Stars with significant Stanton magnitude adjustments typically are 1) faint, 2) have a high color index and 3) were measured by photography, not by photoelectric means.
Webda_id | X | Y | RA_J2000 | Dec_J2000 | Photometry_type | Johnson_V | Johnson_V_se | Johnson_CI | m_V | m_V_se | m_V_Diff |
0014 | -2.93 | 5.8 | 4 45 48.1 | +19 14 12.8 | Turner photographic | 11.43 | 0.01 | 0.51 | 11.83 | 0.27 | 0.40 |
0038 | -0.43 | -0.65 | 4 46 05.4 | +19 03 32.6 | Turner photographic | 12.28 | 0.01 | 0.61 | 12.76 | 0.27 | 0.48 |
0210 | -1.29 | 0.27 | 4 45 59.4 | +19 05 05.0 | Turner photographic | 12.45 | 0.01 | 0.61 | 12.93 | 0.27 | 0.48 |
0008 | -5.33 | 0.75 | 4 45 31.1 | +19 05 52.9 | Turner photographic | 12.52 | 0.01 | 0.64 | 13.02 | 0.27 | 0.50 |
0032 | 3.79 | -2.87 | 4 46 34.7 | +18 59 49.5 | Turner photographic | 12.89 | 0.01 | 0.69 | 13.43 | 0.27 | 0.54 |
0177 | 3.67 | -3.43 | 4 46 34.0 | +18 58 54.6 | Turner photographic | 12.88 | 0.01 | 0.70 | 13.43 | 0.27 | 0.55 |
0047 | -2.41 | 1.7 | 4 45 51.6 | +19 07 25.5 | Turner photographic | 12.4 | 0.01 | 0.75 | 12.99 | 0.27 | 0.59 |
0007 | -3.57 | -0.16 | 4 45 43.4 | +19 04 20.1 | Turner photographic | 12.41 | 0.01 | 0.80 | 13.04 | 0.27 | 0.63 |
0036 | -0.29 | -3.97 | 4 46 06.2 | +18 58 02.5 | Turner photographic | 12.62 | 0.01 | 0.96 | 13.37 | 0.27 | 0.75 |
0092 | 3.18 | 4.25 | 4 46 30.8 | +19 11 36.8 | Turner photographic | 12.42 | 0.01 | 1.22 | 13.38 | 0.27 | 0.96 |
0006 | -5.05 | -2.75 | 4 45 32.9 | +19 00 04.8 | Turner photographic | 12.18 | 0.01 | 1.44 | 13.31 | 0.27 | 1.13 |