| MJD | V | * | Image | B | * | Image | R | * | Images | I | * | Images | 
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 56140.40 | 17.24± 0.05 | - |  | -- | - | - | 16.69± 0.07 | - |  | -- | - | - | 
| 56599.22 | 17.24± 0.06 | - |  | 18.14± 0.05 | - |  | 16.70± 0.05 | - |  | -- | - | - | 
| 57035.14 | 17.26± 0.04 | - |  | 18.21± 0.06 | - |  | 16.75± 0.05 | - |  | -- | - | - | 
| 57310.16 | 17.29± 0.05 | - |  | 18.18± 0.05 | - |  | 16.79± 0.05 | - |  | -- | - | - | 
| 57406.10 | 17.08± 0.05 | - |  | 17.90± 0.07 | - |  | 16.63± 0.05 | - |  | 16.25± 0.07 | - |  | 
| 57634.41 | 17.12± 0.06 | - |  | 17.97± 0.08 | - |  | 16.65± 0.08 | - |  | -- | - | - | 
| 57638.40 | 17.22± 0.05 | A |   | 18.10± 0.04 | - |  | 16.73± 0.03 | - |  | 16.27± 0.08 | A |   | 
| 57988.43 | 17.14± 0.06 | T |  | -- | - | - | -- | - | - | -- | - | - | 
| 58043.15 | 17.13± 0.04 | A |   | 18.06± 0.05 | A |   | 16.56± 0.06 | A |   | 16.18± 0.09 | - |  | 
| 58073.22 | 17.17± 0.04 | - |  | 18.14± 0.05 | - |  | -- | - | - | -- | - | - | 
| 58108.13 | 17.18± 0.05 | A |   | 18.09± 0.05 | A |   | -- | - | - | 16.21± 0.08 | A |   | 
| 58316.35 | 17.23± 0.04 | - |  | 18.13± 0.04 | - |  | -- | - | - | -- | - | - | 
| 58339.40 | 17.16± 0.05 | - |  | 18.00± 0.06 | - |  | 16.66± 0.06 | - |  | -- | - | - | 
| 58373.15 | 17.24± 0.06 | - |  | 18.17± 0.07 | - |  | -- | - | - | -- | - | - | 
| 58375.16 | 17.15± 0.05 | - |  | -- | - | - | -- | - | - | 16.23± 0.09 | - |  | 
| 58433.02 | 17.18± 0.05 | - |  | -- | - | - | 16.67± 0.05 | - |  | 16.20± 0.10 | - |  | 
| 58673.38 | 17.16± 0.03 | - |  | 18.12± 0.05 | - |  | -- | - | - | -- | - | - | 
| 58695.39 | 17.24± 0.04 | - |  | -- | - | - | 16.73± 0.04 | - |  | -- | - | - | 
| 58696.41 | 17.23± 0.05 | - |  | 18.13± 0.08 | - |  | 16.70± 0.07 | - |   | -- | - | - | 
| 58750.20 | 17.16± 0.04 | A |   | 18.11± 0.03 | - |  | 16.63± 0.05 | - |  | 16.29± 0.08 | - |  | 
| 58757.17 | 17.15± 0.05 | - |  | -- | - | - | 16.66± 0.05 | - |  | -- | - | - | 
| 58779.18 | 17.07± 0.04 | - |  | 17.97± 0.04 | - |  | -- | - | - | -- | - | - | 
| 58784.14 | 17.15± 0.04 | A |   | -- | - | - | 16.66± 0.04 | - |  | 16.17± 0.08 | - |  | 
| 58812.20 | 17.07± 0.06 | - |  | -- | - | - | 16.59± 0.06 | - |  | -- | - | - | 
| 59059.40 | 17.06± 0.06 | - |  | -- | - | - | 16.60± 0.04 | - |  | 16.16± 0.08 | - |  | 
| 59081.34 | 17.07± 0.05 | A |   | 17.90± 0.05 | A |   | 16.58± 0.05 | A |   | 16.13± 0.07 | - |  | 
| 59082.38 | 17.10± 0.05 | - |  | 17.92± 0.03 | - |    | 16.60± 0.04 | - |    | -- | - | - | 
| 59084.25 | -- | - | - | -- | - | - | 16.60± 0.04 | T |  | -- | - | - | 
| 59161.14 | 17.14± 0.04 | - |  | -- | - | - | 16.66± 0.04 | - |  | 16.26± 0.09 | - |  | 
| 59171.15 | 17.11± 0.05 | A |   | 17.97± 0.06 | A |   | 16.61± 0.05 | - |  | 16.19± 0.07 | A |   | 
| 59227.14 | 17.19± 0.05 | A |   | 18.07± 0.05 | A |   | 16.68± 0.04 | A |   | 16.18± 0.07 | - |  | 
| 59415.39 | 17.30± 0.06 | T |  | -- | - | - | -- | - | - | -- | - | - | 
| 59441.42 | 17.26± 0.06 | T |  | -- | - | - | -- | - | - | -- | - | - | 
| 59442.41 | 17.27± 0.05 | - |  | -- | - | - | 16.76± 0.04 | - |  | -- | - | - | 
| 59463.33 | 17.19± 0.05 | A |   | 18.07± 0.06 | A |   | -- | - | - | 16.27± 0.07 | - |  | 
| 59522.13 | 16.99± 0.05 | - |  | -- | - | - | 16.51± 0.05 | - |  | 16.10± 0.07 | - |  | 
| 59525.12 | 17.01± 0.05 | - |  | -- | - | - | 16.56± 0.04 | - |  | -- | - | - | 
| 59546.20 | 17.03± 0.05 | A |   | 17.85± 0.03 | - |  | -- | - | - | 16.11± 0.07 | - |  | 
| 59551.14 | 17.06± 0.06 | A |   | -- | - | - | -- | - | - | 16.16± 0.08 | - |  | 
| 59583.20 | 17.17± 0.04 | - |  | -- | - | - | 16.68± 0.04 | - |  | -- | - | - | 
| 59608.14 | 17.15± 0.05 | - |  | 18.03± 0.08 | - |  | 16.64± 0.05 | - |  | -- | - | - | 
| 59794.38 | 17.18± 0.05 | - |  | -- | - | - | 16.68± 0.04 | - |  | -- | - | - | 
| 59849.19 | 17.20± 0.05 | A |   | 18.03± 0.04 | - |  | 16.66± 0.05 | - |  | -- | - | - | 
| 59851.19 | 17.19± 0.05 | - |  | 18.07± 0.04 | - |  | -- | - | - | 16.20± 0.09 | - |  | 
| 59854.19 | 17.24± 0.04 | - |  | -- | - | - | 16.72± 0.04 | - |  | 16.28± 0.08 | - |  | 
| 59879.18 | 17.11± 0.04 | - |  | 17.95± 0.04 | - |  | 16.66± 0.05 | - |  | -- | - | - | 
| 59903.26 | 17.03± 0.04 | - |  | 17.75± 0.05 | - |  | 16.55± 0.05 | - |  | 16.13± 0.08 | - |  | 
| 59904.15 | 17.06± 0.04 | - |  | 17.85± 0.03 | - |   | 16.59± 0.04 | - |   | 16.21± 0.08 | - |   | 
| 59932.20 | 17.06± 0.05 | A |   | 17.82± 0.04 | - |  | 16.54± 0.05 | - |  | -- | - | - | 
| 60172.40 | 17.03± 0.05 | - |  | 17.80± 0.03 | - |  | -- | - | - | -- | - | - | 
| 60205.19 | 17.04± 0.05 | - |  | 17.84± 0.05 | - |  | -- | - | - | -- | - | - | 
| 60227.15 | 17.14± 0.04 | - |  | -- | - | - | 16.65± 0.06 | - |  | -- | - | - | 
| 60261.16 | 17.23± 0.05 | A |   | -- | - | - | 16.70± 0.05 | - |  | 16.25± 0.08 | A |   | 
| 60262.18 | 17.28± 0.05 | - |  | 18.23± 0.04 | - |  | 16.78± 0.05 | - |   | -- | - | - | 
| 60290.22 | 17.31± 0.05 | A |   | 18.30± 0.05 | A |   | 16.79± 0.06 | - |  | 16.29± 0.08 | - |  | 
| 60292.23 | 17.30± 0.06 | A |   | -- | - | - | 16.75± 0.05 | - |  | 16.30± 0.09 | - |  | 
| 60342.13 | 17.08± 0.05 | - |  | -- | - | - | 16.59± 0.05 | - |  | -- | - | - | 
| 60506.34 | 17.13± 0.05 | - |  | -- | - | - | 16.64± 0.04 | - |  | -- | - | - | 
| 60529.40 | 17.06± 0.05 | - |  | 17.81± 0.07 | - |  | 16.58± 0.05 | - |  | -- | - | - | 
| 60533.41 | 17.06± 0.06 | - |  | 17.89± 0.04 | - |  | -- | - | - | 16.21± 0.07 | - |  | 
| 60556.31 | 17.08± 0.05 | - |  | -- | - | - | -- | - | - | 16.19± 0.08 | - |  | 
| 60562.27 | 17.14± 0.05 | - |  | 17.94± 0.04 | - |  | -- | - | - | 16.27± 0.07 | - |  | 
| 60592.13 | 17.18± 0.05 | A |   | 17.98± 0.05 | A |   | 16.66± 0.05 | A |   | -- | - | - | 
| 60612.17 | 17.15± 0.05 | - |  | -- | - | - | -- | - | - | 16.19± 0.07 | - |  | 
| 60651.20 | 17.18± 0.06 | A |   | 18.16± 0.04 | - |  | 16.65± 0.05 | - |  | -- | - | - | 


If the brightness variation is true variability then there should be a correlation between brightness changes recorded in different filter bands. The following table are the R-squared linear correlation factors calculated for the pairs of bands. The number in parentheses next to the R-squared value is the number of elements used to calculate the correlation factor. The number in square brackets next to the band is the range of magnitudes measured.
| V [0.32 mag] | B [0.55 mag] | R [0.28 mag] | |
|---|---|---|---|
| B [0.55 mag] | 0.89 (38) | ||
| R [0.28 mag] | 0.90 (44) | 0.72 (25) | |
| I [0.20 mag] | 0.57 (28) | 0.37 (16) | 0.65 (18) | 
The plots below are provided to check the values in the table above and also to show any non-linear correlations


Welch & Stetson (1993, AJ, 105, 1813) present a method for varible star detection in CCD images from automated surveys. Data from two bands are compared and two statistics are calculated: R and I.
The I-statistic has an expectation value of zero for stars that are NOT variable. A larger non-zero I-value indicates a higher likelihood that the star is variable. The R statistic indicates how the color of the star changes as the variable grows brighter with R = 1.0 being no change in color.
R and I values have only been calculated if there are more than four (4) matched measurements of brightness in each band.
| V (I|R) | B (I|R) | R (I|R) | |
|---|---|---|---|
| B (I|R) | 4.89 | 1.95 | ||
| R (I|R) | 2.27 | 1.22 | 2.72 | 0.09 | |
| I (I|R) | 0.86 | 2.26 | 1.49 | 4.54 | 0.91 | 1.93 | 
By John C. Martin, University of Illinois Springfield Henry R. Barber Research Observatory
Generated on 2025-08-04 15:53:14 UT-5