 31:14:31.6 24.86 0.03 24.93 0.07 5247 12:26:26.31 31:14:37.4 24.80 0.03 24.78 0.07 4679 12:26:24.50 31:14:32.8 24.86 0.03 24.97 0.08 4858 12:26:23.21 31:14:36.2 24.99 0.03 24.63 0.06 4477 12:26:25.20 31:14:29.9 24.80 0.03 23.89 0.06 2853 12:26:23.95 31:14:15.5 24.98 0.03 24.41 0.06 5759 12:26:21.96 31:14:52.2 25.31 0.03 25.25 0.09 6060 12:26:24.46 31:14:56.6 25.25 0.03 24.85 0.08 Magnitudes of secondary standards are based on ALLFRAME photometry. Errors quoted do not include uncertainty in the photometric calibration Table 11c: Secondary Standards WF-4 ID RA(2000) Dec(2000) V sigmaV I sigmaI 4461 12:26:28.17 31:14:17.4 23.49 0.01 22.61 0.01 3383 12:26:27.71 31:14:17.5 22.74 0.01 22.46 0.02 6234 12:26:29.82 31:14:12.1 23.47 0.01 23.60 0.04 1946 12:26:27.26 31:14:24.0 23.92 0.02 23.17 0.03 1155 12:26:27.01 31:14:30.1 23.83 0.02 23.66 0.04 6238 12:26:29.74 31:14:01.4 24.00 0.01 23.03 0.03 2262 12:26:27.40 31:14:27.5 23.54 0.01 22.78 0.04 6575 12:26:31.23 31:14:11.3 25.39 0.03 23.26 0.02 6202 12:26:29.67 31:14:01.0 24.61 0.03 24.42 0.06 1012 12:26:27.17 31:14:56.8 24.81 0.03 24.89 0.06 6362 12:26:30.26 31:14:23.9 25.14 0.03 25.21 0.08 5799 12:26:29.28 31:14:23.7 25.13 0.04 23.39 0.03 3390 12:26:27.81 31:14:29.8 24.83 0.03 24.26 0.06 Magnitudes of secondary standards are based on ALLFRAME photometry. Errors quoted do not include uncertainty in the photometric calibration.