| MJD | V | * | Image | B | * | Image | R | * | Images | I | * | Images | 
|---|---|---|---|---|---|---|---|---|---|---|---|---|
| 56140.37 | 17.05± 0.05 | - |  | -- | - | - | 16.86± 0.08 | - |  | -- | - | - | 
| 56599.17 | 16.94± 0.05 | - |  | 17.02± 0.06 | - |  | 16.75± 0.05 | - |  | -- | - | - | 
| 56976.16 | 17.01± 0.04 | - |  | 17.13± 0.06 | - |  | 16.84± 0.05 | - |  | -- | - | - | 
| 56982.22 | 16.99± 0.06 | - |  | 17.08± 0.06 | - |  | 16.84± 0.07 | - |  | -- | - | - | 
| 57038.13 | 17.10± 0.04 | - |  | 17.16± 0.05 | - |  | 16.93± 0.04 | - |  | -- | - | - | 
| 57310.13 | 17.00± 0.05 | - |  | 17.10± 0.07 | - |  | 16.79± 0.05 | - |  | -- | - | - | 
| 57328.19 | 16.90± 0.05 | - |  | 16.98± 0.07 | - |  | 16.75± 0.07 | - |  | -- | - | - | 
| 57335.18 | 16.95± 0.06 | - |  | -- | - | - | 16.78± 0.04 | - |  | -- | - | - | 
| 57401.10 | 17.02± 0.04 | - |  | 17.11± 0.05 | - |  | -- | - | - | -- | - | - | 
| 57634.34 | 16.97± 0.04 | - |  | 17.11± 0.07 | - |  | 16.85± 0.05 | - |  | 16.64± 0.06 | - |  | 
| 57638.43 | 16.94± 0.06 | - |  | -- | - | - | -- | - | - | 16.56± 0.10 | - |  | 
| 57687.13 | 17.09± 0.04 | - |  | 17.24± 0.06 | - |  | 16.90± 0.04 | - |  | 16.74± 0.06 | - |  | 
| 57964.33 | 17.01± 0.04 | - |  | 17.07± 0.07 | - |  | 16.85± 0.05 | - |  | 16.72± 0.06 | - |  | 
| 58045.18 | 16.99± 0.05 | - |  | 17.07± 0.07 | - |  | 16.81± 0.06 | - |  | -- | - | - | 
| 58073.20 | 17.03± 0.04 | - |  | 17.09± 0.07 | - |  | -- | - | - | -- | - | - | 
| 58103.18 | 16.98± 0.05 | T |  | -- | - | - | -- | - | - | -- | - | - | 
| 58108.11 | 16.92± 0.05 | - |  | 17.00± 0.08 | - |  | -- | - | - | 16.44± 0.07 | - |  | 
| 58312.39 | 16.84± 0.05 | - |  | 16.94± 0.07 | - |  | -- | - | - | -- | - | - | 
| 58317.37 | 16.86± 0.04 | - |  | 16.95± 0.07 | - |  | 16.67± 0.04 | - |  | -- | - | - | 
| 58341.34 | 16.95± 0.06 | - |  | -- | - | - | -- | - | - | 16.60± 0.07 | - |  | 
| 58342.40 | 17.01± 0.05 | - |  | 17.09± 0.07 | - |  | 16.87± 0.05 | - |  | -- | - | - | 
| 58375.14 | 16.89± 0.04 | - |  | -- | - | - | 16.74± 0.05 | - |  | -- | - | - | 
| 58420.08 | 17.05± 0.04 | A |   | 17.14± 0.06 | A |   | 16.79± 0.04 | - |  | 16.70± 0.07 | A |   | 
| 58433.00 | 16.95± 0.05 | - |  | -- | - | - | 16.75± 0.05 | - |  | 16.66± 0.06 | - |  | 
| 58672.39 | 16.94± 0.07 | - |  | -- | - | - | 16.74± 0.05 | - |  | 16.64± 0.09 | - |  | 
| 58695.36 | 16.85± 0.05 | - |  | 16.96± 0.05 | - |  | 16.67± 0.04 | - |  | -- | - | - | 
| 58784.12 | 16.88± 0.05 | - |  | 16.96± 0.05 | - |  | -- | - | - | -- | - | - | 
| 58812.22 | 16.94± 0.05 | - |  | -- | - | - | -- | - | - | 16.58± 0.05 | - |  | 
| 58902.07 | 16.84± 0.04 | - |  | -- | - | - | 16.68± 0.04 | - |  | -- | - | - | 
| 59059.38 | 16.90± 0.05 | - |  | 16.98± 0.05 | - |  | -- | - | - | -- | - | - | 
| 59081.26 | 16.92± 0.05 | - |  | -- | - | - | 16.75± 0.05 | - |  | -- | - | - | 
| 59084.34 | -- | - | - | -- | - | - | 16.70± 0.04 | T |  | -- | - | - | 
| 59161.07 | 16.88± 0.05 | - |  | 16.98± 0.06 | - |  | 16.70± 0.04 | - |  | -- | - | - | 
| 59171.09 | 16.81± 0.05 | - |  | -- | - | - | -- | - | - | 16.47± 0.06 | - |  | 
| 59227.08 | 16.82± 0.04 | - |  | 16.99± 0.04 | - |  | 16.63± 0.04 | - |  | -- | - | - | 
| 59415.36 | 16.86± 0.04 | - |  | -- | - | - | 16.68± 0.04 | - |  | -- | - | - | 
| 59441.39 | 16.89± 0.05 | - |  | 17.03± 0.06 | - |  | -- | - | - | -- | - | - | 
| 59463.30 | 16.88± 0.04 | A |   | -- | - | - | -- | - | - | 16.52± 0.05 | - |  | 
| 59523.15 | 16.88± 0.04 | - |  | -- | - | - | 16.69± 0.04 | - |  | -- | - | - | 
| 59525.15 | 16.85± 0.04 | - |  | 16.96± 0.04 | - |  | -- | - | - | -- | - | - | 
| 59546.15 | 16.84± 0.04 | - |  | -- | - | - | -- | - | - | 16.40± 0.05 | - |  | 
| 59551.11 | 16.79± 0.04 | - |  | 16.95± 0.05 | - |  | -- | - | - | -- | - | - | 
| 59583.15 | 16.83± 0.04 | - |  | -- | - | - | 16.62± 0.04 | - |  | -- | - | - | 
| 59608.07 | 16.84± 0.04 | - |  | -- | - | - | -- | - | - | 16.48± 0.05 | - |  | 
| 59794.35 | 16.89± 0.04 | T |  | -- | - | - | -- | - | - | -- | - | - | 
| 59823.24 | 16.78± 0.04 | - |  | 16.92± 0.04 | - |  | -- | - | - | -- | - | - | 
| 59851.13 | 16.90± 0.04 | - |  | -- | - | - | 16.73± 0.04 | - |  | -- | - | - | 
| 59854.22 | 16.92± 0.04 | - |  | 17.06± 0.05 | - |  | -- | - | - | -- | - | - | 
| 59879.12 | 16.79± 0.04 | - |  | -- | - | - | -- | - | - | 16.39± 0.06 | A |   | 
| 59904.12 | 16.83± 0.04 | - |  | 16.98± 0.04 | - |  | 16.66± 0.04 | - |  | 16.51± 0.06 | - |  | 
| 59932.13 | 16.80± 0.06 | - |  | -- | - | - | 16.63± 0.05 | - |  | -- | - | - | 
| 60172.37 | 16.86± 0.04 | - |  | 16.99± 0.04 | - |  | -- | - | - | -- | - | - | 
| 60205.15 | 16.83± 0.04 | - |  | -- | - | - | 16.66± 0.05 | - |  | -- | - | - | 
| 60227.12 | 16.88± 0.04 | - |  | -- | - | - | -- | - | - | 16.56± 0.06 | - |  | 
| 60262.13 | 16.93± 0.04 | - |  | 17.07± 0.04 | - |  | 16.77± 0.04 | - |  | -- | - | - | 
| 60290.15 | 16.81± 0.04 | - |  | 16.96± 0.05 | - |  | -- | - | - | 16.48± 0.06 | - |  | 
| 60292.18 | 16.83± 0.04 | - |  | -- | - | - | 16.67± 0.05 | - |  | -- | - | - | 
| 60342.08 | 16.96± 0.04 | - |  | -- | - | - | 16.77± 0.05 | - |  | -- | - | - | 
| 60504.38 | 16.93± 0.04 | - |  | 17.08± 0.04 | - |  | 16.76± 0.05 | - |  | -- | - | - | 
| 60529.36 | 16.98± 0.04 | - |  | -- | - | - | -- | - | - | 16.59± 0.06 | - |  | 
| 60556.24 | 16.88± 0.04 | - |  | 17.01± 0.05 | - |  | 16.73± 0.04 | - |  | -- | - | - | 
| 60594.10 | 16.86± 0.05 | - |  | -- | - | - | -- | - | - | 16.61± 0.06 | - |  | 
| 60612.14 | 16.88± 0.05 | - |  | -- | - | - | 16.70± 0.05 | - |  | -- | - | - | 
| 60651.14 | 16.95± 0.04 | - |  | 17.10± 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 [0.31 mag] | R [0.30 mag] | |
|---|---|---|---|
| B [0.31 mag] | 0.86 (34) | ||
| R [0.30 mag] | 0.92 (36) | 0.77 (20) | |
| I [0.35 mag] | 0.73 (20) | 0.76 (7) | 0.73 (7) | 
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) | 2.45 | 0.72 | ||
| R (I|R) | 3.02 | 1.08 | 2.11 | 0.18 | |
| I (I|R) | 2.84 | 1.12 | 2.75 | 0.83 | 2.01 | 1.53 | 
By John C. Martin, University of Illinois Springfield Henry R. Barber Research Observatory
Generated on 2025-08-04 15:53:14 UT-5